Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Black hole-neutron star binaries with high spins and large mass asymmetries: I. Properties of quasi-equilibrium sequences
As of 19 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:2409.06767.
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 2026-08-18T06:34:40.430872+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-10T16:31:09.745017Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-08-06T18:10:16.252104Z
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 a69d04af-f9f3-4f38-89b3-05927cf17bcc · inbound
Implications of Magnetic Flux-Disk Mass Correlation in Black Hole-Neutron Star Mergers for GRB sub-populations cites this paper.
Implications of Magnetic Flux-Disk Mass Correlation in Black Hole-Neutron Star Mergers for GRB sub-populations Black hole-neutron star binaries with high spins and large mass asymmetries: I. Properties of quasi-equilibrium sequences
Reference 31
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T16:31:09.745017Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 16d47f38-b00f-4585-ae32-fb8d353aba38 · inbound
Black-hole - neutron-star mergers: new numerical-relativity simulations and multipolar effective-one-body model with spin precession and eccentricity cites this paper.
Black-hole - neutron-star mergers: new numerical-relativity simulations and multipolar effective-one-body model with spin precession and eccentricity Black hole-neutron star binaries with high spins and large mass asymmetries: I. Properties of quasi-equilibrium sequences
Reference 84
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T21:32:50.606501Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 2dc5284f-eceb-4d25-be35-d09f86adefb3 · inbound
Combining (post-)Newtonian ideas with quasi-equilibrium (QE) sequence analysis for black hole-neutron star (BHNS) gravitational wave events cites this paper.
Combining (post-)Newtonian ideas with quasi-equilibrium (QE) sequence analysis for black hole-neutron star (BHNS) gravitational wave events Black hole-neutron star binaries with high spins and large mass asymmetries: I. Properties of quasi-equilibrium sequences
Reference 22
- Resolution
- verified exact
- local_arxiv, observed 2026-08-06T18:10:16.306352Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.
Observation b8b0fcfd-91e4-492f-b0f7-5775ba60ff7e · inbound
Black hole-neutron star binaries with high spins and large mass asymmetries: III. Properties of the ejected material and its electromagnetic signatures cites this paper.
Black hole-neutron star binaries with high spins and large mass asymmetries: III. Properties of the ejected material and its electromagnetic signatures Black hole-neutron star binaries with high spins and large mass asymmetries: I. Properties of quasi-equilibrium sequences
Reference 80
- Resolution
- unresolved
- no resolver link, observed 2026-08-01T09:55:44.686399Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.