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The Virmos Project

Published online by Cambridge University Press:  14 August 2015

D. MacCagni ,
O. Le Fèvre ,
G. Vettolani ,
D. Mancini ,
J.P. Picat ,
J.G. Cuby ,
Y. Mellier  and
A. Mazure
D. MacCagni
Affiliation:
IFCTR/CNR, Milano, Italy dario@ifctr.mi.cnr.it
O. Le Fèvre
Affiliation:
LAS, Marseille, France lefevre@cosobs.obspm.fr
G. Vettolani
Affiliation:
IRA/CNR, Bologna, Italy vettolani@astbo1.bo.cnr.it
D. Mancini
Affiliation:
OAC, Napoli, Italy mancini@astrna.na.astro.it
J.P. Picat
Affiliation:
Observatoire Midi-Pyrénées, Toulouse, France picat@srvdec.obs-mip.fr
J.G. Cuby
Affiliation:
ESO, Garching, Germany jcuby@eso.org
Y. Mellier
Affiliation:
IAP, Paris, France mellier@iap.fr
A. Mazure
Affiliation:
LAS, Marseille, France mazure@astrsp-mrs.fr

Extract

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Large and deep spectroscopic samples of galaxies are essential to study galaxies and large scale structure evolution out to look-back times ~ 10% the current age of the vmiverse. Keeping this scientific and observational goal in mind, we designed and are presently building two wide-field imaging spectrographs to be installed at the Nasmyth foci of the ESO-VLT Unit Telescopes 3 and 4.

Type
II. Joint Discussions
Information
Highlights of Astronomy , Volume 11 , Issue 1: Highlights of Astronomy. As presented at the XXIIIrd General Assembly of the IAU (Part A), 1997 , 1998 , pp. 492
Copyright
Copyright © Kluwer 1998