Cmb-hd: Astro2020 RFI Response

Neelima Sehgal, Simone Aiola, Yashar Akrami, Kaustuv moni Basu, Michael Boylan-Kolchin, Sean Bryan, Caitlin M Casey, Sébastien Clesse, Francis-Yan Cyr-Racine, Luca Di Mascolo, Simon Dicker, Thomas Essinger-Hileman, Simone Ferraro, George Fuller, Nicholas Galitzki, Dongwon Han, Matthew Hasselfield, Gil Holder, Bhuvnesh Jain, Bradley R. JohnsonMatthew Johnson, Pamela Klaassen, Amanda MacInnis, Mathew Madhavacheril, Philip Mauskopf, Daan Meerburg, Joel Meyers, Tony Mroczkowski, Suvodip Mukherjee, Moritz Münchmeyer, Sigurd Kirkevold Naess, Daisuke Nagai, Toshiya Namikawa, Laura Newburgh, Nam Nguyen, Michael Niemack, Benjamin D. Oppenheimer, Elena Pierpaoli, Emmanuel Schaan, Blake Sherwin, Anže Slosar, David Spergel, Eric Switzer, Pranjal Trivedi, Yu-Dai Tsai, Alexander van Engelen, Benjamin Wandelt, Edward Wollack

Research output: Working paperPreprintAcademic

Abstract

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.
Original languageEnglish
DOIs
Publication statusSubmitted - 28-Feb-2020
Externally publishedYes

Keywords

  • astro-ph.CO
  • astro-ph.IM
  • hep-ph

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