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Record W2972724383 · doi:10.1093/mnras/stz2522

The CFHT large area <i>U</i> -band deep survey (CLAUDS)

2019· article· en· W2972724383 on OpenAlexafffundabout
Marcin Sawicki, S. Arnouts, Jiasheng Huang, Jean Coupon, Anneya Golob, Stephen Gwyn, S. Foucaud, T. Moutard, Ikuru Iwata, Chengze Liu, Lingjian Chen, G. Desprez, Yuichi Harikane, Yoshiaki Ono, Michael A. Strauss, Masayuki Tanaka, Nathalie Thibert, Michael L. Balogh, Kevin Bundy, S. C. Chapman, James E. Gunn, Bau-Ching Hsieh, O. Ilbert, Yipeng Jing, O. LeFèvre, Cheng Li, Yuichi Matsuda, Satoshi Miyazaki, Tohru Nagao, Atsushi J. Nishizawa, Masami Ouchi, Kazuhiro Shimasaku, J. D. Silverman, Sylvain de la Torre, L. Tresse, Wei-Hao Wang, Chris J. Willott, Tōru Yamada, Xiaohu Yang, H. K. C. Yee

Bibliographic record

VenueMonthly Notices of the Royal Astronomical Society · 2019
Typearticle
Languageen
FieldPhysics and Astronomy
TopicGalaxies: Formation, Evolution, Phenomena
Canadian institutionsCanadian Institute for Theoretical AstrophysicsDalhousie UniversityUniversity of TorontoUniversity of WaterlooHerzberg Institute of AstrophysicsSaint Mary's University
FundersNatural Sciences and Engineering Research Council of CanadaNational Astronomical Observatory of JapanChinese Academy of SciencesJapan Society for the Promotion of ScienceMinistry of Education, Culture, Sports, Science and TechnologyJapan Science and Technology AgencyNational Research CouncilPrinceton University
KeywordsPhysicsSubaru TelescopeGalaxyPhotometry (optics)RedshiftLarge Synoptic Survey TelescopeAstrophysicsTelescopeAstronomyRemote sensingStarsGeography

Abstract

fetched live from OpenAlex

ABSTRACT The Canada–France–Hawaii Telescope (CFHT) Large Area U-band Deep Survey (CLAUDS) uses data taken with the MegaCam mosaic imager on CFHT to produce images of 18.60 deg$^2$ with median seeing of FWHM = 0.92 arcsec and to a median depth of $U = 27.1$ AB (5$\sigma$ in 2 arcsec apertures), with selected areas that total 1.36 deg$^2$ reaching a median depth of $U=27.7$ AB. These are the deepest U-band images assembled to date over this large an area. These data are located in four fields also imaged to comparably faint levels in $grizy$ and several narrowband filters as part of the Hyper Suprime–Cam (HSC) Subaru Strategic Program (HSC-SSP). These CFHT and Subaru data sets will remain unmatched in their combination of area and depth until the advent of the Large Synoptic Survey Telescope. This paper provides an overview of the scientific motivation for CLAUDS and gives details of the observing strategy, observations, data reduction, and data merging with the HSC-SSP. Three early applications of these deep data are used to illustrate the potential of the data set: deep U-band galaxy number counts, z$\sim$ 3 Lyman break galaxy selection, and photometric redshifts improved by adding CLAUDS U to the Subaru HSC $grizy$ photometry.

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)0.001
metaresearch head score (Gemma)0.001
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 score0.426
Threshold uncertainty score0.848

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0010.001
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0020.002
Science and technology studies0.0010.000
Scholarly communication0.0010.000
Open science0.0010.001
Research integrity0.0000.000
Insufficient payload (model declined to judge)0.0050.001

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 head0.006
GPT teacher head0.189
Teacher spread0.183 · 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

Citations104
Published2019
Admission routes3
Has abstractyes

Explore more

Same venueMonthly Notices of the Royal Astronomical SocietySame topicGalaxies: Formation, Evolution, PhenomenaFrench-language works237,207