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20052024
most citedPlanck 2013 results. XVI. Cosmological parameters

6.6k citations · 11.8k across the 35 of their papers we have counts for

collaborators

34 papers

astro-ph.CO2024

LSPE-STRIP on-sky calibration strategy using bright celestial sources

R. T. Génova-Santos, M. Bersanelli, C. Franceschet +21

In this paper we describe the global on-sky calibration strategy of the LSPE-Strip instrument. Strip is a microwave telescope operating in the Q- and W-bands (central frequencies o…

hep-ex2022★ 6 cited

Neutrinos from Stored Muons (nuSTORM)

L. Alvarez Ruso, T. Alves, S. Boyd +9

The 2020 Update of the European Strategy for Particle Physics (ESPP) (see https://cds.cern.ch/record/2720129 ) recommended that muon beam R\&D should be considered a high-priority…

astro-ph.CO2015★ 80 cited

Planck 2013 results. XXXI. Consistency of the Planck data

Planck Collaboration, P. A. R. Ade, M. Arnaud +180

The Planck design and scanning strategy provide many levels of redundancy that can be exploited to provide tests of internal consistency. One of the most important is the compariso…

astro-ph.GA2014★ 30 cited

Planck intermediate results. XXXI. Microwave survey of Galactic supernova remnants

Planck Collaboration, M. Arnaud, M. Ashdown +160

The all-sky Planck survey in 9 frequency bands was used to search for emission from all 274 known Galactic supernova remnants. Of these, 16 were detected in at least two Planck fre…

astro-ph.CO2014★ 222 cited

Planck intermediate results. XXX. The angular power spectrum of polarized dust emission at intermediate and high Galactic latitudes

Planck Collaboration, R. Adam, P. A. R. Ade +230

The polarized thermal emission from Galactic dust is the main foreground present in measurements of the polarization of the cosmic microwave background (CMB) at frequencies above 1…

astro-ph.CO2014★ 6 cited

Foreground removal requirements for measuring large-scale CMB B-modes in light of BICEP2

A. Bonaldi, S. Ricciardi, M. L. Brown

The most convincing confirmation that the B-mode polarization signal detected at degree scales by BICEP2 is due to the Cosmic Microwave Background (CMB) would be the measurement of…