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Record W3180268056 · doi:10.3847/1538-4357/ac7043

Superclustering with the Atacama Cosmology Telescope and Dark Energy Survey. I. Evidence for Thermal Energy Anisotropy Using Oriented Stacking

2022· article· en· W3180268056 on OpenAlexafffund
Martine Lokken, Renée Hložek, Alexander van Engelen, Mathew S. Madhavacheril, Eric J. Baxter, Joseph DeRose, C. Doux, Shivam Pandey, E. S. Rykoff, George Stein, C. To, T. M. C. Abbott, Susmita Adhikari, M. Aguena, S. Allam, F. Andrade-Oliveira, J. Annis, Nicholas Battaglia, G. M. Bernstein, E. Bertin, J. Richard Bond, D. Brooks, Erminia Calabrese, A. Carnero Rosell, M. Carrasco Kind, J. Carretero, R. Cawthon, A. Choi, M. Costanzi, M. Crocce, L. N. da Costa, M. E. S. Pereira, J. De Vicente, S. Desai, J. P. Dietrich, P. Doel, Jo Dunkley, S. Everett, A. E. Evrard, Simone Ferraro, B. Flaugher, P. Fosalba, J. Frieman, Patricio A. Gallardo, J. García-Bellido, E. Gaztañaga, D. W. Gerdes, T. Giannantonio, D. Gruen, R. A. Gruendl, J. Gschwend, G. Gutiérrez, J. Colin Hill, Matt Hilton, Adam D. Hincks, S. R. Hinton, D. L. Hollowood, K. Honscheid, B. Hoyle, Zhiqi Huang, John P. Hughes, Dragan Huterer, B. Jain, D. J. James, T. Jeltema, K. Kuehn, M. Lima, M. A. G. Maia, J. L. Marshall, J. J. McMahon, P. Melchior, F. Menanteau, R. Miquel, J. J. Mohr, Kavilan Moodley, R. Morgan, F. Nati, Lyman A. Page, R. L. C. Ogando, A. Palmese, F. Paz-Chinchón, A. A. Plazas, A. Pieres, A. K. Romer, Eduardo Rozo, E. Sánchez, V. Scarpine, A. Schillaci, M. Schubnell, S. Serrano, I. Sevilla-Noarbe, E. Sheldon, T. Shin, Cristobál Sifón, M. Smith, M. Soares-Santos, E. Suchyta, M. E. C. Swanson, G. Tarlé, D. Thomas, D. L. Tucker, T N Varga, J. Weller, Risa H. Wechsler, R. D. Wilkinson, Edward J. Wollack, Zhilei Xu

Bibliographic record

VenueThe Astrophysical Journal · 2022
Typearticle
Languageen
FieldPhysics and Astronomy
TopicGalaxies: Formation, Evolution, Phenomena
Canadian institutionsCanadian Institute for Theoretical AstrophysicsPerimeter InstituteUniversity of Toronto
FundersSLAC National Accelerator LaboratoryIntegrated Electronics Engineering Center, Binghamton UniversityEuropean Regional Development FundScience and Technology Facilities CouncilNatural Sciences and Engineering Research Council of CanadaUniversity of Illinois at Urbana-ChampaignEuropean Research CouncilNational Institute of Standards and TechnologyInstitut de Física d'Altes EnergiesConnaught FundFundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de JaneiroCentro de Investigaciones Energéticas, Medioambientales y TecnológicasConselho Nacional de Desenvolvimento Científico e TecnológicoGeneralitat de CatalunyaOffice of ScienceUniversity of EdinburghUniversity of SussexUniversity of NottinghamUniversity of TorontoOhio State UniversityNational Research FoundationComisión Nacional de Investigación Científica y TecnológicaNational Aeronautics and Space AdministrationUniversity College LondonUniversity of CambridgeNational Energy Research Scientific Computing CenterUniversity of PortsmouthUniversity of ChicagoMinistério da Ciência, Tecnologia e InovaçãoLawrence Berkeley National LaboratoryFinanciadora de Estudos e ProjetosUniversity of PennsylvaniaHigh Energy PhysicsDeutsche ForschungsgemeinschaftArgonne National LaboratoryCentres de Recerca de CatalunyaMinisterio de Ciencia e InnovaciónEuropean CommissionU.S. Department of EnergyPrinceton UniversityUniversity of MichiganFermilabNational Science Foundation
KeywordsPhysicsCosmic microwave backgroundGalaxy clusterAstrophysicsDark energyCosmologyGalaxyAstronomySouth Pole TelescopeLarge Synoptic Survey TelescopeTelescopeAnisotropyOptics

Abstract

fetched live from OpenAlex

Abstract The cosmic web contains filamentary structure on a wide range of scales. On the largest scales, superclustering aligns multiple galaxy clusters along intercluster bridges, visible through their thermal Sunyaev–Zel’dovich signal in the cosmic microwave background. We demonstrate a new, flexible method to analyze the hot gas signal from multiscale extended structures. We use a Compton y-map from the Atacama Cosmology Telescope (ACT) stacked on redMaPPer cluster positions from the optical Dark Energy Survey (DES). Cutout images from the y-map are oriented with large-scale structure information from DES galaxy data such that the superclustering signal is aligned before being overlaid. We find evidence of an extended quadrupole moment of the stacked y signal at the 3.5σ level, demonstrating that the large-scale thermal energy surrounding galaxy clusters is anisotropically distributed. We compare our ACT × DES results with the Buzzard simulations, finding broad agreement. Using simulations, we highlight the promise of this novel technique for constraining the evolution of anisotropic, non-Gaussian structure using future combinations of microwave and optical surveys.

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)0.001
metaresearch head score (Gemma)0.001
Version: metacan-v3-hybrid-931329e0061cValidation status: machine_predicted_unvalidated
Candidate categoriesnone
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Observational · Consensus signal: Observational
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.033
Threshold uncertainty score0.065

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0010.001
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.001
Bibliometrics0.0010.001
Science and technology studies0.0000.000
Scholarly communication0.0010.000
Open science0.0010.001
Research integrity0.0000.000
Insufficient payload (model declined to judge)0.0010.000

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 head0.023
GPT teacher head0.245
Teacher spread0.221 · 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 designObservational
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".

Quick stats

Citations17
Published2022
Admission routes2
Has abstractyes

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