8.6 Hour Period in XMMU J115113.3-623730

Details 8.6 Hour Period in XMMU J115113.3-623730 8.6 Hour Period in XMMU J115113.3-623730

Aug 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010atel.2777....1p&link_type=abstract

The Astronomer's Telegram, #2777

Astronomy and Astrophysics

Astrophysics

Optical, X-Ray, Cataclysmic Variables, Novae

Scientific paper

We have obtained time-series differential photometry of XMMU J115113.3-623730, the eruptive star reported by Greiner et al. (ATel #2746) and Hughes et al. (ATel #2771). Coverage consisted of 17 separate time series in V and unfiltered light, from 19 July to 6 August 2010, using several telescopes in the Center for Backyard Astrophysics (CBA) network. We used overlaps of V-light and unfiltered-light time series to convert the latter to a V scale; this produced an overall calibration uncertainty of 0.10-0.15 mag.

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