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evidence atoms
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Locator and citation
locator
title:X-ray spectroscopy of accretion (Reynold et al., Miller et al.)
imported
2026-05-29T02:16:32.250252+00:00
extraction mode
manual_curation
authors
reviewer:will-blair
Caveats
No source-specific caveats are recorded.
observational · vf_bd2636edddee7205
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.
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
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