Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
MeerKAT discovers a jet-driven bow shock near GRS 1915+105. How an invisible large-scale jet sculpts a microquasar's environment
As of 16 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2504.17425.
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 2026-08-15T06:32:42.880941+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-15T14:41:13.190763Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-07-08T13:54:58.452987Z
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 df966ebd-1dfd-4947-bd56-7ba38227c9da · inbound
An intrinsic decline of accretion activity in GRS 1915+105 cites this paper.
An intrinsic decline of accretion activity in GRS 1915+105 MeerKAT discovers a jet-driven bow shock near GRS 1915+105. How an invisible large-scale jet sculpts a microquasar's environment
Reference 78
- Resolution
- verified exact
- local_arxiv, observed 2026-07-08T13:54:58.454348Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.
Observation 529e50c4-4d97-4d1c-9e9a-4783bb555b5e · 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 MeerKAT discovers a jet-driven bow shock near GRS 1915+105. How an invisible large-scale jet sculpts a microquasar's environment
Reference 57
- Resolution
- unresolved
- no resolver link, observed 2026-08-07T20:40:57.031205Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 138b16b2-869d-4498-a910-4eaedb8cc35f · 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 MeerKAT discovers a jet-driven bow shock near GRS 1915+105. How an invisible large-scale jet sculpts a microquasar's environment
Reference 57
- Resolution
- unresolved
- no resolver link, observed 2026-08-15T14:41:13.190763Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.