activity
20032006
most citedINTEGRAL observations of recurrent fast X-ray transient sources

172 citations · 464 across the 13 of their papers we have counts for

collaborators

12 papers

astro-ph2006

The frontier of darkness: the cases of GRB 040223, GRB 040422, GRB 040624

P. D'Avanzo, P. Filliatre, P. Goldoni +23

Understanding the reasons for the faintness of the optical/near-infrared afterglows of the so-called dark bursts is essential to assess whether they form a subclass of GRBs, and he…

astro-ph2005★ 172 cited

INTEGRAL observations of recurrent fast X-ray transient sources

V. Sguera, E. J. Barlow, A. J. Bird +9

Fast X-ray Transients (FXTs) are believed to be non-recurrent bright X-ray sources lasting less than a day and occuring at serendipitous positions, they can best detected and disco…

astro-ph2005★ 11 cited

Detection and analysis of a new INTEGRAL hard X-ray transient, IGR J17285-2922

E. J. Barlow, A. J. Bird, D. J. Clark +10

We present the transient nature of INTEGRAL source IGR J17285-2922, identified from a single period of activity during an IBIS/ISGRI Galactic Centre Deep Exposure in September 2003…

astro-ph2005★ 102 cited

Evidence of polarisation in the prompt gamma-ray emission from GRB 930131 and GRB 960924

D. R. Willis, E. J. Barlow, A. J. Bird +7

The true nature of the progenitor to GRBs remains elusive; one characteristic that would constrain our understanding of the GRB mechanism considerably is gamma-ray polarimetry meas…

astro-ph2005★ 1 cited

INTEGRAL and XMM-Newton observations of the low-luminosity and X-ray rich burst GRB 040223

S. McGlynn, S. McBreen, L. Hanlon +6

GRB 040223 was observed by INTEGRAL and XMM-Newton. GRB 040223 has a peak flux of (1.6+/-0.13) x10^-8 ergs cm^-2 s^-1, a fluence of (4.4+/-0.4)x10^-7 ergs cm^-2 and a steep photon…

astro-ph2005★ 54 cited

INTEGRAL IGR J18135-1751=HESS J1813-178: A new cosmic high energy accelerator from keV to TeV

P. Ubertini, L. Bassani, A. Malizia +10

We report the discovery of a soft gamma ray source, namely IGR J18135-1751, detected with the IBIS imager on board the INTEGRAL satellite. The source is persistent and has a 20-100…