activity
20082025
most citedSearch for a Dark Matter annihilation signal from the Galactic Center halo with H.E.S.S

270 citations · 3.3k across the 65 of their papers we have counts for

collaborators
Showing astro-ph.HEShow all

43 papers · 1 filter

astro-ph.HE2021★ 11 cited

A Search for the 3.5 keV Line from the Milky Way's Dark Matter Halo with HaloSat

E. M. Silich, K. Jahoda, L. Angelini +5

Previous detections of an X-ray emission line near 3.5 keV in galaxy clusters and other dark matter-dominated objects have been interpreted as observational evidence for the decay…

astro-ph.HE2021★ 9 cited

A HaloSat Analysis of the Cygnus Superbubble

Jesse Bluem, Philip Kaaret, William Fuelberth +5

The Cygnus Superbubble (CSB) is a region of soft X-ray emission approximately 13 degrees wide in the direction of the local spiral arm. Such a large region might be the result of s…

astro-ph.HE2020★ 7 cited

Global X-Ray Properties of the Vela and Puppis A Supernova Remnants

E. M. Silich, P. Kaaret, A. Zajczyk +5

The Vela and Puppis A supernova remnants (SNRs) comprise a large emission region of diameter in the soft X-ray sky. The HaloSat CubeSat mission provides the first…

astro-ph.HE2014★ 22 cited

A Search for Pulsations from Geminga Above 100 GeV with VERITAS

E. Aliu, S. Archambault, A. Archer +81

We present the results of 71.6 hours of observations of the Geminga pulsar (PSR J0633+1746) with the VERITAS very-high-energy gamma-ray telescope array. Data taken with VERITAS bet…

astro-ph.HE2014★ 27 cited

Discovery of the VHE gamma-ray source HESS J1832-093 in the vicinity of SNR G22.7-0.2

H. E. S. S. Collaboration, :, A. Abramowski +218

The region around the supernova remnant (SNR) W41 contains several TeV sources and has prompted the H.E.S.S. Collaboration to perform deep observations of this field of view. This…

astro-ph.HE2014★ 75 cited

Multiwavelength observations of Mrk 501 in 2008

MAGIC Collaboration, J. Aleksić, S. Ansoldi +256

Mrk 501 is one of the brightest blazars at TeV energies and has been extensively studied since its first VHE detection in 1996. Our goal is to characterize in detail the source gam…