bigbounce/spin-torsion cosmology research program
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SurveysLAMOST

LAMOST DR10

Large Sky Area Multi-Object Fiber Spectroscopic Telescope Data Release 10. Largest spectroscopic survey before DESI. Transfer-learning run exposed training set bias.

QC CAUTION
11.4M spectra
44,075 anomalies (0.39%)
Optical spectroscopy (3700-9100 Å)
Readiness
QC CAUTION
LAMOST

~56% B-dominant cross-transfer (empirical; the 98% figure was a synthetic schematic not a measurement). Native retrain reduces anomaly count 21.4x (43,915 -> 2,054 at S>5). Path-C native model in progress.

Cost~$40
Runtime~18.3h
Sources11.4M spectra
Anomalies44,075
Rate0.39%
BandOptical
Key Findings
Results that define how this survey should be used in the paper set.
  • 0144,075 anomalies from 11.4M spectra (0.39%)
  • 02~56% B-dominant (empirical cross-transfer; 98% was synthetic schematic, not measured)
  • 038 UMAP clusters, mostly single population
  • 04Rankings are model-dependent — LAMOST-native model needed
Pipeline
ModelDESI BigAE transfer
WavelengthOptical spectroscopy (3700-9100 Å)
Cost~$40
Runtime~18.3h
Top Anomalies