Astronomy and Astrophysics – Astronomy
Scientific paper
Jul 1990
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990spie.1235..610r&link_type=abstract
IN: Instrumentation in astronomy VII; Proceedings of the Meeting, Tucson, AZ, Feb. 13-17, 1990 (A91-29601 11-35). Bellingham, WA
Astronomy and Astrophysics
Astronomy
6
Charge Coupled Devices, Fabry-Perot Spectrometers, Intergalactic Media, Interstellar Gas, Ionized Gases, Angular Resolution, Diffuse Radiation, Emission Spectra, Line Spectra
Scientific paper
The use of the University of Wisconsin 15-cm-diameter pressure-scanned Fabry-Perot spectrometer to detect and characterize faint optical emission lines from the Galaxy and the earth atmosphere is described, and a more powerful multichannel spectrometer is proposed. The fundamental principles and advantages of Fabry-Perot instruments are explained; the need for higher throughput is pointed out; the gains possible with a multichannel spectrometer are determined; and test results demonstrating the feasibility of multichannel spectrometry with either photomultiplier or CCD detectors are summarized. It is estimated that a multichannel spectrometer mounted at the Nasmyth focus of a 3.5-m or 8-m telescope would have a beam diameter of 10 or 4 arcmin, respectively, making it possible to probe ionized gas in the disks and halos of galaxies at emission measures less than about 1/cm to the 6th pc and spectral resolution 10 km/sec.
Harlander Jens
Reynolds Ron J.
Roesler Fred L.
Scherb Frank
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