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Andrew M. Taylor

Researcher at Dublin Institute for Advanced Studies

Publications -  197
Citations -  7707

Andrew M. Taylor is an academic researcher from Dublin Institute for Advanced Studies. The author has contributed to research in topics: Cosmic ray & Blazar. The author has an hindex of 47, co-authored 186 publications receiving 6863 citations. Previous affiliations of Andrew M. Taylor include University of Geneva & Max Planck Society.

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Journal ArticleDOI

Acceleration of petaelectronvolt protons in the Galactic Centre

A. Abramowski, +229 more
- 24 Mar 2016 - 
TL;DR: Deep γ-ray observations with arcminute angular resolution of the region surrounding the Galactic Centre are reported, which show the expected tracer of the presence of petaelectronvolt protons within the central 10 parsecs of the Galaxy, and it is proposed that the supermassive black hole Sagittarius A* is linked to this PeVatron.
Journal ArticleDOI

EGMF Constraints from Simultaneous GeV-TeV Observations of Blazars

TL;DR: In this paper, the authors investigate constraints on the EGMF derived from observations of blazars for which TeV observations simultaneous with those by the Fermi telescope were reported.
Journal ArticleDOI

Extragalactic magnetic fields constraints from simultaneous GeV–TeV observations of blazars

TL;DR: In this paper, the EGMF bound on the hidden assumptions it rests upon was derived from the simultaneous GeV-TeV data on the blazars RGB J0710+591, 1ES 0229+200 and 1ES 1218+304.
Journal ArticleDOI

Search for TeV Gamma-ray Emission from GRB 100621A, an extremely bright GRB in X-rays, with H.E.S.S

A. Abramowski, +220 more
TL;DR: In this article, the authors show that the long gamma-ray burst (GRB) 100621A, at the time the brightest X-ray transient ever detected by Swift-XRT in the 0.3-10 keV range, has been observed with the HESS.
Journal ArticleDOI

Search for TeV Gamma-ray Emission from GRB 100621A, an extremely bright GRB in X-rays, with H.E.S.S

A. Abramowski, +214 more
TL;DR: In this paper, the authors show that the long gamma-ray burst (GRB) 100621A, at the time the brightest X-ray transient ever detected by Swift-XRT in the $0.3\textrm{--}10$ keV range, has been observed with the H.E.S. imaging air Cherenkov telescope array, sensitive to gamma radiation in the very high energy (VHE, $>100$ GeV) regime.