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Record W2134988917 · doi:10.1088/0004-637x/780/1/75

HerMES: CANDIDATE HIGH-REDSHIFT GALAXIES DISCOVERED WITH<i>HERSCHEL</i>/SPIRE,

2013· article· en· W2134988917 on OpenAlexaff
C. D. Dowell, A. Conley, J. Glenn, V. Arumugam, V. Asboth, F. Bertoldi, M. Béthermin, J. Böck, A. Boselli, Carrie Bridge, V. Buat, D. Burgarella, A. Cabrera‐Lavers, Caitlin M. Casey, S. C. Chapman, D. L. Clements, L. Conversi, Asantha Cooray, H. Dannerbauer, Francesco De Bernardis, T. P. Ellsworth-Bowers, D. Farrah, A. Franceschini, M. Griffin, Mark Gurwell, M. Halpern, E. Hatziminaoglou, S. Heinis, E. Ibar, R. J. Ivison, Nicolas Laporte, L. Marchetti, P. Martínez-Navajas, G. Marsden, G. Morrison, H. T. Nguyen, B. O’Halloran, Seb Oliver, A. Omont, M. J. Page, Ανδρέας Παπαγεωργίου, C. P. Pearson, G. Petitpas, I. Pérez‐Fournon, M. Pohlen, Dominik A. Riechers, D. Rigopoulou, I. G. Roseboom, M. Rowan-Robinson, J. Sayers, B. Schulz, D. Scott, N. Seymour, D. L. Shupe, A. J. Smith, A. Streblyanska, M. Symeonidis, M. Vaccari, I. Valtchanov, J. D. Vieira, M. Viero, L. Wang, J. L. Wardlow, C. K. Xu, M. Zemcov

Bibliographic record

VenueThe Astrophysical Journal · 2013
Typearticle
Languageen
FieldPhysics and Astronomy
TopicGalaxies: Formation, Evolution, Phenomena
Canadian institutionsDalhousie UniversityUniversity of British Columbia
FundersScience and Technology Facilities CouncilNational Aeronautics and Space Administration
KeywordsPhysicsAstrophysicsGalaxySpire (mollusc)RedshiftLuminosity functionLuminosityStar formationPopulationLuminous infrared galaxyFlux (metallurgy)Astronomy

Abstract

fetched live from OpenAlex

We present a method for selecting $z&gt;4$ dusty, star forming galaxies (DSFGs) using Herschel/SPIRE 250/350/500 $μm$ flux densities to search for red sources. We apply this method to 21 deg$^2$ of data from the HerMES survey to produce a catalog of 38 high-$z$ candidates. Follow-up of the first 5 of these sources confirms that this method is efficient at selecting high-$z$ DSFGs, with 4/5 at $z=4.3$ to $6.3$ (and the remaining source at $z=3.4$), and that they are some of the most luminous dusty sources known. Comparison with previous DSFG samples, mostly selected at longer wavelengths (e.g., 850 $μm$) and in single-band surveys, shows that our method is much more efficient at selecting high-$z$ DSFGs, in the sense that a much larger fraction are at $z&gt;3$. Correcting for the selection completeness and purity, we find that the number of bright ($S_{500\,μm} \ge 30$ mJy), red Herschel sources is $3.3 \pm 0.8$ deg$^{-2}$. This is much higher than the number predicted by current models, suggesting that the DSFG population extends to higher redshifts than previously believed. If the shape of the luminosity function for high-$z$ DSFGs is similar to that at $z\sim2$, rest-frame UV based studies may be missing a significant component of the star formation density at $z=4$ to $6$, even after correction for extinction.

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 categoriesInsufficient payload (model declined to judge)
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Observational · Consensus signal: Observational
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.010
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 studies0.0010.000
Scholarly communication0.0000.001
Open science0.0010.000
Research integrity0.0000.001
Insufficient payload (model declined to judge)0.0010.001

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 head0.005
GPT teacher head0.191
Teacher spread0.186 · 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 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

Citations121
Published2013
Admission routes1
Has abstractyes

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