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Paper Citation Record · LEDGER

Symbiotic star T CrB as an extreme SU UMa type dwarf nova

As of 20 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2307.13838.

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

pith.paper-citation-record.v1
2307.13838 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 2026-08-16T10:56:23.221055Z

measured 0 of 1 external citation measurements

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

Source: cited_works

Reference resolution

0 of 0 outbound references displayed

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  • malformed identifier0
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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 73acac7e-9619-4d64-b641-ae8a211aef62 · 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 Symbiotic star T CrB as an extreme SU UMa type dwarf nova

Reference 125

Resolution
malformed identifier
no resolver link, observed 2026-08-16T10:56:23.221055Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-16T10:56:23.221055Z digest=sha256:fea1c035d316e8f9464079ec12de0bb68778cb682cb8b9406f3221830dd386fa

Observation a99b4cce-46b0-4323-8446-1f9ba2f71122 · inbound

When will T Coronae Borealis next erupt as a nova? Constraints from recurrence, orbital phase, and accretion-state evolution cites this paper.

When will T Coronae Borealis next erupt as a nova? Constraints from recurrence, orbital phase, and accretion-state evolution Symbiotic star T CrB as an extreme SU UMa type dwarf nova

Reference 28

Resolution
unresolved
no resolver link, observed 2026-08-01T23:47:55.293424Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T23:47:55.293424Z digest=sha256:806dc254b08f19af7767321d83c8f6bd4d05e904dae5c0388cd953cfd9d42c2a