VizieR Online Data Catalog: beta Cephei light curves from KELT project (Labadie-Bartz+, 2020)

The Kilodegree Extremely Little Telescope (KELT) is a photometric survey designed to discover transiting exoplanets orbiting stars in the magnitude range of 7<~V<~12, with light curves for ~4.9 million objects across ~70% of the sky. The KELT survey employs two small-aperture (42mm) wide-field (26°x26°) telescopes, with a northern location at Winer Observatory in Arizona in the United States, and a southern location at the South African Astronomical Observatory near Sutherland, South Africa. The effective passband is roughly equivalent to a broad R-band filter.

Raw data are the direct products of the difference imaging pipeline. We also have a detrending procedure using the TFA algorithm from Kovacs+ (2002A&A...391..369K), which removes common trends to the data analogous to the Kepler Cotrending Basis Vectors (CBVs).

(7 data files).