# Please edit this file with care to maintain the # correct format so that SPOT can still read it. # Generated by SPOT on: 6/15/2006 12:1:50 HEADER: FILE_VERSION=14.0, STATUS = PROPOSAL AOT_TYPE: IRS Peakup Image AOR_LABEL: seppcon-143P-KM AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: Kowal-Mrkos EPHEMERIS: NAIF_ID=1000057, NAIF_NAME=Kowal-Mrkos OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES RED: EXPOSURE_TIME=14, N_CYCLES_SEQ=1 BLUE: EXPOSURE_TIME=14, N_CYCLES_SEQ=1 DITHER_PATTERN: TYPE=5Positions DITHER_SCALE: small SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=588.0, SLEW_TIME=17.4, SETTLE_TIME=54.0, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=911, DOWNLINK_VOLUME=2465830, VERSION=S14.1.0 INTEGRATION_TIME: IRS_RED=73.40032,IRS_BLUE=73.40032 TIMING1: START_DATE=2007 Feb 15, START_TIME=19:50:00, END_DATE=2007 Mar 26, END_TIME=16:39:00 COMMENT_START: In almost all cases, a given comet is brighter in one observability window compared to the other(s) in Cycle 3. This is our motivation for having a timing constraint. Generally the constraint covers the full interval of the brightest window in the Cycle. COMMENT_END: AOT_TYPE: IRS Peakup Image AOR_LABEL: seppcon-47P-AJ AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: Ashbrook-Jackson EPHEMERIS: NAIF_ID=1000003, NAIF_NAME=Ashbrook-Jackson OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES RED: EXPOSURE_TIME=14, N_CYCLES_SEQ=1 BLUE: EXPOSURE_TIME=14, N_CYCLES_SEQ=1 DITHER_PATTERN: TYPE=5Positions DITHER_SCALE: small SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=588.0, SLEW_TIME=17.4, SETTLE_TIME=54.0, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=911, DOWNLINK_VOLUME=2465830, VERSION=S14.1.0 INTEGRATION_TIME: IRS_RED=73.40032,IRS_BLUE=73.40032 TIMING1: START_DATE=2007 Mar 20, START_TIME=18:19:00, END_DATE=2007 May 1, END_TIME=07:24:00 COMMENT_START: In almost all cases, a given comet is brighter in one observability window compared to the other(s) in Cycle 3. This is our motivation for having a timing constraint. Generally the constraint covers the full interval of the brightest window in the Cycle. COMMENT_END: AOT_TYPE: IRS Peakup Image AOR_LABEL: seppcon-48P-J AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: Johnson EPHEMERIS: NAIF_ID=1000049, NAIF_NAME=Johnson OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES RED: EXPOSURE_TIME=14, N_CYCLES_SEQ=1 BLUE: EXPOSURE_TIME=14, N_CYCLES_SEQ=1 DITHER_PATTERN: TYPE=5Positions DITHER_SCALE: small SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=588.0, SLEW_TIME=17.4, SETTLE_TIME=54.0, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=911, DOWNLINK_VOLUME=2465830, VERSION=S14.1.0 INTEGRATION_TIME: IRS_RED=73.40032,IRS_BLUE=73.40032 TIMING1: START_DATE=2006 Nov 5, START_TIME=10:49:00, END_DATE=2006 Dec 15, END_TIME=17:51:00 TIMING2: START_DATE=2007 Apr 3, START_TIME=16:10:00, END_DATE=2007 Apr 18, END_TIME=12:00:00 COMMENT_START: In almost all cases, a given comet is brighter in one observability window compared to the other(s) in Cycle 3. This is our motivation for having a timing constraint. Generally the constraint covers the full interval of the brightest window in the Cycle. COMMENT_END: AOT_TYPE: IRS Peakup Image AOR_LABEL: seppcon-7P-PW AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: Pons-Winnecke EPHEMERIS: NAIF_ID=1000069, NAIF_NAME=Pons-Winnecke OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES RED: EXPOSURE_TIME=14, N_CYCLES_SEQ=1 BLUE: EXPOSURE_TIME=14, N_CYCLES_SEQ=2 DITHER_PATTERN: TYPE=5Positions DITHER_SCALE: small SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=698.0, SLEW_TIME=17.4, SETTLE_TIME=54.0, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=911, DOWNLINK_VOLUME=3698745, VERSION=S14.1.0 INTEGRATION_TIME: IRS_RED=73.40032,IRS_BLUE=146.80064 TIMING1: START_DATE=2007 Mar 31, START_TIME=17:44:00, END_DATE=2007 May 9, END_TIME=11:42:00 COMMENT_START: In almost all cases, a given comet is brighter in one observability window compared to the other(s) in Cycle 3. This is our motivation for having a timing constraint. Generally the constraint covers the full interval of the brightest window in the Cycle. COMMENT_END: AOT_TYPE: IRS Peakup Image AOR_LABEL: seppcon-P04F3-NEAT AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: NEAT (P/2004 F3) EPHEMERIS: NAIF_ID=1000486, NAIF_NAME=NEAT (P/2004 F3) OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES RED: EXPOSURE_TIME=14, N_CYCLES_SEQ=1 BLUE: EXPOSURE_TIME=14, N_CYCLES_SEQ=2 DITHER_PATTERN: TYPE=5Positions DITHER_SCALE: small SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=698.0, SLEW_TIME=17.4, SETTLE_TIME=54.0, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=911, DOWNLINK_VOLUME=3698745, VERSION=S14.1.0 INTEGRATION_TIME: IRS_RED=73.40032,IRS_BLUE=146.80064 TIMING1: START_DATE=2006 Aug 22, START_TIME=00:00:00, END_DATE=2006 Aug 28, END_TIME=20:57:00 TIMING2: START_DATE=2006 Dec 15, START_TIME=21:37:00, END_DATE=2007 Jan 28, END_TIME=01:58:00 COMMENT_START: In almost all cases, a given comet is brighter in one observability window compared to the other(s) in Cycle 3. This is our motivation for having a timing constraint. Generally the constraint covers the full interval of the brightest window in the Cycle. COMMENT_END: AOT_TYPE: IRS Peakup Image AOR_LABEL: seppcon-129P-SL3 AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: Shoemaker-Levy 3 EPHEMERIS: NAIF_ID=1000180, NAIF_NAME=Shoemaker-Levy 3 OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES RED: EXPOSURE_TIME=14, N_CYCLES_SEQ=1 BLUE: EXPOSURE_TIME=14, N_CYCLES_SEQ=2 DITHER_PATTERN: TYPE=5Positions DITHER_SCALE: small SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=698.0, SLEW_TIME=17.4, SETTLE_TIME=54.0, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=911, DOWNLINK_VOLUME=3698745, VERSION=S14.1.0 INTEGRATION_TIME: IRS_RED=73.40032,IRS_BLUE=146.80064 TIMING1: START_DATE=2007 Apr 13, START_TIME=00:00:00, END_DATE=2007 May 7, END_TIME=01:45:00 COMMENT_START: In almost all cases, a given comet is brighter in one observability window compared to the other(s) in Cycle 3. This is our motivation for having a timing constraint. Generally the constraint covers the full interval of the brightest window in the Cycle. COMMENT_END: AOT_TYPE: IRS Peakup Image AOR_LABEL: seppcon-P05GF8-LONEOS AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: LONEOS (P/2005 GF8) EPHEMERIS: NAIF_ID=1000562, NAIF_NAME=LONEOS (P/2005 GF8) OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES RED: EXPOSURE_TIME=14, N_CYCLES_SEQ=1 BLUE: EXPOSURE_TIME=14, N_CYCLES_SEQ=2 DITHER_PATTERN: TYPE=5Positions DITHER_SCALE: small SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=698.0, SLEW_TIME=17.4, SETTLE_TIME=54.0, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=911, DOWNLINK_VOLUME=3698745, VERSION=S14.1.0 INTEGRATION_TIME: IRS_RED=73.40032,IRS_BLUE=146.80064 TIMING1: START_DATE=2006 Oct 26, START_TIME=13:31:00, END_DATE=2006 Dec 7, END_TIME=15:26:00 COMMENT_START: In almost all cases, a given comet is brighter in one observability window compared to the other(s) in Cycle 3. This is our motivation for having a timing constraint. Generally the constraint covers the full interval of the brightest window in the Cycle. COMMENT_END: AOT_TYPE: IRS Peakup Image AOR_LABEL: seppcon-31P-SW2 AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: Schwassmann-Wachmann 2 EPHEMERIS: NAIF_ID=1000080, NAIF_NAME=Schwassmann-Wachmann 2 OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES RED: EXPOSURE_TIME=14, N_CYCLES_SEQ=1 BLUE: EXPOSURE_TIME=14, N_CYCLES_SEQ=2 DITHER_PATTERN: TYPE=5Positions DITHER_SCALE: small SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=698.0, SLEW_TIME=17.4, SETTLE_TIME=54.0, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=911, DOWNLINK_VOLUME=3698745, VERSION=S14.1.0 INTEGRATION_TIME: IRS_RED=73.40032,IRS_BLUE=146.80064 TIMING1: START_DATE=2006 Oct 28, START_TIME=16:00:00, END_DATE=2006 Dec 8, END_TIME=09:30:00 COMMENT_START: In almost all cases, a given comet is brighter in one observability window compared to the other(s) in Cycle 3. This is our motivation for having a timing constraint. Generally the constraint covers the full interval of the brightest window in the Cycle. COMMENT_END: AOT_TYPE: IRS Peakup Image AOR_LABEL: seppcon-14P-Wolf AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: Wolf EPHEMERIS: NAIF_ID=1000110, NAIF_NAME=Wolf OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES RED: EXPOSURE_TIME=14, N_CYCLES_SEQ=1 BLUE: EXPOSURE_TIME=14, N_CYCLES_SEQ=3 DITHER_PATTERN: TYPE=5Positions DITHER_SCALE: small SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=808.0, SLEW_TIME=17.4, SETTLE_TIME=54.0, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=911, DOWNLINK_VOLUME=4931660, VERSION=S14.1.0 INTEGRATION_TIME: IRS_RED=73.40032,IRS_BLUE=220.20096 TIMING1: START_DATE=2007 Mar 20, START_TIME=16:52:00, END_DATE=2007 May 3, END_TIME=04:38:00 COMMENT_START: In almost all cases, a given comet is brighter in one observability window compared to the other(s) in Cycle 3. This is our motivation for having a timing constraint. Generally the constraint covers the full interval of the brightest window in the Cycle. COMMENT_END: AOT_TYPE: IRS Peakup Image AOR_LABEL: seppcon-119P-PH AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: Parker-Hartley EPHEMERIS: NAIF_ID=1000120, NAIF_NAME=Parker-Hartley OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES RED: EXPOSURE_TIME=14, N_CYCLES_SEQ=1 BLUE: EXPOSURE_TIME=14, N_CYCLES_SEQ=3 DITHER_PATTERN: TYPE=5Positions DITHER_SCALE: small SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=808.0, SLEW_TIME=17.4, SETTLE_TIME=54.0, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=911, DOWNLINK_VOLUME=4931660, VERSION=S14.1.0 INTEGRATION_TIME: IRS_RED=73.40032,IRS_BLUE=220.20096 TIMING1: START_DATE=2007 Jan 6, START_TIME=18:25:00, END_DATE=2007 Feb 16, END_TIME=05:35:00 COMMENT_START: In almost all cases, a given comet is brighter in one observability window compared to the other(s) in Cycle 3. This is our motivation for having a timing constraint. Generally the constraint covers the full interval of the brightest window in the Cycle. COMMENT_END: AOT_TYPE: IRS Peakup Image AOR_LABEL: seppcon-74P-SC AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: Smirnova-Chernykh EPHEMERIS: NAIF_ID=1000088, NAIF_NAME=Smirnova-Chernykh OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES RED: EXPOSURE_TIME=14, N_CYCLES_SEQ=1 BLUE: EXPOSURE_TIME=14, N_CYCLES_SEQ=3 DITHER_PATTERN: TYPE=5Positions DITHER_SCALE: small SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=808.0, SLEW_TIME=17.4, SETTLE_TIME=54.0, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=911, DOWNLINK_VOLUME=4931660, VERSION=S14.1.0 INTEGRATION_TIME: IRS_RED=73.40032,IRS_BLUE=220.20096 TIMING1: START_DATE=2006 Sep 1, START_TIME=12:00:00, END_DATE=2006 Sep 25, END_TIME=00:25:00 TIMING2: START_DATE=2007 Jan 15, START_TIME=22:29:00, END_DATE=2007 Feb 25, END_TIME=08:24:00 COMMENT_START: In almost all cases, a given comet is brighter in one observability window compared to the other(s) in Cycle 3. This is our motivation for having a timing constraint. Generally the constraint covers the full interval of the brightest window in the Cycle. COMMENT_END: AOT_TYPE: IRS Peakup Image AOR_LABEL: seppcon-107P-WH AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: 4015 Wilson-Harrington EPHEMERIS: NAIF_ID=2004015, NAIF_NAME=4015 Wilson-Harrington OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES RED: EXPOSURE_TIME=14, N_CYCLES_SEQ=2 BLUE: EXPOSURE_TIME=14, N_CYCLES_SEQ=4 DITHER_PATTERN: TYPE=5Positions DITHER_SCALE: small SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=1028.0, SLEW_TIME=17.4, SETTLE_TIME=54.0, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=911, DOWNLINK_VOLUME=7397490, VERSION=S14.1.0 INTEGRATION_TIME: IRS_RED=146.80064,IRS_BLUE=293.6013 TIMING1: START_DATE=2007 Jan 7, START_TIME=06:33:00, END_DATE=2007 Feb 14, END_TIME=23:27:00 TIMING2: START_DATE=2007 May 31, START_TIME=01:29:00, END_DATE=2007 Jun 20, END_TIME=12:00:00 COMMENT_START: In almost all cases, a given comet is brighter in one observability window compared to the other(s) in Cycle 3. This is our motivation for having a timing constraint. Generally the constraint covers the full interval of the brightest window in the Cycle. COMMENT_END: AOT_TYPE: IRS Peakup Image AOR_LABEL: seppcon-118P-SL4 AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: Shoemaker-Levy 4 EPHEMERIS: NAIF_ID=1000150, NAIF_NAME=Shoemaker-Levy 4 OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES RED: EXPOSURE_TIME=14, N_CYCLES_SEQ=2 BLUE: EXPOSURE_TIME=14, N_CYCLES_SEQ=5 DITHER_PATTERN: TYPE=5Positions DITHER_SCALE: small SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=1138.0, SLEW_TIME=17.4, SETTLE_TIME=54.0, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=911, DOWNLINK_VOLUME=8630405, VERSION=S14.1.0 INTEGRATION_TIME: IRS_RED=146.80064,IRS_BLUE=367.00162 TIMING1: START_DATE=2006 Sep 1, START_TIME=14:50:00, END_DATE=2006 Oct 12, END_TIME=18:52:00 TIMING2: START_DATE=2007 May 11, START_TIME=15:47:00, END_DATE=2007 Jun 10, END_TIME=12:00:00 COMMENT_START: In almost all cases, a given comet is brighter in one observability window compared to the other(s) in Cycle 3. This is our motivation for having a timing constraint. Generally the constraint covers the full interval of the brightest window in the Cycle. COMMENT_END: AOT_TYPE: IRS Peakup Image AOR_LABEL: seppcon-P05L4-Chrst AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: Christensen (P/2005 L4) EPHEMERIS: NAIF_ID=1001646, NAIF_NAME=Christensen (P/2005 L4) OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES RED: EXPOSURE_TIME=14, N_CYCLES_SEQ=3 BLUE: EXPOSURE_TIME=14, N_CYCLES_SEQ=6 DITHER_PATTERN: TYPE=5Positions DITHER_SCALE: small SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=1358.0, SLEW_TIME=17.4, SETTLE_TIME=54.0, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=911, DOWNLINK_VOLUME=11096240, VERSION=S14.1.0 INTEGRATION_TIME: IRS_RED=220.20096,IRS_BLUE=440.40192 TIMING1: START_DATE=2007 Feb 3, START_TIME=03:13:00, END_DATE=2007 Mar 16, END_TIME=20:49:00 COMMENT_START: In almost all cases, a given comet is brighter in one observability window compared to the other(s) in Cycle 3. This is our motivation for having a timing constraint. Generally the constraint covers the full interval of the brightest window in the Cycle. COMMENT_END: AOT_TYPE: IRS Peakup Image AOR_LABEL: seppcon-P05R2-vN AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: Van Ness (P/2005 R2) EPHEMERIS: NAIF_ID=1001663, NAIF_NAME=Van Ness (P/2005 R2) OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES RED: EXPOSURE_TIME=14, N_CYCLES_SEQ=3 BLUE: EXPOSURE_TIME=14, N_CYCLES_SEQ=7 DITHER_PATTERN: TYPE=5Positions DITHER_SCALE: small SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=1468.0, SLEW_TIME=17.4, SETTLE_TIME=54.0, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=911, DOWNLINK_VOLUME=12329155, VERSION=S14.1.0 INTEGRATION_TIME: IRS_RED=220.20096,IRS_BLUE=513.80225 TIMING1: START_DATE=2006 Oct 21, START_TIME=21:39:00, END_DATE=2006 Dec 2, END_TIME=00:57:00 COMMENT_START: In almost all cases, a given comet is brighter in one observability window compared to the other(s) in Cycle 3. This is our motivation for having a timing constraint. Generally the constraint covers the full interval of the brightest window in the Cycle. COMMENT_END: AOT_TYPE: IRS Peakup Image AOR_LABEL: seppcon-137P-SL2 AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: Shoemaker-Levy 2 EPHEMERIS: NAIF_ID=1000126, NAIF_NAME=Shoemaker-Levy 2 OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES RED: EXPOSURE_TIME=14, N_CYCLES_SEQ=3 BLUE: EXPOSURE_TIME=14, N_CYCLES_SEQ=8 DITHER_PATTERN: TYPE=5Positions DITHER_SCALE: small SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=1578.0, SLEW_TIME=17.4, SETTLE_TIME=54.0, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=911, DOWNLINK_VOLUME=13562070, VERSION=S14.1.0 INTEGRATION_TIME: IRS_RED=220.20096,IRS_BLUE=587.2026 TIMING1: START_DATE=2007 Mar 13, START_TIME=09:20:00, END_DATE=2007 Apr 20, END_TIME=19:42:00 COMMENT_START: In almost all cases, a given comet is brighter in one observability window compared to the other(s) in Cycle 3. This is our motivation for having a timing constraint. Generally the constraint covers the full interval of the brightest window in the Cycle. COMMENT_END: AOT_TYPE: IRS Peakup Image AOR_LABEL: seppcon-172P-Yeung AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: Yeung EPHEMERIS: NAIF_ID=1000388, NAIF_NAME=Yeung OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES RED: EXPOSURE_TIME=14, N_CYCLES_SEQ=4 BLUE: EXPOSURE_TIME=14, N_CYCLES_SEQ=8 DITHER_PATTERN: TYPE=5Positions DITHER_SCALE: small SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=1688.0, SLEW_TIME=17.4, SETTLE_TIME=54.0, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=911, DOWNLINK_VOLUME=14794985, VERSION=S14.1.0 INTEGRATION_TIME: IRS_RED=293.6013,IRS_BLUE=587.2026 TIMING1: START_DATE=2006 Oct 5, START_TIME=15:11:00, END_DATE=2006 Nov 16, END_TIME=14:53:00 COMMENT_START: In almost all cases, a given comet is brighter in one observability window compared to the other(s) in Cycle 3. This is our motivation for having a timing constraint. Generally the constraint covers the full interval of the brightest window in the Cycle. COMMENT_END: AOT_TYPE: IRS Peakup Image AOR_LABEL: seppcon-121P-SH2 AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: Shoemaker-Holt 2 EPHEMERIS: NAIF_ID=1000141, NAIF_NAME=Shoemaker-Holt 2 OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES RED: EXPOSURE_TIME=14, N_CYCLES_SEQ=4 BLUE: EXPOSURE_TIME=14, N_CYCLES_SEQ=8 DITHER_PATTERN: TYPE=5Positions DITHER_SCALE: small SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=1688.0, SLEW_TIME=17.4, SETTLE_TIME=54.0, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=911, DOWNLINK_VOLUME=14794985, VERSION=S14.1.0 INTEGRATION_TIME: IRS_RED=293.6013,IRS_BLUE=587.2026 TIMING1: START_DATE=2006 Jul 15, START_TIME=12:15:00, END_DATE=2006 Aug 28, END_TIME=09:43:00 COMMENT_START: In almost all cases, a given comet is brighter in one observability window compared to the other(s) in Cycle 3. This is our motivation for having a timing constraint. Generally the constraint covers the full interval of the brightest window in the Cycle. COMMENT_END: AOT_TYPE: IRS Peakup Image AOR_LABEL: seppcon-P05R1-NEAT AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: NEAT (P/2005 R1) EPHEMERIS: NAIF_ID=1001662, NAIF_NAME=NEAT (P/2005 R1) OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES RED: EXPOSURE_TIME=14, N_CYCLES_SEQ=4 BLUE: EXPOSURE_TIME=14, N_CYCLES_SEQ=9 DITHER_PATTERN: TYPE=5Positions DITHER_SCALE: small SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=1798.0, SLEW_TIME=17.4, SETTLE_TIME=54.0, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=911, DOWNLINK_VOLUME=16027900, VERSION=S14.1.0 INTEGRATION_TIME: IRS_RED=293.6013,IRS_BLUE=660.6029 TIMING1: START_DATE=2006 Nov 22, START_TIME=23:50:00, END_DATE=2007 Jan 3, END_TIME=05:44:00 COMMENT_START: In almost all cases, a given comet is brighter in one observability window compared to the other(s) in Cycle 3. This is our motivation for having a timing constraint. Generally the constraint covers the full interval of the brightest window in the Cycle. COMMENT_END: AOT_TYPE: IRS Peakup Image AOR_LABEL: seppcon-68P-Klem AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: Klemola EPHEMERIS: NAIF_ID=1000051, NAIF_NAME=Klemola OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES RED: EXPOSURE_TIME=14, N_CYCLES_SEQ=3 BLUE: EXPOSURE_TIME=14, N_CYCLES_SEQ=9 DITHER_PATTERN: TYPE=5Positions DITHER_SCALE: small SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=1688.0, SLEW_TIME=17.4, SETTLE_TIME=54.0, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=911, DOWNLINK_VOLUME=14794985, VERSION=S14.1.0 INTEGRATION_TIME: IRS_RED=220.20096,IRS_BLUE=660.6029 TIMING1: START_DATE=2007 Jan 29, START_TIME=11:10:00, END_DATE=2007 Mar 9, END_TIME=09:44:00 COMMENT_START: In almost all cases, a given comet is brighter in one observability window compared to the other(s) in Cycle 3. This is our motivation for having a timing constraint. Generally the constraint covers the full interval of the brightest window in the Cycle. COMMENT_END: AOT_TYPE: IRS Peakup Image AOR_LABEL: seppcon-P01YX127-LIN AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: LINEAR (P/2001 YX127) EPHEMERIS: NAIF_ID=1000381, NAIF_NAME=LINEAR (P/2001 YX127) OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES RED: EXPOSURE_TIME=14, N_CYCLES_SEQ=4 BLUE: EXPOSURE_TIME=14, N_CYCLES_SEQ=10 DITHER_PATTERN: TYPE=5Positions DITHER_SCALE: small SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=1909.0, SLEW_TIME=17.4, SETTLE_TIME=54.0, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=918, DOWNLINK_VOLUME=17260815, VERSION=S14.1.0 INTEGRATION_TIME: IRS_RED=293.6013,IRS_BLUE=734.00323 TIMING1: START_DATE=2006 Oct 8, START_TIME=22:03:00, END_DATE=2006 Nov 19, END_TIME=14:26:00 COMMENT_START: In almost all cases, a given comet is brighter in one observability window compared to the other(s) in Cycle 3. This is our motivation for having a timing constraint. Generally the constraint covers the full interval of the brightest window in the Cycle. COMMENT_END: AOT_TYPE: IRS Peakup Image AOR_LABEL: seppcon-6P-dA AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: d'Arrest EPHEMERIS: NAIF_ID=1000017, NAIF_NAME=d'Arrest OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES RED: EXPOSURE_TIME=14, N_CYCLES_SEQ=4 BLUE: EXPOSURE_TIME=14, N_CYCLES_SEQ=10 DITHER_PATTERN: TYPE=5Positions DITHER_SCALE: small SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=1909.0, SLEW_TIME=17.4, SETTLE_TIME=54.0, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=918, DOWNLINK_VOLUME=17260815, VERSION=S14.1.0 INTEGRATION_TIME: IRS_RED=293.6013,IRS_BLUE=734.00323 TIMING1: START_DATE=2007 Jan 8, START_TIME=09:58:00, END_DATE=2007 Feb 17, END_TIME=19:52:00 COMMENT_START: In almost all cases, a given comet is brighter in one observability window compared to the other(s) in Cycle 3. This is our motivation for having a timing constraint. Generally the constraint covers the full interval of the brightest window in the Cycle. COMMENT_END: AOT_TYPE: IRS Peakup Image AOR_LABEL: seppcon-173P-M5 AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: Mueller 5 EPHEMERIS: NAIF_ID=1000149, NAIF_NAME=Mueller 5 OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES RED: EXPOSURE_TIME=14, N_CYCLES_SEQ=4 BLUE: EXPOSURE_TIME=14, N_CYCLES_SEQ=10 DITHER_PATTERN: TYPE=5Positions DITHER_SCALE: small SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=1909.0, SLEW_TIME=17.4, SETTLE_TIME=54.0, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=918, DOWNLINK_VOLUME=17260815, VERSION=S14.1.0 INTEGRATION_TIME: IRS_RED=293.6013,IRS_BLUE=734.00323 TIMING1: START_DATE=2006 Oct 15, START_TIME=12:00:00, END_DATE=2006 Oct 31, END_TIME=10:30:00 TIMING2: START_DATE=2007 Feb 20, START_TIME=11:14:00, END_DATE=2007 Apr 2, END_TIME=00:27:00 COMMENT_START: In almost all cases, a given comet is brighter in one observability window compared to the other(s) in Cycle 3. This is our motivation for having a timing constraint. Generally the constraint covers the full interval of the brightest window in the Cycle. COMMENT_END: AOT_TYPE: IRS Peakup Image AOR_LABEL: seppcon-101P-Ch AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: Chernykh EPHEMERIS: NAIF_ID=1000011, NAIF_NAME=Chernykh OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES RED: EXPOSURE_TIME=14, N_CYCLES_SEQ=5 BLUE: EXPOSURE_TIME=14, N_CYCLES_SEQ=12 DITHER_PATTERN: TYPE=5Positions DITHER_SCALE: small SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=2239.0, SLEW_TIME=17.4, SETTLE_TIME=54.0, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=918, DOWNLINK_VOLUME=20959565, VERSION=S14.1.0 INTEGRATION_TIME: IRS_RED=367.00162,IRS_BLUE=880.80383 TIMING1: START_DATE=2007 Apr 21, START_TIME=23:07:00, END_DATE=2007 Jun 1, END_TIME=16:23:00 COMMENT_START: In almost all cases, a given comet is brighter in one observability window compared to the other(s) in Cycle 3. This is our motivation for having a timing constraint. Generally the constraint covers the full interval of the brightest window in the Cycle. COMMENT_END: AOT_TYPE: IRS Peakup Image AOR_LABEL: seppcon-78P-Geh2 AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: Gehrels 2 EPHEMERIS: NAIF_ID=1000030, NAIF_NAME=Gehrels 2 OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES RED: EXPOSURE_TIME=14, N_CYCLES_SEQ=6 BLUE: EXPOSURE_TIME=14, N_CYCLES_SEQ=13 DITHER_PATTERN: TYPE=5Positions DITHER_SCALE: small SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=2459.0, SLEW_TIME=17.4, SETTLE_TIME=54.0, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=918, DOWNLINK_VOLUME=23425400, VERSION=S14.1.0 INTEGRATION_TIME: IRS_RED=440.40192,IRS_BLUE=954.20416 TIMING1: START_DATE=2006 Jun 20, START_TIME=00:00:00, END_DATE=2006 Jun 29, END_TIME=20:00:00 TIMING2: START_DATE=2007 Feb 3, START_TIME=00:24:00, END_DATE=2007 Mar 13, END_TIME=15:04:00 COMMENT_START: In almost all cases, a given comet is brighter in one observability window compared to the other(s) in Cycle 3. This is our motivation for having a timing constraint. Generally the constraint covers the full interval of the brightest window in the Cycle. COMMENT_END: AOT_TYPE: IRS Peakup Image AOR_LABEL: seppcon-127P-HO AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: Holt-Olmstead EPHEMERIS: NAIF_ID=1000127, NAIF_NAME=Holt-Olmstead OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES RED: EXPOSURE_TIME=14, N_CYCLES_SEQ=6 BLUE: EXPOSURE_TIME=14, N_CYCLES_SEQ=14 DITHER_PATTERN: TYPE=5Positions DITHER_SCALE: small SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=2569.0, SLEW_TIME=17.4, SETTLE_TIME=54.0, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=918, DOWNLINK_VOLUME=24658315, VERSION=S14.1.0 INTEGRATION_TIME: IRS_RED=440.40192,IRS_BLUE=1027.6045 TIMING1: START_DATE=2006 Jun 20, START_TIME=00:00:00, END_DATE=2006 Jul 24, END_TIME=11:42:00 TIMING2: START_DATE=2007 Feb 25, START_TIME=16:32:00, END_DATE=2007 Apr 6, END_TIME=02:09:00 COMMENT_START: In almost all cases, a given comet is brighter in one observability window compared to the other(s) in Cycle 3. This is our motivation for having a timing constraint. Generally the constraint covers the full interval of the brightest window in the Cycle. COMMENT_END: AOT_TYPE: IRS Peakup Image AOR_LABEL: seppcon-79P-dTH AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: du Toit-Hartley EPHEMERIS: NAIF_ID=1000022, NAIF_NAME=du Toit-Hartley OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES RED: EXPOSURE_TIME=14, N_CYCLES_SEQ=6 BLUE: EXPOSURE_TIME=14, N_CYCLES_SEQ=15 DITHER_PATTERN: TYPE=5Positions DITHER_SCALE: small SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=2679.0, SLEW_TIME=17.4, SETTLE_TIME=54.0, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=918, DOWNLINK_VOLUME=25891230, VERSION=S14.1.0 INTEGRATION_TIME: IRS_RED=440.40192,IRS_BLUE=1101.0048 TIMING1: START_DATE=2006 Aug 31, START_TIME=20:22:00, END_DATE=2006 Oct 9, END_TIME=12:31:00 COMMENT_START: In almost all cases, a given comet is brighter in one observability window compared to the other(s) in Cycle 3. This is our motivation for having a timing constraint. Generally the constraint covers the full interval of the brightest window in the Cycle. COMMENT_END: AOT_TYPE: IRS Peakup Image AOR_LABEL: seppcon-131P-M2 AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: Mueller 2 EPHEMERIS: NAIF_ID=1000123, NAIF_NAME=Mueller 2 OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES RED: EXPOSURE_TIME=14, N_CYCLES_SEQ=6 BLUE: EXPOSURE_TIME=14, N_CYCLES_SEQ=15 DITHER_PATTERN: TYPE=5Positions DITHER_SCALE: small SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=2679.0, SLEW_TIME=17.4, SETTLE_TIME=54.0, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=918, DOWNLINK_VOLUME=25891230, VERSION=S14.1.0 INTEGRATION_TIME: IRS_RED=440.40192,IRS_BLUE=1101.0048 TIMING1: START_DATE=2007 Jan 13, START_TIME=06:58:00, END_DATE=2007 Feb 21, END_TIME=21:08:00 COMMENT_START: In almost all cases, a given comet is brighter in one observability window compared to the other(s) in Cycle 3. This is our motivation for having a timing constraint. Generally the constraint covers the full interval of the brightest window in the Cycle. COMMENT_END: AOT_TYPE: IRS Peakup Image AOR_LABEL: seppcon-33P-Daniel AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: Daniel EPHEMERIS: NAIF_ID=1000018, NAIF_NAME=Daniel OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES RED: EXPOSURE_TIME=14, N_CYCLES_SEQ=6 BLUE: EXPOSURE_TIME=14, N_CYCLES_SEQ=16 DITHER_PATTERN: TYPE=5Positions DITHER_SCALE: small SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=2789.0, SLEW_TIME=17.4, SETTLE_TIME=54.0, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=918, DOWNLINK_VOLUME=27124145, VERSION=S14.1.0 INTEGRATION_TIME: IRS_RED=440.40192,IRS_BLUE=1174.4052 TIMING1: START_DATE=2006 Oct 12, START_TIME=06:26:00, END_DATE=2006 Nov 25, END_TIME=20:42:00 COMMENT_START: In almost all cases, a given comet is brighter in one observability window compared to the other(s) in Cycle 3. This is our motivation for having a timing constraint. Generally the constraint covers the full interval of the brightest window in the Cycle. COMMENT_END: AOT_TYPE: IRS Peakup Image AOR_LABEL: seppcon-P04V5-LINHill AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: LINEAR-Hill (P/2004 V5-A) EPHEMERIS: NAIF_ID=1000527, NAIF_NAME=LINEAR-Hill (P/2004 V5-A) OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES RED: EXPOSURE_TIME=14, N_CYCLES_SEQ=6 BLUE: EXPOSURE_TIME=14, N_CYCLES_SEQ=17 DITHER_PATTERN: TYPE=5Positions DITHER_SCALE: small SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=2899.0, SLEW_TIME=17.4, SETTLE_TIME=54.0, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=918, DOWNLINK_VOLUME=28357060, VERSION=S14.1.0 INTEGRATION_TIME: IRS_RED=440.40192,IRS_BLUE=1247.8054 TIMING1: START_DATE=2006 Jun 20, START_TIME=00:00:00, END_DATE=2006 Jul 21, END_TIME=16:04:00 TIMING2: START_DATE=2007 Feb 20, START_TIME=05:37:00, END_DATE=2007 Mar 31, END_TIME=07:57:00 COMMENT_START: In almost all cases, a given comet is brighter in one observability window compared to the other(s) in Cycle 3. This is our motivation for having a timing constraint. Generally the constraint covers the full interval of the brightest window in the Cycle. COMMENT_END: AOT_TYPE: IRS Peakup Image AOR_LABEL: seppcon-P03S1-NEAT AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: NEAT (P/2003 S1) EPHEMERIS: NAIF_ID=1000453, NAIF_NAME=NEAT (P/2003 S1) OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES RED: EXPOSURE_TIME=14, N_CYCLES_SEQ=6 BLUE: EXPOSURE_TIME=14, N_CYCLES_SEQ=17 DITHER_PATTERN: TYPE=5Positions DITHER_SCALE: small SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=2899.0, SLEW_TIME=17.4, SETTLE_TIME=54.0, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=918, DOWNLINK_VOLUME=28357060, VERSION=S14.1.0 INTEGRATION_TIME: IRS_RED=440.40192,IRS_BLUE=1247.8054 TIMING1: START_DATE=2006 Jun 20, START_TIME=00:00:00, END_DATE=2006 Jul 14, END_TIME=10:20:00 TIMING2: START_DATE=2007 Feb 9, START_TIME=03:50:00, END_DATE=2007 Mar 19, END_TIME=14:43:00 COMMENT_START: In almost all cases, a given comet is brighter in one observability window compared to the other(s) in Cycle 3. This is our motivation for having a timing constraint. Generally the constraint covers the full interval of the brightest window in the Cycle. COMMENT_END: AOT_TYPE: IRS Peakup Image AOR_LABEL: seppcon-130P-McNH AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: McNaught-Hughes EPHEMERIS: NAIF_ID=1000134, NAIF_NAME=McNaught-Hughes OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES RED: EXPOSURE_TIME=14, N_CYCLES_SEQ=7 BLUE: EXPOSURE_TIME=14, N_CYCLES_SEQ=17 DITHER_PATTERN: TYPE=5Positions DITHER_SCALE: small SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=3009.0, SLEW_TIME=17.4, SETTLE_TIME=54.0, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=918, DOWNLINK_VOLUME=29589975, VERSION=S14.1.0 INTEGRATION_TIME: IRS_RED=513.80225,IRS_BLUE=1247.8054 TIMING1: START_DATE=2006 Oct 28, START_TIME=10:55:00, END_DATE=2006 Dec 7, END_TIME=17:30:00 COMMENT_START: In almost all cases, a given comet is brighter in one observability window compared to the other(s) in Cycle 3. This is our motivation for having a timing constraint. Generally the constraint covers the full interval of the brightest window in the Cycle. COMMENT_END: AOT_TYPE: IRS Peakup Image AOR_LABEL: seppcon-77P-Longm AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: Longmore EPHEMERIS: NAIF_ID=1000059, NAIF_NAME=Longmore OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES RED: EXPOSURE_TIME=14, N_CYCLES_SEQ=8 BLUE: EXPOSURE_TIME=14, N_CYCLES_SEQ=22 DITHER_PATTERN: TYPE=5Positions DITHER_SCALE: small SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=3669.0, SLEW_TIME=17.4, SETTLE_TIME=54.0, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=918, DOWNLINK_VOLUME=36987470, VERSION=S14.1.0 INTEGRATION_TIME: IRS_RED=587.2026,IRS_BLUE=1614.807 TIMING1: START_DATE=2006 Sep 20, START_TIME=00:00:00, END_DATE=2006 Oct 12, END_TIME=21:44:00 TIMING2: START_DATE=2007 Jan 28, START_TIME=14:52:00, END_DATE=2007 Mar 10, END_TIME=15:17:00 COMMENT_START: In almost all cases, a given comet is brighter in one observability window compared to the other(s) in Cycle 3. This is our motivation for having a timing constraint. Generally the constraint covers the full interval of the brightest window in the Cycle. COMMENT_END: AOT_TYPE: IRS Peakup Image AOR_LABEL: seppcon-22P-K AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: Kopff EPHEMERIS: NAIF_ID=1000054, NAIF_NAME=Kopff OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES RED: EXPOSURE_TIME=14, N_CYCLES_SEQ=8 BLUE: EXPOSURE_TIME=14, N_CYCLES_SEQ=23 DITHER_PATTERN: TYPE=5Positions DITHER_SCALE: small SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=3779.0, SLEW_TIME=17.4, SETTLE_TIME=54.0, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=918, DOWNLINK_VOLUME=38220385, VERSION=S14.1.0 INTEGRATION_TIME: IRS_RED=587.2026,IRS_BLUE=1688.2074 TIMING1: START_DATE=2007 Apr 13, START_TIME=00:16:00, END_DATE=2007 May 21, END_TIME=12:59:00 COMMENT_START: In almost all cases, a given comet is brighter in one observability window compared to the other(s) in Cycle 3. This is our motivation for having a timing constraint. Generally the constraint covers the full interval of the brightest window in the Cycle. COMMENT_END: AOT_TYPE: IRS Peakup Image AOR_LABEL: seppcon-P04VR8-LONEOS AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: LONEOS (P/2004 VR8) EPHEMERIS: NAIF_ID=1000532, NAIF_NAME=LONEOS (P/2004 VR8) OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES RED: EXPOSURE_TIME=14, N_CYCLES_SEQ=9 BLUE: EXPOSURE_TIME=14, N_CYCLES_SEQ=24 DITHER_PATTERN: TYPE=5Positions DITHER_SCALE: small SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=4000.0, SLEW_TIME=17.4, SETTLE_TIME=54.0, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=925, DOWNLINK_VOLUME=40686220, VERSION=S14.1.0 INTEGRATION_TIME: IRS_RED=660.6029,IRS_BLUE=1761.6077 TIMING1: START_DATE=2006 Jul 27, START_TIME=00:00:00, END_DATE=2006 Aug 12, END_TIME=16:29:00 COMMENT_START: In almost all cases, a given comet is brighter in one observability window compared to the other(s) in Cycle 3. This is our motivation for having a timing constraint. Generally the constraint covers the full interval of the brightest window in the Cycle. COMMENT_END: AOT_TYPE: IRS Peakup Image AOR_LABEL: seppcon-43P-WoH AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: Wolf-Harrington EPHEMERIS: NAIF_ID=1000111, NAIF_NAME=Wolf-Harrington OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES RED: EXPOSURE_TIME=14, N_CYCLES_SEQ=9 BLUE: EXPOSURE_TIME=14, N_CYCLES_SEQ=28 DITHER_PATTERN: TYPE=5Positions DITHER_SCALE: small SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=4440.0, SLEW_TIME=17.4, SETTLE_TIME=54.0, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=925, DOWNLINK_VOLUME=45617880, VERSION=S14.1.0 INTEGRATION_TIME: IRS_RED=660.6029,IRS_BLUE=2055.209 TIMING1: START_DATE=2006 Aug 5, START_TIME=18:05:00, END_DATE=2006 Sep 14, END_TIME=22:21:00 TIMING2: START_DATE=2007 May 1, START_TIME=12:00:00, END_DATE=2007 May 16, END_TIME=15:42:00 COMMENT_START: In almost all cases, a given comet is brighter in one observability window compared to the other(s) in Cycle 3. This is our motivation for having a timing constraint. Generally the constraint covers the full interval of the brightest window in the Cycle. COMMENT_END: AOT_TYPE: IRS Peakup Image AOR_LABEL: seppcon-94P-Rus4 AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: Russell 4 EPHEMERIS: NAIF_ID=1000075, NAIF_NAME=Russell 4 OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES RED: EXPOSURE_TIME=14, N_CYCLES_SEQ=11 BLUE: EXPOSURE_TIME=14, N_CYCLES_SEQ=28 DITHER_PATTERN: TYPE=5Positions DITHER_SCALE: small SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=4660.0, SLEW_TIME=17.4, SETTLE_TIME=54.0, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=925, DOWNLINK_VOLUME=48083710, VERSION=S14.1.0 INTEGRATION_TIME: IRS_RED=807.4035,IRS_BLUE=2055.209 TIMING1: START_DATE=2006 Jun 20, START_TIME=00:00:00, END_DATE=2006 Jul 25, END_TIME=02:29:00 TIMING2: START_DATE=2006 Nov 14, START_TIME=16:31:00, END_DATE=2006 Dec 10, END_TIME=12:00:00 COMMENT_START: In almost all cases, a given comet is brighter in one observability window compared to the other(s) in Cycle 3. This is our motivation for having a timing constraint. Generally the constraint covers the full interval of the brightest window in the Cycle. COMMENT_END: AOT_TYPE: IRS Peakup Image AOR_LABEL: seppcon-89P-Rus2 AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: Russell 2 EPHEMERIS: NAIF_ID=1000073, NAIF_NAME=Russell 2 OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES RED: EXPOSURE_TIME=14, N_CYCLES_SEQ=11 BLUE: EXPOSURE_TIME=14, N_CYCLES_SEQ=30 DITHER_PATTERN: TYPE=5Positions DITHER_SCALE: small SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=4880.0, SLEW_TIME=17.4, SETTLE_TIME=54.0, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=925, DOWNLINK_VOLUME=50549545, VERSION=S14.1.0 INTEGRATION_TIME: IRS_RED=807.4035,IRS_BLUE=2202.0095 TIMING1: START_DATE=2007 Jan 8, START_TIME=12:00:00, END_DATE=2007 Jan 14, END_TIME=05:58:00 TIMING2: START_DATE=2007 May 1, START_TIME=08:01:00, END_DATE=2007 Jun 10, END_TIME=18:21:00 COMMENT_START: In almost all cases, a given comet is brighter in one observability window compared to the other(s) in Cycle 3. This is our motivation for having a timing constraint. Generally the constraint covers the full interval of the brightest window in the Cycle. COMMENT_END: AOT_TYPE: IRS Peakup Image AOR_LABEL: seppcon-32P-CS AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: Comas Sola EPHEMERIS: NAIF_ID=1000015, NAIF_NAME=Comas Sola OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES RED: EXPOSURE_TIME=14, N_CYCLES_SEQ=14 BLUE: EXPOSURE_TIME=14, N_CYCLES_SEQ=32 DITHER_PATTERN: TYPE=5Positions DITHER_SCALE: small SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=5430.0, SLEW_TIME=17.4, SETTLE_TIME=54.0, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=925, DOWNLINK_VOLUME=56714125, VERSION=S14.1.0 INTEGRATION_TIME: IRS_RED=1027.6045,IRS_BLUE=2348.8103 TIMING1: START_DATE=2006 Jul 15, START_TIME=11:53:00, END_DATE=2006 Aug 26, END_TIME=14:37:00 COMMENT_START: In almost all cases, a given comet is brighter in one observability window compared to the other(s) in Cycle 3. This is our motivation for having a timing constraint. Generally the constraint covers the full interval of the brightest window in the Cycle. COMMENT_END: AOT_TYPE: IRS Peakup Image AOR_LABEL: seppcon-163P-NEAT AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: NEAT EPHEMERIS: NAIF_ID=1000521, NAIF_NAME=NEAT OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES RED: EXPOSURE_TIME=14, N_CYCLES_SEQ=15 BLUE: EXPOSURE_TIME=14, N_CYCLES_SEQ=32 DITHER_PATTERN: TYPE=5Positions DITHER_SCALE: small SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=5540.0, SLEW_TIME=17.4, SETTLE_TIME=54.0, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=925, DOWNLINK_VOLUME=57947040, VERSION=S14.1.0 INTEGRATION_TIME: IRS_RED=1101.0048,IRS_BLUE=2348.8103 TIMING1: START_DATE=2006 Jul 15, START_TIME=00:00:00, END_DATE=2006 Aug 16, END_TIME=08:21:00 COMMENT_START: In almost all cases, a given comet is brighter in one observability window compared to the other(s) in Cycle 3. This is our motivation for having a timing constraint. Generally the constraint covers the full interval of the brightest window in the Cycle. COMMENT_END: AOT_TYPE: IRS Peakup Image AOR_LABEL: seppcon-P04V3-SidSpr AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: Siding Spring (P/2004 V3) EPHEMERIS: NAIF_ID=1000520, NAIF_NAME=Siding Spring (P/2004 V3) OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES RED: EXPOSURE_TIME=14, N_CYCLES_SEQ=10 BLUE: EXPOSURE_TIME=14, N_CYCLES_SEQ=32 DITHER_PATTERN: TYPE=5Positions DITHER_SCALE: small SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=4990.0, SLEW_TIME=17.4, SETTLE_TIME=54.0, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=925, DOWNLINK_VOLUME=51782460, VERSION=S14.1.0 INTEGRATION_TIME: IRS_RED=734.00323,IRS_BLUE=2348.8103 TIMING1: START_DATE=2006 Aug 10, START_TIME=18:17:00, END_DATE=2006 Sep 30, END_TIME=03:03:00 COMMENT_START: In almost all cases, a given comet is brighter in one observability window compared to the other(s) in Cycle 3. This is our motivation for having a timing constraint. Generally the constraint covers the full interval of the brightest window in the Cycle. COMMENT_END: AOT_TYPE: IRS Peakup Image AOR_LABEL: seppcon-120P-M1 AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: Mueller 1 EPHEMERIS: NAIF_ID=1000116, NAIF_NAME=Mueller 1 OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES RED: EXPOSURE_TIME=14, N_CYCLES_SEQ=12 BLUE: EXPOSURE_TIME=14, N_CYCLES_SEQ=33 DITHER_PATTERN: TYPE=5Positions DITHER_SCALE: small SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=5320.0, SLEW_TIME=17.4, SETTLE_TIME=54.0, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=925, DOWNLINK_VOLUME=55481210, VERSION=S14.1.0 INTEGRATION_TIME: IRS_RED=880.80383,IRS_BLUE=2422.2104 TIMING1: START_DATE=2007 Jan 6, START_TIME=00:10:00, END_DATE=2007 Feb 14, END_TIME=09:19:00 COMMENT_START: In almost all cases, a given comet is brighter in one observability window compared to the other(s) in Cycle 3. This is our motivation for having a timing constraint. Generally the constraint covers the full interval of the brightest window in the Cycle. COMMENT_END: AOT_TYPE: IRS Peakup Image AOR_LABEL: seppcon-P02X2-NEAT AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: NEAT (P/2002 X2) EPHEMERIS: NAIF_ID=1000422, NAIF_NAME=NEAT (P/2002 X2) OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES RED: EXPOSURE_TIME=14, N_CYCLES_SEQ=11 BLUE: EXPOSURE_TIME=14, N_CYCLES_SEQ=34 DITHER_PATTERN: TYPE=5Positions DITHER_SCALE: small SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=5320.0, SLEW_TIME=17.4, SETTLE_TIME=54.0, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=925, DOWNLINK_VOLUME=55481205, VERSION=S14.1.0 INTEGRATION_TIME: IRS_RED=807.4035,IRS_BLUE=2495.6108 TIMING1: START_DATE=2006 Jul 31, START_TIME=05:52:00, END_DATE=2006 Sep 10, END_TIME=02:01:00 TIMING2: START_DATE=2007 Apr 4, START_TIME=09:34:00, END_DATE=2007 May 11, END_TIME=10:30:00 COMMENT_START: In almost all cases, a given comet is brighter in one observability window compared to the other(s) in Cycle 3. This is our motivation for having a timing constraint. Generally the constraint covers the full interval of the brightest window in the Cycle. COMMENT_END: AOT_TYPE: IRS Peakup Image AOR_LABEL: seppcon-P04DO29-SpL AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: Spacewatch-LINEAR (P/2004 DO29) EPHEMERIS: NAIF_ID=1000481, NAIF_NAME=Spacewatch-LINEAR (P/2004 DO29) OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES RED: EXPOSURE_TIME=14, N_CYCLES_SEQ=12 BLUE: EXPOSURE_TIME=14, N_CYCLES_SEQ=39 DITHER_PATTERN: TYPE=5Positions DITHER_SCALE: small SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=5981.0, SLEW_TIME=17.4, SETTLE_TIME=54.0, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=937, DOWNLINK_VOLUME=62878705, VERSION=S14.1.0 INTEGRATION_TIME: IRS_RED=880.80383,IRS_BLUE=2862.6125 TIMING1: START_DATE=2006 Aug 31, START_TIME=11:42:00, END_DATE=2006 Oct 13, END_TIME=09:20:00 COMMENT_START: In almost all cases, a given comet is brighter in one observability window compared to the other(s) in Cycle 3. This is our motivation for having a timing constraint. Generally the constraint covers the full interval of the brightest window in the Cycle. COMMENT_END: AOT_TYPE: IRS Peakup Image AOR_LABEL: seppcon-P05JQ5-Cata AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: Catalina (P/2005 JQ5) EPHEMERIS: NAIF_ID=1000567, NAIF_NAME=Catalina (P/2005 JQ5) OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES RED: EXPOSURE_TIME=14, N_CYCLES_SEQ=17 BLUE: EXPOSURE_TIME=14, N_CYCLES_SEQ=39 DITHER_PATTERN: TYPE=5Positions DITHER_SCALE: small SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=6531.0, SLEW_TIME=17.4, SETTLE_TIME=54.0, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=937, DOWNLINK_VOLUME=69043280, VERSION=S14.1.0 INTEGRATION_TIME: IRS_RED=1247.8054,IRS_BLUE=2862.6125 TIMING1: START_DATE=2006 Nov 20, START_TIME=03:14:00, END_DATE=2006 Dec 29, END_TIME=00:01:00 COMMENT_START: In almost all cases, a given comet is brighter in one observability window compared to the other(s) in Cycle 3. This is our motivation for having a timing constraint. Generally the constraint covers the full interval of the brightest window in the Cycle. COMMENT_END: AOT_TYPE: IRS Peakup Image AOR_LABEL: seppcon-113P-Spi AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: Spitaler EPHEMERIS: NAIF_ID=1000146, NAIF_NAME=Spitaler OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES RED: EXPOSURE_TIME=14, N_CYCLES_SEQ=17 BLUE: EXPOSURE_TIME=14, N_CYCLES_SEQ=39 DITHER_PATTERN: TYPE=5Positions DITHER_SCALE: small SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=6531.0, SLEW_TIME=17.4, SETTLE_TIME=54.0, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=937, DOWNLINK_VOLUME=69043280, VERSION=S14.1.0 INTEGRATION_TIME: IRS_RED=1247.8054,IRS_BLUE=2862.6125 TIMING1: START_DATE=2006 Sep 30, START_TIME=18:17:00, END_DATE=2006 Nov 11, END_TIME=12:37:00 COMMENT_START: In almost all cases, a given comet is brighter in one observability window compared to the other(s) in Cycle 3. This is our motivation for having a timing constraint. Generally the constraint covers the full interval of the brightest window in the Cycle. COMMENT_END: AOT_TYPE: IRS Peakup Image AOR_LABEL: seppcon-50P-Ar AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: Arend EPHEMERIS: NAIF_ID=1000001, NAIF_NAME=Arend OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES RED: EXPOSURE_TIME=14, N_CYCLES_SEQ=17 BLUE: EXPOSURE_TIME=14, N_CYCLES_SEQ=40 DITHER_PATTERN: TYPE=5Positions DITHER_SCALE: small SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=6641.0, SLEW_TIME=17.4, SETTLE_TIME=54.0, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=937, DOWNLINK_VOLUME=70276195, VERSION=S14.1.0 INTEGRATION_TIME: IRS_RED=1247.8054,IRS_BLUE=2936.013 TIMING1: START_DATE=2006 Sep 19, START_TIME=11:09:00, END_DATE=2006 Nov 2, END_TIME=23:34:00 COMMENT_START: In almost all cases, a given comet is brighter in one observability window compared to the other(s) in Cycle 3. This is our motivation for having a timing constraint. Generally the constraint covers the full interval of the brightest window in the Cycle. COMMENT_END: AOT_TYPE: IRS Peakup Image AOR_LABEL: seppcon-54P-dVSN AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: de Vico-Swift-NEAT EPHEMERIS: NAIF_ID=1000414, NAIF_NAME=de Vico-Swift-NEAT OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES RED: EXPOSURE_TIME=14, N_CYCLES_SEQ=14 BLUE: EXPOSURE_TIME=14, N_CYCLES_SEQ=41 DITHER_PATTERN: TYPE=5Positions DITHER_SCALE: small SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=6421.0, SLEW_TIME=17.4, SETTLE_TIME=54.0, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=937, DOWNLINK_VOLUME=67810365, VERSION=S14.1.0 INTEGRATION_TIME: IRS_RED=1027.6045,IRS_BLUE=3009.413 TIMING1: START_DATE=2007 Feb 9, START_TIME=04:08:00, END_DATE=2007 Mar 19, END_TIME=23:41:00 COMMENT_START: In almost all cases, a given comet is brighter in one observability window compared to the other(s) in Cycle 3. This is our motivation for having a timing constraint. Generally the constraint covers the full interval of the brightest window in the Cycle. COMMENT_END: AOT_TYPE: IRS Peakup Image AOR_LABEL: seppcon-124P-Mrkos AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: Mrkos EPHEMERIS: NAIF_ID=1000142, NAIF_NAME=Mrkos OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES RED: EXPOSURE_TIME=14, N_CYCLES_SEQ=19 BLUE: EXPOSURE_TIME=14, N_CYCLES_SEQ=44 DITHER_PATTERN: TYPE=5Positions DITHER_SCALE: small SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=7301.0, SLEW_TIME=17.4, SETTLE_TIME=54.0, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=937, DOWNLINK_VOLUME=77673695, VERSION=S14.1.0 INTEGRATION_TIME: IRS_RED=1394.606,IRS_BLUE=3229.614 TIMING1: START_DATE=2006 Aug 15, START_TIME=03:41:00, END_DATE=2006 Sep 27, END_TIME=06:38:00 COMMENT_START: In almost all cases, a given comet is brighter in one observability window compared to the other(s) in Cycle 3. This is our motivation for having a timing constraint. Generally the constraint covers the full interval of the brightest window in the Cycle. COMMENT_END: AOT_TYPE: IRS Peakup Image AOR_LABEL: seppcon-37P-F AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: Forbes EPHEMERIS: NAIF_ID=1000028, NAIF_NAME=Forbes OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES RED: EXPOSURE_TIME=14, N_CYCLES_SEQ=19 BLUE: EXPOSURE_TIME=14, N_CYCLES_SEQ=45 DITHER_PATTERN: TYPE=5Positions DITHER_SCALE: small SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=7411.0, SLEW_TIME=17.4, SETTLE_TIME=54.0, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=937, DOWNLINK_VOLUME=78906610, VERSION=S14.1.0 INTEGRATION_TIME: IRS_RED=1394.606,IRS_BLUE=3303.0146 TIMING1: START_DATE=2007 Feb 8, START_TIME=02:04:00, END_DATE=2007 Mar 20, END_TIME=04:54:00 COMMENT_START: In almost all cases, a given comet is brighter in one observability window compared to the other(s) in Cycle 3. This is our motivation for having a timing constraint. Generally the constraint covers the full interval of the brightest window in the Cycle. COMMENT_END: AOT_TYPE: IRS Peakup Image AOR_LABEL: seppcon-159P-LONEOS AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: LONEOS EPHEMERIS: NAIF_ID=1000470, NAIF_NAME=LONEOS OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES RED: EXPOSURE_TIME=14, N_CYCLES_SEQ=14 BLUE: EXPOSURE_TIME=14, N_CYCLES_SEQ=45 DITHER_PATTERN: TYPE=5Positions DITHER_SCALE: small SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=6861.0, SLEW_TIME=17.4, SETTLE_TIME=54.0, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=937, DOWNLINK_VOLUME=72742030, VERSION=S14.1.0 INTEGRATION_TIME: IRS_RED=1027.6045,IRS_BLUE=3303.0146 TIMING1: START_DATE=2007 Jan 15, START_TIME=19:30:00, END_DATE=2007 Feb 26, END_TIME=15:29:00 COMMENT_START: In almost all cases, a given comet is brighter in one observability window compared to the other(s) in Cycle 3. This is our motivation for having a timing constraint. Generally the constraint covers the full interval of the brightest window in the Cycle. COMMENT_END: AOT_TYPE: IRS Peakup Image AOR_LABEL: seppcon-57P-dTND AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: duToit-Neujmin-Delporte EPHEMERIS: NAIF_ID=1000397, NAIF_NAME=duToit-Neujmin-Delporte OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES RED: EXPOSURE_TIME=14, N_CYCLES_SEQ=20 BLUE: EXPOSURE_TIME=14, N_CYCLES_SEQ=46 DITHER_PATTERN: TYPE=5Positions DITHER_SCALE: small SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=7631.0, SLEW_TIME=17.4, SETTLE_TIME=54.0, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=937, DOWNLINK_VOLUME=81372440, VERSION=S14.1.0 INTEGRATION_TIME: IRS_RED=1468.0065,IRS_BLUE=3376.4148 TIMING1: START_DATE=2007 May 19, START_TIME=00:57:00, END_DATE=2007 Jun 27, END_TIME=14:09:00 COMMENT_START: In almost all cases, a given comet is brighter in one observability window compared to the other(s) in Cycle 3. This is our motivation for having a timing constraint. Generally the constraint covers the full interval of the brightest window in the Cycle. COMMENT_END: AOT_TYPE: IRS Peakup Image AOR_LABEL: seppcon-132P-HRA2 AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: Helin-Roman-Alu 2 EPHEMERIS: NAIF_ID=1000133, NAIF_NAME=Helin-Roman-Alu 2 OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES RED: EXPOSURE_TIME=14, N_CYCLES_SEQ=21 BLUE: EXPOSURE_TIME=14, N_CYCLES_SEQ=46 DITHER_PATTERN: TYPE=5Positions DITHER_SCALE: small SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=7741.0, SLEW_TIME=17.4, SETTLE_TIME=54.0, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=937, DOWNLINK_VOLUME=82605355, VERSION=S14.1.0 INTEGRATION_TIME: IRS_RED=1541.4067,IRS_BLUE=3376.4148 TIMING1: START_DATE=2007 May 20, START_TIME=00:00:00, END_DATE=2007 Jun 20, END_TIME=07:09:00 COMMENT_START: In almost all cases, a given comet is brighter in one observability window compared to the other(s) in Cycle 3. This is our motivation for having a timing constraint. Generally the constraint covers the full interval of the brightest window in the Cycle. COMMENT_END: AOT_TYPE: IRS Peakup Image AOR_LABEL: seppcon-149P-M4 AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: Mueller 4 EPHEMERIS: NAIF_ID=1000139, NAIF_NAME=Mueller 4 OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES RED: EXPOSURE_TIME=14, N_CYCLES_SEQ=14 BLUE: EXPOSURE_TIME=14, N_CYCLES_SEQ=47 DITHER_PATTERN: TYPE=5Positions DITHER_SCALE: small SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=7081.0, SLEW_TIME=17.4, SETTLE_TIME=54.0, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=937, DOWNLINK_VOLUME=75207860, VERSION=S14.1.0 INTEGRATION_TIME: IRS_RED=1027.6045,IRS_BLUE=3449.815 TIMING1: START_DATE=2006 Sep 1, START_TIME=12:00:00, END_DATE=2006 Sep 25, END_TIME=00:20:00 TIMING2: START_DATE=2007 Jan 3, START_TIME=17:40:00, END_DATE=2007 Feb 18, END_TIME=04:07:00 COMMENT_START: In almost all cases, a given comet is brighter in one observability window compared to the other(s) in Cycle 3. This is our motivation for having a timing constraint. Generally the constraint covers the full interval of the brightest window in the Cycle. COMMENT_END: AOT_TYPE: IRS Peakup Image AOR_LABEL: seppcon-146P-ShLIN AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: Shoemaker-LINEAR EPHEMERIS: NAIF_ID=1000084, NAIF_NAME=Shoemaker-LINEAR OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES RED: EXPOSURE_TIME=14, N_CYCLES_SEQ=22 BLUE: EXPOSURE_TIME=14, N_CYCLES_SEQ=47 DITHER_PATTERN: TYPE=5Positions DITHER_SCALE: small SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=7961.0, SLEW_TIME=17.4, SETTLE_TIME=54.0, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=937, DOWNLINK_VOLUME=85071185, VERSION=S14.1.0 INTEGRATION_TIME: IRS_RED=1614.807,IRS_BLUE=3449.815 TIMING1: START_DATE=2006 Jul 13, START_TIME=23:58:00, END_DATE=2006 Aug 22, END_TIME=11:21:00 COMMENT_START: In almost all cases, a given comet is brighter in one observability window compared to the other(s) in Cycle 3. This is our motivation for having a timing constraint. Generally the constraint covers the full interval of the brightest window in the Cycle. COMMENT_END: AOT_TYPE: IRS Peakup Image AOR_LABEL: seppcon-162P-SidSpr AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: Siding Spring EPHEMERIS: NAIF_ID=1000525, NAIF_NAME=Siding Spring OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES RED: EXPOSURE_TIME=14, N_CYCLES_SEQ=21 BLUE: EXPOSURE_TIME=14, N_CYCLES_SEQ=49 DITHER_PATTERN: TYPE=5Positions DITHER_SCALE: small SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=8076.0, SLEW_TIME=17.4, SETTLE_TIME=54.0, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=937, DOWNLINK_VOLUME=86304105, VERSION=S14.1.0 INTEGRATION_TIME: IRS_RED=1541.4067,IRS_BLUE=3596.6157 TIMING1: START_DATE=2006 Jun 20, START_TIME=00:00:00, END_DATE=2006 Jul 11, END_TIME=03:11:00 TIMING2: START_DATE=2007 Feb 9, START_TIME=18:09:00, END_DATE=2007 Mar 19, END_TIME=22:20:00 COMMENT_START: In almost all cases, a given comet is brighter in one observability window compared to the other(s) in Cycle 3. This is our motivation for having a timing constraint. Generally the constraint covers the full interval of the brightest window in the Cycle. COMMENT_END: AOT_TYPE: IRS Peakup Image AOR_LABEL: seppcon-69P-Taylor AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: Taylor EPHEMERIS: NAIF_ID=1000092, NAIF_NAME=Taylor OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES RED: EXPOSURE_TIME=14, N_CYCLES_SEQ=21 BLUE: EXPOSURE_TIME=14, N_CYCLES_SEQ=49 DITHER_PATTERN: TYPE=5Positions DITHER_SCALE: small SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=8076.0, SLEW_TIME=17.4, SETTLE_TIME=54.0, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=937, DOWNLINK_VOLUME=86304105, VERSION=S14.1.0 INTEGRATION_TIME: IRS_RED=1541.4067,IRS_BLUE=3596.6157 TIMING1: START_DATE=2006 Jul 27, START_TIME=18:56:00, END_DATE=2006 Sep 9, END_TIME=19:35:00 COMMENT_START: In almost all cases, a given comet is brighter in one observability window compared to the other(s) in Cycle 3. This is our motivation for having a timing constraint. Generally the constraint covers the full interval of the brightest window in the Cycle. COMMENT_END: AOT_TYPE: IRS Peakup Image AOR_LABEL: seppcon-141P-Mach2 AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: Machholz 2 EPHEMERIS: NAIF_ID=1000152, NAIF_NAME=Machholz 2 OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES RED: EXPOSURE_TIME=14, N_CYCLES_SEQ=21 BLUE: EXPOSURE_TIME=14, N_CYCLES_SEQ=50 DITHER_PATTERN: TYPE=5Positions DITHER_SCALE: small SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=8186.0, SLEW_TIME=17.4, SETTLE_TIME=54.0, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=937, DOWNLINK_VOLUME=87537020, VERSION=S14.1.0 INTEGRATION_TIME: IRS_RED=1541.4067,IRS_BLUE=3670.0159 TIMING1: START_DATE=2006 Jun 20, START_TIME=00:00:00, END_DATE=2006 Jul 20, END_TIME=07:30:00 TIMING2: START_DATE=2007 Feb 15, START_TIME=07:50:00, END_DATE=2007 Mar 25, END_TIME=05:45:00 COMMENT_START: In almost all cases, a given comet is brighter in one observability window compared to the other(s) in Cycle 3. This is our motivation for having a timing constraint. Generally the constraint covers the full interval of the brightest window in the Cycle. COMMENT_END: AOT_TYPE: IRS Peakup Image AOR_LABEL: seppcon-P03S2-NEAT AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: NEAT (P/2003 S2) EPHEMERIS: NAIF_ID=1000454, NAIF_NAME=NEAT (P/2003 S2) OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES RED: EXPOSURE_TIME=14, N_CYCLES_SEQ=19 BLUE: EXPOSURE_TIME=14, N_CYCLES_SEQ=50 DITHER_PATTERN: TYPE=5Positions DITHER_SCALE: small SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=7966.0, SLEW_TIME=17.4, SETTLE_TIME=54.0, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=937, DOWNLINK_VOLUME=85071190, VERSION=S14.1.0 INTEGRATION_TIME: IRS_RED=1394.606,IRS_BLUE=3670.0159 TIMING1: START_DATE=2007 Jan 22, START_TIME=04:25:00, END_DATE=2007 Mar 2, END_TIME=13:07:00 COMMENT_START: In almost all cases, a given comet is brighter in one observability window compared to the other(s) in Cycle 3. This is our motivation for having a timing constraint. Generally the constraint covers the full interval of the brightest window in the Cycle. COMMENT_END: AOT_TYPE: IRS Peakup Image AOR_LABEL: seppcon-171P-Spahr AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: Spahr EPHEMERIS: NAIF_ID=1000239, NAIF_NAME=Spahr OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES RED: EXPOSURE_TIME=14, N_CYCLES_SEQ=23 BLUE: EXPOSURE_TIME=14, N_CYCLES_SEQ=50 DITHER_PATTERN: TYPE=5Positions DITHER_SCALE: small SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=8407.0, SLEW_TIME=17.4, SETTLE_TIME=54.0, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=944, DOWNLINK_VOLUME=90002850, VERSION=S14.1.0 INTEGRATION_TIME: IRS_RED=1688.2074,IRS_BLUE=3670.0159 TIMING1: START_DATE=2007 Mar 11, START_TIME=13:12:00, END_DATE=2007 Apr 22, END_TIME=05:26:00 COMMENT_START: In almost all cases, a given comet is brighter in one observability window compared to the other(s) in Cycle 3. This is our motivation for having a timing constraint. Generally the constraint covers the full interval of the brightest window in the Cycle. COMMENT_END: AOT_TYPE: IRS Peakup Image AOR_LABEL: seppcon-160P-LIN AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: LINEAR EPHEMERIS: NAIF_ID=1000511, NAIF_NAME=LINEAR OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES RED: EXPOSURE_TIME=14, N_CYCLES_SEQ=19 BLUE: EXPOSURE_TIME=14, N_CYCLES_SEQ=50 DITHER_PATTERN: TYPE=5Positions DITHER_SCALE: small SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=7966.0, SLEW_TIME=17.4, SETTLE_TIME=54.0, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=937, DOWNLINK_VOLUME=85071190, VERSION=S14.1.0 INTEGRATION_TIME: IRS_RED=1394.606,IRS_BLUE=3670.0159 TIMING1: START_DATE=2006 Dec 8, START_TIME=01:42:00, END_DATE=2007 Jan 16, END_TIME=07:01:00 COMMENT_START: In almost all cases, a given comet is brighter in one observability window compared to the other(s) in Cycle 3. This is our motivation for having a timing constraint. Generally the constraint covers the full interval of the brightest window in the Cycle. COMMENT_END: AOT_TYPE: IRS Peakup Image AOR_LABEL: seppcon-56P-SB AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: Slaughter-Burnham EPHEMERIS: NAIF_ID=1000087, NAIF_NAME=Slaughter-Burnham OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES RED: EXPOSURE_TIME=14, N_CYCLES_SEQ=18 BLUE: EXPOSURE_TIME=14, N_CYCLES_SEQ=50 DITHER_PATTERN: TYPE=5Positions DITHER_SCALE: small SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=7856.0, SLEW_TIME=17.4, SETTLE_TIME=54.0, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=937, DOWNLINK_VOLUME=83838275, VERSION=S14.1.0 INTEGRATION_TIME: IRS_RED=1321.2058,IRS_BLUE=3670.0159 TIMING1: START_DATE=2006 Dec 19, START_TIME=11:16:00, END_DATE=2007 Jan 27, END_TIME=14:35:00 COMMENT_START: In almost all cases, a given comet is brighter in one observability window compared to the other(s) in Cycle 3. This is our motivation for having a timing constraint. Generally the constraint covers the full interval of the brightest window in the Cycle. COMMENT_END: AOT_TYPE: IRS Peakup Image AOR_LABEL: seppcon-152P-HL AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: Helin-Lawrence EPHEMERIS: NAIF_ID=1000145, NAIF_NAME=Helin-Lawrence OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES RED: EXPOSURE_TIME=14, N_CYCLES_SEQ=17 BLUE: EXPOSURE_TIME=14, N_CYCLES_SEQ=50 DITHER_PATTERN: TYPE=5Positions DITHER_SCALE: small SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=7746.0, SLEW_TIME=17.4, SETTLE_TIME=54.0, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=937, DOWNLINK_VOLUME=82605355, VERSION=S14.1.0 INTEGRATION_TIME: IRS_RED=1247.8054,IRS_BLUE=3670.0159 TIMING1: START_DATE=2006 Sep 8, START_TIME=03:47:00, END_DATE=2006 Oct 18, END_TIME=18:04:00 TIMING2: START_DATE=2007 Feb 8, START_TIME=10:24:00, END_DATE=2007 Mar 9, END_TIME=12:00:00 COMMENT_START: In almost all cases, a given comet is brighter in one observability window compared to the other(s) in Cycle 3. This is our motivation for having a timing constraint. Generally the constraint covers the full interval of the brightest window in the Cycle. COMMENT_END: AOT_TYPE: IRS Peakup Image AOR_LABEL: seppcon-123P-WH AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: West-Hartley EPHEMERIS: NAIF_ID=1000164, NAIF_NAME=West-Hartley OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES RED: EXPOSURE_TIME=14, N_CYCLES_SEQ=21 BLUE: EXPOSURE_TIME=14, N_CYCLES_SEQ=50 DITHER_PATTERN: TYPE=5Positions DITHER_SCALE: small SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=8186.0, SLEW_TIME=17.4, SETTLE_TIME=54.0, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=937, DOWNLINK_VOLUME=87537020, VERSION=S14.1.0 INTEGRATION_TIME: IRS_RED=1541.4067,IRS_BLUE=3670.0159 TIMING1: START_DATE=2006 Oct 11, START_TIME=00:58:00, END_DATE=2006 Nov 22, END_TIME=02:41:00 COMMENT_START: In almost all cases, a given comet is brighter in one observability window compared to the other(s) in Cycle 3. This is our motivation for having a timing constraint. Generally the constraint covers the full interval of the brightest window in the Cycle. COMMENT_END: AOT_TYPE: MIPS Photometry AOR_LABEL: seppcon-P05S3-Read-1st AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: Read (P/2005 S3) EPHEMERIS: NAIF_ID=1001667, NAIF_NAME=Read (P/2005 S3) OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES MICRON_24: FIELD_SIZE = SMALL, EXPOSURE_TIME = 10, N_CYCLES = 1 SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=450.7, SLEW_TIME=5.0, SETTLE_TIME=8.0, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=674, DOWNLINK_VOLUME=3536102, VERSION=S14.1.0 INTEGRATION_TIME: MIPS_24=165.675,MIPS_70=0.0,MIPS_160=0.0 TIMING1: START_DATE=2007 Apr 27, START_TIME=20:09:00, END_DATE=2007 Jun 8, END_TIME=20:45:00 COMMENT_START: In almost all cases, a given comet is brighter in one observability window compared to the other(s) in Cycle 3. This is our motivation for having a timing constraint. Generally the constraint covers the full interval of the brightest window in the Cycle. COMMENT_END: AOT_TYPE: MIPS Photometry AOR_LABEL: seppcon-P05S3-Read-2nd AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: Read (P/2005 S3) EPHEMERIS: NAIF_ID=1001667, NAIF_NAME=Read (P/2005 S3) OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES MICRON_24: FIELD_SIZE = SMALL, EXPOSURE_TIME = 10, N_CYCLES = 1 SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=450.7, SLEW_TIME=5.0, SETTLE_TIME=8.0, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=674, DOWNLINK_VOLUME=3536102, VERSION=S14.1.0 INTEGRATION_TIME: MIPS_24=165.675,MIPS_70=0.0,MIPS_160=0.0 AOT_TYPE: MIPS Photometry AOR_LABEL: seppcon-P05T5-Brgtn-1st AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: Broughton (P/2005 T5) EPHEMERIS: NAIF_ID=1001674, NAIF_NAME=Broughton (P/2005 T5) OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES MICRON_24: FIELD_SIZE = SMALL, EXPOSURE_TIME = 10, N_CYCLES = 1 SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=450.7, SLEW_TIME=5.0, SETTLE_TIME=8.0, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=674, DOWNLINK_VOLUME=3536102, VERSION=S14.1.0 INTEGRATION_TIME: MIPS_24=165.675,MIPS_70=0.0,MIPS_160=0.0 TIMING1: START_DATE=2006 Sep 21, START_TIME=04:33:00, END_DATE=2006 Nov 1, END_TIME=15:59:00 COMMENT_START: In almost all cases, a given comet is brighter in one observability window compared to the other(s) in Cycle 3. This is our motivation for having a timing constraint. Generally the constraint covers the full interval of the brightest window in the Cycle. COMMENT_END: AOT_TYPE: MIPS Photometry AOR_LABEL: seppcon-P05T5-Brgtn-2nd AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: Broughton (P/2005 T5) EPHEMERIS: NAIF_ID=1001674, NAIF_NAME=Broughton (P/2005 T5) OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES MICRON_24: FIELD_SIZE = SMALL, EXPOSURE_TIME = 10, N_CYCLES = 1 SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=450.7, SLEW_TIME=5.0, SETTLE_TIME=8.0, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=674, DOWNLINK_VOLUME=3536102, VERSION=S14.1.0 INTEGRATION_TIME: MIPS_24=165.675,MIPS_70=0.0,MIPS_160=0.0 AOT_TYPE: MIPS Photometry AOR_LABEL: seppcon-139P-VO-1st AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: Vaisala-Oterma EPHEMERIS: NAIF_ID=1000238, NAIF_NAME=Vaisala-Oterma OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES MICRON_24: FIELD_SIZE = SMALL, EXPOSURE_TIME = 10, N_CYCLES = 1 SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=450.7, SLEW_TIME=5.0, SETTLE_TIME=8.0, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=674, DOWNLINK_VOLUME=3536102, VERSION=S14.1.0 INTEGRATION_TIME: MIPS_24=165.675,MIPS_70=0.0,MIPS_160=0.0 TIMING1: START_DATE=2006 Oct 27, START_TIME=00:43:00, END_DATE=2006 Dec 8, END_TIME=13:59:00 COMMENT_START: In almost all cases, a given comet is brighter in one observability window compared to the other(s) in Cycle 3. This is our motivation for having a timing constraint. Generally the constraint covers the full interval of the brightest window in the Cycle. COMMENT_END: AOT_TYPE: MIPS Photometry AOR_LABEL: seppcon-139P-VO-2nd AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: Vaisala-Oterma EPHEMERIS: NAIF_ID=1000238, NAIF_NAME=Vaisala-Oterma OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES MICRON_24: FIELD_SIZE = SMALL, EXPOSURE_TIME = 10, N_CYCLES = 1 SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=450.7, SLEW_TIME=5.0, SETTLE_TIME=8.0, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=674, DOWNLINK_VOLUME=3536102, VERSION=S14.1.0 INTEGRATION_TIME: MIPS_24=165.675,MIPS_70=0.0,MIPS_160=0.0 AOT_TYPE: MIPS Photometry AOR_LABEL: seppcon-C05W2-Chrst-1st AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: Christensen (C/2005 W2) EPHEMERIS: NAIF_ID=1001678, NAIF_NAME=Christensen (C/2005 W2) OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES MICRON_24: FIELD_SIZE = SMALL, EXPOSURE_TIME = 10, N_CYCLES = 1 SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=450.7, SLEW_TIME=5.0, SETTLE_TIME=8.0, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=674, DOWNLINK_VOLUME=3536102, VERSION=S14.1.0 INTEGRATION_TIME: MIPS_24=165.675,MIPS_70=0.0,MIPS_160=0.0 TIMING1: START_DATE=2006 Dec 10, START_TIME=21:59:00, END_DATE=2007 Jan 22, END_TIME=03:51:00 COMMENT_START: In almost all cases, a given comet is brighter in one observability window compared to the other(s) in Cycle 3. This is our motivation for having a timing constraint. Generally the constraint covers the full interval of the brightest window in the Cycle. COMMENT_END: AOT_TYPE: MIPS Photometry AOR_LABEL: seppcon-C05W2-Chrst-2nd AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: Christensen (C/2005 W2) EPHEMERIS: NAIF_ID=1001678, NAIF_NAME=Christensen (C/2005 W2) OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES MICRON_24: FIELD_SIZE = SMALL, EXPOSURE_TIME = 10, N_CYCLES = 1 SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=450.7, SLEW_TIME=5.0, SETTLE_TIME=8.0, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=674, DOWNLINK_VOLUME=3536102, VERSION=S14.1.0 INTEGRATION_TIME: MIPS_24=165.675,MIPS_70=0.0,MIPS_160=0.0 AOT_TYPE: MIPS Photometry AOR_LABEL: seppcon-P98VS24-LIN-1st AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: LINEAR (P/1998 VS24) EPHEMERIS: NAIF_ID=1000243, NAIF_NAME=LINEAR (P/1998 VS24) OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES MICRON_24: FIELD_SIZE = SMALL, EXPOSURE_TIME = 10, N_CYCLES = 1 SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=450.7, SLEW_TIME=5.0, SETTLE_TIME=8.0, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=674, DOWNLINK_VOLUME=3536102, VERSION=S14.1.0 INTEGRATION_TIME: MIPS_24=165.675,MIPS_70=0.0,MIPS_160=0.0 TIMING1: START_DATE=2006 Oct 17, START_TIME=18:09:00, END_DATE=2006 Nov 29, END_TIME=04:38:00 COMMENT_START: In almost all cases, a given comet is brighter in one observability window compared to the other(s) in Cycle 3. This is our motivation for having a timing constraint. Generally the constraint covers the full interval of the brightest window in the Cycle. COMMENT_END: AOT_TYPE: MIPS Photometry AOR_LABEL: seppcon-P98VS24-LIN-2nd AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: LINEAR (P/1998 VS24) EPHEMERIS: NAIF_ID=1000243, NAIF_NAME=LINEAR (P/1998 VS24) OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES MICRON_24: FIELD_SIZE = SMALL, EXPOSURE_TIME = 10, N_CYCLES = 1 SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=450.7, SLEW_TIME=5.0, SETTLE_TIME=8.0, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=674, DOWNLINK_VOLUME=3536102, VERSION=S14.1.0 INTEGRATION_TIME: MIPS_24=165.675,MIPS_70=0.0,MIPS_160=0.0 AOT_TYPE: MIPS Photometry AOR_LABEL: seppcon-P05W3-Kwlski-1st AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: Kowalski (P/2005 W3) EPHEMERIS: NAIF_ID=1002312, NAIF_NAME=Kowalski (P/2005 W3) OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES MICRON_24: FIELD_SIZE = SMALL, EXPOSURE_TIME = 10, N_CYCLES = 1 SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=450.7, SLEW_TIME=5.0, SETTLE_TIME=8.0, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=674, DOWNLINK_VOLUME=3536102, VERSION=S14.1.0 INTEGRATION_TIME: MIPS_24=165.675,MIPS_70=0.0,MIPS_160=0.0 TIMING1: START_DATE=2006 Dec 6, START_TIME=12:07:00, END_DATE=2007 Jan 18, END_TIME=12:45:00 COMMENT_START: In almost all cases, a given comet is brighter in one observability window compared to the other(s) in Cycle 3. This is our motivation for having a timing constraint. Generally the constraint covers the full interval of the brightest window in the Cycle. COMMENT_END: AOT_TYPE: MIPS Photometry AOR_LABEL: seppcon-P05W3-Kwlski-2nd AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: Kowalski (P/2005 W3) EPHEMERIS: NAIF_ID=1002312, NAIF_NAME=Kowalski (P/2005 W3) OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES MICRON_24: FIELD_SIZE = SMALL, EXPOSURE_TIME = 10, N_CYCLES = 1 SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=450.7, SLEW_TIME=5.0, SETTLE_TIME=8.0, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=674, DOWNLINK_VOLUME=3536102, VERSION=S14.1.0 INTEGRATION_TIME: MIPS_24=165.675,MIPS_70=0.0,MIPS_160=0.0 AOT_TYPE: MIPS Photometry AOR_LABEL: seppcon-P02O8-NEAT-1st AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: NEAT (P/2002 O8) EPHEMERIS: NAIF_ID=1000402, NAIF_NAME=NEAT (P/2002 O8) OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES MICRON_24: FIELD_SIZE = SMALL, EXPOSURE_TIME = 10, N_CYCLES = 1 SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=450.7, SLEW_TIME=5.0, SETTLE_TIME=8.0, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=674, DOWNLINK_VOLUME=3536102, VERSION=S14.1.0 INTEGRATION_TIME: MIPS_24=165.675,MIPS_70=0.0,MIPS_160=0.0 TIMING1: START_DATE=2006 Dec 15, START_TIME=00:00:00, END_DATE=2007 Jan 12, END_TIME=22:07:00 TIMING2: START_DATE=2007 Apr 30, START_TIME=18:33:00, END_DATE=2007 Jun 11, END_TIME=06:50:00 COMMENT_START: In almost all cases, a given comet is brighter in one observability window compared to the other(s) in Cycle 3. This is our motivation for having a timing constraint. Generally the constraint covers the full interval of the brightest window in the Cycle. COMMENT_END: AOT_TYPE: MIPS Photometry AOR_LABEL: seppcon-P02O8-NEAT-2nd AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: NEAT (P/2002 O8) EPHEMERIS: NAIF_ID=1000402, NAIF_NAME=NEAT (P/2002 O8) OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES MICRON_24: FIELD_SIZE = SMALL, EXPOSURE_TIME = 10, N_CYCLES = 1 SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=450.7, SLEW_TIME=5.0, SETTLE_TIME=8.0, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=674, DOWNLINK_VOLUME=3536102, VERSION=S14.1.0 INTEGRATION_TIME: MIPS_24=165.675,MIPS_70=0.0,MIPS_160=0.0 AOT_TYPE: MIPS Photometry AOR_LABEL: seppcon-P05JD108-CatNEAT-1st AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: Catalina-NEAT (P/2005 JD108) EPHEMERIS: NAIF_ID=1001650, NAIF_NAME=Catalina-NEAT (P/2005 JD108) OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES MICRON_24: FIELD_SIZE = SMALL, EXPOSURE_TIME = 10, N_CYCLES = 1 SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=450.7, SLEW_TIME=5.0, SETTLE_TIME=8.0, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=674, DOWNLINK_VOLUME=3536102, VERSION=S14.1.0 INTEGRATION_TIME: MIPS_24=165.675,MIPS_70=0.0,MIPS_160=0.0 TIMING1: START_DATE=2006 Jul 22, START_TIME=18:31:00, END_DATE=2006 Aug 28, END_TIME=20:42:00 TIMING2: START_DATE=2006 Dec 23, START_TIME=03:21:00, END_DATE=2007 Jan 3, END_TIME=00:00:00 COMMENT_START: In almost all cases, a given comet is brighter in one observability window compared to the other(s) in Cycle 3. This is our motivation for having a timing constraint. Generally the constraint covers the full interval of the brightest window in the Cycle. COMMENT_END: AOT_TYPE: MIPS Photometry AOR_LABEL: seppcon-P05JD108-CatNEAT-2nd AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: Catalina-NEAT (P/2005 JD108) EPHEMERIS: NAIF_ID=1001650, NAIF_NAME=Catalina-NEAT (P/2005 JD108) OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES MICRON_24: FIELD_SIZE = SMALL, EXPOSURE_TIME = 10, N_CYCLES = 1 SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=450.7, SLEW_TIME=5.0, SETTLE_TIME=8.0, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=674, DOWNLINK_VOLUME=3536102, VERSION=S14.1.0 INTEGRATION_TIME: MIPS_24=165.675,MIPS_70=0.0,MIPS_160=0.0 AOT_TYPE: MIPS Photometry AOR_LABEL: seppcon-P05Y2-McN-1st AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: McNaught (P/2005 Y2) EPHEMERIS: NAIF_ID=1002315, NAIF_NAME=McNaught (P/2005 Y2) OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES MICRON_24: FIELD_SIZE = SMALL, EXPOSURE_TIME = 10, N_CYCLES = 2 SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=604.7, SLEW_TIME=5.0, SETTLE_TIME=8.0, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=674, DOWNLINK_VOLUME=6630192, VERSION=S14.1.0 INTEGRATION_TIME: MIPS_24=312.47565,MIPS_70=0.0,MIPS_160=0.0 TIMING1: START_DATE=2006 Aug 1, START_TIME=20:13:00, END_DATE=2006 Sep 15, END_TIME=23:25:00 COMMENT_START: In almost all cases, a given comet is brighter in one observability window compared to the other(s) in Cycle 3. This is our motivation for having a timing constraint. Generally the constraint covers the full interval of the brightest window in the Cycle. COMMENT_END: AOT_TYPE: MIPS Photometry AOR_LABEL: seppcon-P05Y2-McN-2nd AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: McNaught (P/2005 Y2) EPHEMERIS: NAIF_ID=1002315, NAIF_NAME=McNaught (P/2005 Y2) OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES MICRON_24: FIELD_SIZE = SMALL, EXPOSURE_TIME = 10, N_CYCLES = 2 SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=604.7, SLEW_TIME=5.0, SETTLE_TIME=8.0, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=674, DOWNLINK_VOLUME=6630192, VERSION=S14.1.0 INTEGRATION_TIME: MIPS_24=312.47565,MIPS_70=0.0,MIPS_160=0.0 AOT_TYPE: MIPS Photometry AOR_LABEL: seppcon-P01CV8-LIN-1st AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: LINEAR (P/2001 CV8) EPHEMERIS: NAIF_ID=1000331, NAIF_NAME=LINEAR (P/2001 CV8) OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES MICRON_24: FIELD_SIZE = SMALL, EXPOSURE_TIME = 10, N_CYCLES = 3 SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=758.7, SLEW_TIME=5.0, SETTLE_TIME=8.0, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=674, DOWNLINK_VOLUME=9724282, VERSION=S14.1.0 INTEGRATION_TIME: MIPS_24=459.27628,MIPS_70=0.0,MIPS_160=0.0 TIMING1: START_DATE=2006 Dec 23, START_TIME=08:23:00, END_DATE=2007 Feb 1, END_TIME=10:45:00 COMMENT_START: In almost all cases, a given comet is brighter in one observability window compared to the other(s) in Cycle 3. This is our motivation for having a timing constraint. Generally the constraint covers the full interval of the brightest window in the Cycle. COMMENT_END: AOT_TYPE: MIPS Photometry AOR_LABEL: seppcon-P01CV8-LIN-2nd AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: LINEAR (P/2001 CV8) EPHEMERIS: NAIF_ID=1000331, NAIF_NAME=LINEAR (P/2001 CV8) OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES MICRON_24: FIELD_SIZE = SMALL, EXPOSURE_TIME = 10, N_CYCLES = 3 SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=758.7, SLEW_TIME=5.0, SETTLE_TIME=8.0, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=674, DOWNLINK_VOLUME=9724282, VERSION=S14.1.0 INTEGRATION_TIME: MIPS_24=459.27628,MIPS_70=0.0,MIPS_160=0.0 AOT_TYPE: MIPS Photometry AOR_LABEL: seppcon-P99WJ7-Korl-1st AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: Korlevic (P/1999 WJ7) EPHEMERIS: NAIF_ID=1000292, NAIF_NAME=Korlevic (P/1999 WJ7) OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES MICRON_24: FIELD_SIZE = SMALL, EXPOSURE_TIME = 10, N_CYCLES = 3 SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=758.7, SLEW_TIME=5.0, SETTLE_TIME=8.0, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=674, DOWNLINK_VOLUME=9724282, VERSION=S14.1.0 INTEGRATION_TIME: MIPS_24=459.27628,MIPS_70=0.0,MIPS_160=0.0 TIMING1: START_DATE=2006 Oct 3, START_TIME=04:44:00, END_DATE=2006 Oct 11, END_TIME=00:00:00 TIMING2: START_DATE=2007 Jun 9, START_TIME=00:55:00, END_DATE=2007 Jul 17, END_TIME=12:26:00 COMMENT_START: In almost all cases, a given comet is brighter in one observability window compared to the other(s) in Cycle 3. This is our motivation for having a timing constraint. Generally the constraint covers the full interval of the brightest window in the Cycle. COMMENT_END: AOT_TYPE: MIPS Photometry AOR_LABEL: seppcon-P99WJ7-Korl-2nd AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: Korlevic (P/1999 WJ7) EPHEMERIS: NAIF_ID=1000292, NAIF_NAME=Korlevic (P/1999 WJ7) OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES MICRON_24: FIELD_SIZE = SMALL, EXPOSURE_TIME = 10, N_CYCLES = 3 SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=758.7, SLEW_TIME=5.0, SETTLE_TIME=8.0, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=674, DOWNLINK_VOLUME=9724282, VERSION=S14.1.0 INTEGRATION_TIME: MIPS_24=459.27628,MIPS_70=0.0,MIPS_160=0.0 AOT_TYPE: MIPS Photometry AOR_LABEL: seppcon-P04H2-Larsen-1st AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: Larsen (P/2004 H2) EPHEMERIS: NAIF_ID=1000492, NAIF_NAME=Larsen (P/2004 H2) OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES MICRON_24: FIELD_SIZE = SMALL, EXPOSURE_TIME = 10, N_CYCLES = 3 SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=758.7, SLEW_TIME=5.0, SETTLE_TIME=8.0, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=674, DOWNLINK_VOLUME=9724282, VERSION=S14.1.0 INTEGRATION_TIME: MIPS_24=459.27628,MIPS_70=0.0,MIPS_160=0.0 TIMING1: START_DATE=2006 Jul 18, START_TIME=09:54:00, END_DATE=2006 Aug 29, END_TIME=05:28:00 COMMENT_START: In almost all cases, a given comet is brighter in one observability window compared to the other(s) in Cycle 3. This is our motivation for having a timing constraint. Generally the constraint covers the full interval of the brightest window in the Cycle. COMMENT_END: AOT_TYPE: MIPS Photometry AOR_LABEL: seppcon-P04H2-Larsen-2nd AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: Larsen (P/2004 H2) EPHEMERIS: NAIF_ID=1000492, NAIF_NAME=Larsen (P/2004 H2) OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES MICRON_24: FIELD_SIZE = SMALL, EXPOSURE_TIME = 10, N_CYCLES = 3 SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=758.7, SLEW_TIME=5.0, SETTLE_TIME=8.0, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=674, DOWNLINK_VOLUME=9724282, VERSION=S14.1.0 INTEGRATION_TIME: MIPS_24=459.27628,MIPS_70=0.0,MIPS_160=0.0 AOT_TYPE: MIPS Photometry AOR_LABEL: seppcon-P02LZ11-LIN-1st AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: LINEAR (P/2002 LZ11) EPHEMERIS: NAIF_ID=1000467, NAIF_NAME=LINEAR (P/2002 LZ11) OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES MICRON_24: FIELD_SIZE = SMALL, EXPOSURE_TIME = 10, N_CYCLES = 5 SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=1066.7, SLEW_TIME=5.0, SETTLE_TIME=8.0, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=674, DOWNLINK_VOLUME=15912464, VERSION=S14.1.0 INTEGRATION_TIME: MIPS_24=752.87756,MIPS_70=0.0,MIPS_160=0.0 TIMING1: START_DATE=2007 Feb 1, START_TIME=00:00:00, END_DATE=2007 Feb 16, END_TIME=23:29:00 TIMING2: START_DATE=2007 Jun 5, START_TIME=01:47:00, END_DATE=2007 Jul 15, END_TIME=21:32:00 COMMENT_START: In almost all cases, a given comet is brighter in one observability window compared to the other(s) in Cycle 3. This is our motivation for having a timing constraint. Generally the constraint covers the full interval of the brightest window in the Cycle. COMMENT_END: AOT_TYPE: MIPS Photometry AOR_LABEL: seppcon-P02LZ11-LIN-2nd AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: LINEAR (P/2002 LZ11) EPHEMERIS: NAIF_ID=1000467, NAIF_NAME=LINEAR (P/2002 LZ11) OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES MICRON_24: FIELD_SIZE = SMALL, EXPOSURE_TIME = 10, N_CYCLES = 5 SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=1066.7, SLEW_TIME=5.0, SETTLE_TIME=8.0, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=674, DOWNLINK_VOLUME=15912464, VERSION=S14.1.0 INTEGRATION_TIME: MIPS_24=752.87756,MIPS_70=0.0,MIPS_160=0.0 AOT_TYPE: MIPS Photometry AOR_LABEL: seppcon-93P-Lov1-1st AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: Lovas 1 EPHEMERIS: NAIF_ID=1000060, NAIF_NAME=Lovas 1 OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES MICRON_24: FIELD_SIZE = SMALL, EXPOSURE_TIME = 10, N_CYCLES = 6 SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=1220.7, SLEW_TIME=5.0, SETTLE_TIME=8.0, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=674, DOWNLINK_VOLUME=19006554, VERSION=S14.1.0 INTEGRATION_TIME: MIPS_24=899.6782,MIPS_70=0.0,MIPS_160=0.0 TIMING1: START_DATE=2006 Sep 21, START_TIME=23:05:00, END_DATE=2006 Oct 4, END_TIME=12:00:00 COMMENT_START: In almost all cases, a given comet is brighter in one observability window compared to the other(s) in Cycle 3. This is our motivation for having a timing constraint. Generally the constraint covers the full interval of the brightest window in the Cycle. COMMENT_END: AOT_TYPE: MIPS Photometry AOR_LABEL: seppcon-93P-Lov1-2nd AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: Lovas 1 EPHEMERIS: NAIF_ID=1000060, NAIF_NAME=Lovas 1 OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES MICRON_24: FIELD_SIZE = SMALL, EXPOSURE_TIME = 10, N_CYCLES = 6 SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=1220.7, SLEW_TIME=5.0, SETTLE_TIME=8.0, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=674, DOWNLINK_VOLUME=19006554, VERSION=S14.1.0 INTEGRATION_TIME: MIPS_24=899.6782,MIPS_70=0.0,MIPS_160=0.0 AOT_TYPE: MIPS Photometry AOR_LABEL: seppcon-P03KV2-LIN-1st AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: LINEAR (P/2003 KV2) EPHEMERIS: NAIF_ID=1000441, NAIF_NAME=LINEAR (P/2003 KV2) OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES MICRON_24: FIELD_SIZE = SMALL, EXPOSURE_TIME = 10, N_CYCLES = 7 SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=1374.7, SLEW_TIME=5.0, SETTLE_TIME=8.0, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=674, DOWNLINK_VOLUME=22100644, VERSION=S14.1.0 INTEGRATION_TIME: MIPS_24=1046.4789,MIPS_70=0.0,MIPS_160=0.0 TIMING1: START_DATE=2006 Oct 22, START_TIME=17:00:00, END_DATE=2006 Dec 3, END_TIME=15:18:00 COMMENT_START: In almost all cases, a given comet is brighter in one observability window compared to the other(s) in Cycle 3. This is our motivation for having a timing constraint. Generally the constraint covers the full interval of the brightest window in the Cycle. COMMENT_END: AOT_TYPE: MIPS Photometry AOR_LABEL: seppcon-P03KV2-LIN-2nd AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: LINEAR (P/2003 KV2) EPHEMERIS: NAIF_ID=1000441, NAIF_NAME=LINEAR (P/2003 KV2) OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES MICRON_24: FIELD_SIZE = SMALL, EXPOSURE_TIME = 10, N_CYCLES = 7 SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=1374.7, SLEW_TIME=5.0, SETTLE_TIME=8.0, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=674, DOWNLINK_VOLUME=22100644, VERSION=S14.1.0 INTEGRATION_TIME: MIPS_24=1046.4789,MIPS_70=0.0,MIPS_160=0.0 AOT_TYPE: MIPS Photometry AOR_LABEL: seppcon-P05K3-McN-1st AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: McNaught (P/2005 K3) EPHEMERIS: NAIF_ID=1000584, NAIF_NAME=McNaught (P/2005 K3) OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES MICRON_24: FIELD_SIZE = SMALL, EXPOSURE_TIME = 10, N_CYCLES = 10 SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=1903.3147, SLEW_TIME=15.0, SETTLE_TIME=23.614737, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=864, DOWNLINK_VOLUME=31824928, VERSION=S14.1.0 INTEGRATION_TIME: MIPS_24=1505.7551,MIPS_70=0.0,MIPS_160=0.0 TIMING1: START_DATE=2006 Dec 15, START_TIME=05:51:00, END_DATE=2007 Jan 24, END_TIME=01:20:00 COMMENT_START: In almost all cases, a given comet is brighter in one observability window compared to the other(s) in Cycle 3. This is our motivation for having a timing constraint. Generally the constraint covers the full interval of the brightest window in the Cycle. COMMENT_END: AOT_TYPE: MIPS Photometry AOR_LABEL: seppcon-P05K3-LIN-2nd AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: McNaught (P/2005 K3) EPHEMERIS: NAIF_ID=1000584, NAIF_NAME=McNaught (P/2005 K3) OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES MICRON_24: FIELD_SIZE = SMALL, EXPOSURE_TIME = 10, N_CYCLES = 10 SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=1903.3147, SLEW_TIME=15.0, SETTLE_TIME=23.614737, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=864, DOWNLINK_VOLUME=31824928, VERSION=S14.1.0 INTEGRATION_TIME: MIPS_24=1505.7551,MIPS_70=0.0,MIPS_160=0.0 AOT_TYPE: MIPS Photometry AOR_LABEL: seppcon-P04T1-LINNT-1st AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: LINEAR-NEAT (P/2004 T1) EPHEMERIS: NAIF_ID=1000513, NAIF_NAME=LINEAR-NEAT (P/2004 T1) OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES MICRON_24: FIELD_SIZE = SMALL, EXPOSURE_TIME = 10, N_CYCLES = 10 SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=1903.3148, SLEW_TIME=15.0, SETTLE_TIME=23.614763, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=864, DOWNLINK_VOLUME=31824928, VERSION=S14.1.0 INTEGRATION_TIME: MIPS_24=1505.7551,MIPS_70=0.0,MIPS_160=0.0 TIMING1: START_DATE=2007 Jan 25, START_TIME=15:29:00, END_DATE=2007 Mar 6, END_TIME=02:30:00 COMMENT_START: In almost all cases, a given comet is brighter in one observability window compared to the other(s) in Cycle 3. This is our motivation for having a timing constraint. Generally the constraint covers the full interval of the brightest window in the Cycle. COMMENT_END: AOT_TYPE: MIPS Photometry AOR_LABEL: seppcon-P04T1-LINNT-2nd AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: LINEAR-NEAT (P/2004 T1) EPHEMERIS: NAIF_ID=1000513, NAIF_NAME=LINEAR-NEAT (P/2004 T1) OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES MICRON_24: FIELD_SIZE = SMALL, EXPOSURE_TIME = 10, N_CYCLES = 10 SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=1903.3148, SLEW_TIME=15.0, SETTLE_TIME=23.614763, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=864, DOWNLINK_VOLUME=31824928, VERSION=S14.1.0 INTEGRATION_TIME: MIPS_24=1505.7551,MIPS_70=0.0,MIPS_160=0.0 AOT_TYPE: MIPS Photometry AOR_LABEL: seppcon-148P-AndLIN-1st AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: Anderson-LINEAR EPHEMERIS: NAIF_ID=1000328, NAIF_NAME=Anderson-LINEAR OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES MICRON_24: FIELD_SIZE = SMALL, EXPOSURE_TIME = 10, N_CYCLES = 12 SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=2211.3147, SLEW_TIME=15.0, SETTLE_TIME=23.614746, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=864, DOWNLINK_VOLUME=38013108, VERSION=S14.1.0 INTEGRATION_TIME: MIPS_24=1799.3564,MIPS_70=0.0,MIPS_160=0.0 TIMING1: START_DATE=2006 Oct 20, START_TIME=09:36:00, END_DATE=2006 Nov 30, END_TIME=04:10:00 COMMENT_START: In almost all cases, a given comet is brighter in one observability window compared to the other(s) in Cycle 3. This is our motivation for having a timing constraint. Generally the constraint covers the full interval of the brightest window in the Cycle. COMMENT_END: AOT_TYPE: MIPS Photometry AOR_LABEL: seppcon-148P-AndLIN-2nd AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: Anderson-LINEAR EPHEMERIS: NAIF_ID=1000328, NAIF_NAME=Anderson-LINEAR OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES MICRON_24: FIELD_SIZE = SMALL, EXPOSURE_TIME = 10, N_CYCLES = 12 SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=2211.3147, SLEW_TIME=15.0, SETTLE_TIME=23.614746, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=864, DOWNLINK_VOLUME=38013108, VERSION=S14.1.0 INTEGRATION_TIME: MIPS_24=1799.3564,MIPS_70=0.0,MIPS_160=0.0 AOT_TYPE: MIPS Photometry AOR_LABEL: seppcon-169P-NEAT-1st AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: NEAT EPHEMERIS: NAIF_ID=1001656, NAIF_NAME=NEAT OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES MICRON_24: FIELD_SIZE = SMALL, EXPOSURE_TIME = 10, N_CYCLES = 12 SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=2211.3147, SLEW_TIME=15.0, SETTLE_TIME=23.614737, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=864, DOWNLINK_VOLUME=38013108, VERSION=S14.1.0 INTEGRATION_TIME: MIPS_24=1799.3564,MIPS_70=0.0,MIPS_160=0.0 TIMING1: START_DATE=2007 Feb 11, START_TIME=14:27:00, END_DATE=2007 Mar 21, END_TIME=20:43:00 COMMENT_START: In almost all cases, a given comet is brighter in one observability window compared to the other(s) in Cycle 3. This is our motivation for having a timing constraint. Generally the constraint covers the full interval of the brightest window in the Cycle. COMMENT_END: AOT_TYPE: MIPS Photometry AOR_LABEL: seppcon-169P-NEAT-2nd AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: NEAT EPHEMERIS: NAIF_ID=1001656, NAIF_NAME=NEAT OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES MICRON_24: FIELD_SIZE = SMALL, EXPOSURE_TIME = 10, N_CYCLES = 12 SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=2211.3147, SLEW_TIME=15.0, SETTLE_TIME=23.614737, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=864, DOWNLINK_VOLUME=38013108, VERSION=S14.1.0 INTEGRATION_TIME: MIPS_24=1799.3564,MIPS_70=0.0,MIPS_160=0.0 AOT_TYPE: MIPS Photometry AOR_LABEL: seppcon-138P-SL7-1st AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: Shoemaker-Levy 7 EPHEMERIS: NAIF_ID=1000137, NAIF_NAME=Shoemaker-Levy 7 OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES MICRON_24: FIELD_SIZE = SMALL, EXPOSURE_TIME = 10, N_CYCLES = 12 SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=2211.3147, SLEW_TIME=15.0, SETTLE_TIME=23.614735, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=864, DOWNLINK_VOLUME=38013108, VERSION=S14.1.0 INTEGRATION_TIME: MIPS_24=1799.3564,MIPS_70=0.0,MIPS_160=0.0 TIMING1: START_DATE=2007 Jan 22, START_TIME=04:18:00, END_DATE=2007 Mar 2, END_TIME=21:11:00 COMMENT_START: In almost all cases, a given comet is brighter in one observability window compared to the other(s) in Cycle 3. This is our motivation for having a timing constraint. Generally the constraint covers the full interval of the brightest window in the Cycle. COMMENT_END: AOT_TYPE: MIPS Photometry AOR_LABEL: seppcon-138P-SL7-2nd AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: Shoemaker-Levy 7 EPHEMERIS: NAIF_ID=1000137, NAIF_NAME=Shoemaker-Levy 7 OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES MICRON_24: FIELD_SIZE = SMALL, EXPOSURE_TIME = 10, N_CYCLES = 12 SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=2211.3147, SLEW_TIME=15.0, SETTLE_TIME=23.614735, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=864, DOWNLINK_VOLUME=38013108, VERSION=S14.1.0 INTEGRATION_TIME: MIPS_24=1799.3564,MIPS_70=0.0,MIPS_160=0.0 AOT_TYPE: MIPS Photometry AOR_LABEL: seppcon-P03O3-LIN-1st AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: LINEAR (P/2003 O3) EPHEMERIS: NAIF_ID=1000448, NAIF_NAME=LINEAR (P/2003 O3) OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES MICRON_24: FIELD_SIZE = SMALL, EXPOSURE_TIME = 10, N_CYCLES = 12 SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=2211.3147, SLEW_TIME=15.0, SETTLE_TIME=23.614752, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=864, DOWNLINK_VOLUME=38013108, VERSION=S14.1.0 INTEGRATION_TIME: MIPS_24=1799.3564,MIPS_70=0.0,MIPS_160=0.0 TIMING1: START_DATE=2007 Feb 12, START_TIME=00:00:00, END_DATE=2007 Feb 25, END_TIME=02:08:00 TIMING2: START_DATE=2007 Jun 11, START_TIME=21:49:00, END_DATE=2007 Jul 21, END_TIME=16:37:00 COMMENT_START: In almost all cases, a given comet is brighter in one observability window compared to the other(s) in Cycle 3. This is our motivation for having a timing constraint. Generally the constraint covers the full interval of the brightest window in the Cycle. COMMENT_END: AOT_TYPE: MIPS Photometry AOR_LABEL: seppcon-P03O3-LIN-2nd AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: LINEAR (P/2003 O3) EPHEMERIS: NAIF_ID=1000448, NAIF_NAME=LINEAR (P/2003 O3) OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES MICRON_24: FIELD_SIZE = SMALL, EXPOSURE_TIME = 10, N_CYCLES = 12 SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=2211.3147, SLEW_TIME=15.0, SETTLE_TIME=23.614752, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=864, DOWNLINK_VOLUME=38013108, VERSION=S14.1.0 INTEGRATION_TIME: MIPS_24=1799.3564,MIPS_70=0.0,MIPS_160=0.0 AOT_TYPE: MIPS Photometry AOR_LABEL: seppcon-15P-F-1st AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: Finlay EPHEMERIS: NAIF_ID=1000027, NAIF_NAME=Finlay OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES MICRON_24: FIELD_SIZE = SMALL, EXPOSURE_TIME = 10, N_CYCLES = 12 SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=2211.3147, SLEW_TIME=15.0, SETTLE_TIME=23.614738, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=864, DOWNLINK_VOLUME=38013108, VERSION=S14.1.0 INTEGRATION_TIME: MIPS_24=1799.3564,MIPS_70=0.0,MIPS_160=0.0 TIMING1: START_DATE=2007 Feb 21, START_TIME=21:50:00, END_DATE=2007 Apr 2, END_TIME=09:41:00 COMMENT_START: In almost all cases, a given comet is brighter in one observability window compared to the other(s) in Cycle 3. This is our motivation for having a timing constraint. Generally the constraint covers the full interval of the brightest window in the Cycle. COMMENT_END: AOT_TYPE: MIPS Photometry AOR_LABEL: seppcon-15P-F-2nd AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: Finlay EPHEMERIS: NAIF_ID=1000027, NAIF_NAME=Finlay OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES MICRON_24: FIELD_SIZE = SMALL, EXPOSURE_TIME = 10, N_CYCLES = 12 SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=2211.3147, SLEW_TIME=15.0, SETTLE_TIME=23.614738, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=864, DOWNLINK_VOLUME=38013108, VERSION=S14.1.0 INTEGRATION_TIME: MIPS_24=1799.3564,MIPS_70=0.0,MIPS_160=0.0 AOT_TYPE: MIPS Photometry AOR_LABEL: seppcon-P02JN16-LIN-1st AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: LINEAR (P/2002 JN16) EPHEMERIS: NAIF_ID=1000393, NAIF_NAME=LINEAR (P/2002 JN16) OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES MICRON_24: FIELD_SIZE = SMALL, EXPOSURE_TIME = 10, N_CYCLES = 12 SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=2211.3147, SLEW_TIME=15.0, SETTLE_TIME=23.614742, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=864, DOWNLINK_VOLUME=38013108, VERSION=S14.1.0 INTEGRATION_TIME: MIPS_24=1799.3564,MIPS_70=0.0,MIPS_160=0.0 TIMING1: START_DATE=2006 Dec 9, START_TIME=00:00:00, END_DATE=2006 Dec 23, END_TIME=15:54:00 TIMING2: START_DATE=2007 Apr 9, START_TIME=00:16:00, END_DATE=2007 May 19, END_TIME=10:11:00 COMMENT_START: In almost all cases, a given comet is brighter in one observability window compared to the other(s) in Cycle 3. This is our motivation for having a timing constraint. Generally the constraint covers the full interval of the brightest window in the Cycle. COMMENT_END: AOT_TYPE: MIPS Photometry AOR_LABEL: seppcon-P02JN16-LIN-2nd AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: LINEAR (P/2002 JN16) EPHEMERIS: NAIF_ID=1000393, NAIF_NAME=LINEAR (P/2002 JN16) OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES MICRON_24: FIELD_SIZE = SMALL, EXPOSURE_TIME = 10, N_CYCLES = 12 SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=2211.3147, SLEW_TIME=15.0, SETTLE_TIME=23.614742, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=864, DOWNLINK_VOLUME=38013108, VERSION=S14.1.0 INTEGRATION_TIME: MIPS_24=1799.3564,MIPS_70=0.0,MIPS_160=0.0 AOT_TYPE: MIPS Photometry AOR_LABEL: seppcon-168P-Herg-1st AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: Hergenrother EPHEMERIS: NAIF_ID=1000242, NAIF_NAME=Hergenrother OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES MICRON_24: FIELD_SIZE = SMALL, EXPOSURE_TIME = 10, N_CYCLES = 14 SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=2519.3147, SLEW_TIME=15.0, SETTLE_TIME=23.61477, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=864, DOWNLINK_VOLUME=44201288, VERSION=S14.1.0 INTEGRATION_TIME: MIPS_24=2092.9578,MIPS_70=0.0,MIPS_160=0.0 TIMING1: START_DATE=2007 May 9, START_TIME=08:59:00, END_DATE=2007 Jun 19, END_TIME=00:50:00 COMMENT_START: In almost all cases, a given comet is brighter in one observability window compared to the other(s) in Cycle 3. This is our motivation for having a timing constraint. Generally the constraint covers the full interval of the brightest window in the Cycle. COMMENT_END: AOT_TYPE: MIPS Photometry AOR_LABEL: seppcon-168P-Herg-2nd AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: Hergenrother EPHEMERIS: NAIF_ID=1000242, NAIF_NAME=Hergenrother OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES MICRON_24: FIELD_SIZE = SMALL, EXPOSURE_TIME = 10, N_CYCLES = 14 SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=2519.3147, SLEW_TIME=15.0, SETTLE_TIME=23.61477, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=864, DOWNLINK_VOLUME=44201288, VERSION=S14.1.0 INTEGRATION_TIME: MIPS_24=2092.9578,MIPS_70=0.0,MIPS_160=0.0 AOT_TYPE: MIPS Photometry AOR_LABEL: seppcon-P05XA54-LONHill-1st AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: LONEOS-Hill (P/2005 XA54) EPHEMERIS: NAIF_ID=1002317, NAIF_NAME=LONEOS-Hill (P/2005 XA54) OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES MICRON_24: FIELD_SIZE = SMALL, EXPOSURE_TIME = 10, N_CYCLES = 14 SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=2519.3147, SLEW_TIME=15.0, SETTLE_TIME=23.61476, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=864, DOWNLINK_VOLUME=44201288, VERSION=S14.1.0 INTEGRATION_TIME: MIPS_24=2092.9578,MIPS_70=0.0,MIPS_160=0.0 TIMING1: START_DATE=2007 Apr 26, START_TIME=23:52:00, END_DATE=2007 Jun 6, END_TIME=23:34:00 COMMENT_START: In almost all cases, a given comet is brighter in one observability window compared to the other(s) in Cycle 3. This is our motivation for having a timing constraint. Generally the constraint covers the full interval of the brightest window in the Cycle. COMMENT_END: AOT_TYPE: MIPS Photometry AOR_LABEL: seppcon-P05XA54-LONHill-2nd AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: LONEOS-Hill (P/2005 XA54) EPHEMERIS: NAIF_ID=1002317, NAIF_NAME=LONEOS-Hill (P/2005 XA54) OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES MICRON_24: FIELD_SIZE = SMALL, EXPOSURE_TIME = 10, N_CYCLES = 14 SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=2519.3147, SLEW_TIME=15.0, SETTLE_TIME=23.61476, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=864, DOWNLINK_VOLUME=44201288, VERSION=S14.1.0 INTEGRATION_TIME: MIPS_24=2092.9578,MIPS_70=0.0,MIPS_160=0.0 AOT_TYPE: MIPS Photometry AOR_LABEL: seppcon-P05Q4-LIN-1st AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: LINEAR (P/2005 Q4) EPHEMERIS: NAIF_ID=1001661, NAIF_NAME=LINEAR (P/2005 Q4) OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES MICRON_24: FIELD_SIZE = SMALL, EXPOSURE_TIME = 10, N_CYCLES = 14 SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=2519.3147, SLEW_TIME=15.0, SETTLE_TIME=23.614733, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=864, DOWNLINK_VOLUME=44201288, VERSION=S14.1.0 INTEGRATION_TIME: MIPS_24=2092.9578,MIPS_70=0.0,MIPS_160=0.0 TIMING1: START_DATE=2007 Jan 27, START_TIME=20:52:00, END_DATE=2007 Mar 7, END_TIME=20:47:00 COMMENT_START: In almost all cases, a given comet is brighter in one observability window compared to the other(s) in Cycle 3. This is our motivation for having a timing constraint. Generally the constraint covers the full interval of the brightest window in the Cycle. COMMENT_END: AOT_TYPE: MIPS Photometry AOR_LABEL: seppcon-P05Q4-LIN-2nd AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: LINEAR (P/2005 Q4) EPHEMERIS: NAIF_ID=1001661, NAIF_NAME=LINEAR (P/2005 Q4) OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES MICRON_24: FIELD_SIZE = SMALL, EXPOSURE_TIME = 10, N_CYCLES = 14 SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=2519.3147, SLEW_TIME=15.0, SETTLE_TIME=23.614733, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=864, DOWNLINK_VOLUME=44201288, VERSION=S14.1.0 INTEGRATION_TIME: MIPS_24=2092.9578,MIPS_70=0.0,MIPS_160=0.0 AOT_TYPE: MIPS Photometry AOR_LABEL: seppcon-P00Y3-Scotti-1st AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: Scotti (P/2000 Y3) EPHEMERIS: NAIF_ID=1000323, NAIF_NAME=Scotti (P/2000 Y3) OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES MICRON_24: FIELD_SIZE = SMALL, EXPOSURE_TIME = 10, N_CYCLES = 8 SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=1595.3147, SLEW_TIME=15.0, SETTLE_TIME=23.614744, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=864, DOWNLINK_VOLUME=25636744, VERSION=S14.1.0 INTEGRATION_TIME: MIPS_24=1212.1538,MIPS_70=0.0,MIPS_160=0.0 TIMING1: START_DATE=2006 Aug 31, START_TIME=04:44:00, END_DATE=2006 Oct 11, END_TIME=03:25:00 TIMING2: START_DATE=2007 May 2, START_TIME=20:18:00, END_DATE=2007 Jun 10, END_TIME=15:01:00 COMMENT_START: In almost all cases, a given comet is brighter in one observability window compared to the other(s) in Cycle 3. This is our motivation for having a timing constraint. Generally the constraint covers the full interval of the brightest window in the Cycle. COMMENT_END: AOT_TYPE: MIPS Photometry AOR_LABEL: seppcon-P00Y3-Scotti-2nd AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: Scotti (P/2000 Y3) EPHEMERIS: NAIF_ID=1000323, NAIF_NAME=Scotti (P/2000 Y3) OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES MICRON_24: FIELD_SIZE = SMALL, EXPOSURE_TIME = 10, N_CYCLES = 8 SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=1595.3147, SLEW_TIME=15.0, SETTLE_TIME=23.614744, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=864, DOWNLINK_VOLUME=25636744, VERSION=S14.1.0 INTEGRATION_TIME: MIPS_24=1212.1538,MIPS_70=0.0,MIPS_160=0.0 AOT_TYPE: MIPS Photometry AOR_LABEL: seppcon-11P-TSL-1st AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: Tempel-Swift-LINEAR EPHEMERIS: NAIF_ID=1000365, NAIF_NAME=Tempel-Swift-LINEAR OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES MICRON_24: FIELD_SIZE = SMALL, EXPOSURE_TIME = 10, N_CYCLES = 14 SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=2519.3147, SLEW_TIME=15.0, SETTLE_TIME=23.614742, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=864, DOWNLINK_VOLUME=44201288, VERSION=S14.1.0 INTEGRATION_TIME: MIPS_24=2092.9578,MIPS_70=0.0,MIPS_160=0.0 TIMING1: START_DATE=2006 Aug 15, START_TIME=15:25:00, END_DATE=2006 Sep 25, END_TIME=12:40:00 COMMENT_START: In almost all cases, a given comet is brighter in one observability window compared to the other(s) in Cycle 3. This is our motivation for having a timing constraint. Generally the constraint covers the full interval of the brightest window in the Cycle. COMMENT_END: AOT_TYPE: MIPS Photometry AOR_LABEL: seppcon-11P-TSL-2nd AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: Tempel-Swift-LINEAR EPHEMERIS: NAIF_ID=1000365, NAIF_NAME=Tempel-Swift-LINEAR OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES MICRON_24: FIELD_SIZE = SMALL, EXPOSURE_TIME = 10, N_CYCLES = 14 SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=2519.3147, SLEW_TIME=15.0, SETTLE_TIME=23.614742, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=864, DOWNLINK_VOLUME=44201288, VERSION=S14.1.0 INTEGRATION_TIME: MIPS_24=2092.9578,MIPS_70=0.0,MIPS_160=0.0 AOT_TYPE: MIPS Photometry AOR_LABEL: seppcon-16P-Br2-1st AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: Brooks 2 EPHEMERIS: NAIF_ID=1000008, NAIF_NAME=Brooks 2 OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES MICRON_24: FIELD_SIZE = SMALL, EXPOSURE_TIME = 10, N_CYCLES = 16 SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=2960.5442, SLEW_TIME=35.0, SETTLE_TIME=54.844242, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=1244, DOWNLINK_VOLUME=51273488, VERSION=S14.1.0 INTEGRATION_TIME: MIPS_24=2424.3076,MIPS_70=0.0,MIPS_160=0.0 TIMING1: START_DATE=2006 Jul 17, START_TIME=03:09:00, END_DATE=2006 Aug 26, END_TIME=18:30:00 COMMENT_START: In almost all cases, a given comet is brighter in one observability window compared to the other(s) in Cycle 3. This is our motivation for having a timing constraint. Generally the constraint covers the full interval of the brightest window in the Cycle. COMMENT_END: AOT_TYPE: MIPS Photometry AOR_LABEL: seppcon-16P-Br2-2nd AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: Brooks 2 EPHEMERIS: NAIF_ID=1000008, NAIF_NAME=Brooks 2 OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES MICRON_24: FIELD_SIZE = SMALL, EXPOSURE_TIME = 10, N_CYCLES = 16 SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=2960.5442, SLEW_TIME=35.0, SETTLE_TIME=54.844242, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=1244, DOWNLINK_VOLUME=51273488, VERSION=S14.1.0 INTEGRATION_TIME: MIPS_24=2424.3076,MIPS_70=0.0,MIPS_160=0.0 AOT_TYPE: MIPS Photometry AOR_LABEL: seppcon-144P-Kush-1st AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: Kushida EPHEMERIS: NAIF_ID=1000148, NAIF_NAME=Kushida OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES MICRON_24: FIELD_SIZE = SMALL, EXPOSURE_TIME = 10, N_CYCLES = 16 SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=2960.5442, SLEW_TIME=35.0, SETTLE_TIME=54.84423, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=1244, DOWNLINK_VOLUME=51273488, VERSION=S14.1.0 INTEGRATION_TIME: MIPS_24=2424.3076,MIPS_70=0.0,MIPS_160=0.0 TIMING1: START_DATE=2007 Jun 11, START_TIME=22:41:00, END_DATE=2007 Jul 20, END_TIME=14:14:00 COMMENT_START: In almost all cases, a given comet is brighter in one observability window compared to the other(s) in Cycle 3. This is our motivation for having a timing constraint. Generally the constraint covers the full interval of the brightest window in the Cycle. COMMENT_END: AOT_TYPE: MIPS Photometry AOR_LABEL: seppcon-144P-Kush-2nd AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: Kushida EPHEMERIS: NAIF_ID=1000148, NAIF_NAME=Kushida OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES MICRON_24: FIELD_SIZE = SMALL, EXPOSURE_TIME = 10, N_CYCLES = 16 SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=2960.5442, SLEW_TIME=35.0, SETTLE_TIME=54.84423, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=1244, DOWNLINK_VOLUME=51273488, VERSION=S14.1.0 INTEGRATION_TIME: MIPS_24=2424.3076,MIPS_70=0.0,MIPS_160=0.0 AOT_TYPE: MIPS Photometry AOR_LABEL: seppcon-P02S1-Skiff-1st AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: Skiff (P/2002 S1) EPHEMERIS: NAIF_ID=1000412, NAIF_NAME=Skiff (P/2002 S1) OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES MICRON_24: FIELD_SIZE = SMALL, EXPOSURE_TIME = 10, N_CYCLES = 12 SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=2211.3147, SLEW_TIME=15.0, SETTLE_TIME=23.614737, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=864, DOWNLINK_VOLUME=38013108, VERSION=S14.1.0 INTEGRATION_TIME: MIPS_24=1799.3564,MIPS_70=0.0,MIPS_160=0.0 TIMING1: START_DATE=2006 Jun 22, START_TIME=10:07:00, END_DATE=2006 Aug 3, END_TIME=06:08:00 TIMING2: START_DATE=2007 Feb 24, START_TIME=02:39:00, END_DATE=2007 Apr 7, END_TIME=09:54:00 COMMENT_START: In almost all cases, a given comet is brighter in one observability window compared to the other(s) in Cycle 3. This is our motivation for having a timing constraint. Generally the constraint covers the full interval of the brightest window in the Cycle. COMMENT_END: AOT_TYPE: MIPS Photometry AOR_LABEL: seppcon-P02S1-Skiff-2nd AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: Skiff (P/2002 S1) EPHEMERIS: NAIF_ID=1000412, NAIF_NAME=Skiff (P/2002 S1) OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES MICRON_24: FIELD_SIZE = SMALL, EXPOSURE_TIME = 10, N_CYCLES = 12 SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=2211.3147, SLEW_TIME=15.0, SETTLE_TIME=23.614737, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=864, DOWNLINK_VOLUME=38013108, VERSION=S14.1.0 INTEGRATION_TIME: MIPS_24=1799.3564,MIPS_70=0.0,MIPS_160=0.0 AOT_TYPE: MIPS Photometry AOR_LABEL: seppcon-P03HT15-LIN-1st AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: LINEAR (P/2003 HT15) EPHEMERIS: NAIF_ID=1000445, NAIF_NAME=LINEAR (P/2003 HT15) OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES MICRON_24: FIELD_SIZE = SMALL, EXPOSURE_TIME = 10, N_CYCLES = 10 SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=1903.3147, SLEW_TIME=15.0, SETTLE_TIME=23.614748, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=864, DOWNLINK_VOLUME=31824928, VERSION=S14.1.0 INTEGRATION_TIME: MIPS_24=1505.7551,MIPS_70=0.0,MIPS_160=0.0 TIMING1: START_DATE=2006 Jul 8, START_TIME=10:53:00, END_DATE=2006 Aug 24, END_TIME=22:52:00 TIMING2: START_DATE=2006 Dec 4, START_TIME=21:53:00, END_DATE=2006 Dec 18, END_TIME=12:00:00 COMMENT_START: In almost all cases, a given comet is brighter in one observability window compared to the other(s) in Cycle 3. This is our motivation for having a timing constraint. Generally the constraint covers the full interval of the brightest window in the Cycle. COMMENT_END: AOT_TYPE: MIPS Photometry AOR_LABEL: seppcon-P03HT15-LIN-2nd AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: LINEAR (P/2003 HT15) EPHEMERIS: NAIF_ID=1000445, NAIF_NAME=LINEAR (P/2003 HT15) OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES MICRON_24: FIELD_SIZE = SMALL, EXPOSURE_TIME = 10, N_CYCLES = 10 SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=1903.3147, SLEW_TIME=15.0, SETTLE_TIME=23.614748, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=864, DOWNLINK_VOLUME=31824928, VERSION=S14.1.0 INTEGRATION_TIME: MIPS_24=1505.7551,MIPS_70=0.0,MIPS_160=0.0 AOT_TYPE: MIPS Photometry AOR_LABEL: seppcon-P04A1-LONEOS-1st AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: LONEOS (P/2004 A1) EPHEMERIS: NAIF_ID=1000473, NAIF_NAME=LONEOS (P/2004 A1) OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES MICRON_24: FIELD_SIZE = SMALL, EXPOSURE_TIME = 10, N_CYCLES = 12 SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=2211.3147, SLEW_TIME=15.0, SETTLE_TIME=23.61474, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=864, DOWNLINK_VOLUME=38013108, VERSION=S14.1.0 INTEGRATION_TIME: MIPS_24=1799.3564,MIPS_70=0.0,MIPS_160=0.0 TIMING1: START_DATE=2006 Jun 20, START_TIME=04:02:00, END_DATE=2006 Aug 1, END_TIME=04:17:00 COMMENT_START: In almost all cases, a given comet is brighter in one observability window compared to the other(s) in Cycle 3. This is our motivation for having a timing constraint. Generally the constraint covers the full interval of the brightest window in the Cycle. COMMENT_END: AOT_TYPE: MIPS Photometry AOR_LABEL: seppcon-P04A1-LONEOS-2nd AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: LONEOS (P/2004 A1) EPHEMERIS: NAIF_ID=1000473, NAIF_NAME=LONEOS (P/2004 A1) OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES MICRON_24: FIELD_SIZE = SMALL, EXPOSURE_TIME = 10, N_CYCLES = 12 SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=2211.3147, SLEW_TIME=15.0, SETTLE_TIME=23.61474, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=864, DOWNLINK_VOLUME=38013108, VERSION=S14.1.0 INTEGRATION_TIME: MIPS_24=1799.3564,MIPS_70=0.0,MIPS_160=0.0 AOT_TYPE: MIPS Photometry AOR_LABEL: seppcon-P01R6-LINSk-1st AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: LINEAR-Skiff (P/2001 R6) EPHEMERIS: NAIF_ID=1000354, NAIF_NAME=LINEAR-Skiff (P/2001 R6) OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES MICRON_24: FIELD_SIZE = SMALL, EXPOSURE_TIME = 10, N_CYCLES = 15 SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=2739.9294, SLEW_TIME=25.0, SETTLE_TIME=39.229485, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=1054, DOWNLINK_VOLUME=47737392, VERSION=S14.1.0 INTEGRATION_TIME: MIPS_24=2258.6328,MIPS_70=0.0,MIPS_160=0.0 TIMING1: START_DATE=2007 Feb 25, START_TIME=05:27:00, END_DATE=2007 Apr 5, END_TIME=15:12:00 COMMENT_START: In almost all cases, a given comet is brighter in one observability window compared to the other(s) in Cycle 3. This is our motivation for having a timing constraint. Generally the constraint covers the full interval of the brightest window in the Cycle. COMMENT_END: AOT_TYPE: MIPS Photometry AOR_LABEL: seppcon-P01R6-LINSk-2nd AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: LINEAR-Skiff (P/2001 R6) EPHEMERIS: NAIF_ID=1000354, NAIF_NAME=LINEAR-Skiff (P/2001 R6) OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES MICRON_24: FIELD_SIZE = SMALL, EXPOSURE_TIME = 10, N_CYCLES = 15 SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=2739.9294, SLEW_TIME=25.0, SETTLE_TIME=39.229485, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=1054, DOWNLINK_VOLUME=47737392, VERSION=S14.1.0 INTEGRATION_TIME: MIPS_24=2258.6328,MIPS_70=0.0,MIPS_160=0.0 AOT_TYPE: MIPS Photometry AOR_LABEL: seppcon-51P-Harr-1st AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: Harrington EPHEMERIS: NAIF_ID=1000363, NAIF_NAME=Harrington OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES MICRON_24: FIELD_SIZE = SMALL, EXPOSURE_TIME = 10, N_CYCLES = 15 SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=2739.9294, SLEW_TIME=25.0, SETTLE_TIME=39.22949, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=1054, DOWNLINK_VOLUME=47737392, VERSION=S14.1.0 INTEGRATION_TIME: MIPS_24=2258.6328,MIPS_70=0.0,MIPS_160=0.0 TIMING1: START_DATE=2006 Jun 23, START_TIME=04:02:00, END_DATE=2006 Aug 2, END_TIME=11:21:00 COMMENT_START: In almost all cases, a given comet is brighter in one observability window compared to the other(s) in Cycle 3. This is our motivation for having a timing constraint. Generally the constraint covers the full interval of the brightest window in the Cycle. COMMENT_END: AOT_TYPE: MIPS Photometry AOR_LABEL: seppcon-51P-Harr-2nd AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: Harrington EPHEMERIS: NAIF_ID=1000363, NAIF_NAME=Harrington OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES MICRON_24: FIELD_SIZE = SMALL, EXPOSURE_TIME = 10, N_CYCLES = 15 SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=2739.9294, SLEW_TIME=25.0, SETTLE_TIME=39.22949, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=1054, DOWNLINK_VOLUME=47737392, VERSION=S14.1.0 INTEGRATION_TIME: MIPS_24=2258.6328,MIPS_70=0.0,MIPS_160=0.0 AOT_TYPE: MIPS Photometry AOR_LABEL: seppcon-62P-Tsu1-1st AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: Tsuchinshan 1 EPHEMERIS: NAIF_ID=1000097, NAIF_NAME=Tsuchinshan 1 OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES MICRON_24: FIELD_SIZE = SMALL, EXPOSURE_TIME = 10, N_CYCLES = 18 SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=3201.9294, SLEW_TIME=25.0, SETTLE_TIME=39.229473, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=1054, DOWNLINK_VOLUME=57019662, VERSION=S14.1.0 INTEGRATION_TIME: MIPS_24=2699.0347,MIPS_70=0.0,MIPS_160=0.0 TIMING1: START_DATE=2006 Aug 28, START_TIME=03:07:00, END_DATE=2006 Oct 8, END_TIME=10:01:00 COMMENT_START: In almost all cases, a given comet is brighter in one observability window compared to the other(s) in Cycle 3. This is our motivation for having a timing constraint. Generally the constraint covers the full interval of the brightest window in the Cycle. COMMENT_END: AOT_TYPE: MIPS Photometry AOR_LABEL: seppcon-62P-Tsu1-2nd AOR_STATUS: new MOVING_TARGET: YES TARGET_TYPE: MOVING SINGLE TARGET_NAME: Tsuchinshan 1 EPHEMERIS: NAIF_ID=1000097, NAIF_NAME=Tsuchinshan 1 OBJECT_AVOIDANCE: EARTH = YES, OTHERS = YES MICRON_24: FIELD_SIZE = SMALL, EXPOSURE_TIME = 10, N_CYCLES = 18 SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO RESOURCE_EST: TOTAL_DURATION=3201.9294, SLEW_TIME=25.0, SETTLE_TIME=39.229473, SLEW_OVERHEAD=215.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=1054, DOWNLINK_VOLUME=57019662, VERSION=S14.1.0 INTEGRATION_TIME: MIPS_24=2699.0347,MIPS_70=0.0,MIPS_160=0.0 CONSTRAINT: TYPE=SHADOW, NAME=shadow-P05S3, SHADOW_BEFORE_PRIMARY=NO RANGE_START: DAYS=0, TIME=04:00:00 RANGE_END: DAYS=1, TIME=00:00:00 AORS: AOR_PRIMARY=seppcon-P05S3-Read-1st, AOR_SHADOW=seppcon-P05S3-Read-2nd COMMENT_START: The interval of time between the two AORs is designed to give us a reasonable chance of detecting the comet in the shadow frame before it moves out of the MIPS FOV. However the comet has a proper motion that varies with time, so the interval we give here is an estimate, and it may not be suitable for all days within the observability window. Once we know when the MIPS campaign within the window will occur (from the BIC Plan), we can provide a more accurate range of times. COMMENT_END: CONSTRAINT: TYPE=SHADOW, NAME=shadow-P05T5, SHADOW_BEFORE_PRIMARY=NO RANGE_START: DAYS=0, TIME=01:00:00 RANGE_END: DAYS=0, TIME=10:00:00 AORS: AOR_PRIMARY=seppcon-P05T5-Brgtn-1st, AOR_SHADOW=seppcon-P05T5-Brgtn-2nd COMMENT_START: The interval of time between the two AORs is designed to give us a reasonable chance of detecting the comet in the shadow frame before it moves out of the MIPS FOV. However the comet has a proper motion that varies with time, so the interval we give here is an estimate, and it may not be suitable for all days within the observability window. Once we know when the MIPS campaign within the window will occur (from the BIC Plan), we can provide a more accurate range of times. COMMENT_END: CONSTRAINT: TYPE=SHADOW, NAME=shadow-139P, SHADOW_BEFORE_PRIMARY=NO RANGE_START: DAYS=0, TIME=01:00:00 RANGE_END: DAYS=1, TIME=00:00:00 AORS: AOR_PRIMARY=seppcon-139P-VO-1st, AOR_SHADOW=seppcon-139P-VO-2nd COMMENT_START: The interval of time between the two AORs is designed to give us a reasonable chance of detecting the comet in the shadow frame before it moves out of the MIPS FOV. However the comet has a proper motion that varies with time, so the interval we give here is an estimate, and it may not be suitable for all days within the observability window. Once we know when the MIPS campaign within the window will occur (from the BIC Plan), we can provide a more accurate range of times. COMMENT_END: CONSTRAINT: TYPE=SHADOW, NAME=shadow-C05W2, SHADOW_BEFORE_PRIMARY=NO RANGE_START: DAYS=0, TIME=01:00:00 RANGE_END: DAYS=1, TIME=06:00:00 AORS: AOR_PRIMARY=seppcon-C05W2-Chrst-1st, AOR_SHADOW=seppcon-C05W2-Chrst-2nd COMMENT_START: The interval of time between the two AORs is designed to give us a reasonable chance of detecting the comet in the shadow frame before it moves out of the MIPS FOV. However the comet has a proper motion that varies with time, so the interval we give here is an estimate, and it may not be suitable for all days within the observability window. Once we know when the MIPS campaign within the window will occur (from the BIC Plan), we can provide a more accurate range of times. COMMENT_END: CONSTRAINT: TYPE=SHADOW, NAME=shadow-P98VS24, SHADOW_BEFORE_PRIMARY=NO RANGE_START: DAYS=0, TIME=02:00:00 RANGE_END: DAYS=1, TIME=00:00:00 AORS: AOR_PRIMARY=seppcon-P98VS24-LIN-1st, AOR_SHADOW=seppcon-P98VS24-LIN-2nd COMMENT_START: The interval of time between the two AORs is designed to give us a reasonable chance of detecting the comet in the shadow frame before it moves out of the MIPS FOV. However the comet has a proper motion that varies with time, so the interval we give here is an estimate, and it may not be suitable for all days within the observability window. Once we know when the MIPS campaign within the window will occur (from the BIC Plan), we can provide a more accurate range of times. COMMENT_END: CONSTRAINT: TYPE=SHADOW, NAME=shadow-P05W3, SHADOW_BEFORE_PRIMARY=NO RANGE_START: DAYS=0, TIME=01:00:00 RANGE_END: DAYS=0, TIME=08:00:00 AORS: AOR_PRIMARY=seppcon-P05W3-Kwlski-1st, AOR_SHADOW=seppcon-P05W3-Kwlski-2nd COMMENT_START: The interval of time between the two AORs is designed to give us a reasonable chance of detecting the comet in the shadow frame before it moves out of the MIPS FOV. However the comet has a proper motion that varies with time, so the interval we give here is an estimate, and it may not be suitable for all days within the observability window. Once we know when the MIPS campaign within the window will occur (from the BIC Plan), we can provide a more accurate range of times. COMMENT_END: CONSTRAINT: TYPE=SHADOW, NAME=shadow-P02O8, SHADOW_BEFORE_PRIMARY=NO RANGE_START: DAYS=0, TIME=02:00:00 RANGE_END: DAYS=0, TIME=18:00:00 AORS: AOR_PRIMARY=seppcon-P02O8-NEAT-1st, AOR_SHADOW=seppcon-P02O8-NEAT-2nd COMMENT_START: The interval of time between the two AORs is designed to give us a reasonable chance of detecting the comet in the shadow frame before it moves out of the MIPS FOV. However the comet has a proper motion that varies with time, so the interval we give here is an estimate, and it may not be suitable for all days within the observability window. Once we know when the MIPS campaign within the window will occur (from the BIC Plan), we can provide a more accurate range of times. COMMENT_END: CONSTRAINT: TYPE=SHADOW, NAME=shadow-P05JD108, SHADOW_BEFORE_PRIMARY=NO RANGE_START: DAYS=0, TIME=01:00:00 RANGE_END: DAYS=0, TIME=07:00:00 AORS: AOR_PRIMARY=seppcon-P05JD108-CatNEAT-1st, AOR_SHADOW=seppcon-P05JD108-CatNEAT-2nd COMMENT_START: The interval of time between the two AORs is designed to give us a reasonable chance of detecting the comet in the shadow frame before it moves out of the MIPS FOV. However the comet has a proper motion that varies with time, so the interval we give here is an estimate, and it may not be suitable for all days within the observability window. Once we know when the MIPS campaign within the window will occur (from the BIC Plan), we can provide a more accurate range of times. COMMENT_END: CONSTRAINT: TYPE=SHADOW, NAME=shadow-P05Y2, SHADOW_BEFORE_PRIMARY=NO RANGE_START: DAYS=0, TIME=01:00:00 RANGE_END: DAYS=0, TIME=07:00:00 AORS: AOR_PRIMARY=seppcon-P05Y2-McN-1st, AOR_SHADOW=seppcon-P05Y2-McN-2nd COMMENT_START: The interval of time between the two AORs is designed to give us a reasonable chance of detecting the comet in the shadow frame before it moves out of the MIPS FOV. However the comet has a proper motion that varies with time, so the interval we give here is an estimate, and it may not be suitable for all days within the observability window. Once we know when the MIPS campaign within the window will occur (from the BIC Plan), we can provide a more accurate range of times. COMMENT_END: CONSTRAINT: TYPE=SHADOW, NAME=shadow-P01CV8, SHADOW_BEFORE_PRIMARY=NO RANGE_START: DAYS=0, TIME=01:00:00 RANGE_END: DAYS=0, TIME=10:00:00 AORS: AOR_PRIMARY=seppcon-P01CV8-LIN-1st, AOR_SHADOW=seppcon-P01CV8-LIN-2nd COMMENT_START: The interval of time between the two AORs is designed to give us a reasonable chance of detecting the comet in the shadow frame before it moves out of the MIPS FOV. However the comet has a proper motion that varies with time, so the interval we give here is an estimate, and it may not be suitable for all days within the observability window. Once we know when the MIPS campaign within the window will occur (from the BIC Plan), we can provide a more accurate range of times. COMMENT_END: CONSTRAINT: TYPE=SHADOW, NAME=shadow-P99WJ7, SHADOW_BEFORE_PRIMARY=NO RANGE_START: DAYS=0, TIME=02:00:00 RANGE_END: DAYS=0, TIME=12:00:00 AORS: AOR_PRIMARY=seppcon-P99WJ7-Korl-1st, AOR_SHADOW=seppcon-P99WJ7-Korl-2nd COMMENT_START: The interval of time between the two AORs is designed to give us a reasonable chance of detecting the comet in the shadow frame before it moves out of the MIPS FOV. However the comet has a proper motion that varies with time, so the interval we give here is an estimate, and it may not be suitable for all days within the observability window. Once we know when the MIPS campaign within the window will occur (from the BIC Plan), we can provide a more accurate range of times. COMMENT_END: CONSTRAINT: TYPE=SHADOW, NAME=shadow-P04H2, SHADOW_BEFORE_PRIMARY=NO RANGE_START: DAYS=0, TIME=02:00:00 RANGE_END: DAYS=0, TIME=09:00:00 AORS: AOR_PRIMARY=seppcon-P04H2-Larsen-1st, AOR_SHADOW=seppcon-P04H2-Larsen-2nd COMMENT_START: The interval of time between the two AORs is designed to give us a reasonable chance of detecting the comet in the shadow frame before it moves out of the MIPS FOV. However the comet has a proper motion that varies with time, so the interval we give here is an estimate, and it may not be suitable for all days within the observability window. Once we know when the MIPS campaign within the window will occur (from the BIC Plan), we can provide a more accurate range of times. COMMENT_END: CONSTRAINT: TYPE=SHADOW, NAME=shadow-P02LZ11, SHADOW_BEFORE_PRIMARY=NO RANGE_START: DAYS=0, TIME=02:00:00 RANGE_END: DAYS=0, TIME=16:00:00 AORS: AOR_PRIMARY=seppcon-P02LZ11-LIN-1st, AOR_SHADOW=seppcon-P02LZ11-LIN-2nd COMMENT_START: The interval of time between the two AORs is designed to give us a reasonable chance of detecting the comet in the shadow frame before it moves out of the MIPS FOV. However the comet has a proper motion that varies with time, so the interval we give here is an estimate, and it may not be suitable for all days within the observability window. Once we know when the MIPS campaign within the window will occur (from the BIC Plan), we can provide a more accurate range of times. COMMENT_END: CONSTRAINT: TYPE=SHADOW, NAME=shadow-93P, SHADOW_BEFORE_PRIMARY=NO RANGE_START: DAYS=0, TIME=01:00:00 RANGE_END: DAYS=0, TIME=15:00:00 AORS: AOR_PRIMARY=seppcon-93P-Lov1-1st, AOR_SHADOW=seppcon-93P-Lov1-2nd COMMENT_START: The interval of time between the two AORs is designed to give us a reasonable chance of detecting the comet in the shadow frame before it moves out of the MIPS FOV. However the comet has a proper motion that varies with time, so the interval we give here is an estimate, and it may not be suitable for all days within the observability window. Once we know when the MIPS campaign within the window will occur (from the BIC Plan), we can provide a more accurate range of times. COMMENT_END: CONSTRAINT: TYPE=SHADOW, NAME=shadow-P03KV2, SHADOW_BEFORE_PRIMARY=NO RANGE_START: DAYS=0, TIME=01:00:00 RANGE_END: DAYS=0, TIME=09:00:00 AORS: AOR_PRIMARY=seppcon-P03KV2-LIN-1st, AOR_SHADOW=seppcon-P03KV2-LIN-2nd COMMENT_START: The interval of time between the two AORs is designed to give us a reasonable chance of detecting the comet in the shadow frame before it moves out of the MIPS FOV. However the comet has a proper motion that varies with time, so the interval we give here is an estimate, and it may not be suitable for all days within the observability window. Once we know when the MIPS campaign within the window will occur (from the BIC Plan), we can provide a more accurate range of times. COMMENT_END: CONSTRAINT: TYPE=SHADOW, NAME=shadow-P05K3, SHADOW_BEFORE_PRIMARY=NO RANGE_START: DAYS=0, TIME=02:00:00 RANGE_END: DAYS=0, TIME=12:00:00 AORS: AOR_PRIMARY=seppcon-P05K3-McN-1st, AOR_SHADOW=seppcon-P05K3-LIN-2nd COMMENT_START: The interval of time between the two AORs is designed to give us a reasonable chance of detecting the comet in the shadow frame before it moves out of the MIPS FOV. However the comet has a proper motion that varies with time, so the interval we give here is an estimate, and it may not be suitable for all days within the observability window. Once we know when the MIPS campaign within the window will occur (from the BIC Plan), we can provide a more accurate range of times. COMMENT_END: CONSTRAINT: TYPE=SHADOW, NAME=shadow-P04T1, SHADOW_BEFORE_PRIMARY=NO RANGE_START: DAYS=0, TIME=03:00:00 RANGE_END: DAYS=1, TIME=00:00:00 AORS: AOR_PRIMARY=seppcon-P04T1-LINNT-1st, AOR_SHADOW=seppcon-P04T1-LINNT-2nd COMMENT_START: The interval of time between the two AORs is designed to give us a reasonable chance of detecting the comet in the shadow frame before it moves out of the MIPS FOV. However the comet has a proper motion that varies with time, so the interval we give here is an estimate, and it may not be suitable for all days within the observability window. Once we know when the MIPS campaign within the window will occur (from the BIC Plan), we can provide a more accurate range of times. COMMENT_END: CONSTRAINT: TYPE=SHADOW, NAME=shadow-148P, SHADOW_BEFORE_PRIMARY=NO RANGE_START: DAYS=0, TIME=02:00:00 RANGE_END: DAYS=1, TIME=00:00:00 AORS: AOR_PRIMARY=seppcon-148P-AndLIN-1st, AOR_SHADOW=seppcon-148P-AndLIN-2nd COMMENT_START: The interval of time between the two AORs is designed to give us a reasonable chance of detecting the comet in the shadow frame before it moves out of the MIPS FOV. However the comet has a proper motion that varies with time, so the interval we give here is an estimate, and it may not be suitable for all days within the observability window. Once we know when the MIPS campaign within the window will occur (from the BIC Plan), we can provide a more accurate range of times. COMMENT_END: CONSTRAINT: TYPE=SHADOW, NAME=shadow-169P, SHADOW_BEFORE_PRIMARY=NO RANGE_START: DAYS=0, TIME=02:00:00 RANGE_END: DAYS=0, TIME=12:00:00 AORS: AOR_PRIMARY=seppcon-169P-NEAT-1st, AOR_SHADOW=seppcon-169P-NEAT-2nd COMMENT_START: The interval of time between the two AORs is designed to give us a reasonable chance of detecting the comet in the shadow frame before it moves out of the MIPS FOV. However the comet has a proper motion that varies with time, so the interval we give here is an estimate, and it may not be suitable for all days within the observability window. Once we know when the MIPS campaign within the window will occur (from the BIC Plan), we can provide a more accurate range of times. COMMENT_END: CONSTRAINT: TYPE=SHADOW, NAME=shadow-138P, SHADOW_BEFORE_PRIMARY=NO RANGE_START: DAYS=0, TIME=02:00:00 RANGE_END: DAYS=0, TIME=12:00:00 AORS: AOR_PRIMARY=seppcon-138P-SL7-1st, AOR_SHADOW=seppcon-138P-SL7-2nd COMMENT_START: The interval of time between the two AORs is designed to give us a reasonable chance of detecting the comet in the shadow frame before it moves out of the MIPS FOV. However the comet has a proper motion that varies with time, so the interval we give here is an estimate, and it may not be suitable for all days within the observability window. Once we know when the MIPS campaign within the window will occur (from the BIC Plan), we can provide a more accurate range of times. COMMENT_END: CONSTRAINT: TYPE=SHADOW, NAME=shadow-P03O3, SHADOW_BEFORE_PRIMARY=NO RANGE_START: DAYS=0, TIME=02:00:00 RANGE_END: DAYS=0, TIME=18:00:00 AORS: AOR_PRIMARY=seppcon-P03O3-LIN-1st, AOR_SHADOW=seppcon-P03O3-LIN-2nd COMMENT_START: The interval of time between the two AORs is designed to give us a reasonable chance of detecting the comet in the shadow frame before it moves out of the MIPS FOV. However the comet has a proper motion that varies with time, so the interval we give here is an estimate, and it may not be suitable for all days within the observability window. Once we know when the MIPS campaign within the window will occur (from the BIC Plan), we can provide a more accurate range of times. COMMENT_END: CONSTRAINT: TYPE=SHADOW, NAME=shadow-15P, SHADOW_BEFORE_PRIMARY=NO RANGE_START: DAYS=0, TIME=02:00:00 RANGE_END: DAYS=0, TIME=12:00:00 AORS: AOR_PRIMARY=seppcon-15P-F-1st, AOR_SHADOW=seppcon-15P-F-2nd COMMENT_START: The interval of time between the two AORs is designed to give us a reasonable chance of detecting the comet in the shadow frame before it moves out of the MIPS FOV. However the comet has a proper motion that varies with time, so the interval we give here is an estimate, and it may not be suitable for all days within the observability window. Once we know when the MIPS campaign within the window will occur (from the BIC Plan), we can provide a more accurate range of times. COMMENT_END: CONSTRAINT: TYPE=SHADOW, NAME=shadow-P02JN16, SHADOW_BEFORE_PRIMARY=NO RANGE_START: DAYS=0, TIME=02:00:00 RANGE_END: DAYS=0, TIME=12:00:00 AORS: AOR_PRIMARY=seppcon-P02JN16-LIN-1st, AOR_SHADOW=seppcon-P02JN16-LIN-2nd COMMENT_START: The interval of time between the two AORs is designed to give us a reasonable chance of detecting the comet in the shadow frame before it moves out of the MIPS FOV. However the comet has a proper motion that varies with time, so the interval we give here is an estimate, and it may not be suitable for all days within the observability window. Once we know when the MIPS campaign within the window will occur (from the BIC Plan), we can provide a more accurate range of times. COMMENT_END: CONSTRAINT: TYPE=SHADOW, NAME=shadow-168P, SHADOW_BEFORE_PRIMARY=NO RANGE_START: DAYS=0, TIME=01:00:00 RANGE_END: DAYS=0, TIME=12:00:00 AORS: AOR_PRIMARY=seppcon-168P-Herg-1st, AOR_SHADOW=seppcon-168P-Herg-2nd COMMENT_START: The interval of time between the two AORs is designed to give us a reasonable chance of detecting the comet in the shadow frame before it moves out of the MIPS FOV. However the comet has a proper motion that varies with time, so the interval we give here is an estimate, and it may not be suitable for all days within the observability window. Once we know when the MIPS campaign within the window will occur (from the BIC Plan), we can provide a more accurate range of times. COMMENT_END: CONSTRAINT: TYPE=SHADOW, NAME=shadow-P05XA54, SHADOW_BEFORE_PRIMARY=NO RANGE_START: DAYS=0, TIME=02:00:00 RANGE_END: DAYS=0, TIME=10:00:00 AORS: AOR_PRIMARY=seppcon-P05XA54-LONHill-1st, AOR_SHADOW=seppcon-P05XA54-LONHill-2nd COMMENT_START: The interval of time between the two AORs is designed to give us a reasonable chance of detecting the comet in the shadow frame before it moves out of the MIPS FOV. However the comet has a proper motion that varies with time, so the interval we give here is an estimate, and it may not be suitable for all days within the observability window. Once we know when the MIPS campaign within the window will occur (from the BIC Plan), we can provide a more accurate range of times. COMMENT_END: CONSTRAINT: TYPE=SHADOW, NAME=shadow-P05Q4, SHADOW_BEFORE_PRIMARY=NO RANGE_START: DAYS=0, TIME=03:00:00 RANGE_END: DAYS=1, TIME=00:00:00 AORS: AOR_PRIMARY=seppcon-P05Q4-LIN-1st, AOR_SHADOW=seppcon-P05Q4-LIN-2nd COMMENT_START: The interval of time between the two AORs is designed to give us a reasonable chance of detecting the comet in the shadow frame before it moves out of the MIPS FOV. However the comet has a proper motion that varies with time, so the interval we give here is an estimate, and it may not be suitable for all days within the observability window. Once we know when the MIPS campaign within the window will occur (from the BIC Plan), we can provide a more accurate range of times. COMMENT_END: CONSTRAINT: TYPE=SHADOW, NAME=shadow-P00Y3, SHADOW_BEFORE_PRIMARY=NO RANGE_START: DAYS=0, TIME=02:00:00 RANGE_END: DAYS=0, TIME=12:00:00 AORS: AOR_PRIMARY=seppcon-P00Y3-Scotti-1st, AOR_SHADOW=seppcon-P00Y3-Scotti-2nd COMMENT_START: The interval of time between the two AORs is designed to give us a reasonable chance of detecting the comet in the shadow frame before it moves out of the MIPS FOV. However the comet has a proper motion that varies with time, so the interval we give here is an estimate, and it may not be suitable for all days within the observability window. Once we know when the MIPS campaign within the window will occur (from the BIC Plan), we can provide a more accurate range of times. COMMENT_END: CONSTRAINT: TYPE=SHADOW, NAME=shadow-11P, SHADOW_BEFORE_PRIMARY=NO RANGE_START: DAYS=0, TIME=02:00:00 RANGE_END: DAYS=0, TIME=16:00:00 AORS: AOR_PRIMARY=seppcon-11P-TSL-1st, AOR_SHADOW=seppcon-11P-TSL-2nd COMMENT_START: The interval of time between the two AORs is designed to give us a reasonable chance of detecting the comet in the shadow frame before it moves out of the MIPS FOV. However the comet has a proper motion that varies with time, so the interval we give here is an estimate, and it may not be suitable for all days within the observability window. Once we know when the MIPS campaign within the window will occur (from the BIC Plan), we can provide a more accurate range of times. COMMENT_END: CONSTRAINT: TYPE=SHADOW, NAME=shadow-16P, SHADOW_BEFORE_PRIMARY=NO RANGE_START: DAYS=0, TIME=02:00:00 RANGE_END: DAYS=0, TIME=20:00:00 AORS: AOR_PRIMARY=seppcon-16P-Br2-1st, AOR_SHADOW=seppcon-16P-Br2-2nd COMMENT_START: The interval of time between the two AORs is designed to give us a reasonable chance of detecting the comet in the shadow frame before it moves out of the MIPS FOV. However the comet has a proper motion that varies with time, so the interval we give here is an estimate, and it may not be suitable for all days within the observability window. Once we know when the MIPS campaign within the window will occur (from the BIC Plan), we can provide a more accurate range of times. COMMENT_END: CONSTRAINT: TYPE=SHADOW, NAME=shadow-144P, SHADOW_BEFORE_PRIMARY=NO RANGE_START: DAYS=0, TIME=01:00:00 RANGE_END: DAYS=0, TIME=10:00:00 AORS: AOR_PRIMARY=seppcon-144P-Kush-1st, AOR_SHADOW=seppcon-144P-Kush-2nd COMMENT_START: The interval of time between the two AORs is designed to give us a reasonable chance of detecting the comet in the shadow frame before it moves out of the MIPS FOV. However the comet has a proper motion that varies with time, so the interval we give here is an estimate, and it may not be suitable for all days within the observability window. Once we know when the MIPS campaign within the window will occur (from the BIC Plan), we can provide a more accurate range of times. COMMENT_END: CONSTRAINT: TYPE=SHADOW, NAME=shadow-P02S1, SHADOW_BEFORE_PRIMARY=NO RANGE_START: DAYS=0, TIME=02:00:00 RANGE_END: DAYS=0, TIME=18:00:00 AORS: AOR_PRIMARY=seppcon-P02S1-Skiff-1st, AOR_SHADOW=seppcon-P02S1-Skiff-2nd COMMENT_START: The interval of time between the two AORs is designed to give us a reasonable chance of detecting the comet in the shadow frame before it moves out of the MIPS FOV. However the comet has a proper motion that varies with time, so the interval we give here is an estimate, and it may not be suitable for all days within the observability window. Once we know when the MIPS campaign within the window will occur (from the BIC Plan), we can provide a more accurate range of times. COMMENT_END: CONSTRAINT: TYPE=SHADOW, NAME=shadow-P03HT15, SHADOW_BEFORE_PRIMARY=NO RANGE_START: DAYS=0, TIME=01:00:00 RANGE_END: DAYS=0, TIME=10:00:00 AORS: AOR_PRIMARY=seppcon-P03HT15-LIN-1st, AOR_SHADOW=seppcon-P03HT15-LIN-2nd COMMENT_START: The interval of time between the two AORs is designed to give us a reasonable chance of detecting the comet in the shadow frame before it moves out of the MIPS FOV. However the comet has a proper motion that varies with time, so the interval we give here is an estimate, and it may not be suitable for all days within the observability window. Once we know when the MIPS campaign within the window will occur (from the BIC Plan), we can provide a more accurate range of times. COMMENT_END: CONSTRAINT: TYPE=SHADOW, NAME=shadow-P04A1, SHADOW_BEFORE_PRIMARY=NO RANGE_START: DAYS=0, TIME=01:00:00 RANGE_END: DAYS=0, TIME=12:00:00 AORS: AOR_PRIMARY=seppcon-P04A1-LONEOS-1st, AOR_SHADOW=seppcon-P04A1-LONEOS-2nd COMMENT_START: The interval of time between the two AORs is designed to give us a reasonable chance of detecting the comet in the shadow frame before it moves out of the MIPS FOV. However the comet has a proper motion that varies with time, so the interval we give here is an estimate, and it may not be suitable for all days within the observability window. Once we know when the MIPS campaign within the window will occur (from the BIC Plan), we can provide a more accurate range of times. COMMENT_END: CONSTRAINT: TYPE=SHADOW, NAME=shadow-P01R6, SHADOW_BEFORE_PRIMARY=NO RANGE_START: DAYS=0, TIME=02:00:00 RANGE_END: DAYS=0, TIME=16:00:00 AORS: AOR_PRIMARY=seppcon-P01R6-LINSk-1st, AOR_SHADOW=seppcon-P01R6-LINSk-2nd COMMENT_START: The interval of time between the two AORs is designed to give us a reasonable chance of detecting the comet in the shadow frame before it moves out of the MIPS FOV. However the comet has a proper motion that varies with time, so the interval we give here is an estimate, and it may not be suitable for all days within the observability window. Once we know when the MIPS campaign within the window will occur (from the BIC Plan), we can provide a more accurate range of times. COMMENT_END: CONSTRAINT: TYPE=SHADOW, NAME=shadow-51P, SHADOW_BEFORE_PRIMARY=NO RANGE_START: DAYS=0, TIME=02:00:00 RANGE_END: DAYS=0, TIME=16:00:00 AORS: AOR_PRIMARY=seppcon-51P-Harr-1st, AOR_SHADOW=seppcon-51P-Harr-2nd COMMENT_START: The interval of time between the two AORs is designed to give us a reasonable chance of detecting the comet in the shadow frame before it moves out of the MIPS FOV. However the comet has a proper motion that varies with time, so the interval we give here is an estimate, and it may not be suitable for all days within the observability window. Once we know when the MIPS campaign within the window will occur (from the BIC Plan), we can provide a more accurate range of times. COMMENT_END: CONSTRAINT: TYPE=SHADOW, NAME=shadow-62P, SHADOW_BEFORE_PRIMARY=NO RANGE_START: DAYS=0, TIME=02:00:00 RANGE_END: DAYS=1, TIME=00:00:00 AORS: AOR_PRIMARY=seppcon-62P-Tsu1-1st, AOR_SHADOW=seppcon-62P-Tsu1-2nd COMMENT_START: The interval of time between the two AORs is designed to give us a reasonable chance of detecting the comet in the shadow frame before it moves out of the MIPS FOV. However the comet has a proper motion that varies with time, so the interval we give here is an estimate, and it may not be suitable for all days within the observability window. Once we know when the MIPS campaign within the window will occur (from the BIC Plan), we can provide a more accurate range of times. COMMENT_END: