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Record W6967396438 · doi:10.5167/uzh-179327

A gravitational-wave measurement of the Hubble constant following the second observing run of Advanced LIGO and Virgo

2019· article· en· W6967396438 on OpenAlexfundno aff

Bibliographic record

VenueZurich Open Repository and Archive (University of Zurich) · 2019
Typearticle
Languageen
FieldPhysics and Astronomy
TopicPulsars and Gravitational Waves Research
Canadian institutionsnot available
FundersDivision of Human Resource DevelopmentScience and Technology Facilities CouncilICTP South American Institute for Fundamental ResearchIstituto Nazionale di Fisica NucleareAbdus Salam International Centre for Theoretical PhysicsNemzeti Kutatási Fejlesztési és Innovációs HivatalLeverhulme TrustScottish Funding CouncilRussian Science FoundationInstitut des Origines de LyonMinistero dello Sviluppo EconomicoMinistry of Education, IndiaNational Research Foundation of KoreaHungarian Scientific Research FundGeneralitat ValencianaCouncil of Scientific and Industrial Research, IndiaCentre National de la Recherche ScientifiqueIndustry CanadaNational Natural Science Foundation of ChinaEuropean CommissionGovern de les Illes BalearsNederlandse Organisatie voor Wetenschappelijk OnderzoekNational Research FoundationRussian Foundation for Basic ResearchEuropean Regional Development FundScottish Universities Physics AllianceConseil Régional, Île-de-FranceNational Research, Development and Innovation OfficeAgencia Estatal de InvestigaciónSchweizerischer Nationalfonds zur Förderung der Wissenschaftlichen ForschungScience and Engineering Research BoardNational Science Foundation
KeywordsLIGOHubble's lawGalaxyNeutron starSkyBinary numberCosmologyBinary black hole

Abstract

fetched live from OpenAlex

This paper presents the gravitational-wave measurement of the Hubble constant H0 using the detections from the first and second observing runs of the Advanced LIGO and Virgo detector network. The presence of the transient electromagnetic counterpart of the binary neutron star GW170817 led to the first standard-siren measurement of H0. Here we additionally use binary black hole detections in conjunction with galaxy catalogs and report a joint measurement. Our updated measurement is H0=68+14−7km s−1Mpc−1 (68.3% highest density posterior interval with a flat-in-log prior) which is a 7\% improvement over the GW170817-only value of 68+18−8km s−1Mpc−1. A significant additional contribution currently comes from GW170814, a loud and well-localized detection from a part of the sky thoroughly covered by the Dark Energy Survey. Inclusion of contributions from all binary black hole detections entails a thorough marginalization over unknown population parameters. With numerous detections anticipated over the upcoming years, an exhaustive understanding of other systematic effects are also going to become increasingly important. These results establish the path to cosmology using gravitational-wave observations with and without transient electromagnetic counterparts.

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)0.003
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 score0.007
Threshold uncertainty score0.015

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0010.003
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0020.002
Science and technology studies0.0000.000
Scholarly communication0.0010.000
Open science0.0000.001
Research integrity0.0000.001
Insufficient payload (model declined to judge)0.0010.001

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 head0.014
GPT teacher head0.236
Teacher spread0.222 · 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

Citations0
Published2019
Admission routes1
Has abstractyes

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