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 |
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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] |
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ISSN: | 1063-7729 1562-6881 |
DOI: | 10.1134/1.1463100 |