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20182022
most citedThe design of the Ali CMB Polarization Telescope receiver

22 citations · 43 across the 4 of their papers we have counts for

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astro-ph.IM20222 cited

Simons Observatory Focal-Plane Module: Detector Re-biasing With Bias-step Measurements

Yuhan Wang, Tanay Bhandarkar, Steve K. Choi +14

The Simons Observatory is a ground-based cosmic microwave background survey experiment that consists of three 0.5 m small-aperture telescopes and one 6 m large-aperture telescope,…

astro-ph.IM2021

The Simons Observatory: the Large Aperture Telescope (LAT)

Zhilei Xu, Shunsuke Adachi, Peter Ade +57

The Simons Observatory (SO) is a Cosmic Microwave Background (CMB) experiment to observe the microwave sky in six frequency bands from 30GHz to 290GHz. The Observatory -- at

astro-ph.IM2021

The Simons Observatory Large Aperture Telescope Receiver

Ningfeng Zhu, Tanay Bhandarkar, Gabriele Coppi +68

The Simons Observatory (SO) Large Aperture Telescope Receiver (LATR) will be coupled to the Large Aperture Telescope located at an elevation of 5,200 m on Cerro Toco in Chile. The…

astro-ph.IM202112 cited

Simons Observatory Small Aperture Telescope overview

Kenji Kiuchi, Shunsuke Adachi, Aamir M. Ali +51

The Simons Observatory (SO) is a cosmic microwave background (CMB) experiment from the Atacama Desert in Chile comprising three small-aperture telescopes (SATs) and one large-apert…

astro-ph.IM202122 cited

The design of the Ali CMB Polarization Telescope receiver

Maria Salatino, Jason E. Austermann, Keith L. Thompson +72

Ali CMB Polarization Telescope (AliCPT-1) is the first CMB degree-scale polarimeter to be deployed on the Tibetan plateau at 5,250m above sea level. AliCPT-1 is a 90/150 GHz 72 cm…

astro-ph.IM20207 cited

The Simons Observatory: the Large Aperture Telescope Receiver (LATR) Integration and Validation Results

Zhilei Xu, Tanay Bhandarkar, Gabriele Coppi +42

The Simons Observatory (SO) will observe the cosmic microwave background (CMB) from Cerro Toco in the Atacama Desert of Chile. The observatory consists of three 0.5 m Small Apertur…