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Paper Citation Record · LEDGER

Where are the Intermediate Mass Black Holes?

As of 4 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:1903.08144.

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

pith.paper-citation-record.v1
1903.08144 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 3 of 3 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-03T06:30:56.289259+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-06-29T02:10:05.154016Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-10T06:15:00.866473Z

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 464966c0-6d3e-4f82-bf80-ec853f598d8b · inbound

Gravitational wave surrogate model for spinning, intermediate mass ratio binaries based on perturbation theory and numerical relativity cites this paper.

Gravitational wave surrogate model for spinning, intermediate mass ratio binaries based on perturbation theory and numerical relativity Where are the Intermediate Mass Black Holes?

Reference 28

Resolution
verified exact
local_arxiv, observed 2026-05-23T23:43:38.550585Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-03T06:30:56.289259+00:00.

source=pdf_text observed=2026-05-23T23:38:37.094812Z digest=sha256:6a8851faa7e4ccdde36aa39d03ad619be4413b014da5571ab6cf049617411f5e

Observation 0f86197f-55b6-4140-903c-c4a364c6ab1e · inbound

Dark Matter's influence on Evolution of MBHB in Dwarf Galaxies: A Case Study of Leo I dSph cites this paper.

Dark Matter's influence on Evolution of MBHB in Dwarf Galaxies: A Case Study of Leo I dSph Where are the Intermediate Mass Black Holes?

Reference 8

Resolution
verified exact
arxiv_id, observed 2026-05-10T15:30:32.599680Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-03T06:30:56.289259+00:00.

source=arxiv_source observed=2026-05-10T15:28:36.674948Z digest=sha256:732b02867a2fab5b1d63130e03caf7f4173aef1d57cf88625a0ab5d95e0309df

Observation a7369dab-4a7f-400f-a3f9-5c202118ab27 · inbound

Too shy to spin? Cosmic wallflowers as proto-globular clusters cites this paper.

Too shy to spin? Cosmic wallflowers as proto-globular clusters Where are the Intermediate Mass Black Holes?

Reference 295

Resolution
verified exact
local_arxiv, observed 2026-06-29T02:13:00.530751Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-03T06:30:56.289259+00:00.

source=arxiv_source observed=2026-06-29T02:10:05.154016Z digest=sha256:ccfefd8aef121198617ce6d01f47a29a913089fce8937e2eb9e3ad367d2b10f3