activity
20152022
most citedObservations of Fast Radio Bursts at Frequencies down to 400 Megahertz

188 citations · 517 across the 6 of their papers we have counts for

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Showing 2018Show all

7 papers · 1 filter

astro-ph.CO2018

Mass Calibration of Optically Selected DES clusters using a Measurement of CMB-Cluster Lensing with SPTpol Data

S. Raghunathan, S. Patil, E. Baxter +129

We use cosmic microwave background (CMB) temperature maps from the 500 deg SPTpol survey to measure the stacked lensing convergence of galaxy clusters from the Dark Energy Su…

astro-ph.IM2018

Year two instrument status of the SPT-3G cosmic microwave background receiver

A. N. Bender, P. A. R. Ade, Z. Ahmed +86

The South Pole Telescope (SPT) is a millimeter-wavelength telescope designed for high-precision measurements of the cosmic microwave background (CMB). The SPT measures both the tem…

astro-ph.IM2018

Characterization and performance of the second-year SPT-3G focal plane

D. Dutcher, P. A. R. Ade, Z. Ahmed +68

The third-generation instrument for the 10-meter South Pole Telescope, SPT-3G, was first installed in January 2017. In addition to completely new cryostats, secondary telescope opt…

astro-ph.IM2018

Broadband anti-reflective coatings for cosmic microwave background experiments

A. Nadolski, A. M. Kofman, J. D. Vieira +71

The desire for higher sensitivity has driven ground-based cosmic microwave background (CMB) experiments to employ ever larger focal planes, which in turn require larger reimaging o…

astro-ph.IM2018

Digital frequency multiplexing with sub-Kelvin SQUIDs

Amy E. Lowitz, Amy N. Bender, Matthew A. Dobbs +1

Digital frequency multiplexing (dfMux) is a readout architecture for transition edge sensor-based detector arrays and is used on telescopes including SPT-3G, POLARBEAR-2, and LiteB…

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…