3.6k citations
Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.
- National Institute for AstrophysicsIT865 papers
- Centre National de la Recherche ScientifiqueFR635 papers
- Astronomical Observatory of RomeIT475 papers
- Commissariat à l'Énergie Atomique et aux Énergies AlternativesFR368 papers
- Brera Astronomical ObservatoryIT355 papers
- Goddard Space Flight CenterUS343 papers
- University of PaduaIT336 papers
- Astrophysique, Instrumentation et ModélisationFR332 papers
- California Institute of TechnologyUS323 papers
- Université Paris CitéFR321 papers
- Arcetri Astrophysical ObservatoryIT317 papers
- University College LondonGB308 papers
8 papers · 1 filter
The Spectral Energy Distribution of Fermi bright blazars
A. A. Abdo, M. Ackermann, M. Ajello +107
(Abridged) We have conducted a detailed investigation of the broad-band spectral properties of the γ-ray selected blazars of the Fermi LAT Bright AGN Sample (LBAS). By combining ou…
Supermodel Analysis of Galaxy Clusters
R. Fusco-Femiano, A. Cavaliere, A. Lapi
[abridged] We present the analysis of the X-ray brightness and temperature profiles for six clusters belonging to both the Cool Core and Non Cool Core classes, in terms of the Supe…
The origin of the supersoft X-ray--optical/UV flux anticorrelation in the symbiotic binary AG Draconis
A. Skopal, M. Sekeras, R. Gonzalez-Riestra +1
AG Draconis produces a strong supersoft X-ray emission.The X-ray and optical/UV fluxes are in a strict anticorrelation throughout the active and quiescent phases. The aim of this c…
Prospects for GRB Science with the Fermi Large Area Telescope
D. L. Band, M. Axelsson, L. Baldini +54
The LAT instrument on the Fermi mission will reveal the rich spectral and temporal gamma-ray burst phenomena in the > 100 MeV band. The synergy with Fermi's GBM detectors will link…
The Science Case for PILOT III: the Nearby Universe
J. S. Lawrence, M. C. B. Ashley, J. Bailey +20
PILOT (the Pathfinder for an International Large Optical Telescope is a proposed 2.5 m optical/infrared telescope to be located at DomeC on the Antarctic plateau. The atmospheric c…
The Science Case for PILOT I: Summary and Overview
J. S. Lawrence, M. C. B. Ashley, J. Bailey +40
PILOT (the Pathfinder for an International Large Optical Telescope) is a proposed 2.5 m optical/infrared telescope to be located at Dome C on the Antarctic plateau. Conditions at D…
Galaxy Clusters, a Novel Look at Diffuse Baryons Withstanding Dark Matter Gravity
A. Cavaliere, A. Lapi, R. Fusco-Femiano
[abridged] The equilibria of the intracluster plasma (ICP) and of the gravitationally dominant dark matter (DM) are governed by the hydrostatic and the Jeans equation. Jeans, with…
Why do low-mass stars become red giants?
Richard J. Stancliffe, Alessandro Chieffi, John C. Lattanzio +1
We revisit the problem of why stars become red giants. We modify the physics of a standard stellar evolution code in order to determine what does and what does not contribute to a…