The Open Cluster Chemical Abundances and Mapping (OCCAM) Survey: Overview and Membership Methods

Bibcode
2017AAS...22934301D
Donor, J.; Frinchaboy, Peter M.; O'Connell, Julia; Cunha, Katia M. L.; Thompson, Benjamin A.; Melendez, Matthew; Shetrone, Matthew D.; Majewski, Steven R.; Zasowski, Gail; Allende-Prieto, C.; Pinsonneault, Marc H.; Roman-Lopes, Alexandre; Schultheis, Mathias; Stassun, Keivan G.; Apogee Team
Referencia bibliográfica

American Astronomical Society, AAS Meeting #229, id.343.01

Fecha de publicación:
1
2017
Número de autores
15
Número de autores del IAC
1
Número de citas
0
Número de citas referidas
0
Descripción
The Open Cluster Chemical Analysis and Mapping (OCCAM) survey aims to produce a comprehensive, uniform, infrared-based data set for hundreds of open clusters, and constrain key Galactic dynamical and chemical parameters using the SDSS/APOGEE survey. We present the sample and methods being used by the survey to determine membership for the few-star sampling for most clusters as observed by the SDSS/APOGEE. We present verification of the membership method using the DR13 sample, and show an extension of the method by incorporation of proper motion and parallax data from the ESA Gaia mission.This work is supported by an NSF AAG grant AST-1311835.
Tipo
Sin árbitro

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