Pubblicazione eletrtronica che da accesso ai dati già esposti in Le Fevre et al , 2004 Abstract 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.
Redshifts from VIMOS VLT Deep Survey (Le Fevre+ 2004)
MARANO, BRUNO;BONGIORNO, ANGELA;GREGORINI, LORETTA;
2006
Abstract
Pubblicazione eletrtronica che da accesso ai dati già esposti in Le Fevre et al , 2004 Abstract 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.File in questo prodotto:
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