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20022007
most citedObservations of the 599 Hz Accreting X-ray Pulsar IGR J00291+5934 during the 2004 Outburst and in Quiescence

40 citations · 40 across the 1 of their papers we have counts for

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9 papers

astro-ph200740 cited

Observations of the 599 Hz Accreting X-ray Pulsar IGR J00291+5934 during the 2004 Outburst and in Quiescence

M. A. P. Torres, P. G. Jonker, D. Steeghs +10

We report on optical and NIR observations obtained during and after the 2004 December discovery outburst of the X-ray transient and accretion-powered millisecond pulsar IGR J00291+…

astro-ph2005

The broad-band spectrum of Cyg X-2 with INTEGRAL

G. Lavagetto, T. Di Salvo, M. Falanga +7

We study the broad band (3-100 keV) spectrum of Cygnus X-2 with INTEGRAL. We find that the spectrum is well fitted by a Comptonized component with a seed-photons temperature of ~1…

astro-ph2005

Discovery of a redshifted X-ray emission line in the symbiotic neutron star binary 4U 1700+24

A. Tiengo, D. K. Galloway, T. di Salvo +4

We present the spectral analysis of an XMM-Newton observation of the X-ray binary 4U 1700+24, performed during an outburst in August 2002. The EPIC-PN spectrum above 1 keV can be m…

astro-ph2005

A broad iron line in the Chandra/HETG spectrum of 4U 1705-44

T. Di Salvo, R. Iaria, M. Mendez +5

We present the results of a Chandra 30 ks observation of the low mass X-ray binary and atoll source 4U 1705-44. Here we concentrate on the study of discrete features in the energy…

astro-ph2004

X-ray spectroscopy on Abell 478 with XMM-Newton

J. de Plaa, J. S. Kaastra, T. Tamura +3

We report the results from a spatially resolved spectroscopy study with XMM-Newton on the relaxed cluster of galaxies Abell 478. From the EPIC data we extract a temperature profile…

astro-ph2003

MS 1603.6+2600: an Accretion Disc Corona source?

P. G. Jonker, M. van der Klis, C. Kouveliotou +3

We have observed the eclipsing low-mass X-ray binary MS1603.6+2600 with Chandra for 7 ksec. The X-ray spectrum is well fit with a single absorbed powerlaw with an index of ~2. We f…