Intermediate-brightness equatorial spectrophotometric standards

We have obtained spectral energy distributions for 41 7^sup m^-8^sup m^ stars near the celestial equator (δ=±3°). The λλ3100-7600 Å spectral range is studied with a spectral resolution of 50 Å. The relative rms error in the visible is 1-2%, increasing to 3-5% towards the edges of the wavelength inte...

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Veröffentlicht in:Astronomy reports 2002-03, Vol.46 (3), p.224-232
1. Verfasser: Tereshchenko, V M
Format: Artikel
Sprache:eng
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Zusammenfassung:We have obtained spectral energy distributions for 41 7^sup m^-8^sup m^ stars near the celestial equator (δ=±3°). The λλ3100-7600 Å spectral range is studied with a spectral resolution of 50 Å. The relative rms error in the visible is 1-2%, increasing to 3-5% towards the edges of the wavelength interval studied. All stars are referenced to a single standard, the circumpolar star HD 221525. The synthetic colors of common stars are compared with those observed in four photometric systems: U BV, W BV R, uvby, and that of the TYCHO catalog. The program stars are recommended as secondary spectrophotometric standards.[PUBLICATION ABSTRACT]
ISSN:1063-7729
1562-6881
DOI:10.1134/1.1463100