activity
19962022
most citedHi-GAL: the Herschel infrared Galactic Plane Survey

614 citations · 1.8k across the 25 of their papers we have counts for

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Showing astro-ph.COShow all

11 papers · 1 filter

astro-ph.CO2019★ 14 cited

Energy Density, Temperature and Entropy Dynamics in Perturbative Reheating

Alessandro Di Marco, Giancarlo De Gasperis, Gianfranco Pradisi +1

We discuss the perturbative decay of the energy density of a non standard inflaton field and the corresponding creation of the energy density of the relativistic fields …

astro-ph.CO2017★ 19 cited

Exploring cosmic origins with CORE: mitigation of systematic effects

P. Natoli, M. Ashdown, R. Banerji +123

We present an analysis of the main systematic effects that could impact the measurement of CMB polarization with the proposed CORE space mission. We employ timeline-to-map simulati…

astro-ph.CO2017★ 64 cited

Exploring cosmic origins with CORE: gravitational lensing of the CMB

Anthony Challinor, Rupert Allison, Julien Carron +110

Lensing of the CMB is now a well-developed probe of large-scale clustering over a broad range of redshifts. By exploiting the non-Gaussian imprints of lensing in the polarization o…

astro-ph.CO2016★ 146 cited

Exploring Cosmic Origins with CORE: Inflation

CORE Collaboration, Fabio Finelli, Martin Bucher +129

We forecast the scientific capabilities to improve our understanding of cosmic inflation of CORE, a proposed CMB space satellite submitted in response to the ESA fifth call for a m…

astro-ph.CO2016★ 135 cited

Exploring Cosmic Origins with CORE: Cosmological Parameters

Eleonora Di Valentino, Thejs Brinckmann, Martina Gerbino +125

We forecast the main cosmological parameter constraints achievable with the CORE space mission which is dedicated to mapping the polarisation of the Cosmic Microwave Background (CM…

astro-ph.CO2012★ 10 cited

Planck intermediate results. VI: The dynamical structure of PLCKG214.6+37.0, a Planck discovered triple system of galaxy clusters

Planck Collaboration, P. A. R. Ade, N. Aghanim +200

The survey of galaxy clusters performed by Planck through the Sunyaev-Zeldovich effect has already discovered many interesting objects, thanks to the whole coverage of the sky. One…

astro-ph.CO2012★ 39 cited

Planck intermediate results. VII. Statistical properties of infrared and radio extragalactic sources from the Planck Early Release Compact Source Catalogue at frequencies between 100 and 857 GHz

Planck Collaboration, P. A. R. Ade, N. Aghanim +188

(abridged for arXiv) We make use of the Planck all-sky survey to derive number counts and spectral indices of extragalactic sources -- infrared and radio sources -- from the Planck…

astro-ph.CO2012★ 203 cited

Planck Intermediate Results. V. Pressure profiles of galaxy clusters from the Sunyaev-Zeldovich effect

Planck Collaboration, P. A. R. Ade, N. Aghanim +214

Taking advantage of the all-sky coverage and broad frequency range of the Planck satellite, we study the Sunyaev-Zeldovich (SZ) and pressure profiles of 62 nearby massive clusters…

astro-ph.CO2012★ 20 cited

Planck Intermediate Results II: Comparison of Sunyaev-Zeldovich measurements from Planck and from the Arcminute Microkelvin Imager for 11 galaxy clusters

Planck, AMI Collaborations, : +195

A comparison is presented of Sunyaev-Zeldovich measurements for 11 galaxy clusters as obtained by Planck and by the ground-based interferometer, the Arcminute Microkelvin Imager. A…

astro-ph.CO2011★ 156 cited

Planck Early Results. X. Statistical analysis of Sunyaev-Zeldovich scaling relations for X-ray galaxy clusters

Planck Collaboration, N. Aghanim, M. Arnaud +197

All-sky data from the Planck survey and the Meta-Catalogue of X-ray detected Clusters of galaxies (MCXC) are combined to investigate the relationship between the thermal Sunyaev-Ze…

astro-ph.CO2011★ 83 cited

Planck early results XIV: ERCSC validation and extreme radio sources

Planck Collaboration, P. A. R. Ade, N. Aghanim +206

Planck's all sky surveys at 30-857 GHz provide an unprecedented opportunity to follow the radio spectra of a large sample of extragalactic sources to frequencies 2-20 times higher…