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Table 3

Broad-band imaging analysis results – structural parameters and morphological host galaxy classification.

Name Telescope/instrument Ref.a reb b/ac PAd Class.e

PG 0026 + 129 HST NICMOS (F160W) (1) 4.400 3.566 3.563 (3.6) 12 (3.0 kpc) 0.82 85° B
PG 0050 + 124 HST WFPC2 (F814W) 2.826 2.684 2.669 (2.8) 87 (10.2 kpc) 0.73  −58° B+D
PG 0052 + 251 HST WFPC2 (F606W) (2) 2.705 3.368 2.704 (1.0) 35 (9.4 kpc) 0.65  −8° D
SDSS J0057 + 1446 SDSS (i′) 1.002 0.990 0.989 (2.7) 37 (10.8 kpc) 0.52  −50° B?
SDSS (r′) 1.018 0.985 0.984 (6.7) 22 (6.4 kpc) 0.62  −49°
RBS 219 LB Apogee U42 (R) 1.505 1.508 1.505 (1.1) 38 (10.1 kpc) 0.79 28° D(V)
SDSS J0155 − 0857 SDSS (i′) 1.180 1.150 1.148 (5.4) 13 (3.4 kpc) 0.62 32° B?
SDSS (r′) 1.136 1.139 1.132 (1.7) 24 (6.8 kpc) 0.57 31°
PG 0157 + 001 HST WFPC2 (F675W) (3) 6.406 6.471 6.360 (1.5) 49 (13.8 kpc) 0.89 15° D/M
SDSS J0836 + 4426 SDSS (i′) 0.984 0.979 0.980 (6.1) 02 (0.8 kpc) 0.52  −83° ?
SDSS (r′) 0.994 0.984 0.984 (12.0) 02 (0.8 kpc) 0.90 16°
SDSS J0948 + 4335 SDSS (i′) 1.244 1.259 1.243 (1.2) 24 (8.7 kpc) 0.80  −31° D(V)
SDSS (r′) 1.052 1.083 1.051 (0.8) 27 (9.8 kpc) 0.79  −27°
SDSS J1131 + 2632 SDSS (i′) 1.213 1.255 1.212 (0.8) 37 (14.2 kpc) 0.74  −70° M(V)
SDSS (r′) 1.111 1.174 1.105 (0.7) 34 (13.1 kpc) 0.75  −73°
PKS 1217 + 023 HST WFPC2 (F675W) (4) 4.850 4.722 4.719 (3.15) 25 (9.7 kpc) 0.79 85° B
3C 273 HST WFPC2 (F606W) (5) 1.941 1.823 1.814 (2.8) 50 (13.7 kpc) 0.80 78° B
SDSS J1230 + 6621 SDSS (i′) 1.340 1.340 1.339 (1.7) 18 (5.6 kpc) 0.85 15° D?
SDSS (r′) 1.047 1.052 1.047 (1.1) 18 (5.6 kpc) 0.73 24°
HE 1228 + 0131 SDSS (i′) 1.038 1.006 0.992 (9.9) 03 (0.6 kpc) 0.66  −48° ?
SDSS (r′) 1.122 1.110 1.104 (9.0) 08 (1.7 kpc) 0.68  −63°
SDSS J1230 + 1100 SDSS (i′) 0.878 0.867 0.864 (6.1) 02 (0.8 kpc) 0.77  −86° ?
SDSS (r′) 1.055 1.047 1.043 (8.5) 02 (0.8 kpc) 0.82  −30°
SDSS J1444 + 0633 SDSS (i′) 0.982 0.975 0.972 (12.1) 13 (4.4 kpc) 0.68 85° ?
SDSS (r′) 0.981 0.974 0.974 (7.2) 17 (5.4 kpc) 0.70 90°
PG 1427 + 480 SDSS (i′) 1.438 1.408 ... 09 (3.2 kpc) 0.90 34° B?
SDSS (r′) 1.039 1.033 1.032 (6.8) 06 (2.1 kpc) 0.79 20°
PKS 1545 + 210 HST WFPC2 (F606W) (5) 2.667 2.606 2.603 (3.0) 18 (7.4 kpc) 0.85 77° B
PG 1612 + 261 SDSS (i′) 1.057 1.053 1.047 (2.2) 16 (3.7 kpc) 0.37 10° D(V)
SDSS (r′) 1.057 1.068 1.047 (1.7) 17 (3.96 kpc) 0.40 11°
SDSS J1655 + 2146 SDSS (i′) 1.795 1.662 ... 02 (0.5 kpc) 0.94 51° ?
SDSS (r′) 1.188 1.140 ... 06 (1.6 kpc) 0.82 30°
PG 1700 + 518 HST WFPC2 (F547M) (1) 1.800 1.742 ... 14 (6.2 kpc) 0.80 23° M(V)
PG 2130 + 099 HST WFPC2 (F606W) (6) 1.870 1.875 1.833 (1.8) 120 (14 kpc) 0.36 60° B+D
NTT SOFI (H) 1.417 1.372 1.360 (2.4) 73 (8.6 kpc) 0.31 51°
PHL 1811 HST ACS (F625W) (7) 1.591 1.552 ... 17 (5.3 kpc) 0.52 72° D(V)
NTT SOFI (H) 1.156 1.128 1.091 (9.6) 07 (2.2 kpc) 0.48 59°
LB Apogee U42 (R) 1.263 1.248 1.243 (8.5) 17 (5.3 kpc) 0.59 60°
HE 2158 − 0107f SDSS (z) 0.884 0.880 0.880 (6.2) 02 (0.7 kpc) 0.93 43° B?
NTT SOFI (H) ... ... ... ... ... ...
PG 2214 + 139 NTT SOFI (H) 1.014 1.063 0.950 (1.8) 29 (3.7 kpc) 0.97 64° B
SDSS (i′) 1.825 1.380 1.299 (5.4) 42 (5.4 kpc) 0.94 63°
SDSS (r′) 2.326 1.814 1.684 (5.8) 41 (5.3 kpc) 0.94 56°
HE 2307 − 0254 NTT SOFI (H) 0.542 0.542 0.542 (6.2) 02 (0.7 kpc) 0.67 35° B?
PKS 2349 − 014 HST WFPC2 (F606W) (8) 2.649 2.441 2.436 (3.3) 56 (16.5 kpc) 0.81 83° B/M
HE 2353 − 0420 LB Apogee U42 (R) 0.940 0.957 0.939 (0.7) 38 (13.9 kpc) 0.49 15° D(V)

Notes. 

(a)

References to the articles in which a morphological analysis of these data was initally presented.

(b)

Effective radius re of the best-fitting realistic host-galaxy model given in apparent and physical scale.

(c)

Axis ratio of the minor to major axis of the best-fitting model.

(d)

Position angle of the major axis of the best-fitting model oriented such that 0° is North and 90° is East.

(e)

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.

(f)

Unresolved host galaxy.

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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