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M. Perri

86 papers hereh-index 6522.4k citations452 works total

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

author position
  • first author3
  • middle author51
  • last author3

Across the 57 of 86 papers where every author was matched, so the position is known.

fields
  • astro-ph48
  • astro-ph.HE29
  • astro-ph.IM9
same name
  • M. Perri — 46 papers
  • M. Perri — 4 papers
  • M. Perri — 1 paper, h 3
  • M. Perri — 1 paper
  • M. Perri — 1 paper
  • M. Perri — 1 paper

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
19982022
most citedAn online repository of Swift/XRT light curves of GRBs

903 citations · 4.6k across the 57 of their papers we have counts for

collaborators
Showing 2018Show all

3 papers · 1 filter

astro-ph.HE2018

Authenticating the Presence of a Relativistic Massive Black Hole Binary in OJ 287 Using its General Relativity Centenary Flare: Improved Orbital Parameters

Lankeswar Dey, M. J. Valtonen, A. Gopakumar +5

Results from regular monitoring of relativistic compact binaries like PSR 1913+16 are consistent with the dominant (quadrupole) order emission of gravitational waves (GWs). We show…

astro-ph.HE2018

The extreme HBL behaviour of Markarian 501 during 2012

M. L. Ahnen, S. Ansoldi, L. A. Antonelli +276

A multiwavelength campaign was organized to take place between March and July of 2012. Excellent temporal coverage was obtained with more than 25 instruments, including the MAGIC,…

astro-ph.HE2018

The Bright γ-ray Flare of 3C 279 in June 2015: AGILE Detection and Multifrequency Follow-up Observations

C. Pittori, F. Lucarelli, F. Verrecchia +44

We report the AGILE detection and the results of the multifrequency follow-up observations of a bright γ-ray flare of the blazar 3C 279 in June 2015. We use AGILE-GRID and Fermi-…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.