Pith. sign in

Paper Citation Record · LEDGER

Pulsating low-mass white dwarfs in the frame of new evolutionary sequences: IV. The secular rate of period change

As of 12 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:1701.08880.

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

pith.paper-citation-record.v1
1701.08880 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 2026-08-12T06:34:41.77262+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-03T20:37:50.107837Z

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 91a647ff-a06d-420f-b1aa-11f958284213 · 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 Pulsating low-mass white dwarfs in the frame of new evolutionary sequences: IV. The secular rate of period change

Reference 64

Resolution
unresolved
no resolver link, observed 2026-08-03T20:37:50.107837Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-03T20:37:50.107837Z digest=sha256:89d72f12f41d627aa9cb5b26205d47267c8a9efcf72fa0611a033bdb10dc74df

Observation 5e5a25ba-a74e-4f54-b511-3cbc3665ee06 · inbound

Asteroseismic study of KUV03442+0719 with parallax constraints cites this paper.

Asteroseismic study of KUV03442+0719 with parallax constraints Pulsating low-mass white dwarfs in the frame of new evolutionary sequences: IV. The secular rate of period change

Reference 40

Resolution
unresolved
no resolver link, observed 2026-08-01T00:24:15.218821Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T00:24:15.218821Z digest=sha256:4ad6959e817ff949a970e0aaa11f79f49ca3ff90dc5609fc2e7f006f9ffd8087

Observation 19ea2f52-6b77-4c91-9369-3655e6fc9f25 · 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 Pulsating low-mass white dwarfs in the frame of new evolutionary sequences: IV. The secular rate of period change

Reference 52

Resolution
unresolved
no resolver link, observed 2026-07-30T15:34:28.991031Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-30T15:34:28.991031Z digest=sha256:91cb9c0f3ed654485ee6666a9dd08fd91af9054ba5cd68ae718f1f71c6c4ab75