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Home All issues Volume 504 / No 3 (September IV 2009) A&A, 504 3 (2009) 789-805 Full HTML
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Table 1:

Table of observations.
VVDS ID $\alpha $ $\delta$ z $I_{\rm AB}$ Field $t_{\rm exp}$ Seeing Run ID
  J2000 J2000   mag   hours $^{\prime\prime}$  
(1) (2) (3) (4) (5) (6) (7) (8) (9)
020116027 02:25:51.133 -04:45:04.48 1.5259 22.875 VVDS-02h 1.67 0.65 075.A-0318(A)
020182331 02:26:44.260 -04:35:51.89 1.2286 22.729 VVDS-02h 3 0.72 078.A-0177(A)
020147106 02:26:45.386 -04:40:47.39 1.5174 22.502 VVDS-02h 2 0.74 075.A-0318(A)
020261328 02:27:11.049 -04:25:31.60 1.5291 23.897 VVDS-02h 1 0.61 075.A-0318(A)
220596913 22:14:29.184 +00:22:18.89 1.2667 21.841 VVDS-22h 1.75 0.47 075.A-0318(A)
220584167 22:15:23.038 +00:18:47.01 1.4637 22.036 VVDS-22h 1.75 0.74 075.A-0318(A)
220544103 22:15:25.708 +00:06:39.53 1.3970 22.469 VVDS-22h 1 0.69 075.A-0318(A)
220015726 22:15:42.455 +00:29:03.59 1.3091 22.473 VVDS-22h 2 0.58 075.A-0318(A)
220014252 22:17:45.690 +00:28:39.47 1.3097 22.101 VVDS-22h 2 0.70 075.A-0318(A)
(1) Source VVDS identification number, (2) and (3) coordinates, (4) VVDS spectroscopic redshift, (5) AB magnitude in I-band, (6) VVDS-22h wide field ( $17.5 \leq I_{\rm AB} \leq 22.5$) and VVDS-02h deep field ( $17.5 \leq I_{\rm AB} \leq 24.0$), (7) exposure time, (8) median seeing of SINFONI observations measured on PSF stars, (9) ESO program.

Source LaTeX | All tables | In the text

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