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2020-02-28
CMB-HD: Astro2020 RFI Response
Neelima SehgalSimone AiolaYashar AkramiKaustuv moni BasuMichael Boylan-KolchinSean BryanCaitlin M CaseySébastien ClesseFrancis-Yan Cyr-RacineLuca Di MascoloSimon DickerThomas Essinger-HilemanSimone FerraroGeorge FullerNicholas GalitzkiDongwon HanMatthew HasselfieldGil HolderBhuvnesh JainBradley R. JohnsonMatthew JohnsonPamela KlaassenAmanda MacInnisMathew MadhavacherilPhilip MauskopfDaan MeerburgJoel MeyersTony MroczkowskiSuvodip MukherjeeMoritz MünchmeyerSigurd Kirkevold NaessDaisuke NagaiToshiya NamikawaLaura NewburghNam NguyenMichael NiemackBenjamin D. OppenheimerElena PierpaoliEmmanuel SchaanBlake SherwinAnže SlosarDavid SpergelEric SwitzerPranjal TrivediYu-Dai TsaiAlexander van EngelenBenjamin WandeltEdward Wollack
文献摘要
CMB-HD is a proposed ultra-deep (0.5 uk-arcmin), high-resolution (15 arcseconds) millimeter-wave survey over half the sky that would answer many outstanding questions in both fundamental physics of the Universe and astrophysics. This survey would be delivered in 7.5 years of observing 20,000 square degrees, using two new 30-meter-class off-axis cross-Dragone telescopes to be located at Cerro Toco in the Atacama Desert. Each telescope would field 800,000 detectors (200,000 pixels), for a total of 1.6 million detectors.
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