activity
19982021
most citedINTEGRAL Detection of the First Prompt Gamma-Ray Signal Coincident with the Gravitational Wave Event GW170817

916 citations · 1.8k across the 23 of their papers we have counts for

collaborators

26 papers

astro-ph.IM2021

INTEGRAL reloaded: spacecraft, instruments and ground system

Erik Kuulkers, Carlo Ferrigno, Peter Kretschmar +85

ESA's INTErnational Gamma-Ray Astrophysics Laboratory (INTEGRAL) was launched on 17 Oct 2002 at 06:41 CEST. Since then, it has been providing long, uninterrupted observations (up t…

astro-ph.HE2020★ 11 cited

Multi-messenger astronomy with INTEGRAL

C. Ferrigno, V. Savchenko, A. Coleiro +19

At the time of defining the science objectives of the INTernational Gamma-Ray Astrophysics Laboratory (INTEGRAL), such a rapid and spectacular development of multi-messenger astron…

astro-ph.HE2020★ 81 cited

Advances in Understanding High-Mass X-ray Binaries with INTEGRAL and Future Directions

Peter Kretschmar, Felix Fürst, Lara Sidoli +48

High mass X-ray binaries are among the brightest X-ray sources in the Milky Way, as well as in nearby Galaxies. Thanks to their highly variable emissions and complex phenomenology,…

astro-ph.HE2018★ 14 cited

Optical/X-ray correlations during the V404 Cyg June 2015 outburst

J. Alfonso-Garzón, C. Sánchez-Fernández, P. A. Charles +6

We present a multiwavelength analysis of the simultaneous optical and X-ray light curves of the microquasar V404 Cyg during the June 2015 outburst. We have performed a comprehensiv…

astro-ph.HE2017★ 916 cited

INTEGRAL Detection of the First Prompt Gamma-Ray Signal Coincident with the Gravitational Wave Event GW170817

V. Savchenko, C. Ferrigno, E. Kuulkers +20

We report the e INTernational Gamma-ray Astrophysics Laboratory (INTEGRAL) detection of the short gamma-ray burst GRB 170817A (discovered by Fermi-GBM) with a signal-to-noise ratio…

astro-ph.HE2016★ 41 cited

Gamma-Ray emission from SN2014J near maximum optical light

J. Isern, P. Jean, E. Bravo +17

The optical light curve of Type Ia supernovae (SNIa) is powered by thermalized gamma-rays produced by the decay of 56Ni and 56Co, the main radioactive isotopes synthesized by the t…