output
20022011
most citedInteraction Ruling Animal Collective Behaviour Depends on Topological rather than Metric Distance: Evidence from a Field Study

2.1k citations

Showing 2006 · astro-phShow all

81 papers · 2 filters

astro-ph2006189 cited

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…

astro-ph20061k cited

zCOSMOS: A Large VLT/VIMOS redshift survey covering 0 < z < 3 in the COSMOS field

S. J. Lilly, O. Le Fevre, A. Renzini +42

zCOSMOS is a large redshift survey that is being undertaken in the COSMOS field using 600 hours of observation with the VIMOS spectrograph on the 8-m VLT. The survey is designed to…

astro-ph20067 cited

Interferometric observations of eta Carinae with VINCI/VLTI

Pierre Kervella

Context: The bright star eta Carinae is the most massive and luminous star in our region of the Milky Way. Though it has been extensively studied using many different techniques, i…

astro-ph200631 cited

Determination of the light curve of the Rosetta target Asteroid (2867) Steins by the OSIRIS cameras onboard Rosetta

M. Kueppers, S. Mottola, S. C. Lowry +9

Context: In 2004 asteroid (2867) Steins has been selected as a flyby target for the Rosetta mission. Determination of its spin period and the orientation of its rotation axis are e…

astro-ph2006328 cited

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…

astro-ph2006140 cited

Excitation of solar-like oscillations across the HR diagram

R. Samadi, D. Georgobiani, R. Trampedach R. +3

We extend semi-analytical computations of excitation rates for solar oscillation modes to those of other solar-like oscillating stars to compare them with recent observations. Nume…