activity
20092013
most citedA double-peaked outburst of A 0535+26 observed with INTEGRAL, RXTE, and Suzaku

37 citations · 37 across the 1 of their papers we have counts for

collaborators

11 papers

astro-ph.HE2013★ 37 cited

A double-peaked outburst of A 0535+26 observed with INTEGRAL, RXTE, and Suzaku

I. Caballero, K. Pottschmidt, D. M. Marcu +18

The Be/X-ray binary A 0535+26 showed a normal (type I) outburst in August 2009. It is the fourth in a series of normal outbursts associated with the periastron, but is unusual by p…

astro-ph.HE2011

Study of the many fluorescent lines and the absorption variability in GX 301-2 with XMM-Newton

F. Fuerst, S. Suchy, I. Kreykenbohm +7

We present an in-depth study of the High Mass X-ray Binary (HMXB) GX 301-2 during its pre-periastron flare using data from the XMM-Newton satellite. The energy spectrum shows a pow…

astro-ph.HE2011

The Be/X-ray binary A0535+26 during its recent 2009/2010 outbursts

I. Caballero, K. Pottschmidt, A. Santangelo +20

The Be/X-ray binary A0535+26 showed a giant outburst in December 2009 that reached ~5.14 Crab in the 15-50 keV range. Unfortunately, due to Sun constraints it could not be observed…

astro-ph.HE2011

X-ray Spectroscopy of MXB 1728-34 with XMM-Newton

Elise Egron, Tiziana Di Salvo, Luciano Burderi +8

We have analysed an XMM-Newton observation of the low mass X-ray binary and atoll source MXB 1728-34. The source was in a low luminosity state during the XMM-Newton observation, co…

astro-ph.HE2011

Suzaku observations of the HMXB 1A 1118-61

Slawomir Suchy, Katja Pottschmidt, Richard E. Rothschild +12

We present broad band analysis of the Be/X-ray transient 1A 1118-61 by Suzaku at the peak of its 3rd observed outburst in January 2009 and 2 weeks later when the source flux had de…

astro-ph.HE2010

4U 1909+07: a well-hidden pearl

F. Fuerst, I. Kreykenbohm, S. Suchy +4

We present the first detailed spectral and timing analysis of the High Mass X-ray Binary (HMXB) 4U 1909+07 with INTEGRAL and RXTE. 4U 1909+07 is detected in the ISGRI 20-40 keV ene…