Freeform three-mirror anastigmatic large-aperture telescope and receiver optics for CMB-S4
dc.contributor.author | Gallardo, Patricio A. | |
dc.contributor.author | Puddu, Roberto | |
dc.contributor.author | Harrington, Kathleen | |
dc.contributor.author | Benson, Bradford | |
dc.contributor.author | Carlstrom, John E. | |
dc.contributor.author | Dicker, Simon R. | |
dc.contributor.author | Emerson, Nick | |
dc.contributor.author | Gudmundsson, Jon E. | |
dc.contributor.author | Limon, Michele | |
dc.contributor.author | Mcmahon, Jeff | |
dc.contributor.author | Nagy, Johanna M. | |
dc.contributor.author | Natoli, Tyler | |
dc.contributor.author | Niemack, Michael D. | |
dc.contributor.author | Padin, Stephen | |
dc.contributor.author | Ruhl, John | |
dc.contributor.author | Simon, Sara M. | |
dc.date.accessioned | 2025-01-20T17:08:16Z | |
dc.date.available | 2025-01-20T17:08:16Z | |
dc.date.issued | 2024 | |
dc.description.abstract | CMB-S4, the next-generation ground-based cosmic microwave background (CMB) observatory, will provide detailed maps of the CMB at millimeter wavelengths to dramatically advance our understanding of the origin and evolution of the universe. CMB-S4 will deploy large- and small-aperture telescopes with hundreds of thousands of detectors to observe the CMB at arcminute and degree resolutions at millimeter wavelengths. Inflationary science benefits from a deep delensing survey at arcminute resolutions capable of observing a large field of view at millimeter wavelengths. This kind of survey acts as a complement to a degree angular resolution survey. The delensing survey requires a nearly uniform distribution of cameras per frequency band across the focal plane. We present a large-throughput (9.4 degrees field of view), large-aperture (5-m diameter) freeform three-mirror anastigmatic telescope and an array of 85 cameras for CMB observations at arcminute resolutions, which meets the needs of the delensing survey of CMB-S4. A detailed prescription of this three-mirror telescope and cameras is provided, with a series of numerical calculations that indicates expected optical performance and mechanical tolerance. | |
dc.fuente.origen | WOS | |
dc.identifier.doi | 10.1364/AO.501744 | |
dc.identifier.eissn | 2155-3165 | |
dc.identifier.issn | 1559-128X | |
dc.identifier.uri | https://doi.org/10.1364/AO.501744 | |
dc.identifier.uri | https://repositorio.uc.cl/handle/11534/90934 | |
dc.identifier.wosid | WOS:001173250400001 | |
dc.issue.numero | 2 | |
dc.language.iso | en | |
dc.pagina.final | 321 | |
dc.pagina.inicio | 310 | |
dc.revista | Applied optics | |
dc.rights | acceso restringido | |
dc.title | Freeform three-mirror anastigmatic large-aperture telescope and receiver optics for CMB-S4 | |
dc.type | artículo | |
dc.volumen | 63 | |
sipa.index | WOS | |
sipa.trazabilidad | WOS;2025-01-12 |
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