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J. Cotzomi

Researcher at Benemérita Universidad Autónoma de Puebla

Publications -  46
Citations -  2465

J. Cotzomi is an academic researcher from Benemérita Universidad Autónoma de Puebla. The author has contributed to research in topics: Observatory & Cherenkov radiation. The author has an hindex of 15, co-authored 30 publications receiving 2062 citations.

Papers
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Properties and performance of the prototype instrument for the Pierre Auger Observatory

J. Abraham, +356 more
TL;DR: The first phase of the Pierre Auger Observatory has been completed and all of the sub-systems that will be used in the full instrument to be tested under field conditions as discussed by the authors.
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Extended gamma-ray sources around pulsars constrain the origin of the positron flux at Earth

Anushka Udara Abeysekara, +116 more
- 17 Nov 2017 - 
TL;DR: In this paper, the authors reported the detection, using the High-Altitude Water Cherenkov Observatory (HAWC), of extended tera-electron volt gamma-ray emission coincident with the locations of two nearby middle-aged pulsars (Geminga and PSR B0656+14).
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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.