Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Subtraction of the confusion foreground and parameter uncertainty of resolvable galactic binaries on the networks of space-based gravitational-wave detectors
As of 13 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2307.05568.
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 2026-08-13T06:32:02.005865+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-12T20:55:58.169391Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-07-03T15:08:32.997482Z
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 c5c284fb-8bbf-44e1-92cd-c3e82d4bcfb4 · inbound
Constraining the Galactic Structure using Time Domain Gravitational Wave Signal from Double White Dwarfs Detected by Space Gravitational Wave Detectors cites this paper.
Constraining the Galactic Structure using Time Domain Gravitational Wave Signal from Double White Dwarfs Detected by Space Gravitational Wave Detectors Subtraction of the confusion foreground and parameter uncertainty of resolvable galactic binaries on the networks of space-based gravitational-wave detectors
Reference 64
- Resolution
- unresolved
- no resolver link, observed 2026-08-12T20:55:58.169391Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation c3925e5d-f491-4db6-95b2-187fb825f239 · inbound
Constraining Kerr supermassive black hole properties using gravitational waves from inspiraling stellar-mass binary black holes cites this paper.
Constraining Kerr supermassive black hole properties using gravitational waves from inspiraling stellar-mass binary black holes Subtraction of the confusion foreground and parameter uncertainty of resolvable galactic binaries on the networks of space-based gravitational-wave detectors
Reference 70
- Resolution
- verified exact
- arxiv_id, observed 2026-07-03T15:08:32.998761Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.