bigbounce/spin-torsion cosmology research program
research live

SurveysLAMOST

LAMOST DR10

Legacy/superseded pipeline record retained for methodology and archive context. Historical candidate counts and classifications are unreconciled, are not current discovery results, and do not provide evidence for a bounce.

QC CAUTION
11.4M spectra
0 anomalies (Legacy / superseded)
Optical spectroscopy (3700-9100 Å)
Readiness
QC CAUTION
LAMOST

LEGACY / SUPERSEDED — Historical pipeline-quality note retained for audit context; it is not a current catalog-quality assertion.

Cost~$40
Runtime~18.3h
Sources11.4M spectra
Anomalies0
RateLegacy / superseded
BandOptical
Key Findings
Results that define how this survey should be used in the paper set.
  • 01Historical, unreconciled pipeline output — 44,075 anomalies from 11.4M spectra (0.39%)
  • 02Historical, unreconciled pipeline output — ~56% B-dominant (empirical cross-transfer; 98% was synthetic schematic, not measured)
  • 03Historical, unreconciled pipeline output — 8 UMAP clusters, mostly single population
  • 04Historical, unreconciled pipeline output — Rankings are model-dependent — LAMOST-native model needed
Pipeline
ModelDESI BigAE transfer
WavelengthOptical spectroscopy (3700-9100 Å)
Cost~$40
Runtime~18.3h
Top Anomalies