Paper
21 August 1998 Portable telescope for surveys of diffuse near-infrared line emission
Eric W. Klumpe, Daniel T. Jaffe
Author Affiliations +
Abstract
Spectroscopic studies of degree-scale IR line emission from telescopes on the Earth's surface are very challenging. Not only does the emission from atmospheric OH molecules fluctuate in time and vary spatially, but also the extent of interstellar clouds makes it impossible to establish a zero point for flux measurements close to the emission regions. Beam-switching can solve both problems, but traditional telescopes cannot switch between fields that are several degrees apart before the OH emission changes significantly. We present here the design for a telescope we have constructed in order to obtain quantitative measures of the extended, UV-excited, near-IR line flux from the Galactic Center and from nearby star-forming clouds. It uses a coelostat to beam-switch across angels as large as 10 degrees in less than 1 second. Its 20 arc-minute beamsize, combined with its 150 mm aperture, gives it a surface brightness sensitivity comparable to much larger telescopes, while maintaining portability. This telescope, integrated with a Fabry-Perot spectrometer, has been used successfully at both McDonald Observatory and the Cerro Tololo Interamerican Observatory and has mapped near-IR molecular hydrogen emission over the inner 10 degrees of the Galaxy for the first time.
© (1998) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Eric W. Klumpe and Daniel T. Jaffe "Portable telescope for surveys of diffuse near-infrared line emission", Proc. SPIE 3354, Infrared Astronomical Instrumentation, (21 August 1998); https://doi.org/10.1117/12.317338
Advertisement
Advertisement
RIGHTS & PERMISSIONS
Get copyright permission  Get copyright permission on Copyright Marketplace
KEYWORDS
Telescopes

Mirrors

Spectroscopy

Stars

Clouds

Fabry–Perot interferometers

Space telescopes

RELATED CONTENT

Stratospheric Observatory for Infrared Astronomy (SOFIA)
Proceedings of SPIE (August 28 1998)
Single-aperture far-infrared observatory (SAFIR)
Proceedings of SPIE (March 05 2003)
POST: a polar stratospheric telescope
Proceedings of SPIE (June 01 1994)
Conceptual design for a second generation space telescope
Proceedings of SPIE (November 01 1993)
The Optics Support Structure Of The MMT
Proceedings of SPIE (June 03 1987)

Back to Top