Paper
13 October 1986 A Wide-Field Multi-Object Spectroscopy (MOS) System
F G Watson
Author Affiliations +
Abstract
Multi-object slit spectroscopy with a wide-field telescope is potentially a very effective way of collecting large quantities of data for statistical analysis on a wide variety of astronomical object-classes. A pilot-model system with 40 channels has been developed for the 1.2-metre UK Schmidt telescope, and has been extensively tested with photographic detection of the spectra. The commissioning of a dedicated cooled CCD camera in the immediate future is expected to lead to the rapid implementation of a user service with the system.
© (1986) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
F G Watson "A Wide-Field Multi-Object Spectroscopy (MOS) System", Proc. SPIE 0627, Instrumentation in Astronomy VI, (13 October 1986); https://doi.org/10.1117/12.968160
Lens.org Logo
CITATIONS
Cited by 9 scholarly publications.
Advertisement
Advertisement
RIGHTS & PERMISSIONS
Get copyright permission  Get copyright permission on Copyright Marketplace
KEYWORDS
Telescopes

Stars

Spectrographs

Molybdenum

Cameras

Photography

Astronomy

RELATED CONTENT

First light of UT 15-band dichroic-mirror camera
Proceedings of SPIE (July 25 2008)
FLAIR wide-field multiobject spectroscopy system
Proceedings of SPIE (July 01 1990)
Image acquisition system with three CCD cameras
Proceedings of SPIE (September 24 2012)
A Versatile Fiber Coupled CCD/Echelle Spectrograph System
Proceedings of SPIE (October 13 1986)
Theme On Two Wide-Coverage Spectrograph Cameras
Proceedings of SPIE (October 13 1986)

Back to Top