Table 1.
Target properties of the large SUBWAYS campaign.
| Name (1) | z (2) |
 (3) |
log LX (4) | log Lbol (5) | log MBH (6) | log Lbol/LEdd (7) | log F2−10 keV (8) |
|---|---|---|---|---|---|---|---|
| (1020 cm−2) | ( erg s−1) | ( erg s−1) | (M⊙) | (erg cm−2 s−1) | |||
| PG0052+251 | 0.15445 | 3.96 | 44.609 ± 0.003 | 46.00 | 8.41 (a) | −0.51 | −11.204 ± 0.003 |
| PG0953+414 | 0.23410 | 1.09 | 44.595 ± 0.004 | 46.08 | 8.24 (a) | −0.26 | −11.664 ± 0.004 |
| PG1626+554 | 0.13170 | 1.55 ( † ) | 44.076 ± 0.004 | 45.42 | 8.54 (a) | −1.22 | −11.600 ± 0.004 |
| PG1202+281 | 0.16501 | 1.74 | 44.400 ± 0.004 | 45.77 | 8.61 (a) | −0.94 | −11.469 ± 0.004 |
| PG1435−067 | 0.12900 | 4.84 | 43.684 ± 0.007 | 44.98 | 7.77 (b) | −0.89 | −11.962 ± 0.007 |
| SDSSJ144414+0633 | 0.20768 | 2.57 | 44.467 ± 0.004 | 45.84 | 8.10 (c) | −0.36 | −11.634 ± 0.004 |
| 2MASXJ165315+2349 | 0.10300 | 4.15 | 43.790 ± 0.006 | 45.37 | 6.98 (e) | 0.29 | −11.529 ± 0.007 |
| PG1216+069 | 0.33130 | 1.51 | 44.769 ± 0.004 | 46.24 | 9.20 (a) | −1.06 | −11.810 ± 0.005 |
| PG0947+396 (Obs1) | 0.20553 | 1.91 ( † ) | 44.208 ± 0.007 | 45.55 | 8.68 (a) | −1.24 | −11.887 ± 0.008 |
| PG0947+396 (Obs2) | 0.20553 | 1.91 ( † ) | 44.146 ± 0.006 | 45.55 | 8.68 (a) | −1.24 | −11.954 ± 0.007 |
| WISEJ053756−0245 | 0.11000 | 15.0 | 43.688 ± 0.005 | 44.86 | 7.73 (e) | −0.97 | −11.777 ± 0.006 |
| HB891529+050 | 0.21817 | 3.93 | 44.219 ± 0.005 | 45.52 | 8.75 (c) | −1.33 | −11.918 ± 0.005 |
| PG1307+085 | 0.15384 | 2.10 | 44.312 ± 0.003 | 45.70 | 7.90 (a) | −0.30 | −11.512 ± 0.003 |
| PG1425+267 | 0.36361 | 1.57 | 44.823 ± 0.004 | 46.31 | 9.22 (c) | −1.01 | −11.823 ± 0.005 |
| PG1352+183 | 0.15147 | 1.55 | 43.889 ± 0.004 | 45.21 | 8.42 (a) | −1.31 | −11.921 ± 0.005 |
| 2MASXJ105144+3539 (e) | 0.15900 | 2.20 | 43.692 ± 0.008 | 44.88 | 8.40 (c) | −1.62 | −12.068 ± 0.009 |
| 2MASXJ0220−0728 | 0.21343 | 2.42 | 44.213 ± 0.005 | 45.51 | 8.42 (e) | −1.01 | −11.888 ± 0.006 |
| LBQS1338−0038 | 0.23745 | 1.68 | 44.520 ± 0.003 | 45.91 | 7.77 (c) | 0.04 | −11.707 ± 0.004 |
| Archival targets | |||||||
| PG0804+761 (d) | 0.10000 | 7.09 | 44.330 ± 0.002 | 45.71 | 8.31 (d) | −0.33 | −11.087 ± 0.003 |
| PG1416−129 | 0.12900 | 3.34 | 44.170 ± 0.005 | 45.58 | 9.05 (a) | −1.57 | −11.447 ± 0.005 |
| PG1402+261 | 0.16400 | 1.22 | 44.030 ± 0.004 | 45.39 | 7.94 (a) | −0.65 | −11.874 ± 0.004 |
| HB89 1257+286 | 0.09100 | 1.04 | 43.551 ± 0.002 | 45.15 | 7.46 (c) | −0.41 | −11.831 ± 0.002 |
| PG1114+445 | 0.14400 | 1.93 ( † ) | 44.088 ± 0.003 | 45.53 | 8.59 (a) | −1.16 | −11.602 ± 0.003 |
Notes. (1) Target name; (2) Redshift; (3) Galactic absorption measured by HI4PI Collaboration (2016) or Murphy et al. (1996)( † ); (4) 2–10 keV intrinsic luminosity measured in this work by using the clumin convolution model in XSPEC; (5) bolometric luminosity derived from the X-ray luminosity assuming the bolometric correction of Duras et al. (2020); (6) log of black hole mass from the measurements carried out in Bianchi et al. (2009)(a), Xie et al. (2017)(b), Perna et al. (2017)(c), Kaspi et al. (2000b)(d) and this work(e); (7) Eddington ratio; (8) 2–10 keV fluxes from the available spectra measured with cflux in XSPEC. The LX and Lbol measured in this work are consistent with the ones that were used during the SUBWAYS selection process.
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