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Record W4306996170 · doi:10.1093/mnras/stad1167

Mapping gas around massive galaxies: cross-correlation of DES Y3 galaxies and Compton-<i>y</i>maps from SPT and<i>Planck</i>

2023· article· en· W4306996170 on OpenAlexafffund
Javier Sánchez, Y. Omori, C. Chang, L. E. Bleem, Thomas O. Crawford, A Drlica-Wagner, S. Raghunathan, Georgios Zacharegkas, T. M. C. Abbott, M. Aguena, A. Alarcon, S. Allam, O. Alves, A. Amon, S. Àvila, Eric J. Baxter, K. Bechtol, B. A. Benson, G. M. Bernstein, E. Bertin, S. Bocquet, David H. Brooks, D. L. Burke, A. Campos, J. E. Carlstrom, A. Carnero Rosell, M. Carrasco Kind, J. Carretero, F. J. Castander, R. Cawthon, C. L. Chang, Angela Chen, A. Choi, Ryan Chown, M. Costanzi, A. T. Crites, M. Crocce, L. N. da Costa, M. E. S. Pereira, T. de Haan, J. De Vicente, Joseph DeRose, S Desai, H. T. Diehl, M. Dobbs, Scott Dodelson, P. Doel, J. Elvin-Poole, W. Everett, S Everett, I. Ferrero, B. Flaugher, P. Fosalba, J. García-Bellido, M. Gatti, E. M. George, D. W. Gerdes, G. Giannini, D. Gruen, R. A. Gruendl, J. Gschwend, G. Gutiérrez, N. W. Halverson, S. R. Hinton, G. P. Holder, W. L. Holzapfel, K. Honscheid, J. D. Hrubes, D. J. James, L. Knox, K. Kuehn, N. Kuropatkin, O. Lahav, A. T. Lee, D. Luong-Van, N. MacCrann, J. L. Marshall, J. McCullough, J. J. McMahon, P. Melchior, J. Mena-Fernández, F. Menanteau, R. Miquel, L. M. Mocanu, J. J. Mohr, J. Muir, J. Myles, T. Natoli, S. Padin, A. Palmese, S. Pandey, F. Paz-Chinchón, A. Pieres, A. A. Plazas, A. Porredon, C. Pryke, Marco Raveri, C. L. Reichardt, M. Rodríguez-Monroy, Ashley J. Ross, J. E. Ruhl, E. S. Rykoff, C. Sánchez, E. Sánchez, V. Scarpine, K. K. Schaffer, I. Sevilla-Noarbe, E. Sheldon, E. Shirokoff, M. Smith, M. Soares-Santos, Z. Staniszewski, A. A. Stark, E. Suchyta, M. E. C. Swanson, G. Tarlé, D. Thomas, M. A. Troxel, D. L. Tucker, J. D. Vieira, M. Vincenzi, N. Weaverdyck, R. Williamson, B. Yanny, B. Yin

Bibliographic record

VenueMonthly Notices of the Royal Astronomical Society · 2023
Typearticle
Languageen
FieldPhysics and Astronomy
TopicGalaxies: Formation, Evolution, Phenomena
Canadian institutionsUniversity of TorontoPerimeter InstituteMcGill UniversityCanadian Institute for Advanced ResearchCanadian Institute for Theoretical AstrophysicsWestern University
FundersSLAC National Accelerator LaboratoryH2020 European Research CouncilIntegrated Electronics Engineering Center, Binghamton UniversityEuropean Regional Development FundAustralian Research CouncilNatural Sciences and Engineering Research Council of CanadaScience and Technology Facilities CouncilUniversity of Colorado BoulderUniversity of Illinois at Urbana-ChampaignInstitut de Física d'Altes EnergiesConselho Nacional de Desenvolvimento Científico e TecnológicoEuropean CommissionMinisterio de Ciencia e InnovaciónGeneralitat de CatalunyaOffice of ScienceUniversity of EdinburghLawrence Berkeley National LaboratoryUniversity of PennsylvaniaFinanciadora de Estudos e ProjetosFundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de JaneiroUniversity of SussexUniversity of NottinghamNational Energy Research Scientific Computing CenterUniversity of PortsmouthUniversity College LondonUniversity of MichiganOhio State UniversityMinistério da Ciência, Tecnologia e InovaçãoLudwig-Maximilians-Universität MünchenHigh Energy PhysicsMcGill UniversityDeutsche ForschungsgemeinschaftArgonne National LaboratoryCentres de Recerca de CatalunyaUniversity of ChicagoU.S. Department of EnergyFermilabNational Science Foundation
KeywordsPhysicsAstrophysicsRedshiftGalaxyHydrostatic equilibriumHaloPlanckAstronomy

Abstract

fetched live from OpenAlex

ABSTRACT We cross-correlate positions of galaxies measured in data from the first three years of the Dark Energy Survey with Compton-y maps generated using data from the South Pole Telescope (SPT) and the Planck mission. We model this cross-correlation measurement together with the galaxy autocorrelation to constrain the distribution of gas in the Universe. We measure the hydrostatic mass bias or, equivalently, the mean halo bias-weighted electron pressure 〈bhPe 〉, using large-scale information. We find 〈bhPe 〉 to be $[0.16^{+0.03}_{-0.04},0.28^{+0.04}_{-0.05},0.45^{+0.06}_{-0.10},0.54^{+0.08}_{-0.07},0.61^{+0.08}_{-0.06},0.63^{+0.07}_{-0.08}]$ meV cm−3 at redshifts z ∼ [0.30, 0.46, 0.62, 0.77, 0.89, 0.97]. These values are consistent with previous work where measurements exist in the redshift range. We also constrain the mean gas profile using small-scale information, enabled by the high-resolution of the SPT data. We compare our measurements to different parametrized profiles based on the cosmo-OWLS hydrodynamical simulations. We find that our data are consistent with the simulation that assumes an AGN heating temperature of 108.5 K but are incompatible with the model that assumes an AGN heating temperature of 108.0 K. These comparisons indicate that the data prefer a higher value of electron pressure than the simulations within r500c of the galaxies’ haloes.

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 score0.016
Threshold uncertainty score0.032

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 head0.009
GPT teacher head0.206
Teacher spread0.197 · 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
Published2023
Admission routes2
Has abstractyes

Explore more

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