Stellar Astrophysics Using Ultra-High Precision CCD Time Series Photometry

Details Stellar Astrophysics Using Ultra-High Precision CCD Time Series Photometry Stellar Astrophysics Using Ultra-High Precision CCD Time Series Photometry

May 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001aas...198.4601h&link_type=abstract

American Astronomical Society, 198th AAS Meeting, #46.01; Bulletin of the American Astronomical Society, Vol. 33, p.847

Astronomy and Astrophysics

Astrophysics

Scientific paper

Using time-series CCD photometry and a wide-field imager, we have extended the techniques of differential photometry to provide robust photometric precisions for each star over the entire field of view. Reaching photometric precisions of 2 milli-magnitudes, we produced high cadence light curves for over 12,000 stars at mid- and high galactic latitude. The fraction of stars seen to be variable is higher than the canonical wisdom, being 10-14 will present the details of our techniques, sample light curves, methods to access the data, and a summary of astrophysical uses of such high precision data.

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