Trends in observational UV stellar spectroscopy

Details Trends in observational UV stellar spectroscopy Trends in observational UV stellar spectroscopy

Jun 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977cosp.meetq....h&link_type=abstract

COSPAR, Plenary Meeting, 20th, Tel Aviv, Israel, June 7-18, 1977, Paper. 5 p.

Computer Science

Stellar Spectrophotometry, Technology Assessment, Ultraviolet Spectrometers, Ultraviolet Spectroscopy, Balloon-Borne Instruments, Gratings (Spectra), Iue, Light Sources, Radiation Detectors, Rocket-Borne Instruments, Signal To Noise Ratios

Scientific paper

The development of instruments for UV stellar spectroscopy since 1965 is discussed. Reasons for using gratings rather than Fourier techniques in such instruments are considered, and advantages of multichannel detection systems are noted. Several instruments designed for rocketborne, balloonborne, and spaceborne UV spectroscopic observations are compared on the basis of two factors of merit.

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