Table 1
Radio and infrared data for the 35 LIRG systems of our sample.
Name | RA | Dec | S1.49 GHz | S8.44 GHz |
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log L1.4 GHz | log LIR | qIR | IR8 | Radio structure | Alternative | |
(J2000) | (J2000) | (mJy) | (mJy) | (W Hz-1) | (L⊙) | 1.49 GHz | 8.44 GHz | name | ||||
(1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | (10) | (11) | (12) | (13) |
|
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(1) NGC 0034 (S) |
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− 12°06m26s | 56.0 ± 0.3 | 15.21 ± 0.01 | 0.748 ± 0.002 | 16.68 | 11.431 | 2.75 | 11.901 | COM? | EXT? | NGC 0017 |
(2) IC 1623A/B |
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− 17°30m24s | 201.27 ± 0.09 | 13.491 ± 0.003 | 1.558 ± 0.001 | 17.25 | 11.706 | 2.45 | 9.521 | CMX | CMX | Arp 236 |
(3) CGCG 436-030 |
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14°21m42s | 41.4 ± 0.2 | 13.337 ± 0.009 | 0.654 ± 0.002 | 16.96 | 11.686 | 2.72 | 11.464 | COM? | CMX | MCG |
+02-04-025 | ||||||||||||
(4) IRAS F01364-1042 |
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− 10°27m12s | 15.9 ± 0.1 | 8.35 ± 0.02 | 0.371 ± 0.006 | 16.94 | 11.848 | 2.90 | 55.498 | COM? | COM? | 2MASX J0138 |
5289-1027113 | ||||||||||||
(5) IRAS F01417+1651 |
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17°06m08s | 38.4 ± 0.5 | 19.95 ± 0.05 | 0.378 ± 0.003 | 16.83 | 11.639 | 2.81 | 36.755 | COM | COM | III Zw 035 |
(6) UGC 02369 (S) |
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14°58m15s | 41.9 ± 0.2 | 8.917 ± 0.007 | 0.892 ± 0.002 | 16.98 | 11.66 | 2.68 | 14.333 | CMX | CMX | |
(7) IRAS F03359+1523 |
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15°32m53s | 17.4 ± 0.1 | 7.46 ± 0.01 | 0.490 ± 0.005 | 16.70 | 11.545 | 2.85 | 21.425 | EXT | CMX | |
(8) ESO 550-IG025 (N) |
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− 18°48m39s | 15.79 ± 0.06 | 6.68 ± 0.01 | 0.495 ± 0.005 | 16.57 | 11.133 | 2.56 | – | COM | DB | MCG |
-03-12-002 | ||||||||||||
(9) ESO 550-IG025 (S) |
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− 18°48m56s | 12.44 ± 0.07 | 3.024 ± 0.003 | 0.815 ± 0.005 | 16.47 | 11.268 | 2.80 | – | COM | DF | MCG |
-03-12-002 | ||||||||||||
(10) IRAS F05189-2524 |
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− 25°21m45s | 26.9 ± 0.2 | 10.97 ± 0.02 | 0.518 ± 0.005 | 17.07 | 12.163 | 3.09 | 10.660 | COM | EXT? | 2MASX J0521 |
0136-2521450 | ||||||||||||
(11) NGC 2623 |
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25°45m16s | 95.6 ± 0.7 | 34.63 ± 0.03 | 0.585 ± 0.001 | 16.92 | 11.597 | 2.68 | 29.703 | COM | COM? | Arp 243 |
(12) IRAS F08572+3915 |
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39°03m53s | 5.4 ± 0.1 | 4.07 ± 0.02 | 0.17 ± 0.04 | 16.69 | 12.163 | 3.48 | 4.949 | COM | COM | |
(13) UGC 04881 (NE) |
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44°19m58s | 19.8 ± 0.2 | 7.41 ± 0.02 | 0.566 ± 0.004 | 16.89 | 11.578 | 2.69 | 21.656 | COM? | COM? | MCG |
+08-17-065 | ||||||||||||
(14) UGC 04881 (SW) |
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44°19m51s | 8.00 ± 0.07 | 1.102 ± 0.004 | 1.143 ± 0.004 | 16.50 | 11.243 | 2.74 | 21.656 | DF | DF | Arp 055 |
(15) UGC 05101 |
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61°21m11s | 133.9 ± 0.6 | 51.05 ± 0.06 | 0.556 ± 0.001 | 17.72 | 12.015 | 2.30 | 17.085 | COM? | EXT | MCG |
+10-14-026 | ||||||||||||
(16) IRAS F10173+0828 |
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08°13m33s | 7.9 ± 0.1 | 5.21 ± 0.04 | 0.24 ± 0.01 | 16.70 | 11.861 | 3.16 | 102.227 | COM | COM | 2MASX J1020 |
0023+0813342 | ||||||||||||
(17) IRAS F10565+2448 |
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24°32m34s | 44.9 ± 0.4 | 12.70 ± 0.01 | 0.728 ± 0.002 | 17.34 | 12.083 | 2.75 | 18.245 | COM | EXT | 2MASX J1059 |
1815+2432343 | ||||||||||||
(18) MCG +07-23-019 |
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40°50m59s | 28.2 ± 0.1 | 10.27 ± 0.01 | 0.582 ± 0.003 | 16.94 | 11.668 | 2.73 | 14.881 | EXT | EXT | Arp 148 |
(19) UGC 06436 (NW) |
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14°40m35s | 13.9 ± 0.1 | 3.354 ± 0.005 | 0.822 ± 0.007 | 16.63 | 11.456 | 2.83 | 11.430 | COM? | COM? | IRAS F11231 |
+1456 | ||||||||||||
(20) UGC 06436 (SE) |
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14°40m06s | 6.09 ± 0.09 | 1.207 ± 0.005 | 0.933 ± 0.007 | 16.27 | 11.178 | 2.91 | COM? | COM? | IC 2810 | |
(21) NGC 3690 (E) |
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58°33m46s | 271.7 ± 0.2 | 89.94 ± 0.06 | 0.637 ± 0.001 | 16.93 | 11.668 | 2.74 | 12.707 | CMX | CMX | IC 694 |
(22) NGC 3690 (W) |
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58°33m40s | 118.1 ± 0.2 | 23.32 ± 0.01 | 0.935 ± 0.001 | 16.56 | 11.578 | 3.01 | 12.707 | CMX | CMX | IC 694 |
(23) IRAS F12112+0305 (NE) |
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02°48m41s | 18.3 ± 0.3 | 8.06 ± 0.02 | 0.473 ± 0.009 | 17.43 | 12.123 | 2.69 | 29.811t | COM | COM | |
(24) IRAS F12112+0305 (SW) |
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02°48m38s | 4.6 ± 0.1 | 1.67 ± 0.01 | 0.586 ± 0.009 | 16.84 | 11.990 | 3.15 | 29.811t | COM | COM | |
(25) UGC 08058 |
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56°52m24s | 239.9 ± 1.4 | 266.5 ± 0.5 | − 0.060 ± 0.001 | 18.04 | 12.571 | 2.53 | 8.272 | COM | COM? | Mrk 231 |
(26) VV 250a (NW) |
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62°07m45s | 6.7 ± 0.1 | 1.475 ± 0.008 | 0.87 ± 0.02 | 16.22 | 11.115 | 2.89 | 10.514 | COM | CMX | UGC 08335 (W) |
(27) VV 250a (SE) |
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62°07m28s | 40.9 ± 0.4 | 32.67 ± 0.02 | 0.13 ± 0.02 | 17.01 | 11.709 | 2.70 | 10.514 | COM | CMX | UGC 08335 (E) |
(28) UGC 08387 |
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34°08m21s | 100.5 ± 0.5 | 33.93 ± 0.01 | 0.626 ± 0.001 | 17.17 | 11.731 | 2.56 | 15.105 | COM? | CMX | Arp 193 |
(29) NGC 5256 (NE) |
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48°16m41s | 25.8 ± 0.2 | 7.88 ± 0.01 | 0.684 ± 0.001 | 17.16 | 11.132 | 2.41 | 10.371 | COM | COM | Mrk 266 (NE) |
(30) NGC 5256 (SW) |
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48°16m32s | 31.9 ± 0.2 | 8.603 ± 0.003 | 0.757 ± 0.001 | 16.82 | 11.355 | 2.54 | – | EXT | EXT | Mrk 266 (SW) |
(31) NGC 5256 (C) |
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48°16m35s | 38.3 ± 0.2 | 3.789 ± 0.003 | 1.334 ± 0.001 | 16.50 | – | – | – | EXT | EXT | Mrk 266 (C) |
(32) NGC 5257 (NW) |
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00°50m24s | 6.27 ± 0.04 | 1.115 ± 0.002 | 0.99 ± 0.05 | 15.95 | 11.312 | 3.36 | 6.159 | CMX | CMX | Arp 240 |
(33) UGC 08696 | ![]() |
55°53m13s | 129.5 ± 0.6 | 43.75 ± 0.06 | 0.725 ± 0.001 | 17.68 | 12.209 | 2.53 | 27.983 | COM? | CMX | Mrk 273 |
(34) IRAS F14348-1447 (NE) |
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− 15°00m21s | 12.5 ± 0.1 | 3.55 ± 0.01 | 0.727 ± 0.003 | 17.39 | 11.950 | 2.56 | 24.887t | COM | COM | |
(35) IRAS F14348-1447 (SW) |
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− 15°00m24s | 20.28 ± 0.1 | 6.05 ± 0.01 | 0.697 ± 0.003 | 17.59 | 12.193 | 2.60 | 24.887t | COM | COM | |
(36) VV 340a (N) |
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24°37m02s | 55.4 ± 0.1 | 3.099 ± 0.005 | 1.66 ± 0.01 | 17.23 | 11.658 | 2.43 | 6.958 | DBDB | DB | UGC 09618 |
(37) VV 705 (N) |
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42°44m44s | 26.4 ± 0.2 | 8.23 ± 0.01 | 0.673 ± 0.002 | 17.04 | 11.849 | 2.81 | 14.589 | COM? | COM? | I ZW 107 |
(38) VV 705 (S) |
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42°44m38s | 18.0 ± 0.1 | 2.178 ± 0.008 | 1.217 ± 0.002 | 16.88 | 11.120 | 2.24 | COM? | COM? | I ZW 107 | |
(39) IRAS F15250+3608 |
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35°58m36s | 12.1 ± 0.2 | 10.34 ± 0.06 | 0.09 ± 0.01 | 17.00 | 12.081 | 3.08 | 11.320 | COM | COM | |
(40) UGC 09913 |
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23°30m11s | 303.5 ± 1.9 | 147.09 ± 0.09 | 0.417 ± 0.001 | 17.46 | 12.275 | 2.82 | 72.130 | COM? | DB | Arp 220 |
(41) NGC 6090 |
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52°27m26s | 45.24 ± 0.06 | 0.513 ± 0.004 | 2.583 ± 0.003 | 17.02 | 11.580 | 2.56 | 8.525 | DB | DB | I ZW 135 |
(42) IRAS F17132+5313 (NE) |
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53°10m31s | 5.92 ± 0.1 | 2.31 ± 0.01 | 1.065 ± 0.009 | 17.00 | 11.876 | 2.88 | 11.440t | EXT | DF | |
(43) IRAS F17132+5313 (SW) |
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53°10m28s | 14.71 ± 0.1 | 2.320 ± 0.004 | 0.542 ± 0.009 | 16.60 | 11.206 | 2.60 | 11.440t | COM | COM | |
(44) IRAS F22491-1808 |
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− 17°52m23s | 5.37 ± 0.05 | 2.82 ± 0.01 | 0.37 ±0.01 | 16.93 | 12.201 | 3.27 | 33.912 | COM? | COM? | |
(45) IC 5298 |
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25°33m23s | 25.5 ± 0.1 | 7.079 ± 0.009 | 0.740 ± 0.004 | 16.65 | 11.600 | 2.95 | 15.843 | COM | CMX | ZW 475.065 |
(46) Mrk 0331 (N) |
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20°35m10s | 63.7 ± 0.2 | 15.743 ± 0.008 | 0.806 ± 0.002 | 16.69 | 11.497 | 2.81 | 11.549 | COM? | CMX | UGC 12812 (E) |
Notes. Columns: (1) Name of the galaxy; systems are marked with the relative position to each other (e.g. N, S, E, W); the numbers before the object names are used in Fig. 5. (2) and (3) Right Ascension (J2000) and Declination (J2000), respectively, at the radio position with maximum flux density at 1.49 GHz. (4) and (5) Integrated flux density at 1.49 and 8.44 GHz, respectively, of the galaxy where flux above 3σ is being considered in the calculation. We also give the error on the measurement. (6) Radio spectral index calculated between 1.49 and 8.44 GHz. (7) The radio luminosity at 1.49 GHz calculated using the standard relation between flux and luminosity; the values of luminosity distance are taken from Diaz-Santos et al. (2010). (8) The total infrared luminosity calculated from 8 to 1000 μm for each galaxy (see Diaz-Santos et al. 2010). (9) The parameter qIR = log 10 [ (SIR(8 − 1000μm)/ 3.75 × 1012W m-2)/(S1.4 GHz/ W m-2 Hz-1)] (Helou et al. 1985). (10) The ratio of total IR luminosity to the luminosity at 8 μm (IR8; e.g. Elbaz et al. 2011). (11) and (12) The radio structure at 1.49 and 8.44 GHz, respectively: COM for compact; EXT for extended; CMX for complex, DB for double; DBDB for double double; and DF for diffuse; a “?” indicates uncertainty in the classification. (13) Gives an alternative name for the galaxy. The base-10 logarithm of the total infrared luminosity of IRAS F14348-1447 is 12.390. Here we give the fractional contribution of the two components to the total infrared luminosity. The fractional contribution was calculated by doing photometry on the 8 and 24 μm maps of the object. Similarly for IRAS F12112+0305 log 10(LIR) = 12.363 and for IRAS F17132+5313 log 10(LIR) = 11.961. A (t) next to the values of IR8 stands for total measurement for the system.
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