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Paper Citation Record · LEDGER

Two decades of optical timing of the shortest-period binary star system HM Cancri

As of 6 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2211.09834.

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

pith.paper-citation-record.v1
2211.09834 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 2026-08-06T06:34:29.942622+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-01T02:17:55.381443Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-24T05:23:56.538208Z

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 828936b3-3cae-4f03-b04f-b5616b81524e · inbound

Waveform Modelling for the Laser Interferometer Space Antenna cites this paper.

Waveform Modelling for the Laser Interferometer Space Antenna Two decades of optical timing of the shortest-period binary star system HM Cancri

Reference 148

Resolution
verified exact
arxiv_id, observed 2026-05-24T05:23:56.540790Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

source=pdf_text observed=2026-05-24T05:21:16.199631Z digest=sha256:cc47c34076b5c615071ff6f1be4d618c1df666518eaa14b9abfb66bb94726804

Observation aa3c0d35-504a-4694-abe5-644e1236b695 · inbound

V407 Vul: a triple star system with an AM CVn detectable by gravitational wave observatories cites this paper.

V407 Vul: a triple star system with an AM CVn detectable by gravitational wave observatories Two decades of optical timing of the shortest-period binary star system HM Cancri

Reference 185

Resolution
unresolved
no resolver link, observed 2026-08-01T02:17:55.381443Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T02:17:55.381443Z digest=sha256:a76614f9b65a1a18c806046469b5b019d78d8595db95b6784214f8b6b5c16e9a

Observation 6f19e840-06ae-4226-816c-6832d4b40fe3 · inbound

SRG/eROSITA X-ray selected cataclysmic variable candidates observed in SDSS-V DR20 cites this paper.

SRG/eROSITA X-ray selected cataclysmic variable candidates observed in SDSS-V DR20 Two decades of optical timing of the shortest-period binary star system HM Cancri

Reference 75

Resolution
unresolved
no resolver link, observed 2026-07-31T22:10:39.522082Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-31T22:10:39.522082Z digest=sha256:8e0dc67bcaec89ae3032868033e423a5e9d23aac4abf553d9933333709cd118b