Pith. sign in

Paper Citation Record · LEDGER

Quantifying the Coexistence of Massive Black Holes and Dense Nuclear Star Clusters

As of 13 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:0907.5250.

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

pith.paper-citation-record.v1
0907.5250 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 2026-08-13T06:32:02.005865+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-07-01T04:45:13.319437Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-01T11:05:42.134126Z

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 dab222b8-0c37-415a-98fe-bfe8aa26c7df · inbound

N-body next-to-leading order gravitational spin-orbit interaction via effective field theory cites this paper.

N-body next-to-leading order gravitational spin-orbit interaction via effective field theory Quantifying the Coexistence of Massive Black Holes and Dense Nuclear Star Clusters

Reference 93

Resolution
verified exact
local_arxiv, observed 2026-05-15T03:03:57.064143Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.

source=pdf_text observed=2026-05-15T03:03:16.273348Z digest=sha256:b677c33c5eb679369ae491efcde773b3ae20be436b3c42a58ed649a6cb6e3555

Observation 880b94f8-2097-4f81-a220-7e4f38d1e7ea · inbound

Unveiling the properties of galaxy cores excavated by supermassive black hole binaries with SHARP cites this paper.

Unveiling the properties of galaxy cores excavated by supermassive black hole binaries with SHARP Quantifying the Coexistence of Massive Black Holes and Dense Nuclear Star Clusters

Reference 139

Resolution
metadata mismatch
local_arxiv, observed 2026-07-01T11:05:42.135538Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.

source=arxiv_source observed=2026-07-01T04:45:13.319437Z digest=sha256:cca618cba412c960a58c203c5f8c783f96756fbcd07761dae3a66e185a94647e