VizieR Online Data Catalog: The BAM pipeline applied to K2 LCs of red giants (Zinn+, 2019)

In this paper, we work with two sets of K2 light curves: (1) the Campaign 1 (C1) target sample from the K2 Galactic Archaeology Program (GAP; Stello+ 2015ApJ...809L...3S & 2017, J/ApJ/835/83), which comprises 8630 stars, and (2) all non-GAP C1 targets, 13016 in total. Results from the Bayesian Asteroseismology data Modeling (BAM) for the former sample have been published in Stello+ (2017, J/ApJ/835/83).

We apply the BAM pipeline to 13016 C1 targets with VJ light curves not in the GAP sample. We identify 31 red giants that have detectable oscillation excesses. An additional 73 objects are potential giants. See Section 4.

(1 data file).