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Record W2984655719 · doi:10.1093/mnras/stz3188

X-ray study of the double source plane gravitational lens system Eye of Horus observed with <i>XMM–Newton</i>

2019· article· en· W2984655719 on OpenAlexfundno aff
Keigo Tanaka, Ayumi Tsuji, Hiroki Akamatsu, J. H. H. Chan, Jean Coupon, Eiichi Egami, F. Finet, Ryuichi Fujimoto, Yuto Ichinohe, Anton T. Jaelani, Chien‐Hsiu Lee, Ikuyuki Mitsuishi, Anupreeta More, Surhud More, Masamune Oguri, N. Okabe, Naomi Ota, Cristian E. Rusu, Alessandro Sonnenfeld, Masayuki Tanaka, Shutaro Ueda, Kenneth C. Wong

Bibliographic record

VenueMonthly Notices of the Royal Astronomical Society · 2019
Typearticle
Languageen
FieldPhysics and Astronomy
TopicGalaxies: Formation, Evolution, Phenomena
Canadian institutionsnot available
FundersJapan Society for the Promotion of ScienceSmithsonian Astrophysical ObservatoryLos Alamos National LaboratoryNational Astronomical Observatory of JapanJapan Science and Technology AgencyQueen's UniversityChinese Academy of SciencesEötvös Loránd TudományegyetemAcademia SinicaUniversity of MarylandDurham UniversitySpace Telescope Science InstituteMinistry of Science and Technology, TaiwanPrinceton UniversityMinistry of Education, Culture, Sports, Science and TechnologyKorea Astronomy and Space Science InstituteNational Aeronautics and Space AdministrationUniversity of Hawai'iUniversity of EdinburghJohns Hopkins UniversityNational Science Foundation
KeywordsPhysicsAstrophysicsHydrostatic equilibriumGalaxyCluster (spacecraft)RADIUSGravitationLens (geology)Gravitational lensPlane (geometry)Galaxy clusterAstronomyGeometryOptics

Abstract

fetched live from OpenAlex

ABSTRACT A double source plane (DSP) system is a precious probe for the density profile of distant galaxies and cosmological parameters. However, these measurements could be affected by the surrounding environment of the lens galaxy. Thus, it is important to evaluate the cluster-scale mass for detailed mass modelling. We observed the Eye of Horus, a DSP system discovered by the Hyper Suprime-Cam Subaru Strategic Survey (HSC–SSP), with XMM–Newton. We detected two X-ray extended emissions, originating from two clusters, one centred at the Eye of Horus, and the other located ∼100 arcsec north-east to the Eye of Horus. We determined the dynamical mass assuming hydrostatic equilibrium, and evaluated their contributions to the lens mass interior of the Einstein radius. The contribution of the former cluster is $1.1^{+1.2}_{-0.5}\times 10^{12}\, \mathrm{M}_{\odot }$, which is $21\!-\!76{{\ \rm per\ cent}}$ of the total mass within the Einstein radius. The discrepancy is likely due to the complex gravitational structure along the line of sight. On the other hand, the contribution of the latter cluster is only $\sim 2{{\ \rm per\ cent}}$ on the Eye of Horus. Therefore, the influence associated with this cluster can be ignored.

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)0.000
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
Metaresearch0.0000.000
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0010.000
Science and technology studies0.0010.000
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 head0.184
Teacher spread0.176 · 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

Citations2
Published2019
Admission routes1
Has abstractyes

Explore more

Same venueMonthly Notices of the Royal Astronomical Society→Same topicGalaxies: Formation, Evolution, Phenomena→French-language works237,207→