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Record W4402659177 · doi:10.3847/1538-4357/adb622

Superclustering with the Atacama Cosmology Telescope and Dark Energy Survey. II. Anisotropic Large-scale Coherence in Hot Gas, Galaxies, and Dark Matter

2025· article· en· W4402659177 on OpenAlexafffund
Martine Lokken, Alexander van Engelen, M. Aguena, S. Allam, Dhayaa Anbajagane, D. Bacon, Eric J. Baxter, J. Blazek, S. Bocquet, J. R. Bond, D. Brooks, Erminia Calabrese, A. Carnero Rosell, J. Carretero, M. Costanzi, L. N. da Costa, William R. Coulton, S. Desai, Peter Doel, C. Doux, Adriaan J. Duivenvoorden, Jo Dunkley, Zhiqi Huang, S. Everett, I. Ferrero, J. Frieman, J. García-Bellido, M. Gatti, E. Gaztañaga, G. Giannini, Vera Gluscevic, D. Gruen, R. A. Gruendl, Yilun Guan, G. Gutiérrez, S. R. Hinton, Renée Hložek, D.L Hollowood, K. Honscheid, D. J. James, K. Kuehn, O. Lahav, S Lee, Mathew S. Madhavacheril, Gabriela A. Marques, J. L. Marshall, J. Mena-Fernández, F. Menanteau, R. Miquel, J. Myles, Michael D. Niemack, S. B. Pandey, M. E. S. Pereira, A. Pieres, A. A. Plazas, A. Porredon, M. Rodríguez-Monroy, A. Roodman, S. Samuroff, E. Sánchez, D. Sanchez Cid, B. Santiago, M. Schubnell, I. Sevilla-Noarbe, Cristobál Sifón, Suzanne T. Staggs, E. Suchyta, M. E. C. Swanson, G. Tarlé, C-H. To, N. Weaverdyck, P. Wiseman, Edward J. Wollack

Bibliographic record

VenueThe Astrophysical Journal · 2025
Typearticle
Languageen
FieldPhysics and Astronomy
TopicGalaxies: Formation, Evolution, Phenomena
Canadian institutionsCanadian Institute for Theoretical AstrophysicsUniversity of Toronto
FundersSLAC National Accelerator LaboratoryIntegrated Electronics Engineering Center, Binghamton UniversityEuropean Regional Development FundScience and Technology Facilities CouncilNatural Sciences and Engineering Research Council of CanadaOffice of ScienceUniversity of Illinois at Urbana-ChampaignNational Institute of Standards and TechnologyInstitut de Física d'Altes EnergiesFundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de JaneiroAgencia Nacional de Investigación y DesarrolloGeneralitat de CatalunyaUniversity of SussexUniversity of TorontoNational Aeronautics and Space AdministrationUniversity College LondonFlatiron HealthNational Energy Research Scientific Computing CenterHigh Energy PhysicsDeutsche ForschungsgemeinschaftArgonne National LaboratoryCentres de Recerca de CatalunyaConselho Nacional de Desenvolvimento Científico e TecnológicoGovernment of OntarioUniversity of PortsmouthCanadian Institute for Advanced ResearchOhio State UniversityMinistério da Ciência, Tecnologia e InovaçãoLawrence Berkeley National LaboratoryFinanciadora de Estudos e ProjetosUniversity of PennsylvaniaMinisterio de Ciencia e InnovaciónEuropean CommissionU.S. Department of EnergyPrinceton UniversityFermilabNational Science FoundationSimons FoundationCompute CanadaUniversity of Chicago
KeywordsPhysicsAstrophysicsDark matterCosmologyDark energyCosmic microwave backgroundSouth Pole TelescopeWeak gravitational lensingGalaxyGalaxy clusterRedshiftHaloBaryonAnisotropy

Abstract

fetched live from OpenAlex

Abstract Statistics that capture the directional dependence of the baryon distribution in the cosmic web enable unique tests of cosmology and astrophysical feedback. We use constrained oriented stacking of thermal Sunyaev–Zel’dovich (tSZ) maps to measure the anisotropic distribution of hot gas 2.5–40 Mpc away from galaxy clusters embedded in massive filaments and superclusters. The cluster selection and orientation (at a scale of ∼15 Mpc) use Dark Energy Survey (DES) Year 3 data, while expanded tSZ maps from the Atacama Cosmology Telescope Data Release 6 enable a ∼3× more significant measurement of the extended gas compared to the technique’s proof-of-concept. Decomposing stacks into cosine multipoles of order m, we detect a dipole (m = 1) and quadrupole (m = 2) at 8σ–10σ, as well as evidence for m = 4 signal at up to 6σ, indicating sensitivity to late-time non-Gaussianity. We compare to Cardinal simulations with spherical gas models pasted onto dark matter halos. The fiducial tSZ data can discriminate between two models that deplete pressure differently in low-mass halos (mimicking astrophysical feedback), preferring higher average pressure in extended structures. However, uncertainty in the amount of cosmic infrared background contamination reduces the constraining power. Additionally, we apply the technique to DES galaxy density and weak lensing to study for the first time their oriented relationships with tSZ. In the tSZ-to-lensing relation, averaged on 7.5 Mpc (transverse) scales, we observe dependence on redshift but not shape or radial distance. Thus, on large scales, the superclustering of gas pressure, galaxies, and total matter is coherent in shape and extent.

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 score0.014
Threshold uncertainty score0.029

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0010.001
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0010.001
Science and technology studies0.0000.000
Scholarly communication0.0010.000
Open science0.0000.001
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 head0.005
GPT teacher head0.199
Teacher spread0.194 · 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

Citations4
Published2025
Admission routes2
Has abstractyes

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