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Record W7117559560 · doi:10.1093/mnras/staf2284

Probing infrared eXcess to investigate early-Universe dust (PIXIEDust)

2025· article· en· W7117559560 on OpenAlexfundno aff
Tom J. L. C. Bakx, Hiddo Algera, Jean-Baptiste Jolly, Clarke J. Esmerian, K. K. Knudsen, Laura Sommovigo, Joris Witstok, Stefano Carniani, Jianhang Chen, Stephen Eales, A. Ferrara, Yoshinobu Fudamoto, Masato Hagimoto, Takuya Hashimoto, Hanae Inami, Akio Inoue, T. Khouri, Ikki Mitsuhashi, Gunnar Nyman, Gustav Olander, S. Serjeant, Renske Smit, Ilsang Yoon, Jorge A. Zavala, S. Aalto, Caitlin M. Casey, Yoichi Tamura, W. H. T. Vlemmings

Bibliographic record

VenueMonthly Notices of the Royal Astronomical Society · 2025
Typearticle
Languageen
FieldPhysics and Astronomy
TopicGalaxies: Formation, Evolution, Phenomena
Canadian institutionsnot available
FundersNational Science Foundation, United Arab EmiratesNational Research FoundationKnut och Alice Wallenbergs StiftelseAlberta Livestock and Meat AgencyJapan Society for the Promotion of ScienceDanmarks GrundforskningsfondMinistry of Education, Culture, Sports, Science and Technology
KeywordsCosmic dustRedshiftSupernovaMillimeterInfraredInterstellar mediumDust laneCircumstellar dust

Abstract

fetched live from OpenAlex

ABSTRACT Despite the implied presence of dust through reddened UV emission in high-redshift galaxies, no dust emission has been detected in the (sub)millimetre regime beyond $z > 8.3$. This study combines around 200 h of Atacama Large Millimetre/submillimetre Array (ALMA) and Northern Extended Millimetre Array (NOEMA) observations on 10 $z > 8$ galaxies, revealing no significant dust emission down to a $1 \sigma$ depth of 2.0, 2.0, and $1.5 \, \mu$Jy at rest-frame 158, 88 $\mu$m, and across all the data, respectively. This constrains average dust masses to be below $< 10^{5}$ M$_{\odot }$ at $3 \sigma$ and dust-to-stellar mass ratios to be below $3.7 \times {} 10^{-4}$ (assuming $T_{\rm dust} = 50$ K and $\beta _{\rm dust} = 2.0$). Binning by redshift ($8 < z < 9.5$ and $9.5 < z < 15$), UV-continuum slope ($\beta _{\rm UV} \lessgtr -2$), and stellar mass ($\log _{10} M_{\ast }/{\rm {M}_{\odot }} \lessgtr 9$) yields similarly stringent constraints. Combined with other studies, these results are consistent with inefficient dust build-up in the $z > 8$ Universe, likely due to inefficient supernova production, limited interstellar grain growth and/or ejection by outflows. We provide data and tools online to facilitate community-wide high-redshift dust searches.

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: Simulation or modeling · Consensus signal: none
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.003
Threshold uncertainty score0.009

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0000.000
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0010.001
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 head0.007
GPT teacher head0.196
Teacher spread0.189 · 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 designSimulation or modeling
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

Citations3
Published2025
Admission routes1
Has abstractyes

Explore more

Same venueMonthly Notices of the Royal Astronomical Society→Same topicGalaxies: Formation, Evolution, Phenomena→French-language works237,207→