Table 1.
Target sample, ordered by increasing source redshift.
| Target | RA | Dec |
 |
zL | log μIRLIR | log μIRSFR | μIR | log(μL3000) ( * ) | log ( * ) |
|---|---|---|---|---|---|---|---|---|---|
| J2000 | [L⊙] | [M⊙ yr−1] | [erg s−1] [M⊙] | ||||||
| J1524+4409 | 15:24:45.63 | 44:09:49.6 | 1.211 | 0.320 | 12.2 |
2.7 |
7.4 (a) | 45.585 ± 0.005 | 9.54 ± 0.20 |
| B1608+656 ( * *) | 16:09:13.96 | 65:32:29.0 | 1.394 | 0.630 | 11.9 |
2.4 |
10.8 (b) | – | – |
| J1330+1810 | 13:30:18.65 | 18:10:32.1 | 1.394 | 0.373 | 12.8 |
3.3 |
24 ± 1 (c) | 45.969 ± 0.006 | 9.19 ± 0.02 |
| J1455+1447 | 14:55:01.91 | 14:47:34.8 | 1.426 | 0.42 | 12.6 |
3.1 |
12.7 ± 2 (d) | 45.944 ± 0.002 | 8.46 ± 0.03 |
| J1633+3134 ( * *) | 16:33:49.00 | 31:34:12.0 | 1.523 | 0.684 | 12.9 |
3.5 |
10 ± 5 | 46.439 ± 0.002 | 9.27 ± 0.03 |
| J0924+0219 | 09:24:55.83 | 02:19:23.6 | 1.525 | 0.393 | 12.5 |
3.0 |
17 ± 1 (e) | 45.970 ± 0.002 | 8.76 ± 0.11 |
| J1650+4251 | 16:50:43.33 | 42:51:49.3 | 1.543 | 0.577 | 12.5 |
3.0 |
10 ± 5 | 46.391 ± 0.001 | 9.60 ± 0.02 |
| B1152+200 ( * *) | 11:55:18.29 | 19:39:42.0 | 1.019 | 0.438 | 12.2 |
2.7 |
10 ± 5 | 46.062 ± 0.001 | 9.73 ± 0.02 |
| B1600+434 ( * *) | 16:01:40.48 | 43:16:47.4 | 1.59 | 0.414 | 12.4 |
2.9 |
10 ± 5 | – | – |
| J0806+2006 | 08:06:23.70 | 20:06:31.8 | 1.542 | 0.573 | 12.4 |
2.9 |
10 ± 5 | 45.981 ± 0.002 | 8.70 ± 0.10 |
Notes. Columns give the following information: target name, celestial coordinates, redshift, lens redshift, IR luminosities, IR-based SFR, intrinsic luminosity at 3000 Å and MgII-based BH mass. The last two are adopted from Stacey et al. (2018) and are not corrected for the lensing magnification. ( * )Taken from Rakshit et al. (2020). B1152+656 and B1600+434 do not have available SDSS spectra. ( * *)Sources are classified as radio–loud, “jetted” QSOs (Stacey et al. 2018).
References. (a)Oguri et al. (2008), (b)Barvainis & Ivison (2002), (c)Stacey et al. (2022), (d)Kayo et al. (2010), (e)Stacey et al. (2021).
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