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Record W3163615747 · doi:10.1093/mnras/stab2505

The mass and galaxy distribution around SZ-selected clusters

2021· preprint· en· W3163615747 on OpenAlexafffund
T. Shin, Bhuvnesh Jain, Susmita Adhikari, Eric J. Baxter, C. Chang, Shivam Pandey, Andrés N. Salcedo, David H. Weinberg, Ariel Amsellem, Nicholas Battaglia, Matthew Belyakov, Tara Dacunha, S. J. Goldstein, Andrey V. Kravtsov, T N Varga, T. M. C. Abbott, M. Aguena, A. Alarcon, S. Allam, A. Amon, F. Andrade-Oliveira, J. Annis, David Bacon, K. Bechtol, M. R. Becker, G. M. Bernstein, E. Bertin, S. Bocquet, J. R. Bond, D. Brooks, E. Buckley‐Geer, D. L. Burke, A. Campos, A. Carnero Rosell, M. Carrasco Kind, J. Carretero, Ritchie Chen, A. Choi, M. Costanzi, L. N. da Costa, J. DeRose, S. Desai, J. De Vicente, Mark J. Devlin, H. T. Diehl, J. P. Dietrich, Scott Dodelson, P. Doel, C. Doux, A. Drlica-Wagner, K. Eckert, J. Elvin-Poole, S. Everett, Simone Ferraro, I. Ferrero, A. Ferté, B. Flaugher, J. Frieman, Patricio A. Gallardo, M. Gatti, E. Gaztañaga, D. W. Gerdes, D. Gruen, R. A. Gruendl, G. Gutiérrez, I. Harrison, W G Hartley, J. Colin Hill, Matt Hilton, S. R. Hinton, John P. Hughes, D. J. James, Mike Jarvis, T. Jeltema, Brian J. Koopman, E. Krause, K. Kuehn, N. Kuropatkin, O. Lahav, M. Lima, Martine Lokken, N. MacCrann, Mathew S. Madhavacheril, M. A. G. Maia, J. McCullough, J. J. McMahon, P. Melchior, F. Menanteau, R. Miquel, J. J. Mohr, Kavilan Moodley, R. Morgan, J. Myles, F. Nati, A Navarro-Alsina, Michael D. Niemack, R. L. C. Ogando, Lyman A. Page, A. Palmese, Bruce Partridge, F. Paz-Chinchón, M. E. S. Pereira, A. Pieres, J. Prat, Marco Raveri, M. Rodríguez-Monroy, R. P. Rollins, A. K. Romer, E. S. Rykoff, Maria Salatino, C. Sánchez, E. Sánchez, B. Santiago, V. Scarpine, A. Schillaci, L. F. Secco, S. Serrano, I. Sevilla-Noarbe, E. Sheldon, B. D. Sherwin, Cristobál Sifón, M. Smith, M. Soares-Santos, Suzanne T. Staggs, E. Suchyta, M. E. C. Swanson, G. Tarlé, D. Thomas, C. To, M. A. Troxel, I. Tutusaus, Eve M. Vavagiakis, J. Weller, Edward J. Wollack, B. Yanny, B. Yin, Y. Zhang

Bibliographic record

VenueMonthly Notices of the Royal Astronomical Society · 2021
Typepreprint
Languageen
FieldPhysics and Astronomy
TopicGalaxies: Formation, Evolution, Phenomena
Canadian institutionsCanadian Institute for Theoretical AstrophysicsPerimeter InstituteUniversity of Toronto
FundersSLAC National Accelerator LaboratoryLawrence Berkeley National LaboratoryFermilabUniversity of EdinburghIntegrated Electronics Engineering Center, Binghamton UniversityMinistério da Ciência, Tecnologia e InovaçãoScience and Technology Facilities CouncilUniversity of Illinois at Urbana-ChampaignEuropean Regional Development FundInstitut Périmètre de physique théoriqueUniversity of SussexInstitut de Física d'Altes EnergiesInyuvesi Yakwazulu-NataliOhio State UniversityLeibniz-RechenzentrumU.S. Department of EnergyFundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de JaneiroCentro de Investigaciones Energéticas, Medioambientales y TecnológicasMinistry of Colleges and UniversitiesConselho Nacional de Desenvolvimento Científico e TecnológicoUniversity of TorontoGeneralitat de CatalunyaOffice of ScienceGauss Centre for SupercomputingNational Research FoundationArgonne National LaboratoryComisión Nacional de Investigación Científica y TecnológicaPartnership for Advanced Computing in Europe AISBLIndustry CanadaNational Aeronautics and Space AdministrationUniversity College LondonGovernment of CanadaUniversity of CambridgeHigh Energy PhysicsDeutsche ForschungsgemeinschaftHigher Education Funding Council for EnglandCentres de Recerca de CatalunyaGovernment of OntarioStanford UniversityFinanciadora de Estudos e ProjetosUniversity of PennsylvaniaUniversity of PortsmouthUniversity of ChicagoMinisterio de Ciencia e InnovaciónEuropean CommissionPrinceton UniversityUniversity of NottinghamLeibniz-GemeinschaftNational Science FoundationUniversity of MichiganCompute Canada
KeywordsPhysicsAstrophysicsGalaxy clusterWeak gravitational lensingDark matterGalaxyHaloRedshiftCluster (spacecraft)Mass distributionAstronomy

Abstract

fetched live from OpenAlex

ABSTRACT We present measurements of the radial profiles of the mass and galaxy number density around Sunyaev–Zel’dovich (SZ)-selected clusters using both weak lensing and galaxy counts. The clusters are selected from the Atacama Cosmology Telescope Data Release 5 and the galaxies from the Dark Energy Survey Year 3 data set. With signal-to-noise ratio of 62 (45) for galaxy (weak lensing) profiles over scales of about 0.2–20 h−1 Mpc, these are the highest precision measurements for SZ-selected clusters to date. Because SZ selection closely approximates mass selection, these measurements enable several tests of theoretical models of the mass and light distribution around clusters. Our main findings are: (1) The splashback feature is detected at a consistent location in both the mass and galaxy profiles and its location is consistent with predictions of cold dark matter N-body simulations. (2) The full mass profile is also consistent with the simulations. (3) The shapes of the galaxy and lensing profiles are remarkably similar for our sample over the entire range of scales, from well inside the cluster halo to the quasilinear regime. We measure the dependence of the profile shapes on the galaxy sample, redshift, and cluster mass. We extend the Diemer & Kravtsov model for the cluster profiles to the linear regime using perturbation theory and show that it provides a good match to the measured profiles. We also compare the measured profiles to predictions of the standard halo model and simulations that include hydrodynamics. Applications of these results to cluster mass estimation, cosmology, and astrophysics are discussed.

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)0.000
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 score0.006
Threshold uncertainty score0.012

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0000.001
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0010.000
Science and technology studies0.0000.000
Scholarly communication0.0000.000
Open science0.0000.000
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 head0.006
GPT teacher head0.192
Teacher spread0.186 · 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

Citations3
Published2021
Admission routes2
Has abstractyes

Explore more

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