Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Mass ejection by pulsational pair instability in very massive stars and implications for luminous supernovae
As of 7 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:1511.01695.
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 2026-08-07T06:34:17.273281+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-07-11T11:50:26.030339Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-07-02T04:26:36.046603Z
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 ad72bf0d-181c-442c-8b24-749080bdd60a · inbound
Massquerade: Impacts of Mass Ratio Reversals on Binary Black Hole Merger Rates and Mass Distributions cites this paper.
Massquerade: Impacts of Mass Ratio Reversals on Binary Black Hole Merger Rates and Mass Distributions Mass ejection by pulsational pair instability in very massive stars and implications for luminous supernovae
Reference 231
- Resolution
- verified exact
- local_arxiv, observed 2026-05-22T09:31:21.379697Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation bf69ec74-435e-47c5-b5c9-baad60d45cfb · inbound
Can current models predict the local black hole merger rate? cites this paper.
Can current models predict the local black hole merger rate? Mass ejection by pulsational pair instability in very massive stars and implications for luminous supernovae
Reference 83
- Resolution
- verified exact
- local_arxiv, observed 2026-06-28T13:02:10.782597Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation e2142ff5-c793-427b-abc7-12797777f2ad · inbound
Targeting black holes from metal-poor progenitors with next-generation gravitational-wave detectors cites this paper.
Targeting black holes from metal-poor progenitors with next-generation gravitational-wave detectors Mass ejection by pulsational pair instability in very massive stars and implications for luminous supernovae
Reference 103
- Resolution
- verified exact
- local_arxiv, observed 2026-07-02T04:26:36.048058Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.