Astrophysical Journal Supplement Series, Dec 1, 2008
We present photometry for globular and open cluster stars observed with the Sloan Digital Sky Sur... more We present photometry for globular and open cluster stars observed with the Sloan Digital Sky Survey (SDSS). In order to exploit over 100 million stellar objects with r < 22.5 mag observed by SDSS, we need to understand the characteristics of stars in the SDSS ugriz filters. While star clusters provide important calibration samples for stellar colors, the regions close
Astrophysical Journal Supplement Series, Dec 1, 2008
We present photometry for globular and open cluster stars observed with the Sloan Digital Sky Sur... more We present photometry for globular and open cluster stars observed with the Sloan Digital Sky Survey (SDSS). In order to exploit over 100 million stellar objects with r < 22.5 mag observed by SDSS, we need to understand the characteristics of stars in the SDSS ugriz filters. While star clusters provide important calibration samples for stellar colors, the regions close
Astrophysical Journal Supplement Series, Dec 1, 2008
We present photometry for globular and open cluster stars observed with the Sloan Digital Sky Sur... more We present photometry for globular and open cluster stars observed with the Sloan Digital Sky Survey (SDSS). In order to exploit over 100 million stellar objects with r < 22.5 mag observed by SDSS, we need to understand the characteristics of stars in the SDSS ugriz filters. While star clusters provide important calibration samples for stellar colors, the regions close
Astrophysical Journal Supplement Series, Dec 1, 2008
We present photometry for globular and open cluster stars observed with the Sloan Digital Sky Sur... more We present photometry for globular and open cluster stars observed with the Sloan Digital Sky Survey (SDSS). In order to exploit over 100 million stellar objects with r < 22.5 mag observed by SDSS, we need to understand the characteristics of stars in the SDSS ugriz filters. While star clusters provide important calibration samples for stellar colors, the regions close
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Papers by Viktor Malanushenko