970 citations
- B. Åsman6 profiles37 · h 98
- A. Sopczak2 profiles36 · h 83
- L. Mundim2 profiles35 · h 124
- M. Begalli5 profiles35 · h 68
- M. Besançon2 profiles35 · h 132
- Y. Arnoud2 profiles35
- D. Wicke3 profiles34 · h 64
- P. Jonsson5 profiles34
- P. Verdier2 profiles34 · h 114
- D. Schaile6 profiles33 · h 87
- M. Mulders4 profiles31 · h 118
- C. Bélanger-Champagne2 profiles30
- Centre National de la Recherche ScientifiqueFR228 papers
- Sorbonne UniversitéFR131 papers
- Commissariat à l'Énergie Atomique et aux Énergies AlternativesFR79 papers
- Université Paris-SudFR70 papers
- CEA Paris-SaclayFR68 papers
- Délégation Paris 7FR59 papers
- Institut National de Physique Nucléaire et de Physique des ParticulesFR55 papers
- Laboratoire de Physique Nucléaire et de Hautes ÉnergiesFR53 papers
- Charles UniversityCZ42 papers
- Université Grenoble AlpesFR42 papers
- Institut de Mathématiques de Jussieu-Paris Rive GaucheFR41 papers
- Lyon 1 UniversitéFR41 papers
4 papers · 2 filters
Orbital X-Ray Variability of the Microquasar LS 5039
V. Bosch-Ramon, J. M. Paredes, M. Ribo +3
The properties of the orbit and the donor star in the high mass X-ray binary microquasar LS 5039 indicate that accretion processes should mainly occur via a radiatively driven wind…
Observations of Selected AGN with H.E.S.S
F. Aharonian et al.
A sample of selected active galactic nuclei (AGN) was observed in 2003 and 2004 with the High Energy Stereoscopic System (H.E.S.S.), an array of imaging atmospheric-Cherenkov teles…
Determination of stellar shape in microlensing event MOA 2002-BLG-33
N. J. Rattenbury, F. Abe, D. P. Bennett +30
We report a measurement of the shape of the source star in microlensing event MOA 2002-BLG-33. The lens for this event was a close binary whose centre-of-mass passed almost directl…
Further evidence for the presence of a neutron star in 4U 2206+54. INTEGRAL and VLA observations
P. Blay, M. Ribo, I. Negueruela +5
The majority of High Mass X-ray Binaries (HMXBs) behave as X-ray pulsars, revealing that they contain a magnetised neutron star. Among the four HMXBs not showing pulsations, and th…