Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Binary compact object coalescence rates: The role of elliptical galaxies
As of 4 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:0908.3635.
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 2026-08-04T06:34:03.388597+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-07-11T11:50:26.030339Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-06-25T23:08:41.025771Z
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 59effed9-51d5-4567-94f2-9ec0b2cd3ad7 · inbound
Inferring the properties of a population of compact binaries in presence of selection effects cites this paper.
Inferring the properties of a population of compact binaries in presence of selection effects Binary compact object coalescence rates: The role of elliptical galaxies
Reference 75
- Resolution
- verified exact
- arxiv_id, observed 2026-05-09T04:54:56.110611Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.
Observation 992ae7e1-6286-47a8-b527-0a8abec5019e · inbound
Distinguishing Neutron Star vs. Low-Mass Black Hole Binaries with Late Inspiral & Postmerger Gravitational Waves $-$ Sensitivity to Transmuted Black Holes and Non-Annihilating Dark Matter cites this paper.
Distinguishing Neutron Star vs. Low-Mass Black Hole Binaries with Late Inspiral & Postmerger Gravitational Waves $-$ Sensitivity to Transmuted Black Holes and Non-Annihilating Dark Matter Binary compact object coalescence rates: The role of elliptical galaxies
Reference 115
- Resolution
- verified exact
- local_arxiv, observed 2026-05-19T03:47:02.283821Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.
Observation caded6d1-74dd-4713-84f8-bf52ec1c4615 · inbound
Using SKAO to Understand the Clustering of Gravitational Wave Sources cites this paper.
Using SKAO to Understand the Clustering of Gravitational Wave Sources Binary compact object coalescence rates: The role of elliptical galaxies
Reference 162
- Resolution
- verified exact
- local_arxiv, observed 2026-06-25T23:08:41.027188Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.