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20152026
most citedThe Simons Observatory: Science goals and forecasts

1.5k citations · 6.2k across the 92 of their papers we have counts for

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Showing 2021Show all

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astro-ph.CO2021

The Simons Observatory: a new open-source power spectrum pipeline applied to the Planck legacy data

Zack Li, Thibaut Louis, Erminia Calabrese +12

We present a reproduction of the Planck 2018 angular power spectra at , and associated covariance matrices, for intensity and polarization maps at 100, 143 and 217 GHz.…

astro-ph.IM2021★ 7 cited

The 90 and 150 GHz universal focal-plane modules for the Simons Observatory

Heather McCarrick, Kam Arnold, Zachary Atkins +21

The Simons Observatory (SO) is a suite of telescopes located in the Atacama Desert in Chile that will make sensitive measurements of the cosmic microwave background. There are a ho…

astro-ph.IM2021★ 21 cited

The Atacama Cosmology Telescope: Measurement and Analysis of 1D Beams for DR4

Marius Lungu, Emilie R. Storer, Matthew Hasselfield +28

We describe the measurement and treatment of the telescope beams for the Atacama Cosmology Telescope's fourth data release, DR4. Observations of Uranus are used to measure the cent…

astro-ph.GA2021★ 30 cited

The Simons Observatory: Galactic Science Goals and Forecasts

Brandon S. Hensley, Susan E. Clark, Valentina Fanfani +31

Observing in six frequency bands from 27 to 280 GHz over a large sky area, the Simons Observatory (SO) is poised to address many questions in Galactic astrophysics in addition to i…

astro-ph.IM2021★ 19 cited

The Atacama Cosmology Telescope: Modeling Bulk Atmospheric Motion

Thomas W. Morris, Ricardo Bustos, Erminia Calabrese +17

Fluctuating atmospheric emission is a dominant source of noise for ground-based millimeter-wave observations of the CMB temperature anisotropy at angular scales $\gtrsim 0.5^{\circ…

astro-ph.IM2021★ 4 cited

The Simons Observatory: Magnetic Shielding Measurements for the Universal Multiplexing Module

Zachary B. Huber, Yaqiong Li, Eve M. Vavagiakis +14

The Simons Observatory (SO) includes four telescopes that will measure the temperature and polarization of the cosmic microwave background using over 60,000 highly sensitive transi…

astro-ph.IM2021★ 6 cited

Simons Observatory Focal-Plane Module: In-lab Testing and Characterization Program

Yuhan Wang, Kaiwen Zheng, Zachary Atkins +20

The Simons Observatory (SO) is a ground-based cosmic microwave background instrument to be sited in the Atacama Desert in Chile. SO will deploy 60,000 transition-edge sensor bolome…

astro-ph.CO2021★ 134 cited

The Atacama Cosmology Telescope: Constraints on Pre-Recombination Early Dark Energy

J. Colin Hill, Erminia Calabrese, Simone Aiola +40

The early dark energy (EDE) scenario aims to increase the value of the Hubble constant () inferred from cosmic microwave background (CMB) data over that found in CDM, via t…

astro-ph.CO2021★ 101 cited

CCAT-prime Collaboration: Science Goals and Forecasts with Prime-Cam on the Fred Young Submillimeter Telescope

Prime collaboration, M. Aravena, J. E. Austermann +84

We present a detailed overview of the science goals and predictions for the Prime-Cam direct detection camera/spectrometer being constructed by the CCAT-prime collaboration for ded…

astro-ph.GA2021★ 17 cited

Atacama Cosmology Telescope measurements of a large sample of candidates from the Massive and Distant Clusters of WISE Survey: Sunyaev-Zeldovich effect confirmation of MaDCoWS candidates using ACT

John Orlowski-Scherer, Luca Di Mascolo, Tanay Bhandarkar +35

Galaxy clusters are an important tool for cosmology, and their detection and characterization are key goals for current and future surveys. Using data from the Wide-field Infrared…

astro-ph.IM2021★ 50 cited

The Simons Observatory microwave SQUID multiplexing detector module design

Heather McCarrick, Erin Healy, Zeeshan Ahmed +56

Advances in cosmic microwave background (CMB) science depend on increasing the number of sensitive detectors observing the sky. New instruments deploy large arrays of superconducti…

astro-ph.CO2021★ 13 cited

Constraining CMB temperature evolution with Sunyaev-Zel'dovich galaxy clusters from the Atacama Cosmology Telescope

Yunyang Li, Adam D. Hincks, Stefania Amodeo +30

The Sunyaev-Zel'dovich (SZ) effect introduces a specific distortion of the blackbody spectrum of the cosmic microwave background (CMB) radiation when it scatters off hot gas in clu…

astro-ph.EP2021★ 22 cited

The Atacama Cosmology Telescope: A search for Planet 9

Sigurd Naess, Simone Aiola, Nick Battaglia +37

We use Atacama Cosmology Telescope (ACT) observations at 98 GHz (2015--2019), 150 GHz (2013--2019) and 229 GHz (2017--2019) to perform a blind shift-and-stack search for Planet 9.…

astro-ph.GA2021★ 33 cited

The Atacama Cosmology Telescope: Microwave Intensity and Polarization Maps of the Galactic Center

Yilun Guan, Susan E. Clark, Brandon S. Hensley +30

We present arcminute-resolution intensity and polarization maps of the Galactic center made with the Atacama Cosmology Telescope (ACT). The maps cover a 32 deg field at 98, 150…

astro-ph.IM2021★ 13 cited

The Simons Observatory: the Large Aperture Telescope (LAT)

Zhilei Xu, Shunsuke Adachi, Peter Ade +57

The Simons Observatory (SO) is a Cosmic Microwave Background (CMB) experiment to observe the microwave sky in six frequency bands from 30GHz to 290GHz. The Observatory -- at …

astro-ph.CO2021★ 29 cited

The Atacama Cosmology Telescope: Summary of DR4 and DR5 Data Products and Data Access

Maya Mallaby-Kay, Zachary Atkins, Simone Aiola +57

Two recent large data releases for the Atacama Cosmology Telescope (ACT), called DR4 and DR5, are available for public access. These data include temperature and polarization maps…

astro-ph.IM2021★ 48 cited

The Simons Observatory Large Aperture Telescope Receiver

Ningfeng Zhu, Tanay Bhandarkar, Gabriele Coppi +68

The Simons Observatory (SO) Large Aperture Telescope Receiver (LATR) will be coupled to the Large Aperture Telescope located at an elevation of 5,200 m on Cerro Toco in Chile. The…

astro-ph.IM2021★ 5 cited

The Integration and Testing Program for the Simons Observatory Large Aperture Telescope Optics Tubes

Kathleen Harrington, Carlos Sierra, Grace Chesmore +18

The Simons Observatory (SO) will be a cosmic microwave background (CMB) survey experiment with three small-aperture telescopes and one large-aperture telescope, which will observe…

astro-ph.IM2021★ 4 cited

CCAT-prime: Designs and status of the first light 280 GHz MKID array and Mod-Cam receiver

Cody J. Duell, Eve M. Vavagiakis, Jason Austermann +23

The CCAT-prime project's first light array will be deployed in Mod-Cam, a single-module testbed and first light cryostat, on the Fred Young Submillimeter Telescope (FYST) in Chile'…

astro-ph.IM2021★ 6 cited

In situ Performance of the Low Frequency Arrayfor Advanced ACTPol

Yaqiong Li, Jason E. Austermann, James A. Beall +24

The Advanced Atacama Cosmology Telescope Polarimeter (AdvACT) \cite{thornton} is an upgrade for the Atacama Cosmology Telescope using Transition Edge Sensor (TES) detector arrays t…

astro-ph.CO2021★ 59 cited

The Atacama Cosmology Telescope: Detection of the Pairwise Kinematic Sunyaev-Zel'dovich Effect with SDSS DR15 Galaxies

Victoria Calafut, Patricio A. Gallardo, Eve M. Vavagiakis +49

We present a 5.4 detection of the pairwise kinematic Sunyaev-Zel'dovich (kSZ) effect using Atacama Cosmology Telescope (ACT) and CMB observations in combination wi…

astro-ph.CO2021★ 33 cited

The Atacama Cosmology Telescope: Probing the Baryon Content of SDSS DR15 Galaxies with the Thermal and Kinematic Sunyaev-Zel'dovich Effects

Eve M. Vavagiakis, Patricio A. Gallardo, Victoria Calafut +49

We present high signal-to-noise measurements (up to 12) of the average thermal Sunyaev Zel'dovich (tSZ) effect from optically selected galaxy groups and clusters and estimate th…