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Record W4366328384 · doi:10.1093/mnras/stad2618

First detection of the BAO signal from early DESI data

2023· article· en· W4366328384 on OpenAlexaff
Jeongin Moon, D. Valcin, M. Rashkovetskyi, Christoph Saulder, J. Aguilar, S. P. Ahlen, Shadab Alam, S. Bailey, C. Baltay, Robert Blum, D. Brooks, E. Burtin, E. Chaussidon, Kyle Dawson, Axel de la Macorra, Arnaud de M attia, G. Dhungana, Daniel J. Eisenstein, B. Flaugher, Andreu Font-Ribera, J. E. Forero-Romero, C. García-Quintero, Satya Gontcho A Gontcho, Julien Guy, M. Hanif, Klaus Honscheid, Mustapha Ishak, R. Kehoe, Sumi Kim, Theodore Kisner, Anthony Kremin, Martin Landriau, L. Le Guillou, Michael Levi, Marc Manera, Paul Martini, Patrick McDonald, Aaron Meisner, Ramon Miquel, John Moustakas, Adam Myers, S. Nadathur, Richard Neveux, Jeffrey A. Newman, Jundan Nie, Nikhil Padmanabhan, N. Palanque‐Delabrouille, Will J. Percival, Alejandro Pérez Fernández, Claire Poppett, Francisco Prada, Anand Raichoor, Ashley J Ross, Graziano Rossi, Lado Samushia, David J. Schlegel, Hee‐Jong Seo, G. Tarlé, M. Vargas-Magaña, Andrei Variu, Benjamin Alan Weaver, Martin White, Christophe Yèche, Sihan Yuan, Cheng Zhao, Rongpu Zhou, Zhimin Zhou, Hu Zou

Bibliographic record

VenueMonthly Notices of the Royal Astronomical Society · 2023
Typearticle
Languageen
FieldPhysics and Astronomy
TopicGalaxies: Formation, Evolution, Phenomena
Canadian institutionsPerimeter InstituteUniversity of Waterloo
FundersHigh Energy PhysicsDivision of Astronomical SciencesOffice of ScienceCommissariat à l'Énergie Atomique et aux Énergies AlternativesMinisterio de Ciencia e InnovaciónScience and Technology Facilities CouncilSejong UniversityNational Research FoundationNational Research Foundation of KoreaU.S. Department of EnergyGordon and Betty Moore FoundationSimons FoundationMinistry of Education, Science and TechnologyKorea Astronomy and Space Science InstituteConsejo Nacional de Ciencia y TecnologíaNational Science Foundation
KeywordsPhysicsBaryon acoustic oscillationsSpectrographDark energyGalaxyRedshiftAstrophysicsCosmologyAstronomySpectral line

Abstract

fetched live from OpenAlex

ABSTRACT We present the first detection of the baryon acoustic oscillations (BAOs) signal obtained using unblinded data collected during the initial 2 months of operations of the Stage-IV ground-based Dark Energy Spectroscopic Instrument (DESI). From a selected sample of 261 291 luminous red galaxies spanning the redshift interval 0.4 < z < 1.1 and covering 1651 square degrees with a 57.9 per cent completeness level, we report a ∼5σ level BAO detection and the measurement of the BAO location at a precision of 1.7 per cent. Using a bright galaxy sample of 109 523 galaxies in the redshift range 0.1 < z < 0.5, over 3677 square degrees with a 50.0 per cent completeness, we also detect the BAO feature at ∼3σ significance with a 2.6 per cent precision. These first BAO measurements represent an important milestone, acting as a quality control on the optimal performance of the complex robotically actuated, fibre-fed DESI spectrograph, as well as an early validation of the DESI spectroscopic pipeline and data management system. Based on these first promising results, we forecast that DESI is on target to achieve a high-significance BAO detection at sub-per cent precision with the completed 5-yr survey data, meeting the top-level science requirements on BAO measurements. This exquisite level of precision will set new standards in cosmology and confirm DESI as the most competitive BAO experiment for the remainder of this decade.

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)0.001
metaresearch head score (Gemma)0.002
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 score0.003
Threshold uncertainty score0.006

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0010.002
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 integrity0.0000.001
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 head0.013
GPT teacher head0.197
Teacher spread0.185 · 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

Citations39
Published2023
Admission routes1
Has abstractyes

Explore more

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