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Blog Archives

February 7, 2014 by Lars Mohrmann

H.E.S.S. observations of the Crab during its March 2013 GeV gamma-ray flare

Context. On March 4, 2013 the Fermi-LAT and AGILE reported a flare from the direction of the Crab nebula in which the high-energy (HE; E > 100 MeV) flux was six times above its quiescent level.…

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February 6, 2014 by Lars Mohrmann

HESS J1818–154, a new composite supernova remnant discovered in TeV gamma rays and X-rays

Composite supernova remnants (SNRs) constitute a small subclass of the remnants of massive stellar explosions where non-thermal radiation is observed from both the expanding shell-like shock front and from a pulsar wind nebula (PWN)…

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December 20, 2013 by Lars Mohrmann

Long-term TeV and X-Ray Observations of the Gamma-Ray Binary HESS J0632+057

HESS J0632+057 is the only gamma-ray binary known so far whose position in the sky allows observations with ground-based observatories in both the northern and southern hemispheres. Here we report on long-term observations of…

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November 27, 2013 by Lars Mohrmann

Discovery of very high energy γ-ray emission from the BL Lacertae object PKS 0301−243 with H.E.S.S.

The active galactic nucleus PKS 0301−243 (z = 0.266) is a high-synchrotron-peaked BL Lac object that is detected at high energies (HE, 100 MeV <E < 100 GeV) by Fermi/LAT. This paper reports on the discovery of PKS 0301−243 at very…

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November 20, 2013 by Lars Mohrmann

Constraints on axionlike particles with H.E.S.S. from the irregularity of the PKS 2155–304 energy spectrum

Axionlike particles (ALPs) are hypothetical light (sub-eV) bosons predicted in some extensions of the Standard Model of particle physics. In astrophysical environments comprising high-energy gamma rays and turbulent magnetic fields, the existence of ALPs…

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August 1, 2013 by Lars Mohrmann

HESS and Fermi-LAT discovery of γ-rays from the blazar 1ES 1312−423

A deep observation campaign carried out by the High Energy Stereoscopic System (HESS) on Centaurus A enabled the discovery of γ-rays from the blazar 1ES 1312−423, 2° away from the radio galaxy. With a differential…

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June 12, 2013 by Lars Mohrmann

H.E.S.S. discovery of VHE γ-rays from the quasar PKS 1510−089

The quasar PKS 1510−089 (z = 0.361) was observed with the H.E.S.S. array of imaging atmospheric Cherenkov telescopes during high states in the optical and GeV bands, to search for very high energy (VHE, defined as E ≥ 0.1 TeV)…

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June 5, 2013 by Lars Mohrmann

Discovery of high and very high-energy emission from the BL Lacertae object SHBL J001355.9–185406

The detection of the high-frequency peaked BL Lac object (HBL) SHBL J001355.9–185406 (z = 0.095) at high (HE; 100 MeV < E < 300 GeV) and very high-energy (VHE; E > 100 GeV) with the Fermi Large Area Telescope (LAT) and the…

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April 11, 2013 by Lars Mohrmann

Discovery of TeV γ-ray emission from PKS 0447–439 and derivation of an upper limit on its redshift

Very high-energy γ-ray emission from PKS 0447−439 was detected with the H.E.S.S. Cherenkov telescope array in December 2009. This blazar is one of the brightest extragalactic objects in the Fermi bright source list and has…

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March 1, 2013 by Lars Mohrmann

H.E.S.S. observations of the binary system PSR B1259-63/LS 2883 around the 2010/2011 periastron passage

Aims. We present very high energy (VHE; E > 100 GeV) data from the γ-ray binary system PSR B1259-63/LS 2883 taken around its periastron passage on 15th of December 2010 with the High Energy Stereoscopic System…

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Browse other months

Recent sources

Too Young to Be This Large: The Puzzling Case of HESS J1813–178January 1, 2026
V4641 Sagittarii – the not-so-unremarkable microquasarDecember 1, 2025
The Vela Pulsar – the most Highly Energetic ClockNovember 1, 2023
HESS J1645−455 – A gem on the ring?October 1, 2023
The identity crisis of the blazar PKS 1510-089August 1, 2023

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Atmosphere black holes Blazar building Cosmic rays Extragalactic Galactic Center galactic plane galactic source Gamma-ray binary gamma-rays microquasar neutrinos Nova publication pulsar Technical

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Last sources of the month

Too Young to Be This Large: The Puzzling Case of HESS J1813–178January 1, 2026
V4641 Sagittarii – the not-so-unremarkable microquasarDecember 1, 2025
The Vela Pulsar – the most Highly Energetic ClockNovember 1, 2023

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