activity
20042026
most citedThe Atlas3D project -- I. A volume-limited sample of 260 nearby early-type galaxies: science goals and selection criteria

1.1k citations · 16.5k across the 175 of their papers we have counts for

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astro-ph2008★ 27 cited

An improved limit on the neutrino mass with CMB and redshift-dependent halo bias-mass relations from SDSS, DEEP2, and Lyman-Break Galaxies

Francesco De Bernardis, Paolo Serra, Asantha Cooray +1

We use measurements of luminosity-dependent galaxy bias at several different redshifts, SDSS at , DEEP2 at and LBGs at , combined with WMAP five-year cosmic mi…

astro-ph2008★ 17 cited

Impact of Point Source Clustering on Cosmological Parameters with CMB Anisotropies

Paolo Serra, Asantha Cooray, Alexandre Amblard +2

The faint radio point sources that are unresolved in cosmic microwave background (CMB) anisotropy maps are likely to be a biased tracer of the large-scale structure dark matter dis…

astro-ph2008★ 24 cited

Anisotropies in the Cosmic Neutrino Background after WMAP 5-year Data

Francesco De Bernardis, Luca Pagano, Paolo Serra +2

We search for the presence of cosmological neutrino background (CNB) anisotropies in recent WMAP 5-year data using their signature imprinted on modifications to cosmic microwave ba…

astro-ph2008★ 23 cited

Weak Lensing of the Primary CMB Bispectrum

Asantha Cooray, Devdeep Sarkar, Paolo Serra

The cosmic microwave background (CMB) bispectrum is a well-known probe of the non-Gaussianity of primordial perturbations. Just as the intervening large-scale structure modifies th…

astro-ph2008★ 32 cited

Cosmic Shear from Scalar-Induced Gravitational Waves

Devdeep Sarkar, Paolo Serra, Asantha Cooray +2

Weak gravitational lensing by foreground density perturbations generates a gradient mode in the shear of background images. In contrast, cosmological tensor perturbations induce a…

astro-ph2008★ 93 cited

Finding Evidence for Massive Neutrinos using 3D Weak Lensing

T. D. Kitching, A. F. Heavens, L. Verde +2

In this paper we investigate the potential of 3D cosmic shear to constrain massive neutrino parameters. We find that if the total mass is substantial (near the upper limits from LS…