VizieR Online Data Catalog: KIC red giants radial modes amplitude & lifetime (Vrard+, 2018)

Author(s)

M. Vrard, T. Kallinger, B. Mosser, C. Barban, F. Baudin, K. Belkacem, M. S. Cunha

Abstract

The two first data files contains the seismic global parameters of the stars listed in the paper. Each star is identified with its KIC number (Kepler Input Catalog).The large separation are derived from the fit of the radial and quadrupole oscillation modes. The frequency of maximum oscillation power are derived from the autocorrelation of the oscillation spectra. The global radial mode width are obtained from the mode widths of the three radial modes closer to the frequency of maximum oscillation power. The bolometric mode amplitude are derived from the mode amplitude of the three radial mode with the highest mode amplitudes. The radial mode widths and amplitudes are extracted from the lorentzians fit that was performed on those modes. The stellar mass is derived from the seismic scaling relations. The evolutionary status is derived according to the method developped by Vrard et al. (2016A&A...588A..87V, Cat. J/A+A/588/A87) and Kallinger et al. (2012A&A...541A..51K) The other files contain the raw data that was obtained from the radial mode fitting. The mode frequencies, widths and amplitudes are derived from lorentzians fit that was performed over the star radial modes with the FREQ method.(3 data files).

Organisation(s)

Department of Astrophysics

Publication date

2018

Austrian Fields of Science 2012

103004 Astrophysics, 103003 Astronomy

Keywords

Portal url

https://ucrisportal.univie.ac.at/en/publications/2f65c976-a5d4-4109-8d91-a1a06c945ef3