Cold optical design for the Large Aperture Simons Observatory telescope
| dc.contributor.author | Dicker, S. R. | |
| dc.contributor.author | Gallardo, P. A. | |
| dc.contributor.author | Gudmundsson, J. E | |
| dc.contributor.author | Mauskopf, P. D. | |
| dc.contributor.author | Ali, A. | |
| dc.contributor.author | Ashton, P. C. | |
| dc.contributor.author | Coppi, G. | |
| dc.contributor.author | Devlin, M. J. | |
| dc.contributor.author | Galitzki, N. | |
| dc.contributor.author | Ho, S. P. | |
| dc.contributor.author | Hill, C. A. | |
| dc.contributor.author | Hubmayr, J. | |
| dc.contributor.author | Keating, B. | |
| dc.contributor.author | Lee, A. T. | |
| dc.contributor.author | Limon, M. | |
| dc.contributor.author | Matsuda, F. | |
| dc.contributor.author | McMahon, J. | |
| dc.contributor.author | Niemack, M. D. | |
| dc.contributor.author | Orlowski-Scherer, J. L. | |
| dc.contributor.author | Piccirillo, L. | |
| dc.contributor.author | Salatino, M. | |
| dc.contributor.author | Simon, S. M. | |
| dc.contributor.author | Staggs, S. T. | |
| dc.contributor.author | Thornton, R. | |
| dc.contributor.author | Ullom, J. N. | |
| dc.contributor.author | Vavagiakis, E. M. | |
| dc.contributor.author | Wollack, E. J. | |
| dc.contributor.author | Xu, Z. | |
| dc.contributor.author | Zhu, N. | |
| dc.contributor.department | Faculty of Physical Sciences | |
| dc.date.accessioned | 2025-11-20T10:02:27Z | |
| dc.date.available | 2025-11-20T10:02:27Z | |
| dc.date.issued | 2018-08-15 | |
| dc.description.abstract | The Simons Observatory will consist of a single large (6 m diameter) telescope and a number of smaller (0.5 m diameter) refracting telescopes designed to measure the polarization of the Cosmic Microwave Background to unprecedented accuracy. The large aperture telescope is the same design as the CCAT-prime telescope, a modified Crossed Dragone design with a field-of-view of over 7.8 degrees diameter at 90 GHz. This paper presents an overview of the cold reimaging optics for this telescope and what drove our choice of 350-400 mm diameter silicon lenses in a 2.4 m cryostat over other possibilities. We will also consider the future expandability of this design to CMB Stage-4 and beyond. | en |
| dc.format.extent | 7489666 | |
| dc.identifier.citation | Dicker, S R, Gallardo, P A, Gudmundsson, J E, Mauskopf, P D, Ali, A, Ashton, P C, Coppi, G, Devlin, M J, Galitzki, N, Ho, S P, Hill, C A, Hubmayr, J, Keating, B, Lee, A T, Limon, M, Matsuda, F, McMahon, J, Niemack, M D, Orlowski-Scherer, J L, Piccirillo, L, Salatino, M, Simon, S M, Staggs, S T, Thornton, R, Ullom, J N, Vavagiakis, E M, Wollack, E J, Xu, Z & Zhu, N 2018 'Cold optical design for the Large Aperture Simons Observatory telescope'. | en |
| dc.identifier.other | 110605169 | |
| dc.identifier.other | a1a2457b-2bf9-4daf-81b7-63fef4be6174 | |
| dc.identifier.other | ArXiv: http://arxiv.org/abs/1808.05058v2 | |
| dc.identifier.uri | https://hdl.handle.net/20.500.11815/7957 | |
| dc.language.iso | en | |
| dc.rights | info:eu-repo/semantics/restrictedAccess | en |
| dc.subject | astro-ph.IM | en |
| dc.title | Cold optical design for the Large Aperture Simons Observatory telescope | en |
| dc.type | /dk/atira/pure/researchoutput/researchoutputtypes/workingpaper/preprint | en |
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