Table 2: Properties of the host galaxiesa.
Name z K-corr $m_{\rm H, nuc}$ $m_{\rm H, host}$ $\mu_{\rm e}^{{b}}$ $r_{\rm e}$ $R_{\rm e}$ $M_{\rm H, nuc}^{{c}}$ $M_{\rm H, host}^{{d}}$ $L_{\rm nuc}/L_{\rm host}$ Note $\chi^2_{\rm psf+gal}/\chi^2_{\rm psf}$
    mag mag mag mag  arcsec  kpc mag mag      
(1) (2) (3) (4) (5) (6) (7) (8) (9) (10) (11) (12) (13)
HS 0010+3611 0.530 0.12 15.03 17.26 14.68 $1.3\pm0.6$ $10.5\pm5.0$ -28.0 $-25.9\pm0.3$ 7.8 R 0.93
1E 0112+3256 0.764 0.18 17.94 18.18 15.46 $0.9\pm0.5$ $8.9\pm4.9$ -26.1 $-26.0\pm0.3$ 1.25 R 0.70
PB 6708 0.868 0.22 17.13 >18.50       -27.2 >-26.1 >3.5 U  
KUV 03086-0447 0.755 0.17 15.16 17.14 14.61 $1.0\pm0.5$ $9.7\pm4.9$ -28.8 $-27.0\pm0.3$ 6.2 R 0.63
US 3828 0.515 0.11 15.70 17.28 14.52 $1.2\pm0.5$ $9.8\pm4.1$ -27.3 $-25.8\pm0.3$ 6.9 R 0.85
MS 08287+6614 0.610 0.13 16.45 17.42 13.97 $0.8\pm0.4$ $6.9\pm3.6$ -27.0 $-26.1\pm0.2$ 2.4 R 0.65
TON 392 0.654 0.14 14.41 17.07 14.23 $1.0\pm0.4$ $8.9\pm3.7$ -29.2 $-26.6\pm0.3$ 11.6 R 0.93
US 971 0.703 0.15 16.57 18.27 15.78 $1.1\pm0.6$ $10.1\pm5.7$ -27.2 $-25.7\pm0.2$ 4.8 R 0.94
HE 0955-0009 0.597 0.13 15.18 >17.20       -28.2 >-26.3 >6.4 U  
HE 1100-1109 0.994 0.30 15.23 17.93 17.99 $2.5\pm0.7$ $27.3\pm7.6$ -29.5 $-27.1\pm0.2$ 12.0 R 0.86
CSO 769 0.850 0.22 16.42 17.99 16.19 $1.2\pm0.5$ $13.4\pm5.1$ -27.9 $-26.5\pm0.3$ 4.2 R 0.98
HS 1623+7313 0.621 0.14 15.86 18.18 15.68 $1.2\pm0.5$ $10.5\pm4.5$ -27.6 $-25.4\pm0.2$ 8.5 R 0.86
HS 2138+1313 0.810 0.20 15.57 >18.00       -28.6 >-26.4 >9.4 U  
LBQS 2249-0154 0.832 0.21 16.38 17.43 14.36 $0.7\pm0.3$ $7.1\pm3.1$ -27.9 $-27.0\pm0.5$ 2.6 R 0.67
ZC 2351+010B 0.810 0.20 16.86 18.52 16.59 $1.2\pm0.6$ $12.3\pm6.1$ -27.3 $-25.9\pm0.6$ 4.6 R 0.92
a Columns (1) and (2) give the name and the redshift of the object; (3) the K-correction for first-ranked elliptical galaxies from Neugebauer et al. (1985), interpolated to the redshifts of the RQQs; (4) and (5) the apparent H-band nuclear and host galaxy magnitude; (6) the effective surface brightness $\mu_{\rm e}$; (7) and (8) the bulge scale-length in arcsec and kpc; (9) and (10) the absolute H-band nuclear and host galaxy magnitude; (11) the nucleus/host galaxy luminosity ratio; (12) R = resolved, U = unresolved; and (13) the ratio of the $\chi^2_{\rm psf+gal}$ and $\chi^2_{\rm psf}$. b Corrected for cosmological dimming. c The RQQ nuclei are assumed to have power-law spectra with $\alpha\sim-1$ and therefore to have negligible K-correction. d Corrected for K-correction.

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