NASA Logo

NTRS

NTRS - NASA Technical Reports Server

Back to Results
A new Fabry-Perot spectrometer for observations of diffuse near-infrared line emissionWe describe a new Fabry-Perot spectrometer that is optimized for the detection of extended, low-surface-brightness line emission from 1.4 to 2.4 microns. The instrument combines high throughput and high sensitivity, yet limits the background radiation falling on the detector. The instrument has a single 20 sec - 200 sec beam and a resolving power lambda/delta(lambda) approximately 2500. The system is background shot-noise limited in the K window and limited by a combination of read noise, dark-current shot noise, and fluctuations in the OH airglow lines in the H window. We present sample data of some of the lowest-surface-brightness H2 line emission in the near infrared obtained to date.
Document ID
19950044248
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Luhman, M. L.
(Univ. of Texas, Austin, TX United States)
Jaffe, D. T.
(Univ. of Texas, Austin, TX United States)
Keller, L. D.
(Univ. of Texas, Austin, TX United States)
Soojong, Pak
(Univ. of Texas, Austin, TX United States)
Date Acquired
August 16, 2013
Publication Date
February 1, 1995
Publication Information
Publication: Astronomical Society of the Pacific, Publications
Volume: 107
Issue: 708
ISSN: 0004-6280
Subject Category
Instrumentation And Photography
Accession Number
95A75847
Distribution Limits
Public
Copyright
Other

Available Downloads

There are no available downloads for this record.
No Preview Available