activity
20172022
most citedModeling the high-energy emission in GRB 110721A and implications on the early multiwavelength and polarimetric observations

31 citations · 77 across the 7 of their papers we have counts for

collaborators

9 papers

astro-ph.HE20213 cited

A source of gamma rays coincident with the shell of the supernova remnant CTB 80

M. Araya, C. Herrera

CTB 80 (G69.0+2.7) is a relatively old (50--80 kyr) supernova remnant (SNR) with a complex radio morphology showing three extended radio arms and a radio and X-ray nebula near the…

astro-ph.HE2020

HAWC and Fermi-LAT Detection of Extended Emission from the Unidentified Source 2HWC J2006+341

A. Albert, R. Alfaro, C. Alvarez +71

The discovery of the TeV point source 2HWC J2006+341 was reported in the second HAWC gamma-ray catalog. We present a follow-up study of this source here. The TeV emission is best d…

astro-ph.HE20209 cited

G279.0+1.1: a new extended source of high-energy gamma rays

Miguel Araya

G279.0+1.1 is a supernova remnant (SNR) with poorly known parameters, first detected as a dim radio source and classified as an evolved system. An analysis of data from the Fermi-L…

astro-ph.HE2019

Exploring the nature of 2HWC J2006+341 with HAWC and Fermi-LAT

Miguel Araya

The High Altitude Water Cherenkov (HAWC) gamma-ray observatory is carrying out a detailed survey of the northern sky at TeV energies. 2HWC J2006+341 is a newly discovered source re…

astro-ph.HE20195 cited

Revealing a new region of gamma-ray emission in the vicinity of HESS J1825-137

M. Araya, A. M. W. Mitchell, R. D. Parsons

HESS J1825-137 is a bright very-high-energy (VHE) gamma-ray source that has been firmly established as a pulsar wind nebula (PWN), and one of the most extended gamma-ray objects wi…

astro-ph.HE2018

Analysis of Fermi-LAT observations, UHECRs and neutrinos from the radio galaxy Centaurus B

N. Fraija, M. Araya, A. Galvan-Gamez +1

Centaurus B (Cen B) is one of the closest and brightest radio-loud galaxy in the southern sky. This radio galaxy, proposed as a plausible candidate for accelerating ultra-high-ener…