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Paper Citation Record · LEDGER

Orbital migration of low-mass planets in evolutionary radiative models: Avoiding catastrophic infall

As of 12 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1003.0925.

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

pith.paper-citation-record.v1
1003.0925 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 2026-08-12T06:34:41.77262+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-01T13:29:14.422807Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-06-28T13:22:15.666830Z

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 b113f4b4-4b4d-4dc9-b006-f84d33b1c1bc · inbound

Accretion of Primordial Black Holes in Stellar Interiors cites this paper.

Accretion of Primordial Black Holes in Stellar Interiors Orbital migration of low-mass planets in evolutionary radiative models: Avoiding catastrophic infall

Reference 277

Resolution
verified exact
local_arxiv, observed 2026-06-28T13:22:15.668155Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:0e87dcc29893202f626604f5443d2fbc46366ffac1dadeb04b16cd7fb37bb4bd

Observation 591a3493-a8c7-40bd-8679-de9f2e1b82da · inbound

Dynamical formation of long-period exoplanets systems in evolving binary stars cites this paper.

Dynamical formation of long-period exoplanets systems in evolving binary stars Orbital migration of low-mass planets in evolutionary radiative models: Avoiding catastrophic infall

Reference 119

Resolution
unresolved
no resolver link, observed 2026-08-01T13:29:14.422807Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T13:29:14.422807Z digest=sha256:2238409629f15fe8c6be9abb36b8e9d7475cd669f6a737d8d1d0854951d9ca35