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Paper Citation Record · LEDGER

Extreme mass ratio inspiral rates: dependence on the massive black hole mass

As of 22 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:0901.1667.

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

pith.paper-citation-record.v1
0901.1667 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 2026-08-21T06:32:19.484+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-01T00:50:16.340461Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-05-13T22:38:38.728030Z

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 865f38fe-e39c-4c0f-8d25-cad824bd932a · inbound

String Axiverse cites this paper.

String Axiverse Extreme mass ratio inspiral rates: dependence on the massive black hole mass

Reference 69

Resolution
verified exact
local_arxiv, observed 2026-05-13T22:38:38.730545Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

source=pdf_text observed=2026-05-13T22:38:38.367037Z digest=sha256:27f5bd143384eb6ff4cf42f3932f44b2698d834314d5c180d13b27b50ed76816

Observation 0d4b30e8-6f68-45f5-8cf6-8d2bcc888c04 · inbound

From S2 to LISA: Astrometric Bounds on Extreme-Mass-Ratio Inspirals and Bursts cites this paper.

From S2 to LISA: Astrometric Bounds on Extreme-Mass-Ratio Inspirals and Bursts Extreme mass ratio inspiral rates: dependence on the massive black hole mass

Reference 38

Resolution
unresolved
no resolver link, observed 2026-08-01T00:50:16.340461Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T00:50:16.340461Z digest=sha256:896f7416acf3d73a73ae5a2e049193678d72f1f8262d2ad9b4dd7bdcb6e0909e