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Blog Archives

July 1, 2005 by H.E.S.S. Collaboration

Discovery of the binary pulsar PSR B1259-63 in very-high-energy gamma rays around periastron with H.E.S.S.

We report the discovery of very-high-energy (VHE) gamma-ray emission of the binary system PSR B1259-63/SS 2883 of a radio pulsar orbiting a massive, luminous Be star in a highly eccentric orbit. The observations around…

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July 1, 2005 by H.E.S.S. Collaboration

Observations of Selected AGN with H.E.S.S.

A sample of selected active galactic nuclei (AGN) was observed in 2003 and 2004 with the High Energy Stereoscopic System (H.E.S.S.), an array of imaging atmospheric-Cherenkov telescopes in Namibia. The redshifts of these candidate…

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July 1, 2005 by H.E.S.S. Collaboration

Serendipitous discovery of the unidentified extended TeV gamma-ray source HESS J1303-631

The serendipitous discovery of an unidentified extended TeVgamma-ray source close to the galactic plane named HESS J1303-631 at a significance of 21 standard deviations is reported. The observations were performed between February and June…

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July 1, 2005 by H.E.S.S. Collaboration

Upper limits to the SN1006 multi-TeV gamma-ray flux from H.E.S.S. observations

Observations of the shell-type supernova remnant SN1006 have been carried out with the H.E.S.S. system of Cherenkov telescopes during 2003 (18.2h with two operating telescopes) and 2004 (6.3h with all four telescopes). No evidence…

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July 1, 2005 by H.E.S.S. Collaboration

Observations of Mkn 421 in 2004 with HESS at large zenith angles

Mkn 421 was observed during a high flux state for nine nights in April and May 2004 with the fully operational High Energy Stereoscopic System (H.E.S.S.) in Namibia. The observations were carried out at…

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July 1, 2005 by H.E.S.S. Collaboration

Detection of TeV gamma-ray emission from the shell-type supernova remnant RX J0852.0-4622 with H.E.S.S

We report the detection of TeV gamma-rays from the shell-type supernova remnant RX J0852.0-4622 with data of 3.2 h of live time recorded with H.E.S.S. in February 2004. An excess of (700 +/- 60)…

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July 1, 2005 by H.E.S.S. Collaboration

Discovery of VHE gamma rays from PKS 2005-489

The high-frequency peaked BL Lac PKS 2005-489 (z=0.071) was observed in 2003 and 2004 with the H.E.S.S. stereoscopic array of imaging atmospheric-Cherenkov telescopes in Namibia. A signal was detected at the 6.7 sigma level…

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July 1, 2004 by H.E.S.S. Collaboration

High energy particle acceleration in the shell of a supernova remnant

A significant fraction of the energy density of the interstellar medium is in the form of high-energy charged particles (cosmic rays). The origin of these particles remains uncertain. Although it is generally accepted that…

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July 1, 2004 by H.E.S.S. Collaboration

The trigger system of the H.E.S.S. telescope array

H.E.S.S. — The High Energy Stereoscopic System– is a new system of large atmospheric Cherenkov telescopes for GeV/TeV Gamma-ray astronomy. This paper describes the trigger system of H.E.S.S. with emphasis on the multi-telescope array…

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July 1, 2004 by H.E.S.S. Collaboration

Calibration of cameras of the H.E.S.S. detector

H.E.S.S. – the High Energy Stereoscopic System- is a new system of large atmospheric Cherenkov telescopes for GeV/TeV astronomy. Each of the four telescopes of 107 m^2 mirror area is equipped with a 960-pixel…

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Browse other months

Recent sources

H.E.S.S.’ most distant blazar: PKS 0346−27February 1, 2026
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

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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

H.E.S.S.’ most distant blazar: PKS 0346−27February 1, 2026
Too Young to Be This Large: The Puzzling Case of HESS J1813–178January 1, 2026
V4641 Sagittarii – the not-so-unremarkable microquasarDecember 1, 2025

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