Table 3
Broad-band imaging analysis results – structural parameters and morphological host galaxy classification.
Name | Telescope/instrument | Ref.a |
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reb | b/ac | PAd | Class.e |
|
|||||||||
PG 0026 + 129 | HST NICMOS (F160W) | (1) | 4.400 | 3.566 | 3.563 (3.6) | 1![]() |
0.82 | 85° | B |
PG 0050 + 124 | HST WFPC2 (F814W) | 2.826 | 2.684 | 2.669 (2.8) | 8![]() |
0.73 | −58° | B+D | |
PG 0052 + 251 | HST WFPC2 (F606W) | (2) | 2.705 | 3.368 | 2.704 (1.0) | 3![]() |
0.65 | −8° | D |
SDSS J0057 + 1446 | SDSS (i′) | 1.002 | 0.990 | 0.989 (2.7) | 3![]() |
0.52 | −50° | B? | |
SDSS (r′) | 1.018 | 0.985 | 0.984 (6.7) | 2![]() |
0.62 | −49° | |||
RBS 219 | LB Apogee U42 (R) | 1.505 | 1.508 | 1.505 (1.1) | 3![]() |
0.79 | 28° | D(V) | |
SDSS J0155 − 0857 | SDSS (i′) | 1.180 | 1.150 | 1.148 (5.4) | 1![]() |
0.62 | 32° | B? | |
SDSS (r′) | 1.136 | 1.139 | 1.132 (1.7) | 2![]() |
0.57 | 31° | |||
PG 0157 + 001 | HST WFPC2 (F675W) | (3) | 6.406 | 6.471 | 6.360 (1.5) | 4![]() |
0.89 | 15° | D/M |
SDSS J0836 + 4426 | SDSS (i′) | 0.984 | 0.979 | 0.980 (6.1) | 0![]() |
0.52 | −83° | ? | |
SDSS (r′) | 0.994 | 0.984 | 0.984 (12.0) | 0![]() |
0.90 | 16° | |||
SDSS J0948 + 4335 | SDSS (i′) | 1.244 | 1.259 | 1.243 (1.2) | 2![]() |
0.80 | −31° | D(V) | |
SDSS (r′) | 1.052 | 1.083 | 1.051 (0.8) | 2![]() |
0.79 | −27° | |||
SDSS J1131 + 2632 | SDSS (i′) | 1.213 | 1.255 | 1.212 (0.8) | 3![]() |
0.74 | −70° | M(V) | |
SDSS (r′) | 1.111 | 1.174 | 1.105 (0.7) | 3![]() |
0.75 | −73° | |||
PKS 1217 + 023 | HST WFPC2 (F675W) | (4) | 4.850 | 4.722 | 4.719 (3.15) | 2![]() |
0.79 | 85° | B |
3C 273 | HST WFPC2 (F606W) | (5) | 1.941 | 1.823 | 1.814 (2.8) | 5![]() |
0.80 | 78° | B |
SDSS J1230 + 6621 | SDSS (i′) | 1.340 | 1.340 | 1.339 (1.7) | 1![]() |
0.85 | 15° | D? | |
SDSS (r′) | 1.047 | 1.052 | 1.047 (1.1) | 1![]() |
0.73 | 24° | |||
HE 1228 + 0131 | SDSS (i′) | 1.038 | 1.006 | 0.992 (9.9) | 0![]() |
0.66 | −48° | ? | |
SDSS (r′) | 1.122 | 1.110 | 1.104 (9.0) | 0![]() |
0.68 | −63° | |||
SDSS J1230 + 1100 | SDSS (i′) | 0.878 | 0.867 | 0.864 (6.1) | 0![]() |
0.77 | −86° | ? | |
SDSS (r′) | 1.055 | 1.047 | 1.043 (8.5) | 0![]() |
0.82 | −30° | |||
SDSS J1444 + 0633 | SDSS (i′) | 0.982 | 0.975 | 0.972 (12.1) | 1![]() |
0.68 | 85° | ? | |
SDSS (r′) | 0.981 | 0.974 | 0.974 (7.2) | 1![]() |
0.70 | 90° | |||
PG 1427 + 480 | SDSS (i′) | 1.438 | 1.408 | ... | 0![]() |
0.90 | 34° | B? | |
SDSS (r′) | 1.039 | 1.033 | 1.032 (6.8) | 0![]() |
0.79 | 20° | |||
PKS 1545 + 210 | HST WFPC2 (F606W) | (5) | 2.667 | 2.606 | 2.603 (3.0) | 1![]() |
0.85 | 77° | B |
PG 1612 + 261 | SDSS (i′) | 1.057 | 1.053 | 1.047 (2.2) | 1![]() |
0.37 | 10° | D(V) | |
SDSS (r′) | 1.057 | 1.068 | 1.047 (1.7) | 1![]() |
0.40 | 11° | |||
SDSS J1655 + 2146 | SDSS (i′) | 1.795 | 1.662 | ... | 0![]() |
0.94 | 51° | ? | |
SDSS (r′) | 1.188 | 1.140 | ... | 0![]() |
0.82 | 30° | |||
PG 1700 + 518 | HST WFPC2 (F547M) | (1) | 1.800 | 1.742 | ... | 1![]() |
0.80 | 23° | M(V) |
PG 2130 + 099 | HST WFPC2 (F606W) | (6) | 1.870 | 1.875 | 1.833 (1.8) | 12![]() |
0.36 | 60° | B+D |
NTT SOFI (H) | 1.417 | 1.372 | 1.360 (2.4) | 7![]() |
0.31 | 51° | |||
PHL 1811 | HST ACS (F625W) | (7) | 1.591 | 1.552 | ... | 1![]() |
0.52 | 72° | D(V) |
NTT SOFI (H) | 1.156 | 1.128 | 1.091 (9.6) | 0![]() |
0.48 | 59° | |||
LB Apogee U42 (R) | 1.263 | 1.248 | 1.243 (8.5) | 1![]() |
0.59 | 60° | |||
HE 2158 − 0107f | SDSS (z) | 0.884 | 0.880 | 0.880 (6.2) | 0![]() |
0.93 | 43° | B? | |
NTT SOFI (H) | ... | ... | ... | ... | ... | ... | |||
PG 2214 + 139 | NTT SOFI (H) | 1.014 | 1.063 | 0.950 (1.8) | 2![]() |
0.97 | 64° | B | |
SDSS (i′) | 1.825 | 1.380 | 1.299 (5.4) | 4![]() |
0.94 | 63° | |||
SDSS (r′) | 2.326 | 1.814 | 1.684 (5.8) | 4![]() |
0.94 | 56° | |||
HE 2307 − 0254 | NTT SOFI (H) | 0.542 | 0.542 | 0.542 (6.2) | 0![]() |
0.67 | 35° | B? | |
PKS 2349 − 014 | HST WFPC2 (F606W) | (8) | 2.649 | 2.441 | 2.436 (3.3) | 5![]() |
0.81 | 83° | B/M |
HE 2353 − 0420 | LB Apogee U42 (R) | 0.940 | 0.957 | 0.939 (0.7) | 3![]() |
0.49 | 15° | D(V) |
Notes.
References to the articles in which a morphological analysis of these data was initally presented.
Effective radius re of the best-fitting realistic host-galaxy model given in apparent and physical scale.
Position angle of the major axis of the best-fitting model oriented such that 0° is North and 90° is East.
Our host galaxy morphological classification into: B (bulge-dominated), D (disc-dominated), B+D (bulge+disc component), M (Merger or strongly interacting), B?/D? (only tentative classifications), ? (unconstrained). We append (V) to the classification, if it is due to a visual inspection of the image.
References. (1) Veilleux et al. (2009); (2) Bahcall et al. (1996); (3) McLure et al. (1999); (4) Dunlop et al. (2003); (5) Bahcall et al. (1997); (6) Kim et al. (2008); (7) Jenkins et al. (2005); (8) Bahcall et al. (1995).
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