Time-Resolved CCD Photometry of the Optical Counterpart of Swift J2319.4+2619

Details Time-Resolved CCD Photometry of the Optical Counterpart of Swift J2319.4+2619 Time-Resolved CCD Photometry of the Optical Counterpart of Swift J2319.4+2619

Dec 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007atel.1318....1s&link_type=abstract

The Astronomer's Telegram, #1318

Astronomy and Astrophysics

Astronomy

1

Optical, Cataclysmic Variables

Scientific paper

We report the results of time-resolved CCD photometry of the Swift polar candidate recently identified by Mukai et al. (ATel#1309). A five-hour time series of V-band photometry at ~1 min time resolution was obtained with the Mount Laguna Observatory 1-m reflector during the interval 2007 Dec. 03.08 - 03.29 UT. These data reveal a strong, nearly sinusoidal modulation in the light curve with a period of ~0.12 day, and a peak-to-peak amplitude of ~1 mag (ranging from V~17.5 to V~16.5).

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