Hostname: page-component-586b7cd67f-vdxz6 Total loading time: 0 Render date: 2024-11-29T10:27:16.588Z Has data issue: false hasContentIssue false
  • English
  • Français

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

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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