GX 339-4 is rising into outburst, and a deep optical quiescent magnitude observed by Faulkes Telescope South

Lewis, F.; Russell, D. M.; Shahbaz, T.
Bibliographical reference

The Astronomer's Telegram, #4162

Advertised on:
6
2012
Number of authors
3
IAC number of authors
2
Citations
5
Refereed citations
5
Description
We report a gradual (~ 1 mag in 50 days) optical re-brightening of the black hole X-ray binary, GX 339-4. We have been monitoring the source with the 2-m Faulkes Telescope (FT) South (located at Siding Spring, Australia) in SDSS i'-band, Bessel R and Bessel V filters (200-second exposures; see e.g. Cadolle Bel et al. 2011). The images are reduced using the FT pipeline.