7.1k citations
- Centre National de la Recherche ScientifiqueFR2.3k papers
- Sorbonne UniversitéFR1.8k papers
- Université Paris CitéFR1.3k papers
- Observatoire de ParisFR771 papers
- Laboratoire d’études spatiales et d’instrumentation en astrophysiqueFR615 papers
- Sorbonne Paris CitéFR555 papers
- École Normale Supérieure - PSLFR508 papers
- Délégation Paris 7FR490 papers
- Université Paris-SaclayFR477 papers
- Commissariat à l'Énergie Atomique et aux Énergies AlternativesFR401 papers
- Université Grenoble AlpesFR361 papers
- CEA Paris-SaclayFR349 papers
208 papers · 1 filter
Search for long-term variability of HESS J1745-290
H. E. S. S. Collaboration, :, A. Acharyya +116
At the center of our Galaxy lies the bright γ-ray point-like source HESS J1745-290, which is compatible in position with Sgr A star, although an association between the two remains…
Young Massive Star Clusters as TeV Emitters: Constraints from H.E.S.S. and LHAASO
Rowan Batzofin, Pierre Cristofari, Kathrin Egberts
Young massive star clusters (YMSCs) have been proposed as excellent candidates for the main sources of Galactic cosmic rays (CRs) up to the PeV range. The detection and study of ga…
Blazar flares from plasma blobs crossing the broad-line region
Sébastien Le Bihan, Anton Dmytriiev, Andreas Zech
The blazar 3C 279 is well known for its rapid and large-amplitude variability. On 20 December 2013, the source exhibited an orphan γ-ray flare characterized by a flux-doubling time…
Chasing Gamma-Ray Signals from Binary Neutron Star Coalescences with the Cherenkov Telescope Array: Prospects and Observing Strategies
S. Abe, J. Abhir, A. Abhishek +457
The detection of gravitational waves (GWs) from a binary neutron star (BNS) merger by Advanced LIGO and Advanced Virgo (GW170817), together with its electromagnetic counterpart, th…
Pulsar Discoveries from the TRAPUM UHF Survey of Fermi-LAT Sources
Tinn Thongmeearkom, Colin J. Clark, Rene P. Breton +25
The Fermi Large Area Telescope (LAT) provides advantages for radio pulsar searches by enabling efficient target selection. We can confidently point radio telescopes to the position…
Can a single supernova remnant account for the gamma-ray emission of G106.3+2.7?
P. Cristofari, G. Emery, T. Lubrano di Vavaria +4
SNR G106.3+2.7 is a complex TeV emitting source whose emission is still poorly understood. It has especially been at the center of numerous discussions on its potential for being a…