Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Estimating Black Hole Spin from AGN SED Fitting: The Impact of General-Relativistic Ray Tracing
As of 14 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:2304.01253.
A citation records a reference. It does not transfer a finding from one paper to another.
Coverage vector
One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-14T06:32:32.682623+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-03T01:34:15.510382Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-05-11T20:51:10.731008Z
Reference resolution
0 of 0 outbound references displayed
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External citation measurements
No source-named external measurement is stored.
Outbound references
No outbound reference observations are available for this paper version.
Pith citing papers
Observation 029d28c3-1ac6-4b72-93b3-0642734d0be8 · inbound
The Dependence of the Mean Spectral Energy Distributions on the Accretion Rate for Quasars with $z < 0.75$ from the Sloan Digital Sky Survey cites this paper.
The Dependence of the Mean Spectral Energy Distributions on the Accretion Rate for Quasars with $z < 0.75$ from the Sloan Digital Sky Survey Estimating Black Hole Spin from AGN SED Fitting: The Impact of General-Relativistic Ray Tracing
Reference 19
- Resolution
- verified exact
- arxiv_id, observed 2026-05-11T20:51:10.734230Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.
Observation 2210d001-d9c6-47dc-98b0-336c0b5e0c3b · inbound
Physically motivated AGN emissivity profiles and their effects on quasar microlensing signatures. 1. Multi-epoch accretion disc size inference cites this paper.
Physically motivated AGN emissivity profiles and their effects on quasar microlensing signatures. 1. Multi-epoch accretion disc size inference Estimating Black Hole Spin from AGN SED Fitting: The Impact of General-Relativistic Ray Tracing
Reference 199
- Resolution
- unresolved
- no resolver link, observed 2026-07-12T03:29:42.101488Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 490a6a6c-334e-424a-9189-b6eea3ea4e16 · inbound
The COLIBRE-SKIRT pipeline: Calibration-free dust radiative transfer postprocessing for cosmological simulations cites this paper.
The COLIBRE-SKIRT pipeline: Calibration-free dust radiative transfer postprocessing for cosmological simulations Estimating Black Hole Spin from AGN SED Fitting: The Impact of General-Relativistic Ray Tracing
Reference 196
- Resolution
- unresolved
- no resolver link, observed 2026-08-02T00:50:15.597879Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 150ee356-be8e-4d21-8219-23004a0bbd3f · inbound
Energy-dependent Optical/Near-infrared and X-ray Correlations in Swift J1727.8-1613 cites this paper.
Energy-dependent Optical/Near-infrared and X-ray Correlations in Swift J1727.8-1613 Estimating Black Hole Spin from AGN SED Fitting: The Impact of General-Relativistic Ray Tracing
Reference 99
- Resolution
- unresolved
- no resolver link, observed 2026-08-03T01:34:15.510382Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.