Table 3: Comparison of average host galaxy properties with other RQQ samplesa.
Sample Filter N $\langle z\rangle$ $M_{\rm B}$ $\langle M_{\rm H, nuc}\rangle$c $\langle M_{\rm H, host}\rangle$c
(1) (2) (3) (4) (5) (6) (7)
RQQ (this work) H 12 $0.720\pm0.142$ $-25.8\pm0.9$ -27.8 $\pm$ 1.1 -26.3 $\pm$ 0.6
RQQ/R+Ub (this work) H 15 0.728 $\pm$ 0.138 $-25.8\pm0.9$ -27.9 $\pm$ 1.0 -26.2 $\pm$ 0.6
RQQ (McLeod & Rieke 1994a) H 22/24 0.103 $\pm$ 0.029   $-25.1\pm0.5$ -24.9 $\pm$ 0.6
RQQ (Taylor et al. 1996) K 19/19 0.157 $\pm$ 0.062 -23.8 $\pm$ 0.6 $-26.1\pm0.9$ -25.7 $\pm$ 0.7
RQQ (Dunlop et al. 2003) R 13/13 0.175 $\pm$ 0.01   -24.3 $\pm$ 0.6 -25.9 $\pm$ 0.2
RQQ (Bahcall et al. 1997) V 14/14 0.183 $\pm$ 0.046 $-24.9\pm0.5$   -25.1 $\pm$ 0.6
RQQ (McLeod & Rieke 1994b) H 18/20 0.196 $\pm$ 0.047   -26.5 $\pm$ 0.9 -25.7 $\pm$ 0.6
RQQ (Percival et al. 2001) K 12/14 0.362 $\pm$ 0.061 $-25.6\pm0.8$ -27.4 $\pm$ 0.9 -25.0 $\pm$ 0.4
RQQ (Floyd et al. 2004) V 10/10 0.390 $\pm$ 0.031   -26.2 $\pm$ 1.5 -26.3 $\pm$ 0.3
RQQ (Hooper et al. 1997) R 10/10 0.433 $\pm$ 0.032   -25.8 $\pm$ 0.8 -25.6 $\pm$ 0.5
RQQ (Kukula et al. 2001) J 4/5 0.931 $\pm$ 0.038   -25.4 $\pm$ 0.9 -26.1 $\pm$ 0.5
RQQ (Falomo et al. 2004) H/K 6/7 1.519 $\pm$ 0.165 $-26.7\pm0.8$ -29.2 $\pm$ 1.2 -26.6 $\pm$ 0.2
RQQ (Peng et al. 2006) H 14/14 1.54 $\pm$ 0.21   $-27.9\pm1.2$ -26.1 $\pm$ 0.8
RQQ (Kotilainen et al. 2006) H/K 6/6 1.56 $\pm$ 0.25 $-25.5\pm0.5$ -27.3 $\pm$ 0.5 -26.6 $\pm$ 0.9
RQQ (Kukula et al. 2001) H 5/5 $1.856\pm0.120$   $-27.3\pm0.5$ $-26.6\pm0.9$
             
L* (Mobasher et al. 1993) K 136 0.077 $\pm$ 0.030     -25.0 $\pm$ 0.2
BCG (Thuan & Puschell 1989) H 84 0.074 $\pm$ 0.026     -26.3 $\pm$ 0.3
BCG (Aragon-Salamanca et al. 1998) K 25 0.449 $\pm$ 0.266     -27.0 $\pm$ 0.3
FSRQ (Kotilainen et al. 1998) H 9/16 0.671 $\pm$ 0.157 $-26.2\pm1.1$ -29.7 $\pm$ 0.8 -26.7 $\pm$ 1.2
SSRQ (Kotilainen & Falomo 2000) H 16/19 0.690 $\pm$ 0.088 $-25.6\pm1.0$ -28.3 $\pm$ 1.3 $-27.0\pm1.2$
a Column (1) gives the sample; (2) the filter; (3) the resolved/total number of objects in the sample; (4) the average redshift of the sample; (5) the absolute B-band magnitude of the quasar, and (6) and (7) the average H-band nuclear and host galaxy absolute magnitude of the sample.
b R = resolved; U = unresolved.
c Transformation of magnitudes to H-band assumes V-H=3.0, R-H=2.5, H-K=0.2, and J-H=0.9 for the hosts and H-K=1 for the nucleus.

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