2.6k citations
- S. Funk4 profiles47 · h 89
- O. Reimer3 profiles45 · h 108
- A. Reimer2 profiles44 · h 120
- B. Giebels3 profiles40 · h 83
- C. Favuzzi3 profiles34 · h 115
- F. Longo6 profiles34 · h 126
- F. Loparco4 profiles34 · h 117
- G. Barbiellini3 profiles34 · h 130
- P. Fusco2 profiles34 · h 117
- P. Spinelli2 profiles34 · h 117
- S. Rainò2 profiles34 · h 118
- C. Cecchi3 profiles33 · h 110
- Centre National de la Recherche ScientifiqueFR376 papers
- Laboratoire de Physique ThéoriqueFR117 papers
- Commissariat à l'Énergie Atomique et aux Énergies AlternativesFR84 papers
- Université Paris CitéFR80 papers
- CEA Paris-SaclayFR78 papers
- Institut National de Physique Nucléaire et de Physique des ParticulesFR72 papers
- Université Toulouse III - Paul SabatierFR61 papers
- École PolytechniqueFR60 papers
- Laboratoire Charles CoulombFR60 papers
- Laboratoire Leprince-RinguetFR60 papers
- Sorbonne UniversitéFR47 papers
- Institut de Recherche sur les Lois Fondamentales de l'UniversFR42 papers
29 papers · 2 filters
H.E.S.S. observations of the supernova remnant RX J0852.0-4622: shell-type morphology and spectrum of a widely extended VHE gamma-ray source
HESS Collaboration, F. A. Aharonian
The shell-type supernova remnant RX J0852.0-4622 was observed with the High Energy Stereoscopic System (H.E.S.S.) of Atmospheric Cherenkov Telescopes between December 2004 and May…
Near-Infrared Spectroscopy of Carbon-Enhanced Metal-Poor Stars. I. A SOAR/OSIRIS Pilot Study
Timothy C. Beers, Thirupathi Sivarani, Brian Marstellar +3
We report on an abundance analysis for a pilot study of seven Carbon-Enhanced Metal-Poor (CEMP) stars, based on medium-resolution optical and near-infrared spectroscopy. The optica…
Primary particle acceleration above 100 TeV in the shell-type Supernova Remnant RX J1713.7-3946 with deep H.E.S.S. observations
The HESS Collaboration, F. Aharonian
We present deep H.E.S.S. observations of the supernova remnant (SNR) RX J1713.7-3946. Combining data of three years - from 2003 to 2005 - we obtain significantly increased statisti…
First stars VII. Lithium in extremely metal poor dwarfs
P. Bonifacio, P. Molaro, T. Sivarani +12
Aims. This study aims to determine the level and constancy of the Spite plateau as definitively as possible from homogeneous high-quality VLT-UVES spectra of 19 of the most metal-p…
Rubidium-Rich Asymptotic Giant Branch Stars
D. A. Garcia-Hernandez, P. Garcia-Lario, B. Plez +3
A long debated issue concerning the nucleosynthesis of neutron-rich elements in Asymptotic Giant Branch (AGB) stars is the identification of the neutron source. We report intermedi…
Pointer states for primordial fluctuations in inflationary cosmology
C. Kiefer, I. Lohmar, D. Polarski +1
Primordial fluctuations in inflationary cosmology acquire classical properties through decoherence when their wavelengths become larger than the Hubble scale. Although decoherence…