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Paper Citation Record · LEDGER

The evolution of white dwarfs resulting from helium-enhanced, low-metallicity progenitor stars

As of 15 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1611.06191.

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

pith.paper-citation-record.v1
1611.06191 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 2026-08-14T06:32:32.682623+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-14T04:29:55.084178Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-08-14T04:29:56.128215Z

Reference resolution

0 of 0 outbound references displayed

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  • 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 43838103-49ff-4450-906d-da1cd53b8ad4 · inbound

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

Asteroseismic study of KUV03442+0719 with parallax constraints The evolution of white dwarfs resulting from helium-enhanced, low-metallicity progenitor stars

Reference 5

Resolution
unresolved
no resolver link, observed 2026-08-01T00:24:09.830768Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T00:24:09.830768Z digest=sha256:4571cd3934e6253e57d6b9b368453717800a27c096aecfab6e5b6a431c520b4a

Observation 62eb4010-3fa7-4847-b23a-0c9c9912037e · inbound

White dwarf-neutron star matter transition and the effect of light elements cites this paper.

White dwarf-neutron star matter transition and the effect of light elements The evolution of white dwarfs resulting from helium-enhanced, low-metallicity progenitor stars

Reference 83

Resolution
verified exact
local_arxiv, observed 2026-08-14T04:29:56.136386Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

source=pdf_text observed=2026-08-14T04:29:55.084178Z digest=sha256:771cdefc05236faf15d7f4a73b110ede8914150c4ba882a9aa00f8d2b2503887