record state
frontier-ownedReview status
This finding is part of accepted frontier state. Review events, reviewable changes, and proof state explain how it can change.
unreviewed
frontiers / frontier
Finding bundle
back to staterecord state
frontier-ownedThis finding is part of accepted frontier state. Review events, reviewable changes, and proof state explain how it can change.
finding statement
finding typeNo entity list is declared.
evidence
source-boundtheoretical · manual state transition
proof impact
packet context1 reviewable changes and 0 evaluation records are attached to this finding id.
Evidence and conditions
method
manual state transition
evidence type
theoretical
conditions
Provenance
source title
GWTC-3 population analysis with 66 confident events
authors
reviewer:will-blair
The probability of a gravitational-wave component being a neutron star rather than a black hole (P_NS) varies by 51-100% for GW190425's primary but < 10% for GW190814's secondary, driven primarily by pairing preferences and spin distributions in compact-binary population models.
vs_a942ba614a62766c · manual_curation
outgoing
vf_e0ee8afc69ddd823Population classification probabilities depend on machine-learning model outputs for chirp mass and mass-ratio inference
events
vev_42133bbb89c46cb1finding.assertedManual finding added to frontier state
reviewer:will-blair · 2026-05-29
reviewable changes
vpr_9b11e91c8cd43e02finding.addManual finding added to frontier state
applied · reviewer:will-blair · 2026-05-29
evaluations
No evaluation record targets this finding id.