MétaCan
Menu
← Back to cohort
Record W2229796775 · doi:10.1051/0004-6361/201527377

SDSS-IV eBOSS emission-line galaxy pilot survey

2016· article· en· W2229796775 on OpenAlexfundno aff
Johan Comparat, Timothée Delubac, S. Jouvel, A. Raichoor, Jean‐Paul Kneib, C. Yèche, F. B. Abdalla, C. Le Cras, Claudia Maraston, D. Wilkinson, Guangtun Zhu, Eric Jullo, Francisco Prada, David J. Schlegel, Z. Xu, Hu Zou, Julian Bautista, Dmitry Bizyaev, A. Bolton, Joel R. Brownstein, Kyle Dawson, S. Escoffier, P. Gaulme, Karen Kinemuchi, Elena Malanushenko, Viktor Malanushenko, V. Mariappan, Jeffrey A. Newman, D. Oravetz, K. Pan, Will J. Percival, A. Prakash, D. P. Schneider, Audrey Simmons, T. M. C. Abbott, S. Allam, M. Banerji, A. Benoit-Lévy, E. Bertin, D. Brooks, D. Capozzi, A. Carnero Rosell, M. Carrasco Kind, J. Carretero, F. J. Castander, C. E. Cunha, L. N. da Costa, S. Desai, P. Doel, T. F. Eifler, J. Estrada, B. Flaugher, P. Fosalba, J. Frieman, E. Gaztañaga, D. W. Gerdes, D. Gruen, R. A. Gruendl, G. Gutiérrez, K. Honscheid, D. J. James, K. Kuehn, N. Kuropatkin, O. Lahav, M. Lima, M. A. G. Maia, M. March, J. L. Marshall, R. Miquel, K. Reil, N. Roe, A. K. Romer, A. Roodman, E. S. Rykoff, M. Šako, E. Sánchez, V. Scarpine, I. Sevilla-Noarbe, M. Soares-Santos, F. Sobreira, E. Suchyta, M. E. C. Swanson, G. Tarlé, J. Thaler, D. Thomas, A. R. Walker, Y. Zhang

Bibliographic record

VenueAstronomy and Astrophysics · 2016
Typearticle
Languageen
FieldPhysics and Astronomy
TopicGalaxies: Formation, Evolution, Phenomena
Canadian institutionsnot available
FundersSLAC National Accelerator LaboratoryArgonne National LaboratoryCentro de Investigaciones Energéticas, Medioambientales y TecnológicasSmithsonian Astrophysical ObservatoryOffice of ScienceUniversity of Colorado BoulderLawrence Berkeley National LaboratoryJet Propulsion LaboratoryUniversity of Illinois at Urbana-ChampaignMax-Planck-Institut für AstrophysikUniversity of SussexInstitut de Física d'Altes EnergiesUniversidad Nacional Autónoma de MéxicoYale UniversityU.S. Department of EnergyFundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de JaneiroConselho Nacional de Desenvolvimento Científico e TecnológicoScience and Technology Facilities CouncilYork UniversityMinistério da Ciência, Tecnologia e InovaçãoMinisterio de Economía y CompetitividadLeibniz-GemeinschaftAgence Nationale de la RechercheDeutsche ForschungsgemeinschaftFermilabMax-Planck-Institut für AstronomieIntegrated Electronics Engineering Center, Binghamton UniversityUniversity of EdinburghUniversity of NottinghamEuropean CommissionCarnegie Institution for ScienceInstituto de Astrofísica de CanariasUniversity of CambridgeCentre National de la Recherche ScientifiqueNational Science FoundationUniversity of MichiganUniversity of Notre DameCarnegie Mellon UniversityUniversity of California, Los AngelesUniversity of WashingtonAlfred P. Sloan FoundationJohns Hopkins UniversityCarnegie Institution of WashingtonUniversity of PortsmouthNew Mexico State UniversityUniversity of UtahVanderbilt UniversityUniversity of ChicagoOhio State UniversitySmithsonian InstitutionCalifornia Institute of TechnologyUniversity College LondonNational Aeronautics and Space AdministrationFinanciadora de Estudos e ProjetosUniversity of Pennsylvania
KeywordsSpectrographSkyRedshiftGalaxyPhysicsBaryonAstrophysicsEmission spectrumAstronomySpectral line

Abstract

fetched live from OpenAlex

The Sloan Digital Sky Survey IV extended Baryonic Oscillation Spectroscopic Survey (SDSS-IV/eBOSS) will observe 195 000 emission-line galaxies (ELGs) to measure the baryonic acoustic oscillation (BAO) standard ruler at redshift 0.9. To test different ELG selection algorithms, 9000 spectra were observed with the SDSS spectrograph as a pilot survey based on data from several imaging surveys. First, using visual inspection and redshift quality flags, we show that the automated spectroscopic redshifts assigned by the pipeline meet the quality requirements for a reliable BAO measurement. We also show the correlations between sky emission, signal-to-noise ratio in the emission lines, and redshift error. Then we provide a detailed description of each target selection algorithm we tested and compare them with the requirements of the eBOSS experiment. As a result, we provide reliable redshift distributions for the different target selection schemes we tested. Finally, we determine an target selection algorithms that is best suited to be applied on DECam photometry because they fulfill the eBOSS survey efficiency requirements.

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)0.001
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 score0.007
Threshold uncertainty score0.014

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0010.001
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0010.001
Science and technology studies0.0000.000
Scholarly communication0.0000.000
Open science0.0000.001
Research integrity0.0000.000
Insufficient payload (model declined to judge)0.0030.001

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 head0.014
GPT teacher head0.219
Teacher spread0.205 · 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

Citations51
Published2016
Admission routes1
Has abstractyes

Explore more

Same venueAstronomy and Astrophysics→Same topicGalaxies: Formation, Evolution, Phenomena→French-language works237,207→