activity
20102023
most citedThe Simons Observatory: Science goals and forecasts

1.5k citations · 6.1k across the 90 of their papers we have counts for

collaborators
Showing 2018Show all

15 papers · 1 filter

astro-ph.IM2018★ 20 cited

Measurements of tropospheric ice clouds with a ground-based CMB polarization experiment, POLARBEAR

Satoru Takakura, Mario A. O. Aguilar-Faúndez, Yoshiki Akiba +45

The polarization of the atmosphere has been a long-standing concern for ground-based experiments targeting cosmic microwave background (CMB) polarization. Ice crystals in upper tro…

astro-ph.IM2018★ 18 cited

Studies of Systematic Uncertainties for Simons Observatory: Detector Array Effects

Kevin T. Crowley, Sara M. Simon, Max Silva-Feaver +36

In this proceeding, we present studies of instrumental systematic effects for the Simons Obsevatory (SO) that are associated with the detector system and its interaction with the f…

astro-ph.IM2018★ 47 cited

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★ 8 cited

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★ 15 cited

Design and characterization of the SPT-3G receiver

J. A. Sobrin, P. A. R. Ade, Z. Ahmed +68

The SPT-3G receiver was commissioned in early 2017 on the 10-meter South Pole Telescope (SPT) to map anisotropies in the cosmic microwave background (CMB). New optics, detector, an…

astro-ph.IM2018★ 10 cited

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★ 8 cited

Studies of Systematic Uncertainties for Simons Observatory: Optical Effects and Sensitivity Considerations

Patricio A. Gallardo, Jon Gudmundsson, Brian J. Koopman +32

The Simons Observatory (SO) is a new experiment that aims to measure the cosmic microwave background (CMB) in temperature and polarization. SO will measure the polarized sky over a…

astro-ph.IM2018★ 72 cited

The Simons Observatory: Instrument Overview

Nicholas Galitzki, Aamir Ali, Kam S. Arnold +75

The Simons Observatory (SO) will make precise temperature and polarization measurements of the cosmic microwave background (CMB) using a set of telescopes which will cover angular…

astro-ph.CO2018★ 1.5k cited

The Simons Observatory: Science goals and forecasts

The Simons Observatory Collaboration, Peter Ade, James Aguirre +247

The Simons Observatory (SO) is a new cosmic microwave background experiment being built on Cerro Toco in Chile, due to begin observations in the early 2020s. We describe the scient…

astro-ph.IM2018★ 20 cited

BoloCalc: a sensitivity calculator for the design of Simons Observatory

Charles A. Hill, Sarah Marie M. Bruno, Sara M. Simon +34

The Simons Observatory (SO) is an upcoming experiment that will study temperature and polarization fluctuations in the cosmic microwave background (CMB) from the Atacama Desert in…

astro-ph.IM2018★ 15 cited

A large-diameter cryogenic rotation stage for half-wave plate polarization modulation on the POLARBEAR-2 experiment

Charles A. Hill, Akito Kusaka, Paul Barton +15

We describe the design of a cryogenic rotation stage (CRS) for use with the cryogenic half-wave plate (CHWP) polarization modulator on the POLARBEAR-2b and POLARBEAR-2c (PB2b/c) co…

astro-ph.IM2018★ 18 cited

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…

astro-ph.IM2018

Developments of highly-multiplexed, multi-chroic pixels for Balloon-Borne Platforms

François Aubin, Shaul Hanany, Bradley R. Johnson +4

We present our work to develop and characterize low thermal conductance bolometers that are part of sinuous antenna multi-chroic pixels (SAMP). We use longer, thinner and meandered…

astro-ph.IM2018★ 7 cited

Commercialization of micro-fabrication of antenna-coupled Transition Edge Sensor bolometer detectors for studies of the Cosmic Microwave Background

Aritoki Suzuki, Chris Bebek, Maurice Garcia-Sciveres +6

We report on the development of commercially fabricated multi-chroic antenna coupled Transition Edge Sensor (TES) bolometer arrays for Cosmic Microwave Background (CMB) polarimetry…

astro-ph.IM2018★ 11 cited

Hierarchical sinuous-antenna phased array for millimeter wavelengths

Ari Cukierman, Adrian T. Lee, Christopher Raum +2

We present the design, fabrication and measured performance of a hierarchical sinuous-antenna phased array coupled to superconducting transition-edge-sensor (TES) bolometers for mi…