X-shooter, the new wide band intermediate resolution spectrograph at the ESO Very Large Telescope

J. Vernet(European Southern Observatory), H. Dekker(European Southern Observatory), S. D’Odorico(European Southern Observatory), L. Kaper(University of Amsterdam), P. Kjærgaard, F. Hammer(Janssen (France)), S. Randich(Arcetri Astrophysical Observatory), F. M. Zerbi(Brera Astronomical Observatory), P. Groot(Radboud University Nijmegen), J. Hjorth, Isabelle Guinouard(Galaxies, Etoiles, Physique et Instrumentation), R. Navarro(AstroTec Holding (Netherlands)), T. Adolfse(Radboud University Nijmegen), P. Albers(Radboud University Nijmegen), J.-P. Amans(Galaxies, Etoiles, Physique et Instrumentation), Jesper Andersen, M. I. Andersen, Pierre Binétruy(Laboratoire AstroParticule et Cosmologie), Paul Bristow(European Southern Observatory), R. Castillo(European Southern Observatory), F. Chemla(Galaxies, Etoiles, Physique et Instrumentation), L. Christensen(Technical University of Munich), P. Conconi(Brera Astronomical Observatory), Ralf Conzelmann(European Southern Observatory), JS Dam(Radboud University Nijmegen), Vincenzo De Caprio(Astronomical Observatory of Capodimonte), A. de Ugarte Postigo, B. Délabre(European Southern Observatory), P. Di Marcantonio(Trieste Astronomical Observatory), M. Downing(European Southern Observatory), Eddy Elswijk(Netherlands Institute for Radio Astronomy), Gert Finger(European Southern Observatory), Gerhard W. Fischer(European Southern Observatory), H. Flores(Janssen (France)), P. François(Janssen (France)), P. Goldoni(Laboratoire AstroParticule et Cosmologie), L. Guglielmi(Laboratoire AstroParticule et Cosmologie), R. Haigron(Galaxies, Etoiles, Physique et Instrumentation), Hiddo Hanenburg(AstroTec Holding (Netherlands)), Inge Hendriks(Radboud University Nijmegen), M. Horrobin(University of Cologne), D. Horville(Galaxies, Etoiles, Physique et Instrumentation), Niels Christian Jessen(DTU Space), F. Kerber(European Southern Observatory), L. Kern(European Southern Observatory), M. Kiekebusch(European Southern Observatory), Pawel Kleszcz(Netherlands Institute for Radio Astronomy), Jens Klougart, Jan Kragt(Netherlands Institute for Radio Astronomy), H. H. Larsen, J. L. Lizon(European Southern Observatory), C. Lucuix(European Southern Observatory), V. Mainieri(European Southern Observatory), R. Manuputy(Centrum Wiskunde & Informatica), C. Martayan(European Southern Observatory), E. Mason(Space Telescope Science Institute), Ruben Mazzoleni(Brera Astronomical Observatory), Niels Michaelsen, A. Modigliani(European Southern Observatory), S. Moehler(European Southern Observatory), P. Møller(European Southern Observatory), A. N. Sørensen, P. Nørregaard, Céline Péroux(Centre National de la Recherche Scientifique), F. Patat(European Southern Observatory), Eduardo Peña(European Southern Observatory), J. Pragt(Netherlands Institute for Radio Astronomy), Claudio Reinero(European Southern Observatory), F. Rigal(Netherlands Institute for Radio Astronomy), Marco Riva(Brera Astronomical Observatory), R. Roelfsema(Netherlands Institute for Radio Astronomy), F. Royer(Janssen (France)), G. G. Sacco(Rochester Institute of Technology), P. Santin(Trieste Astronomical Observatory), Ton Schoenmaker(AstroTec Holding (Netherlands)), P. Spanò(Brera Astronomical Observatory), E. Sweers(Radboud University Nijmegen), Rik ter Horst(Netherlands Institute for Radio Astronomy), Matteo Tintori, N. Tromp(Netherlands Institute for Radio Astronomy), Pieter van Dael(Radboud University Nijmegen), Harriet van der Vliet(Radboud University Nijmegen), L. Venema(Netherlands Institute for Radio Astronomy), M. Vidali, J. Vinther(European Southern Observatory), Pascal Vola(Centre National de la Recherche Scientifique), R. Winters(Radboud University Nijmegen), Dennis W. Wistisen, Gerben Wulterkens(Radboud University Nijmegen), A. Zacchei(Trieste Astronomical Observatory)
Astronomy and Astrophysics
September 30, 2011
Cited by 1,185Open Access
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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 ~ 4000−17 000, depending on wavelength and slit width) with fixed échelle spectral format (prism cross-dispersers) in the three arms. It includes a 1.8″ × 4″ 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.


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