Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
University of Wisconsin, USA
UTAustin
Gemini Observatory
Univ. of Texas
University of Wisconsin, Madison
University of Texas
UT Austin
UTexas
University of Texas at Austin
WIYN
Royal Observatory, Edinburgh, Scotland; Michigan, University, Ann Arbor
Siena College
Gemini
Gemini Obs.
Department of Astronomy, University of Texas at Austin, 1 University Station, C1400, Austin, TX 78712; McDonald Observatory, Fort Davis, TX 79734.
University of Wisconsin
Department of Astronomy, 475 N. Charter Street, University of Wisconsin, Madison, WI 53706, USA
Univ TX-Austin
University of Texas, Austin
Embry-Riddle Aeronautical University
Department of Astronomy, University of Texas at Austin, Austin, TX, USA; Department of Physics, Siena College, Loudonville, NY
Department of Astronomy, University of Texas at Austin, Austin, TX 78759, USA
University of Texasas
University of Texasas-Austin
Department of Astronomy, University of Texas at Austin, Austin, TX 78712; McDonald Observatory, Fort Davis, TX 79734.
Department of Astronomy, University of Texas at Austin, RLM 15.308, C-1400, Austin, TX 78712-1083 Observatoires
Physics Department, Siena College, 515 Loudon Road, Loudonville, NY 12211, USA
Department of Astronomy, University of Texas at Austin, 1 University Station C1400, Austin, TX 78712-0259, USA; Visiting Scientist, Department of Physics, Florida International University, Miami, FL, USA
University of Texas, McDonald Obs.
Michigan, University, Ann Arbor
Siena College, Loudonville, NY, USA
Siena College, Loudonville, NY, USA; University of Texas, Austin, TX, USA
Gemini Obs
University of Wisconsin, Madison, Wisconsin 53706
Michigan Univ., Ann Arbor; Cambridge Univ. Inst. of Astronomy, United Kingdom
Department of Astron
(Teff,log g,[Fe/H]) Classification of Low-Resolution Stellar Spectra using Artificial Neural Networks
A Bayesian Approach to Parameters of Galactic Globular Clusters
A Deep Wide-Area Proper Motion Survey
A Detailed Model Atmosphere Analysis of Cool White Dwarfs in the Sloan Digital Sky Survey
A method for obtaining the age and scale height of the thick disk from faint Stromgren photometry
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