MétaCan
Menu
← Back to cohort
Record W7116941877 · doi:10.1103/n7p5-pc66

Atacama Cosmology Telescope: A measurement of galaxy cluster temperatures through relativistic corrections to the thermal Sunyaev-Zeldovich effect

2025· article· en· W7116941877 on OpenAlexafffund
Adriaan J. Duivenvoorden, Zachary Atkins, Nicholas Battaglia, E. S. Battistelli, J Richard Bond, Hongbo Cai, Erminia Calabrese, S. Choi, Kevin D. Crowley, Mark J. Devlin, Jo Dunkley, Yilun Guan, Carlos Hervías-Caimapo, J. Colin Hill, Matt Hilton, Adam D. Hincks, Mathew S. Madhavacheril, Joshiwa van Marrewijk, Fiona McCarthy, Kavilan Moodley, Tony Mroczkowski, Michael D. Niemack, Lyman Page, Bruce Partridge, E. Schaan, Neelima Sehgal, B. D. Sherwin, Cristóbal Sifón, David N. Spergel, Alexander Van Engelen, Eve M. Vavagiakis, Edward J. Wollack

Bibliographic record

VenuePhysical review. D/Physical review. D. · 2025
Typearticle
Languageen
FieldPhysics and Astronomy
TopicGalaxies: Formation, Evolution, Phenomena
Canadian institutionsCanadian Institute for Theoretical AstrophysicsUniversity of Toronto
FundersFaculty of Arts and SciencesNational Institute of Standards and TechnologyAgencia Nacional de Investigación y DesarrolloUniversity of British ColumbiaUniversity of TorontoNiagara Community FoundationNational Energy Research Scientific Computing CenterNational Aeronautics and Space AdministrationCanada Foundation for InnovationUniversity of PennsylvaniaPrinceton UniversityNational Science FoundationCompute CanadaSimons FoundationGovernment of OntarioNatural Sciences and Engineering Research Council of CanadaFlatiron Health
KeywordsCosmologyGalaxy clusterAmplitudeCluster (spacecraft)GalaxyMeasure (data warehouse)ObservatoryStack (abstract data type)Thermal

Abstract

fetched live from OpenAlex

The high electron temperature in galaxy clusters ( > 1 keV or > 10 7 K ) leads to corrections at the level of a few percent in their thermal Sunyaev-Zeldovich effect signatures. Both the size and frequency dependence of these corrections, which are known as relativistic temperature corrections, depend upon the temperature of the objects. In this work we exploit this effect to measure the average temperature of a stack of Compton- y selected clusters. Specifically, we apply the “spectroscopic method” and search for the temperature that best fits the clusters’ signal measured at frequencies from 30 to 545 GHz by the Atacama Cosmology Telescope and satellite. We measure the average temperature of clusters detected in the Atacama Cosmology Telescope maps to be 8.5 ± 2.4 keV , with an additional systematic error of comparable amplitude dominated by passband uncertainty. Upcoming surveys, such as the Simons Observatory and CMB-S4, have the potential to dramatically improve upon these measurements and thereby enable precision studies of cluster temperatures with millimeter observations. The key challenge for future observations will be mitigating instrumental systematic effects, which already limit this analysis.

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)0.002
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 score0.020
Threshold uncertainty score0.041

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0010.002
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.001
Bibliometrics0.0010.002
Science and technology studies0.0010.000
Scholarly communication0.0010.001
Open science0.0010.001
Research integrity0.0010.001
Insufficient payload (model declined to judge)0.0060.003

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 head0.011
GPT teacher head0.356
Teacher spread0.345 · 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

Citations1
Published2025
Admission routes2
Has abstractyes

Explore more

Same venuePhysical review. D/Physical review. D.→Same topicGalaxies: Formation, Evolution, Phenomena→French-language works237,207→