The Simons Observatory: Design, integration, and testing of the small aperture telescopes
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2024
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| author | Galitzki, Nicholas Tsan, Tran Spisak, Jake Randall, Michael Silva-Feaver, Max Seibert, Joseph Lashner, Jacob Adachi, Shunsuke Adkins, Sean M. Alford, Thomas Arnold, Kam Ashton, Peter C. Austermann, Jason E. Baccigalupi, Carlo Bazarko, Andrew Beall, James A. Bhimani, Sanah Bixler, Bryce Coppi, Gabriele Corbett, Lance Crowley, Kevin D. Crowley, Kevin T. Day-Weiss, Samuel Dicker, Simon Dow, Peter N. Duell, Cody J. Duff, Shannon M. Gerras, Remington G. Groh, John C. Gudmundsson, Jon E. Harrington, Kathleen Hasegawa, Masaya Healy, Erin Henderson, Shawn W. Hubmayr, Johannes Iuliano, Jeffrey Johnson, Bradley R. Keating, Brian Keller, Ben Kiuchi, Kenji Kofman, Anna M. Koopman, Brian J. Kusaka, Akito Lee, Adrian T. Lew, Richard A. Lin, Lawrence T. Link, Michael J Lucas, Tammy J. Lungu, Marius Mangu, Aashrita McMahon, Jeffrey J Miller, Amber D. Moore, Jenna E. Morshed, Magdy Nakata, Hironobu Nati, Federico Newburgh, Laura B. Nguyen, David V. Niemack, Michael D. Page, Lyman A. Sakaguri, Kana Sakurai, Yuki Rao, Mayuri Sathyanarayana Saunders, Lauren J. Shroyer, Jordan E. Sugiyama, Junna Tajima, Osamu Takeuchi, Atsuto Bua, Refilwe Tanah Teply, Grant Terasaki, Tomoki Ullom, Joel N. Van Lanen, Jeffrey L. Vavagiakis, Eve M. Vissers, Michael R Walters, Liam Wang, Yuhan Xu, Zhilei Yamada, Kyohei Zheng, Kaiwen |
| author_facet | Galitzki, Nicholas Tsan, Tran Spisak, Jake Randall, Michael Silva-Feaver, Max Seibert, Joseph Lashner, Jacob Adachi, Shunsuke Adkins, Sean M. Alford, Thomas Arnold, Kam Ashton, Peter C. Austermann, Jason E. Baccigalupi, Carlo Bazarko, Andrew Beall, James A. Bhimani, Sanah Bixler, Bryce Coppi, Gabriele Corbett, Lance Crowley, Kevin D. Crowley, Kevin T. Day-Weiss, Samuel Dicker, Simon Dow, Peter N. Duell, Cody J. Duff, Shannon M. Gerras, Remington G. Groh, John C. Gudmundsson, Jon E. Harrington, Kathleen Hasegawa, Masaya Healy, Erin Henderson, Shawn W. Hubmayr, Johannes Iuliano, Jeffrey Johnson, Bradley R. Keating, Brian Keller, Ben Kiuchi, Kenji Kofman, Anna M. Koopman, Brian J. Kusaka, Akito Lee, Adrian T. Lew, Richard A. Lin, Lawrence T. Link, Michael J Lucas, Tammy J. Lungu, Marius Mangu, Aashrita McMahon, Jeffrey J Miller, Amber D. Moore, Jenna E. Morshed, Magdy Nakata, Hironobu Nati, Federico Newburgh, Laura B. Nguyen, David V. Niemack, Michael D. Page, Lyman A. Sakaguri, Kana Sakurai, Yuki Rao, Mayuri Sathyanarayana Saunders, Lauren J. Shroyer, Jordan E. Sugiyama, Junna Tajima, Osamu Takeuchi, Atsuto Bua, Refilwe Tanah Teply, Grant Terasaki, Tomoki Ullom, Joel N. Van Lanen, Jeffrey L. Vavagiakis, Eve M. Vissers, Michael R Walters, Liam Wang, Yuhan Xu, Zhilei Yamada, Kyohei Zheng, Kaiwen |
| contents | The Simons Observatory (SO) is a cosmic microwave background (CMB) survey experiment that includes small-aperture telescopes (SATs) observing from an altitude of 5,200 m in the Atacama Desert in Chile. The SO SATs will cover six spectral bands between 27 and 280 GHz to search for primordial B-modes to a sensitivity of $σ(r)=0.002$, with quantified systematic errors well below this value. Each SAT is a self-contained cryogenic telescope with a 35$^\circ$ field of view, 42 cm diameter optical aperture, 40 K half-wave plate, 1 K refractive optics, and $<0.1$ K focal plane that holds $>12,000$ TES detectors. We describe the nominal design of the SATs and present details about the integration and testing for one operating at 93 and 145 GHz. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2405_05550 |
| institution | arXiv |
| publishDate | 2024 |
| record_format | arxiv |
| spellingShingle | The Simons Observatory: Design, integration, and testing of the small aperture telescopes Galitzki, Nicholas Tsan, Tran Spisak, Jake Randall, Michael Silva-Feaver, Max Seibert, Joseph Lashner, Jacob Adachi, Shunsuke Adkins, Sean M. Alford, Thomas Arnold, Kam Ashton, Peter C. Austermann, Jason E. Baccigalupi, Carlo Bazarko, Andrew Beall, James A. Bhimani, Sanah Bixler, Bryce Coppi, Gabriele Corbett, Lance Crowley, Kevin D. Crowley, Kevin T. Day-Weiss, Samuel Dicker, Simon Dow, Peter N. Duell, Cody J. Duff, Shannon M. Gerras, Remington G. Groh, John C. Gudmundsson, Jon E. Harrington, Kathleen Hasegawa, Masaya Healy, Erin Henderson, Shawn W. Hubmayr, Johannes Iuliano, Jeffrey Johnson, Bradley R. Keating, Brian Keller, Ben Kiuchi, Kenji Kofman, Anna M. Koopman, Brian J. Kusaka, Akito Lee, Adrian T. Lew, Richard A. Lin, Lawrence T. Link, Michael J Lucas, Tammy J. Lungu, Marius Mangu, Aashrita McMahon, Jeffrey J Miller, Amber D. Moore, Jenna E. Morshed, Magdy Nakata, Hironobu Nati, Federico Newburgh, Laura B. Nguyen, David V. Niemack, Michael D. Page, Lyman A. Sakaguri, Kana Sakurai, Yuki Rao, Mayuri Sathyanarayana Saunders, Lauren J. Shroyer, Jordan E. Sugiyama, Junna Tajima, Osamu Takeuchi, Atsuto Bua, Refilwe Tanah Teply, Grant Terasaki, Tomoki Ullom, Joel N. Van Lanen, Jeffrey L. Vavagiakis, Eve M. Vissers, Michael R Walters, Liam Wang, Yuhan Xu, Zhilei Yamada, Kyohei Zheng, Kaiwen Instrumentation and Methods for Astrophysics Cosmology and Nongalactic Astrophysics The Simons Observatory (SO) is a cosmic microwave background (CMB) survey experiment that includes small-aperture telescopes (SATs) observing from an altitude of 5,200 m in the Atacama Desert in Chile. The SO SATs will cover six spectral bands between 27 and 280 GHz to search for primordial B-modes to a sensitivity of $σ(r)=0.002$, with quantified systematic errors well below this value. Each SAT is a self-contained cryogenic telescope with a 35$^\circ$ field of view, 42 cm diameter optical aperture, 40 K half-wave plate, 1 K refractive optics, and $<0.1$ K focal plane that holds $>12,000$ TES detectors. We describe the nominal design of the SATs and present details about the integration and testing for one operating at 93 and 145 GHz. |
| title | The Simons Observatory: Design, integration, and testing of the small aperture telescopes |
| topic | Instrumentation and Methods for Astrophysics Cosmology and Nongalactic Astrophysics |
| url | https://arxiv.org/abs/2405.05550 |