Redshifts from VIMOS VLT Deep Survey (Le Fevre+, 2004)

Details Redshifts from VIMOS VLT Deep Survey (Le Fevre+, 2004) Redshifts from VIMOS VLT Deep Survey (Le Fevre+, 2004)

May 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006ycat..34281043l&link_type=abstract

VizieR On-line Data Catalog: J/A+A/428/1043. Originally published in: 2004A&A...428.1043L

Computer Science

Surveys, Redshifts

Scientific paper

Observations with VIMOS have been obtained between October 31 and December 6, 2002. Observing conditions were photometric with an image quality between 0.6 and 1.2-arcsec FWHM. We have moved the telescope, hence the objects along the slits, in a sequence of 5 positions with offsets -1.4, -0.7, 0, +0.7, +1.4-arcsec from the reference pointing position. This is necessary to compute the fringing pattern produced above 8300{AA} by the thinned EEV CCDs used in VIMOS, and remove it during processing.
(1 data file).

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