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

<i>Gaia</i>Data Release 3

2022· article· en· W4281725952 on OpenAlexfundno aff
P. Montegriffo, M. Bellazzini, F. De Angeli, R. Andrae, M. A. Barstow, D. Bossini, A. Bragaglia, P. W. Burgess, C. Cacciari, J. M. Carrasco, N. Chornay, L. Delchambre, D. W. Evans, M. Fouesneau, Y. Frémat, D. Garabato, C. Jordi, M. Manteiga, D. Massari, L. Palaversa, E. Pancino, M. Riello, D. Ruz Mieres, N. Sanna, R. Santovena, R. Sordo, A. Vallenari, N. A. Walton

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.

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)0.002
metaresearch head score (Gemma)0.006
Version: metacan-v3-hybrid-931329e0061cValidation status: machine_predicted_unvalidated
Candidate categoriesnone
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Not applicable · Consensus signal: Not applicable
GenreCandidate signal: Dataset · Consensus signal: Dataset
Teacher disagreement score0.038
Threshold uncertainty score0.108

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0020.006
Meta-epidemiology (narrow)0.0010.001
Meta-epidemiology (broad)0.0010.002
Bibliometrics0.0050.005
Science and technology studies0.0010.000
Scholarly communication0.0030.001
Open science0.0020.002
Research integrity0.0010.002
Insufficient payload (model declined to judge)0.0320.059

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

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 designNot applicable
Domainnot available
GenreDataset

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

Citations83
Published2022
Admission routes1
Has abstractyes

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