CoRoT photometry of three O-type stars (Blomme+, 2011)

Details CoRoT photometry of three O-type stars (Blomme+, 2011) CoRoT photometry of three O-type stars (Blomme+, 2011)

Jul 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011ycat..35339004b&link_type=abstract

VizieR On-line Data Catalog: J/A+A/533/A4. Originally published in: 2011A&A...533A...4B

Physics

Stars: O, Photometry

Scientific paper

We use a prewhitening technique to analyse the CoRoT photometry, and list the frequencies, semi-amplitudes and phases (with their respective error bars). The phases are defined with t=0 corresponding to the first non-flagged data point. We also list the standard deviation at each stage in the prewhitening and the significance of the frequency under the assumption of red noise. Red-noise significant frequencies are noted as well as those frequencies that remain present if we split the data set in two halves.
(3 data files).

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