ZEU-HESS

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2018-06-18
16:16
[PUBDB-2018-02322] Journal Article
; ; ; et al
Characterising the VHE diffuse emission in the central 200 parsecs of our Galaxy with H.E.S.S.
The diffuse very high-energy (VHE; >100 GeV) γ-ray emission observed in the central 200 pc of the Milky Way by H.E.S.S. was found to follow dense matter distribution in the central molecular zone (CMZ) up to a longitudinal distance of about 130 pc to the Galactic centre (GC), where the flux rapidly decreases [...]
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ddc:520
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2018-05-23
11:19
OpenAccess [PUBDB-2018-02055] Report/Journal Article
; ; ; et al
Search for γ -Ray Line Signals from Dark Matter Annihilations in the Inner Galactic Halo from 10 Years of Observations with H.E.S.S.
[arXiv:1805.05741]
Spectral lines are among the most powerful signatures for dark matter (DM) annihilation searches in very-high-energy γ rays. The central region of the Milky Way halo is one of the most promising targets given its large amount of DM and proximity to Earth [...]
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ddc:550
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2018-05-23
11:06
OpenAccess [PUBDB-2018-02054] Report/Journal Article
; ; ; et al
The population of TeV pulsar wind nebulae in the H.E.S.S. Galactic Plane Survey
[arXiv:1702.08280]
The nine-year H.E.S.S. Galactic Plane Survey (HGPS) has yielded the most uniform observation scan of the inner Milky Way in the TeV gamma-ray band to date. [...]
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2018-05-22
14:48
OpenAccess [PUBDB-2018-02035] Report/Journal Article
; ; ; et al
The H.E.S.S. Galactic plane survey
[arXiv:1804.02432]
We present the results of the most comprehensive survey of the Galactic plane in very high-energy (VHE) γ-rays, including a public release of Galactic sky maps, a catalog of VHE sources, and the discovery of 16 new sources of VHE γ-rays. The High Energy Spectroscopic System (H.E.S.S.) Galactic plane survey (HGPS) was a decade-long observation program carried out by the H.E.S.S. [...]
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2018-05-22
14:35
OpenAccess [PUBDB-2018-02031] Report/Journal Article
; ; ; et al
Systematic search for very-high-energy gamma-ray emission from bow shocks of runaway stars
[arXiv:1705.02263]
Context. Runaway stars form bow shocks by ploughing through the interstellar medium at supersonic speeds and are promising sources of non-thermal emission of photons. [...]
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2018-05-22
14:04
OpenAccess [PUBDB-2018-02028] Report/Journal Article
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Constraints on particle acceleration in SS433/W50 from MAGIC and H.E.S.S. observations
[arXiv:1707.03658]
Context. The large jet kinetic power and non-thermal processes occurring in the microquasar SS 433 make this source a good candidate for a very high-energy (VHE) gamma-ray emitter. [...]
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2018-05-22
13:48
OpenAccess [PUBDB-2018-02027] Report/Journal Article
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Population study of Galactic supernova remnants at very high $\gamma$-ray energies with H.E.S.S.
[arXiv:1802.05172]
Shell-type supernova remnants (SNRs) are considered prime candidates for the acceleration of Galactic cosmic rays (CRs) up to the knee of the CR spectrum at E ≈ 3 × 10$^{15}$ eV. Our Milky Way galaxy hosts more than 350 SNRs discovered at radio wavelengths and at high energies, of which 220 fall into the H.E.S.S. [...]
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2018-05-22
13:35
OpenAccess [PUBDB-2018-02025] Report/Journal Article
; ; ; et al
HESS J1741−302: a hidden accelerator in the Galactic plane
[arXiv:1711.01350]
The H.E.S.S. Collaboration has discovered a new very high energy (VHE, E > 0.1 TeV) γ-ray source, HESS J1741−302, located in the Galactic plane. [...]
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2018-04-23
13:37
OpenAccess [PUBDB-2018-01824] Report/Journal Article
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A search for new supernova remnant shells in the Galactic plane with H.E.S.S.
[arXiv:1801.06020]
A search for new supernova remnants (SNRs) has been conducted using TeV gamma-ray data from the H.E.S.S. Galactic plane survey. [...]
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2018-03-26
14:17
OpenAccess [PUBDB-2018-01567] Report/Journal Article
; ; ; et al
H.E.S.S. discovery of very high energy $\gamma$-ray emission from PKS 0625-354
[arXiv:1802.07611]
PKS 0625−354 (z = 0.055) was observed with the four High Energy Stereoscopic System (H.E.S.S.) telescopes in 2012 during 5.5 h. The source was detected above an energy threshold of 200 GeV at a significance level of 6.1σ. [...]
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