Table 1
Compact far-infrared sources, selected by largest ΣFIR and/or ΩBB/ Ωmeasured.
Name | Morph | RA | Dec | z | log(LFIR) | R e,70 | log(ΣFIR) | ΩBB/ Ωm |
J2000 | J2000 | L ⊙ | kpc | L⊙ kpc-2 | ||||
(1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) |
|
||||||||
III Zw 035 | D | 26.1280 | 17.1021 | 0.0274 | 11.47 | 0.272 | 11.81 | 0.05 |
NGC 1266 | 49.0036 | –2.4273 | 0.0072 | 10.32 | <0.066 | >11.89 | >0.13 | |
IRAS F05189-2524 | 80.2558 | –25.3622 | 0.0426 | 11.75 | 0.386 | 11.78 | 0.04 | |
NGC 2623 | 129.6000 | 25.7550 | 0.0185 | 11.41 | 0.218 | 11.93 | 0.10 | |
IRAS F09111-1007W | D | 138.4016 | –10.3245 | 0.0550 | 11.75 | 0.456 | 11.64 | 0.10 |
IRAS F10173+0828 | 155.0011 | 8.2260 | 0.0491 | 11.57 | 0.317 | 11.77 | 0.04 | |
IRAS F12224-0624 | 186.2663 | –6.6811 | 0.0264 | 11.12 | 0.175 | 11.83 | 0.11 | |
NGC 4418 | 186.7277 | –0.8776 | 0.0073 | 10.81 | 0.056 | 12.52 | 0.14 | |
Mkn 231 | 194.0590 | 56.8738 | 0.0422 | 12.23 | <0.386 | >12.26 | >0.11 | |
IC 0860 | 198.7647 | 24.6188 | 0.0112 | 10.82 | 0.095 | 12.07 | 0.10 | |
IRAS 13120-5453 | 198.7765 | –55.1568 | 0.0308 | 12.10 | 0.451 | 11.99 | 0.15 | |
ESO 173-G015 | 201.8483 | –57.4898 | 0.0097 | 11.42 | 0.297 | 11.67 | 0.09 | |
Mkn 273 | 206.1758 | 55.8875 | 0.0378 | 11.93 | <0.317 | >12.13 | >0.12 | |
IRAS F14378-3651 | 220.2455 | –37.0754 | 0.0676 | 11.94 | 0.465 | 11.81 | 0.05 | |
CGCG 049-057 | 228.3046 | 7.2257 | 0.0130 | 11.12 | 0.163 | 11.90 | 0.15 | |
Arp 220 | 233.7381 | 23.5038 | 0.0181 | 12.11 | 0.246 | 12.53 | 0.35 | |
IRAS F17207-0014 | 260.8416 | –0.2838 | 0.0428 | 12.27 | 0.564 | 11.97 | 0.10 | |
NGC 7479 | 346.2359 | 12.3229 | 0.0079 | 10.27 | 0.118 | 11.32 | 0.23 |
Notes. (2) “D” denotes a pair/double galaxy (3), (4) Measured FIR position. For small and symmetric objects, this may be less accurate than the best literature position. (9) Ratio of solid angle of a blackbody emitting half of the FIR flux at the temperature fitting the PACS photometry to measured half light solid angle.
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