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arXiv · 1908.07495

PICO: Probe of Inflation and Cosmic Origins

S. Hanany·M. Alvarez·E. Artis·P. Ashton·J. Aumont·R. Aurlien·R. Banerji·R. B. Barreiro·J. G. Bartlett·S. Basak·N. Battaglia·J. Bock·K. K. Boddy·M. Bonato·J. Borrill·F. Bouchet·F. Boulanger·B. Burkhart·J. Chluba·D. Chuss·S. Clark·J. Cooperrider·B. P. Crill·G. De Zotti·J. Delabrouille·E. Di Valentino·J. Didier·O. Dore·H. K. Eriksen·J. Errard·T. Essinger-Hileman·S. Feeney·J. Filippini·L. Fissel·R. Flauger·U. Fuskeland·V. Gluscevic·K. M. Gorski·D. Green·B. Hensley·D. Herranz·J. C. Hill·E. Hivon·R. Hlozek·J. Hubmayr·B. R. Johnson·W. Jones·T. Jones·L. Knox·A. Kogut·M. Lopez-Caniego·C. Lawrence·A. Lazarian·Z. Li·M. Madhavacheril·J. B. Melin·J. Meyers·C. Murray·M. Negrello·G. Novak·R. O'Brient·C. Paine·T. Pearson·L. Pogosian·C. Pryke·G. Puglisi·M. Remazeilles·G. Rocha·M. Schmittfull·D. Scott·P. Shirron·I. Stephens·B. Sutin·M. Tomasi·A. Trangsrud·A. van Engelen·F. Vansyngel·I. K. Wehus·Q. Wen·S. Xu·K. Young·A. Zonca
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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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S. Hanany, M. Alvarez, E. Artis, P. Ashton, J. Aumont, R. Aurlien, R. Banerji, R. B. Barreiro, J. G. Bartlett, S. Basak, N. Battaglia, J. Bock, K. K. Boddy, M. Bonato, J. Borrill, F. Bouchet, F. Boulanger, B. Burkhart, J. Chluba, D. Chuss, S. Clark, J. Cooperrider, B. P. Crill, G. De Zotti, J. Delabrouille, E. Di Valentino, J. Didier, O. Dore, H. K. Eriksen, J. Errard, T. Essinger-Hileman, S. Feeney, J. Filippini, L. Fissel, R. Flauger, U. Fuskeland, V. Gluscevic, K. M. Gorski, D. Green, B. Hensley, D. Herranz, J. C. Hill, E. Hivon, R. Hlozek, J. Hubmayr, B. R. Johnson, W. Jones, T. Jones, L. Knox, A. Kogut, M. Lopez-Caniego, C. Lawrence, A. Lazarian, Z. Li, M. Madhavacheril, J. B. Melin, J. Meyers, C. Murray, M. Negrello, G. Novak, R. O'Brient, C. Paine, T. Pearson, L. Pogosian, C. Pryke, G. Puglisi, M. Remazeilles, G. Rocha, M. Schmittfull, D. Scott, P. Shirron, I. Stephens, B. Sutin, M. Tomasi, A. Trangsrud, A. van Engelen, F. Vansyngel, I. K. Wehus, Q. Wen, S. Xu, K. Young, A. Zonca. 2019-08-20. PICO: Probe of Inflation and Cosmic Origins. https://arxiv.org/abs/1908.07495

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