Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Late-time Evolution of Composite Supernova Remnants: Deep Chandra Observations and Hydrodynamical Modeling of a Crushed Pulsar Wind Nebula in SNR G327.1-1.1
As of 3 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1506.03069.
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 2026-08-03T06:30:56.289259+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-03T15:48:47.371272Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-07-02T20:37:21.961243Z
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 fff08645-5630-4056-b425-b0c5bfb3affa · inbound
Self-confinement of relativistic pair beams in magnetized interstellar plasmas: the case of pulsar X-ray filaments cites this paper.
Self-confinement of relativistic pair beams in magnetized interstellar plasmas: the case of pulsar X-ray filaments Late-time Evolution of Composite Supernova Remnants: Deep Chandra Observations and Hydrodynamical Modeling of a Crushed Pulsar Wind Nebula in SNR G327.1-1.1
Reference 3
- Resolution
- unresolved
- no resolver link, observed 2026-08-03T15:48:47.371272Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 78cfc287-8902-4295-b0a0-fb3346be556d · inbound
Understanding Pulsar Wind Nebulae with the SKA cites this paper.
Understanding Pulsar Wind Nebulae with the SKA Late-time Evolution of Composite Supernova Remnants: Deep Chandra Observations and Hydrodynamical Modeling of a Crushed Pulsar Wind Nebula in SNR G327.1-1.1
Reference 139
- Resolution
- verified exact
- local_arxiv, observed 2026-07-02T20:37:21.962559Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-03T06:30:56.289259+00:00.