activity
20052026
most citedSpectroscopic identification of r-process nucleosynthesis in a double neutron star merger

1k citations · 1k across the 7 of their papers we have counts for

collaborators

8 papers

astro-ph.HE2026

Failed jet breakout in the metal-poor broad-lined type Ic supernova 2026gzf

Antonio Martin-Carrillo, Christina C. Thöne, James K. Leung +103

A long-standing question in the death of massive stars is the role of relativistic jets. While many gamma-ray bursts and some fast X-ray transients seem to be associated with broad…

astro-ph.HE2026★ 1 cited

GRB 210704A: A Luminous Fast Blue Transient in a GRB Afterglow at

Daniëlle L. A. Pieterse, Andrew J. Levan, Maria E. Ravasio +27

We present detailed, multi-wavelength analysis of GRB 210704A: a Fermi Gamma-ray Burst Monitor discovered and Fermi Large Area Telescope (LAT) detected gamma-ray burst (GRB). The b…

astro-ph.HE2025★ 1 cited

EP 250108a/SN 2025kg: Observations of the most nearby Broad-Line Type Ic Supernova following an Einstein Probe Fast X-ray Transient

J. C. Rastinejad, A. J. Levan, P. G. Jonker +66

With a small sample of fast X-ray transients (FXTs) with multi-wavelength counterparts discovered to date, the progenitors of FXTs and their connections to gamma-ray bursts (GRBs)…

astro-ph.IM2017★ 8 cited

MAORY science cases white book

G. Fiorentino, M. Bellazzini, P. Ciliegi +9

MAORY is the Adaptive Optic (AO) module that will be installed at the E-ELT at the first light of the telescope. It will provide two different types of AO correction, a very high c…

astro-ph.HE2017★ 1k cited

Spectroscopic identification of r-process nucleosynthesis in a double neutron star merger

E. Pian, P. D'Avanzo, S. Benetti +81

The merger of two neutron stars is predicted to give rise to three major detectable phenomena: a short burst of gamma-rays, a gravitational wave signal, and a transient optical/nea…

astro-ph.HE2009★ 1 cited

Properties of Gamma Ray Bursts at different redshifts

G. Pizzichini, E. Maiorano, M. Genghini +1

GRBs are now detected up to z = 8.26 . We try to find differences, in their restframe properties, which could be related either to distance or to observing conditions.

astro-ph2005

The GRB of 1999 January 23: prompt emission and broad-band afterglow modeling

A. Corsi, L. Piro, E. Kuulkers +13

We report on BeppoSAX simultaneous X- and gamma-ray observations of the bright gamma-ray burst (GRB) 990123. We present the broad-band spectrum of the prompt emission, including op…

astro-ph2005

GRB990123: multiwavelength afterglow study

E. Maiorano, N. Masetti, E. Palazzi +13

We report on the BeppoSAX and multiwavelength data analysis of the afterglow of Gamma-Ray Burst (GRB) 990123. Mainly due to its exceptional brightness, this is the only source for…