activity
20002026
most citedEuclid. I. Overview of the Euclid mission

550 citations · 4k across the 88 of their papers we have counts for

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Showing 2010Show all

7 papers · 1 filter

astro-ph.CO2010★ 60 cited

Toward a Universal Formulation of the Halo Mass Function

P. S. Corasaniti, I. Achitouv

We compute the dark matter halo mass function using the excursion set formalism for a diffusive barrier with linearly drifting average which captures the main features of the ellip…

astro-ph.CO2010★ 61 cited

Precision cosmology with a wide area XMM cluster survey

M. Pierre, F. Pacaud, J. B. Juin +3

We explore the cosmological constraints expected from wide area XMM-type cluster surveys covering 50-200 deg2, under realistic observing conditions. We perform a Fisher matrix anal…

astro-ph.CO2010★ 3 cited

The Herschel-SPIRE Legacy Survey (HSLS): the scientific goals of a shallow and wide submillimeter imaging survey with SPIRE

Asantha Cooray, Steve Eales, Scott Chapman +247

A large sub-mm survey with Herschel will enable many exciting science opportunities, especially in an era of wide-field optical and radio surveys and high resolution cosmic microwa…

astro-ph.CO2010★ 42 cited

Introducing the Dark Energy Universe Simulation Series (DEUSS)

Y. Rasera, J-M. Alimi, J. Courtin +4

In this "Invisible Universe" proceedings, we introduce the Dark Energy Universe Simulation Series (DEUSS) which aim at investigating the imprints of realistic dark energy models on…

astro-ph.CO2010

Primordial non-Gaussianity in density fluctuations

F. Fraschetti, J. M. Alimi, J. Courtin +1

We present N-body cosmological numerical simulations including a primordial non-Gaussianity in the density fluctuation field quantified by the non-linear parameter . We hav…

astro-ph.CO2010★ 3 cited

The innocuousness of adiabatic instabilities in coupled scalar field-dark matter models

Pier Stefano Corasaniti

Non-minimally coupled scalar field models suffer of unstable growing modes at the linear perturbation level. The nature of these instabilities depends on the dynamical state of the…