Pith. sign in

Paper Citation Record · LEDGER

Stellar Black Holes and Compact Stellar Remnants

As of 14 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2311.15778.

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

pith.paper-citation-record.v1
2311.15778 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 2026-08-14T06:32:32.682623+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-10T21:32:15.562912Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-08-10T18:16:17.926450Z

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 684e8aca-1243-4a28-9cb2-db26032b3b8d · inbound

Impact of accretion-induced chemically homogeneous evolution on stellar and compact binary populations cites this paper.

Impact of accretion-induced chemically homogeneous evolution on stellar and compact binary populations Stellar Black Holes and Compact Stellar Remnants

Reference 21

Resolution
unresolved
no resolver link, observed 2026-08-10T21:32:15.562912Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T21:32:15.562912Z digest=sha256:b804c2941e819001e451517d0a073c2f39dbd9ae9a2a423845fe05b7a9ef1431

Observation 32e86998-badd-4d75-ab4c-b343aae0c829 · inbound

A Possible Mass Ratio and Spin-Orbit Misalignment Correlation for Mergers of Binary Black Holes in Nuclear Star Clusters cites this paper.

A Possible Mass Ratio and Spin-Orbit Misalignment Correlation for Mergers of Binary Black Holes in Nuclear Star Clusters Stellar Black Holes and Compact Stellar Remnants

Reference 37

Resolution
metadata mismatch
local_arxiv, observed 2026-08-10T13:43:45.451570Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

source=pdf_text observed=2026-08-10T13:41:03.210723Z digest=sha256:e36a81973e95a8cb186c63c019d866f6dd5bdab25d40df56a2388fdee89dcdb9