activity
20162021
most citedThe Simons Observatory: Science goals and forecasts

1.5k citations · 1.8k across the 14 of their papers we have counts for

collaborators

14 papers

astro-ph.IM2021★ 5 cited

Characterization, deployment, and in-flight performance of the BLAST-TNG cryogenic receiver

Ian Lowe, Peter A. R. Ade, Peter C. Ashton +30

The Next Generation Balloon-borne Large Aperture Submillimeter Telescope (BLAST-TNG) is a submillimeter polarimeter designed to map interstellar dust and galactic foregrounds at 25…

astro-ph.IM2021★ 4 cited

In-flight performance of the BLAST-TNG telescope platform

Gabriele Coppi, Peter A. R. Ade, Peter C. Ashton +30

The Next Generation Balloon-Borne Large Aperture Submillimeter Telescope (BLAST-TNG) was a unique instrument for characterizing the polarized submillimeter sky at high-angular reso…

astro-ph.IM2020★ 30 cited

Full-Array Noise Performance of Deployment-Grade SuperSpec mm-wave On-Chip Spectrometers

K. S. Karkare, P. S. Barry, C. M. Bradford +15

SuperSpec is an on-chip filter-bank spectrometer designed for wideband moderate-resolution spectroscopy at millimeter wavelengths, employing TiN kinetic inductance detectors. Super…

astro-ph.IM2020★ 18 cited

In-flight performance of the LEKIDs of the OLIMPO experiment

A. Paiella, P. A. R. Ade, E. S. Battistelli +22

We describe the in-flight performance of the horn-coupled Lumped Element Kinetic Inductance Detector arrays of the balloon-borne OLIMPO experiment. These arrays have been designed…

astro-ph.IM2019★ 79 cited

The Simons Observatory: Astro2020 Decadal Project Whitepaper

The Simons Observatory Collaboration, Maximilian H. Abitbol, Shunsuke Adachi +280

The Simons Observatory (SO) is a ground-based cosmic microwave background (CMB) experiment sited on Cerro Toco in the Atacama Desert in Chile that promises to provide breakthrough…

astro-ph.IM2019★ 12 cited

Kinetic Inductance Detectors and readout electronics for the OLIMPO experiment

A. Paiella, E. S. Battistelli, M. G. Castellano +13

Kinetic Inductance Detectors (KIDs) are superconductive lowtemperature detectors useful for astrophysics and particle physics. We have developed arrays of lumped elements KIDs (…

astro-ph.IM2019★ 31 cited

Kinetic Inductance Detectors for the OLIMPO experiment: in--flight operation and performance

S. Masi, P. de Bernardis, A. Paiella +22

We report on the performance of lumped--elements Kinetic Inductance Detector (KID) arrays for mm and sub--mm wavelengths, operated at 0.3K during the stratospheric flight of the OL…

astro-ph.IM2018★ 28 cited

Kinetic Inductance Detectors for the OLIMPO experiment: design and pre-flight characterization

A. Paiella, A. Coppolecchia, L. Lamagna +15

We designed, fabricated, and characterized four arrays of horn--coupled, lumped element kinetic inductance detectors (LEKIDs), optimized to work in the spectral bands of the balloo…

astro-ph.IM2018★ 10 cited

Design and Characterization of a Balloon-Borne Diffraction-Limited Submillimeter Telescope Platform for BLAST-TNG

Nathan P. Lourie, Francisco E. Angile, Peter C. Ashton +16

The Next Generation Balloon-borne Large Aperture Submillimeter Telescope (BLAST-TNG) is a submillimeter mapping experiment planned for a 28 day long-duration balloon (LDB) flight f…

astro-ph.IM2018★ 12 cited

Preflight Characterization of the BLAST-TNG Receiver and Detector Arrays

Nathan P. Lourie, Peter A. R. Ade, Francisco E. Angile +26

The Next Generation Balloon-borne Large Aperture Submillimeter Telescope (BLAST-TNG) is a submillimeter mapping experiment planned for a 28 day long-duration balloon (LDB) flight f…

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.IM2017★ 5 cited

A Superconducting Phase Shifter and Traveling Wave Kinetic Inductance Parametric Amplifier for W-Band Astronomy

George Che, Samuel Gordon, Peter Day +7

The W-Band () sky contains a plethora of information about star formation, galaxy evolution and the cosmic microwave background. We have designed and fabrica…

astro-ph.IM2016★ 46 cited

An Open Source, FPGA-based LeKID readout for BLAST-TNG: Pre-flight Results

Samuel Gordon, Bradley Dober, Adrian Sinclair +17

We present a highly frequency multiplexed readout for large-format superconducting detector arrays intended for use in the next generation of balloon-borne and space-based sub-mill…

astro-ph.IM2016★ 18 cited

Instrumental performance and results from testing of the BLAST-TNG receiver, submillimeter optics, and MKID arrays

Nicholas Galitzki, Peter Ade, Francesco E. Angile +39

Polarized thermal emission from interstellar dust grains can be used to map magnetic fields in star forming molecular clouds and the diffuse interstellar medium (ISM). The Balloon-…