R. Cornils

Primary particle acceleration above 100 TeV in the shell-type supernova remnant RX J1713.7 − 3946 with deep H.E.S.S. observations (Corrigendum)

F. Aharonian, A. G. Akhperjanian, A. R. Bazer‐Bachi, M. Beilicke et autres

International audience

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Erratum to “Observations of the Sagittarius dwarf galaxy by the HESS experiment and search for a dark matter signal” [Astropart. Phys. 29(1) (2008) 55–62]

F. Aharonian, A. G. Akhperjanian, A. R. Bazer‐Bachi, M. Beilicke et autres

de, am, ch, fr, gb, Afrique du Sud, ie, cz, au (code pays fourni par la source)

HESS OBSERVATIONS OF THE PROMPT AND AFTERGLOW PHASES OF GRB 060602B

F. Aharonian, A. G. Akhperjanian, U. Barres de Almeida, A. R. Bazer‐Bachi et autres

We report on the first completely simultaneous observation of a gamma-ray burst (GRB) using an array of Imaging Atmospheric Cherenkov Telescopes, which is sensitive to photons in the very high energy (VHE) γ-ray range (≳ 100 GeV). On 2006 June 2, the …

ie, de, am, gb, fr, pl, Afrique du Sud, cz (code pays fourni par la source)

Discovery of a VHE gamma-ray source coincident with the supernova remnant CTB 37A

F. Aharonian, A. G. Akhperjanian, U. Barres de Almeida, A. R. Bazer‐Bachi et autres

Aims. The supernova remnant (SNR) complex CTB 37 is an interesting candidate for observations with very high energy (VHE) γ-ray telescopes such as HESS. In this region, three SNRs are seen. One of them is potentially associated with several molecular clouds, a …

ie, de, am, gb, fr, pl, Afrique du Sud, us, jp, cz (code pays fourni par la source)

HESS upper limits for Kepler's supernova remnant

F. Aharonian, A. G. Akhperjanian, U. Barres de Almeida, A. R. Bazer‐Bachi et autres

Aims. Observations of Kepler's supernova remnant (G4.5+6.8) with the HESS telescope array in 2004 and 2005 with a total live time of 13 h are presented.

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Chandra and HESS observations of the supernova remnant CTB 37B

F. Aharonian, A. G. Akhperjanian, U. Barres de Almeida, A. R. Bazer‐Bachi et autres

We discovered the >100 GeV γ-ray source, HESS J1713-381, apparently associated with the shell-type supernova remnant (SNR) CTB 37B, using HESS in 2006. In 2007 we performed X-ray follow-up observations with Chandra with the aim of identifying a synchrotron counterpart to the …

ie, de, am, gb, fr, pl, Afrique du Sud, us, cz (code pays fourni par la source)

Exploring a SNR/molecular cloud association within HESS J1745–303

F. Aharonian, A. G. Akhperjanian, U. Barres de Almeida, A. R. Bazer‐Bachi et autres

Aims. HESS J1745-303 is an extended, unidentified VHE (very high energy) gamma-ray source discovered using HESS in the Galactic Plane Survey. Since no obvious counterpart has previously been found in longer-wavelength data, the processes that power the VHE emission are not well …

ie, de, am, gb, fr, pl, Afrique du Sud, us, cz (code pays fourni par la source)

Discovery of VHE γ-rays from the high-frequency-peaked BL Lacertae object RGB J0152+017

F. Aharonian, A. G. Akhperjanian, U. Barres de Almeida, A. R. Bazer‐Bachi et autres

Aims. The BL Lac object RGB J0152+017 () was predicted to be a very high-energy (VHE; >100 GeV) γ-ray source, due to its high X-ray and radio fluxes. Our aim is to understand the radiative processes by investigating the observed emission and …

ie, de, am, gb, fr, pl, Afrique du Sud, ca (code pays fourni par la source)

Discovery of very-high-energy γ-ray emission from the vicinity of PSR J1913+1011 with HESS

F. Aharonian, A. G. Akhperjanian, U. Barres de Almeida, A. R. Bazer‐Bachi et autres

The HESS experiment, an array of four Imaging Atmospheric Cherenkov Telescopes with high sensitivity and large field-of-view, has been used to search for emitters of very-high-energy (VHE, >100 GeV) γ-rays along the Galactic plane, covering the region 30° 60°, 280° 330°, and …

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Discovery of very high energy gamma-ray emission coincident with molecular clouds in the W 28 (G6.4-0.1) field

F. Aharonian, A. G. Akhperjanian, A. R. Bazer‐Bachi, B. Behera et autres

Aims. Observations of shell-type supernova remnants (SNRs) in the GeV to multi-TeV γ-ray band, coupled with those at millimetre radio wavelengths, are motivated by the search for cosmic-ray accelerators in our Galaxy. The old-age mixed-morphology SNR W 28 (distance ~2 kpc) is …

ie, de, am, fr, gb, pl, Afrique du Sud, jp, cz (code pays fourni par la source)

Observations of the Sagittarius dwarf galaxy by the HESS experiment and search for a dark matter signal

F. Aharonian, A. G. Akhperjanian, A. R. Bazer‐Bachi, M. Beilicke et autres

de, am, fr, gb, Afrique du Sud (code pays fourni par la source)

Upper limits from HESS active galactic nuclei observations in 2005–2007

F. Aharonian, A. G. Akhperjanian, U. Barres de Almeida, A. R. Bazer‐Bachi et autres

Aims.Very high energy (VHE; GeV) γ-ray studies were performed for 18 active galactic nuclei (AGN) from a variety of AGN classes.

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