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Article . 2014 . Peer-reviewed
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PRISM (Polarized Radiation Imaging and Spectroscopy Mission): an extended white paper

Authors: PRISM Collaboration; André, Philippe; Baccigalupi, Carlo; Banday, Anthony; Barbosa, Domingos; Barreiro, Belen; Bartlett, James; +136 Authors

PRISM (Polarized Radiation Imaging and Spectroscopy Mission): an extended white paper

Abstract

PRISM (Polarized Radiation Imaging and Spectroscopy Mission) was proposed to ESA in May 2013 as a large-class mission for investigating within the framework of the ESA Cosmic Vision program a set of important scientific questions that require high resolution, high sensitivity, full-sky observations of the sky emission at wavelengths ranging from millimeter-wave to the far-infrared. PRISM's main objective is to explore the distant universe, probing cosmic history from very early times until now as well as the structures, distribution of matter, and velocity flows throughout our Hubble volume. PRISM will survey the full sky in a large number of frequency bands in both intensity and polarization and will measure the absolute spectrum of sky emission more than three orders of magnitude better than COBE FIRAS. The aim of this Extended White Paper is to provide a more detailed overview of the highlights of the new science that will be made possible by PRISM

Figure 8 replaced by the correct version, affiliations of authors added, and minor changes to match the published JCAP version

Countries
Ireland, France, France, France, Netherlands, France, France, France, Italy, Netherlands, France, Netherlands, United Kingdom, France, United Kingdom, Italy, United Kingdom, Poland, United Kingdom, Italy, France, Italy, Spain, Spain, Italy, France, France, Italy
Keywords

[SDU.ASTR.CO] Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], Cosmology and Nongalactic Astrophysics (astro-ph.CO), [SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], Astronomy, 500, cosmological parameters from CMBR, FOS: Physical sciences, MICROWAVE BACKGROUND SPECTRUM; SOUTH-POLE TELESCOPE; COSMOLOGICAL HYDROGEN RECOMBINATION; PROBE WMAP OBSERVATIONS; POWER SPECTRUM; DARK-MATTER; RELATIVISTIC CORRECTIONS; EARLY UNIVERSE; SUBMILLIMETER GALAXIES; CMB POLARIZATION, 520, [PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], [PHYS.ASTR.CO] Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], cmbr detectors; cosmological parameters from cmbr; cmbr experiments, CMBR experiments, CMBR detectors; CMBR experiments; cosmological parameters from CMBR, CMBR detectors, CMBR detectors; CMBR experiments; cosmological parameters from CMBR; MICROWAVE BACKGROUND SPECTRUM; SOUTH-POLE TELESCOPE; COSMOLOGICAL HYDROGEN RECOMBINATION; PROBE WMAP OBSERVATIONS; POWER SPECTRUM; DARK-MATTER; RELATIVISTIC CORRECTIONS; EARLY UNIVERSE; SUBMILLIMETER GALAXIES; CMB POLARIZATION, Astrophysics - Cosmology and Nongalactic Astrophysics

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This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
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popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
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impulse
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