Free Access

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.

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.