Starspots on AP063 and AP117 Imaged via Matrix Light-curve Inversion

Details Starspots on AP063 and AP117 Imaged via Matrix Light-curve Inversion Starspots on AP063 and AP117 Imaged via Matrix Light-curve Inversion

Dec 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003aas...203.8309h&link_type=abstract

American Astronomical Society Meeting 203, #83.09; Bulletin of the American Astronomical Society, Vol. 35, p.1339

Astronomy and Astrophysics

Astronomy

Scientific paper

Matrix Light-curve Inversion (MLI) is a technique for imaging spotted stars using the variations in their light curves. MLI makes no a priori assumptions regarding the number of spots, their sizes, or their shapes. The resolution in latitude is improved when light curves obtained through multiple photometric filters are simultaneously inverted. We present images of two stars in the α Persei cluster, AP063 and AP117, based on BVRI CCD photometry obtained at the Michigan-Dartmouth-MIT Observatory from September 18-26, 2001.

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