Apparent non-variable stars from the Kepler mission

Author(s)
E. Paunzen, F. Binder, A. Cyniburk, M. N. Duffek, F. Haberhauer, C. Heinreichsberger, H. Kohlhofer, L. Kueß, H. M. Maitzen, T. Saalmann, A. M. Schanz, S. Schauer, K. Schmidt, A. Tokareva, I. Wizani
Abstract

Context. The analysis of non-variable stars is generally neglected in the literature. However, such objects are needed for many calibration processes and for testing pulsational models. The photometric time series of the Kepler satellite mission still stand as the most accurate data available today and are excellently suited to the search for non-variable stars. Aims. We analysed all long-cadence light curves for stars not reported as a variable so far from the Kepler satellite mission. Using the known characteristics and flaws of these data sets, we defined three different frequency ranges where we searched for non-variability. Methods. We used the Lomb-Scargle periodogram and the false-alarm probability (FAP) to analyse the cleaned data sets of 138 451 light curves. We then used log FAP ≥ - 2 to define a star as 'non-variable' in the ranges below 0.1 c/d, 0.1 to 2.0 c/d, and 2.0 to 25.0 c/d, respectively. Furthermore, we also calculated the standard deviation of the mean light curve to obtain another parameter. Results. In total, we found 14 154 stars that fulfil the set criteria. These objects are mostly cooler than the 7000 K populating the whole main sequence (MS) to the red giant branch (RGB).

Organisation(s)
Department of Astrophysics, International Office
External organisation(s)
Masaryk University, University of Vienna
Journal
Astronomy and Astrophysics
Volume
687
No. of pages
7
ISSN
0004-6361
DOI
https://doi.org/10.1051/0004-6361/202244572
Publication date
07-2024
Peer reviewed
Yes
Austrian Fields of Science 2012
103003 Astronomy, 103004 Astrophysics
Keywords
ASJC Scopus subject areas
Astronomy and Astrophysics, Space and Planetary Science
Portal url
https://ucrisportal.univie.ac.at/en/publications/b708e568-cc0e-4621-b13b-ee82b695caf6