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19952008
most citedDiscovery of the INTEGRAL X/Gamma-ray transient IGR J00291+5934: a Comptonised accreting ms pulsar ?

26 citations · 29 across the 7 of their papers we have counts for

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astro-ph20081 cited

Broad-Band Spectrum of The Black Hole Candidate IGR J17497-2821 Studied with Suzaku

A. Paizis, K. Ebisawa, H. Takahashi +9

The broad-band 1-300 keV Suzaku spectrum of IGR J17497-2821, the X-ray transient discovered by INTEGRAL in September 2006, is presented. Suzaku observed IGR J17497-2821 on Septembe…

astro-ph20082 cited

Iron Emission Lines on the Galactic Ridge Observed with Suzaku

Shigeo Yamauchi, Ken Ebisawa, Yasuo Tanaka +5

In order to elucidate origin of the Galactic Ridge X-ray Emission, we analyzed Suzaku data taken at various regions along the Galactic plane and studied their Fe-K emission line fe…

astro-ph200526 cited

Discovery of the INTEGRAL X/Gamma-ray transient IGR J00291+5934: a Comptonised accreting ms pulsar ?

S. E. Shaw, N. Mowlavi, J. Rodriguez +8

We report the discovery of a high-energy transient with the IBIS/ISGRI detector on board the INTEGRAL observatory. The source, namely IGR J00291+5934, was first detected on 2nd Dec…

astro-ph2004

The INTEGRAL View of the Galactic Nucleus

A. Goldwurm, G. Belanger, P. Goldoni +15

We present the preliminary results of the observational campaign performed in 2003 to study the Galactic Nucleus with INTEGRAL. The mosaicked images obtained with the IBIS/ISGRI co…

astro-ph2004

A Chandra Deep X-ray Exposure on the Galactic Plane and Near Infrared Identification

K. Ebisawa, A. Paizis, T. J. -L. Couvoisier +13

Using the Chandra ACIS-I instruments, we have carried out a deep X-ray observation on the Galactic plane region at (l,b) ~ (28.5, 0.0), where no discrete X-ray sources have been kn…

astro-ph2004

The INTEGRAL LMXRB Monitoring Programme

A. Paizis, T. J. -L. Courvoisier, O. Vilhu +21

Our collaboration is responsible for the study of a sample of 72 low mass X-ray binaries (LMXRB) using the INTEGRAL Core Programme data. In this paper we describe the monitoring pr…