activity
20142016
most citedA Joint Analysis of BICEP2/Keck Array and Planck Data

985 citations · 1.9k across the 6 of their papers we have counts for

collaborators

8 papers

astro-ph.CO2024

Euclid preparation: 6x2 pt analysis of Euclid's spectroscopic and photometric data sets

Euclid Collaboration, L. Paganin, M. Bonici +252

We present cosmological parameter forecasts for the Euclid 6x2pt statistics, which include the galaxy clustering and weak lensing main probes together with previously neglected cro…

astro-ph.GA2024

Euclid preparation. XLIX. Selecting active galactic nuclei using observed colours

Euclid Collaboration, L. Bisigello, M. Massimo +244

Euclid will cover over 14000 with two optical and near-infrared spectro-photometric instruments, and is expected to detect around ten million active galactic nuclei (AGN)…

astro-ph.CO201665 cited

Planck intermediate results. L. Evidence for spatial variation of the polarized thermal dust spectral energy distribution and implications for CMB -mode analysis

Planck Collaboration, N. Aghanim, M. Ashdown +156

The characterization of the Galactic foregrounds has been shown to be the main obstacle in the challenging quest to detect primordial B-modes in the polarized microwave sky. We mak…

astro-ph.CO2015985 cited

A Joint Analysis of BICEP2/Keck Array and Planck Data

BICEP2/Keck, Planck Collaborations, : +276

We report the results of a joint analysis of data from BICEP2/Keck Array and Planck. BICEP2 and Keck Array have observed the same approximately 400 deg patch of sky centered on…

astro-ph.GA2014422 cited

Planck intermediate results. XIX. An overview of the polarized thermal emission from Galactic dust

Planck Collaboration, P. A. R. Ade, N. Aghanim +199

This paper presents the large-scale polarized sky as seen by Planck HFI at 353 GHz, which is the most sensitive Planck channel for dust polarization. We construct and analyse large…

astro-ph.GA2014190 cited

Planck intermediate results. XXII. Frequency dependence of thermal emission from Galactic dust in intensity and polarization

Planck Collaboration, P. A. R. Ade, M. I. R. Alves +177

Planck has mapped the intensity and polarization of the sky at microwave frequencies with unprecedented sensitivity. We make use of the Planck 353 GHz I, Q, and U Stokes maps as du…