670 citations
- National Institute for AstrophysicsIT39 papers
- Centre National de la Recherche ScientifiqueFR36 papers
- Commissariat à l'Énergie Atomique et aux Énergies AlternativesFR24 papers
- CEA Paris-SaclayFR21 papers
- Max Planck Institute for AstrophysicsDE21 papers
- Global Social ObservatoryCH19 papers
- Goddard Space Flight CenterUS19 papers
- Leibniz Institute for Astrophysics PotsdamDE18 papers
- Osservatorio astronomico di BolognaIT18 papers
- Astronomical Observatory of RomeIT17 papers
- Istituto di Radioastronomia di BolognaIT17 papers
- University of GenevaCH17 papers
81 papers
Chandra and Spitzer Imaging of the Infrared Cluster in NGC 2071
S. L. Skinner, K. R. Sokal, S. T. Megeath +5
We present results of a sensitive Chandra X-ray observation and Spitzer mid-IR observations of the infrared cluster lying north of the NGC 2071 reflection nebula in the Orion B mol…
Compton reflection in AGN with Simbol-X
V. Beckmann, T. J. -L. Courvoisier, N. Gehrels +5
AGN exhibit complex hard X-ray spectra. Our current understanding is that the emission is dominated by inverse Compton processes which take place in the corona above the accretion…
The hard X-ray view of bright infrared galaxies
R. Walter, N. Cabral
Aims. The synthesis of the cosmic X-ray background (CXB) requires a large population of Compton-thick active galactic nuclei that have not been detected so far. We probe whether br…
Neutrino signal from gamma-ray loud binaries powered by high energy protons
A. Neronov, M. Ribordy
We present a hadronic model of activity for Galactic gamma-ray-loud binaries, in which the multi-TeV neutrino flux from the source can be much higher and/or harder than the detecte…
Broad-Band Spectrum of The Black Hole Candidate IGR J17497-2821 Studied with Suzaku
A. Paizis, K. Ebisawa, H. Takahashi +9
The broad-band 1-300 keV Suzaku spectrum of IGR J17497-2821, the X-ray transient discovered by INTEGRAL in September 2006, is presented. Suzaku observed IGR J17497-2821 on Septembe…
Physical properties of galaxies and their evolution in the VIMOS VLT Deep Survey. II. Extending the mass-metallicity relation to the range z=0.89-1.24
E. Perez-Montero, T. Contini, F. Lamareille +39
Aims. We present a continuation of our study about the relation between stellar mass and gas-phase metallicity in the VIMOS VLT Deep Survey (VVDS). In this work we extend the deter…