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Record W4292421616 · doi:10.3847/1538-3881/aca5f9

The Target-selection Pipeline for the Dark Energy Spectroscopic Instrument

2023· article· en· W4292421616 on OpenAlexaff
Adam D. Myers, John Moustakas, S. Bailey, Benjamin A. Weaver, Andrew P. Cooper, J. E. Forero-Romero, Bela Abolfathi, D. M. Alexander, D. Brooks, E. Chaussidon, Chia-Hsun Chuang, Kyle Dawson, Arjun Dey, Biprateep Dey, G. Dhungana, Peter Doel, Kevin Fanning, E. Gaztañaga, Satya Gontcho A Gontcho, Alma X. González‐Morales, ChangHoon Hahn, H. K. Herrera-Alcantar, K. Honscheid, Mustapha Ishak, Tanveer Karim, D. Kirkby, Theodore Kisner, S. E. Koposov, Ting-Wen Lan, Martin Landriau, Dustin Lang, M. E. Levi, C. Magneville, L. Napolitano, Paul Martini, Aaron Meisner, Jeffrey A. Newman, N. Palanque‐Delabrouille, Will J. Percival, Claire Poppett, Francisco Prada, Anand Raichoor, Ashley J. Ross, Edward F. Schlafly, David J. Schlegel, M. Schubnell, T. Tan, G. Tarlé, Michael Wilson, Christophe Yèche, Rongpu Zhou, Zhimin Zhou, Hu Zou

Bibliographic record

VenueThe Astronomical Journal · 2023
Typearticle
Languageen
FieldPhysics and Astronomy
TopicAstronomy and Astrophysical Research
Canadian institutionsUniversity of WaterlooPerimeter Institute
FundersLawrence Berkeley National LaboratoryHigh Energy PhysicsDivision of Astronomical SciencesScience and Technology Facilities CouncilOffice of ScienceMinisterio de Ciencia e InnovaciónJet Propulsion LaboratoryMinistry of Science and Technology, TaiwanCommissariat à l'Énergie Atomique et aux Énergies AlternativesChinese Academy of SciencesNational Science FoundationEuropean Space AgencyNational Aeronautics and Space AdministrationU.S. Department of EnergyCalifornia Institute of TechnologyGordon and Betty Moore FoundationConsejo Nacional de Ciencia y Tecnología
KeywordsPhysicsDark energyGalaxyAstronomyQSOSMilky WayAstrophysicsPipeline (software)SkyQuasarCosmologyComputer science

Abstract

fetched live from OpenAlex

Abstract In 2021 May, the Dark Energy Spectroscopic Instrument (DESI) began a 5 yr survey of approximately 50 million total extragalactic and Galactic targets. The primary DESI dark-time targets are emission line galaxies, luminous red galaxies, and quasars. In bright time, DESI will focus on two surveys known as the Bright Galaxy Survey and the Milky Way Survey. DESI also observes a selection of “secondary” targets for bespoke science goals. This paper gives an overview of the publicly available pipeline ( desitarget ) used to process targets for DESI observations. Highlights include details of the different DESI survey targeting phases, the targeting ID ( TARGETID ) used to define unique targets, the bitmasks used to indicate a particular type of target, the data model and structure of DESI targeting files, and examples of how to access and use the desitarget code base. This paper will also describe “supporting” DESI target classes, such as standard stars, sky locations, and random catalogs that mimic the angular selection function of DESI targets. The DESI target-selection pipeline is complex and sizable; this paper attempts to summarize the most salient information required to understand and work with DESI targeting data.

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 distilled prediction

Teacher imitation

Not calibrated prevalence, not ground truth. Human validation pending. Learned from the 10,348 direct Codex labels and 10,348 direct Gemma labels. Candidate is the union of thresholded teacher heads; consensus is their intersection. These outputs are machine_predicted_unvalidated and are not human labels or direct frontier model labels.

metaresearch head score (Codex)0.001
metaresearch head score (Gemma)0.000
Version: codex-gemma-dda1882f352aValidation status: machine_predicted_unvalidated
Candidate categoriesScience and technology studies
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Other design · Consensus signal: none
GenreCandidate signal: Empirical · Consensus signal: none
Teacher disagreement score0.879
Threshold uncertainty score0.999

Codex and Gemma teacher scores by category

CategoryCodexGemma
Metaresearch0.0010.000
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0000.000
Science and technology studies0.0020.000
Scholarly communication0.0000.000
Open science0.0010.000
Research integrity0.0000.001
Insufficient payload (model declined to judge)0.0000.000

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 head0.014
GPT teacher head0.275
Teacher spread0.261 · 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 teacher head, not a consensus.

Study designOther design
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

Citations134
Published2023
Admission routes1
Has abstractyes

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