Stellar Variability Studies with SMEI

Details Stellar Variability Studies with SMEI Stellar Variability Studies with SMEI

Dec 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003agufmsh41c..08p&link_type=abstract

American Geophysical Union, Fall Meeting 2003, abstract #SH41C-08

Astronomy and Astrophysics

Astronomy

7539 Stellar Astronomy

Scientific paper

The Solar Mass Ejection Imager (SMEI) instrument images most of the sky every 105 minutes. From this unique dataset, the brightnesses of stars down to and below the eight magnitude can be measured to investigate their variability. This paper presents the methods developed to extract the stellar brightnesses, and the accuracies obtained as a function of brightness and crowding. Example lightcurves are given.

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