THE SEGUE STELLAR PARAMETER PIPELINE. I. DESCRIPTION AND COMPARISON OF INDIVIDUAL METHODS

Abstract

We describe the development and implementation of the Sloan Extension for Galactic Exploration and Understanding (SEGUE) Stellar Parameter Pipeline (SSPP). The SSPP is derived, using multiple techniques, radial velocities, and the fundamental stellar atmospheric parameters (effective temperature, surface gravity, and metallicity) for AFGK-type stars, based on medium-resolution spectroscopy and ugriz photometry obtained during the course of the original Sloan Digital Sky Survey (SDSS-I) and its Galactic extension (SDSS-II/SEGUE). The SSPP also provides spectral classification for a much wider range of stars, including stars with temperatures outside the window where atmospheric parameters can be estimated with the current approaches. This is Paper I in a series of papers on the SSPP; it provides an overview of the SSPP, and tests of its performance using several external data sets. Random and systematic errors are critically examined for the current version of the SSPP, which has been used for the sixth public data release of the SDSS (DR-6).

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Affiliated Institutions

• Texas Tech University US
• Harvard University US
• Chinese Academy of Sciences CN
• University of California, Santa Cruz US
• National Astronomical Observatories CN
• University of Ljubljana SI
• Joint Institute for Nuclear Astrophysics US
• Australian National University AU
• Rensselaer Polytechnic Institute US
• Fermi National Accelerator Laboratory US
• Max Planck Institute for Astronomy DE
• Michigan State University US
• The University of Texas at Austin US

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