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.
Le Fevre O., Vettolani G., Paltani S., Tresse L., Zamorani G., Le Brun V., et al. (2006). Redshifts from VIMOS VLT Deep Survey (Le Fevre+ 2004). STRASBOURG : Centre de donnee stellaire de Strasbourg.
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.I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.
