Table 1.
Properties of our targets, from Webb et al. (2015a).
| Galaxy ID | RA | Dec | zspec | LIR | M⋆ | SFR | sSFR | sSFRMS |
|---|---|---|---|---|---|---|---|---|
| (hh:mm:ss.s) | (dd:mm:ss.s) | (1011 L⊙) | (1011 M⊙) | (M⊙ yr−1) | (Gyr−1) | (Gyr−1) | ||
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) |
| 3C 244.1 | 10:33:34.0 | +58:14:35.5 | 0.430 | 16.1 ± 1.2 | 1.0 | 281 ± 218 |
 |
0.12 |
| SDSS J161112.65+550823.5 | 16:11:12.7 | +55:08:23.6 | 0.907 | 43.7 ± 15.8 | 1.8 | 766 ± 275 |
 |
0.30 |
Notes. The table lists: (1) Galaxy name; (2–3) J2000 equatorial coordinates; (4) spectroscopic redshift; (5) Total infrared luminosity inferred from 24 μm observer frame Spitzer MIPS fluxes and using the Chary & Elbaz (2001) model; (6) Stellar mass estimated using 3.6 μm observer frame Spitzer IRAC fluxes, Bruzual & Charlot (2003) stellar population modeling, and typical rest-frame K-band mass-to-light ratio of red galaxies (Bell et al. 2003); (7) SFR estimated from LIR using the Kennicutt (1998) relation; (8) Specific SFR determined as sSFR = SFR/M⋆; (9) sSFR for main sequence field galaxies with redshift and stellar mass of our targets estimated using the relation found by Speagle et al. (2014).
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