From the Inner to Outer Milky Way: A Photometric Sample of 2.6 Million Red Clump Stars
arXiv:2002.02961 · doi:10.1093/mnras/staa1226
Abstract
Large pristine samples of red clump stars are highly sought after given that they are standard candles and give precise distances even at large distances. However, it is difficult to cleanly select red clumps stars because they can have the same T and log as red giant branch stars. Recently, it was shown that the asteroseismic parameters, P and , which are used to accurately select red clump stars, can be derived from spectra using the change in the surface carbon to nitrogen ratio ([C/N]) caused by mixing during the red giant branch. This change in [C/N] can also impact the spectral energy distribution. In this study, we predict the P, , T and log using 2MASS, AllWISE, \gaia, and Pan-STARRS data in order to select a clean sample of red clump stars. We achieve a contamination rate of 20\%, equivalent to what is achieved when selecting from T and log derived from low resolution spectra. Finally, we present two red clump samples. One sample has a contamination rate of 20\% and 405,000 red clump stars. The other has a contamination of 33\% and 2.6 million red clump stars which includes 75,000 stars at distances 10 kpc. For |b|>30 degrees we find 15,000 stars with contamination rate of 9\%. The scientific potential of this catalog for studying the structure and formation history of the Galaxy is vast given that it includes millions of precise distances to stars in the inner bulge and distant halo where astrometric distances are imprecise.
18 pages, 13 figures, 2 tables, submitted to MNRAS
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