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Table 1.

Log of the HST UV grating observations of the targets in the SUBWAYS sample.

Object Redshift log Lbol log MBH Prop. HST Grating/ Obs. Date Exp.
Name z (erg s−1) (M) ID Inst. Central λ yyyy-mm-dd (ks)
2MASS J02201457-0728591 0.21343 (1) 46.33 8.42 15890 COS G140L/1105 2020-01-03 4.4
2MASS J10514425+3539306 0.15881 (1) 44.88 8.40
2MASS J14025120+2631175 0.18762 (1) 45.44 8.55 15890 COS G140L/1105 2019-12-03 4.4
2MASS J16531505+2349427 0.10344 (1) 45.37 6.98
HB89 1257+286 0.09117 (1) 44.58 7.46 4952 FOS G130H/1600 1993-07-15 0.8
HB89 1529+050 0.21817 (1) 45.17 8.75 15890 COS G140L/1105 2019-08-30 7.0
LBQS 1338-0038 0.23745 (1) 45.27 7.77 15890 COS G140L/1105 2020-01-28 4.3
PG 0052+251 0.15445 (2) 45.72 8.41 15890 COS G140L/1105 2019-11-20 1.8
14268 COS G130M/1291,1327 2015-10-03 3.0
14268 COS G160M/1589,1623 2015-10-03 3.0
PG 0804+761 0.10000 (3) 45.27 8.31 11686 COS G130M/1291,1300,1309,1318 2010-06-12 6.0
11686 COS G160M/1589,1600,1611,1623 2010-06-12 6.3
PG 0947+396 0.20553 (1) 45.89 8.68 15890 COS G140L/1105 2020-04-25 0.3
15890 COS G130M/1222 2020-04-25 0.7
15890 COS G160M/1600 2020-04-25 0.6
15890 COS G185M/1953 2020-04-26 1.0
PG 0953+414 0.23410 (4) 46.33 8.24 15890 COS G140L/1105 2020-04-04 1.5
12038 COS G130M/1291,1300,1309,1318 2011-10-18 5.3
12038 COS G160M/1589,1600,1611,1623 2011-10-18 5.6
PG 1114+445 0.14373 (1) 45.87 8.59 6484 FOS G130H/1600 1996-11-23 12.8
6484 FOS G190H/2300 1996-11-23 4.4
6781 FOS G130H/1600 1996-05-13 9.3
6781 FOS G190H/2300 1996-05-13 1.6
9871 STIS G140M/1173,1400 2004-05-28 5.3
9871 STIS G230M/1769 2004-05-28 2.9
PG 1202+281 0.16501 (5) 46.30 8.61 15890 COS G140L/1105 2019-12-14 0.9
15890 COS G130M/1327 2019-12-14 2.9
12248 COS G130M/1309,1327 2011-04-14 2.9
12248 COS G160M/1577,1600 2011-04-14 4.8
PG 1216+069 0.33130 (6) 45.84 9.20 15890 COS G140L/1105 2019-12-26 1.8
15890 COS G185M/1953 2019-12-26 2.3
12025 COS G130M/1291,1300,1309,1318 2012-02-04 5.1
12025 COS G160M/1589,1600,1611,1623 2012-02-04 5.6
PG 1307+085 0.15384 (1) 44.86 7.90 15890 COS G140L/1105 2019-11-30 1.8
12569 COS G130M/1309,1327 2012-06-16 2.0
PG 1352+183 0.15147 (1) 46.26 8.42 15890 COS G140L/1105 2020-01-12 1.8
13448 COS G130M/1291 2014-07-31 8.2
13448 COS G160M/1600 2014-07-31 8.7
PG 1402+261 0.16430 (7) 46.34 7.94 6781 FOS G130H/1600 1996-08-25 1.6
6781 FOS G190H/2300 1996-08-25 0.2
PG 1416-129 0.12894 (2) 45.74 9.05 6528 FOS G190H/2300 1996-08-23 1.0
PG 1425+267 0.36361 (1) 46.06 9.22 15890 COS G140L/1105 2020-01-25 3.6
15890 COS G230L/3360 2020-01-25 0.4
12603 COS G130M/1291,1327 2012-06-23 2.2
14729 COS G160M/1600 2017-05-29 5.4
PG 1427+480 0.22063 (1) 45.82 8.09 15890 COS G140L/1105 2019-10-28 0.9
15890 COS G185M/1864 2019-10-28 5.6
PG 1435-067 0.12900 (8) 45.51 7.77 15890 COS G140L/1105 2020-01-19 1.8
12569 COS G130M/1291,1309 2012-02-29 2.1
PG 1626+554 0.13170 (9) 46.02 8.54 15890 COS G140L/1105 2020-07-13 1.8
12029 COS G130M/1291,1300,1309,1318 2011-06-15 3.9
12029 COS G160M/1589,1600,1611,1623 2011-06-15 4.3
SDSS J144414.66+063306.7 0.20768 (1) 45.34 8.10 15890 COS G140L/1105 2019-12-22 1.8
WISE J053756.30-024513.1 0.10983 (1) 44.86 7.73

Notes. The SUBWAYS targets observed with HST overlap with those observed in X-rays (Paper I) with the following exceptions: three of the SUBWAYS targets that are studied in X-rays in Paper I are too heavily reddened and thus are not observed with HST: 2MASS J10514425+3539306, 2MASS J16531505+2349427, and WISE J053756.30-024513.1; two of the targets that are observed with HST are excluded in Paper I due to lack of sufficient X-ray data: 2MASS J14025120+2631175 and PG 1427+480. The new HST data that we obtained in HST Cycle 27 correspond to the proposal ID number 15890 (16 targets) and the remaining targets have only archival HST data (5 targets). References for cosmological redshifts z are: (1) Albareti et al. (2017); (2) Ho & Kim (2009); (3) Schmidt & Green (1983); (4) Marziani et al. (1996); (5) Albareti et al. (2015); (6) Ganguly et al. (2013); (7) Hu et al. (2021); (8) Monroe et al. (2016); (9) Tang et al. (2012). For references of the bolometric luminosities, Lbol, and the black hole masses, MBH, see Paper I and references therein. Targets are ordered alphabetically by their name for ease in looking them up.

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