Table 1
Characteristics of the QSO sample.
Name | Alt. name | α (J2000) | δ (J2000) | za | mBb | MBc | f1.4 GHzd | f5 GHze | Rf | Class.g |
|
||||||||||
PG 0026 + 129 | 00![]() ![]() ![]() |
13°16′05![]() |
0.142 | 14.95 | −24.24 | 7.1 | 5.1 | 1.08 | RI | |
PG 0050 + 124 | I Zw 1 | 00![]() ![]() ![]() |
12°41′35![]() |
0.061 | 14.39 | −22.86 | 8.3 | 2.6 | 0.33 | RQ |
PG 0052 + 251 | 00![]() ![]() ![]() |
25°25′39![]() |
0.155 | 15.42 | −23.97 | 7.1 | 0.7 | 0.24 | RQ | |
SDSS J0057 + 1446 | 00![]() ![]() ![]() |
14°46′10![]() |
0.172 | 15.58 | −24.05 | 2.4 | 0.48 | RQ | ||
HE 0132 − 0441 | RBS 219 | 01![]() ![]() ![]() |
−04°26′36![]() |
0.154 | 16.25 | −23.12 | 7.4 | 2.9 | 2.03 | RI |
SDSS J0155 − 0857 | 01![]() ![]() ![]() |
−08°57′04![]() |
0.165 | 16.83 | −22.71 | <0.9 | <0.58 | RQ | ||
HE 0157 − 0406 | 01![]() ![]() ![]() |
−03°52′00![]() |
0.218 | 17.09 | −23.11 | <0.9 | <0.75 | RQ | ||
PG 0157 + 001 | Mrk 1014 | 01![]() ![]() ![]() |
00°23′41![]() |
0.164 | 15.20 | −24.32 | 26.2 | 8.0 | 2.12 | RI |
SDSS J0836 + 4426 | 08![]() ![]() ![]() |
44°26′02![]() |
0.254 | 15.54 | −25.03 | 10.0 | 1.93 | RI | ||
SDSS J0948 + 4335 | 09![]() ![]() ![]() |
43°35′19![]() |
0.226 | 16.81 | −23.48 | <0.9 | <0.56 | RQ | ||
SDSS J1131 + 2632 | 11![]() ![]() ![]() |
26°32′07![]() |
0.244 | 17.41 | −23.06 | 2.7 | 2.90 | RI | ||
HE 1217 + 0220 | PKS 1217+023 | 12![]() ![]() ![]() |
02°03′41![]() |
0.239 | 17.23 | −23.20 | 652.0 | 440.0 | 757.18 | RL |
HE 1226 + 0219 | 3C 273 | 12![]() ![]() ![]() |
02°03′07![]() |
0.158 | 11.42 | −28.01 | 55 296.0 | 37 000.0 | 302.22 | RL |
SDSS J1230 + 6621 | 12![]() ![]() ![]() |
66°21′54![]() |
0.184 | 16.75 | −23.05 | <2.5 | <1.46 | RQ? | ||
HE 1228 + 0131 | 12![]() ![]() ![]() |
01°15′21![]() |
0.117 | 14.82 | −23.92 | 1.4 | 0.2 | 0.04 | RQ | |
SDSS J1230 + 1100 | 12![]() ![]() ![]() |
11°00′11![]() |
0.236 | 16.61 | −23.78 | < 1.0 | < 0.52 | RQ | ||
PG 1427 + 480 | 14![]() ![]() ![]() |
47°47′27![]() |
0.221 | 16.33 | −23.90 | < 0.9 | 0.0 | 0.02 | RQ | |
SDSS J1444 + 0633 | 14![]() ![]() ![]() |
06°33′06![]() |
0.208 | 17.10 | −22.99 | < 1.0 | < 0.81 | RQ | ||
HE 1453 − 0303 | 14![]() ![]() ![]() |
−03°15′27![]() |
0.206 | 15.68 | −24.39 | 2.7 | 0.58 | RQ | ||
PG 1545 + 210 | PKS 1545+210 | 15![]() ![]() ![]() |
20°52′17![]() |
0.266 | 16.05 | −24.63 | 1560.0 | 720.0 | 418.15 | RL |
PG 1612 + 261 | TON 256 | 16![]() ![]() ![]() |
26°04′16![]() |
0.131 | 16.00 | −23.00 | 17.9 | 5.1 | 2.81 | RI |
SDSS J1655 + 2146 | 16![]() ![]() ![]() |
21°46′01![]() |
0.154 | 16.00 | −23.37 | 6.6 | 1.94 | RI | ||
PG 1700 + 518 | 17![]() ![]() ![]() |
51°49′21![]() |
0.292 | 15.43 | −25.48 | 21.6 | 7.2 | 2.36 | RI | |
PG 2130 + 099 | Mrk 1513 | 21![]() ![]() ![]() |
10°08′19![]() |
0.061 | 14.62 | −22.63 | 6.0 | 2.0 | 0.32 | RQ |
HE 2152 − 0936 | PHL 1811 | 21![]() ![]() ![]() |
−09°22′24![]() |
0.192 | 14.26 | −25.63 | 1.2 | 0.07 | RQ | |
HE 2158 − 0107 | 22![]() ![]() ![]() |
−00°53′01![]() |
0.213 | 16.69 | −23.45 | 1.6 | 0.88 | RQ | ||
HE 2158 + 0115 | RBS 1812 | 22![]() ![]() ![]() |
01°29′56![]() |
0.160 | 16.63 | −22.83 | < 0.9 | < 0.48 | RQ | |
PG 2214 + 139 | Mrk 304 | 22![]() ![]() ![]() |
14°14′28![]() |
0.067 | 14.98 | −22.48 | < 2.5 | 0.2 | 0.05 | RQ |
HE 2307 − 0254 | 23![]() ![]() ![]() |
−02°38′13![]() |
0.221 | 16.90 | −23.34 | < 2.5 | < 1.68 | RQ? | ||
HE 2349 − 0125 | PKS 2349 − 014 | 23![]() ![]() ![]() |
−01°09′13![]() |
0.174 | 16.03 | −23.63 | 1623.2 | 622.7 | 355.46 | RL |
HE 2353 − 0420 | 23![]() ![]() ![]() |
−04°04′00![]() |
0.229 | 17.23 | −23.09 | < 2.5 | < 2.27 | RQ? |
Notes.
Absolute magnitudes MB taking into account Galactic foreground extinction and an appropriate k-correction (Wisotzki 2000).
Radio fluxes at 1.4 GHz in mJy as measured by the NVSS all-sky survey or the FIRST survey when available.
Radio fluxes at 5 GHz in mJy taken from Kellermann et al. (1989) and an unpublished catalog (Gopal-Krishna et al., priv. comm.), if available. Values marked with † were estimated from the radio flux at 1.4 GHz assuming a spectral index of α = −0.5.
Ratio R of the 5 GHz radio to optical flux density at 4400 Å. The optical flux density fν(4400 Å) in mJy was estimated from the optical B band magnitude with the relation mB = −2.5log fν(4400 Å) − 48.36 (Schmidt & Green 1983).
Radio classification of the QSO following Kellermann et al. (1989) into radio loud (RL) and radio quiet (RQ) and radio intermediate (RI) QSOs. An unambigous classification for a few object cannot be made due to upper limits in R.
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