Pith. sign in

Paper Citation Record · LEDGER

Jet launching from binary black hole-neutron star mergers: Dependence on black hole spin, binary mass ratio and magnetic field orientation

As of 15 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:1810.08618.

A citation records a reference. It does not transfer a finding from one paper to another.

pith.paper-citation-record.v1
1810.08618 v3

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 4 of 4 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-15T06:32:42.880941+00:00

measured 4 of 4 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-14T11:35:56.332477Z

measured 0 of 1 external citation measurements

A source-named dated measurement, never combined with another source.

Source: arxiv_reference, observed 2026-05-09T04:41:38.308626Z

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 90cfb055-6fb5-4c9f-b9b4-7839ae6da9f8 · inbound

Electromagnetic counterparts of black hole-neutron star mergers: dependence on the neutron star properties cites this paper.

Electromagnetic counterparts of black hole-neutron star mergers: dependence on the neutron star properties Jet launching from binary black hole-neutron star mergers: Dependence on black hole spin, binary mass ratio and magnetic field orientation

Reference 69

Resolution
unresolved
no resolver link, observed 2026-08-14T11:35:56.332477Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T11:35:56.332477Z digest=sha256:ebcd265076806ddf2c122921cf50d68056cfd6ddf63e2570ee5bbf27fa3830fa

Observation 7a231ea6-7aca-4dc0-9233-b3c2034aaec4 · inbound

General-relativistic resistive-magnetohydrodynamics simulations of self-consistent magnetized rotating neutron stars cites this paper.

General-relativistic resistive-magnetohydrodynamics simulations of self-consistent magnetized rotating neutron stars Jet launching from binary black hole-neutron star mergers: Dependence on black hole spin, binary mass ratio and magnetic field orientation

Reference 62

Resolution
verified exact
arxiv_id, observed 2026-07-04T23:17:41.562416Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

source=pdf_text observed=2026-05-23T20:56:06.983493Z digest=sha256:e3747477b89a2c6e9b9a67611a04d805af28954c16e9e845da768b5454142fe7

Observation 4111bc96-ef4e-46b8-ab2b-a79756ed9436 · inbound

Impact of rotation on magnetic field stability and orientation in isolated neutron stars cites this paper.

Impact of rotation on magnetic field stability and orientation in isolated neutron stars Jet launching from binary black hole-neutron star mergers: Dependence on black hole spin, binary mass ratio and magnetic field orientation

Reference 59

Resolution
unresolved
no resolver link, observed 2026-08-05T15:20:07.331790Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-05T15:20:07.331790Z digest=sha256:183d68763a6dcbd5c6b307094a4aac37a78056a82cd180fb475430b20f52bd42

Observation dea222b9-49d1-42f0-b678-9c667a1c7572 · 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 Jet launching from binary black hole-neutron star mergers: Dependence on black hole spin, binary mass ratio and magnetic field orientation

Reference 53

Resolution
unresolved
no resolver link, observed 2026-08-01T09:55:41.816164Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T09:55:41.816164Z digest=sha256:3ca6edeadafe2101867e7a1a028991876ec9958c3fb4e211745a272c5551e311