Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
An exact analytic treatment of propagating mass accretion rate fluctuations in X-ray binaries
As of 7 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:1306.3823.
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 2026-08-07T06:34:17.273281+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-06T17:00:41.734267Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-06-26T23:30:14.734053Z
Reference resolution
0 of 0 outbound references displayed
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- malformed identifier0
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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 c98d3993-196a-4824-bbe6-f0fe65b4a025 · inbound
Quasi-Periodic Oscillations due to radiative feedback mechanism between the disc and corona cites this paper.
Quasi-Periodic Oscillations due to radiative feedback mechanism between the disc and corona An exact analytic treatment of propagating mass accretion rate fluctuations in X-ray binaries
Reference 32
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T17:00:41.734267Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 1cf585bb-38f0-4026-91a0-920c70566e15 · inbound
Discovery of a quasi-periodic oscillation non-harmonically related to the Type-C QPO in the hard intermedidate state of MAXI J1820+070 cites this paper.
Discovery of a quasi-periodic oscillation non-harmonically related to the Type-C QPO in the hard intermedidate state of MAXI J1820+070 An exact analytic treatment of propagating mass accretion rate fluctuations in X-ray binaries
Reference 115
- Resolution
- verified exact
- local_arxiv, observed 2026-06-26T23:30:14.735283Z
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 10b6b486-4aa2-4f46-9390-399ad2c5291a · 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 An exact analytic treatment of propagating mass accretion rate fluctuations in X-ray binaries
Reference 231
- Resolution
- unresolved
- no resolver link, observed 2026-07-12T03:29:42.101488Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.