activity
20182026
most citedThe Simons Observatory: Science goals and forecasts

1.5k citations · 1.8k across the 18 of their papers we have counts for

collaborators

18 papers

astro-ph.HE2026★ 1 cited

Plasma Dynamics of Radiative Cooling Accretion Flow in AM Herculis with XRISM

Yukikatsu Terada, Kaya Mori, Takayuki Hayashi +14

We present XRISM/Resolve high-resolution X-ray spectroscopy of the prototypical magnetic cataclysmic variable AM Herculis. All satellite lines of highly ionized Fe are fully resolv…

astro-ph.IM2024

CCAT: Prime-Cam Optics Overview and Status Update

Zachary B. Huber, Lawrence T. Lin, Eve M. Vavagiakis +17

Prime-Cam is a first-generation science instrument for the CCAT Observatory's six-meter aperture Fred Young Submillimeter Telescope (FYST). FYST's crossed-Dragone design provides h…

astro-ph.IM2024

CCAT: Detector Noise Limited Performance of the RFSoC-based Readout Electronics for mm/sub-mm/far-IR KIDs

Adrian K. Sinclair, James Burgoyne, Anthony I. Huber +16

The Fred Young Submillimeter Telescope (FYST), on Cerro Chajnantor in the Atacama desert of Chile, will conduct wide-field and small deep-field surveys of the sky with more than 10…

astro-ph.IM2024★ 2 cited

CCAT: Comparisons of 280 GHz TiN and Al Kinetic Inductance Detector Arrays

Cody J. Duell, Jason Austermann, James Beall +27

The CCAT Collaboration's six-meter Fred Young Submillimeter Telescope is scheduled to begin observing in the Chilean Atacama in 2025, targeting a variety of science goals throughou…

astro-ph.IM2024

CCAT: FYST Prime-Cam Readout Software: A framework for massively scalable KID arrays

James R. Burgoyne, Adrian K. Sinclair, Scott C. Chapman +12

We outline the development of the readout software for the Prime-Cam and Mod-Cam instruments on the CCAT Fred Young Submillimeter Telescope (FYST), primecam_readout. The instrument…

astro-ph.IM2022★ 2 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,…