output
19922026
most citedObservation of a new particle in the search for the Standard Model Higgs boson with the ATLAS detector at the LHC

10.9k citations

Showing 2015 · astro-ph.HEShow all

10 papers · 2 filters

astro-ph.HE2015★ 11 cited

Multi-Wavelength Observations of GRB 111228A and Implications for the Fireball and its environment

Li-Ping Xin, Yuan-Zhu Wang, Ting-Ting Lin +10

Observations of very early multi-wavelength afterglows are critical to reveal the properties of the radiating fireball and its environment as well as the central engine of gamma-ra…

astro-ph.HE2015★ 96 cited

Energetic Gamma Radiation from Rapidly Rotating Black Holes

Kouichi Hirotani, Hung-Yi Pu

Supermassive black holes are believed to be the central power house of active galactic nuclei. Applying the pulsar outer-magnetospheric particle accelerator theory to black-hole ma…

astro-ph.HE2015★ 219 cited

Resolved Magnetic-Field Structure and Variability Near the Event Horizon of Sagittarius A*

Michael D. Johnson, Vincent L. Fish, Sheperd S. Doeleman +45

Near a black hole, differential rotation of a magnetized accretion disk is thought to produce an instability that amplifies weak magnetic fields, driving accretion and outflow. The…

astro-ph.HE2015★ 396 cited

Dense magnetized plasma associated with a fast radio burst

Kiyoshi Masui, Hsiu-Hsien Lin, Jonathan Sievers +15

Fast Radio Bursts are bright, unresolved, non-repeating, broadband, millisecond flashes, found primarily at high Galactic latitudes, with dispersion measures much larger than expec…

astro-ph.HE2015★ 139 cited

The population of X-ray supernova remnants in the Large Magellanic Cloud

P. Maggi, F. Haberl, P. J. Kavanagh +11

We present a comprehensive X-ray study of the population of supernova remnants (SNRs) in the LMC. Using primarily XMM-Newton, we conduct a systematic spectral analysis of LMC SNRs…

astro-ph.HE2015★ 143 cited

Teraelectronvolt pulsed emission from the Crab pulsar detected by MAGIC

MAGIC Collaboration, S. Ansoldi, L. A. Antonelli +139

Aims: To investigate the extension of the very-high-energy spectral tail of the Crab pulsar at energies above 400 GeV. Methods: We analyzed 320 hours of good quality data of…