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20112025
most citedCMB-S4 Science Book, First Edition

352 citations · 1.1k across the 43 of their papers we have counts for

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Showing 2019Show all

7 papers · 1 filter

astro-ph.CO2019★ 28 cited

Dust moments: towards a new modelling of the galactic dust emission for CMB B-modes analysis

Anna Mangilli, Jonathan Aumont, Aditya Rotti +4

The characterization of the spectral energy distribution (SED) of dust emission has become a critical issue in the quest for primordial B-modes. The dust SED is often approximated…

astro-ph.CO2019★ 10 cited

New Horizons in Cosmology with Spectral Distortions of the Cosmic Microwave Background

J. Chluba, M. H. Abitbol, N. Aghanim +27

Voyage 2050 White Paper highlighting the unique science opportunities using spectral distortions of the cosmic microwave background (CMB). CMB spectral distortions probe many proce…

astro-ph.CO2019★ 39 cited

Microwave Spectro-Polarimetry of Matter and Radiation across Space and Time

Jacques Delabrouille, Maximilian H. Abitbol, Nabila Aghanim +77

This paper discusses the science case for a sensitive spectro-polarimetric survey of the microwave sky. Such a survey would provide a tomographic and dynamic census of the three-di…

astro-ph.CO2019★ 51 cited

CMB Spectral Distortions: Status and Prospects

A. Kogut, M. H. Abitbol, J. Chluba +5

Departures of the energy spectrum of the cosmic microwave background (CMB) from a perfect blackbody probe a fundamental property of the universe -- its thermal history. Current upp…

astro-ph.IM2019★ 79 cited

The Simons Observatory: Astro2020 Decadal Project Whitepaper

The Simons Observatory Collaboration, Maximilian H. Abitbol, Shunsuke Adachi +280

The Simons Observatory (SO) is a ground-based cosmic microwave background (CMB) experiment sited on Cerro Toco in the Atacama Desert in Chile that promises to provide breakthrough…

astro-ph.CO2019★ 39 cited

The Power Spectra of Polarized, Dusty Filaments

Kevin M. Huffenberger, Aditya Rotti, David C. Collins

We develop an analytic model for the power spectra of polarized filamentary structures as a way to study the Galactic polarization foreground to the Cosmic Microwave Background. Ou…