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Record W3169603385 · doi:10.1051/0004-6361/202140735

<i>Gaia</i> Early Data Release 3

2021· article· en· W3169603385 on OpenAlexaff
S. T. Hodgkin, D. L. Harrison, E. Breedt, T. Wevers, G. Rixon, A. Delgado, A. Yoldas, Z. Kostrzewa-Rutkowska, Ł. Wyrzykowski, M. van Leeuwen, N. Blagorodnova, H. Campbell, D. Eappachen, M. Fraser, N. Ihanec, S. E. Koposov, K. Kruszyńska, G. Marton, Krzysztof A. Rybicki, A. G. A. Brown, P. W. Burgess, G. Busso, S. Cowell, F. De Angeli, C. Diener, D. W. Evans, G. Gilmore, G. Holland, P. G. Jonker, F. van Leeuwen, F. Mignard, P. Osborne, J. Portell, T. Prusti, P. J. Richards, M. Riello, G. M. Seabroke, N. A. Walton, P. Ábrahám, G. Altavilla, Steven G. Baker, U. Bastian, P. T. O’Brien, J. H. J. de Bruijne, T. Butterley, J. M. Carrasco, J. Castañeda, J. S. Clark, G. Clementini, C. M. Copperwheat, M. Cropper, G. Damljanović, M. Davidson, C. J. Davis, M. Dennefeld, V. S. Dhillon, M. Dominik, P. Esquej, L. Eyer, C. Fabricius, Mitja Fridman, D. Froebrich, N. Garralda, A. Gomboc, J. J. González-Vidal, R. Guerra, N. C. Hambly, L. K. Hardy, B. Holl, A. Hourihane, J. Japelj, Д. А. Канн, Csaba Kiss, C. Knigge, U. Kolb, S. Komossa, Á. Kóspál, Gábor Kovács, M. Kun, G. Leto, Fraser Lewis, S. P. Littlefair, A. Mahabal, C. G. Mundell, Z. Nagy, D. Padeletti, L. Palaversa, A. Pigulski, M. L. Pretorius, W. van Reeven, V. A. R. M. Ribeiro, M. Roelens, N. Rowell, N. Schartel, A. Scholz, A. Schwope, Brigitta Sipőcz, S. J. Smartt, M. Smith, I. Serraller, D. Steeghs, M. Sullivan, L. Szabados, E. Szegedi-Elek, P. Tisserand, L. Tomasella, Sjoert van Velzen, P. A. Whitelock, Richard Wilson, D. R. Young

Bibliographic record

VenueAstronomy and Astrophysics · 2021
Typearticle
Languageen
FieldPhysics and Astronomy
TopicGamma-ray bursts and supernovae
Canadian institutionsUniversity of LethbridgeScience North
FundersInstitut de Ciències del CosmosFundação para a Ciência e a TecnologiaBiotechnology and Biological Sciences Research CouncilMinistério da Ciência, Tecnologia e Ensino SuperiorUniversitat de BarcelonaIstituto Nazionale di AstrofisicaNederlandse Organisatie voor Wetenschappelijk OnderzoekMinisterstwo Edukacji i NaukiUniversity of BristolUniversity of EdinburghEuropean CommissionMinistarstvo Prosvete, Nauke i Tehnološkog RazvojaScience Foundation IrelandUK Space AgencyUniversity of CambridgeUniversity of LeicesterJavna Agencija za Raziskovalno Dejavnost RSLeverhulme TrustScience and Technology Facilities CouncilNational Research FoundationUniversity College LondonAgenzia Spaziale ItalianaEuropean Space Agency
KeywordsPhysicsPhotometry (optics)AstrometrySupernovaSkyGalaxyAstronomyAstrophysicsTransit (satellite)StarsFalse alarmFalse positive paradoxComputer scienceArtificial intelligence

Abstract

fetched live from OpenAlex

Context. Since July 2014, the Gaia mission has been engaged in a high-spatial-resolution, time-resolved, precise, accurate astrometric, and photometric survey of the entire sky. Aims. We present the Gaia Science Alerts project, which has been in operation since 1 June 2016. We describe the system which has been developed to enable the discovery and publication of transient photometric events as seen by Gaia . Methods. We outline the data handling, timings, and performances, and we describe the transient detection algorithms and filtering procedures needed to manage the high false alarm rate. We identify two classes of events: (1) sources which are new to Gaia and (2) Gaia sources which have undergone a significant brightening or fading. Validation of the Gaia transit astrometry and photometry was performed, followed by testing of the source environment to minimise contamination from Solar System objects, bright stars, and fainter near-neighbours. Results. We show that the Gaia Science Alerts project suffers from very low contamination, that is there are very few false-positives. We find that the external completeness for supernovae, C E = 0.46, is dominated by the Gaia scanning law and the requirement of detections from both fields-of-view. Where we have two or more scans the internal completeness is C I = 0.79 at 3 arcsec or larger from the centres of galaxies, but it drops closer in, especially within 1 arcsec. Conclusions. The per-transit photometry for Gaia transients is precise to 1% at G = 13, and 3% at G = 19. The per-transit astrometry is accurate to 55 mas when compared to Gaia DR2. The Gaia Science Alerts project is one of the most homogeneous and productive transient surveys in operation, and it is the only survey which covers the whole sky at high spatial resolution (subarcsecond), including the Galactic plane and bulge.

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 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 categoriesMeta-epidemiology (narrow)
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Not applicable · Consensus signal: none
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.889
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 studies0.0000.000
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 head0.014
GPT teacher head0.221
Teacher spread0.206 · 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 teacher head, not a consensus.

Study designNot applicable
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

Citations131
Published2021
Admission routes1
Has abstractyes

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