MétaCan
ENFR
Menu
Cohort builder

4,299,418 works, Canadian by any of four routes.

Every filter state is a URL; the URL is the query; the query is citable via /q/⟨hash⟩. The page, the API and the export parse the same parameters.

Export CSVExport JSONAPI query

The current cohort, streamed from the database: every work column, the machine labels, the provisional scores, and the per-row validation status. Exports are capped at 100,000 rows. Mints a permanent /q/ link for this exact query. The same filters always produce the same link, whoever asks.

Search term
Author
Year range
→
Sort
Language
Type
Field
Venue
Topic
Stellar, planetary, and galactic studies
Retraction
Abstract
Evidence source
Study design
Label agreement
Label status

Direct Codex and Gemma labels are unvalidated and sparse. Distilled predictions cover the full frame and are also unvalidated. Choose the evidence source explicitly; absence of a direct label is never a negative label.

affaffiliation
fundfunder
venuejournal
aboutaboutness

The four routes compose: require the funder route and exclude affiliation to get the funder-only stratum no affiliation-based frame ever sees.

6,765 results · 1 filter active ·
Results by year
20002025
Publication date
Categories
Machine labels · sparse coverage
Evidence
Language
Type
Citations
An unlabeled work is unknown, not a negative. Label coverage is reported on every query.
6,765 works in the cohort · of 4,299,418page 125 of 136

Labels cover 2 of 6,765 works in this cohort. The rest are unlabeled, which is not a negative label: the label table is sparse today and grows as labeling rounds land.

Distilled predictions cover 6,765 of 6,765 works in this cohort. Predictions are machine_predicted_unvalidated. The Gemma side is a direct model label for every work (title-only); the Codex side is a distilled, calibrated classifier. Candidate is the union; consensus is the intersection.

affno abstractunlabeled
Spatially Resolved Spectroscopy of Proto-Planetary Nebulae
Miwa Goto, W. Gässler, Yutaka Hayano, Masanori Iye, Yukiko Kamata, Tomio Kanzawa +6 more
2005· book-chapter· en· ESO astrophysics symposia· Physics and Astronomy
machine prediction:candidate · noneconsensus · none
0
citations
affunlabeled
Dust Features in Carbon-rich Planetary Nebulae
Albertina Pei, Kevin Volk
2003· article· en· Symposium - International Astronomical Union· Physics and Astronomy
machine prediction:candidate · noneconsensus · none
0
citations
fundno affunlabeled
NGTS-28Ab: A short period transiting brown dwarf
Beth A Henderson, S. L. Casewell, M. R. Goad, Jack S Acton, Maximilian N. Günther, Louise D. Nielsen +40 more
2024· preprint· en· arXiv (Cornell University)· Physics and Astronomy
machine prediction:candidate · noneconsensus · none
0
citations
affunlabeled
How do red giants respond to mass loss?
K. Pavlovskii, Natalia Ivanova
2012· article· en· Proceedings of the International Astronomical Union· Physics and Astronomy
machine prediction:candidate · noneconsensus · none
0
citations
aboutno affunlabeled
and
2013· article· en· Physics and Astronomy
machine prediction:candidate · insufficient_payloadconsensus · none
0
citations
affunlabeled
Dayside Land on Tidally-Locked Rocky Planets
2021· article· en· Zenodo (CERN European Organization for Nuclear Research)· Physics and Astronomy
machine prediction:candidate · noneconsensus · none
0
citations
affunlabeled
HST Observations of the Main Sequence of M4
Harvey B. Richer, G. G. Fahlman, J. Brewer, S. Davis, J. Kalirai, P. B. Stetson +5 more
2004· preprint· en· arXiv (Cornell University)· Physics and Astronomy
machine prediction:candidate · noneconsensus · none
0
citations
aboutno affunlabeled
New Books
2006· article· en· Physics Today· Physics and Astronomy
machine prediction:candidate · noneconsensus · none
0
citations
aboutno affunlabeled
News from the CFHT/ESPaDOnS spectropolarimeter
C. Moutou, Lison Malo, N. Manset, L. Selliez-Vandernotte, M. E. Desrochers
2015· preprint· en· arXiv (Cornell University)· Physics and Astronomy
machine prediction:candidate · noneconsensus · none
0
citations
← previousnext →

How this was built: Screen · Findings · About