Stellar Photometry in SDSS Filters u'g'r'i'z' in SA 57 and SA 68

Details Stellar Photometry in SDSS Filters u'g'r'i'z' in SA 57 and SA 68 Stellar Photometry in SDSS Filters u'g'r'i'z' in SA 57 and SA 68

Dec 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995aas...187.3203s&link_type=abstract

American Astronomical Society, 187th AAS Meeting, #32.03; Bulletin of the American Astronomical Society, Vol. 27, p.1328

Astronomy and Astrophysics

Astronomy

Scientific paper

Using the filter system for the Sloan Digital Sky Survey, I present photometry of stars at two galactic latitudes, 86.2deg and 35.5deg . The number densities and color distributions agree with standard galactic models. The bi-modal color distributions reflect halo and disk components. These distributions can be used to determine the mean color shift with an accuracy better than 0.1 mag. In color-color space, the stellar locus agrees with colors calculated for the main sequence, demonstrating usefulness of this system for selecting non-stellar objects based on photometry alone.

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