Table 1
General properties of the (U)LIRGs in the VIMOS sample.
| ID1 | ID2 | α | δ | z | References | D | Scale | log LIR | Class | Spectral | References | |
| IRAS | Other | (J2000) | (J2000) | (Mpc) | (pc/arcsec) | (L⊙) | Classification | |||||
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | (10) | (11) | (12) | |
|
|
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| F01159−4443 | ESO 244−G012 | 01:18:08.1 | –44:27:40 | 0.022903 | 1 | 99.8 | 462 | 11.48 | 1 | H(N), H/S(S) | 4, 5 | |
| F01341–3735 | ESO-297−G011/G012 | 01:36:24.0 | –37:19:14 | 0.017305 | 2 | 75.1 | 352 | 11.18 | 1 | H(both) | 4, 5 | |
| F04315−0840 | NGC 1614 | 04:34:00.0 | –08:34:46 | 0.015938 | 3 | 69.1 | 325 | 11.69 | 2 | H | 1, 5 | |
| F05189−2524 | 05:21:01.4 | –25:21:46 | 0.042563 | 4 | 188.2 | 839 | 12.19 | 2 | S | 3 | ||
| F06035−7102 | 06:02:54.5 | –71:03:08 | 0.079465 | 5 | 360.7 | 1501 | 12.26 | 1 | H | 2 | ||
| F06076−2139 | 06:09:45.1 | –21:40:22 | 0.037446 | 5 | 165.0 | 743 | 11.67 | 1 | – | – | ||
| F06206−6315a | 06:21:00.9 | –63:17:23 | 0.092441 | 5 | 423.3 | 1720 | 12.27 | 1 | S | 2 | ||
| F06259−4708 | ESO 255−IG 007 | 06:27:21.1 | –47:10:38 | 0.038790 | 6 | 171.1 | 769 | 11.91 | 1 | H(N) | 4 | |
| F06295−1735 | ESO 557−G002 | 06:31:46.3 | –17:37:15 | 0.021298 | 7 | 92.7 | 431 | 11.27 | 0 | H | 5 | |
| F06592−6313 | 06:59:40.3 | –63:17:53 | 0.022956 | 5 | 100.0 | 464 | 11.22 | 0 | H | 5 | ||
| F07027−6011 | AM 0702−601 | 07:03:27.5 | –60:16:05 | 0.031322 | 5 | 137.4 | 626 | 11.64 | 0 | S(N) | 4 | |
| F07160−6215 | NGC 2369 | 07:16:37.7 | –62:20:37 | 0.010807 | 2 | 46.7 | 221 | 11.16 | 0 | ... | ... | |
| 08355−4944 | 08:37:02.3 | –49:54:32 | 0.025898 | 8 | 113.1 | 521 | 11.60 | 2 | ... | ... | ||
| 08424−3130 | ESO 432−IG006 | 08:44:27.6 | –31:41:41 | 0.016165 | 5 | 70.1 | 329 | 11.04 | 1 | ... | ... | |
| F08520−6850 | ESO 60−IG016 | 08:52:31.2 | –69:01:59 | 0.046315 | 9 | 205.4 | 909 | 11.83 | 1 | ... | ... | |
| 09022−3615 | 09:04:12.8 | –36:27:02 | 0.059641 | 5 | 267.0 | 1153 | 12.32 | 2 | ... | ... | ||
| F09437+0317 | IC-563/ 564 | 09:46:20.3 | +03:03:22 | 0.020467 | 10 | 89.0 | 415 | 11.21 | 1/0 | ... | ... | |
| F10015−0614 | NGC-3110 | 10:04:02.7 | –06:28:35 | 0.016858 | 2 | 73.1 | 343 | 11.31 | 0 | H | 5 | |
| F10038−3338 | IC 2545 | 10:06:04.2 | –33:53:04 | 0.034100 | 5 | 149.9 | 679 | 11.77 | 2 | ... | ... | |
| F10257−4339b | NGC 3256 | 10:27:52.4 | –43:54:25 | 0.009354 | 2 | 40.4 | 192 | 11.69 | 2 | H | 7 | |
| F10409−4556 | ESO 264−G036 | 10:43:07.0 | –46:12:43 | 0.021011 | 11 | 91.4 | 425 | 11.26 | 0 | H/L | 5 | |
| F10567−4310 | ESO 264−G057 | 10:59:02.4 | –43:26:33 | 0.017199 | 5 | 74.6 | 350 | 11.07 | 0 | H | 5 | |
| F11255−4120b | ESO 319−G022 | 11:27:56.1 | –41:37:06 | 0.016351 | 5 | 70.9 | 333 | 11.04 | 0 | H | 5 | |
| F11506−3851 | ESO 320−G030 | 11:53:12.0 | –39:07:54 | 0.010781 | 3 | 46.6 | 221 | 11.30 | 0 | H | 6 | |
| F12043−3140b | ESO 440−IG 058 | 12:06:53.0 | –31:57:05 | 0.023203 | 12 | 101.1 | 468 | 11.37 | 1 | L/HII(N)/HII(S) | 5, 6 | |
| F12115−4656 | ESO 267−G030 | 12:14:12.6 | –47:13:37 | 0.018489 | 5 | 80.3 | 375 | 11.11 | 0 | H | 5 | |
| 12116−5615 | 12:14:21.4 | –56:32:32 | 0.027102 | 8 | 118.5 | 545 | 11.61 | 2/0 | ... | ... | ||
| F12596−1529a | MCG−02−33−098 | 13:02:20.5 | –15:46:05 | 0.015921 | 13 | 69.0 | 324 | 11.07 | 1 | H(both) | 1, 5 | |
| F13001−2339 | ESO 507−G070 | 13:02:51.3 | –23:55:09 | 0.021702 | 14 | 94.5 | 439 | 11.48 | 2/0/1 | L | 5 | |
| F13229−2934 | NGC 5135 | 13:25:43.0 | –29:49:54 | 0.013693 | 2 | 59.3 | 280 | 11.29 | 0 | S | 4, 5 | |
| F14544−4255 | IC 4518 | 14:57:43.1 | –43:08:01 | 0.015728 | 15 | 68.2 | 320 | 11.11 | 1 | S(W) | 5 | |
| F17138−1017 | 17:16:36.3 | –10:20:40 | 0.017335 | 16 | 75.2 | 352 | 11.41 | 2/0 | H | 5 | ||
| F18093−5744 | IC 4687/4686 | 18:13:38.6 | –57:43:36 | 0.017345 | 17 | 75.3 | 353 | 11.57 | 1 | H(both) | 4, 5 | |
| F21130−4446c | 21:16:19.0 | –44:33:32 | 0.092554 | 5 | 423.9 | 1722 | 12.09 | 2 | H | 2 | ||
| F21453−3511 | NGC 7130 | 21:48:19.6 | –34:57:05 | 0.016151 | 10 | 70.0 | 329 | 11.41 | 2 | L/S | 1, 5 | |
| F22132−3705 | IC 5179 | 22:16:10.0 | –36:50:36 | 0.011415 | 18 | 49.3 | 234 | 11.22 | 0 | H | 1 | |
| F22491−1808c | 22:51:49.0 | –17:52:28 | 0.077760 | 5 | 352.5 | 1471 | 12.17 | 1 | H | 3 | ||
| F23128−5919c | AM 2312-591 | 23:15:46.6 | –59:03:14 | 0.044601 | 19 | 197.5 | 878 | 12.06 | 1 | H/L/S | 2, 4 | |
Notes. Column (1): object designation in the IRAS Faint source catalogue (FSC). For the four sources that are not in the FSC, the identification in the IRAS Point source catalogue (PSC) is given, which has no prefix “F”. Column (2): other name. Columns (3) and (4): right ascension (hours, minutes and seconds) and declination (degrees, arcminutes and arcseconds) from the IRAS FSC. The exceptions are IRAS 08355-4944, IRAS F08424-3130, IRAS 09022-3615 and IRAS 12116-5615, for which the positions are taken from the IRAS PSC. Column (5): redshifts of the IRAS sources from the NASA Extragalactic Database (NED). The references for the redshift values are given in Col. (6). 1: da Costa et al. (1991); 2: The HI Parkes All Sky Survey Catalogue (HIPAS); 3: de Vaucouleurs et al. (1991); 4: Huchra et al. (1983); 5: Strauss et al. (1992); 6: Lauberts et al. (1979); 7: Chamaraux et al. (1999); 8: Sanders et al. (1995); 9: West et al. (1981); 10: de Vaucouleurs et al. (1976); 11: Jones et al. (2009); 12: Kaldare et al. (2003); 13: Huchra et al. (1992); 14: Pimbblet et al. (2006); 15: Visvanathan & Yamada (1996); 16: Shier & Fischer (1998); 17: Martin et al. (1978); 18: Mathewson et al. (1992); 19: Hwang et al. (2007); Column (7): luminosity distances assuming a ΛCDM cosmology with H0 = 70 km s-1 Mpc-1, ΩM = 0.7, ΩM = 0.3 and using the Edward L. Wright Cosmology calculator, which is based on the prescription given by Wright (2006). Column (8): scales. Column (9): infrared luminosity (LIR) = L(8–1000 μm), in units of solar bolometric luminosity, calculated using the fluxes in the four IRAS bands as given in Sanders et al. (2003) when available. Otherwise, the standard prescription in Sanders & Mirabel (1996) with the values in the IRAS Point and Faint source catalogues (Moshir & et al. 1990) was used. Column (10): morphology class. For those objects for which the morphological classification is controversial, the various possible classes are shown in the table (see text for details). Column (11): nuclear optical spectroscopic classification. H: HII galaxy, L: LINER, S: Seyfert 2 and Column (12): references for the spectroscopic data. 1: Veilleux et al. (1995); 2: Duc et al. (1997); 3: Veilleux et al. (1999); 4: Kewley et al. (2001); 5: Corbett et al. (2003). 6: van den Broek et al. (1991); 7: Lípari et al. (2000).
The morphological classification of these objects has been modified with respect to that of Paper I.
In Paper I these four objects were named using the designation in the IRAS Point source catalogue. For the work presented here we decided to use the designation in the IRAS Faint source catalogue. This includes the prefix “F” and a slightly different sequence of numbers.
These objects, although not presented in Table 1 in Paper I, were observed and eventually included in our VIMOS sample.
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