Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Physical properties of IP Pegasi: an eclipsing dwarf nova with an unusually cool white dwarf
As of 14 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 1 inbound Pith citation observation for arXiv:0911.1637.
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 2026-08-13T06:32:02.005865+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-12T05:50:00.108344Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-08-12T05:50:00.443985Z
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 b7087908-c9b0-4b41-b362-b2b31b44b6e9 · inbound
A gravitational wave detectable candidate Type Ia supernova progenitor cites this paper.
A gravitational wave detectable candidate Type Ia supernova progenitor Physical properties of IP Pegasi: an eclipsing dwarf nova with an unusually cool white dwarf
Reference 55
- Resolution
- verified exact
- local_arxiv, observed 2026-08-12T05:50:00.449592Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.