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S

S. Hernandez

Researcher at National Autonomous University of Mexico

Publications -  65
Citations -  2067

S. Hernandez 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 22, co-authored 51 publications receiving 1566 citations.

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The 2HWC HAWC Observatory Gamma-Ray Catalog

Anushka Udara Abeysekara, +112 more
TL;DR: In this article, the authors presented the first catalog of TeV gamma-ray sources realized with data from the newly completed High Altitude Water Cherenkov Observatory (HAWC), which is the most sensitive wide field-of-view TeV telescope currently in operation, with a one-year survey sensitivity of ∼5% of the flux of the Crab Nebula.
Journal ArticleDOI

Observation of the Crab Nebula with the HAWC Gamma-Ray Observatory

Anushka Udara Abeysekara, +106 more
TL;DR: Abeysekara et al. as discussed by the authors presented a time-integrated analysis of the Crab using 507 live days of HAWC data from 2014 November to 2016 June.
Journal ArticleDOI

The 2HWC HAWC Observatory Gamma Ray Catalog

Anushka Udara Abeysekara, +110 more
TL;DR: In this paper, the authors presented a catalog of TeV gamma-ray sources realized with the recently completed High Altitude Water Cherenkov Observatory (HAWC), which is the most sensitive wide field-of-view TeV telescope currently in operation, with a 1-year survey sensitivity of ~5-10% of the flux of the Crab Nebula.
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.