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Record W4318751871 · doi:10.48550/arxiv.2301.12395

J-PLUS: Towards an homogeneous photometric calibration using Gaia BP/RP low-resolution spectra

2023· preprint· en· W4318751871 on OpenAlexfundno aff
C. López-Sanjuán, H. Vázquez Ramió, K. Xiao, H. Yuan, J. M. Carrasco, J. Varela, D. Cristòbal-Hornillos, Pier-Emmanuel Tremblay, A. Ederoclite, A. Marín-Franch, A. J. Cenarro, P. Coelho, S. Daflon, A. del Pino, H. Domínguez Sánchez, J. A. Fernández-Ontiveros, A. Hernán-Caballero, F. Jiménez-Esteban, J. Alcaniz, Raúl E. Angulo, R. A. Dupke, C. Hernández–Monteagudo, M. Moles, L. Sodré

Bibliographic record

VenuearXiv (Cornell University) · 2023
Typepreprint
Languageen
FieldPhysics and Astronomy
TopicStellar, planetary, and galactic studies
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
KeywordsPhotometry (optics)PhysicsAstrophysicsPhotometerStarsWhite dwarfPhotometric systemSkySpectral lineCalibrationTelescopeSpectral resolutionAstronomy

Abstract

fetched live from OpenAlex

We present the photometric calibration of the twelve optical passbands for the Javalambre Photometric Local Universe Survey (J-PLUS) third data release (DR3), comprising 1642 pointings of two square degrees each. We selected nearly 1.5 million main sequence stars with a signal-to-noise ratio larger than ten in the twelve 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, to obtain an 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. 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, J0378, and J0395; and ~7 mmag in J0410, J0430, g, J0515, r, J0660, i, J0861, and z. The estimated accuracy in the calibration along the surveyed area is better than 1% for all the passbands. 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 twelve 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.

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)0.003
metaresearch head score (Gemma)0.004
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 score0.012
Threshold uncertainty score0.023

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0030.004
Meta-epidemiology (narrow)0.0010.001
Meta-epidemiology (broad)0.0010.001
Bibliometrics0.0020.002
Science and technology studies0.0000.000
Scholarly communication0.0010.001
Open science0.0010.002
Research integrity0.0000.001
Insufficient payload (model declined to judge)0.0010.002

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 head0.090
GPT teacher head0.215
Teacher spread0.125 · 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
Published2023
Admission routes1
Has abstractyes

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