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Record W4292421621 · doi:10.3847/1538-4357/aca5fa

The DESI Survey Validation: Results from Visual Inspection of Bright Galaxies, Luminous Red Galaxies, and Emission-line Galaxies

2023· preprint· en· W4292421621 on OpenAlexaff
Ting-Wen Lan, Rita Tojeiro, E. Armengaud, J. X. Prochaska, T. M. Davis, D. M. Alexander, Anand Raichoor, Rongpu Zhou, Christophe Yèche, C. Balland, S. BenZvi, A. Berti, R. E. A. Canning, Anthony Carr, H. Chittenden, Shaun Cole, M.-C. Cousinou, Kyle Dawson, Biprateep Dey, Kelly A. Douglass, A. C. Edge, S. Escoffier, A. Glanville, Satya Gontcho A Gontcho, J. Guy, ChangHoon Hahn, Cullan Howlett, Ho Seong Hwang, Linhua Jiang, András Kovács, Mar Mezcua, S. Moore, S. Nadathur, Minji Oh, David Parkinson, A. Rocher, Ashley J. Ross, V. Ruhlmann-Kleider, Cristiano G. Sabiu, Khaled Said, Christoph Saulder, D. Sierra-Porta, Benjamin J. Weiner, Jiaxi Yu, Pauline Zarrouk, Yucheng Zhang, Hu Zou, S. P. Ahlen, S. Bailey, D. Brooks, Andrew P. Cooper, Axel de la Macorra, Arjun Dey, G. Dhungana, P. Doel, Sarah Eftekharzadeh, K. Fanning, Andreu Font-Ribera, Lehman H. Garrison, E. Gaztañaga, R. Kehoe, Theodore Kisner, Martin Landriau, L. Le Guillou, M. E. Levi, C. Magneville, Aaron Meisner, R. Miquel, John Moustakas, Adam D. Myers, Jeffrey A. Newman, Jundan Nie, N. Palanque‐Delabrouille, Will J. Percival, Claire Poppett, Francisco Prada, M. Schubnell, G. Tarlé, B. A. Weaver, Kai Zhang, Zhimin Zhou

Bibliographic record

VenuearXiv (Cornell University) · 2023
Typepreprint
Languageen
FieldEngineering
TopicCCD and CMOS Imaging Sensors
Canadian institutionsPerimeter InstituteUniversity of Waterloo
Fundersnot available
KeywordsPhysicsLuminous infrared galaxyAstrophysicsGalaxyGalaxy groupAstronomyElliptical galaxy

Abstract

fetched live from OpenAlex

The Dark Energy Spectroscopic Instrument (DESI) Survey has obtained a set of spectroscopic measurements of galaxies to validate the final survey design and target selections. To assist in these tasks, we visually inspect (VI) DESI spectra of approximately 2,500 bright galaxies, 3,500 luminous red galaxies (LRGs), and 10,000 emission line galaxies (ELGs), to obtain robust redshift identifications. We then utilize the VI redshift information to characterize the performance of the DESI operation. Based on the VI catalogs, our results show that the final survey design yields samples of bright galaxies, LRGs, and ELGs with purity greater than $99\%$. Moreover, we demonstrate that the precision of the redshift measurements is approximately 10 km/s for bright galaxies and ELGs and approximately 40 km/s for LRGs. The average redshift accuracy is within 10 km/s for the three types of galaxies. The VI process also helps improve the quality of the DESI data by identifying spurious spectral features introduced by the pipeline. Finally, we show examples of unexpected real astronomical objects, such as Ly$\alpha$ emitters and strong lensing candidates, identified by VI. These results demonstrate the importance and utility of visually inspecting data from incoming and upcoming surveys, especially during their early operation phases.

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)0.005
metaresearch head score (Gemma)0.009
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 score0.024

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0050.009
Meta-epidemiology (narrow)0.0010.000
Meta-epidemiology (broad)0.0010.001
Bibliometrics0.0040.002
Science and technology studies0.0010.001
Scholarly communication0.0010.001
Open science0.0010.002
Research integrity0.0010.000
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 head0.071
GPT teacher head0.200
Teacher spread0.129 · 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
Published2023
Admission routes1
Has abstractyes

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