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Record W4389943295 · doi:10.1051/0004-6361/202346012

J-PLUS: Toward a homogeneous photometric calibration using <i>Gaia</i> BP/RP low-resolution spectra

2023· article· en· W4389943295 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 · 2023
Typearticle
Languageen
FieldEngineering
TopicCCD and CMOS Imaging Sensors
Canadian institutionsnot available
FundersPlanetary Science DivisionNational Astronomical Observatories, Chinese Academy of SciencesEuropean Regional Development FundAgencia Estatal de InvestigaciónScience Mission DirectorateMax-Planck-Institut für AstronomieJiangsu Association for Science and TechnologySmithsonian Astrophysical ObservatoryNational Development and Reform CommissionEuropean CommissionMinisterio de Ciencia e InnovaciónUniversitat de BarcelonaConselho Nacional de Desenvolvimento Científico e TecnológicoMinisterio de Economía y CompetitividadQueen's UniversityChinese Academy of SciencesFundação de Amparo à Pesquisa do Estado de São PauloSpace Telescope Science InstituteNational Central UniversityInstitut de Ciències del CosmosFinanciadora de Estudos e ProjetosQueen's University BelfastMinisterio de Ciencia, Innovación y UniversidadesGordon and Betty Moore FoundationEötvös Loránd TudományegyetemLos Alamos National LaboratoryEuropean Space AgencyJohns Hopkins UniversityNational Science FoundationNational Aeronautics and Space AdministrationDurham UniversitySmithsonian Institution
KeywordsPhysicsAstrophysicsHomogeneousCalibrationSpectral lineLow resolutionResolution (logic)AstronomySpectral resolutionHigh resolutionRemote sensingStatistical physics

Abstract

fetched live from OpenAlex

Aims . We present the photometric calibration of the 12 optical passbands for the Javalambre Photometric Local Universe Survey (J-PLUS) third data release (DR3) comprising 1642 pointings of two square degrees each. Methods . We selected nearly 1.5 million main sequence stars with a signal-to-noise ratio larger than ten in the 12 J-PLUS passbands and available low-resolution ( R = 20–80) spectrum from the blue and red photometers (BP/RP) in Gaia DR3. We compared the synthetic photometry from BP/RP spectra with the J-PLUS instrumental magnitudes after correcting for the magnitude and color terms between both systems in order to obtain a homogeneous photometric solution for J-PLUS. To circumvent the current limitations in the absolute calibration of the BP/RP spectra, the absolute color scale was derived using the locus of 109 white dwarfs closer than 100 pc with a negligible interstellar extinction. Finally, the absolute flux scale was anchored to the Panoramic Survey Telescope and Rapid Response System (Pan-STARRS) photometry in the r band. Results . The precision of the J-PLUS photometric calibration estimated from duplicated objects observed in adjacent pointings and by comparison with the spectro-photometric standard star GD 153 is ~12 mmag in u , J 0378, and J 0395, and it is ~7 mmag in J 0410, J 0430, ɡ , J 0515, r , J 0660, i , J 0861, and z . The estimated accuracy in the calibration along the surveyed area is better than 1% for all the passbands. Conclusions . The Gaia BP/RP spectra provide a high-quality, homogeneous photometric reference in the optical range across the full sky in spite of their current limitations as an absolute reference. The calibration method for J-PLUS DR3 reaches an absolute precision and accuracy of 1% in the 12 optical filters within an area of 3284 square degrees.

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 categoriesnone
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Simulation or modeling · Consensus signal: Simulation or modeling
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.279
Threshold uncertainty score0.810

Codex and Gemma teacher scores by category

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

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 head0.011
GPT teacher head0.201
Teacher spread0.189 · 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