output
20052022
most citedSupernova Constraints and Systematic Uncertainties from the First 3 Years of the Supernova Legacy Survey

906 citations

Showing 2021Show all

11 papers · 1 filter

astro-ph.IM20213 cited

Current status of PAPYRUS : the pyramid based adaptive optics system at LAM/OHP

Muslimov E., Levraud N., Chambouleyron V. +23

The Provence Adaptive optics Pyramid Run System (PAPYRUS) is a pyramid-based Adaptive Optics (AO) system that will be installed at the Coude focus of the 1.52m telescope (T152) at…

astro-ph.IM20213 cited

Experimental validation of active control of low-order aberrations with a Zernike sensor through a Lyot coronagraph

Raphaël Pourcelot, Mamadou N'Diaye, Emiel H. Por +11

Future large segmented space telescopes and their coronagraphic instruments are expected to provide the resolution and sensitivity to observe Earth-like planets with a 10^10 contra…

nlin.CD20214 cited

Bogolyubov's averaging theorem applied to the Kramers-Henneberger Hamiltonian

Elena Floriani, Jonathan Dubois, Cristel Chandre

We apply Bogolyubov's averaging theorem to the motion of an electron of an atom driven by a linearly polarized laser field in the Kramers-Henneberger frame. We provide estimates of…

astro-ph.GA20219 cited

Evolution of the galaxy merger fraction in the CLAUDS+HSC-SSP deep fields

Nathalie Thibert, Marcin Sawicki, Andy Goulding +3

We estimate the evolution of the galaxy-galaxy merger fraction for galaxies over in the 18.6 deg deep CLAUDS+HSC-SSP surveys. We do…

astro-ph.CO20212 cited

Testing the predictions of axisymmetric distribution functions of galactic dark matter with hydrodynamical simulations

Mihael Petač, Julien Lavalle, Arturo Núñez-Castiñeyra +1

Signal predictions for galactic dark matter (DM) searches often rely on assumptions on the DM phase-space distribution function (DF) in halos. This applies to both particle (e.g. $…

astro-ph.CO202140 cited

The X-CLASS survey: A catalogue of 1646 X-ray-selected galaxy clusters up to z1.5

E. Koulouridis, N. Clerc, T. Sadibekova +25

Cosmological probes based on galaxy clusters rely on cluster number counts and large-scale structure information. X-ray cluster surveys are well suited for this purpose, since they…