Paper
24 September 2012 Upgrading CRIRES-VLT to cross-dispersed mode
E. Oliva, A. Hatzes, N. Piskunov, A. Reiners, H. U. Käufl, D. Ferruzzi, A. Tozzi, L. Origlia
Author Affiliations +
Abstract
The cryogenic high resolution IR echelle spectrograph CRIRES is the ESO infrared (0.95−5.4 μm) high resolution spectrograph operating at the Nasmyth A focus of VLT-UT1. The instrument provides long-slit (31") spectroscopy with resolving power up to R=100,000 over a quite narrow wavelengths range, about 1/70 of the central wavelength. Observations of compact objects (e.g. stellar photospheres) could be made much more efficient by implementing a cross-dispersed mode, which increases the simultaneous spectral coverage by an order of magnitude or more. This paper presents the design of a relatively simple system to add cross-dispersed modes to CRIRES with a minimum impact on the instrument optics and mechanics.
© (2012) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
E. Oliva, A. Hatzes, N. Piskunov, A. Reiners, H. U. Käufl, D. Ferruzzi, A. Tozzi, and L. Origlia "Upgrading CRIRES-VLT to cross-dispersed mode", Proc. SPIE 8446, Ground-based and Airborne Instrumentation for Astronomy IV, 84462N (24 September 2012); https://doi.org/10.1117/12.924969
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Cited by 2 scholarly publications.
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KEYWORDS
Prisms

Spectrographs

Sensors

Lithography

Spectrometers

Infrared radiation

Infrared spectroscopy

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