Search Results for author: Michael D. Niemack

Found 11 papers, 5 papers with code

The Integration and Testing Program for the Simons Observatory Large Aperture Telescope Optics Tubes

no code implementations3 Feb 2021 Kathleen Harrington, Carlos Sierra, Grace Chesmore, Shreya Sutariya, Aamir M. Ali, Steve K. Choi, Nicholas F. Cothard, Simon Dicker, Nicholas Galitzki, Shuay-Pwu Patty Ho, Anna M. Kofman, Brian J. Koopman, Jack Lashner, Jeff McMahon, Michael D. Niemack, John Orlowski-Scherer, Joseph Seibert, Max Silva-Feaver, Eve M. Vavagiakis, Zhilei Xu, Ningfeng Zhu

The Simons Observatory (SO) will be a cosmic microwave background (CMB) survey experiment with three small-aperture telescopes and one large-aperture telescope, which will observe from the Atacama Desert in Chile.

Instrumentation and Methods for Astrophysics

In situ Performance of the Low Frequency Arrayfor Advanced ACTPol

no code implementations7 Jan 2021 Yaqiong Li, Jason E. Austermann, James A. Beall, Sarah Marie Bruno, Steve K. Choi, Nicholas F. Cothard, Kevin T. Crowley, Shannon M. Duff, Shuay-Pwu Patty Ho, Joseph E. Golec, Gene C. Hilton, Matthew Hasselfield, Johannes Hubmay, Brian J. Koopman, Marius Lungu, Jeff McMahon, Michael D. Niemack, LymanA. Page, Maria Salatino, Sara M. Simon, Suzanne T. Staggs, Jason R. Stevens, Joel N. Ullom, Eve M. Vavagiakis, YuHan Wang, Edward J. Wollack, Zhilei Xu

The Advanced Atacama Cosmology Telescope Polarimeter (AdvACT) \cite{thornton} is an upgrade for the Atacama Cosmology Telescope using Transition Edge Sensor (TES) detector arrays to measure cosmic microwave background (CMB) temperature and polarization anisotropies in multiple frequencies.

Instrumentation and Methods for Astrophysics

CCAT-prime: Designs and status of the first light 280 GHz MKID array and Mod-Cam receiver

no code implementations18 Dec 2020 Cody J. Duell, Eve M. Vavagiakis, Jason Austermann, Scott C. Chapman, Steve K. Choi, Nicholas F. Cothard, Brad Dober, Patricio Gallardo, Jiansong Gao, Christopher Groppi, Terry L. Herter, Gordon J. Stacey, Zachary Huber, Johannes Hubmayr, Doug Johnstone, Yaqiong Li, Philip Mauskopf, Jeff McMahon, Michael D. Niemack, Thomas Nikola, Kayla Rossi, Sara Simon, Adrian K. Sinclair, Michael Vissers, Jordan Wheeler, Bugao Zou

The CCAT-prime project's first light array will be deployed in Mod-Cam, a single-module testbed and first light cryostat, on the Fred Young Submillimeter Telescope (FYST) in Chile's high Atacama desert in late 2022.

Instrumentation and Methods for Astrophysics

Comparing complex impedance and bias step measurements of Simons Observatory transition edge sensors

no code implementations15 Dec 2020 Nicholas F. Cothard, Aamir M. Ali, Jason E. Austermann, Steve K. Choi, Kevin T. Crowley, Bradley J. Dober, Cody J. Duell, Shannon M. Duff, Patricio Gallardo, Gene C. Hilton, Shuay-Pwu Patty Ho, Johannes Hubmayr, Michael J. Link, Michael D. Niemack, Rita F. Sonka, Suzanne T. Staggs, Eve M. Vavagiakis, Edward J. Wollack, Zhilei Xu

The Simons Observatory (SO) will perform ground-based observations of the cosmic microwave background (CMB) with several small and large aperture telescopes, each outfitted with thousands to tens of thousands of superconducting aluminum manganese (AlMn) transition-edge sensor bolometers (TESs).

Instrumentation and Methods for Astrophysics

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