H.E.S.S. CollaborationH.E.S.S. Collaboration
  • About H.E.S.S.
    • H.E.S.S. Collaboration
      • Organisation
    • H.E.S.S. Science
    • H.E.S.S. Telescopes
    • H.E.S.S. Prize
  • News
    • Announcements
    • Press releases
    • Archival news
  • Source of the Month
  • For scientists
    • Publications
      • Journals
      • Conferences
      • Astronomers Telegram
    • External Proposals
      • Visibility calculator
    • HESS GRB observations
      • Interactive Tool (Public)
      • Interactive Tool (Internal)
    • Public test data release
    • Telescope specifications
  • Contact

Blog Archives

January 15, 2019 by Lars Mohrmann

Particle transport within the pulsar wind nebula HESS J1825–137

Context. We present a detailed view of the pulsar wind nebula (PWN) HESS J1825–137. We aim to constrain the mechanisms dominating the particle transport within the nebula, accounting for its anomalously large size and…

Read more

January 11, 2019 by Lars Mohrmann

The 2014 TeV γ-Ray Flare of Mrk 501 Seen with H.E.S.S.: Temporal and Spectral Constraints on Lorentz Invariance Violation

The blazar Mrk 501 (z = 0.034) was observed at very-high-energy (VHE, E ≳ 100 GeV) gamma-ray wavelengths during a bright flare on the night of 2014 June 23–24 (MJD 56832) with the H.E.S.S. phase-II array of Cherenkov telescopes.…

Read more

December 3, 2018 by Lars Mohrmann

First ground-based measurement of sub-20 GeV to 100 GeV γ-Rays from the Vela pulsar with H.E.S.S. II

Aims. We report on the measurement and investigation of pulsed high-energy γ-ray emission from the Vela pulsar, PSR B0833−45, based on observations with the largest telescope of H.E.S.S., CT5, in monoscopic mode, and on…

Read more

November 23, 2018 by Lars Mohrmann

Searches for gamma-ray lines and ‘pure WIMP’ spectra from Dark Matter annihilations in dwarf galaxies with H.E.S.S.

Dwarf spheroidal galaxies are among the most promising targets for detecting signals of Dark Matter (DM) annihilations. The H.E.S.S. experiment has observed five of these systems for a total of about 130 hours. The…

Read more

November 8, 2018 by Lars Mohrmann

The γ-ray spectrum of the core of Centaurus A as observed with H.E.S.S. and Fermi-LAT

Centaurus A (Cen A) is the nearest radio galaxy discovered as a very-high-energy (VHE; 100 GeV–100 TeV) γ-ray source by the High Energy Stereoscopic System (H.E.S.S.). It is a faint VHE γ-ray emitter, though…

Read more

October 5, 2018 by Lars Mohrmann

VHE γ-ray discovery and multiwavelength study of the blazar 1ES 2322−409

A hotspot at a position compatible with the BL Lac object 1ES 2322-409 was serendipitously detected with H.E.S.S. during observations performed in 2004 and 2006 on the blazar PKS 2316-423. Additional data on 1ES…

Read more

September 20, 2018 by Lars Mohrmann

The starburst galaxy NGC 253 revisited by H.E.S.S. and Fermi-LAT

Context. NGC 253 is one of only two starburst galaxies found to emit γ-rays from hundreds of MeV to multi-TeV energies. Accurate measurements of the very-high-energy (VHE; E > 100 GeV) and high-energy (HE;…

Read more

July 13, 2018 by Lars Mohrmann

Multimessenger observations of a flaring blazar coincident with high-energy neutrino IceCube-170922A

Previous detections of individual astrophysical sources of neutrinos are limited to the Sun and the supernova 1987A, whereas the origins of the diffuse flux of high-energy cosmic neutrinos remain unidentified. On 22 September 2017,…

Read more

May 15, 2018 by Lars Mohrmann

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.

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…

Read more

April 9, 2018 by Lars Mohrmann

The H.E.S.S. Galactic plane survey

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…

Read more

Posts pagination

Previous 1 … 6 7 8 … 25 Next
70/243

Browse other months

Recent sources

A H.E.S.S. Retrospective on Gamma-Ray BurstsApril 1, 2026
Hidden by the Shell – A Pulsar Wind Nebula Emerges in Vela JuniorMarch 1, 2026
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

Fields

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

Contact

You can contact us for scientific queries and general information using:
contact.hess@hess-experiment.eu

Data Privacy Statement

https://www.mpi-hd.mpg.de/mpi/de/datenschutzhinweis
H.E.S.S. collaboration official website. Proudly Built By H.E.S.S. members.
(c) 2004-2026 by the H.E.S.S. collaboration.

Last sources of the month

A H.E.S.S. Retrospective on Gamma-Ray BurstsApril 1, 2026
Hidden by the Shell – A Pulsar Wind Nebula Emerges in Vela JuniorMarch 1, 2026
H.E.S.S.’ most distant blazar: PKS 0346−27February 1, 2026

Internal

  • Log in
  • Entries feed
  • Comments feed
  • WordPress.org
H.E.S.S. Collaboration
Manage Consent
To provide the best experiences, we use technologies like cookies to store and/or access device information. Consenting to these technologies will allow us to process data such as browsing behavior or unique IDs on this site. Not consenting or withdrawing consent, may adversely affect certain features and functions.
Functional Always active
The technical storage or access is strictly necessary for the legitimate purpose of enabling the use of a specific service explicitly requested by the subscriber or user, or for the sole purpose of carrying out the transmission of a communication over an electronic communications network.
Preferences
The technical storage or access is necessary for the legitimate purpose of storing preferences that are not requested by the subscriber or user.
Statistics
The technical storage or access that is used exclusively for statistical purposes. The technical storage or access that is used exclusively for anonymous statistical purposes. Without a subpoena, voluntary compliance on the part of your Internet Service Provider, or additional records from a third party, information stored or retrieved for this purpose alone cannot usually be used to identify you.
Marketing
The technical storage or access is required to create user profiles to send advertising, or to track the user on a website or across several websites for similar marketing purposes.
  • Manage options
  • Manage services
  • Manage {vendor_count} vendors
  • Read more about these purposes
View preferences
  • {title}
  • {title}
  • {title}