HATNet Pleiades Rotation Period Catalogue (Hartman+, 2010)

Details HATNet Pleiades Rotation Period Catalogue (Hartman+, 2010) HATNet Pleiades Rotation Period Catalogue (Hartman+, 2010)

Apr 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011ycat..74080475h&link_type=abstract

VizieR On-line Data Catalog: J/MNRAS/408/475. Originally published in: 2010MNRAS.408..475H

Physics

Clusters: Open, Stars: Variable, Photometry: Ubv, Photometry: Infrared, Rotational Velocities

Scientific paper

Photometric time-series observations of the Pleiades cluster were obtained between 2008 September 15 and 2009 March 16 using the identical HAT-9 and HAT-10 11-cm aperture robotic telescopes located at Mauna Kea Observatory (MKO) in Hawaii and at Fred L. Whipple Observatory (FLWO) in Arizona, respectively.
This catalogue contains photometric rotation periods for stars in the Pleiades open cluster. Most of the periods were measured from light curves obtained with the Hungarian-made Automated Telescope Network (HATNet) of small aperture robotic telescopes located in Arizona and Hawaii. A handful of stars with periods from the literature that were not recovered with the HATNet data are also included in the catalogue.
(5 data files).

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