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Record W2121023735 · doi:10.48550/arxiv.1102.1316

The GALEX Ultraviolet Virgo Cluster Survey (GUViCS). I: The UV luminosity function of the central 12 sq.deg

2011· preprint· en· W2121023735 on OpenAlexaffvenue
A. Boselli, S. Boissier, S. Heinis, L. Cortese, O. Ilbert, T. M. Hughes, O. Cucciati, Jonathan S. Davies, Laura Ferrarese, Riccardo Giovanelli, Martha P. Haynes, M. Baes, N. Brosch, S. C. Chapman, V. Charmandaris, Ilse De Looze, S. di Serego Alighieri, Pierre–Alain Duc, Patrick R. Durrell, Éric Emsellem, J. Fritz, M. Grossi, Andrés Jordán, Kelley M. Hess, L. K. Hunt, Brian R. Kent, D. G. Lambas, A. Lançon, Lauren A. MacArthur, S. C. Madden, L. Magrini, S. Mei, Emmanuel Momjian, R. P. Olowin, Emmanouil Papastergis, M. W. L. Smith, J. M. Solanes, O. Spector, Kristine Spekkens, James E. Taylor, C. Valotto, W. van Driel, J. Verstappen, C. Vlahakis, B. Vollmer, E. M. Xilouris

Bibliographic record

VenueNPARC · 2011
Typepreprint
Languageen
FieldPhysics and Astronomy
TopicGalaxies: Formation, Evolution, Phenomena
Canadian institutionsRoyal Military College of CanadaHerzberg Institute of Astrophysics
FundersLos Alamos National LaboratoryU.S. Naval ObservatoryFermilabMax-Planck-Institut für AstronomieMax-Planck-GesellschaftChinese Academy of SciencesNew Mexico State UniversityUniversity of PortsmouthUniversität BaselUniversity of PittsburghJohns Hopkins UniversityOhio State UniversityCalifornia Institute of TechnologyU.S. Department of EnergyJet Propulsion LaboratoryPrinceton UniversityNational Science FoundationUniversity of WashingtonDrexel UniversityAlfred P. Sloan FoundationNational Aeronautics and Space AdministrationCase Western Reserve University
KeywordsPhysicsAstrophysicsGalaxyVirgo ClusterExtinction (optical mineralogy)AstronomySkyLuminosityUltravioletContext (archaeology)Galaxy clusterOpticsGeography

Abstract

fetched live from OpenAlex

The GALEX Ultraviolet Virgo Cluster Survey (GUViCS) is a complete blind survey of the Virgo cluster covering about 40 sq. deg. in the far UV (FUV, lambda_eff=1539A, Delta-lambda=442A) and about 120 sq. deg. in the near UV (NUV, lambda_eff=2316A, Delta-lambda=1060A). The goal of the survey is to study the ultraviolet (UV) properties of galaxies in a rich cluster environment, spanning a wide luminosity range from giants to dwarfs, and regardless of prior knowledge of their star formation activity. The UV data will be combined with those in other bands (optical: NGVS; far-infrared - submm: HeViCS; HI: ALFALFA) and with our multizone chemo-spectrophotometric models of galaxy evolution to make a complete and exhaustive study of the effects of the environment on the evolution of galaxies in high density regions. We present here the scientific objectives of the survey, describing the observing strategy and briefly discussing different data reduction techniques. Using UV data already in-hand for the central 12 sq. deg. we determine the FUV and NUV luminosity functions of the Virgo cluster core for all cluster members and separately for early- and late-type galaxies and compare it to the one obtained in the field and other nearby clusters (Coma, A1367). This analysis shows that the FUV and NUV luminosity functions of the core of the Virgo clusters are flatter (alpha about -1.1) than those determined in Coma and A1367. We discuss the possible origin of this difference

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: Observational
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.013
Threshold uncertainty score0.809

Codex and Gemma teacher scores by category

CategoryCodexGemma
Metaresearch0.0010.000
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0000.000
Science and technology studies0.0010.000
Scholarly communication0.0000.000
Open science0.0010.001
Research integrity0.0000.001
Insufficient payload (model declined to judge)0.0010.000

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 head0.016
GPT teacher head0.207
Teacher spread0.190 · 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

Citations11
Published2011
Admission routes2
Has abstractyes

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