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Paper Citation Record · LEDGER

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

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.

pith.paper-citation-record.v1
2505.09671 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 5 of 5 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-07T06:34:17.273281+00:00

measured 5 of 5 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-07T04:20:39.474577Z

measured 1 of 1 external citation measurements

A source-named dated measurement, never combined with another source.

Source: arxiv_reference, observed 2026-08-05T02:28:24.338817Z

Reference resolution

0 of 0 outbound references displayed

  • verified exact0
  • verified fuzzy0
  • unresolved0
  • parse uncertain0
  • malformed identifier0
  • metadata mismatch0

External citation measurements

0
arxiv_reference, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 61a4a442-6841-4925-8266-69accaac356c · inbound

Magnetosonic Waves as a Driver of Observed Temperature Fluctuation Patterns in AGN Accretion Disks cites this paper.

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

Resolution
unresolved
no resolver link, observed 2026-08-07T04:20:39.474577Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T04:20:39.474577Z digest=sha256:034d504cffdfaeae52377cda304ee35d9766b4728ee03ce841cb771dc1d29d3b

Reference 31

Resolution
unresolved
no resolver link, observed 2026-08-05T10:54:53.099731Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-05T10:54:53.099731Z digest=sha256:52b3f69f93f2eabd0f40804c591d23bda912bdde5b130022293db22d9500ac2a

Observation 26d2594f-ebf7-443a-8ade-791b3c87331a · inbound

Viscously Spreading Accretion Disks around Black Holes: Implications for TDEs, LFBOTs and other Transients cites this paper.

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

Resolution
unresolved
no resolver link, observed 2026-08-03T17:41:19.498849Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-03T17:41:19.498849Z digest=sha256:b95b5c99646cbeff76b1efda1560ceb1ba80f82735669600c9093a1906ba461c

Reference 79

Resolution
verified exact
arxiv_id, observed 2026-05-21T01:29:21.925808Z

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.

source=arxiv_source observed=2026-05-21T01:25:53.670807Z digest=sha256:83e49885ab7aa7e859f2b77426d138131f5f2de60cfa9acb9a411a9c9f1deb2a

Observation d9c04c9d-fe8e-42c4-9d77-bfb4813824f9 · inbound

Closing the UV Gap: Rest-frame EUV science from high-redshift QSOs as a legacy-defining capability cites this paper.

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

Resolution
verified exact
arxiv_id, observed 2026-06-29T10:43:19.162309Z

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.

source=pdf_text observed=2026-06-29T10:42:31.313175Z digest=sha256:879f0b9f432727efcbe6be268adac8030b76200106c92dff42ca62776af4fd43