Paper Citation Record · LEDGER

A dark jet dominates the power output of the stellar black hole Cygnus X-1

As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:astro-ph/0508228.

A citation records a reference. It does not transfer a finding from one paper to another.

pith.paper-citation-record.v1
astro-ph/0508228 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 3 of 3 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-11T06:34:44.6726+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-07T20:40:56.961619Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-06-29T03:03:03.301542Z

Reference resolution

0 of 0 outbound references displayed

verified exact0
verified fuzzy0
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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 a4abce80-b3fe-4714-96da-2d4b54a55c3e · inbound

Introduction to multi-messenger astronomy cites this paper.

Introduction to multi-messenger astronomy A dark jet dominates the power output of the stellar black hole Cygnus X-1

Reference 69

Resolution: verified exact; local_arxiv, observed 2026-05-24T20:29:53.379578Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

Observation 59e8c1ce-9eb1-47e3-96e4-c7fdfcde1112 · inbound

SKAO and Gamma-Ray Synergies cites this paper.

SKAO and Gamma-Ray Synergies A dark jet dominates the power output of the stellar black hole Cygnus X-1

Reference 13

Resolution: verified exact; local_arxiv, observed 2026-06-29T03:03:03.303177Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

Observation fd16109d-2fc1-4f27-830b-2e78299dc4e7 · inbound

Why do massive stars form bow shocks? Bulk ISM motion as the main driver of bow shock formation and geometry cites this paper.

Why do massive stars form bow shocks? Bulk ISM motion as the main driver of bow shock formation and geometry A dark jet dominates the power output of the stellar black hole Cygnus X-1

Reference 39

Resolution: unresolved; no resolver link, observed 2026-08-07T20:40:56.961619Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.