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20002026
most citedProtons in near earth orbit

205 citations · 2.2k across the 98 of their papers we have counts for

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Showing astro-ph.COShow all

12 papers · 1 filter

astro-ph.CO2024

Spectral Imaging with QUBIC: building astrophysical components from Time-Ordered-Data using Bolometric Interferometry

M. Regnier, T. Laclavere, J-Ch. Hamilton +33

The detection of B-modes in the CMB polarization pattern is a major issue in modern cosmology and must therefore be handled with analytical methods that produce reliable results. W…

astro-ph.CO2024

Spectral Imaging with QUBIC: building frequency maps from Time-Ordered-Data using Bolometric Interferometry

M. Regnier, T. Laclavère, J-Ch. Hamilton +34

The search for relics from the inflation era in the form of B-mode polarization of the CMB is a major challenge in cosmology. The main obstacle appears to come from the complexity…

astro-ph.CO2024

LiteBIRD Science Goals and Forecasts. Mapping the Hot Gas in the Universe

M. Remazeilles, M. Douspis, J. A. Rubiño-Martín +104

We assess the capabilities of the LiteBIRD mission to map the hot gas distribution in the Universe through the thermal Sunyaev-Zeldovich (SZ) effect. Our analysis relies on compreh…

astro-ph.CO2023

Measuring the CMB primordial B-modes with Bolometric Interferometry

A. Mennella, P. Ade, A. Almela +111

The Q&U Bolometric Interferometer for Cosmology (QUBIC) is the first bolometric interferometer designed to measure the primordial B-mode polarization of the Cosmic Microwave Backgr…

astro-ph.CO2023★ 23 cited

Tensor-to-scalar ratio forecasts for extended LiteBIRD frequency configurations

U. Fuskeland, J. Aumont, R. Aurlien +114

LiteBIRD is a planned JAXA-led CMB B-mode satellite experiment aiming for launch in the late 2020s, with a primary goal of detecting the imprint of primordial inflationary gravitat…

astro-ph.CO2022

Polarization angle requirements for CMB B-mode experiments. Application to the LiteBIRD satellite

P. Vielva, E. Martínez-González, F. J. Casas +68

A methodology to provide the polarization angle requirements for different sets of detectors, at a given frequency of a CMB polarization experiment, is presented. The uncertainties…

astro-ph.CO2019★ 1 cited

Spectral Distortions of the CMB as a Probe of Inflation, Recombination, Structure Formation and Particle Physics

J. Chluba, A. Kogut, S. P. Patil +98

Following the pioneering observations with COBE in the early 1990s, studies of the cosmic microwave background (CMB) have focused on temperature and polarization anisotropies. CMB…

astro-ph.CO2017

Forecast analysis and focal plane optimization for a multi-frequency CMB B-modes polarization experiment: the case of LSPE

Roberto Mainini, Massimo Gervasi, Mario Zannoni +1

We present an optimization scheme for the focal plane of a multi-frequency CMB B-modes experiment with a fixed number of detectors and apply it to the specific case of LSPE experim…

astro-ph.CO2013★ 27 cited

An improved upper limit to the CMB circular polarization at large angular scales

R. Mainini, D. Minelli, M. Gervasi +7

Circular polarization of the Cosmic Microwave Background (CMB) offers the possibility of detecting rotations of the universe and magnetic fields in the primeval universe or in dist…

astro-ph.CO2012

A template of atmospheric molecular oxygen circularly polarized emission for CMB experiments

Giulio Fabbian, Sebastiano Spinelli, Massimo Gervasi +2

We compute the polarized signal from atmospheric molecular oxygen due to Zeeman effect in the Earth magnetic field for various sites suitable for CMB measurements such as South Pol…

astro-ph.CO2010

Cosmological observations in the radio domain: the contribution of extragalactic sources

Andrea Tartari, Mario Zannoni, Massimo Gervasi +2

The low frequency tail of the CMB spectrum, down along the radio range (~1 GHz), may carry weak spectral distortions which are fingerprints of processes occurred during different e…

astro-ph.CO2010★ 5 cited

SAGACE: the Spectroscopic Active Galaxies And Clusters Explorer

P. De Bernardis, D. Bagliani, A. Bardi +42

The SAGACE experiment consists of a mm/sub-mm telescope with a 3-m diameter primary mirror, coupled to a cryogenic multi-beam differential spectrometer. SAGACE explores the sky in…