Table 3: Properties of candidate Ly$\alpha $ emission lines. Columns 2-4 list the offsets of the candidate in RA and Dec and in projected kpc at the Ly$\alpha $ emission redshifts (in Col. 5), respectively. Column 6 lists the integrated Ly$\alpha $ flux in units of 10-17  erg cm-2 s-1, and Col. 7 the velocity offset from the DLA redshift. Column 8 lists the integrated signal-to-noise ratio of the Ly$\alpha $ emission line, and Col. 9 gives the line width of the emission lines. Fluxes have not been corrected for Galactic extinction. Column 10 lists the significance class of the detections as described in Sect. 5.5. "Conf.'' implies candidates that were confirmed previously (Djorgovski et al. 1996; Møller et al. 1998).
QSO $\Delta$RA $\Delta$Dec b z $f_{\lambda}$ $\Delta ~ v$ S/N $_{\rm int}$ FWHM significance
  ( $^{\prime \prime }$) ( $^{\prime \prime }$) (kpc)     (km s-1)   (km s-1) class
(1) (2) (3) (4) (5) (6) (7) (8) (9) (10)
Q0151+048A 2.5:0.4 -2.5:1.7 3.3:25.4 1.9363 (150 $\pm $ 70) +225 7 280 $\pm $ 220 conf.
Q0953+4749 -1.2 -0.2 9.0 3.4041 (6.6 $\pm $ 2.9) 0 15 290 $\pm $ 260 2
  -0.5 1.8 11.1 3.9029 (4.9 $\pm $ 2.1) +730 16 570 $\pm $ 230 3
Q1347+112 -2.0 1.5 20.2 2.4835 (3.5 $\pm $ 1.9) +1080 8 190 $\pm $ 370 3
  -4.1 0.4 34.3 2.0568 (4.2 $\pm $ 3.0) +670 7 610 $\pm $ 210 1
Q1425+606 -4.1 0.4 32.3 2.8280 (8.5 $\pm $ 3.1) +80 14 590 $\pm $ 220 3
Q1451+1223 -3.0 3.8 39.2 2.4764 (5.8 $\pm $ 2.6) +640 10 320 $\pm $ 260 3
  -1.0 2.8 22.5 3.1739 (3.1 $\pm $ 2.0) +210 7 <100 3
Q1759+7539 -1.4 3.5 30.0 2.6377 (5.8 $\pm $ 3.0) +1050 10 290 $\pm $ 220 2
  0.1 -1.2 9.4 2.9090 (6.0 $\pm $ 2.9) -80 21 240 $\pm $ 260 1
Q1802+5616 -0.2 -2.0 14.9 3.3820 (3.5 $\pm $ 0.9) -610 10 180 $\pm $ 90 4
  0.2 1.8 12.9 3.7652 (4.6 $\pm $ 1.9) +200 7 <100 2
Q2155+1358 0.7 1.2 10.2 3.3174 (9.4 $\pm $ 3.0) +100 9 780 $\pm $ 210 3
  1.7 1.9 19.4 3.1461 (4.1 $\pm $ 2.4) +290 7 260 $\pm $ 220 3
Q2233+131 0.6 2.3 18.0 3.1543 (9.6 $\pm $ 2.5) +90 9 230 $\pm $ 110 conf.

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