H.E.S.S. CollaborationH.E.S.S. Collaboration
  • The collaboration
    • H.E.S.S. Institutions
    • H.E.S.S. Organisation
    • H.E.S.S. Prize
    • Opportunities
  • Science
    • News
    • Publications
    • H.E.S.S. Data release
    • External Proposals
    • Visibility calculator
  • Sources of the month
  • Contact

H.E.S.S. Publications

Filters
Journal Publication

HESS J1741-302: a hidden accelerator in the Galactic plane

H.E.S.S. Collaboration
Astron. Astrophys. 612 (2018) A13
Journal Publication

Systematic search for very-high-energy gamma-ray emission from bow shocks of runaway stars

H.E.S.S. Collaboration
Astron. Astrophys. 612 (2018) A12
Journal Publication

Extended VHE gamma-ray emission towards SGR1806-20, LBV1806-20, and stellar cluster Cl*1806-20

H.E.S.S. Collaboration
Astron. Astrophys. 612 (2018) A11
Journal Publication

A search for very high-energy flares from the microquasars GRS 1915+105, Circinus X-1, and V4641 Sgr using contemporaneous H.E.S.S. and RXTE observations

H.E.S.S. Collaboration
Astron. Astrophys. 612 (2018) A10
Journal Publication

Characterising the VHE diffuse emission in the central 200 parsecs of our Galaxy with H.E.S.S.

H.E.S.S. Collaboration
Astron. Astrophys. 612 (2018) A9
Journal Publication

The supernova remnant W49B as seen with H.E.S.S. and Fermi-LAT

H.E.S.S. Collaboration
Astron. Astrophys. 612 (2018) A5
Journal Publication

Detailed spectral and morphological analysis of the shell type SNR RCW 86

H.E.S.S. Collaboration
Astron. Astrophys. 612 (2018) A4
Journal Publication

Population study of Galactic supernova remnants at very high gamma-ray energies with H.E.S.S.

H.E.S.S. Collaboration
Astron. Astrophys. 612 (2018) A3
Journal Publication

The Population of TeV Pulsar Wind Nebulae in the H.E.S.S. Galactic Plane Survey

H.E.S.S. Collaboration
Astron. Astrophys. 612 (2018) A2
Journal Publication

Search for gamma-ray line signals from dark matter annihilations in the inner Galactic halo from ten years of observations with H.E.S.S

H.E.S.S. Collaboration
Phys. Rev. Lett. 120 (2018) 201101
Journal Publication

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

H.E.S.S. Collaboration
Astron. Astrophys. 617 (2018) A73
Journal Publication

First Ground-based Measurement of Sub-20 GeV to 100 GeV -rays from the Vela Pulsar with H.E.S.S. II

H.E.S.S. Collaboration
Astron. Astrophys. 620 (2018) A66
Journal Publication

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

H.E.S.S. Collaboration
Science 361 (2018)
Journal Publication

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

H.E.S.S. Collaboration
Astron. Astrophys. 619 (2018) A71
Journal Publication

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

H.E.S.S. Collaboration
JCAP 1811 (2018) 11, 037
Journal Publication

First limits on the very-high energy gamma-ray afterglow emission of a fast radio burst: H.E.S.S. observations of FRB 150418

H.E.S.S. Collaboration
Astron. Astrophys. 597 (2017) A115
Journal Publication

A polarized fast radio burst at low Galactic latitude

H.E.S.S. Collaboration
MNRAS 469 (2017) 4465
Journal Publication

Measurement of the EBL spectral energy distribution using the VHE gamma-ray spectra of H.E.S.S. blazars

H.E.S.S. Collaboration
Astron. Astrophys. 606 (2017) A59
Journal Publication

TeV gamma-ray observations of the binary neutron star merger GW170817 with H.E.S.S

H.E.S.S. Collaboration
Astrophys. J. Lett. 850 (2017) L22
Journal Publication

Multi-messenger Observations of a Binary Neutron Star Merger

H.E.S.S. Collaboration
Astrophys. J. Lett. 848 (2017) L12
Load More
H.E.S.S. did not exist before this date

The H.E.S.S. Collaboration has published over 200 papers in renowned scientific journals, advancing our understanding of the high-energy universe. These publications cover a broad range of topics, from studies of cosmic particle acceleration in supernova remnants to investigations of gamma-ray emission from active galactic nuclei. H.E.S.S. results have consistently pushed the boundaries of gamma-ray astrophysics, providing valuable insights into some of the most energetic processes in the cosmos

Contact

You can contact us for scientific queries and general informations using :
hess-ec@lsw.uni-heidelberg.de

Sources of the month

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
H.E.S.S. collaboration official website. Proudly Built By H.E.S.S. members.
(c) 2004-2025 by the H.E.S.S. collaboration

Last sources of the month

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

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}