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• W3100132516 endingPage "480" @default.
• W3100132516 startingPage "431" @default.
• W3100132516 abstract "The cosmic microwave background radiation (CMB) is now firmly established as a fundamental and essential probe of the geometry, constituents, and birth of the Universe. The CMB is a potent observable because it can be measured with precision and accuracy. Just as importantly, theoretical models of the Universe can predict the characteristics of the CMB to high accuracy, and those predictions can be directly compared to observations. There are multiple aspects associated with making a precise measurement. In this review, we focus on optical components for the instrumentation used to measure the CMB polarization and temperature anisotropy. We begin with an overview of general considerations for CMB observations and discuss common concepts used in the community. We next consider a variety of alternatives available for a designer of a CMB telescope. Our discussion is guided by the ground and balloon-based instruments that have been implemented over the years. In the same vein, we compare the arc-minute resolution Atacama Cosmology Telescope (ACT) and the South Pole Telescope (SPT). CMB interferometers are presented briefly. We conclude with a comparison of the four CMB satellites, Relikt, COBE, WMAP, and Planck, to demonstrate a remarkable evolution in design, sensitivity, resolution, and complexity over the past thirty years." @default.
• W3100132516 created "2020-11-23" @default.
• W3100132516 creator A5033083354 @default.
• W3100132516 creator A5044452776 @default.
• W3100132516 creator A5052249023 @default.
• W3100132516 date "2013-01-01" @default.
• W3100132516 modified "2023-09-25" @default.
• W3100132516 title "CMB Telescopes and Optical Systems" @default.
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