Share Email Print
cover

Proceedings Paper

Opto-mechanical design of a new cross dispersion unit for the CRIRES+ high resolution spectrograph for the VLT
Author(s): Jean Louis Lizon; Barbara Klein; Ernesto Oliva; Tom Löwinger; Guillem Anglada Escude; Dietrich Baade; Paul Bristow; Reinhold J. Dorn; Roman Follert; Jason Grunhut; Artie Hatzes; Ulrike Heiter; Derek Ives; Yves Jung; Florian Kerber; Matt Lockhart; Thomas Marquart; Livia Origlia; Luca Pasquini; Jerome Paufique; N. Piskunov; Eszter Pozna; Ansgar Reiners; Alain Smette; Jonathan Smoker; Ulf Seemann; Eric Stempels; Elena Valenti
Format Member Price Non-Member Price
PDF $14.40 $18.00
cover GOOD NEWS! Your organization subscribes to the SPIE Digital Library. You may be able to download this paper for free. Check Access

Paper Abstract

CRIRES is one of the few IR (0.92-5.2 μm) high-resolution spectrographs in operation at the VLT since 2006. Despite good performance it suffers a limitation that significantly hampers its ability: a small spectral coverage per exposure. The CRIRES upgrade (CRIRES+) proposes to transform CRIRES into a cross-dispersed spectrograph while maintaining the high resolution (100000) and increasing the wavelength coverage by a factor 10 compared to the current capabilities. A major part of the upgrade is the exchange of the actual cryogenic pre-disperser module by a new cross disperser unit. In addition to a completely new optical design, a number of important changes are required on key components and functions like the slit unit and detectors units. We will outline the design of these new units fitting inside a predefined and restricted space. The mechanical design of the new functions including a description and analysis will be presented. Finally we will present the strategy for the implementation of the changes.

Paper Details

Date Published: 24 July 2014
PDF: 10 pages
Proc. SPIE 9147, Ground-based and Airborne Instrumentation for Astronomy V, 91477S (24 July 2014); doi: 10.1117/12.2054800
Show Author Affiliations
Jean Louis Lizon, European Southern Observatory (Germany)
Barbara Klein, European Southern Observatory (Germany)
Ernesto Oliva, INAF - Osservatorio di Arcetri (Italy)
Tom Löwinger, Thüringer Landessternwarte Tautenburg (Germany)
Guillem Anglada Escude, Georg-August-Univ. Göttingen (Germany)
Dietrich Baade, European Southern Observatory (Germany)
Paul Bristow, European Southern Observatory (Germany)
Reinhold J. Dorn, European Southern Observatory (Germany)
Roman Follert, Thüringer Landessternwarte Tautenburg (Germany)
Jason Grunhut, European Southern Observatory (Germany)
Artie Hatzes, Thüringer Landessternwarte Tautenburg (Germany)
Ulrike Heiter, Uppsala Univ. (Sweden)
Derek Ives, European Southern Observatory (Germany)
Yves Jung, European Southern Observatory (Germany)
Florian Kerber, European Southern Observatory (Germany)
Matt Lockhart, European Southern Observatory (Germany)
Thomas Marquart, Uppsala Univ. (Sweden)
Livia Origlia, INAF - Osservatorio di Bologna (Italy)
Luca Pasquini, European Southern Observatory (Germany)
Jerome Paufique, European Southern Observatory (Germany)
N. Piskunov, Uppsala Univ. (Sweden)
Eszter Pozna, European Southern Observatory (Germany)
Ansgar Reiners, Georg-August-Univ. Göttingen (Germany)
Alain Smette, European Southern Observatory (Germany)
Jonathan Smoker, European Southern Observatory (Germany)
Ulf Seemann, Georg-August-Univ. Göttingen (Germany)
Eric Stempels, INAF - Osservatorio di Arcetri (Italy)
Elena Valenti, European Southern Observatory (Germany)


Published in SPIE Proceedings Vol. 9147:
Ground-based and Airborne Instrumentation for Astronomy V
Suzanne K. Ramsay; Ian S. McLean; Hideki Takami, Editor(s)

© SPIE. Terms of Use
Back to Top