Faint spectrophotometric standard stars for large optical telescopes. I

Details Faint spectrophotometric standard stars for large optical telescopes. I Faint spectrophotometric standard stars for large optical telescopes. I

Jul 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984pasp...96..530f&link_type=abstract

Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 96, July 1984, p. 530-536.

Astronomy and Astrophysics

Astronomy

59

Reference Stars, Spectroscopic Telescopes, Stellar Spectrophotometry, White Dwarf Stars, Error Analysis, Spectral Energy Distribution

Scientific paper

The authors present spectral energy distributions over the range λλ3300 - 10000 for a set of five spectrophotometric standards four of which are white dwarfs. These stars are faint (V ≡ 15m.5), equatorial, and exhibit nearly featureless continua, so they can be observed without neutral density filters to calibrate the response of photon-counting spectrographs on large telescopes in both hemispheres.

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