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GX 339-4 in a very low luminosity state

ATel #196; Elena Gallo, Rob Fender (U Amsterdam) & Stephane Corbel (U Paris VII & CEA Saclay)
on 3 Oct 2003; 15:48 UT
Credential Certification: Elena Gallo (egallo@science.uva.nl)

Subjects: Radio, X-ray, Black Hole, Transient

Referred to by ATel #: 230, 2270, 2281, 3383, 4247

A 30 ksec Chandra ACIS-S observation on MJD 52911 reveals the black hole X-ray binary GX 339-4 to have entered a very low luminosity state following a more than 2-year-long outburst period (ATEL #85, #95, #107, #120). The X-ray spectrum is well fitted by an absorbed power-law with photon index 2+/-0.2 and absorption column N_H=7+/-1x10e21 cm^-2. The (unabsorbed) 0.4-11 keV flux is of 3.8e-13 erg sec^-1 cm^-2, with a corresponding luminosity of 4.6e31x(d/kpc)^2 erg sec^-1, comparable to the faintest ever measured from GX 339-4. Simultaneous radio observations with the Australia Telescope Compact Array did not detect the source to an rms noise level of 0.015 mJy/beam at 4.8 GHz.