Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Constraining properties of asymmetric dark matter candidates from gravitational-wave observations
As of 7 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 6 inbound Pith citation observations for arXiv:2210.15739.
A citation records a reference. It does not transfer a finding from one paper to another.
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One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-07T06:34:17.273281+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-06T19:18:33.541661Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-05-24T08:54:15.189327Z
Reference resolution
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External citation measurements
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Outbound references
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Pith citing papers
Observation 0cdb7ce5-9ea0-41eb-9e54-a6d0b0561f41 · inbound
Worldline effective field theory of inspiralling black hole binaries in presence of dark photon and axionic dark matter cites this paper.
Worldline effective field theory of inspiralling black hole binaries in presence of dark photon and axionic dark matter Constraining properties of asymmetric dark matter candidates from gravitational-wave observations
Reference 148
- Resolution
- verified exact
- arxiv_id, observed 2026-05-24T08:54:15.192212Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation a4074b35-0f55-472a-bbea-e417842e156e · inbound
Can Orbital Decay of Accreting Binary Pulsars Probe Dark Matter? cites this paper.
Can Orbital Decay of Accreting Binary Pulsars Probe Dark Matter? Constraining properties of asymmetric dark matter candidates from gravitational-wave observations
Reference 33
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T19:18:33.541661Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 3cc7cdb6-66d1-4488-b6b4-918370de961e · inbound
A case study of GW190425 for classifying binary neutron star versus binary black hole mergers and constraining asymmetric dark matter with gravitational wave detectors cites this paper.
A case study of GW190425 for classifying binary neutron star versus binary black hole mergers and constraining asymmetric dark matter with gravitational wave detectors Constraining properties of asymmetric dark matter candidates from gravitational-wave observations
Reference 33
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T18:39:46.131744Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation df618dad-d7f1-49d9-9d74-b5a7c004f878 · inbound
Effect of Dark matter and $\sigma$-cut potential on radial and non-radial oscillation modes in neutron stars cites this paper.
Effect of Dark matter and $\sigma$-cut potential on radial and non-radial oscillation modes in neutron stars Constraining properties of asymmetric dark matter candidates from gravitational-wave observations
Reference 51
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T16:35:42.510840Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 3f794875-2a6a-46bd-817c-76e1e82586b5 · 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 Constraining properties of asymmetric dark matter candidates from gravitational-wave observations
Reference 47
- Resolution
- verified exact
- arxiv_id, observed 2026-05-19T03:47:02.350012Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation 926640d1-2d71-461b-b5d2-a1a573f538b6 · inbound
Implications for Pulsar Timing Arrays of Sub-solar Black Hole Detections: From LVK to Einstein Telescope and Cosmic Explorer cites this paper.
Implications for Pulsar Timing Arrays of Sub-solar Black Hole Detections: From LVK to Einstein Telescope and Cosmic Explorer Constraining properties of asymmetric dark matter candidates from gravitational-wave observations
Reference 121
- Resolution
- unresolved
- no resolver link, observed 2026-08-05T15:54:19.710924Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.