PICO：暴胀与宇宙起源探测者
天体物理仪器与方法
2019-08-21 v1 宇宙学与河外天体物理
星系天体物理
高能物理 - 理论
摘要
暴胀与宇宙起源探测者（PICO）是一项拟议的探测级空间任务，由工作在 20 至 800 GHz 频段间的成像偏振计组成。我们描述了 PICO 可实现的科学目标，其灵敏度相当于 3300 多个 Planck 任务，以及技术实现、进度与成本。
引用
@article{arxiv.1908.07495,
title = {PICO: Probe of Inflation and Cosmic Origins},
author = {S. Hanany and M. Alvarez and E. Artis and P. Ashton and J. Aumont and R. Aurlien and R. Banerji and R. B. Barreiro and J. G. Bartlett and S. Basak and N. Battaglia and J. Bock and K. K. Boddy and M. Bonato and J. Borrill and F. Bouchet and F. Boulanger and B. Burkhart and J. Chluba and D. Chuss and S. Clark and J. Cooperrider and B. P. Crill and G. De Zotti and J. Delabrouille and E. Di Valentino and J. Didier and O. Dore and H. K. Eriksen and J. Errard and T. Essinger-Hileman and S. Feeney and J. Filippini and L. Fissel and R. Flauger and U. Fuskeland and V. Gluscevic and K. M. Gorski and D. Green and B. Hensley and D. Herranz and J. C. Hill and E. Hivon and R. Hlozek and J. Hubmayr and B. R. Johnson and W. Jones and T. Jones and L. Knox and A. Kogut and M. Lopez-Caniego and C. Lawrence and A. Lazarian and Z. Li and M. Madhavacheril and J. B. Melin and J. Meyers and C. Murray and M. Negrello and G. Novak and R. O'Brient and C. Paine and T. Pearson and L. Pogosian and C. Pryke and G. Puglisi and M. Remazeilles and G. Rocha and M. Schmittfull and D. Scott and P. Shirron and I. Stephens and B. Sutin and M. Tomasi and A. Trangsrud and A. van Engelen and F. Vansyngel and I. K. Wehus and Q. Wen and S. Xu and K. Young and A. Zonca},
journal= {arXiv preprint arXiv:1908.07495},
year = {2019}
}
备注
APC White Paper submitted to the Astro2020 decadal panel; 10 page version of the 50 page mission study report arXiv:1902.10541