Pith. sign in

Paper Citation Record · LEDGER

Brownian motion of supermassive black holes in galaxy cores

As of 6 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1908.04283.

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

pith.paper-citation-record.v1
1908.04283 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 2 of 2 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-06T06:34:29.942622+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-04T00:54:10.165702Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-11T15:51:45.112337Z

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 084e5362-023d-47a6-b6ba-d49c82b86692 · inbound

Self-acceleration of Hardening Binaries cites this paper.

Self-acceleration of Hardening Binaries Brownian motion of supermassive black holes in galaxy cores

Reference 42

Resolution
verified exact
arxiv_id, observed 2026-05-11T15:51:45.117034Z

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.

source=pdf_text observed=2026-05-09T19:04:20.072429Z digest=sha256:53ed4ea10693d95936e5cede6c17e57fbc4777d725d0d35b7ed512c8545e86c5

Observation 4dfa9ad9-c92d-44be-980c-5399ddfa26af · inbound

On an empirical method to build near-equilibrium axisymmetric and triaxial galaxy models cites this paper.

On an empirical method to build near-equilibrium axisymmetric and triaxial galaxy models Brownian motion of supermassive black holes in galaxy cores

Reference 65

Resolution
unresolved
no resolver link, observed 2026-08-04T00:54:10.165702Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-04T00:54:10.165702Z digest=sha256:f493528c3af0e7dc76d8bf2c70f9c656b16191e0fcc263cd97baba5c6ccd421a