Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Celestial Objects as Strongly-Interacting Non-Annihilating Dark Matter Detectors
As of 14 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:2301.03625.
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 2026-08-14T06:32:32.682623+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-12T19:44:24.126382Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-07-02T00:06:25.001990Z
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 a5e0e530-9927-4056-bde4-6fa079e4c205 · inbound
Radiation Exposure from the Dark cites this paper.
Radiation Exposure from the Dark Celestial Objects as Strongly-Interacting Non-Annihilating Dark Matter Detectors
Reference 18
- Resolution
- unresolved
- no resolver link, observed 2026-08-12T19:44:24.126382Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 514c0734-b407-4f4f-b915-7d76ea2a8f27 · inbound
Gravitational Waves as a Probe of Particle Dark Matter cites this paper.
Gravitational Waves as a Probe of Particle Dark Matter Celestial Objects as Strongly-Interacting Non-Annihilating Dark Matter Detectors
Reference 14
- Resolution
- unresolved
- no resolver link, observed 2026-08-11T23:35:29.749324Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 955a4740-43b4-446f-adc0-f14dc372435c · inbound
Can Orbital Decay of Accreting Binary Pulsars Probe Dark Matter? cites this paper.
Can Orbital Decay of Accreting Binary Pulsars Probe Dark Matter? Celestial Objects as Strongly-Interacting Non-Annihilating Dark Matter Detectors
Reference 56
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T19:18:36.269461Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 35df84b0-3971-4735-9377-6cccd9c6d066 · 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 Celestial Objects as Strongly-Interacting Non-Annihilating Dark Matter Detectors
Reference 29
- Resolution
- verified exact
- arxiv_id, observed 2026-05-19T03:47:02.009744Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.
Observation 615d675e-6a83-4fb4-8726-30bbe02cfd93 · inbound
New Windows on Heavy Dark Matter: Mineral Melt Modelling and X-Ray Readout for Muscovite Mica cites this paper.
New Windows on Heavy Dark Matter: Mineral Melt Modelling and X-Ray Readout for Muscovite Mica Celestial Objects as Strongly-Interacting Non-Annihilating Dark Matter Detectors
Reference 77
- Resolution
- verified exact
- arxiv_id, observed 2026-07-02T00:06:25.004177Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.