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20012025
most citedFast infrared variability from a relativistic jet in GX 339-4

138 citations · 503 across the 11 of their papers we have counts for

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astro-ph.HE2019★ 23 cited

Physical constraints from near-infrared fast photometry of the black-hole transient GX 339-4

F. M. Vincentelli, P. Casella, P. Petrucci +9

We present results from the first multi-epoch X-ray/IR fast-photometry campaign on the black-hole transient GX 339--4, during its 2015 outburst decay. We studied the evolution of t…

astro-ph.HE2018★ 31 cited

Characterization of the Infrared/X-ray sub-second variability for the black-hole transient GX 339-4

F. M. Vincentelli, P. Casella, T. J. Maccarone +7

We present a detailed analysis of the X-ray/IR fast variability of the Black-Hole Transient GX 339-4 during its low/hard state in August 2008. Thanks to simultaneous high time-reso…

astro-ph.HE2014★ 3 cited

Simultaneous independent measurements of a truncated inner accretion disc in the low/hard state of GX 3994

D. S. Plant, K. O'Brien, R. P. Fender

We present results from three recent XMM-Newton observations of GX 3394 in the low/hard state, taken during the decay of a bright (peak L) failed outburs…

astro-ph.HE2013★ 79 cited

An evolving compact jet in the black hole X-ray binary MAXI J1836-194

D. M. Russell, T. D. Russell, J. C. A. Miller-Jones +27

We report striking changes in the broadband spectrum of the compact jet of the black hole transient MAXI J1836-194 over state transitions during its discovery outburst in 2011. A f…

astro-ph.HE2012★ 125 cited

Jet spectral breaks in black hole X-ray binaries

D. M. Russell, S. Markoff, P. Casella +10

In X-ray binaries, compact jets are known to commonly radiate at radio to infrared frequencies, whereas at optical to gamma-ray energies, the contribution of the jet is debated. Th…

astro-ph.HE2011★ 27 cited

A late jet rebrightening revealed from multi-wavelength monitoring of the black hole candidate XTE J1752-223

D. M. Russell, P. A. Curran, T. Muñoz-Darias +15

We present optical monitoring of the black hole candidate XTE J1752-223 during its 2009 - 2010 outburst and decay to quiescence. The optical light curve can be described by an expo…