Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
The MPIfR-MeerKAT Galactic Plane survey I -- System setup and early results
As of 21 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:2303.09231.
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 2026-08-21T06:32:19.484+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-15T14:41:13.810627Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-07-11T08:37:53.917139Z
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 084a7ff4-3bea-4e30-b750-2a387b267de1 · inbound
Fastest spinning millisecond pulsars: indicators for quark matter in neutron stars? cites this paper.
Fastest spinning millisecond pulsars: indicators for quark matter in neutron stars? The MPIfR-MeerKAT Galactic Plane survey I -- System setup and early results
Reference 104
- Resolution
- malformed identifier
- no resolver link, observed 2026-08-11T18:36:55.325170Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 67d76282-d824-403c-8f62-2ac523e4e5b4 · inbound
Rapidly Spinning Massive Pulsars as an Indicator of Quark Deconfinement cites this paper.
Rapidly Spinning Massive Pulsars as an Indicator of Quark Deconfinement The MPIfR-MeerKAT Galactic Plane survey I -- System setup and early results
Reference 26
- Resolution
- unresolved
- no resolver link, observed 2026-08-03T17:54:36.593197Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 472f142b-2650-42f2-a4ad-f0e089a5d78a · inbound
Commensal image plane transient search methods with the SKAO cites this paper.
Commensal image plane transient search methods with the SKAO The MPIfR-MeerKAT Galactic Plane survey I -- System setup and early results
Reference 53
- Resolution
- verified exact
- local_arxiv, observed 2026-07-11T08:37:53.921680Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.
Observation c2eef142-7efa-494c-ae27-8a3d80bcacf0 · inbound
Why do massive stars form bow shocks? Bulk ISM motion as the main driver of bow shock formation and geometry cites this paper.
Why do massive stars form bow shocks? Bulk ISM motion as the main driver of bow shock formation and geometry The MPIfR-MeerKAT Galactic Plane survey I -- System setup and early results
Reference 174
- Resolution
- unresolved
- no resolver link, observed 2026-08-07T20:40:57.473952Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 2dc9f673-ba05-453c-a056-620d1b43d9c1 · inbound
Why do massive stars form bow shocks? Bulk ISM motion as the main driver of bow shock formation and geometry cites this paper.
Why do massive stars form bow shocks? Bulk ISM motion as the main driver of bow shock formation and geometry The MPIfR-MeerKAT Galactic Plane survey I -- System setup and early results
Reference 174
- Resolution
- unresolved
- no resolver link, observed 2026-08-15T14:41:13.810627Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.