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Record W4400518670 · doi:10.48550/arxiv.2407.06336

GD-1 Stellar Stream and Cocoon in the DESI Early Data Release

2024· preprint· en· W4400518670 on OpenAlexfundno aff
Monica Valluri, Parker Fagrelius, S. E. Koposov, Ting S. Li, Oleg Y. Gnedin, Eric F. Bell, R. G. Carlberg, Andrew P. Cooper, Jessia N. Aguilar, Carlos Allende Prieto, Vasily Belokurov, Leandro Beraldo e Silva, D. Brooks, Amanda Byström, T. Claybaugh, Kyle Dawson, Arjun Dey, Peter Doel, J. E. Forero-Romero, E. Gaztañaga, Satya Gontcho A Gontcho, Klaus Honscheid, T. Kisner, Andrew Lambert, Martin Landriau, L. Le Guillou, M. E. Levi, Axel de la Macorra, Mark Manera, Paul Martini, G. E. Medina, Aaron Meisner, R. Miquel, John Moustakas, Adam D. Myer, Joan Najita, Claire Poppett, Francisco Prada, Mehdi Rezaie, Graziano Rossi, Alex H. Riley, E. Sánchez, David J. Schlegel, M. Schubnell, David Sprayberry, G. Tarlé, Guillaume F. Thomas, Benjamin A. Weaver, Risa H. Wechsler, Rongpu Zhou, Hu Zou

Bibliographic record

VenuearXiv (Cornell University) · 2024
Typepreprint
Languageen
FieldPhysics and Astronomy
TopicAstronomy and Astrophysical Research
Canadian institutionsnot available
FundersLawrence Berkeley National LaboratoryHigh Energy PhysicsDivision of Astronomical SciencesScience and Technology Facilities CouncilJet Propulsion LaboratoryOffice of ScienceCommissariat à l'Énergie Atomique et aux Énergies AlternativesMinisterio de Ciencia e InnovaciónChinese Academy of SciencesCalifornia Institute of TechnologyU.S. Department of EnergyGordon and Betty Moore FoundationNuclear Safety and Security CommissionNatural Sciences and Engineering Research Council of CanadaNational Science and Technology CouncilAlfred P. Sloan FoundationNational Science FoundationEuropean Space AgencyNational Aeronautics and Space AdministrationConsejo Nacional de Ciencia y Tecnología
KeywordsEnvironmental scienceComputer scienceAstrophysicsPhysics

Abstract

fetched live from OpenAlex

We present 115 new spectroscopically identified members of the GD-1 tidal stream observed with the 5000-fiber Dark Energy Spectroscopic Instrument (DESI). We confirm the existence of a ``cocoon'' which is a broad (FWHM~2.932 deg ~ 460 pc) and kinematically hot (velocity dispersion, sigma ~ 5-8 km/s) component that surrounds a narrower (FWHM~ 0.353 deg ~ 55) and colder (sigma = 3.09+/-0.76 km/s) thin stream component (based on a median per star velocity precision of 2.7 km/s). The cocoon extends over at least a 30 degree segment of the stream observed by DESI. The thin and cocoon components have similar mean values of [Fe/H]: -2.54+/- 0.04 dex and -2.47+/- 0.06 dex suggestive of a common origin. The data are consistent with the following scenarios for the origin of the cocoon. The progenitor of the GD-1 stream was an accreted globular cluster (GC) and: (a) the cocoon was produced by pre-accretion tidal stripping of the GC while it was still inside its parent dwarf galaxy; (b) the cocoon is debris from the parent dwarf galaxy; (c) an initially thin GC tidal stream was heated by impacts from dark subhalos in the Milky Way; (d) an initially thin GC stream was heated by a massive Sagittarius dwarf galaxy; or a combination of some these. Future DESI spectroscopy and detailed modeling may enable us to distinguish between these possible origins.

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)0.001
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 score0.010
Threshold uncertainty score0.020

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0000.001
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0010.001
Science and technology studies0.0000.000
Scholarly communication0.0010.000
Open science0.0000.001
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 head0.095
GPT teacher head0.227
Teacher spread0.132 · 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

Citations0
Published2024
Admission routes1
Has abstractyes

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