most citedSimons Observatory: Characterization of the Large Aperture Telescope Receiver

1 citations · 1 across the 4 of their papers we have counts for

collaborators

9 papers

astro-ph.CO2026

SPT-3G+: A Cosmic Microwave Background Experiment for the South Pole Telescope

T. Natoli, Z. Ahmed, H. Athreya +72

SPT-3G+ is the next survey receiver planned to be installed in early 2029 on the 10-meter South Pole Telescope (SPT). This new receiver will feature 6,020 polarization-sensitive di…

astro-ph.IM2026

The SPT-3G+ receiver design

H. Athreya, Z. Ahmed, J. E. Austermann +71

We present the thermo-mechanical design of the cryostat and camera optics for SPT-3G+, a new receiver being developed for the South Pole Telescope (SPT). The receiver consists of 1…

astro-ph.IM2026

Laser-micromachined silicon-platelet feedhorns for large-scale submillimeter and millimeter-wave focal planes

Jason E. Austermann, James Beall, Andrew Forsman +10

We present the fabrication and characterization of the first silicon-platelet feedhorn arrays produced using laser micromachining. First, we present a demonstration of the technolo…

astro-ph.IM2026

CCAT: Characterization of the first science-grade MKID array for the Prime-Cam 850 GHz module

Anthony I. Huber, Jordan Wheeler, James Burgoyne +16

The Fred Young Submillimeter Telescope (FYST) is a 6-meter crossed-Dragone telescope developed by the CCAT collaboration. Sited at 5600 m on Cerro Chajnantor in the Atacama Plateau…

astro-ph.IM2026

Detectors for CLASS-W2: The second 90 GHz telescope of the Cosmology Large Angular Scale Surveyor

John W. Appel, Kyuyoung Bae, Charles L. Bennett +26

The Cosmology Large Angular Scale Surveyor (CLASS) is measuring the Cosmic Microwave Background (CMB) polarization anisotropy on the largest angular scales (>1 degree) to probe the…

astro-ph.IM2026

CCAT: Silicon-Platelet Feedhorns for Submillimeter Wavelengths

Jason Austermann, James Beall, James R. Burgoyne +12

Silicon-platelet feedhorn arrays are an established technology at millimeter wavelengths that, for some applications, can provide significant advantages over traditional direct-mac…

astro-ph.IM2025

Spectral Characterization of a 90 GHz CLASS Pixel

Gregory Jaehnig, John Appel, Sarah Marie Bruno +10

The Cosmology Large Angular Scale Surveyor (CLASS) is an experiment designed to measure the polarization of the cosmic microwave background on large angular scales to probe cosmic…

astro-ph.IM2025

Development of Silicon Micromachined Waveguide Filter-Banks for On-Chip Spectrometers

Matthew A. Koc, Jason Austermann, James Beall +4

Development of high-speed, spatial-mapping spectrometers in the millimeter and far-infrared frequencies would enable entirely new research avenues in astronomy and cosmology. An "o…

astro-ph.IM2025★ 1 cited

Simons Observatory: Characterization of the Large Aperture Telescope Receiver

Tanay Bhandarkar, Saianeesh K. Haridas, Jeff Iuliano +41

The Simons Observatory (SO) is a ground-based cosmic microwave background (CMB) survey experiment that currently consists of three 0.42m small-aperture telescopes (SATs) and one 6m…