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Record W2901118233 · doi:10.1093/mnras/stz1434

Measurement of the splashback feature around SZ-selected Galaxy clusters with DES, SPT, and ACT

2019· article· en· W2901118233 on OpenAlexaff
T. Shin, Susmita Adhikari, Eric J. Baxter, C. Chang, Bhuvnesh Jain, Nicholas Battaglia, L. E. Bleem, S. Bocquet, Joseph DeRose, D. Gruen, Matt Hilton, Andrey V. Kravtsov, Thomas McClintock, Eduardo Rozo, E. S. Rykoff, T N Varga, Risa H. Wechsler, Hao‐Yi Wu, Z Zhang, Simone Aiola, S. Allam, K. Bechtol, B. A. Benson, E. Bertin, J. R. Bond, M. Brodwin, David H. Brooks, E Buckley-Geer, D. L. Burke, J E Carlstrom, A. Carnero Rosell, M. Carrasco Kind, J. Carretero, F. J. Castander, Steve K. Choi, C. E. Cunha, T M Crawford, L. N. da Costa, J. De Vicente, S Desai, Mark J. Devlin, J. P. Dietrich, P. Doel, Jo Dunkley, T F Eifler, A. E. Evrard, B Flaugher, P Fosalba, P A Gallardo, J. García-Bellido, E. Gaztañaga, D. W. Gerdes, M Gralla, R. A. Gruendl, J Gschwend, N. Gupta, G. Gutiérrez, W. G. Hartley, J. Colin Hill, S P Ho, K Honscheid, B Hoyle, K. M. Huffenberger, John P. Hughes, D J James, T Jeltema, A G Kim, E. Krause, K. Kuehn, O. Lahav, M. Lima, Mathew S. Madhavacheril, M A G Maia, J L Marshall, L. Maurin, J. J. McMahon, F. Menanteau, Carol J. Miller, R Miquel, J. J. Mohr, Sigurd Næss, F. Nati, Michael D. Niemack, R. L. C. Ogando, Lyman A. Page, Bruce Partridge, S Patil, David Rapetti, C L Reichardt, A. K. Romer, E Sanchez, V. Scarpine, R Schindler, S. Serrano, M. Smith, Rory Smith, M Soares-Santos, F Sobreira, Suzanne T. Staggs, A. A. Stark, George Stein, E. Suchyta, M. E. C. Swanson, G. Tarlé, D. Thomas, Edward J. Wollack, Zhilei Xu

Bibliographic record

VenueMonthly Notices of the Royal Astronomical Society · 2019
Typearticle
Languageen
FieldPhysics and Astronomy
TopicGalaxies: Formation, Evolution, Phenomena
Canadian institutionsCanadian Institute for Theoretical AstrophysicsUniversity of Toronto
FundersArgonne National LaboratoryAustralian Research CouncilERAB: The European Foundation for Alcohol ResearchConselho Nacional de Desenvolvimento Científico e TecnológicoDeutsche ForschungsgemeinschaftUniversity of EdinburghScience and Technology Facilities CouncilNational Aeronautics and Space AdministrationUniversity College LondonUniversity of CambridgeMinistério da Ciência, Tecnologia e InovaçãoLawrence Berkeley National LaboratoryFinanciadora de Estudos e ProjetosUniversity of PennsylvaniaHigher Education Funding Council for EnglandUniversity of PortsmouthUniversity of ChicagoOhio State UniversityUniversity of NottinghamStanford UniversityU.S. Department of EnergyUniversity of Illinois at Urbana-ChampaignUniversity of SussexSeventh Framework ProgrammeEuropean Research CouncilGordon and Betty Moore FoundationUniversity of MichiganNational Science Foundation
KeywordsPhysicsAstrophysicsGalaxyFeature (linguistics)Galaxy clusterAstronomy

Abstract

fetched live from OpenAlex

ABSTRACT We present a detection of the splashback feature around galaxy clusters selected using the Sunyaev–Zel’dovich (SZ) signal. Recent measurements of the splashback feature around optically selected galaxy clusters have found that the splashback radius, rsp, is smaller than predicted by N-body simulations. A possible explanation for this discrepancy is that rsp inferred from the observed radial distribution of galaxies is affected by selection effects related to the optical cluster-finding algorithms. We test this possibility by measuring the splashback feature in clusters selected via the SZ effect in data from the South Pole Telescope SZ survey and the Atacama Cosmology Telescope Polarimeter survey. The measurement is accomplished by correlating these cluster samples with galaxies detected in the Dark Energy Survey Year 3 data. The SZ observable used to select clusters in this analysis is expected to have a tighter correlation with halo mass and to be more immune to projection effects and aperture-induced biases, potentially ameliorating causes of systematic error for optically selected clusters. We find that the measured rsp for SZ-selected clusters is consistent with the expectations from simulations, although the small number of SZ-selected clusters makes a precise comparison difficult. In agreement with previous work, when using optically selected redMaPPer clusters with similar mass and redshift distributions, rsp is ∼2σ smaller than in the simulations. These results motivate detailed investigations of selection biases in optically selected cluster catalogues and exploration of the splashback feature around larger samples of SZ-selected clusters. Additionally, we investigate trends in the galaxy profile and splashback feature as a function of galaxy colour, finding that blue galaxies have profiles close to a power law with no discernible splashback feature, which is consistent with them being on their first infall into the cluster.

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 score0.005
Threshold uncertainty score0.010

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0000.001
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0010.001
Science and technology studies0.0000.000
Scholarly communication0.0000.000
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 head0.173
Teacher spread0.168 · 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".

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Citations80
Published2019
Admission routes1
Has abstractyes

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