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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