activity
20032025
most citedLong term variability of Cygnus X-1 V. State definitions with all sky monitors

102 citations · 1.8k across the 68 of their papers we have counts for

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9 papers · 1 filter

astro-ph2008★ 1 cited

The Galactic population of HMXBs as seen with INTEGRAL during its four first years of activity

Jerome Rodriguez, Arash Bodaghee

We collected the parameters (position, absorption, spin, orbital period, etc..), when known, of all Galactic sources detected by INTEGRAL during its four first years of activity. W…

astro-ph2007★ 99 cited

A description of sources detected by INTEGRAL during the first 4 years of observations

A. Bodaghee, T. J. -L. Courvoisier, J. Rodriguez +6

Parameters from the literature, such as positions, photoelectric absorption (nH), spin and orbital periods, and distances or redshifts, were collected for all ~500 sources detected…

astro-ph2006★ 30 cited

The discovery outburst of the X-ray transient IGR J17497-2821 observed with RXTE and ATCA

Jerome Rodriguez, Marion Cadolle Bel, John A. Tomsick +4

We report the results of a series of RXTE and ATCA observations of the recently-discovered X-ray transient IGR J17497-2821. Our 3-200 keV PCA+HEXTE spectral analysis shows very lit…

astro-ph2005★ 44 cited

INTEGRAL and XMM-Newton observations of the X-ray pulsar IGR J16320-4751/AX J1631.9-4752

J. Rodriguez, A. Bodaghee, P. Kaaret +16

We report on observations of the X-ray pulsar IGR J16320-4751 (a.k.a. AX J1631.9-4752) performed simultaneously with INTEGRAL and XMM-Newton. We refine the source position and iden…

astro-ph2005★ 37 cited

IGR J17252-3616: an accreting pulsar observed by INTEGRAL and XMM-Newton

J. A. Zurita Heras, G. De Cesare, R. Walter +5

The discovery of the X-ray source IGR J17252-3616 by INTEGRAL was reported on 9 February 2004. Regular monitoring by INTEGRAL shows that IGR J17252-3616 is a persistent hard X-ray…

astro-ph2005★ 54 cited

IGR J16393-4643: a new heavily-obscured X-ray pulsar

A. Bodaghee, R. Walter, J. A. Zurita Heras +5

An analysis of the high-energy emission from IGR J16393-4643 (=AX J1639.0-4642) is presented using data from INTEGRAL and XMM-Newton. The source is persistent in the 20-40 keV band…