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CERN Accelerating science

Article
Report number arXiv:1310.1554
Title The Polarized Radiation Imaging and Spectroscopy Mission
Author(s)

André, Philippe (AIM, Saclay) ; Baccigalupi, Carlo (SISSA, Trieste) ; Banday, Anthony (IRAP, Toulouse ; Toulouse III U.) ; Barbosa, Domingos (Aveiro U.) ; Barreiro, Belen (Cantabria U., Santander) ; Bartlett, James (APC, Paris ; Caltech, JPL) ; Bartolo, Nicola (Padua U. ; INFN, Padua) ; Battistelli, Elia (Rome U.) ; Battye, Richard (Manchester U.) ; Bendo, George (Manchester U.) ; Benoȋt, Alain (Manchester U.) ; Bernard, Jean-Philippe (IRAP, Toulouse) ; Bersanelli, Marco (Milan U. ; IASF, Milan) ; Béthermin, Matthieu (European Southern Observ.) ; Bielewicz, Pawel (SISSA, Trieste) ; Bonaldi, Anna (Manchester U.) ; Bouchet, François (Paris, Inst. Astrophys. ; UPMC, Paris (main)) ; Boulanger, François (Orsay, IAS) ; Brand, Jan (INFN, Ferrara ; IASF, Bologna) ; Bucher, Martin (APC, Paris) ; Burigana, Carlo (IASF, Bologna ; Ferrara U.) ; Cai, Zhen-Yi (SISSA, Trieste ; Xiamen U. ; Hefei, CUST) ; Camus, Philippe (Neel Lab, Grenoble) ; Casas, Francisco (Cantabria U., Santander) ; Casasola, Viviana (IASF, Bologna) ; Castex, Guillaume (APC, Paris) ; Challinor, Anthony (Paris, Inst. Astrophys. ; Cambridge U., KICC ; Cambridge U., DAMTP) ; Chluba, Jens (Johns Hopkins U.) ; Chon, Gayoung (Garching, Max Planck Inst., MPE) ; Colafrancesco, Sergio (Witwatersrand U.) ; Comis, Barbara (LPSC, Grenoble) ; Cuttaia, Francesco (IASF, Bologna) ; D'Alessandro, Giuseppe (Rome U.) ; Da Silva, Antonio (Porto U., Astron. Dept.) ; Davis, Richard (Manchester U.) ; de Avillez, Miguel (Evora U. ; Berlin, Tech. U.) ; de Bernardis, Paolo (Rome U.) ; de Petris, Marco (Rome U.) ; de Rosa, Adriano (IASF, Bologna) ; de Zotti, Gianfranco (SISSA, Trieste ; Padua Observ.) ; Delabrouille, Jacques (APC, Paris) ; Désert, François-Xavier (Grenoble Observ.) ; Dickinson, Clive (Manchester U.) ; Diego, Jose Maria (Cantabria U., Santander) ; Dunkley, Joanna (Oxford U.) ; Enßlin, Torsten (Garching, Max Planck Inst.) ; Errard, Josquin (LBL, Berkeley) ; Falgarone, Edith (Paris Observ.) ; Ferreira, Pedro (Oxford U.) ; Ferrière, Katia (IRAP, Toulouse) ; Finelli, Fabio (IASF, Bologna ; INFN, Bologna) ; Fletcher, Andrew (Newcastle upon Tyne U.) ; Fosalba, Pablo (ICE, Bellaterra) ; Fuller, Gary (Manchester U.) ; Galli, Silvia (Paris, Inst. Astrophys. ; UPMC, Paris (main)) ; Ganga, Ken (APC, Paris) ; García-Bellido, Juan (Madrid, IFT) ; Ghribi, Adnan (APC, Paris) ; Giard, Martin (IRAP, Toulouse ; Toulouse III U.) ; Giraud-Héraud, Yannick (APC, Paris) ; Gonzalez-Nuevo, Joaquin (SISSA, Trieste ; Cantabria U., Santander) ; Grainge, Keith (Manchester U.) ; Gruppuso, Alessandro (IASF, Bologna) ; Hall, Alex (Edinburgh U., Inst. Astron.) ; Hamilton, Jean-Christophe (APC, Paris) ; Haverkorn, Marijke (Nijmegen U., IMAPP ; Leiden Observ.) ; Hernandez-Monteagudo, Carlos (CEFCA, Teruel) ; Herranz, Diego (Cantabria U., Santander) ; Jackson, Mark (APC, Paris) ; Jaffe, Andrew (Imperial Coll., London) ; Khatri, Rishi (Garching, Max Planck Inst.) ; Kunz, Martin (Geneva U., Dept. Theor. Phys. ; African Inst. Math. Sci., Cape Town) ; Lamagna, Luca (Rome U.) ; Lattanzi, Massimiliano (INFN, Ferrara ; Ferrara U.) ; Leahy, Paddy (Manchester U.) ; Lesgourgues, Julien (Ecole Polytechnique, Lausanne ; CERN ; Annecy, LAPTH) ; Liguori, Michele (Padua U.) ; Liuzzo, Elisabetta (IASF, Bologna) ; Lopez-Caniego, Marcos (Cantabria U., Santander) ; Macias-Perez, Juan (LPSC, Grenoble) ; Maffei, Bruno (Manchester U.) ; Maino, Davide (Milan U.) ; Mangilli, Anna (Paris, Inst. Astrophys.) ; Martinez-Gonzalez, Enrique (Cantabria U., Santander) ; Martins, Carlos J.A.P. (Porto U.) ; Masi, Silvia (Rome U.) ; Massardi, Marcella (IASF, Bologna) ; Matarrese, Sabino (Padua U. ; INFN, Padua) ; Melchiorri, Alessandro (Rome U. ; INFN, Rome) ; Melin, Jean-Baptiste (Porto U.) ; Mennella, Aniello (Milan U.) ; Mignano, Arturo (IASF, Bologna) ; Miville-Deschênes, Marc-Antoine (Orsay, IAS) ; Monfardini, Alessandro (Neel Lab, Grenoble) ; Murphy, Anthony (NUIM, Maynooth) ; Naselsky, Pavel (Bohr Inst.) ; Nati, Federico (Rome U.) ; Natoli, Paolo (INFN, Ferrara ; IASF, Bologna ; Ferrara U. ; ASDC, Frascati) ; Negrello, Mattia (Padua Observ.) ; Noviello, Fabio (Manchester U.) ; O'Sullivan, Créidhe (NUIM, Maynooth) ; Paci, Francesco (SISSA, Trieste) ; Pagano, Luca (Rome U. ; INFN, Rome) ; Paladino, Rosita (IASF, Bologna ; Bologna U.) ; Palanque-Delabrouille, Nathalie (IRFU, SPP, Saclay) ; Paoletti, Daniela (IASF, Milan ; IASF, Bologna) ; Peiris, Hiranya (University Coll. London) ; Perrotta, Francesca (SISSA, Trieste) ; Piacentini, Francesco (Rome U.) ; Piat, Michel (APC, Paris) ; Piccirillo, Lucio (Manchester U.) ; Pisano, Giampaolo (Manchester U. ; Cardiff U.) ; Polenta, Gianluca (ASDC, Frascati ; Rome Observ.) ; Pollo, Agnieszka (Jagiellonian U., Astron. Observ. ; Warsaw, Inst. Nucl. Studies) ; Ponthieu, Nicolas (Neel Lab, Grenoble) ; Remazeilles, Mathieu (APC, Paris ; Manchester U.) ; Ricciardi, Sara (IASF, Bologna) ; Roman, Matthieu (APC, Paris) ; Rosset, Cyrille (APC, Paris) ; Rubino-Martin, Jose-Alberto (IAC, La Laguna ; Laguna U., Tenerife) ; Salatino, Maria (Rome U.) ; Schillaci, Alessandro (Rome U.) ; Shellard, Paul (Cambridge U., DAMTP) ; Silk, Joseph (Paris, Inst. Astrophys. ; Johns Hopkins U. ; Oxford U.) ; Starobinsky, Alexei (Landau ITP, Chernogolovka) ; Stompor, Radek (APC, Paris) ; Sunyaev, Rashid (Garching, Max Planck Inst.) ; Tartari, Andrea (APC, Paris) ; Terenzi, Luca (IASF, Bologna) ; Toffolatti, Luigi (Cantabria U., Santander ; Oviedo U.) ; Tomasi, Maurizio (Milan U. ; IASF, Milan) ; Trappe, Neil (NUIM, Maynooth) ; Tristram, Matthieu (Orsay, LAL) ; Trombetti, Tiziana (IASF, Bologna) ; Tucci, Marco (Geneva U., Dept. Theor. Phys.) ; Van de Weijgaert, Rien (Groningen U.) ; Van Tent, Bartjan (Orsay, LPT) ; Verde, Licia (ICC, Barcelona U. ; ICREA, Barcelona ; Inst. Theor. Astrophys., Oslo) ; Vielva, Patricio (Cantabria U., Santander) ; Wandelt, Ben (Paris, Inst. Astrophys. ; ILP, Paris) ; Watson, Robert (Manchester U.) ; Withington, Stafford (Cambridge U., DAMTP) ; Cabrera, Nicolas (Madrid, IFT)

Publication 2014-02-05
Imprint 06 Oct 2013
Number of pages 55
Note Comments: 55 pages, extended version of the white paper submitted in answer to the call for science themes for the second and third L-class missions within the ESA Cosmic Vision programme
Figure 8 replaced by the correct version, affiliations of authors added, and minor changes to match the published JCAP version
In: JCAP 02 (2014) 006
DOI 10.1088/1475-7516/2014/02/006
Subject category Astrophysics and Astronomy
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
Copyright/License arXiv nonexclusive-distrib. 1.0

5$ as a function of redshift. Right panel: The completeness of the detection for all three effects, as a function of mass. Objects more massive than $4 \times 10^{13}\Msolar$ are detected at more than 5$\sigma$ at all redshifts, a limit extending well down into the relatively unexplored group range (red line). \mission\ is able to measure peculiar velocities over most of the cluster range, i.e., for $M>2 \times 10^{14}\Msolar$ (dashed blue line), and relativistic effects, giving access to cluster temperature, for the more massive systems (dot-dashed green line), both out to high redshift. Note that in practice, the detection depth will be lower close to the galactic plane, where a fraction of the clusters will inevitably be missed (although this should be only a very small fraction of the total)." width="200px"/> 5$ as a function of redshift. Right panel: The completeness of the detection for all three effects, as a function of mass. Objects more massive than $4 \times 10^{13}\Msolar$ are detected at more than 5$\sigma$ at all redshifts, a limit extending well down into the relatively unexplored group range (red line). \mission\ is able to measure peculiar velocities over most of the cluster range, i.e., for $M>2 \times 10^{14}\Msolar$ (dashed blue line), and relativistic effects, giving access to cluster temperature, for the more massive systems (dot-dashed green line), both out to high redshift. Note that in practice, the detection depth will be lower close to the galactic plane, where a fraction of the clusters will inevitably be missed (although this should be only a very small fraction of the total)." width="200px"/> Show more plots


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 Record created 2013-10-08, last modified 2024-06-27


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