Simons Observatory: Predeployment Performance of a Large Aperture Telescope Optics Tube in the 90 and 150 GHz Spectral Bands

Abstract The Simons Observatory will map the temperature and polarization over half of the sky at millimeter wavelengths in six spectral bands from the Atacama Desert in Chile. These data will provide new insights into the genesis, content, and history of our Universe, the astrophysics of galaxies and galaxy clusters, objects in our solar system, and time-varying astrophysical phenomena. This ambitious new instrument suite, initially comprising three 0.5 m diameter small aperture telescopes and one 6 m diameter large aperture telescope, is designed using a common combination of new technologies and new implementations to realize an observatory significantly more sensitive than the previous generation. In this paper, we present the predeployment performance of the first mid-frequency “optics tube,” which will be fielded on the large aperture telescope with sensitivity to the 90 and 150 GHz spectral bands. This optics tube contains lenses, filters, detectors, and readout components, all of which operate at cryogenic temperatures. It is one of seven that form the core of the large aperture telescope receiver in its initial deployment. We describe this optics tube, including details of comprehensive testing methods, new techniques for beam and passband characterization, and its measured performance. The performance metrics include beams, optical efficiency, passbands, and forecasts for the on-sky performance of the system. We forecast a sensitivity that exceeds the requirements of the large aperture telescope with greater than 30% margin in each spectral band and predict that the instrument will realize diffraction-limited performance and the expected detector passbands.

Authors

Publication Details

Journal
The Astrophysical Journal Supplement Series
Published
2025-01-01
DOI
https://doi.org/10.3847/1538-4365/ad8cdc
Citations
3
Primary Topic
Cosmology and Gravitation Theories
Type
article
Field-Weighted Citation Impact
3.46

Funders

Controls
|||
ALL TIME
JAN
FEB
MAR
APR
MAY
JUN
JUL
AUG
SEP
OCT
article

Simons Observatory: Predeployment Performance of a Large Aperture Telescope Optics Tube in the 90 and 150 GHz Spectral Bands

Jon E. Gudmundsson, Bradley R. Johnson, Thomas Alford, Jeffrey L. Van Lanen et al.
3 citations
The Astrophysical Journal Supplement Series
Cosmology and Gravitation Theories
3.46
article

Simons Observatory: Predeployment Performance of a Large Aperture Telescope Optics Tube in the 90 and 150 GHz Spectral Bands

Jon E. Gudmundsson, Bradley R. Johnson, Thomas Alford, Jeffrey L. Van Lanen, Anna M. Kofman, Nicholas Galitzki, Erin Healy, Kaiwen Zheng, Kathleen Harrington, Tammy J. Lucas, Shreya Sutariya, A. O. Bazarko, Rita Sonka, Shannon M. Duff, Jason E. Austermann, Eve M. Vavagiakis, Michael D. Niemack, Jenna Moore, James A. Beall, Joseph E. Golec, Andrew C. Thomas, Tran Tsan, D. Dutcher, Richard A. Lew, Joel N. Ullom, Yuhan Wang, Michael Vissers, Jeffrey Iuliano, Carlos Sierra, Tanay Bhandarkar, F. Nati, Saianeesh K. Haridas, Mark J. Devlin, Simon Dicker, Maximiliano Silva-Feaver, Johannes Hubmayr, Claire S. Lessler, Robinjeet Singh, Michael J. Link, Robert Thornton, J. C. Groh, Benjamin L. Schmitt, Jeffrey McMahon, Grace Chesmore, Peter N. Dow
article en
3 citations

Abstract

Abstract The Simons Observatory will map the temperature and polarization over half of the sky at millimeter wavelengths in six spectral bands from the Atacama Desert in Chile. These data will provide new insights into the genesis, content, and history of our Universe, the astrophysics of galaxies and galaxy clusters, objects in our solar system, and time-varying astrophysical phenomena. This ambitious new instrument suite, initially comprising three 0.5 m diameter small aperture telescopes and one 6 m diameter large aperture telescope, is designed using a common combination of new technologies and new implementations to realize an observatory significantly more sensitive than the previous generation. In this paper, we present the predeployment performance of the first mid-frequency “optics tube,” which will be fielded on the large aperture telescope with sensitivity to the 90 and 150 GHz spectral bands. This optics tube contains lenses, filters, detectors, and readout components, all of which operate at cryogenic temperatures. It is one of seven that form the core of the large aperture telescope receiver in its initial deployment. We describe this optics tube, including details of comprehensive testing methods, new techniques for beam and passband characterization, and its measured performance. The performance metrics include beams, optical efficiency, passbands, and forecasts for the on-sky performance of the system. We forecast a sensitivity that exceeds the requirements of the large aperture telescope with greater than 30% margin in each spectral band and predict that the instrument will realize diffraction-limited performance and the expected detector passbands.

The Astrophysical Journal Supplement SeriesVol. 276(1)
Simons Foundation
Decent work and economic growth
Openalex Percentile: Top 9%
Cosmology and Gravitation Theories
3.46
AI Navigator

Ask Laika to Summarize, Analyze, and Connect papers live on the map.

Summarize Papers & Methodologies

Extract key findings, datasets, and comparative methods across publications.

Benchmark Rankings & Visual Analytics

Rank top research institutions, authors, funders, topics, and journals by Field-Weighted Citation Impact (FWCI) and paper volume with instant charts.

Connect Distant Disciplines

Bridge topological clusters on the map to find hidden collaborative intersections.