| | |
| | |
Stat |
Members: 3645 Articles: 2'504'585 Articles rated: 2609
24 April 2024 |
|
| | | |
|
Article overview
| |
|
X-shooter, the new wide band intermediate resolution spectrograph at the ESO Very Large Telescope | Joel Vernet
; H. Dekker
; S. D'Odorico
; L. Kaper
; P. Kjaergaard
; F. Hammer
; S. Randich
; F. Zerbi
; P. M. Groot
; J. Hjorth
; I. Guinouard
; R. Navarro
; T. Adolfse
; P. W. Albers
; J.-P. Amans
; J. J. Andersen
; M. I. Andersen
; P. Binetruy
; P. Bristow
; R. Castillo
; F. Chemla
; L. Christensen
; P. Conconi
; R. Conzelmann
; J. Dam
; V. De Caprio
; A. De Ugarte Postigo
; B. Delabre
; P. Di Marcantonio
; M. Downing
; E. Elswijk
; G. Finger
; G. Fischer
; H. Flores
; P. Francois
; P. Goldoni
; L. Guglielmi
; R. Haigron
; H. Hanenburg
; I. Hendriks
; M. Horrobin
; D. Horville
; N. C. Jessen
; F. Kerber
; L. Kern
; M. Kiekebusch
; P. Kleszcz
; J. Klougart
; J. Kragt
; H. H. Larsen
; J.-L. Lizon
; C. Lucuix
; V. Mainieri
; R. Manuputy
; C. Martayan
; E. Mason
; R. Mazzoleni
; N. Michaelsen
; A. Modigliani
; S. Moehler
; P. Møller
; A. Norup Sørensen
; P. Nørregaard
; C. Peroux
; F. Patat
; E. Pena
; J. Pragt
; C. Reinero
; F. Riga
; M. Riva
; R. Roelfsema
; F. Royer
; G. Sacco
; P. Santin
; T. Schoenmaker
; P. Spano
; E. Sweers
; R. Ter Horst
; M. Tintori
; N. Tromp
; P. van Dael
; H. van der Vliet
; L. Venema
; M. Vidali
; J. Vinther
; P. Vola
; R. Winters
; D. Wistisen
; G. Wulterkens
; A. Zacchei
; | Date: |
10 Oct 2011 | Abstract: | X-shooter is the first 2nd generation instrument of the ESO Very Large
Telescope(VLT). It is a very efficient, single-target, intermediate-resolution
spectrograph that was installed at the Cassegrain focus of UT2 in 2009. The
instrument covers, in a single exposure, the spectral range from 300 to 2500
nm. It is designed to maximize the sensitivity in this spectral range through
dichroic splitting in three arms with optimized optics, coatings, dispersive
elements and detectors. It operates at intermediate spectral resolution
(R~4,000 - 17,000, depending on wavelength and slit width) with fixed echelle
spectral format (prism cross-dispersers) in the three arms. It includes a
1.8"x4" Integral Field Unit as an alternative to the 11" long slits. A
dedicated data reduction package delivers fully calibrated two-dimensional and
extracted spectra over the full wavelength range. We describe the main
characteristics of the instrument and present its performance as measured
during commissioning, science verification and the first months of science
operations. | Source: | arXiv, 1110.1944 | Services: | Forum | Review | PDF | Favorites |
|
|
No review found.
Did you like this article?
Note: answers to reviews or questions about the article must be posted in the forum section.
Authors are not allowed to review their own article. They can use the forum section.
browser Mozilla/5.0 AppleWebKit/537.36 (KHTML, like Gecko; compatible; ClaudeBot/1.0; +claudebot@anthropic.com)
|
| |
|
|
|
| News, job offers and information for researchers and scientists:
| |