SDSS ultracool and halo WD candidates (Vidrih+, 2007)

Details SDSS ultracool and halo WD candidates (Vidrih+, 2007) SDSS ultracool and halo WD candidates (Vidrih+, 2007)

Nov 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008ycat..73820515v&link_type=abstract

VizieR On-line Data Catalog: J/MNRAS/382/515. Originally published in: 2007MNRAS.382..515V

Astronomy and Astrophysics

Astronomy

Stars: White Dwarf, Photometry: Sdss, Proper Motions

Scientific paper

SDSS is an imaging and spectroscopic survey that has mapped more than a quarter of the sky. Imaging data are produced simultaneously in five photometric bands, namely u, g, r, i and z. The data are processed through pipelines to measure photometric and astrometric properties .
SDSS Stripe 82 covers a ~250deg2 area of sky, consisting of a 2.5{deg} strip along the celestial equator from right ascension -49.5{deg} to +49.5{deg}. The stripe has been repeatedly imaged between June and December each year from 1998 to 2005. Sixty-two of the total of 134 available imaging runs were obtained in 2005.
(3 data files).

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