The SEGUE Survey: Overview Context

Details The SEGUE Survey: Overview Context The SEGUE Survey: Overview Context

Jan 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012aas...21920501r&link_type=abstract

American Astronomical Society, AAS Meeting #219, #205.01

Astronomy and Astrophysics

Astronomy

Scientific paper

The SEGUE-1 and SEGUE-2 projects in SDSS-II and SDSS-III surveyed 400+ sparsely distributed 7 square degree pointings and 387,000 stars in the halo, anti-center and thick disk of the Milky Way. The publicly available data include the spectra, associated ugriz photometry and targeting information, radial velocity, and stellar parameter (metallicity, effective temperature, surface gravity) information. I will describe the survey data, how they were calibrated and how they can be accessed. I will review some additional, recent results from within and outside the collaboration to set the stage for the talks in the session.

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