机译：SPT-3G：南极望远镜的彩色接收器
Fermi National Accelerator Laboratory;
School of Physics and Astronomy Cardiff University;
Kavli Institute for Particle Astrophysics and Cosmology Stanford University;
National Institute of Standards and Technology;
Department of Physics University of California;
Kavli Institute for Cosmological Physics University of Chicago;
Kavli Institute for Cosmological Physics University of Chicago;
Kavli Institute for Cosmological Physics University of Chicago;
Fermi National Accelerator Laboratory;
Kavli Institute for Cosmological Physics University of Chicago;
High-Energy Physics Division Argonne National Laboratory;
Kavli Institute for Cosmological Physics University of Chicago;
Kavli Institute for Cosmological Physics University of Chicago;
High-Energy Physics Division Argonne National Laboratory;
Kavli Institute for Cosmological Physics University of Chicago;
SLAC National Accelerator Laboratory;
Department of Physics McGill University;
Kavli Institute for Cosmological Physics University of Chicago;
Department of Physics University of California;
National Institute of Standards and Technology;
Department of Physics University of California;
Material Science Division Argonne National Laboratory;
Department of Physics McGill University;
Kavli Institute for Cosmological Physics University of Chicago;
CASA Department of Astrophysical and Planetary Sciences University of Colorado;
Physics Department Case Western Reserve University;
Material Science Division Argonne National Laboratory;
Department of Physics McGill University;
Department of Physics University of California;
CASA Department of Astrophysical and Planetary Sciences University of Colorado;
High-Energy Physics Division Argonne National Laboratory;
Department of Physics University of California;
Kavli Institute for Cosmological Physics University of Chicago;
National Institute of Standards and Technology;
Astronomy Department University of Illinois;
Department of Physics University of California;
Department of Physics University of California;
Kavli Institute for Particle Astrophysics and Cosmology Stanford University;
Department of Physics University of California;
Fermi National Accelerator Laboratory;
Material Science Division Argonne National Laboratory;
Department of Physics University of California;
Astronomy Department University of Illinois;
Physics Department Case Western Reserve University;
Fermi National Accelerator Laboratory;
High-Energy Physics Division Argonne National Laboratory;
Department of Physics University of Chicago;
Kavli Institute for Particle Astrophysics and Cosmology Stanford University;
Department of Physics University of California;
Kavli Institute for Cosmological Physics University of Chicago;
Kavli Institute for Cosmological Physics University of Chicago;
Kavli Institute for Cosmological Physics University of Chicago;
University of Chicago;
Department of Physics McGill University;
Astronomy Department University of Illinois;
Dunlap Institute for Astronomy and Astrophysics University of Toronto;
Fermi National Accelerator Laboratory;
Department of Physics McGill University;
Material Science Division Argonne National Laboratory;
Kavli Institute for Cosmological Physics University of Chicago;
Kavli Institute for Cosmological Physics University of Chicago;
Material Science Division Argonne National Laboratory;
Material Science Division Argonne National Laboratory;
Fermi National Accelerator Laboratory;
School of Physics University of Melbourne;
Physics Department Case Western Reserve University;
Kavli Institute for Cosmological Physics University of Chicago;
CASA Department of Astrophysical and Planetary Sciences University of Colorado;
Department of Physics University of California;
Kavli Institute for Cosmological Physics University of Chicago;
Three-Speed Logic Inc;
Kavli Institute for Cosmological Physics University of Chicago;
Harvard-Smithsonian Center for Astrophysics;
Kavli Institute for Particle Astrophysics and Cosmology Stanford University;
Department of Physics University of California;
Kavli Institute for Cosmological Physics University of Chicago;
Kavli Institute for Particle Astrophysics and Cosmology Stanford University;
School of Physics and Astronomy Cardiff University;
National Institute of Standards and Technology;
Dunlap Institute for Astronomy and Astrophysics University of Toronto;
Astronomy Department University of Illinois;
High-Energy Physics Division Argonne National Laboratory;
Department of Physics University of California;
High-Energy Physics Division Argonne National Laboratory;
Kavli Institute for Particle Astrophysics and Cosmology Stanford University;
Department of Astronomy and Astrophysics University of Toronto;
CMB; Instrumentation; Polarimetry; SPT-3G;
机译：SPT-3G：南极望远镜的彩色接收器
机译：南极望远镜检测以前未经证实的普朗克早期的Sunyaev-zel'dovich在南半球的群集
机译：黑暗能量调查第1次结果：暗能调查y1银河弱透镜与南极望远镜+普朗克CMB弱镜头的互相关
机译：SPT-3G：南极望远镜的下一代宇宙微波背景极化实验
机译：银河簇压力曲线和下一代南极望远镜科学和仪器
机译：使用Lofar射频望远镜作为被动式放射系统中的接收器的实验验证
机译：SPT-3G：南极望远镜的下一代宇宙微波背景极化实验
机译：spT-3G：南极望远镜的下一代宇宙微波背景偏振实验。
