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Paper Citation Record · LEDGER

Shallower radius valley around low-mass hosts: Evidence for icy planets, collisions or high-energy radiation scatter

As of 8 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2401.12378.

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

pith.paper-citation-record.v1
2401.12378 v2

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 2026-08-08T06:32:00.761636+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-07T19:09:57.775357Z

measured 1 of 1 external citation measurements

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

Source: arxiv_reference, 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

3
arxiv_reference, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 2a240ef4-1b67-4ff7-9a15-49c97d227228 · inbound

A primordial radius valley as a consequence of planet formation cites this paper.

A primordial radius valley as a consequence of planet formation Shallower radius valley around low-mass hosts: Evidence for icy planets, collisions or high-energy radiation scatter

Reference 45

Resolution
unresolved
no resolver link, observed 2026-08-07T19:09:57.775357Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T19:09:57.775357Z digest=sha256:e33e16742d55aa6be4f98cd5e56bfca2bfeafd900eb074bae01065a7de61b14d

Observation d58152df-8c8b-47f1-9f12-db7124fe2b06 · inbound

Testing the prevalence of hydrogen-silicate miscibility in young sub-Neptunes cites this paper.

Testing the prevalence of hydrogen-silicate miscibility in young sub-Neptunes Shallower radius valley around low-mass hosts: Evidence for icy planets, collisions or high-energy radiation scatter

Reference 23

Resolution
verified exact
arxiv_id, observed 2026-06-30T03:14:14.222963Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

source=pdf_text observed=2026-06-30T03:09:46.398341Z digest=sha256:b5563e8b1111384d5a94756eca63380f278fef2ee90dc0009eb5bedd4818de3e