VIRMOS: Visible and InfraRed Multi-Object Spectrographs for the VLT

被引：25

作者：

Le Fevre, O ^{[1
]}

Vettolani, P ^{[1
]}

Maccagni, D ^{[1
]}

Mancini, D ^{[1
]}

Picat, JP ^{[1
]}

Mellier, Y ^{[1
]}

Mazure, A ^{[1
]}

Saisse, M ^{[1
]}

Cuby, JG ^{[1
]}

Delabre, B ^{[1
]}

Garilli, B ^{[1
]}

Hill, L ^{[1
]}

Prieto, E ^{[1
]}

Arnold, L ^{[1
]}

Conconi, P ^{[1
]}

Cascone, E ^{[1
]}

Mattaini, E ^{[1
]}

Voet, C ^{[1
]}

机构：

[1] CNRS, Astron Spatiale Lab, F-13376 Marseille 12, France

来源：

OPTICAL ASTRONOMICAL INSTRUMENTATION, PTS 1 AND 2 | 1998年 / 3355卷

关键词：

D O I：

10.1117/12.316772

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We present the current design of the VIsible Multi-Object Spectrograph (VIMOS) and the Near InfraRed Multi-Object Spectrograph (NIRMOS) for the European Southern Observatory Very Large Telescope. The basic scientific requirement is to conduct very deep redshift surveys of large quantities of objects, in a minimum number of nights. The technical specifications are to allow for a large multiplex gain over a wide field, and a high efficiency of the optical train, over the 0.37 to 1.8 mu m domain. The baseline technical concept is built around 4 channels, covering 4x7x8 arcmin(2) for VIMOS and 4x7x7 arcmin2 for NIRMOS. Each channel is an imaging spectrograph with a large field adaptation lens, a collimator, grisms or filters, and a F/1.8 camera, coupled to a 2048x4096 pixels CCD for VIMOS, and a 2048(2) HgCdTe Rockwell array for NIRMOS. The unique multiplex gain allows to obtain spectra of up to 840 object simultaneously with VIMOS, and up to 170 with NIRMOS (10 arcsec slits). An integral field spectroscopy mode with more than 6400 fibers coupled to micro-lenses will be available for VIMOS, covering a 1x1 arcmin(2) field. The VLT-VIRMOS survey of more than 150000 galaxies is planned down to magnitudes I-AB=24, coupled to an ultra deep probe to I-AB=26.

引用

页码：8 / 19

页数：2