Columns: (1) Comet, (2) flux density at 16um in mJy, (3) flux density at 22um (for IRS) or 24um (for MIPS) in mJy, (4) V magnitude, (5) Instrument used to observe.
(1) (2) (3) (4) (5)
143P/Kowal-Mrkos 7.05 12.10 20.8 IRS
47P/Ashbrook-Jackson 4.59 6.98 21.4 IRS
48P/Johnson 3.63 5.75 21.6 IRS
7P/Pons-Winnecke 3.13 4.91 21.8 IRS
P/2004 F3 (NEAT) 2.95 4.36 22.0 IRS
129P/Shoemaker-Levy 3 2.82 4.19 22.0 IRS
P/2005 GF8 (LONEOS) 2.72 4.06 22.0 IRS
31P/Schwassmann-W. 2 2.56 4.26 22.0 IRS
14P/Wolf 2.52 3.94 22.0 IRS
P/2005 S3 (Read) 4.46 22.0 MIPS
P/2005 T5 (Broughton) 4.27 22.0 MIPS
139P/Vaisala-Otererma 4.17 22.0 MIPS
107P/Wilson-Harrington 1.97 2.94 22.1 IRS
C/2005 W2 (Christensen) 3.91 22.1 MIPS
P/1998 VS24 (LINEAR) 3.80 22.1 MIPS
119P/Parker-Hartley 2.31 3.53 22.2 IRS
74P/Smirnova-Chernykh 2.21 3.48 22.2 IRS
118P/Shoemaker-Levy 4 1.79 2.96 22.3 IRS
137P/Shoemaker-Levy 2 1.37 2.47 22.5 IRS
P/2005 W3 (Kowalski) 2.78 22.5 MIPS
P/2005 L4 (Christensen) 1.66 2.45 22.6 IRS
68P/Klemola 1.32 2.23 22.6 IRS
P/2002 O8 (NEAT) 2.43 22.6 MIPS
P/2005 R2 (Van Ness) 1.50 2.24 22.7 IRS
121P/Shoemaker-Holt 2 1.36 2.09 22.7 IRS
P/2001 YX127 (LINEAR) 1.28 2.11 22.7 IRS
173P/Mueller 5 1.24 2.05 22.7 IRS
P/2005 JD108 (Catalina-N.) 2.30 22.7 MIPS
172P/Yeung 1.37 2.07 22.8 IRS
P/2005 R1 (NEAT) 1.34 2.04 22.8 IRS
6P/d'Arrest 1.24 1.93 22.8 IRS
101P/Chernykh 1.15 1.78 22.9 IRS
P/2004 V5 (LINEAR-Hill) 0.96 1.65 22.9 IRS
P/2003 S1 (NEAT) 0.95 1.64 22.9 IRS
P/2005 Y2 (McNaught) 1.94 22.9 MIPS
78P/Gehrels 2 1.09 1.65 23.0 IRS
127P/Holt-Olmstead 1.07 1.68 23.0 IRS
79P/du Toit-Hartley 1.03 1.60 23.0 IRS
131P/Mueller 2 1.02 1.60 23.0 IRS
33P/Daniel 0.99 1.56 23.0 IRS
P/2001 CV8 (LINEAR) 1.74 23.0 MIPS
P/1999 WJ7 (Korlevic) 1.69 23.0 MIPS
P/2004 H2 (Larsen) 1.69 23.0 MIPS
130P/McNaught-Hughes 0.95 1.51 23.1 IRS
22P/Kopff 0.82 1.38 23.1 IRS
77P/Longmore 0.85 1.37 23.2 IRS
P/2004 VR8 (LONEOS) 0.80 1.30 23.2 IRS
P/2004 V3 (Siding Spring) 0.69 1.25 23.2 IRS
P/2002 X2 (NEAT) 0.68 1.22 23.2 IRS
43P/Wolf-Harrington 0.75 1.30 23.2 IRS
94P/Russell 4 0.74 1.22 23.3 IRS
89P/Russell 2 0.72 1.19 23.3 IRS
120P/Mueller 1 0.69 1.15 23.3 IRS
P/2004 DO29 (Sp.-L.) 0.63 1.15 23.3 IRS
P/2002 LZ11 (LINEAR) 1.25 23.3 MIPS
54P/de Vico-Swift-NEAT 0.62 1.04 23.4 IRS
159P/LONEOS 0.59 1.07 23.4 IRS
149P/Mueller 4 0.58 1.06 23.4 IRS
32P/Comas Sola 0.70 1.05 23.5 IRS
56P/Slaughter-Burnham 0.53 0.93 23.5 IRS
152P/Helin-Lawrence 0.51 0.96 23.5 IRS
93P/Lovas 1 1.10 23.5 MIPS
P/2005 JQ5 (Catalina) 0.63 0.95 23.6 IRS
163P/NEAT 0.70 1.03 23.6 IRS
113P/Spitaler 0.63 0.97 23.6 IRS
50P/Arend 0.63 0.95 23.6 IRS
124P/Mrkos 0.60 0.91 23.6 IRS
P/2003 S2 (NEAT) 0.54 0.91 23.6 IRS
160P/LINEAR 0.53 0.92 23.6 IRS
123P/West-Hartley 0.49 0.86 23.6 IRS
37P/Forbes 0.59 0.90 23.6 IRS
P/2003 KV2 (LINEAR) 1.02 23.6 MIPS
P/2000 Y3 (Scotti) 0.95 23.6 MIPS
57P/du Toit-Neujmin-D. 0.58 0.89 23.7 IRS
162P/Siding Spring 0.57 0.87 23.7 IRS
171P/Spahr 0.54 0.83 23.7 IRS
69P/Taylor 0.56 0.86 23.7 IRS
141P/Machholz 2 0.56 0.85 23.7 IRS
P/2003 HT15 (LINEAR) 0.84 23.7 MIPS
P/2004 A1 (LONEOS) 0.84 23.7 MIPS
132P/Helin-Roman-Alu 2 0.58 0.86 23.8 IRS
146P/Shoemaker-LINEAR 0.57 0.85 23.8 IRS
P/2005 K3 (McNaught) 0.86 23.8 MIPS
P/2004 T1 (LINEAR-NEAT) 0.84 23.8 MIPS
148P/Anderson-LINEAR 0.83 23.8 MIPS
169P/NEAT 0.82 23.8 MIPS
P/2002 S1 (Skiff) 0.77 23.8 MIPS
138P/Shoemaker-Levy 7 0.81 23.8 MIPS
P/2003 O3 (LINEAR) 0.80 23.8 MIPS
15P/Finlay 0.79 23.8 MIPS
P/2002 JN16 (LINEAR) 0.78 23.9 MIPS
168P/Hergenrother 0.76 23.9 MIPS
P/2005 XA54 (LONEOS-Hill) 0.76 23.9 MIPS
P/2005 Q4 (LINEAR) 0.75 23.9 MIPS
11P/Tempel-Swift-LINEAR 0.74 23.9 MIPS
P/2001 R6 (LINEAR-Skiff) 0.72 23.9 MIPS
51P/Harrington 0.68 24.0 MIPS
16P/Brooks 2 0.69 24.0 MIPS
144P/Kushida 0.69 24.0 MIPS
62P/Tsuchinshan 0.66 24.0 MIPS