Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Common envelope ejection in massive binary stars - Implications for the progenitors of GW150914 and GW151226
As of 4 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:1610.04417.
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 2026-08-04T06:34:03.388597+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-03T02:40:49.689341Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-06-26T09:59:18.263275Z
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 8190d98f-467d-48fe-8b8b-6d0dbb2a47f5 · 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 Common envelope ejection in massive binary stars - Implications for the progenitors of GW150914 and GW151226
Reference 169
- Resolution
- verified exact
- local_arxiv, observed 2026-05-22T09:31:21.753016Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.
Observation c55869bc-2141-46ef-8412-439238f9f0bb · inbound
Comparative Study of Two Luminous Red Novae I. Progenitor Modeling and Dust Formation cites this paper.
Comparative Study of Two Luminous Red Novae I. Progenitor Modeling and Dust Formation Common envelope ejection in massive binary stars - Implications for the progenitors of GW150914 and GW151226
Reference 191
- Resolution
- verified exact
- local_arxiv, observed 2026-06-26T09:59:18.264608Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.
Observation fd27fe15-d720-49cc-92ee-b070c2b72934 · inbound
The IACOB project XIX. Revisiting massive-star evolution with empirical TAMS constraints: updated models, overshoot calibration, and the population of blue supergiants cites this paper.
The IACOB project XIX. Revisiting massive-star evolution with empirical TAMS constraints: updated models, overshoot calibration, and the population of blue supergiants Common envelope ejection in massive binary stars - Implications for the progenitors of GW150914 and GW151226
Reference 161
- Resolution
- unresolved
- no resolver link, observed 2026-08-03T02:40:49.689341Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.