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Record W2040797364 · doi:10.1088/0004-637x/696/2/1164

DISCOVERY OF A GIANT Lyα EMITTER NEAR THE REIONIZATION EPOCH

2009· article· en· W2040797364 on OpenAlexaff
Masami Ouchi, Yoshiaki Ono, Eiichi Egami, Tomoki Saito, Masamune Oguri, Patrick J. McCarthy, D. Farrah, Nobunari Kashikawa, Ivelina Momcheva, Kazuhiro Shimasaku, Kouichiro Nakanishi, Hisanori Furusawa, Masayuki Akiyama, J. S. Dunlop, A. M. J. Mortier, Sadanori Okamura, Masao Hayashi, Michele Cirasuolo, Alan Dressler, Masanori Iye, M. J. Jarvis, Tadayuki Kodama, Crystal L. Martin, R. J. McLure, Kouji Ohta, Tōru Yamada, M. Yoshida

Bibliographic record

VenueThe Astrophysical Journal · 2009
Typearticle
Languageen
FieldPhysics and Astronomy
TopicGalaxies: Formation, Evolution, Phenomena
Canadian institutionsUniversity of British Columbia
FundersJet Propulsion LaboratoryScience and Technology Facilities CouncilNational Astronomical Observatory of JapanNational Aeronautics and Space AdministrationCalifornia Institute of TechnologyW. M. Keck FoundationU.S. Department of Energy
KeywordsPhysicsAstrophysicsReionizationGalaxyAstronomyNebulaStar formationHaloSubaru TelescopeStarsRedshiftSpectral line

Abstract

fetched live from OpenAlex

We report the discovery of a giant Lyα emitter (LAE) with a Spitzer /Infrared Array Camera (IRAC) counterpart near the reionization epoch at z = 6.595. The giant LAE is found from the extensive 1 deg 2 Subaru narrowband survey for z = 6.6 LAEs in the Subaru/ XMM-Newton Deep Survey (SXDS) field, and subsequently identified by deep spectroscopy of Keck/DEIMOS and Magellan/IMACS. Among our 207 LAE candidates, this LAE is not only the brightest narrowband object with L (Lyα) = 3.9 ± 0.2 × 10 43 erg s −1 in our survey volume of 10 6 Mpc 3 , but also a spatially extended Lyα nebula with the largest isophotal area whose major axis is at least ≃3''. This object is more likely to be a large Lyα nebula with a size of ≳17 kpc than to be a strongly lensed galaxy by a foreground object. Our Keck spectrum with medium–high spectral and spatial resolutions suggests that the velocity width is v FWHM = 251 ± 21 km s −1 , and that the line-center velocity changes by ≃60 km s −1 in a 10 kpc range. The stellar mass and star formation rate are estimated to be 0.9–5.0 × 10 10 M ☉ and >34 M ☉ yr −1 , respectively, from the combination of deep optical to infrared images of Subaru, UKIDSS-Ultra Deep Survey, and Spitzer /IRAC. Although the nature of this object is not yet clearly understood, this could be an important object for studying cooling clouds accreting onto a massive halo, or forming-massive galaxies with significant outflows contributing to cosmic reionization and metal enrichment of intergalactic medium.

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)0.000
metaresearch head score (Gemma)0.000
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 score0.001
Threshold uncertainty score0.004

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0000.000
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0010.000
Science and technology studies0.0000.000
Scholarly communication0.0000.000
Open science0.0000.000
Research integrity0.0000.000
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 head0.204
Teacher spread0.198 · 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

Citations155
Published2009
Admission routes1
Has abstractyes

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