328 citations
- B. Giebels5 profiles19 · h 83
- G. Dubus2 profiles19 · h 64
- O. C. de Jager4 profiles19
- C. Boisson3 profiles18 · h 64
- C. Venter2 profiles18 · h 65
- D. Emmanoulopoulos3 profiles18 · h 37
- G. Pühlhofer7 profiles18 · h 48
- H. Sol5 profiles18 · h 62
- K. Kosack2 profiles18 · h 57
- M. Punch2 profiles18 · h 61
- M. Raue4 profiles18 · h 50
- S. Pita4 profiles18 · h 60
- Max Planck Institute for Nuclear PhysicsDE20 papers
- Centre National de la Recherche ScientifiqueFR19 papers
- Commissariat à l'Énergie Atomique et aux Énergies AlternativesFR18 papers
- École PolytechniqueFR18 papers
- Humboldt-Universität zu BerlinDE18 papers
- Institut de Planétologie et d'Astrophysique de GrenobleFR18 papers
- Institut National de Physique Nucléaire et de Physique des ParticulesFR18 papers
- Laboratoire AstroParticule et CosmologieFR18 papers
- Laboratoire de Physique Nucléaire et de Hautes ÉnergiesFR18 papers
- Laboratoire de Physique ThéoriqueFR18 papers
- Laboratoire Leprince-RinguetFR18 papers
- Université Joseph FourierFR18 papers
8 papers · 1 filter
Probing the Nature of the Vela X Cocoon
Stephanie M. LaMassa, Patrick O. Slane, Okkie C. de Jager
Vela X is a pulsar wind nebula (PWN) associated with the active pulsar B0833-45 and contained within the Vela supernova remnant (SNR). A collimated X-ray filament ("cocoon") extend…
Probing the radio to X-ray connection of the Vela X PWN with Fermi LAT and H.E.S.S
O. C. de Jager, P. O. Slane, S. LaMassa
Morphologically it appears as if the Vela X PWN consists of two emission regions: whereas X-ray (1 keV) and very high energy (VHE) H.E.S.S. gamma-ray observations appear to define…
H.E.S.S. Observations of the Prompt and Afterglow Phases of GRB 060602B
HESS Collaboration, F. Aharonian
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 th…
Search for Gamma-rays from Dark Matter annihilations around Intermediate Mass Black Holes with the H.E.S.S. experiment
HESS Collaboration, F Aharonian, G. Bertone
The H.E.S.S. array of Cherenkov telescopes has performed, from 2004 to 2007, a survey of the inner Galactic plane at photon energies above 100 GeV. About 400 hours of data have bee…
A Cosmic Ray Positron Anisotropy due to Two Middle-Aged, Nearby Pulsars?
I. Buesching, O. C. de Jager, M. S. Potgieter +1
Geminga and B0656+14 are the closest pulsars with characteristic ages in the ran ge of 100 kyr to 1 Myr. They both have spindown powers of the order 3e34 erg/s at present. The wind…
Exploring a SNR/Molecular Cloud Association Within HESS J1745-303
HESS Collaboration, F. Aharonian
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…