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20042017
most citedAn extremely luminous panchromatic outburst from the nucleus of a distant galaxy

363 citations · 3.2k across the 58 of their papers we have counts for

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Showing 2011Show all

11 papers · 1 filter

astro-ph.HE2011★ 159 cited

The faint "heartbeats" of IGR J17091-3624: an exceptional black-hole candidate

D. Altamirano, T. Belloni, M. Linares +9

We report on the first 180 days of RXTE observations of the outburst of the black hole candidate IGR J17091-3624. This source exhibits a broad variety of complex light curve patter…

astro-ph.HE2011

Observations of particle acceleration in the blast waves of Gamma-ray Bursts

P. A. Curran

The electron energy distribution index, p, is a fundamental parameter of the process by which electrons at shock fronts are accelerated to relativistic speeds and by which they rad…

astro-ph.HE2011

IGR J17448-3232 point source: A blazar candidate viewed through the Galactic centre?

P. A. Curran, S. Chaty, J. A. Zurita Heras +2

The error region of the INTEGRAL source, IGR J17448-3232, contains an X-ray point source at the edge of a ~3' radius extended X-ray source. It has been suggested that the extended…

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…

astro-ph.HE2011★ 2 cited

A search for near infrared counterparts of 3 pulsar wind nebulae

P. A. Curran, S. Chaty, J. A. Zurita Heras +1

While pulsar wind nebulae (PWNe) and their associated isolated pulsars are commonly detected at X-ray energies, they are much rarer at near infrared (nIR) and optical wavelengths.…

astro-ph.HE2011★ 11 cited

Discovery and identification of infrared counterpart candidates of four Galactic centre low mass X-ray binaries

P. A. Curran, S. Chaty, J. A. Zurita Heras

The near infrared (nIR)/optical counterparts of low mass X-ray binaries (LMXBs) are often observationally dim and reside in high source density fields which make their identificati…