Paper Citation Record · LEDGER

Difficulties with Recovering The Masses of Supermassive Black Holes from Stellar Kinematical Data

As of 20 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:astro-ph/0210379.

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

pith.paper-citation-record.v1
astro-ph/0210379 v2

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 2026-08-20T06:33:59.587034+00:00

measured 4 of 4 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-15T23:46:51.552980Z

measured 1 of 1 external citation measurements

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

Source: pith, observed 2026-08-05T02:28:24.338817Z

Reference resolution

0 of 0 outbound references displayed

verified exact0
verified fuzzy0
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External citation measurements

192
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation bf53624a-958b-460d-90eb-089ef9099322 · inbound

Relativistic structure of a supermassive black hole embedded in the dark matter halo of NGC 4649 (M60) cites this paper.

Relativistic structure of a supermassive black hole embedded in the dark matter halo of NGC 4649 (M60) Difficulties with Recovering The Masses of Supermassive Black Holes from Stellar Kinematical Data

Reference 21

Resolution: unresolved; no resolver link, observed 2026-08-15T23:46:51.552980Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 31beb02e-f16c-4aa2-840d-0a2d966b82b4 · inbound

Predicting intermediate-mass black hole formation in star clusters with machine learning cites this paper.

Predicting intermediate-mass black hole formation in star clusters with machine learning Difficulties with Recovering The Masses of Supermassive Black Holes from Stellar Kinematical Data

Reference 114

Resolution: verified exact; local_arxiv, observed 2026-05-22T09:21:21.038360Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

Observation 663e69ac-a584-4d40-9356-21f98f809afd · inbound

Constraints on Schwarzschild Black Hole in a Generalized Dehnen-Type $(1,4,\gamma)$ Dark Matter Halo via the S2 Star Orbit around Sgr A$^\star$ cites this paper.

Constraints on Schwarzschild Black Hole in a Generalized Dehnen-Type $(1,4,\gamma)$ Dark Matter Halo via the S2 Star Orbit around Sgr A$^\star$ Difficulties with Recovering The Masses of Supermassive Black Holes from Stellar Kinematical Data

Reference 20

Resolution: verified exact; local_arxiv, observed 2026-05-22T05:44:39.137754Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

Observation 8523e336-590f-4a7e-b65c-9edf51e58b30 · inbound

SchwarMAX: a GPU-friendly Schwarzschild orbit-superposition modelling framework cites this paper.

SchwarMAX: a GPU-friendly Schwarzschild orbit-superposition modelling framework Difficulties with Recovering The Masses of Supermassive Black Holes from Stellar Kinematical Data

Reference 38

Resolution: verified exact; local_arxiv, observed 2026-07-02T18:07:15.419760Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.