Table 1
General properties of the LIRG sub-sample.
| ID1 | ID2 | α | δ | z | D | Scale | log LIR | Class | References | |
| IRAS | Other | (J2000) | (J2000) | (Mpc) | (pc/arcsec) | (L⊙) | ||||
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | (10) | |
|
|
||||||||||
| F11255-4120 | ESO 319-G022 | 11:27:54.1 | −41:36:52 | 0.016351 | 70.9 | 333 | 11.04 | 0 | 1 | |
| F10567-4310 | ESO 264-G057 | 10:59:01.8 | −43:26:26 | 0.017199 | 74.6 | 350 | 11.07 | 0 | 1 | |
| F04315-0840 | NGC 1614 | 04:33:59.8 | −08:34:44 | 0.015983 | 69.1 | 325 | 11.69 | 2 | 1, 2 | |
| F21453-3511 | NGC 7130 | 21:48:19.5 | −34:57:05 | 0.016151 | 70.0 | 329 | 11.41 | 2 | 1, 2 | |
Notes. Column (1): object designation in the IRAS faint source catalogue (FSC). Column (2): other name. Columns (3) and (4): right ascension (hours, minutes, and seconds) and declination (degrees, arcminutes, and arcseconds) from the IRAS FSC. Column (5): redshift of the IRAS sources from the NASA Extragalactic Database (NED). Column (6): luminosity distances assuming a ΛDCM cosmology with H0 = 70 km s-1 Mpc-1, ΩM = 0.3 and ΩΛ = 0.7, using the Edward L. Wright Cosmology calculator. Column (7): scale. Column (8): 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 we use the standard prescription in Sanders & Mirabel (1996) with the values in the IRAS point and faint source catalogues. Column (9): morphology class. For further information, see Table 1 in Rodríguez Zaurín et al. (2010).
References. (1) Veilleux et al. (1995); (2) Corbett et al. (2003).
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.