activity
20142017
most citedBlack hole lightning due to particle acceleration at subhorizon scales

184 citations · 302 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.HE20173 cited

Cherenkov Telescope Array Contributions to the 35th International Cosmic Ray Conference (ICRC2017)

F. Acero, B. S. Acharya, V. Acín Portella +1137

List of contributions from the Cherenkov Telescope Array Consortium presented at the 35th International Cosmic Ray Conference, July 12-20 2017, Busan, Korea.

astro-ph.GA201610 cited

Multiband Observations of the Quasar PKS 2326-502 during Active and Quiescent Gamma-Ray States in 2010-2012

Michael S. Dutka, Bryce D. Carpenter, Roopesh Ojha +12

Quasi-simultaneous observations of the Flat Spectrum Radio Quasar PKS 2326-502 were carried out in the gamma-ray, X-ray, UV, optical, near-infrared, and radio bands. Thanks to thes…

astro-ph.HE201612 cited

The MHz-peaked radio spectrum of the unusual gamma-ray source PMN J1603-4904

C. Müller, P. R. Burd, R. Schulz +6

Context. The majority of bright extragalactic gamma-ray sources are blazars. Only a few radio galaxies have been detected by Fermi/LAT. Recently, the GHz-peaked spectrum source PKS…

astro-ph.HE2014184 cited

Black hole lightning due to particle acceleration at subhorizon scales

MAGIC Collaboration, J. Aleksić, S. Ansoldi +151

Supermassive black holes with masses of millions to billions of solar masses are commonly found in the centers of galaxies. Astronomers seek to image jet formation using radio inte…

astro-ph.HE201429 cited

5.9 keV Mn K-shell X-ray luminosity from the decay of 55Fe in Type Ia supernova models

I. R. Seitenzahl, A. Summa, F. Krauss +12

We show that the X-ray line flux of the Mn Kalpha line at 5.9 keV from the decay of 55Fe is a promising diagnostic to distinguish between Type Ia supernova (SN Ia) explosion models…

astro-ph.HE201464 cited

TANAMI Blazars in the IceCube PeV Neutrino Fields

F. Krauß, M. Kadler, K. Mannheim +39

The IceCube Collaboration has announced the discovery of a neutrino flux in excess of the atmospheric background. Due to the steeply falling atmospheric background spectrum, events…