Paper
24 July 2014 A flux calibration device for the SuperNova Integral Field Spectrograph (SNIFS)
Simona Lombardo, Greg Aldering, Akos Hoffmann, Marek Kowalski, Daniel Kuesters, Klaus Reif, Michael Rigault
Author Affiliations +
Abstract
Observational cosmology employing optical surveys often require precise flux calibration. In this context we present SNIFS Calibration Apparatus (SCALA), a flux calibration system developed for the SuperNova Integral Field Spectrograph (SNIFS), operating at the University of Hawaii 2.2 m telescope. SCALA consists of a hexagonal array of 18 small parabolic mirrors distributed over the face of, and feeding parallel light to, the telescope entrance pupil. The mirrors are illuminated by integrating spheres and a wavelength-tunable (from UV to IR) light source, generating light beams with opening angles of 1°. These nearly parallel beams are flat and flux-calibrated at a subpercent level, enabling us to calibrate our “telescope + SNIFS system” at the required precision.
© (2014) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Simona Lombardo, Greg Aldering, Akos Hoffmann, Marek Kowalski, Daniel Kuesters, Klaus Reif, and Michael Rigault "A flux calibration device for the SuperNova Integral Field Spectrograph (SNIFS)", Proc. SPIE 9147, Ground-based and Airborne Instrumentation for Astronomy V, 91474R (24 July 2014); https://doi.org/10.1117/12.2055066
Lens.org Logo
CITATIONS
Cited by 1 scholarly publication.
Advertisement
Advertisement
RIGHTS & PERMISSIONS
Get copyright permission  Get copyright permission on Copyright Marketplace
KEYWORDS
Calibration

Telescopes

Mirrors

Integrating spheres

Projection systems

Spectrographs

Light sources

RELATED CONTENT

Calibration systems for LSST
Proceedings of SPIE (July 22 2014)
Preparing the SALT for near-infrared observations
Proceedings of SPIE (August 29 2022)
DOTIFS: fore-optics and calibration unit design
Proceedings of SPIE (July 09 2018)
The GMT Consortium Large Earth Finder (G CLEF) an...
Proceedings of SPIE (August 09 2016)
Flat field for LAMOST
Proceedings of SPIE (July 11 2008)

Back to Top