XTE J1752-223 has faded to quiescence: optical and infrared magnitudes

Details XTE J1752-223 has faded to quiescence: optical and infrared magnitudes XTE J1752-223 has faded to quiescence: optical and infrared magnitudes

Aug 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010atel.2775....1r&link_type=abstract

The Astronomer's Telegram, #2775

Astronomy and Astrophysics

Astronomy

4

Infra-Red, Optical, X-Ray, Binaries, Black Holes, Transients

Scientific paper

We have been regularly monitoring the outburst decay of the black hole candidate X-ray binary XTE J1752-223 (discovered by RXTE; ATel #2258) with the 2-m Faulkes Telescopes North and South (located at Haleakala on Maui and Siding Spring, Australia, respectively). Exposures in B, V, R and i'-bands (mostly 100-sec exposures each) were taken every ~ 3 days since 2010-03-22 (MJD 55277). The optical counterpart (ATels #2263, #2268, #2424) is detected up until 2010-07-15 (MJD 55392), after which detections become ambiguous due to close field stars in this crowded region of the Galactic plane.

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