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Paper Citation Record · LEDGER

Hydrogen Burning on Accreting White Dwarfs: Stability, Recurrent Novae, and the Post-Novae Supersoft Source

As of 23 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 6 inbound Pith citation observations for arXiv:1309.3375.

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

pith.paper-citation-record.v1
1309.3375 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 6 of 6 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-22T06:32:14.747728+00:00

measured 6 of 6 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-16T10:56:22.855902Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-05-22T05:31:07.061333Z

Reference resolution

0 of 0 outbound references displayed

  • verified exact0
  • verified fuzzy0
  • unresolved0
  • parse uncertain0
  • 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 39739af7-4333-4a16-8ade-83a09b44fc6e · 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 Hydrogen Burning on Accreting White Dwarfs: Stability, Recurrent Novae, and the Post-Novae Supersoft Source

Reference 28

Resolution
unresolved
no resolver link, observed 2026-08-16T10:56:22.855902Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-16T10:56:22.855902Z digest=sha256:affdd716076555f4f3100a940630fe0335d099583906f4fed6822159f60befb7

Observation 95c0956c-79d9-4ca5-a0a1-1382c1efaae8 · inbound

The Recurrent Nova Population in M31 cites this paper.

The Recurrent Nova Population in M31 Hydrogen Burning on Accreting White Dwarfs: Stability, Recurrent Novae, and the Post-Novae Supersoft Source

Reference 27

Resolution
verified exact
arxiv_id, observed 2026-05-10T09:48:48.046908Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

source=pdf_text observed=2026-05-10T05:07:14.789771Z digest=sha256:0c9595f0ab1979976e14c3c9adfad2d5907794c152784a5571fb742657727e97

Observation 02a27d9a-a443-4336-9208-f0a3bacdf456 · inbound

The powerful shocks in RS Oph: NuSTAR X-ray data and a complete review cites this paper.

The powerful shocks in RS Oph: NuSTAR X-ray data and a complete review Hydrogen Burning on Accreting White Dwarfs: Stability, Recurrent Novae, and the Post-Novae Supersoft Source

Reference 242

Resolution
verified exact
local_arxiv, observed 2026-05-22T05:31:07.064918Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:852d6712fa032718e6358b651c8fcc1afd7dce2fba25915a12591bf5c3cf6d0f

Observation 40d80b86-53d7-4bac-80c0-e8f22a36b000 · 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 Hydrogen Burning on Accreting White Dwarfs: Stability, Recurrent Novae, and the Post-Novae Supersoft Source

Reference 87

Resolution
unresolved
no resolver link, observed 2026-08-01T23:48:00.723347Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T23:48:00.723347Z digest=sha256:cad4a7d2e2249989095c8bc9ffaf497ca6a06d460554ae9d329cfa232e2c5449

Observation 6a1a983c-51e4-4c02-b879-fa3c006d050a · inbound

Dynamical formation of long-period exoplanets systems in evolving binary stars cites this paper.

Dynamical formation of long-period exoplanets systems in evolving binary stars Hydrogen Burning on Accreting White Dwarfs: Stability, Recurrent Novae, and the Post-Novae Supersoft Source

Reference 32

Resolution
unresolved
no resolver link, observed 2026-08-01T13:29:02.421189Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T13:29:02.421189Z digest=sha256:d4f24f21fd1eda930cf93be2e922596846ed2553c53ca90b0eb9d8ab0e5500a9

Observation 7b0fa9e2-cef7-47e3-ab81-f1183ef5a111 · inbound

A Century of Novae in the Large Magellanic Cloud cites this paper.

A Century of Novae in the Large Magellanic Cloud Hydrogen Burning on Accreting White Dwarfs: Stability, Recurrent Novae, and the Post-Novae Supersoft Source

Reference 2

Resolution
unresolved
no resolver link, observed 2026-07-30T10:43:49.022784Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-30T10:43:49.022784Z digest=sha256:734fc0ef72fe2c8ce723c4f658e080f081f23f61c6558707d61fa171d1121bd2