PICO: Probe of Inflation and Cosmic Origins
Date Issued
2019
Author(s)
Hanany, Shaul
•
Alvarez, Marcelo
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Artis, Emmanuel
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Ashton, Peter
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Aumont, Jonathan
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Aurlien, Ragnhild
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Banerji, Ranajoy
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Barreiro, R. Belen
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Bartlett, James G.
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Basak, Soumen
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Battaglia, Nick
•
Bock, Jamie
•
Boddy, Kimberly K.
•
•
Borrill, Julian
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Bouchet, François
•
Boulanger, François
•
Burkhart, Blakesley
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Chluba, Jens
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Chuss, David
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Clark, Susan E.
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Cooperrider, Joelle
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Crill, Brendan P.
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DE ZOTTI, Gianfranco
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Delabrouille, Jacques
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Di Valentino, Eleonora
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Didier, Joy
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Doré, Olivier
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Eriksen, Hans K.
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Errard, Josquin
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Essinger-Hileman, Tom
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Feeney, Stephen
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Filippini, Jeffrey
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Fissel, Laura
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Flauger, Raphael
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Fuskeland, Unni
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Gluscevic, Vera
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Gorski, Krzysztof M.
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Green, Dan
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Hensley, Brandon
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Herranz, Diego
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Hill, J. Colin
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Hivon, Eric
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Hložek, Renée
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Hubmayr, Johannes
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Johnson, Bradley R.
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Jones, William
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Jones, Terry
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Knox, Lloyd
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Kogut, Al
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López-Caniego, Marcos
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Lawrence, Charles
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Lazarian, Alex
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Li, Zack
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Madhavacheril, Mathew
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Melin, Jean-Baptiste
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Meyers, Joel
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Murray, Calum
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Negrello, Mattia
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Novak, Giles
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O'Brient, Roger
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Paine, Christopher
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Pearson, Tim
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Pogosian, Levon
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Pryke, Clem
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Puglisi, Giuseppe
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Remazeilles, Mathieu
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Rocha, Graca
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Schmittfull, Marcel
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Scott, Douglas
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Shirron, Peter
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Stephens, Ian
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Sutin, Brian
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Tomasi, Maurizio
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Trangsrud, Amy
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van Engelen, Alexander
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Vansyngel, Flavien
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Wehus, Ingunn K.
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Wen, Qi
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Xu, Siyao
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Young, Karl
•
Zonca, Andrea
Abstract
The Probe of Inflation and Cosmic Origins (PICO) is a proposed probe-scale space mission consisting of an imaging polarimeter operating in frequency bands between 20 and 800 GHz. We describe the science achievable by PICO, which has sensitivity equivalent to more than 3300 Planck missions, the technical implementation, the schedule and cost.
Volume
51
Issue
7
Start page
194
Issn Identifier
2330-9458
Ads BibCode
2019BAAS...51g.194H
Rights
open.access
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