scispace - formally typeset
P

Pedro Miranda-Romagnoli

Researcher at Universidad Autónoma del Estado de Hidalgo

Publications -  111
Citations -  3003

Pedro Miranda-Romagnoli is an academic researcher from Universidad Autónoma del Estado de Hidalgo. The author has contributed to research in topics: Observatory & Gamma ray. The author has an hindex of 27, co-authored 97 publications receiving 2372 citations. Previous affiliations of Pedro Miranda-Romagnoli include National Institute of Astrophysics, Optics and Electronics.

Papers
More filters
Journal ArticleDOI

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

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

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.