Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Millisecond pulsars modelled as strange quark stars admixed with condensed dark matter
As of 17 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:1804.05023.
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 2026-08-17T06:30:58.91139+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-05T11:42:10.433982Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-07-09T23:36:37.357086Z
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 12678206-69bf-43e1-b5da-34c86f655a56 · inbound
Relativistic strange quark stars in Lovelock gravity cites this paper.
Relativistic strange quark stars in Lovelock gravity Millisecond pulsars modelled as strange quark stars admixed with condensed dark matter
Reference 52
- Resolution
- verified exact
- local_arxiv, observed 2026-05-25T02:25:15.272619Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.
Observation e8112ef1-0b51-46da-b5e2-c4d279882234 · inbound
Role of density profile of sub-GeV dark matter in the properties of dark matter admixed quark stars with Bayesian analysis of dark-NJL model cites this paper.
Role of density profile of sub-GeV dark matter in the properties of dark matter admixed quark stars with Bayesian analysis of dark-NJL model Millisecond pulsars modelled as strange quark stars admixed with condensed dark matter
Reference 39
- Resolution
- unresolved
- no resolver link, observed 2026-08-05T11:42:10.433982Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation e583ca35-5ba9-4911-907b-60e936afb769 · inbound
Slowly rotating condensate dark stars beyond the mean-field approximation cites this paper.
Slowly rotating condensate dark stars beyond the mean-field approximation Millisecond pulsars modelled as strange quark stars admixed with condensed dark matter
Reference 44
- Resolution
- verified exact
- local_arxiv, observed 2026-07-09T23:36:37.358285Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.