Photometry of Gliese 372

Details Photometry of Gliese 372 Photometry of Gliese 372

Dec 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999aj....118.2988r&link_type=abstract

The Astronomical Journal, Volume 118, Issue 6, pp. 2988-2992.

Astronomy and Astrophysics

Astronomy

Stars: Binaries: Eclipsing, Stars: Activity, Stars: Individual: Name: Gliese 372

Scientific paper

Photometry of Gliese 372 was obtained during the 1996-1997 and 1997-1998 observing seasons. Our 3σ limit on the presence of night-to-night variations, such as those due to eclipses or starspots, is +/-0.024 mag. Over a single night, our limit on the presence of flares, eclipses, or other photometric variations is typically +/-0.02. If the system is eclipsing, there was a 40% chance that we would have detected the eclipse based on the quoted uncertainties of the ephemeris. The observed lack of flares or photometric variations due to starspots suggests a low level of stellar activity.

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