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researcher

S. Mereghetti

188 papers hereh-index 6118.3k citations1k works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • sole author6
  • first author19
  • middle author99
  • last author17

Across the 141 of 188 papers where every author was matched, so the position is known.

fields
  • astro-ph103
  • astro-ph.HE71
  • astro-ph.IM11
  • astro-ph.SR2
  • physics.space-ph1
same name
  • S. Mereghetti — 40 papers
  • S. Mereghetti — 38 papers, h 21
  • S. Mereghetti — 6 papers, h 9

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

activity
19962022
most citedINTEGRAL Detection of the First Prompt Gamma-Ray Signal Coincident with the Gravitational Wave Event GW170817

916 citations · 4.7k across the 111 of their papers we have counts for

collaborators
Showing 2013Show all

4 papers · 1 filter

astro-ph.HE2013★ 1 cited

Ten years of the INTEGRAL Burst Alert System (IBAS)

Sandro Mereghetti

The INTEGRAL Burst Alert System (IBAS) has been developed to detect and locate in real time the gamma-ray bursts (GRBs) serendipitously observed by INTEGRAL. The IBAS software runs…

astro-ph.HE2013★ 66 cited

Variable gamma-ray emission from the Crab Nebula: short flares and long "waves"

E. Striani, M. Tavani, V. Vittorini +22

Gamma-ray emission from the Crab Nebula has been recently shown to be unsteady. In this paper, we study the flux and spectral variability of the Crab above 100 MeV on different tim…

astro-ph.HE2013

GOLIA: an INTEGRAL archive at INAF-IASF Milano

A. Paizis, S. Mereghetti, D. Götz +5

We present the archive of the INTEGRAL data developed and maintained at INAF-IASF Milano. The archive comprises all the public data currently available (revolutions 0026-1079, i.e.…

astro-ph.HE2013★ 3 cited

Blackbody excess in persistent Be pulsars

N. La Palombara, S. Mereghetti, L. Sidoli +2

We report on the main results obtained thanks to an observation campaign, performed with XMM-Newton, of four persistent, low-luminosity (Lx ~ 10^34 erg/s) and long-period (P > 200…

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