activity
20022011
most citedMulti-wavelength observations of Galactic hard X-ray sources discovered by INTEGRAL. I. The nature of the companion star

146 citations · 1.2k across the 25 of their papers we have counts for

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astro-ph2005

INTEGRAL and RXTE Observations of Centaurus A

Richard E. Rothschild, Joern Wilms, John Tomsick +6

INTEGRAL and RXTE performed three simultaneous observations of the nearby radio galaxy Cen A in 2003 March, 2004 January, and 2004 February with the goals of investigating the geom…

astro-ph2005

The Galactic black hole transient H1743-322 during outburst decay: connections between timing noise, state transitions and radio emission

E. Kalemci, J. A. Tomsick, R. E. Rothschild +3

Multi-wavelength observations of Galactic black hole transients during outburst decay are instrumental for our understanding of the accretion geometry and the formation of outflows…

astro-ph2005

Evolution of the X-Ray Jets from 4U 1755--33

P. Kaaret, S. Corbel, J. A. Tomsick +4

We report on new X-ray observations of the large-scale jets recently discovered in X-rays from the black hole candidate 4U 1755-33. Our observations in 2004 show that the jets foun…

astro-ph2005

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

Discovery of the Millisecond X-Ray Pulsar HETE J1900.1-2455

P. Kaaret, E. H. Morgan, R. Vanderspek +1

We report the discovery of millisecond pulsations from the low-mass X-ray binary HETE J1900.1-2455 which was discovered by the detection of a type I X-ray burst by the High Energy…

astro-ph2005

On the origin of black hole X-ray emission in quiescence: Chandra observations of XTE J1550-564 and H 1743-322

S. Corbel, J. A. Tomsick, P. Kaaret

We report the results of observations of the black hole binaries XTE J1550-564 and H 1743-322 in their quiescent state using the Chandra X-ray Observatory. Both sources are detecte…