activity
20042009
most citedThe 3rd IBIS/ISGRI soft gamma-ray survey catalog

308 citations · 917 across the 16 of their papers we have counts for

collaborators

16 papers

astro-ph.GA2009★ 54 cited

Hard X-ray properties of magnetic cataclysmic variables

S. Scaringi, A. J. Bird, A. J. Norton +10

Hard X-ray surveys have proven remarkably efficient in detecting intermediate polars and asynchronous polars, two of the rarest type of cataclysmic variable (CV). Here we present a…

astro-ph.SR2009★ 10 cited

RXTE confirmation of the intermediate polar status of IGR J15094-6649

O. W. Butters, A. J. Norton, K. Mukai +1

Aims. To establish the X-ray properties of the intermediate polar candidate IGR J15094-6649 and therefore confirm its inclusion into the class. Methods. 42 856 s of X-ray data from…

astro-ph2008★ 35 cited

RXTE determination of the intermediate polar status of XSS J00564+4548, IGR J17195-4100, and XSS J12270-4859

O. W. Butters, A. J. Norton, P. Hakala +2

Aims: We determine the nature of the intermediate polar candidates XSS J00564+4548, IGR J17195-4100, and XSS J12270-4859. Methods: Pointed RXTE observations searched for intermedia…

astro-ph2007★ 19 cited

RXTE confirmation of the Intermediate Polar status of Swift J0732.5-1331

O. W. Butters, E. J. Barlow, A. J. Norton +1

Aims. We intend to establish the X-ray properties of Swift J0732.5-1331 and therefore confirm its status as an intermediate polar. Method. We analysed 36,240 s of X-ray data from R…

astro-ph2006★ 308 cited

The 3rd IBIS/ISGRI soft gamma-ray survey catalog

A. J. Bird, A. Malizia, A. Bazzano +20

In this paper we report on the third soft gamma-ray source catalog obtained with the IBIS/ISGRI gamma-ray imager on board the INTEGRAL satellite. The scientific dataset is based on…

astro-ph2006★ 15 cited

INTEGRAL and Swift observations of the supergiant fast X-ray transient AXJ1845.0-0433=IGRJ18450-0435

V. Sguera, A. J. Bird, A. J. Dean +8

Context: AXJ1845.0-0433 was discovered by ASCA in 1993 during fast outburst activity characterized by several flares on short timescales. Up to now, the source was not detected aga…