Table 2: Photometry of the objects in the 13 $^{\prime \prime }$$\times $13 $^{\prime \prime }$ deconvolved field. The IDs correspond to sources identified in Figs. 1, 2, 3 and 4. The columns successively provide: (1) the object identification, (2-3) the coordinates relative to A, (4-7) the R, J, H and Ks magnitudes, (8-9) the redshift (spectroscopic redshift for A and B, photometric redshift for other objects) and the corresponding error bars, (10) some comments or references. The second line provides the date of observation, while the fifth line provides the magnitude differences between quasars A and B.
ID $\Delta \alpha$ $\Delta \delta$ R J $H_{\rm F160w}$ Ks z $\Delta z$ Comments
  ( $^{\prime \prime }$) ( $^{\prime \prime }$) Apr. 2001 Jun. 2001 Dec. 1997 Jun. 2001      

A

 0 0 $17.45\pm 0.02$ $16.32\pm0.01$ $15.88\pm0.01$ $14.96\pm0.01$ 2.076 0.02 Hewett et al.
B $-4.455\pm 0.005 $ + $2.489\pm0.005$ $20.85\pm0.02$ $20.00\pm0.01$ $19.27\pm 0.01$ $18.58\pm 0.01$ 2.076 0.02 (1989)
$\Delta$  $m_{\rm AB}$     $3.40\pm 0.02$ $3.68\pm 0.01$ $3.39 \pm 0.01$ $3.62 \pm 0.01$      
1 + $0.3\pm 0.051$ $-4.50\pm 0.10$ $26.08\pm 0.05$ $22.66\pm 0.15$ $22.18\pm 0.05$ $20.08\pm 0.17$ 1.1 1.0-1.3 $\chi^2>1$
2 $-1.50\pm 0.20$ $-3.70\pm 0.20$ $24.43\pm 0.05$ $23.81\pm 0.20$ >22.5 $21.35\pm0.30$ _ _ _
3 $-7.86\pm0.01$ $-1.33\pm0.02$ $24.52\pm0.02$ $21.69\pm0.08$ $20.92\pm0.03$ $20.02\pm0.15$ 0.8 0.6-1.1 _
4 $-5.23\pm0.04$ $+5.23\pm0.08$ $22.71\pm0.04$ $21.34\pm0.06$ $21.52\pm0.05$ $20.16\pm0.20$ 1.3 1.0-1.9 $\chi^2 > $1
5 $-1.22\pm0.14$ $+4.11\pm0.02$ $23.53\pm0.06$ $21.66\pm0.07$ $21.17\pm0.04$ $20.30\pm0.15$ 1.2 0.8-1.9 _
6 $+0.82\pm0.10$ $+0.96\pm0.10$ $24.89\pm0.06$ >24.5 >22.5 >24.5 _ _ _
7 $-0.55\pm0.10$ $+1.43\pm0.10$ $23.18\pm0.02$ >24.5 >22.5 >24.5 _ _ _
VR1 + $1.02\pm0.10$ + $2.01\pm0.10$ >27 >24.5 $19.30\pm0.01$ $20.49\pm0.15$ _ _ _
VR2 + $0.26\pm0.10$ + $2.36\pm0.10$ >27 >24.5 $21.69\pm0.04$ $21.60\pm0.40$ _ _ _
VR3 + $1.60\pm0.10$ $-2.6\pm0.10$ >27 >24.5 $20.99\pm0.03$ >24.5 _ _ _


Source LaTeX | All tables | In the text