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Paper Citation Record · LEDGER

Models for the evolution of close binaries with He-Star and WD components towards Type Ia supernova explosions

As of 20 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1603.00768.

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

pith.paper-citation-record.v1
1603.00768 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 2026-08-20T06:33:59.587034+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-12T05:49:59.839253Z

measured 1 of 1 external citation measurements

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

Source: pith, observed 2026-08-05T02:28:24.338817Z

Reference resolution

0 of 0 outbound references displayed

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

External citation measurements

36
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 9b55a1cd-1af2-48a1-ad0f-fc76c7a99302 · inbound

A gravitational wave detectable candidate Type Ia supernova progenitor cites this paper.

A gravitational wave detectable candidate Type Ia supernova progenitor Models for the evolution of close binaries with He-Star and WD components towards Type Ia supernova explosions

Reference 25

Resolution
unresolved
no resolver link, observed 2026-08-12T05:49:59.839253Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-12T05:49:59.839253Z digest=sha256:c25512330f12695aebe44c48e2c123e12a9210c857778469f3f5a269bdb61190

Observation d443c21e-8bf9-48d2-b57f-7b08bfbb5594 · inbound

Studying hot evolved stars with ultraviolet spectroscopy cites this paper.

Studying hot evolved stars with ultraviolet spectroscopy Models for the evolution of close binaries with He-Star and WD components towards Type Ia supernova explosions

Reference 84

Resolution
verified exact
local_arxiv, observed 2026-06-28T03:11:30.954731Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:eebec8e4fc0ce040a80f4d25a6f81560560fc597d8c1f32fade1120ec24a4f43