MétaCan
Menu
Back to cohort
Record W1970196846 · doi:10.1088/0004-637x/709/2/644

GALAXY STELLAR MASS ASSEMBLY BETWEEN 0.2 &lt;<i>z</i>&lt; 2 FROM THE S-COSMOS SURVEY

2010· article· en· W1970196846 on OpenAlexaff
O. Ilbert, M. Salvato, E. Le Floc’h, P. Capak, H. J. McCracken, Bahram Mobasher, Jeyhan S. Kartaltepe, N. Z. Scoville, D. B. Sanders, S. Arnouts, K. Bundy, P. Cassata, Jean‐Paul Kneib, Anton M. Koekemoer, O. Le Fèvre, S. J. Lilly, J. Surace, Yoshiaki Taniguchi, L. Tasca, D. J. Thompson, L. Tresse, Michel Zamojski, G. Zamorani, E. Zucca

Bibliographic record

VenueThe Astrophysical Journal · 2010
Typearticle
Languageen
FieldPhysics and Astronomy
TopicGalaxies: Formation, Evolution, Phenomena
Canadian institutionsUniversity of Toronto
Fundersnot available
KeywordsPhysicsAstrophysicsStellar massElliptical galaxyAstronomyLuminous infrared galaxyGalaxyStar formationGalaxy formation and evolution

Abstract

fetched live from OpenAlex

We follow the galaxy stellar mass assembly by morphological and spectral type in the COSMOS 2 deg 2 field. We derive the stellar mass functions and stellar mass densities from z = 2 to z = 0.2 using 196,000 galaxies selected at F 3.6 μm > 1 μJy with accurate photometric redshifts ( at i + < 22.5). Using a spectral classification, we find that z ∼ 1 is an epoch of transition in the stellar mass assembly of quiescent galaxies. Their stellar mass density increases by 1.1 dex between z = 1.5–2 and z = 0.8–1 (Δ t ∼ 2.5 Gyr), but only by 0.3 dex between z = 0.8–1 and z ∼ 0.1 (Δ t ∼ 6 Gyr). Then, we add the morphological information and find that 80%–90% of the massive quiescent galaxies have an elliptical morphology at z < 0.8. Therefore, a dominant mechanism links the shutdown of star formation and the acquisition of an elliptical morphology in massive galaxies. Still, a significant fraction of quiescent galaxies present a Spi/Irr morphology at low mass (40%–60% at ), but this fraction is smaller than predicted by semi-analytical models using a "halo quenching" recipe. We also analyze the evolution of star-forming galaxies and split them into "intermediate activity" and "high activity" galaxies. We find that the most massive "high activity" galaxies end their high star formation rate phase first. Finally, the space density of massive star-forming galaxies becomes lower than the space density of massive elliptical galaxies at z < 1. As a consequence, the rate of "wet mergers" involved in the formation of the most massive ellipticals must decline very rapidly at z < 1, which could explain the observed slow down in the assembly of these quiescent and massive sources.

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 score0.009
Threshold uncertainty score0.019

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0000.000
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0020.001
Science and technology studies0.0000.000
Scholarly communication0.0000.000
Open science0.0000.000
Research integrity0.0000.000
Insufficient payload (model declined to judge)0.0030.001

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 head0.012
GPT teacher head0.222
Teacher spread0.210 · 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

Citations697
Published2010
Admission routes1
Has abstractyes

Explore more

Same venueThe Astrophysical JournalSame topicGalaxies: Formation, Evolution, PhenomenaFrench-language works237,207