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20182026
most citedDesign and Bolometer Characterization of the SPT-3G First-year Focal Plane

8 citations · 15 across the 2 of their papers we have counts for

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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.IM2024★ 7 cited

Measurement and Modeling of Polarized Atmosphere at the South Pole with SPT-3G

A. Coerver, J. A. Zebrowski, S. Takakura +102

We present the detection and characterization of fluctuations in linearly polarized emission from the atmosphere above the South Pole. These measurements make use of data from the…

astro-ph.IM2019

Performance of Al-Mn Transition-Edge Sensor Bolometers in SPT-3G

A. J. Anderson, P. A. R. Ade, Z. Ahmed +86

SPT-3G is a polarization-sensitive receiver, installed on the South Pole Telescope, that measures the anisotropy of the cosmic microwave background (CMB) from degree to arcminute s…

astro-ph.IM2019

On-sky performance of the SPT-3G frequency-domain multiplexed readout

A. N. Bender, A. J. Anderson, J. S. Avva +86

Frequency-domain multiplexing (fMux) is an established technique for the readout of large arrays of transition edge sensor (TES) bolometers. Each TES in a multiplexing module has a…

astro-ph.IM2019★ 8 cited

Design and Bolometer Characterization of the SPT-3G First-year Focal Plane

W. Everett, P. A. R. Ade, Z. Ahmed +73

During the austral summer of 2016-17, the third-generation camera, SPT-3G, was installed on the South Pole Telescope, increasing the detector count in the focal plane by an order o…

astro-ph.IM2018

Optical Characterization of the SPT-3G Focal Plane

Zhaodi Pan, Peter Ade, Zeeshan Ahmed +73

The third-generation South Pole Telescope camera is designed to measure the cosmic microwave background across three frequency bands (95, 150 and 220 GHz) with ~16,000 transition-e…