Open Access

Table C.1.

Sources characterized with a redshift in our VLT/VIMOS survey (extract).

ID Object RA DEC Impact Parameter gSDSS rSDSS iSDSS Mi z reliability
J2000 J2000 (arcsec) (kpc)
(1) (2) (3) (4) (5) (6) (7) (8) (9) (10) (11) (12)
1 J161931.89+254216.6 244.88286 25.70461 136 - 22.4 21.7 21.9 - 0.0000 a
2 J162005.40+253845.5 245.02251 25.64596 438 - 21.3 20.9 20.8 - 0.0000 a
3 J162018.06+254846.8 245.07525 25.81299 600 - 19.9 19.5 19.4 - 0.0000 a
4 J162011.76+254647.7 245.04902 25.77993 468 - 23.3 21.9 21.5 - 0.0000 a
5 J162006.25+254151.4 245.02604 25.69760 360 - 18.5 17.9 17.7 - 0.0000 a
6 J162017.42+253645.8 245.07258 25.61273 639 - 22.3 20.9 20.2 - 0.0000 a
7 J162014.68+253737.7 245.06115 25.62715 578 - 20.5 19.1 18.5 - 0.0000 a
8 J162013.00+253804.6 245.05416 25.63460 544 - 18.7 18.4 18.2 - 0.0000 a
9 J162018.12+254540.8 245.07551 25.76132 525 - 23.5 22.3 21.7 - 0.0000 a
10 J162013.47+253838.8 245.05613 25.64412 530 - 19.4 18.0 17.3 - 0.0000 a
11 J161900.65+253626.6 244.75272 25.60739 683 - 21.1 20.0 19.4 - 0.0000 a
12 J162000.16+254840.5 245.00066 25.81126 412 - 18.8 18.0 17.8 - 0.0000 a
13 J161910.81+253640.6 244.79505 25.61127 571 - 20.7 20.5 20.3 - 0.0000 a
14 J162004.96+254749.2 245.02067 25.79701 422 - 21.6 21.1 21.0 - 0.0000 a
15 J161908.79+253818.3 244.78663 25.63842 528 - 20.4 20.1 19.9 - 0.0000 a

Notes. The full list of 244 sources is available in the VizieR (CDS) database. (): REDMONSTER did not converge to a z on these sources. Redshift were calculated by a visual inspection on these cases. Columns. (5) and (6) shows the impact parameter of each source to the QSO sightline, in arcseconds and kiloparsecs, respectively. Columns (7), (8), and (9) show the SDSS photometry if available. Column (10) shows the rest-frame i-band absolute magnitude (For galaxies at z < 0.5, the k-correction was calculated using the code available in http://kcor.sai.msu.ru). The uncertainties in the redshift measurements in column (11) are of the order of ∼0.0001. The reliability categories in column (11) are described in Sec. 2.6.1.

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