Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
As of 8 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:2505.09671.
A citation records a reference. It does not transfer a finding from one paper to another.
Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-07T06:34:17.273281+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-07T04:20:39.474577Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-08-05T02:28:24.338817Z
0 of 0 outbound references displayed
External citation measurements
0
arxiv_reference, observed 2026-08-05T02:28:24.338817Z
No outbound reference observations are available for this paper version.
Observation 61a4a442-6841-4925-8266-69accaac356c · inbound
Magnetosonic Waves as a Driver of Observed Temperature Fluctuation Patterns in AGN Accretion Disks Radiation and Magnetic Pressure Support in Accretion Disks around Supermassive Black Holes and The Physical Origin of the Extreme Ultraviolet to Soft X-ray Spectrum
Reference 31
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 69dcb7e7-01e9-4865-9bdb-89848dde3907 · inbound
Do Little Red Dots Vary? Radiation and Magnetic Pressure Support in Accretion Disks around Supermassive Black Holes and The Physical Origin of the Extreme Ultraviolet to Soft X-ray Spectrum
Reference 31
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 26d2594f-ebf7-443a-8ade-791b3c87331a · inbound
Viscously Spreading Accretion Disks around Black Holes: Implications for TDEs, LFBOTs and other Transients Radiation and Magnetic Pressure Support in Accretion Disks around Supermassive Black Holes and The Physical Origin of the Extreme Ultraviolet to Soft X-ray Spectrum
Reference 27
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation bc7e427f-76f9-4697-9260-7d4674e610e3 · inbound
Simulation-Based Prediction of Black Hole Fe K$\alpha$ Line Profiles Radiation and Magnetic Pressure Support in Accretion Disks around Supermassive Black Holes and The Physical Origin of the Extreme Ultraviolet to Soft X-ray Spectrum
Reference 79
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation d9c04c9d-fe8e-42c4-9d77-bfb4813824f9 · inbound
Closing the UV Gap: Rest-frame EUV science from high-redshift QSOs as a legacy-defining capability Radiation and Magnetic Pressure Support in Accretion Disks around Supermassive Black Holes and The Physical Origin of the Extreme Ultraviolet to Soft X-ray Spectrum
Reference 36
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.