Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Measuring the star formation rate with gravitational waves from binary black holes
As of 6 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1808.00901.
A citation records a reference. It does not transfer a finding from one paper to another.
Coverage vector
One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-05T06:32:48.257954+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-06-28T09:07:09.699995Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-07-02T04:26:36.038774Z
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 1f1d7997-143f-4d62-aa13-f6d0824bbf7e · inbound
On the use of the Derivative Approximation for Likelihoods for Gravitational Wave Inference cites this paper.
On the use of the Derivative Approximation for Likelihoods for Gravitational Wave Inference Measuring the star formation rate with gravitational waves from binary black holes
Reference 42
- Resolution
- verified exact
- arxiv_id, observed 2026-05-18T06:35:59.726766Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.
Observation 8e4adffb-1169-4e9c-9d3f-361b798a07b9 · inbound
Targeting black holes from metal-poor progenitors with next-generation gravitational-wave detectors cites this paper.
Targeting black holes from metal-poor progenitors with next-generation gravitational-wave detectors Measuring the star formation rate with gravitational waves from binary black holes
Reference 95
- Resolution
- verified exact
- arxiv_id, observed 2026-07-02T04:26:36.040143Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.