Manuel Aravena, Jason Austermann, Kaustuv Basu, Nicholas Battaglia, Benjamin Beringue, Frank Bertoldi, J. Richard Bond, Patrick Breysse, Ricardo Bustos, Scott C… 展开作者
Manuel Aravena, Jason Austermann, Kaustuv Basu, Nicholas Battaglia, Benjamin Beringue, Frank Bertoldi, J. Richard Bond, Patrick Breysse, Ricardo Bustos, Scott Chapman, Steve Choi, Dongwoo Chung, Nicholas Cothard, Bradley Dober, Cody Duell, Shannon Duff, Rolando Dunner, Jens Erler, Michel Fich, Laura Fissel, Simon Foreman, Patricio Gallardo, Jiansong Gao, Riccardo Giovanelli, Urs Graf, Martha Haynes, Terry Herter, Gene Hilton, Renee Hlozek, Johannes Hubmayr, Doug Johnstone, Laura Keating, Eiichiro Komatsu, Benjamin Magnelli, Phil Mauskopf, Jeffrey McMahon, P. Daniel Meerburg, Joel Meyers, Norm Murray, Michael Niemack, Thomas Nikola, Michael Nolta, Stephen Parshley, Roberto Puddu, Dominik Riechers, Erik Rosolowsky, Sara Simon, Gordon Stacey, Jason Stevens, Juergen Stutzki, Alexander Van Engelen, Eve Vavagiakis, Marco Viero, Michael Vissers, Samantha Walker, Bugao Zou
The Cerro Chajnantor Atacama Telescope-prime (CCAT-prime) is a new 6-m, off-axis, low-emissivity, large field-of-view submillimeter telescope scheduled for first light in the last quarter of 2021. In summary, (a) CCAT-prime uniquely combines a large field-of-view (up to 8-deg), low emissivity telescope (< 2%) and excellent atmospheric transmission (5600-m site) to achieve unprecedented survey capability in the submillimeter. (b) Over five years, CCAT-prime first generation science will address the physics of star formation, galaxy evolution, and galaxy cluster formation; probe the re-ionization of the Universe; improve constraints on new particle species; and provide for improved removal of dust foregrounds to aid the search for primordial gravitational waves. (c) The Observatory is being built with non-federal funds (~ \$40M in private and international investments). Public funding is needed for instrumentation (~ \$8M) and operations (\$1-2M/yr). In return, the community will be able to participate in survey planning and gain access to curated data sets. (d) For second generation science, CCAT-prime will be uniquely positioned to contribute high-frequency capabilities to the next generation of CMB surveys in partnership with the CMB-S4 and/or the Simons Observatory projects or revolutionize wide-field, sub-millimetter line intensity mapping surveys.
CCAT: Silicon-Platelet Feedhorns for Submillimeter Wavelengths
National Institute of Standards and Technology（美国国家标准与技术研究院）；University of Colorado（科罗拉多大学）；University of British Columbia（不列颠哥伦比亚大学）；Dalhousie University（达尔豪斯大学）；University of California, Riverside（加州大学河滨分校）；Cornell University（康奈尔大学）
CCAT: The Prime-Cam Instrument for the Fred Young Submillimeter Telescope -- Overview and Status
Duke University（杜克大学）；Cornell University（康奈尔大学）；Universidad Diego Portales（迭戈·波特莱斯大学）；National Institute of Standards and Technology（美国国家标准与技术研究院）；Universität Bonn（波恩大学）；University of British Columbia（不列颠哥伦比亚大学）；Dalhousie University（达尔豪斯大学）；University of California, Riverside（加州大学河滨分校）；University of Waterloo（滑铁卢大学）；Queen’s University（女王大学）；NRC Herzberg Astronomy and Astrophysics（NRC赫茨伯格天体物理学研究所）；University of Victoria（维多利亚大学）；Cornell Center for Astrophysics and Planetary Sciences, Cornell University（康奈尔大学天体物理学与行星科学中心）；University of Cologne（科隆大学）
CCAT: Magnetic Sensitivity Measurements of Kinetic Inductance Detectors
National Institutes of Standards and Technology（国家标准与技术研究院）；University of California, Riverside（加州大学河滨分校）；Dalhousie University（达尔豪斯大学）；University of British Columbia（不列颠哥伦比亚大学）；Duke University（杜克大学）
CCAT: Optical Responsivity, Noise, and Readout Optimization of KIDs for Prime-Cam
University of California, Riverside（加州大学河滨分校）；Cornell University（康奈尔大学）；University of British Columbia（不列颠哥伦比亚大学）；Dalhousie University（达尔豪斯大学）；Duke University（杜克大学）
CCAT: Design and Characterization of the 350 GHz Instrument Module
Cornell University（康奈尔大学）；National Institute of Standards and Technology（美国国家标准与技术研究院）；University of British Columbia（不列颠哥伦比亚大学）；Dalhousie University（达尔豪斯大学）；University of California, Riverside（加州大学河滨分校）；Duke University（杜克大学）；University of Colorado, Boulder（科罗拉多大学博尔德分校）
CCAT: Characterization of the first science-grade MKID array for the Prime-Cam 850 GHz module
University of British Columbia（不列颠哥伦比亚大学）；National Institute of Standards and Technology（美国国家标准与技术研究院）；Dalhousie University（达尔豪斯大学）；NRC Herzberg Astronomy & Astrophysics Research Centre（NRC赫茨伯格天文学与天体物理学研究中心）；University of California, Riverside（加州大学河滨分校）；Cornell University（康奈尔大学）；Duke University（杜克大学）；Johns Hopkins University（约翰斯·霍普金斯大学）
CCAT: The 410 GHz camera module for FYST - design and testing of the MKID focal plane
Dalhousie University（达尔豪斯大学）；University of British Columbia（不列颠哥伦比亚大学）；University of Victoria（维多利亚大学）；National Institute of Standards and Technology（美国国家标准与技术研究院）；McGill University（麦吉尔大学）；NRC Herzberg Astronomy & Astrophysics Research Centre（加拿大国家研究委员会赫茨伯格天文学与天体物理学研究中心）；Cornell University（康奈尔大学）；Duke University（杜克大学）；Johns Hopkins University（约翰斯·霍普金斯大学）
CCAT: Detector Noise Limited Performance of the RFSoC-based Readout Electronics for mm/sub-mm/far-IR KIDs
University of British Columbia（不列颠哥伦比亚大学）；University of Victoria（维多利亚大学）；Herzberg Astronomy and Astrophysics Research Centre, National Research Council Canada（加拿大国家研究委员会赫茨伯格天文学与天体物理学研究中心）；Cornell University（康奈尔大学）；National Institute of Standards and Technology（美国国家标准与技术研究院）；University of California, Riverside（加州大学河滨分校）；Arizona State University（亚利桑那州立大学）
CCAT: Mod-Cam Readout Overview and Flexible Stripline Performance
Cornell University（康奈尔大学）；University of British Columbia（不列颠哥伦比亚大学）；Dalhousie University（达尔豪斯大学）；University of California, Riverside（加州大学河滨分校）；Arizona State University（亚利桑那州立大学）；Duke University（杜克大学）
CCAT: a two-octave 1.024 GHz KID readout featuring an overlap-channel polyphase synthesis filter bank on RFSoC
University of British Columbia（不列颠哥伦比亚大学）；Johns Hopkins University（约翰斯·霍普金斯大学）；Dalhousie University（达尔豪斯大学）；McGill University（麦吉尔大学）；University of California, Riverside（加州大学河滨分校）；Cornell University（康奈尔大学）
Site Quality Analysis for an Indian Submillimeter Telescope: A Reanalysis-Based Approach
Raman Research Institute（拉曼研究所）；School of Earth and Space Exploration, Arizona State University（亚利桑那州立大学地球与空间探索学院）；Department of Physics, California Institute of Technology（加州理工学院物理系）；Jet Propulsion Laboratory（喷气推进实验室）
The Atacama Large Aperture Submillimeter Telescope (AtLAST): enabling large-scale sub-mm science beyond 2030
Institute of Theoretical Astrophysics, University of Oslo（奥斯陆大学理论天体物理研究所）；Institute of Space Sciences (ICE-CSIC)（空间科学研究所（ICE-CSIC））；Institut d’Estudis Espacials de Catalunya (IEEC)（加泰罗尼亚空间研究学院（IEEC））；Instituto de Astrofísica de Canarias (IAC)（加那利群岛天体物理研究所（IAC））；Departamento de Astrofísica, Universidad de La Laguna（拉古纳大学天体物理学系）；European Southern Observatory (ESO)（欧洲南方天文台（ESO））；OHB Digital Connect（OHB数字连接公司）；Department of Technology Systems, University of Oslo（奥斯陆大学技术系统系）；MPIfR（马克斯·普朗克射电天文研究所）；UK Astronomy Technology Centre, Royal Observatory Edinburgh（英国天体技术中心，爱丁堡皇家天文台）；IPARCOS-UCM, Universidad Complutense de Madrid（马德里康普顿斯大学IPARCOS研究中心）；Department of EEC Engineering, University of Pretoria（比勒陀利亚大学电气工程与电子工程系）；University of Tokyo（东京大学）；INAF Osservatorio Astronomico di Cagliari（意大利国家天体物理研究所卡利亚里天文台）；Nagoya University（名古屋大学）；Rosseland Centre for Solar Physics, University of Oslo（奥斯陆大学罗斯兰太阳物理中心）；ESO（欧洲南方天文台）；ICREA（加泰罗尼亚卓越研究奖计划）；Université Paris-Saclay, Université Paris Cité, CEA, CNRS, AIM（巴黎萨克雷大学、巴黎西岱大学、法国原子能和替代能源委员会、法国国家科学研究中心、AIM）；TU Delft（代尔夫特理工大学）
