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Lara Nava

Researcher at INAF

Publications -  94
Citations -  4026

Lara Nava is an academic researcher from INAF. The author has contributed to research in topics: Gamma-ray burst & Fermi Gamma-ray Space Telescope. The author has an hindex of 32, co-authored 79 publications receiving 3441 citations. Previous affiliations of Lara Nava include International School for Advanced Studies & Istituto Nazionale di Fisica Nucleare.

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GeV emission from gamma‐ray bursts: a radiative fireball?

TL;DR: In this paper, the authors studied the gamma-ray burst emission observed at energies > 100 MeV by the Fermi-Large Area Telescope (LAT) until 2009 October and showed that the observed > 0.1 GeV flux can be interpreted as afterglow emission shortly following the start of the prompt phase emission as seen at smaller frequencies.
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A complete sample of bright swift long gamma-ray bursts. I. Sample presentation, luminosity function and evolution

TL;DR: In this paper, a carefully selected sub-sample of Swift long gamma-ray bursts (GRBs) that is complete in redshift was constructed by considering only bursts with favorable observing conditions for ground-based follow-up searches, which are bright in the 15-150 keV Swift/BAT band, i.e., with 1-s peak photon fluxes in excess to 2.6 photons s{sup −1} cm{sup -2}.
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Compact radio emission indicates a structured jet was produced by a binary neutron star merger

TL;DR: In this paper, the authors present very-long-baseline interferometry observations, performed 207.4 days after the binary neutron star merger event GW170817, using a global network of 32 radio telescopes.
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Spectral properties of 438 GRBs detected by Fermi/GBM

TL;DR: In this paper, the authors presented the results of the spectral analysis of the public data of 438 gamma ray bursts (GRBs) detected by the Fermi Gamma ray Burst Monitor (GBM) up to March 2010.
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A complete sample of bright Swift long gamma-ray bursts: testing the spectral-energy correlations

TL;DR: In this article, the authors used a nearly complete sample of Gamma Ray Bursts (GRBs) detected by the Swift satellite to study the correlations between the spectral peak energy Epeak of the prompt emission, the isotropic energetics Eiso and the Epeak luminosity Liso.