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M. Sutherland

114 papers hereh-index 7020.3k citations194 works total

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

author position
  • first author2
  • middle author25
  • last author3

Across the 30 of 114 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE83
  • astro-ph.IM14
  • hep-ex12
  • hep-ph2
  • astro-ph1
  • astro-ph.CO1
same name
  • M. Sutherland — 33 papers, h 19
  • M. Sutherland — 8 papers, h 8
  • M. Sutherland — 7 papers
  • M. Sutherland — 4 papers, h 3
  • M. Sutherland — 4 papers, h 3
  • M. Sutherland — 1 paper, h 2

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
20072021
most citedMulti-messenger observations of a flaring blazar coincident with high-energy neutrino IceCube-170922A

1.1k citations · 12k across the 112 of their papers we have counts for

collaborators
Showing 2012 · astro-ph.IMShow all

3 papers · 2 filters

astro-ph.IM2012★ 148 cited

Antennas for the Detection of Radio Emission Pulses from Cosmic-Ray induced Air Showers at the Pierre Auger Observatory

P. Abreu, M. Aglietta, M. Ahlers +512

The Pierre Auger Observatory is exploring the potential of the radio detection technique to study extensive air showers induced by ultra-high energy cosmic rays. The Auger Engineer…

astro-ph.IM2012★ 35 cited

The Rapid Atmospheric Monitoring System of the Pierre Auger Observatory

The Pierre Auger Collaboration, P. Abreu, M. Aglietta +508

The Pierre Auger Observatory is a facility built to detect air showers produced by cosmic rays above 10^17 eV. During clear nights with a low illuminated moon fraction, the UV fluo…

astro-ph.IM2012★ 3 cited

A Method for Constraining Cosmic Magnetic Field Models Using Ultra-High Energy Cosmic Rays: The Field Scan Method

Michael S. Sutherland, Brian M. Baughman, James J. Beatty

The Galactic magnetic field, locally observed to be on the order of a few μG, is sufficiently strong to induce deflections in the arrival directions of ultra-high energy cosmic r…

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