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Record W4281725952 · doi:10.1051/0004-6361/202243709

<i>Gaia</i>Data Release 3

2022· article· en· W4281725952 on OpenAlex

Why this work is in the frame

A frame that forgets how it found something cannot be audited. These are the routes that admitted this work.

fundA Canadian funder is recorded on the work.
no affNo Canadian affiliation: this work is invisible to an affiliation-only frame.
No Canadian affiliation. An affiliation-only frame, the usual design, would never have seen this work. It is one of the works that make the case for inverting the frame.

Bibliographic record

VenueAstronomy and Astrophysics · 2022
Typearticle
Languageen
FieldPhysics and Astronomy
TopicScientific Research and Discoveries
Canadian institutionsnot available
FundersLos Alamos National LaboratoryAustralian Research CouncilEuropean Space AgencySmithsonian Astrophysical ObservatoryOffice of ScienceUniversity of Colorado BoulderCarnegie Institution for ScienceUniversity of MelbourneInstituto de Astrofísica de CanariasMax-Planck-Institut für AstrophysikEötvös Loránd TudományegyetemNational Central UniversityYork UniversityMinistério da Ciência, Tecnologia e InovaçãoYale UniversityU.S. Department of EnergyUniversity of QueenslandUniversity of EdinburghQueen's UniversityLawrence Berkeley National LaboratoryMonash UniversityMax-Planck-Institut für AstronomieUniversity of OxfordAustralian National Data ServiceDurham UniversityGordon and Betty Moore FoundationUniversity of SydneyAustralian GovernmentUniversidad Nacional Autónoma de MéxicoSpace Telescope Science InstituteAustralian National UniversityUniversity of PortsmouthUniversity of UtahNew Mexico State UniversityNational Cancer InstituteAustralian Astronomical Optics-MacquarieAstronomy Australia LimitedUniversity of Notre DameCurtin University of TechnologyUniversity of WashingtonAlfred P. Sloan FoundationJohns Hopkins UniversityCarnegie Mellon UniversityPlanetary Science DivisionCarnegie Institution of WashingtonOhio State UniversityVanderbilt UniversityLeibniz-GemeinschaftScience Mission DirectorateNational Computational InfrastructureSmithsonian InstitutionNational Aeronautics and Space AdministrationSwinburne University of TechnologyQueen's University BelfastNational Science Foundation
KeywordsPhysicsAstrophysicsAstronomy

Abstract

fetched live from OpenAlex

Gaia Data Release 3 provides novel flux-calibrated low-resolution spectrophotometry for ≃220 million sources in the wavelength range 330 nm ≤ λ ≤ 1050 nm (XP spectra). Synthetic photometry directly tied to a flux in physical units can be obtained from these spectra for any passband fully enclosed in this wavelength range. We describe how synthetic photometry can be obtained from XP spectra, illustrating the performance that can be achieved under a range of different conditions – for example passband width and wavelength range – as well as the limits and the problems affecting it. Existing top-quality photometry can be reproduced within a few per cent over a wide range of magnitudes and colour, for wide and medium bands, and with up to millimag accuracy when synthetic photometry is standardised with respect to these external sources. Some examples of potential scientific application are presented, including the detection of multiple populations in globular clusters, the estimation of metallicity extended to the very metal-poor regime, and the classification of white dwarfs. A catalogue providing standardised photometry for ≃2.2 × 10 8 sources in several wide bands of widely used photometric systems is provided ( Gaia Synthetic Photometry Catalogue; GSPC) as well as a catalogue of ≃10 5 white dwarfs with DA/non-DA classification obtained with a Random Forest algorithm ( Gaia Synthetic Photometry Catalogue for White Dwarfs; GSPC-WD).

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.

Full frame distilled prediction

Teacher imitation

Not calibrated prevalence, not ground truth. Human validation pending. Learned from the 10,348 direct Codex labels and 10,348 direct Gemma labels. Candidate is the union of thresholded teacher heads; consensus is their intersection. These outputs are machine_predicted_unvalidated and are not human labels or direct frontier model labels.

metaresearch head score (Codex)0.000
metaresearch head score (Gemma)0.000
Version: codex-gemma-dda1882f352aValidation status: machine_predicted_unvalidated
Candidate categoriesInsufficient payload (model declined to judge)
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Not applicable · Consensus signal: none
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.965
Threshold uncertainty score1.000

Codex and Gemma teacher scores by category

CategoryCodexGemma
Metaresearch0.0000.000
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0000.000
Science and technology studies0.0010.000
Scholarly communication0.0000.000
Open science0.0010.001
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 head0.018
GPT teacher head0.251
Teacher spread0.232 · 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