activity
20072026
most citedA double component in GRB 090618: a proto-black hole and a genuinely long GRB

60 citations · 359 across the 24 of their papers we have counts for

collaborators

27 papers

astro-ph.IM2026

HRMOS: a very high-resolution, multi-object spectrograph for the ESO VLT

Andrea Bianco, Sofia Randich, Emma Fernandez Alvar +7

HRMOS (High-Resolution Multi-Object Spectrograph) is a proposed new instrument for the ESO Very Large Telescope (VLT) developed in the context of the ESO VLT Beyond 2030 call. It i…

astro-ph.IM2026

HRMOS: A High-Resolution Multi-Object Spectrograph for the VLT

Laura Magrini, Thomas Bensby, Sofia Randich +174

This White Paper presents the scientific rationale and instrument concept for HRMOS (High-Resolution Multi-Object Spectrograph), a next-generation instrument proposed for the ESO V…

astro-ph.HE2012★ 27 cited

Analysis of GRB 080319B and GRB 050904 within the fireshell model: evidence for a broader spectral energy distribution

Barbara Patricelli, Maria Grazia Bernardini, Carlo Luciano Bianco +5

(Shortened) GRB080319B, with an isotropic energy E_{iso}=1.32x10^{54}erg, and GRB050904, with E_{iso}=1.04x10^{54}erg, offer the possibility of studying the spectral properties of…

astro-ph.HE2012★ 60 cited

A double component in GRB 090618: a proto-black hole and a genuinely long GRB

L. Izzo, R. Ruffini, A. V. Penacchioni +6

The joint X and gamma-ray observations of GRB 090618 by a large number of satellites offer an unprecedented possibility of testing crucial aspects of theoretical models. In particu…

astro-ph.HE2012★ 40 cited

Evidence for a proto-black hole and a double astrophysical component in GRB 101023

A. V. Penacchioni, R. Ruffini, L. Izzo +5

[Shortened] Context: [...] we point out a striking similarity between GRB 101023 and GRB 090618. We explore the possibility that these sources are members of a new GRB family relat…

astro-ph.HE2011

A double component in the prompt emission of GRB 090618

L. Izzo, R. Ruffini, A. V. Penacchioni +6

GRB 090618 offered an unprecedented opportunity to have coordinated data, by the best of the X and Gamma Ray observatories, of the nearest (z = 0.54) energetic source (10 er…