Pith. sign in

Paper Citation Record · LEDGER

Massive Black Hole Binaries from Collisional Runaways

As of 8 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:astro-ph/0512642.

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

pith.paper-citation-record.v1
astro-ph/0512642 v2

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 2026-08-08T06:32:00.761636+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-06T18:35:57.618345Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-11T06:57:50.317396Z

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 d405a665-df99-482a-ab87-27e535fc3362 · inbound

Detecting Intermediate-mass Black Holes Using Miniature Pulsar Timing Arrays in Globular Clusters cites this paper.

Detecting Intermediate-mass Black Holes Using Miniature Pulsar Timing Arrays in Globular Clusters Massive Black Hole Binaries from Collisional Runaways

Reference 34

Resolution
unresolved
no resolver link, observed 2026-08-06T18:35:57.618345Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T18:35:57.618345Z digest=sha256:112e4c4f489264de72b79269a9205897ccdcf15b618fb1780a87b3477191e956

Observation d2e49a2e-bafe-41e3-a33f-14ab23b80986 · inbound

Formation of rotating supergiants via stellar mergers in dense clusters: Implications for black hole natal spins cites this paper.

Formation of rotating supergiants via stellar mergers in dense clusters: Implications for black hole natal spins Massive Black Hole Binaries from Collisional Runaways

Reference 87

Resolution
verified exact
local_arxiv, observed 2026-07-11T06:57:50.319619Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

source=arxiv_source observed=2026-07-11T06:51:42.465920Z digest=sha256:ff7900e244e96828447ed890c371f77fbbcdd0dbb114fefbfd0a6a8d21731a2c