MétaCan
Menu
Back to cohort
Record W4400185560 · doi:10.1051/0004-6361/202450584

The VISTA Variables in the Vía Láctea extended (VVVX) ESO public survey: Completion of the observations and legacy

2024· article· en· W4400185560 on OpenAlexaff
R. K. Saito, M. Hempel, J. Alonso-García, P. W. Lucas, D. Minniti, S. Alonso, Laura D Baravalle, J. Borissova, C. Cáceres, André-Nicolas Chené, N. J. G. Cross, Fernanda Duplancic, E. R. Garro, M. Gómez, V. D. Ivanov, R. Kurtev, A. Luna, D. Majaess, M. G. Navarro, Joyce Pullen, M. Rejkuba, Jason L. Sanders, Leigh C. Smith, Pereira Albino, M. V. Alonso, E. B. Amôres, R. Angeloni, J. I. Arias, M. Arnaboldi, B. Barbuy, A. Bayo, J. C. Beamín, L. R. Bedin, Andrea Bellini, Robert A. Benjamin, E. Bica, C. Bonatto, E. Botan, V. F. Braga, D. A. Brown, Juan Cabral, D. Camargo, A. Caratti o Garatti, J. A. Carballo-Bello, M. Catelan, C. Chavero, M. Chijani, Joan Clària, Georgina Coldwell, Carlos Contreras Peña, R. Contreras Ramos, J. M. Corral-Santana, C. Cortés, M. Cortés‐Contreras, P. Cruz, I. V. Daza-Perilla, Victor P. Debattista, B. Dias, L. Donoso, Richard D’Souza, J. P. Emerson, S. Federle, V. Fermiano, J. Fernández, José G. Fernández-Trincado, María Teresa Ferreira, C. E. Ferreira Lopes, V. Firpo, Catalina Flores, L. Fraga, D. Froebrich, Daniela Galdeano, I. Gavignaud, D. Geisler, Ortwin Gerhard, W. Gieren, O. A. González, L. V. Gramajo, F. Gran, Pablo M. Granitto, M. Griggio, Zhen Guo, S. Gurovich, M. Hilker, H. R. A. Jones, R. Kammers, Michael A. Kuhn, M. Sunil Kumar, Richa Kundu, M. Lares, Mattia Libralato, E. F. Lima, T. J. Maccarone, P. Marchant Cortés, E. L. Martı́n, N. Masetti, N. Matsunaga, F. Mauro, Iain McDonald, Andrea Mejías, Valeria Mesa, F. P. Milla-Castro, J. H. Minniti, C. Moni Bidin, K. Montenegro, C. S. Morris, V. Motta, F. Navarete, C. Navarro, F. Nikzat, J. L. Nilo Castellón, C. Obasi, Mario Ortigoza-Urdaneta, T. Palma, M. C. Parisi, Karla Peña Ramírez, Luis Pereyra, Noelia Pérez, Ilaria Petralia, A. Pichel, G. Pignata, S. Ramírez Alegría, A. F. Rojas, D. Rojas, Alexandre Roman–Lopes, A. C. Rovero, S. Saroon, E. O. Schmidt, A. C. Schröder, M. Schultheis, M. A. Sgró, E. Solano, M. Soto, B. Stecklum, D. Steeghs, Motohide Tamura, P. B. Tissera, A. A. R. Valcarce, C. Valotto, S. Vásquez, C. Villalón, S. Villanova, F. Vivanco Cádiz, R. Zelada Bacigalupo, A. A. Zijlstra, M. Zoccali

Bibliographic record

VenueAstronomy and Astrophysics · 2024
Typearticle
Languageen
FieldPhysics and Astronomy
TopicAstronomy and Astrophysical Research
Canadian institutionsMount Saint Vincent University
FundersScience and Technology Facilities CouncilAgence Nationale de la Recherche
KeywordsPhysicsAstrophysicsAstronomy

Abstract

fetched live from OpenAlex

Context. The ESO public survey VISTA Variables in the Vía Láctea (VVV) surveyed the inner Galactic bulge and the adjacent southern Galactic disk from 2009–2015. Upon its conclusion, the complementary VVV extended (VVVX) survey has expanded both the temporal as well as spatial coverage of the original VVV area, widening it from 562 to 1700 sq. deg., as well as providing additional epochs in JHK s filters from 2016–2023. Aims. With the completion of VVVX observations during the first semester of 2023, we present here the observing strategy, a description of data quality and access, and the legacy of VVVX. Methods. VVVX took ~2000 h, covering about 4% of the sky in the bulge and southern disk. VVVX covered most of the gaps left between the VVV and the VISTA Hemisphere Survey (VHS) areas and extended the VVV time baseline in the obscured regions affected by high extinction and hence hidden from optical observations. Results. VVVX provides a deep JHK s catalogue of ≳1.5 × 10 9 point sources, as well as a K s band catalogue of ~10 7 variable sources. Within the existing VVV area, we produced a 5 D map of the surveyed region by combining positions, distances, and proper motions of well-understood distance indicators such as red clump stars, RR Lyrae, and Cepheid variables. Conclusions. In March 2023 we successfully finished the VVVX survey observations that started in 2016, an accomplishment for ESO Paranal Observatory upon 4200 h of observations for VVV+VVVX. The VVV+VVVX catalogues complement those from the Gaia mission at low Galactic latitudes and provide spectroscopic targets for the forthcoming ESO high-multiplex spectrographs MOONS and 4MOST.

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)0.001
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: Observational · Consensus signal: none
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.835
Threshold uncertainty score0.698

Codex and Gemma teacher scores by category

CategoryCodexGemma
Metaresearch0.0010.000
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0000.001
Science and technology studies0.0010.001
Scholarly communication0.0010.001
Open science0.0010.000
Research integrity0.0000.001
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 head0.033
GPT teacher head0.268
Teacher spread0.235 · 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.

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

Citations34
Published2024
Admission routes1
Has abstractyes

Explore more

Same venueAstronomy and AstrophysicsSame topicAstronomy and Astrophysical ResearchFrench-language works237,207