activity
19972020
most citedDiscovery of the short gamma-ray burst GRB 050709

233 citations · 1.1k across the 32 of their papers we have counts for

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Showing astro-ph.HEShow all

10 papers · 1 filter

astro-ph.HE2020★ 13 cited

Broadband X-ray analysis of 1E 1740.7-2942: constraints on spin, inclination and a tentative black hole mass

Paulo E. Stecchini, Flavio D'Amico, Francisco Jablonski +2

1E 1740.7-2942 is one of the strongest hard X-ray emitters in the Galactic Centre region, believed to be a black hole in a high-mass X-ray binary system. Although extensively studi…

astro-ph.HE2017★ 4 cited

Tandem Swift and INTEGRAL Data to Revisit the Orbital and Superorbital Periods of 1E 1740.7-2942

Paulo Eduardo Stecchini, Manuel Castro, Francisco Jablonski +2

The black hole candidate 1E 1740.7-2942 is one of the strongest hard X-ray sources in the Galactic Center region. No counterparts in longer wavelengths have been identified for thi…

astro-ph.HE2015★ 5 cited

Telescope performance and image simulations of the balloon-borne coded-mask protoMIRAX experiment

A. V. Penacchioni, J. Braga, M. A. Castro +1

In this work we present the results of imaging simulations performed with the help of the GEANT4 package for the protoMIRAX hard X-ray balloon experiment. The instrumental backgrou…

astro-ph.HE2015

Flux and spectral variations of 1E1740.72942 over the years 20032012

Manuel Castro, Flavio D'Amico, Francisco Jablonski +1

The black hole system 1E1740.72942 is usually the brightest hard X-ray source (above 20 keV) near the Galactic Center, but presents some epochs of low emission (be…

astro-ph.HE2015★ 6 cited

Probing the emission physics and weak/soft population of Gamma-Ray Bursts with LOFT

L. Amati, G. Stratta, J. -L. Atteia +36

This is a White Paper in support of the mission concept of the Large Observatory for X-ray Timing (LOFT), proposed as a medium-sized ESA mission. We discuss the potential of LOFT f…

astro-ph.HE2014★ 12 cited

Confirming the thermal Comptonization model for black hole X-ray emission in the low-hard state

M. Castro, F. D'Amico, J. Braga +3

Hard X-ray spectra of black hole binaries in the low/hard state are well modeled by thermal Comptonization of soft seed photons by a corona-type region with \thinspace…