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Paper Citation Record · LEDGER

The impact of mass segregation and star-formation on the rates of gravitational-wave sources from extreme mass ratio inspirals

As of 18 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1609.01715.

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

pith.paper-citation-record.v1
1609.01715 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 2026-08-18T06:34:40.430872+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-15T19:19:59.175035Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-02T23:47:27.917685Z

Reference resolution

0 of 0 outbound references displayed

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  • verified fuzzy0
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  • malformed identifier0
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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 265a9abb-f506-4888-a1ea-d2bdcbdd6f9a · inbound

Time-frequency Imprints of Extreme Mass-Ratio Inspirals in Confusion Gravitational Wave Background cites this paper.

Time-frequency Imprints of Extreme Mass-Ratio Inspirals in Confusion Gravitational Wave Background The impact of mass segregation and star-formation on the rates of gravitational-wave sources from extreme mass ratio inspirals

Reference 4

Resolution
unresolved
no resolver link, observed 2026-08-15T19:19:59.175035Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-15T19:19:59.175035Z digest=sha256:b14a2d37e86409bd1c02788ce568057c151823be1b87237d80431d7997d135a2

Observation d84e10e3-91a5-483f-9683-15a6491db284 · inbound

Thermal emission from dark matter-heated neutron stars in the Galactic Center cites this paper.

Thermal emission from dark matter-heated neutron stars in the Galactic Center The impact of mass segregation and star-formation on the rates of gravitational-wave sources from extreme mass ratio inspirals

Reference 27

Resolution
verified exact
local_arxiv, observed 2026-07-02T23:47:27.918964Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=pdf_text observed=2026-06-27T17:53:29.423458Z digest=sha256:1654e742b742aae8663e72f66597f1cc8ec9881fa1e762b9070781e251d57f4d