Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
As of 12 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:astro-ph/0412597.
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 2026-08-12T06:34:41.77262+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-10T16:29:20.651680Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-07-08T00:54:21.035569Z
0 of 0 outbound references displayed
External citation measurements
No source-named external measurement is stored.
No outbound reference observations are available for this paper version.
Observation c2a890ae-8a0a-4dd6-9e96-26ead62e976c · inbound
Spectro-temporal Investigation of Quasi-periodic Oscillations From Black Hole X-ray Binary 4U 1630-472 Using $\textit{NICER}$ The evolution of black hole states
Reference 13
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 6246347d-338f-499c-a18d-ba4cf1609906 · inbound
Discovery of a quasi-periodic oscillation non-harmonically related to the Type-C QPO in the hard intermedidate state of MAXI J1820+070 The evolution of black hole states
Reference 49
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation a733b7ff-038e-4be2-9164-734b4ccb0cac · inbound
Spectropolarimetric detection of baryonic mass loading in a transient relativistic jet: application to the black hole X-ray binary Swift J1727.8$-$1613 The evolution of black hole states
Reference 33
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation fefbe312-c40a-4442-be48-230783084b6c · inbound
Why do massive stars form bow shocks? Bulk ISM motion as the main driver of bow shock formation and geometry The evolution of black hole states
Reference 125
Source-reported events for the cited work
Unavailable: canonical work link unavailable.