Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
As of 7 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2106.06391.
A citation records a reference. It does not transfer a finding from one paper to another.
Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-06T06:34:29.942622+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-06T21:32:50.473993Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-05-12T08:41:25.444488Z
0 of 0 outbound references displayed
External citation measurements
No source-named external measurement is stored.
No outbound reference observations are available for this paper version.
Observation 0a720d15-1ec0-41d7-9652-3d8b22d9fcb2 · inbound
Black-hole - neutron-star mergers: new numerical-relativity simulations and multipolar effective-one-body model with spin precession and eccentricity On accretion disks formed in MHD simulations of black hole-neutron star mergers with accurate microphysics
Reference 36
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation ff5ac6eb-0efc-4b9f-9b7f-793f432eeec9 · inbound
Effects of magnetically driven shocks on nucleosynthesis and kilonovae from neutron star mergers On accretion disks formed in MHD simulations of black hole-neutron star mergers with accurate microphysics
Reference 26
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.
Observation a712a4e7-3d66-4f1e-90da-82c42ceb365b · inbound
Black hole-neutron star binaries with high spins and large mass asymmetries: III. Properties of the ejected material and its electromagnetic signatures On accretion disks formed in MHD simulations of black hole-neutron star mergers with accurate microphysics
Reference 54
Source-reported events for the cited work
Unavailable: canonical work link unavailable.