activity
20052026
most citedThe Simons Observatory: Science goals and forecasts

1.5k citations · 13.3k across the 244 of their papers we have counts for

collaborators
Showing 2018 · astro-ph.IMShow all

22 papers · 2 filters

astro-ph.IM2018★ 25 cited

On-sky performance of the CLASS Q-band telescope

John W. Appel, Zhilei Xu, Ivan L. Padilla +34

The Cosmology Large Angular Scale Surveyor (CLASS) is mapping the polarization of the Cosmic Microwave Background (CMB) at large angular scales () in search of a…

astro-ph.IM2018★ 22 cited

Feedhorn development and scalability for Simons Observatory and beyond

Sara M. Simon, Joseph E. Golec, Aamir Ali +21

The Simons Observatory (SO) will measure the cosmic microwave background (CMB) in both temperature and polarization over a wide range of angular scales and frequencies from 27-270…

astro-ph.IM2018★ 31 cited

Highly-multiplexed microwave SQUID readout using the SLAC Microresonator Radio Frequency (SMuRF) Electronics for Future CMB and Sub-millimeter Surveys

Shawn W. Henderson, Zeeshan Ahmed, Jason Austermann +29

The next generation of cryogenic CMB and submillimeter cameras under development require densely instrumented sensor arrays to meet their science goals. The readout of large number…

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

Simons Observatory Large Aperture Telescope Receiver Design Overview

Ningfeng Zhu, John L. Orlowski-Scherer, Zhilei Xu +31

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

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.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.IM2018

Optical Design of PICO, a Concept for a Space Mission to Probe Inflation and Cosmic Origins

Karl Young, Marcelo Alvarez, Nicholas Battaglia +28

The Probe of Inflation and Cosmic Origins (PICO) is a probe-class mission concept currently under study by NASA. PICO will probe the physics of the Big Bang and the energy scale of…

astro-ph.IM2018

PICO - the probe of inflation and cosmic origins

Brian Sutin, Marcelo Alvarez, Nicholas Battaglia +31

The Probe of Inflation and Cosmic Origins (PICO) is a NASA-funded study of a Probe-class mission concept. The top-level science objectives are to probe the physics of the Big Bang…

astro-ph.IM2018★ 3 cited

Cold optical design for the Large Aperture Simons Observatory telescope

S. R. Dicker, P. A. Gallardo, J. E Gudmundsson +26

The Simons Observatory will consist of a single large (6 m diameter) telescope and a number of smaller (0.5 m diameter) refracting telescopes designed to measure the polarization o…

astro-ph.IM2018★ 20 cited

The Cosmology Large Angular Scale Surveyor Receiver Design

Jeffrey Iuliano, Joseph Eimer, Lucas Parker +42

The Cosmology Large Angular Scale Surveyor consists of four instruments performing a CMB polarization survey. Currently, the 40 GHz and first 90 GHz instruments are deployed and ob…

astro-ph.IM2018★ 15 cited

Advanced ACTPol TES Device Parameters and Noise Performance in Fielded Arrays

Kevin T. Crowley, Jason E. Austermann, Steve K. Choi +14

The Advanced ACTPol (AdvACT) upgrade to the Atacama Cosmology Telescope (ACT) features arrays of aluminum manganese transition-edge sensors (TESes) optimized for ground-based obser…

astro-ph.IM2018★ 1 cited

BFORE: A CMB Balloon Payload to Measure Reionization, Neutrino Mass, and Cosmic Inflation

Sean Bryan, Peter Ade, J. Richard Bond +21

BFORE is a high-altitude ultra-long-duration balloon mission to map the cosmic microwave background (CMB). During a 28-day mid-latitude flight launched from Wanaka, New Zealand, th…

astro-ph.IM2018★ 17 cited

Design and characterization of the Cosmology Large Angular Scale Surveyor (CLASS) 93 GHz focal plane

Sumit Dahal, Aamir Ali, John W. Appel +44

The Cosmology Large Angular Scale Surveyor (CLASS) aims to detect and characterize the primordial B-mode signal and make a sample-variance-limited measurement of the optical depth…

astro-ph.IM2018★ 1 cited

Variable-delay Polarization Modulators for the CLASS Telescopes

Kathleen Harrington, Joseph Eimer, David T. Chuss +43

The search for inflationary primordial gravitational waves and the measurement of the optical depth to reionization, both through their imprint on the large angular scale correlati…

astro-ph.IM2018★ 17 cited

Low Temperature Detectors for CMB Imaging Arrays

Johannes Hubmayr, Jason E. Austermann, James A. Beall +9

We review advances in low temperature detector (LTD) arrays for Cosmic Microwave Background (CMB) polarization experiments, with a particular emphasis on imaging arrays. We briefly…

astro-ph.IM2018★ 17 cited

Prime-Cam: A first-light instrument for the CCAT-prime telescope

Eve M. Vavagiakis, Zeeshan Ahmed, Aamir Ali +43

CCAT-prime will be a 6-meter aperture telescope operating from sub-mm to mm wavelengths, located at 5600 meters elevation on Cerro Chajnantor in the Atacama Desert in Chile. Its no…

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★ 20 cited

SLAC Microresonator Radio Frequency (SMuRF) Electronics for Read Out of Frequency-Division-Multiplexed Cryogenic Sensors

S. A. Kernasovskiy, S. E. Kuenstner, E. Karpel +20

Large arrays of cryogenic sensors for various imaging applications ranging across x-ray, gamma-ray, Cosmic Microwave Background (CMB), mm/sub-mm, as well as particle detection incr…

astro-ph.IM2018★ 39 cited

Millimeter-Wave Polarimeters Using Kinetic Inductance Detectors for TolTEC and Beyond

J. E. Austermann, J. A. Beall, S. A. Bryan +10

Microwave Kinetic Inductance Detectors (MKIDs) provide a compelling path forward to the large-format polarimeter, imaging, and spectrometer arrays needed for next-generation experi…

astro-ph.IM2018★ 24 cited

The EBEX Balloon Borne Experiment - Detectors and Readout

The EBEX Collaboration, Maximilian Abitbol, Asad M. Aboobaker +37

EBEX was a long-duration balloon-borne experiment to measure the polarization of the cosmic microwave background. The experiment had three frequency bands centered at 150, 250, and…

astro-ph.IM2018★ 137 cited

The LiteBIRD Satellite Mission - Sub-Kelvin Instrument

A. Suzuki, P. A. R. Ade, Y. Akiba +149

Inflation is the leading theory of the first instant of the universe. Inflation, which postulates that the universe underwent a period of rapid expansion an instant after its birth…