by Shaul Hanany, Marcelo Alvarez, Emmanuel Artis, Peter Ashton, Jonathan Aumont, Ragnhild Aurlien, Ranajoy Banerji, R. Belen Barreiro, James G. Bartlett, Soumen Basak, Nick Battaglia, Jamie Bock, Kimberly K. Boddy, Matteo Bonato, Julian Borrill, François Bouchet, François Boulanger, Blakesley Burkhart, Jens Chluba, David Chuss, Susan E. Clark, Joelle Cooperrider, Brendan P. Crill, Gianfranco De Zotti, Jacques Delabrouille, Eleonora Di Valentino, Joy Didier, Olivier Doré, Hans K. Eriksen, Josquin Errard, Tom Essinger-Hileman, Stephen Feeney, Jeffrey Filippini, Laura Fissel, Raphael Flauger, Unni Fuskeland, Vera Gluscevic, Krzysztof M. Gorski, Dan Green, Shaul Hanany, Brandon Hensley, Diego Herranz, J. Colin Hill, Eric Hivon, Renée Hložek, Johannes Hubmayr, Bradley R. Johnson, William Jones, Terry Jones, Lloyd Knox, Al Kogut, Marcos López-Caniego, Charles Lawrence, Alex Lazarian, Zack Li, Mathew Madhavacheril, Jean-Baptiste Melin, Joel Meyers, Calum Murray, Mattia Negrello, Giles Novak, Roger O’Brient, Christopher Paine, Tim Pearson, Levon Pogosian, Clem Pryke, Giuseppe Puglisi, Mathieu Remazeilles, Graca Rocha, Marcel Schmittfull, Douglas Scott, Peter Shirron, Ian Stephens, Brian Sutin, Maurizio Tomasi, Amy Trangsrud, Alexander van Engelen, Flavien Vansyngel, Ingunn K. Wehus, Qi Wen, Siyao Xu, Karl Young, and Andrea Zonca
Published onSep 30, 2019
PICO: Probe of Inflation and Cosmic Origins
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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.
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