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Table 2.

Parameters of the C IV emission line in the HST spectra of the SUBWAYS AGN sample.

Object af ap vmean FWHMmean
2MASS J02201457-0728591 1.19 −0.09 +220 6330
2MASS J14025120+2631175 0.83 +0.12 +100 6190
HB89 1257+286 N/A N/A N/A N/A
HB89 1529+050 1.01 −0.00 −530 8320
LBQS 1338-0038 1.37 −0.18 +680 5180
PG 0052+251 0.93 +0.03 −260 6710
PG 0804+761 0.96 +0.02 −310 5790
PG 0947+396 0.99 +0.00 −150 7170
PG 0953+414 0.98 +0.02 −340 6500
PG 1114+445 0.98 +0.01 −40 6660
PG 1202+281 1.06 −0.05 −300 7340
PG 1216+069 0.91 −0.05 +230 4970
PG 1307+085 0.86 +0.12 −670 5940
PG 1352+183 0.77 +0.14 −1040 5540
PG 1402+261 0.83 +0.11 −1050 6450
PG 1416-129 0.88 +0.04 −460 7000
PG 1425+267 N/A N/A N/A N/A
PG 1427+480 1.15 −0.10 +60 5900
PG 1435-067 0.95 +0.04 −320 6580
PG 1626+554 1.08 −0.08 +160 7060
SDSS J144414.66+063306.7 1.15 −0.10 +160 6890

Notes. The af is the “flux asymmetry” parameter and ap the “profile asymmetry” parameter, as defined in Sect. 4.2. The vmean and FWHMmean are the flux-weighted mean velocity shift and width of the line, respectively, in km s−1. The parameters in this table are calculated using the best-fit model parameters given in Table A.1. For the two objects labeled with “N/A” the HST spectra do not cover the C IV emission line.

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