activity
20182022
most citedTwo-year Cosmology Large Angular Scale Surveyor (CLASS) Observations: A Measurement of Circular Polarization at 40 GHz

25 citations · 57 across the 5 of their papers we have counts for

collaborators

12 papers

astro-ph.IM20222 cited

The Simons Observatory: Design and Measured Performance of a Carbon Fiber Strut for a Cryogenic Truss

Kevin D. Crowley, Peter Dow, Jordan E. Shroyer +25

We present the design and measured performance of a new carbon fiber strut design that is used in a cryogenically cooled truss for the Simons Observatory Small 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.IM20204 cited

Control and systems software for the Cosmology Large Angular Scale Surveyor (CLASS)

Matthew A. Petroff, John W. Appel, Charles L. Bennett +16

The Cosmology Large Angular Scale Surveyor (CLASS) is an array of polarization-sensitive millimeter wave telescopes that observes ~70% of the sky at frequency bands centered near 4…

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…

astro-ph.EP2020

Venus Observations at 40 and 90 GHz with CLASS

Sumit Dahal, Michael K. Brewer, John W. Appel +30

Using the Cosmology Large Angular Scale Surveyor, we measure the disk-averaged absolute Venus brightness temperature to be 432.3 2.8 K and 355.6 1.3 K in the Q and W fr…