activity
19982026
most citedThe Neutron Stars of Soft X-Ray Transients

257 citations · 2.9k across the 77 of their papers we have counts for

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Showing 2010Show all

8 papers · 1 filter

astro-ph.HE2010★ 2 cited

Probing the very high redshift Universe with Gamma-ray Bursts: prospects for observations with future X-ray instruments

S. Campana, R. Salvaterra, G. Tagliaferri +2

Gamma-Ray Bursts (GRBs) are the most violent explosions in the Universe. Long duration GRBs are associated with the collapse of massive stars, rivaling their host galaxies in lumin…

astro-ph.IM2010★ 13 cited

LOFT - a Large Observatory For x-ray Timing

M. Feroci, L. Stella, A. Vacchi +46

The high time resolution observations of the X-ray sky hold the key to a number of diagnostics of fundamental physics, some of which are unaccessible to other types of investigatio…

astro-ph.HE2010★ 28 cited

Challenging GRB models through the broadband dataset of GRB060908

S. Covino, S. Campana, M. L. Conciatore +37

Context: Multiwavelength observations of gamma-ray burst prompt and afterglow emission are a key tool to disentangle the various possible emission processes and scenarios proposed…

astro-ph.HE2010★ 55 cited

The 2008 October Swift detection of X-ray bursts/outburst from the transient SGR-like AXP 1E 1547.0-5408

G. L. Israel, P. Esposito, N. Rea +17

We report on the detailed study of the 2008 October outburst from the anomalous X-ray pulsar (AXP) 1E 1547.0-5408 discovered through the Swift/Burst Alert Telescope (BAT) detection…

astro-ph.HE2010★ 37 cited

The supergiant fast X-ray transients XTE J1739-302 and IGR J08408-4503 in quiescence with XMM-Newton

E. Bozzo, L. Stella, C. Ferrigno +5

Context. Supergiant fast X-ray transients are a subclass of high mass X-ray binaries that host a neutron star accreting mass from the wind of its OB supergiant companion. They are…

astro-ph.HE2010★ 26 cited

INTEGRAL, Swift, and RXTE observations of the 518 Hz accreting transient pulsar Swift J1749.4-2807

C. Ferrigno, E. Bozzo, M. Falanga +7

The burst-only Swift J1749.4-2807 source was discovered in a high X-ray-active state, while during an {INTEGRAL observations of the Galactic bulge on 2010 April 10. Pulsations at 5…