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Paper Citation Record · LEDGER

One of the closest exoplanet pairs to the 3:2 Mean Motion Resonance: K2-19b \& c

As of 23 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1503.00692.

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

pith.paper-citation-record.v1
1503.00692 v4

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 2026-08-23T06:30:58.430688+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-14T15:12:01.434291Z

measured 1 of 1 external citation measurements

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

Source: pith, observed 2026-08-05T02:28:24.338817Z

Reference resolution

0 of 0 outbound references displayed

  • verified exact0
  • verified fuzzy0
  • unresolved0
  • parse uncertain0
  • malformed identifier0
  • metadata mismatch0

External citation measurements

48
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation adf85e49-4025-4dc1-b90e-2c27382572d7 · inbound

Recurrence Network Analysis of Exoplanetary Observables cites this paper.

Recurrence Network Analysis of Exoplanetary Observables One of the closest exoplanet pairs to the 3:2 Mean Motion Resonance: K2-19b \& c

Reference 6

Resolution
unresolved
no resolver link, observed 2026-08-14T15:12:01.434291Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T15:12:01.434291Z digest=sha256:38b3360a3644f4dfe61f8adf68ab5341459791427362568e2e0e2664920be267

Observation 414fa602-9e1b-4c7b-9a57-116954bb593e · inbound

HD 148797: A bright F-type star with two moderate-period low-density sub-Jovian planets. Compact multi-planet architectures are common in the Neptunian savanna cites this paper.

HD 148797: A bright F-type star with two moderate-period low-density sub-Jovian planets. Compact multi-planet architectures are common in the Neptunian savanna One of the closest exoplanet pairs to the 3:2 Mean Motion Resonance: K2-19b \& c

Reference 12

Resolution
verified exact
local_arxiv, observed 2026-07-13T01:29:15.551875Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

source=arxiv_source observed=2026-07-13T01:25:33.763066Z digest=sha256:f96d0f58567d21267047e687a55b62a9e05d396e4027d185c29cb566f842d974