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Paper Citation Record · LEDGER

Star-Planet Interactions in the Radio Domain: Prospect for Their Detection

As of 18 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2409.16038.

A citation records a reference. It does not transfer a finding from one paper to another.

pith.paper-citation-record.v1
2409.16038 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 2 of 2 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-18T06:34:40.430872+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-12T11:55:11.483504Z

measured 0 of 1 external citation measurements

A source-named dated measurement, never combined with another source.

Source: pith, observed 2026-08-05T14:49:34.692219Z

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 4ab7fbf2-149f-4829-b0e0-a8c27143eab2 · inbound

Searching for star-planet interactions in GJ 486 at radio wavelengths with the uGMRT cites this paper.

Searching for star-planet interactions in GJ 486 at radio wavelengths with the uGMRT Star-Planet Interactions in the Radio Domain: Prospect for Their Detection

Reference 53

Resolution
unresolved
no resolver link, observed 2026-08-12T11:55:11.483504Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-12T11:55:11.483504Z digest=sha256:a90d3651ada7db62e80045102ca2e57b951ddc08e67ccb76dc645b6ed9ccb7ed

Observation 5e35ade9-76d0-4a76-9de6-19d49123599b · inbound

Modelling magnetic star-planet interaction in the iconic M dwarfs Proxima Centauri, YZ Ceti and GJ 1151 cites this paper.

Modelling magnetic star-planet interaction in the iconic M dwarfs Proxima Centauri, YZ Ceti and GJ 1151 Star-Planet Interactions in the Radio Domain: Prospect for Their Detection

Reference 48

Resolution
verified exact
local_arxiv, observed 2026-08-05T14:49:34.699379Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=arxiv_source observed=2026-08-05T14:49:33.533166Z digest=sha256:853b6eb282fcfd0a0ad5e05320b1454803365224b0247afe746a4451d2be284b