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Paper Citation Record · LEDGER

Counter evidence against multiple frequency nature of 0.75 mHz oscillation in V4743 Sgr

As of 22 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1702.05375.

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

pith.paper-citation-record.v1
1702.05375 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 2 of 2 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-22T06:32:14.747728+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-01T23:47:56.786406Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-05-22T05:31:07.259390Z

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 8bdfb1f6-e672-48a6-8ec8-3fe103a564b5 · inbound

The powerful shocks in RS Oph: NuSTAR X-ray data and a complete review cites this paper.

The powerful shocks in RS Oph: NuSTAR X-ray data and a complete review Counter evidence against multiple frequency nature of 0.75 mHz oscillation in V4743 Sgr

Reference 213

Resolution
verified exact
local_arxiv, observed 2026-05-22T05:31:07.262265Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:30241dc5612384f18ddcc998e95033fb249342ddea1f1d1ca3f6f83b45ed8c34

Observation 82e1f8fe-9449-415b-ad12-9732de7a9547 · inbound

When will T Coronae Borealis next erupt as a nova? Constraints from recurrence, orbital phase, and accretion-state evolution cites this paper.

When will T Coronae Borealis next erupt as a nova? Constraints from recurrence, orbital phase, and accretion-state evolution Counter evidence against multiple frequency nature of 0.75 mHz oscillation in V4743 Sgr

Reference 41

Resolution
unresolved
no resolver link, observed 2026-08-01T23:47:56.786406Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T23:47:56.786406Z digest=sha256:b04cfb370c3e88388c00da6545484f20b4e8bc4f57bedca774071ee4d8cc84b5