activity
19972021
most citedA detailed spectral and morphological study of the gamma-ray supernova remnant RX J1713.7-3946 with H.E.S.S

311 citations · 875 across the 10 of their papers we have counts for

collaborators

10 papers

astro-ph.HE2021★ 15 cited

Peculiar X-ray transient SRGA J043520.9+552226/AT2019wey discovered with SRG/ART-XC

I. A. Mereminskiy, A. V. Dodin, A. A. Lutovinov +24

Context: During the ongoing all-sky survey, the Mikhail Pavlinsky ART-XC telescope on board the SRG observatory should discover new X-ray sources, many of which can be transient. H…

astro-ph.CO2009★ 91 cited

Discovery of Very High Energy gamma-rays from the blazar S5 0716+714

H. Anderhub

The MAGIC collaboration reports the detection of the blazar S5 0716+714 z=0.31+-0.08 in very high energy gamma-rays. The observations were performed in November 2007 and in April 2…

astro-ph2008★ 140 cited

Fermi LAT Observations of the Vela Pulsar

A. A. Abdo

The Vela pulsar is the brightest persistent source in the GeV sky and thus is the traditional first target for new gamma-ray observatories. We report here on initial Fermi Large Ar…

astro-ph2007★ 111 cited

Discovery of Very High Energy gamma-rays from 1ES 1011+496 at z=0.212

MAGIC Collaboration, J. Albert

We report on the discovery of Very High Energy (VHE) gamma-ray emission from the BL Lacertae object 1ES1011+496. The observation was triggered by an optical outburst in March 2007…

astro-ph2005★ 176 cited

Observation of Gamma Rays from the Galactic Center with the MAGIC Telescope

J. Albert, MAGIC collaboration

Recently, the Galactic Center has been reported to be a source of very high energy (VHE) gamma-rays by the VERITAS, CANGAROO and HESS experiments. The energy spectra as measured by…

astro-ph2005★ 311 cited

A detailed spectral and morphological study of the gamma-ray supernova remnant RX J1713.7-3946 with H.E.S.S

The HESS Collaboration, F. Aharonian

We present results from deep observations of the Galactic shell-type supernova remnant (SNR) RX J1713.7-3946 (also known as G347.3-0.5) conducted with the complete H.E.S.S. array i…