VizieR Online Data Catalog: Mid-eclipse times of KIC 10544976 (Almeida+, 2019)

The KIC 10544976 data were retrieved from the Kepler data search webpages (http://exoplanetarchive.ipac.caltech.edu; http://archive.stsci.edu/pub/kepler/ffi). We use the Presearch Data Conditioning (http://keplergo.arc.nasa.gov/PipelinePDC.shtml) (PDC) and the full frame images (FFIs). Raw photometric data of KIC 10544976 and calibration (flat-field and bias) images were retrieved from the Isaac Newton Group public archive (http://casu.ast.cam.ac.uk/casuadc/ingarch/query). The photometric observations were performed with the Auxiliary-port CAMera attached to the 4.2 m William Herschel Telescope (WHT) and with the Wide Field Camera coupled to the 2.54 m INT at Roque de los Muchachos Observatory. The observations were done on 2008 August 28 and 2014 July 21 (WHT), and on 2017 April 5 (INT). We use the same approach described in Almeida et al. (2013ApJ...766...11A) to derive the mid-eclipse times and their uncertainties. In short, a Markov chain Monte Carlo (MCMC) procedure was performed to sample the mid-eclipse time and to examine the marginal posterior distribution of the probability of the parameters. The median of the distribution provides the mid-eclipse time and the area corresponding to the 1σ percentile provides the uncertainty. Our 2745 new mid-eclipse times from the Kepler, WHT, and INT data, and previous values obtained by Almenara et al. (2012MNRAS.420.3017A) are presented in Table 1.

(1 data file).