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Record W2888259247 · doi:10.1088/1475-7516/2019/02/056

The Simons Observatory: science goals and forecasts

2019· article· en· W2888259247 on OpenAlexafffund
P. A. R. Ade, James Aguirre, Zeeshan Ahmed, Simone Aiola, Aamir Ali, David Alonso, Marcelo A. Alvarez, Kam Arnold, Peter Ashton, Jason E. Austermann, Humna Awan, C. Baccigalupi, Taylor Baildon, Darcy Barron, Richard A. Battye, Eric J. Baxter, A. O. Bazarko, James A. Beall, Rachel Bean, D. Beck, Shawn Beckman, Benjamin Beringue, F. Bianchini, Steven Boada, D. Boettger, J. Richard Bond, Julian Borrill, Sarah Marie Bruno, Sean Bryan, Erminia Calabrese, Victoria Calafut, P. Calisse, Julien Carron, A. Challinor, Grace E. Chesmore, Y. Chinone, Jens Chluba, Hsiao-Mei Sherry Cho, Steve K. Choi, Gabriele Coppi, Nicholas F. Cothard, Kevin Coughlin, Devin Crichton, Kevin D. Crowley, Kevin T. Crowley, A. Cukierman, Rolando Dünner, T. de Haan, Mark J. Devlin, Simon Dicker, Joy Didier, M. Dobbs, Bradley Dober, Cody J. Duell, Shannon M. Duff, Adriaan J. Duivenvoorden, Jo Dunkley, John Dusatko, Josquin Errard, Giulio Fabbian, Stephen M. Feeney, Simone Ferraro, Pedro Fluxá, Katherine Freese, J. Frisch, Andrei V. Frolov, George M. Fuller, Brittany Fuzia, Nicholas Galitzki, Patricio A. Gallardo, José T. Gálvez Ghersi, Jiansong Gao, Eric Gawiser, M. Gerbino, Vera Gluscevic, N. Goeckner-Wald, Joseph E. Golec, Sam Gordon, Megan Gralla, Daniel Green, Arpi Grigorian, J. C. Groh, Chris Groppi, Yilun Guan, Jon E. Gudmundsson, Dongwon Han, Peter Hargrave, M. Hasegawa, Matthew Hasselfield, M. Hattori, Victor Haynes, M. Hazumi, Yizhou He, Erin Healy, Shawn Henderson, Carlos Hervías-Caimapo, Charles A. Hill, J. Colin Hill, G. C. Hilton, Matt Hilton, Adam D. Hincks, G. Hinshaw, Renée Hložek, Shirley Ho, Shuay-Pwu Patty Ho, L. Howe, Zhiqi Huang, Johannes Hubmayr, K. M. Huffenberger, John P. Hughes, Anna Ijjas, Margaret Ikape, K. D. Irwin, A. H. Jaffe, Bhuvnesh Jain, O. Jeong, Daisuke Kaneko, E. Karpel, N. Katayama, Brian Keating, Sarah S. Kernasovskiy, Reijo Keskitalo, Theodore Kisner, Kenta Kiuchi, Jeff Klein, Kenda Knowles, Brian J. Koopman, Arthur Kosowsky, N. Krachmalnicoff, Stephen E. Kuenstner, Chao‐Lin Kuo, A. Kusaka, Jacob Lashner, Adrian V. Lee, Eunseong Lee, D. Leon, Jason S.-Y. Leung, Antony Lewis, Yaqiong Li, Zack Li, M. Limon, Eric V. Linder, C. H. López-Caraballo, Thibaut Louis, Lindsay Lowry, Mathew S. Madhavacheril, D. S. Y. Mak, Felipe Maldonado, Hamdi Mani, Ben Mates, Frederick Matsuda, L. Maurin, P. Mauskopf, Andrew May, Chris McKenney, J. J. McMahon, P. Daniel Meerburg, Joel Meyers, Amber Miller, Mark Mirmelstein, Kavilan Moodley, Moritz Münchmeyer, Charles Munson, Sigurd Næss, F. Nati, M. Navaroli, Laura Newburgh, Hồ Nam Nguyễn, Michael D. Niemack, H. Nishino, John Orlowski-Scherer, Lyman A. Page, Bruce Partridge, J. Peloton, F. Perrotta, Lucio Piccirillo, G. Pisano, D. Poletti, Roberto Puddu, Giuseppe Puglisi, Chris Raum, C. L. Reichardt, M. Remazeilles, Yoel Rephaeli, Dominik A. Riechers, Felipe Rojas, Anirban Roy, Sharon Sadeh, Y. Sakurai, Maria Salatino, Mayuri Sathyanarayana Rao, Emmanuel Schaan, Marcel Schmittfull, Neelima Sehgal, Joseph Seibert, Uroš Seljak, Blake D. Sherwin, Meir Shimon, Carlos Sierra, Jonathan Sievers, S. P. Sikhosana, Maximiliano Silva-Feaver, Sara M. Simon, Adrian K. Sinclair, P. Siritanasak, Kendrick M. Smith, Stephen R. Smith, David N. Spergel, Suzanne T. Staggs, George Stein, Jason Stevens, R. Stompor, Aritoki Suzuki, O. Tajima, S. Takakura, Grant Teply, Daniel B. Thomas, B. Thorne, Robert Thornton, Hy Trac, Calvin Tsai, C. Tucker, Joel N. Ullom, Sunny Vagnozzi, Alexander van Engelen, Jeff Van Lanen, Daniel D. Van Winkle, Eve M. Vavagiakis, C. Vergès, Michael Vissers, Kasey Wagoner, Samantha Walker, Jon Ward, Benjamin Westbrook, N. Whitehorn, Jason A. Williams, Joel Williams, Edward J. Wollack, Zhilei Xu, Byeonghee Yu, Cyndia Yu, Fernando Zago, Hezi Zhang, Ningfeng Zhu

Bibliographic record

VenueJournal of Cosmology and Astroparticle Physics · 2019
Typearticle
Languageen
FieldPhysics and Astronomy
TopicAstrophysics and Cosmic Phenomena
Canadian institutionsPerimeter InstituteSimon Fraser UniversityUniversity of British ColumbiaMcGill UniversityCanadian Institute for Theoretical AstrophysicsUniversity of Toronto
FundersComisión Nacional de Investigación Científica y TecnológicaNuclear PhysicsNatural Sciences and Engineering Research Council of CanadaStockholms UniversitetIsaac Newton TrustScience and Technology Facilities CouncilUniversity of TorontoH2020 Research InfrastructuresAgence Nationale de la RechercheNederlandse Organisatie voor Wetenschappelijk OnderzoekMinistry of Education, Culture, Sports, Science and TechnologyCentre National d’Etudes SpatialesEconomic and Social Research CouncilEuropean CommissionVetenskapsrådetNational Science FoundationJapan Society for the Promotion of ScienceHorizon 2020 Framework ProgrammeUniversity of CambridgeUniversity of MichiganNational Aeronautics and Space Administration
KeywordsPhysicsCosmic microwave backgroundPlanckAstrophysicsObservatorySkyCosmologyReionizationSouth Pole TelescopeTelescopeAstronomyGalaxyAngular resolution (graph drawing)NeutrinoCosmic background radiationBolometerPolarization (electrochemistry)AnisotropyGalaxy clusterRedshiftDetectorOptics

Abstract

fetched live from OpenAlex

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 scientific goals of the experiment, motivate the design, and forecast its performance. SO will measure the temperature and polarization anisotropy of the cosmic microwave background in six frequency bands centered at: 27, 39, 93, 145, 225 and 280 GHz. The initial configuration of SO will have three small-aperture 0.5-m telescopes and one large-aperture 6-m telescope, with a total of 60,000 cryogenic bolometers. Our key science goals are to characterize the primordial perturbations, measure the number of relativistic species and the mass of neutrinos, test for deviations from a cosmological constant, improve our understanding of galaxy evolution, and constrain the duration of reionization. The small aperture telescopes will target the largest angular scales observable from Chile, mapping ≈ 10% of the sky to a white noise level of 2 μK-arcmin in combined 93 and 145 GHz bands, to measure the primordial tensor-to-scalar ratio,r, at a target level of σ(r)=0.003. The large aperture telescope will map ≈ 40% of the sky at arcminute angular resolution to an expected white noise level of 6 μK-arcmin in combined 93 and 145 GHz bands, overlapping with the majority of the Large Synoptic Survey Telescope sky region and partially with the Dark Energy Spectroscopic Instrument. With up to an order of magnitude lower polarization noise than maps from thePlancksatellite, the high-resolution sky maps will constrain cosmological parameters derived from the damping tail, gravitational lensing of the microwave background, the primordial bispectrum, and the thermal and kinematic Sunyaev-Zel'dovich effects, and will aid in delensing the large-angle polarization signal to measure the tensor-to-scalar ratio. The survey will also provide a legacy catalog of 16,000 galaxy clusters and more than 20,000 extragalactic sources.

Fetched live from OpenAlex and de-inverted. Abstracts are not stored in this database: the inverted indexes are 8.6 GB of the frame’s 9.3 GB of text, and the host has 13 GB free.

How this classification was reachedexpand

Full frame machine prediction

Teacher imitation

Not calibrated prevalence, not ground truth. Human validation pending. The Gemma side is a direct model label for every work in the frame, read from the title-only record. The Codex side is a classifier learned from the 10,348 direct Codex labels and calibrated to design-weighted sample rates; fields without enough sample support carry no Codex call. Candidate is the union of the two sides; consensus is their intersection. These outputs are machine_predicted_unvalidated and are not human labels.

metaresearch head score (Codex)0.004
metaresearch head score (Gemma)0.006
Version: metacan-v3-hybrid-931329e0061cValidation status: machine_predicted_unvalidated
Candidate categoriesnone
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Theoretical or conceptual · Consensus signal: none
GenreCandidate signal: Empirical · Consensus signal: none
Teacher disagreement score0.099
Threshold uncertainty score0.197

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0040.006
Meta-epidemiology (narrow)0.0020.001
Meta-epidemiology (broad)0.0010.001
Bibliometrics0.0030.003
Science and technology studies0.0010.001
Scholarly communication0.0050.005
Open science0.0020.002
Research integrity0.0030.004
Insufficient payload (model declined to judge)0.0090.006

Machine scores (provisional)

The two teacher heads of the student model, read on this work. A score orders the frame for review; it never asserts a category, and the validation status ships verbatim with every row.

Baseline scores from an immature model (maturity gate not passed, 7 training rounds). Scores rank; they never assert a category.

Opus teacher head0.009
GPT teacher head0.231
Teacher spread0.222 · how far apart the two teachers sit on this one work
Validation statusscore_only:v0-immature-baseline · verbatim from the scoring run: score_only means the number may rank works, and no category label ships from it

Classification

machine, unvalidated

Machine predicted; a candidate call from one source (direct Gemma or distilled Codex), not a consensus.

The models applied no category: nothing in the taxonomy fit this work.
Study designTheoretical or conceptual
Domainnot available
GenreEmpirical

How this classification was reached, model by model and score by score, is at the end of the page under "How this classification was reached".

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Citations1,549
Published2019
Admission routes2
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