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O

O. Martinez

Researcher at Benemérita Universidad Autónoma de Puebla

Publications -  149
Citations -  4463

O. Martinez is an academic researcher from Benemérita Universidad Autónoma de Puebla. The author has contributed to research in topics: Observatory & Cosmic ray. The author has an hindex of 28, co-authored 132 publications receiving 3723 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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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.
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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.
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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.