Pith. sign in

Paper Citation Record · LEDGER

On the existence of warm H-rich pulsating white dwarfs

As of 19 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:1911.02442.

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

pith.paper-citation-record.v1
1911.02442 v1

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 2026-08-12T11:38:37.839287Z

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

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

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 19f9bdce-3112-4962-85b5-1a022988a565 · inbound

A primer on the formation and evolution of hydrogen deficient Central Stars of Planetary Nebul{\ae} and Related Objects cites this paper.

A primer on the formation and evolution of hydrogen deficient Central Stars of Planetary Nebul{\ae} and Related Objects On the existence of warm H-rich pulsating white dwarfs

Reference 132

Resolution
unresolved
no resolver link, observed 2026-08-12T11:38:37.839287Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-12T11:38:37.839287Z digest=sha256:5a873e9571cc6de46e84f6a4a9d2255bbb26240d61f2656aed3aef9981ef545a

Observation 1815a694-dc07-4a08-928e-b4a24f8c87cb · inbound

Observing bright pulsating white dwarfs with PLATO: A new window into the late stages of stellar evolution cites this paper.

Observing bright pulsating white dwarfs with PLATO: A new window into the late stages of stellar evolution On the existence of warm H-rich pulsating white dwarfs

Reference 74

Resolution
unresolved
no resolver link, observed 2026-08-03T20:37:50.550588Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-03T20:37:50.550588Z digest=sha256:5ae9258241a1add5d4a0190a0e4c4d0955205636dcffa7fae17e7b00a370a3dd

Observation 5a4c8c0b-52e2-4063-aaf1-0fb144ee04ff · inbound

Constraints from parallaxes and average period spacings in the asteroseismic study of 8 DAVs cites this paper.

Constraints from parallaxes and average period spacings in the asteroseismic study of 8 DAVs On the existence of warm H-rich pulsating white dwarfs

Reference 8

Resolution
unresolved
no resolver link, observed 2026-07-30T15:34:28.630801Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-30T15:34:28.630801Z digest=sha256:84132cbfb4e9c92a9e0850776208fde70f853681c5b498d99463da08724a7542