Variability Properties of 4 Million Sources in the $TESS$ Input Catalog Observed with the Kilodegree Extremely Little Telescope Survey
Ryan J. Oelkers, Joseph E. Rodriguez, Keivan G. Stassun, Joshua, Pepper, Garrett Somers, Stella Kafka, Daniel J. Stevens, Thomas G. Beatty,, Robert J. Siverd, Michael B. Lund, Rudolf B. Kuhn, David James, B. Scott, Gaudi

TL;DR
This paper presents a comprehensive catalog of stellar variability and rotation periods for over 4 million sources observed by the KELT survey, including detailed variability measurements and upper limits, facilitating follow-up studies.
Contribution
It provides the first large-scale variability catalog from KELT data, including variability amplitudes, periods, and upper limits for millions of stars, linked with TESS and variable star databases.
Findings
Identified over 52,000 variable stars with significant amplitude fluctuations.
Detected stellar rotation periods for over 62,000 sources.
Achieved sensitivity to variability down to 5 mmag at V~8.
Abstract
The Kilodegree Extremely Little Telescope (KELT) has been surveying more than of the celestial sphere for nearly a decade. While the primary science goal of the survey is the discovery of transiting, large-radii planets around bright host stars, the survey has collected more than images, with a typical cadence between minutes, for more than million sources with apparent visual magnitudes in the approximate range . Here we provide a catalog of 52,741 objects showing significant large-amplitude fluctuations likely caused by stellar variability and 62,229 objects identified with likely stellar rotation periods. The detected variability ranges in -amplitude from 3 mmag to 2.3 mag, and the detected periods range from 0.1 days to 2000 days. We provide variability upper limits for all other 4 million sources. These upper limits are…
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