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Record W2949380767 · doi:10.3847/1538-3881/aa784d

The Apache Point Observatory Galactic Evolution Experiment (APOGEE)

2017· article· en· W2949380767 on OpenAlexaff
Steven R. Majewski, Ricardo P. Schiavon, Peter M. Frinchaboy, Carlos Allende Prieto, Robert H. Barkhouser, Dmitry Bizyaev, Basil Blank, Sophia Brunner, Adam Burton, R. Carrera, Kátia Cunha, Courtney R. Epstein, Greg Fitzgerald, A. E. García Pérez, Fred Hearty, Jon A. Holtzman, Jennifer A. Johnson, Charles R. Lam, J. E. Lawler, Paul Maseman, Szabolcs Mészáros, Matthew Nelson, Duy Coung Nguyen, David L. Nidever, Marc H. Pinsonneault, Matthew Shetrone, Stephen A. Smee, Verne V. Smith, Todd M. Stolberg, Michael F. Skrutskie, E. Walker, John C. Wilson, Gail Zasowski, F. Anders, Sarbani Basu, S. Béland, Michael R. Blanton, Jo Bovy, Joel R. Brownstein, Joleen K. Carlberg, W. J. Chaplin, C. Chiappini, Daniel J. Eisenstein, Y. Elsworth, Diane Feuillet, Scott W. Fleming, Jessica Galbraith-Frew, R. A. García, D. A. García–Hernández, Bruce Gillespie, L. Girardi, James E. Gunn, Sten Hasselquist, Michael Hayden, S. Hekker, Inese I. Ivans, Karen Kinemuchi, Mark A. Klaene, Suvrath Mahadevan, S. Mathur, B. Mosser, Demitri Muna, Jeffrey A. Munn, Robert C. Nichol, R. W. O’Connell, John K. Parejko, A. C. Robin, H. J. Rocha–Pinto, M. Schultheis, Aldo Serenelli, N. Shane, V. Silva Aguirre, Jennifer Sobeck, Benjamin Thompson, T. Nicholas, David H. Weinberg, O. Zamora

Bibliographic record

VenueThe Astronomical Journal · 2017
Typearticle
Languageen
FieldPhysics and Astronomy
TopicStellar, planetary, and galactic studies
Canadian institutionsCanadian Institute for Theoretical AstrophysicsUniversity of Toronto
FundersScience and Technology Facilities Council
KeywordsPhysicsObservatoryAstronomyAstrophysicsPoint (geometry)Geometry

Abstract

fetched live from OpenAlex

Abstract The Apache Point Observatory Galactic Evolution Experiment (APOGEE), one of the programs in the Sloan Digital Sky Survey III (SDSS-III), has now completed its systematic, homogeneous spectroscopic survey sampling all major populations of the Milky Way. After a three-year observing campaign on the Sloan 2.5 m Telescope, APOGEE has collected a half million high-resolution ( R ∼ 22,500), high signal-to-noise ratio (>100), infrared (1.51–1.70 μ m) spectra for 146,000 stars, with time series information via repeat visits to most of these stars. This paper describes the motivations for the survey and its overall design—hardware, field placement, target selection, operations—and gives an overview of these aspects as well as the data reduction, analysis, and products. An index is also given to the complement of technical papers that describe various critical survey components in detail. Finally, we discuss the achieved survey performance and illustrate the variety of potential uses of the data products by way of a number of science demonstrations, which span from time series analysis of stellar spectral variations and radial velocity variations from stellar companions, to spatial maps of kinematics, metallicity, and abundance patterns across the Galaxy and as a function of age, to new views of the interstellar medium, the chemistry of star clusters, and the discovery of rare stellar species. As part of SDSS-III Data Release 12 and later releases, all of the APOGEE data products are publicly available.

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)0.003
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: none
GenreCandidate signal: Empirical · Consensus signal: none
Teacher disagreement score0.029
Threshold uncertainty score0.058

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0030.002
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0010.002
Science and technology studies0.0010.000
Scholarly communication0.0010.001
Open science0.0010.002
Research integrity0.0000.001
Insufficient payload (model declined to judge)0.0070.004

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 head0.023
GPT teacher head0.254
Teacher spread0.231 · 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

Citations1,743
Published2017
Admission routes1
Has abstractyes

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