The Simons Observatory (SO) is a new cosmic microwave background experiment being built on Cerro Toco in Chile, due to begin observations in the early 2020s. We describe the …
MH Abitbol, S Adachi, P Ade, J Aguirre… - arXiv preprint arXiv …, 2019 - arxiv.org
The Simons Observatory (SO) is a ground-based cosmic microwave background (CMB) experiment sited on Cerro Toco in the Atacama Desert in Chile that promises to provide …
N Galitzki, A Ali, KS Arnold, PC Ashton… - … , and Far-Infrared …, 2018 - spiedigitallibrary.org
The Simons Observatory (SO) will make precision temperature and polarization measurements of the cosmic microwave background (CMB) using a series of telescopes …
N Galitzki, T Tsan, J Spisak, M Randall… - The Astrophysical …, 2024 - iopscience.iop.org
Abstract The Simons Observatory (SO) is a cosmic microwave background survey experiment that includes small-aperture telescopes (SATs) observing from an altitude of …
Advances in cosmic microwave background (CMB) science depend on increasing the number of sensitive detectors observing the sky. New instruments deploy large arrays of …
We present geometrical and physical optics simulation results for the Simons Observatory Large Aperture Telescope. This work was developed as part of the general design process …
Abstract The Simons Observatory is a ground-based cosmic microwave background experiment that consists of three 0.4 m small-aperture telescopes and one 6 m Large …
Z Xu, GE Chesmore, S Adachi, AM Ali… - arXiv preprint arXiv …, 2020 - arxiv.org
Controlling stray light at millimeter wavelengths requires special optical design and selection of absorptive materials that should be compatible with cryogenic operating …
CCAT-prime will be a 6-meter aperture telescope operating from sub-mm to mm wavelengths, located at 5600 meters elevation on Cerro Chajnantor in the Atacama Desert …