Paper Citation Record · LEDGER

A Wide Symbiotic Channel to Type Ia Supernovae

As of 18 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:astro-ph/9902304.

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

pith.paper-citation-record.v1
astro-ph/9902304 v2

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 2026-08-18T06:34:40.430872+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-16T10:56:22.779015Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-06-27T18:01:07.990579Z

Reference resolution

0 of 0 outbound references displayed

verified exact0
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 b5d7f299-17d4-4c70-805b-7759f00b9d03 · inbound

Symbiotic stars in the era of modern ground- and space-based surveys cites this paper.

Symbiotic stars in the era of modern ground- and space-based surveys A Wide Symbiotic Channel to Type Ia Supernovae

Reference 7

Resolution: unresolved; no resolver link, observed 2026-08-16T10:56:22.779015Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 0b50ae51-c258-45d5-8a4d-a0adb38e7d9b · inbound

JWST Absorption-Line Analysis of UV-Bright Galaxies at $z=7.2-10.6$: Early Chemical Enrichment Traced by C, O, Mg, Al, Si, and Fe cites this paper.

JWST Absorption-Line Analysis of UV-Bright Galaxies at $z=7.2-10.6$: Early Chemical Enrichment Traced by C, O, Mg, Al, Si, and Fe A Wide Symbiotic Channel to Type Ia Supernovae

Reference 152

Resolution: verified exact; local_arxiv, observed 2026-06-27T18:01:07.991906Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation 63aa8c1a-1616-44fa-bb27-11f5a3f81d74 · inbound

Why is GN-z11 Bright, Compact, and Nitrogen Enhanced? Insights from UV Absorption and Emission Diagnostics cites this paper.

Why is GN-z11 Bright, Compact, and Nitrogen Enhanced? Insights from UV Absorption and Emission Diagnostics A Wide Symbiotic Channel to Type Ia Supernovae

Reference 298

Resolution: unresolved; no resolver link, observed 2026-08-16T00:12:18.948781Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.