Simons Observatory large aperture receiver simulation overview
John L. Orlowski-Scherer, Ningfeng Zhu, Zhilei Xu, Aamir Ali, Kam S., Arnold, Peter C. Ashton, Gabriele Coppi, Mark Devlin, Simon Dicker, Nicholas, Galitzki, Patricio A. Gallardo, Brian Keating, Adrian T. Lee, Michele Limon,, Marius Lungu, Andrew May, Jeff McMahon

TL;DR
This paper presents detailed simulation results for the Simons Observatory's large aperture telescope receiver, focusing on structural, thermal, and vibrational analyses to ensure optimal performance and integrity.
Contribution
It provides comprehensive simulation-based design validation for the SO large aperture receiver, including structural, thermal, and vibrational analyses.
Findings
Structural support system designs validated by FEA
Thermal model ensures compliance with design requirements
Vibrational mode analysis informs suppression strategies
Abstract
The Simons Observatory (SO) will make precision temperature and polarization measurements of the cosmic microwave background (CMB) using a series of telescopes which will cover angular scales between one arcminute and tens of degrees, contain over 60,000 detectors, and sample frequencies between 27 and 270 GHz. SO will consist of a six-meter-aperture telescope coupled to over 30,000 detectors along with an array of half-meter aperture refractive cameras, which together couple to an additional 30,000+ detectors. SO will measure fundamental cosmological parameters of our universe, find high redshift clusters via the Sunyaev-Zeldovich effect, constrain properties of neutrinos, and seek signatures of dark matter through gravitational lensing. In this paper we will present results of the simulations of the SO large aperture telescope receiver (LATR). We will show details of simulations…
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