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Paper Citation Record · LEDGER

On the Distances to the X-ray Binaries Cygnus X-3 and GRS 1915+105

As of 17 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:2309.15027.

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

pith.paper-citation-record.v1
2309.15027 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 2026-08-17T06:30:58.91139+00:00

measured 5 of 5 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-14T04:30:46.924753Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-08T13:54:58.375927Z

Reference resolution

0 of 0 outbound references displayed

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

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 18967cf0-74ac-4abe-a37c-a1d7d1e500af · inbound

Cygnus X-3: A variable petaelectronvolt gamma-ray source cites this paper.

Cygnus X-3: A variable petaelectronvolt gamma-ray source On the Distances to the X-ray Binaries Cygnus X-3 and GRS 1915+105

Reference 57

Resolution
verified exact
arxiv_id, observed 2026-05-16T21:28:33.670756Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

source=pdf_text observed=2026-05-16T21:26:59.901451Z digest=sha256:500d46c9d590100b059683cc621327d1d5414ca96dea05b6ff31fefb7a6316cf

Observation 0ea76e56-8090-4af9-99b7-22d45ce80248 · inbound

An intrinsic decline of accretion activity in GRS 1915+105 cites this paper.

An intrinsic decline of accretion activity in GRS 1915+105 On the Distances to the X-ray Binaries Cygnus X-3 and GRS 1915+105

Reference 54

Resolution
verified exact
local_arxiv, observed 2026-07-08T13:54:58.377068Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:428714d4ecdb0853d5fa1c105d195cf51323736f15c92af052fb385cc0886373

Observation b3894d94-97b3-4cb1-829e-92610791adf7 · inbound

PeV extended emission around Galactic PeVatrons and echos of their flares cites this paper.

PeV extended emission around Galactic PeVatrons and echos of their flares On the Distances to the X-ray Binaries Cygnus X-3 and GRS 1915+105

Reference 4

Resolution
unresolved
no resolver link, observed 2026-08-02T00:29:05.227109Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-02T00:29:05.227109Z digest=sha256:31b1e3a959e7d36be3701e9142eef53103fc9909d64771ec0983beccfa9ed968

Observation e462343b-5c62-4aa3-8f54-0e6acfd36e53 · inbound

Distinct Jet Properties in the X-Ray-Obscured State of GRS 1915+105 cites this paper.

Distinct Jet Properties in the X-Ray-Obscured State of GRS 1915+105 On the Distances to the X-ray Binaries Cygnus X-3 and GRS 1915+105

Reference 31

Resolution
unresolved
no resolver link, observed 2026-08-01T03:20:29.225078Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T03:20:29.225078Z digest=sha256:f903e227f5f99d324e879b1a7a94947f887d9e6228fd1ea2850579a3948989cc

Observation 7f7f4f4b-27c2-4d46-ae68-e5a2cb8cb666 · inbound

Simulation-based inference for AGN jet population modelling: Towards more robust comparisons of black hole jet speeds cites this paper.

Simulation-based inference for AGN jet population modelling: Towards more robust comparisons of black hole jet speeds On the Distances to the X-ray Binaries Cygnus X-3 and GRS 1915+105

Reference 275

Resolution
unresolved
no resolver link, observed 2026-08-14T04:30:46.924753Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T04:30:46.924753Z digest=sha256:1425d2d76586b3adedffd30909102197f39b92b1507bf5d8f51cf834db3f5187