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The SCUBA Half-Degree Extragalactic Survey -- I. Survey motivation, design and data processing

2005· article· en· W2127581133 on OpenAlexaff
A. M. J. Mortier, S. Serjeant, J. S. Dunlop, S. E. Scott, P. A. R. Ade, D. M. Alexander, O. Almaini, I. Aretxaga, C. M. Baugh, Andrew Benson, P. N. Best, A. W. Blain, J. Böck, C. Borys, A. Bressan, C. L. Carilli, Edward L. Chapin, S. C. Chapman, D. L. Clements, K. E. K. Coppin, M. Crawford, Michelle Devlin, Simon Dicker, L. Dunne, S. Eales, A. C. Edge, D. Farrah, M. Fox, Carlos S. Frenk, E. Gaztañaga, W. K. Gear, E. Gonzales-Solares, G. L. Granato, T. R. Greve, Jennifer A. Grimes, Joshua O. Gundersen, M. Halpern, Peter Hargrave, David H. Hughes, R. J. Ivison, M. J. Jarvis, Tim Jenness, Raúl Jiménez, E. van Kampen, Alice King, C. G. Lacey, A. Lawrence, Kyle Q. Lepage, Robert G. Mann, G. Marsden, P. Mauskopf, Barth Netterfield, Seb Oliver, L. Olmi, M. J. Page, J. A. Peacock, Chris Pearson, Will J. Percival, Alexandra Pope, R. S. Priddey, Steve Rawlings, N. Roche, M. Rowan-Robinson, D. Scott, K. Sekiguchi, Marc S. Seigar, L. Silva, Chris Simpson, Ian Smail, J. A. Stevens, Toshinobu Takagi, Gregory S. Tucker, C. Vlahakis, I. Waddington, Jeff Wagg, M. Watson, Chris J. Willott, M. Vaccari

Bibliographic record

VenueMonthly Notices of the Royal Astronomical Society · 2005
Typearticle
Languageen
FieldPhysics and Astronomy
TopicGalaxies: Formation, Evolution, Phenomena
Canadian institutionsHerzberg Institute of AstrophysicsUniversity of TorontoUniversity of British Columbia
Fundersnot available
KeywordsPhysicsJames Clerk Maxwell TelescopeAstrophysicsAstronomyActive galactic nucleusTelescopeGalaxyRedshiftPhotometric redshiftSubaru TelescopeHubble Deep FieldChandra Deep Field SouthExtragalactic background lightPopulationBolometerLuminous infrared galaxyStar formationOptics

Abstract

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The Submillimetre Common-User Bolometer Array (SCUBA) Half-Degree Extragalactic Survey (SHADES) is a major new blank-field extragalactic submillimetre (submm) survey currently underway at the James Clerk Maxwell Telescope (JCMT). Ultimately, SHADES aims to cover half a square degree at 450 and 850 μm to a 4σ depth of ≃ 8 mJy at 850 μm. Two fields are being observed, the Subaru/XMM—Newton Deep Field (SXDF) (02h18m−05°) and the Lockman Hole East (10h52m+ 57°). The survey has three main aims: (i) to investigate the population of high-redshift submm galaxies and the cosmic history of massive dust-enshrouded star formation activity; (ii) to investigate the clustering properties of submm-selected galaxies in order to determine whether these objects could be progenitors of present-day massive ellipticals; and (iii) to investigate the fraction of submm-selected sources that harbour active galactic nuclei. To achieve these aims requires that the submm data be combined with co-spatial information spanning the radio-to-X-ray frequency range. Accordingly, SHADES has been designed to benefit from ultra-deep radio imaging obtained with the Very Large Array (VLA), deep mid-infrared observations from the Spitzer Space Telescope, submm mapping by the Balloon-borne Large Aperture Submillimetre Telescope (BLAST), deep near-infrared imaging with the United Kingdom Infrared Telescope, deep optical imaging with the Subaru Telescope and deep X-ray observations with the XMM—Newton observatory. It is expected that the resulting extensive multiwavelength data set will provide complete photometric redshift information accurate to as well as detailed spectral energy distributions for the vast majority of the submm-selected sources. In this paper, the first of a series on SHADES, we present an overview of the motivation for the survey, describe the SHADES survey strategy, provide a detailed description of the primary data-analysis pipeline and demonstrate the superiority of our adopted matched-filter source-extraction technique over, for example, Emerson-II style methods. We also report on the progress of the survey. As of 2004 February, 720 arcmin2 had been mapped with SCUBA (about 40 per cent of the anticipated final total area) to a median 1σ depth of 2.2 mJy per beam at 850 μm (25 mJy per beam at 450 μm), and the source-extraction routines give a source density of 650 ± 50 sources deg−2 > 3σ at 850 μm. Although uncorrected for Eddington bias, this source density is more than sufficient for providing enough sources to answer the science goals of SHADES, once half a square degree is observed. A refined reanalysis of the original 8-mJy survey Lockman hole data was carried out in order to evaluate the new data-reduction pipeline. Of the 17 most secure sources in the original sample, 12 have been reconfirmed, including 10 of the 11 for which radio identifications were previously secured.

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: Not applicable · Consensus signal: none
GenreCandidate signal: Methods · Consensus signal: none
Teacher disagreement score0.034
Threshold uncertainty score0.067

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0010.001
Meta-epidemiology (narrow)0.0010.000
Meta-epidemiology (broad)0.0000.001
Bibliometrics0.0030.004
Science and technology studies0.0010.001
Scholarly communication0.0020.001
Open science0.0020.002
Research integrity0.0010.001
Insufficient payload (model declined to judge)0.0070.007

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 head0.040
GPT teacher head0.242
Teacher spread0.202 · 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 designNot applicable
Domainnot available
GenreMethods

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".

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Citations89
Published2005
Admission routes1
Has abstractyes

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