Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Formation and Evolution of Binary Neutron Stars
As of 8 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:astro-ph/9710347.
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 2026-08-06T10:25:57.477944Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-08-06T12:16:18.182151Z
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 c9c95883-b331-4ea6-8d46-973ad2bc9c99 · inbound
Forming Double Neutron Stars using Detailed Binary Evolution Models with POSYDON: Comparison to the Galactic Systems cites this paper.
Forming Double Neutron Stars using Detailed Binary Evolution Models with POSYDON: Comparison to the Galactic Systems Formation and Evolution of Binary Neutron Stars
Reference 140
- Resolution
- verified exact
- local_arxiv, observed 2026-08-06T10:25:58.138549Z
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 114f3e84-c08f-4389-b079-487d559c41c3 · inbound
Characterizing Binary Black Hole Subpopulations in GWTC-4 with Binned Gaussian Processes: On the Origins of the $35M_{\odot}$ Peak cites this paper.
Characterizing Binary Black Hole Subpopulations in GWTC-4 with Binned Gaussian Processes: On the Origins of the $35M_{\odot}$ Peak Formation and Evolution of Binary Neutron Stars
Reference 91
- Resolution
- unresolved
- no resolver link, observed 2026-08-03T19:56:47.309465Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.