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most citedExtended gamma-ray sources around pulsars constrain the origin of the positron flux at Earth

528 citations · 3.7k across the 96 of their papers we have counts for

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11 papers · 1 filter

astro-ph.HE2017★ 528 cited

Extended gamma-ray sources around pulsars constrain the origin of the positron flux at Earth

A. U. Abeysekara, A. Albert, R. Alfaro +113

The unexpectedly high flux of cosmic ray positrons detected at Earth may originate from nearby astrophysical sources, dark matter, or unknown processes of cosmic-ray secondary prod…

astro-ph.HE2017★ 65 cited

A Search for Dark Matter in the Galactic Halo with HAWC

A. U. Abeysekara, A. M. Albert, R. Alfaro +100

The High Altitude Water Cherenkov (HAWC) gamma-ray observatory is a wide field-of-view observatory sensitive to 500 GeV - 100 TeV gamma rays and cosmic rays. With its observations…

astro-ph.HE2017★ 93 cited

All-particle cosmic ray energy spectrum measured by the HAWC experiment from 10 to 500 TeV

HAWC Collaboration, R. Alfaro, C. Alvarez +98

We report on the measurement of the all-particle cosmic ray energy spectrum with the High Altitude Water Cherenkov (HAWC) Observatory in the energy range 10 to 500 TeV. HAWC is a g…

astro-ph.HE2017★ 6 cited

HAWC Contributions to the 35th International Cosmic Ray Conference (ICRC2017)

A. U. Abeysekara, A. Albert, R. Alfaro +123

List of proceedings from the HAWC Collaboration presented at the 35th International Cosmic Ray Conference, 12 July - 20 July 2017, Bexco, Busan, Korea.

astro-ph.HE2017

Spectral analysis of Markarian 421 and Markarian 501 with HAWC

S. Coutiño de León, A. Carramiñana, D. Rosa-González

The Hight Altitude Water Cherenkov (HAWC) Gamma-Ray Observatory monitors the gamma-ray sky in the energy range from 100 GeV to 100 TeV and has detected two very high energy (VHE) b…

astro-ph.HE2017★ 110 cited

Dark Matter Limits From Dwarf Spheroidal Galaxies with The HAWC Gamma-Ray Observatory

A. Albert, R. Alfaro, C. Alvarez +78

The High Altitude Water Cherenkov (HAWC) gamma-ray observatory is a wide field of view observatory sensitive to 500 GeV - 100 TeV gamma rays and cosmic rays. It can also perform di…