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 context2 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
X-ray spectroscopy of accretion (Reynold et al., Miller et al.)
authors
reviewer:will-blair
Black hole spin measurements from accretion disk iron Kα line profiles (continuum reflection spectroscopy) in X-ray binaries show characteristic spin distributions (χ_BH ~ 0–0.95) that constrain formation models for dynamically-assembled systems in galactic nuclei.
vs_818f0a1f36d94368 · manual_curation
outgoing
No outgoing links.
events
vev_35c21461ca96316efinding.assertedManual finding added to frontier state
reviewer:will-blair · 2026-05-29
vev_b83b4d1cde524c5afinding.caveatedVerifier caution: X-ray spectroscopy spin range (χ_BH ~ 0–0.95) is plausible; Reynolds and Miller are known experts in this field. However, no specific citation provided to verify the exact spin distribution claimed.
reviewer:will-blair · 2026-05-29
reviewable changes
vpr_c3d63c18d5622bf1finding.addManual finding added to frontier state
applied · reviewer:will-blair · 2026-05-29
vpr_8d896148d69961a5finding.caveatVerifier caution: X-ray spectroscopy spin range (χ_BH ~ 0–0.95) is plausible; Reynolds and Miller are known experts in this field. However, no specific citation provided to verify the exact spin distribution claimed.
applied · reviewer:will-blair · 2026-05-29
evaluations
No evaluation record targets this finding id.