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Paper Citation Record · LEDGER

Planet Engulfment Detections are Rare According to Observations and Stellar Modeling

As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:2210.12121.

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

pith.paper-citation-record.v1
2210.12121 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 4 of 4 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-11T06:34:44.6726+00:00

measured 4 of 4 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-05T10:57:04.578901Z

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

30
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 3baaad49-029a-4fbd-8343-2b0cdb3ac2d5 · inbound

Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations cites this paper.

Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations Planet Engulfment Detections are Rare According to Observations and Stellar Modeling

Reference 22

Resolution
unresolved
no resolver link, observed 2026-08-05T10:57:04.578901Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-05T10:57:04.578901Z digest=sha256:15eafeaac6e108b818fb117467ff3c5c1cfe45654b2dbf998b4fbb40b8e8fef0

Observation f5acae04-6940-4dec-b543-01369cc56557 · 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 Planet Engulfment Detections are Rare According to Observations and Stellar Modeling

Reference 31

Resolution
verified exact
local_arxiv, observed 2026-07-11T05:47:50.186245Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

source=arxiv_source observed=2026-07-11T05:42:50.878434Z digest=sha256:fab2044159c6016bc3fed20f4f80d407c78da817b70b6ccaa1191941ccac3cc8

Observation f16a32a6-4fca-4047-bb2f-6768a14eb1d0 · inbound

The GAPS Programme with HARPS-N at TNG LXXVII. Occurrence rates of small close-in planets in the presence of cold Jupiters cites this paper.

The GAPS Programme with HARPS-N at TNG LXXVII. Occurrence rates of small close-in planets in the presence of cold Jupiters Planet Engulfment Detections are Rare According to Observations and Stellar Modeling

Reference 173

Resolution
unresolved
no resolver link, observed 2026-07-13T03:54:36.358098Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-13T03:54:36.358098Z digest=sha256:739d322b02499ae9fe0f1d21ac9bcb11fc2e3643328f5e88338fa9bb4cd05a5e

Observation 4318be65-8a0c-434b-a402-72d1a3e659ec · inbound

The GAPS Programme with HARPS-N at TNG LXXVII. Occurrence rates of small close-in planets in the presence of cold Jupiters cites this paper.

The GAPS Programme with HARPS-N at TNG LXXVII. Occurrence rates of small close-in planets in the presence of cold Jupiters Planet Engulfment Detections are Rare According to Observations and Stellar Modeling

Reference 173

Resolution
unresolved
no resolver link, observed 2026-07-14T15:15:28.911413Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-14T15:15:28.911413Z digest=sha256:9f25e8f3349bcd1322d2aa158a3f2a031a320316a8dd1ea21e7faac465bf2154