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Ruben Alfaro

Researcher at National Autonomous University of Mexico

Publications -  103
Citations -  2513

Ruben Alfaro is an academic researcher from National Autonomous University of Mexico. The author has contributed to research in topics: Observatory & Cherenkov radiation. The author has an hindex of 23, co-authored 102 publications receiving 1839 citations.

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MonographDOI

Science with the Cherenkov Telescope Array

B. S. Acharya, +580 more
TL;DR: The Cherenkov Telescope Array (CTA) as mentioned in this paper is the major global observatory for very high energy gamma-ray astronomy over the next decade and beyond, covering a huge range in photon energy from 20 GeV to 300 TeV.
Journal ArticleDOI

Sensitivity of the high altitude water Cherenkov detector to sources of multi-TeV gamma rays

Anushka Udara Abeysekara, +103 more
TL;DR: The High Altitude Water Cherenkov (HAWC) observatory as mentioned in this paper is an array of large water-cherenkov detectors sensitive to gamma rays and hadronic cosmic rays in the energy band between 100 GeV and 100 TeV.
Journal ArticleDOI

Multiple Galactic Sources with Emission Above 56 TeV Detected by HAWC

Anushka Udara Abeysekara, +104 more
TL;DR: This first catalog of gamma-ray sources emitting above 56 and 100 TeV with data from the High Altitude Water Cherenkov Observatory, a wide field-of-view observatory capable of detecting gamma rays up to a few hundred TeV, is presented.
Journal ArticleDOI

Measurement of the Crab Nebula Spectrum Past 100 TeV with HAWC

Anushka Udara Abeysekara, +104 more
TL;DR: In this paper, the authors used two independent energy-estimation methods that utilize extensive air shower variables such as the core position, shower angle, and shower lateral energy distribution to estimate the gamma-ray energy of the Crab Nebula.
Journal ArticleDOI

OBSERVATION OF SMALL-SCALE ANISOTROPY IN THE ARRIVAL DIRECTION DISTRIBUTION OF TeV COSMIC RAYS WITH HAWC

Anushka Udara Abeysekara, +107 more
TL;DR: In this article, an analysis of the cosmic-ray arrival direction distribution based on 4.9 × 1010 events recorded between 2013 June and 2014 February shows anisotropy at the 10−4 level on angular scales of about 10°.