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Paper Citation Record · LEDGER

Population synthesis for double white dwarfs. II. Semi-detached systems: AM CVn stars

As of 7 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:astro-ph/0101123.

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

pith.paper-citation-record.v1
astro-ph/0101123 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 2026-08-06T21:47:54.382493Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-08-06T21:47:56.612893Z

Reference resolution

0 of 0 outbound references displayed

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  • 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 45c61d96-631f-49c5-bd5f-d3e9b1e54e20 · 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 Population synthesis for double white dwarfs. II. Semi-detached systems: AM CVn stars

Reference 18

Resolution
verified exact
local_arxiv, observed 2026-08-06T21:47:56.668175Z

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=2026-08-06T21:47:54.382493Z digest=sha256:72abb7583d2c374b5554ff8ab5fcbf63ad4462d598a6a6e99cfc251b33c53d0a

Observation 2c7726aa-3dc6-4dae-8e1a-79e46acc0273 · 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 Population synthesis for double white dwarfs. II. Semi-detached systems: AM CVn stars

Reference 145

Resolution
unresolved
no resolver link, observed 2026-08-01T02:17:55.279406Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T02:17:55.279406Z digest=sha256:f40d965d028d4149c52a8be062ee532c5121eaaf7815e4069b889ecde8e66886