Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
An ultra-massive white dwarf with a mixed hydrogen-carbon atmosphere as a likely merger remnant
As of 6 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2003.00028.
A citation records a reference. It does not transfer a finding from one paper to another.
Coverage vector
One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-06T06:34:29.942622+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-03T20:37:51.362630Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-07-08T08:44:45.317353Z
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 8cafede8-c5e4-4890-8f62-18a7a4e4d16c · 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 An ultra-massive white dwarf with a mixed hydrogen-carbon atmosphere as a likely merger remnant
Reference 90
- Resolution
- unresolved
- no resolver link, observed 2026-08-03T20:37:51.362630Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 4ca0034e-dd27-46d3-99e9-8ac5b16d424c · inbound
Optical transients from non-explosive double white-dwarf mergers: the case of a central neutron star remnant cites this paper.
Optical transients from non-explosive double white-dwarf mergers: the case of a central neutron star remnant An ultra-massive white dwarf with a mixed hydrogen-carbon atmosphere as a likely merger remnant
Reference 18
- Resolution
- malformed identifier
- arxiv_id, observed 2026-05-15T08:55:19.494242Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.
Observation 6803f39f-f1ae-4935-8776-033bf0c41124 · inbound
White dwarfs within 13 pc: Insights from ultraviolet spectroscopy cites this paper.
White dwarfs within 13 pc: Insights from ultraviolet spectroscopy An ultra-massive white dwarf with a mixed hydrogen-carbon atmosphere as a likely merger remnant
Reference 212
- Resolution
- metadata mismatch
- local_arxiv, observed 2026-07-08T08:44:45.319811Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.