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Paper Citation Record · LEDGER

Hot Jupiters and Cool Stars

As of 17 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1407.7879.

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

pith.paper-citation-record.v1
1407.7879 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 2026-08-17T06:30:58.91139+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-07-11T11:50:26.030339Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-06-28T03:41:34.618904Z

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 f275660d-660c-4140-8335-728a59b26947 · inbound

TOI-3664 b, TOI-4034 b & TOI-6564 b: Three new hot Jupiters around stars approaching the terminal age main sequence cites this paper.

TOI-3664 b, TOI-4034 b & TOI-6564 b: Three new hot Jupiters around stars approaching the terminal age main sequence Hot Jupiters and Cool Stars

Reference 116

Resolution
verified exact
local_arxiv, observed 2026-06-28T03:41:34.620178Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:2bb716d5f93873078b9dec569137276546ec0caf0ee2f9fbf6f7bce7db57e0d0

Observation 883e68f5-5d59-4f8f-a5df-a86e1ad2c1c3 · inbound

Dynamical constraints on planet engulfment as the origin of lithium enhancement in TOI-5882 cites this paper.

Dynamical constraints on planet engulfment as the origin of lithium enhancement in TOI-5882 Hot Jupiters and Cool Stars

Reference 24

Resolution
unresolved
no resolver link, observed 2026-07-11T05:42:50.878434Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-11T05:42:50.878434Z digest=sha256:b3eca1319d618fa3db2cb0983eb1838bea125746a171b823045f8a1c853ccd00