Paper
24 September 2012 Development and performance of the MUSE calibration unit
Andreas Kelz, Svend-Marian Bauer, Thomas Hahn, Thomas Jahn, Johan Kosmalski, Florence Laurent, Uwe Laux, Marie Larrieu, Magali Loupias, Jean-Christophe Olaya, Emil Popow, Martin M. Roth, Mudit Srivastava, Ole Streicher, Peter Weilbacher, Roland M. Bacon
Author Affiliations +
Abstract
The Multi-Unit Spectroscopic Explorer (MUSE), an integral-field spectrograph for the ESO Very Large Telescope, has been built and integrated by a consortium of 7 European institutes. MUSE can simultaneously record spectra across a field of view of 1 square arcminute in the wavelength range from 465nm to 930nm. The calibration unit (CU) for MUSE was developed to provide accurate flat fielding, spectral, geometrical, image quality and efficiency calibration for both the wide-field and AO-assisted narrow-field modes. This paper describes the performance of the CU and electronics, from the subsystem validation to the integration, alignment and use in the MUSE instrument.
© (2012) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Andreas Kelz, Svend-Marian Bauer, Thomas Hahn, Thomas Jahn, Johan Kosmalski, Florence Laurent, Uwe Laux, Marie Larrieu, Magali Loupias, Jean-Christophe Olaya, Emil Popow, Martin M. Roth, Mudit Srivastava, Ole Streicher, Peter Weilbacher, and Roland M. Bacon "Development and performance of the MUSE calibration unit", Proc. SPIE 8446, Ground-based and Airborne Instrumentation for Astronomy IV, 84465T (24 September 2012); https://doi.org/10.1117/12.926003
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Cited by 5 scholarly publications.
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KEYWORDS
Copper

Calibration

Photomasks

Lamps

Spectrographs

Sensors

Electronics

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