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Paper Citation Record · LEDGER

Expanding the ultracompacts: gravitational wave-driven mass transfer in the shortest-period binaries with accretion disks

As of 7 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2411.12796.

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

pith.paper-citation-record.v1
2411.12796 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 2026-08-07T06:34:17.273281+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-06T21:47:54.058669Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-08-06T21:47:56.983383Z

Reference resolution

0 of 0 outbound references displayed

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  • verified fuzzy0
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  • 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 02468668-c0ed-4ccc-a352-bdcaa8ec3df5 · inbound

Search for Higher Harmonic Signals from Close White Dwarf Binaries in the mHz Band cites this paper.

Search for Higher Harmonic Signals from Close White Dwarf Binaries in the mHz Band Expanding the ultracompacts: gravitational wave-driven mass transfer in the shortest-period binaries with accretion disks

Reference 14

Resolution
verified exact
local_arxiv, observed 2026-08-06T21:47:57.002065Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

source=pdf_text observed=2026-08-06T21:47:54.058669Z digest=sha256:fd38bf41066074f6e34bccef9c97a431c4a23fa87f3b88924b9b5cde3b46fe75

Observation b1ed5214-e64a-476d-9b69-f5855edbbcd8 · 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 Expanding the ultracompacts: gravitational wave-driven mass transfer in the shortest-period binaries with accretion disks

Reference 204

Resolution
unresolved
no resolver link, observed 2026-08-01T02:17:55.423338Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T02:17:55.423338Z digest=sha256:47e7d31b752a30e13c5945bdd3fcaad1e774afde1dc0403935c142c9b476050c