output
20022025
most citedThe second data release from the European Pulsar Timing Array III. Search for gravitational wave signals

1k citations

Showing 2006Show all

35 papers · 1 filter

astro-ph2006★ 37 cited

The FALCON concept: multi-object adaptive optics and atmospheric tomography for integral field spectroscopy. Principles and performances on an 8 meter telescope

Francois Assemat, Eric Gendron, Francois Hammer

Integral field spectrographs are major instruments to study the mechanisms involved in the formation and the evolution of early galaxies. When combined with multi-object spectrosco…

astro-ph2006★ 1 cited

Investigating the pre-main sequence magnetic chemically peculiar system HD 72106

C. P. Folsom, G. A. Wade, D. A. Hanes +7

The origin of the strong magnetic fields observed in chemically peculiar Ap and Bp stars stars has long been debated. The recent discovery of magnetic fields in the intermediate ma…

astro-ph2006

Uncertainties of the masses of black holes and Eddington ratios in AGN

Suzy Collin

Black hole masses in Active Galactic Nuclei have been determined in 35 objects through reverberation mapping of the emission line region. I mention some uncertainties of the method…

astro-ph2006★ 31 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…

gr-qc2006★ 13 cited

MHD of rotating compact stars with spectral methods: description of the algorithm and tests

S. Bonazzola, L. Villain, M. Bejger

A flexible spectral code for the study of general relativistic magnetohydrodynamics is presented. Aiming at investigating the physics of slowly rotating magnetized compact stars, t…

astro-ph2006

Soft-excess in ULX spectra: disc emission or wind absorption?

A. C. Goncalves, R. Soria

We assess the claim that Ultra-luminous X-ray sources (ULXs) host intermediate-mass black holes (BH) by comparing the cool disc-blackbody model with a range of other models, namell…