Paper Citation Record · LEDGER

Can Planets survive Stellar Evolution?

As of 20 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:astro-ph/0702724.

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

pith.paper-citation-record.v1
astro-ph/0702724 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 3 of 3 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-20T06:33:59.587034+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-01T13:29:20.983151Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-06-28T12:42:09.284595Z

Reference resolution

0 of 0 outbound references displayed

verified exact0
verified fuzzy0
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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 b4e4ebb6-6aa3-4c5c-9cd6-516c20c9c5a0 · inbound

Size limits on tidal debris around white dwarfs: the km-size barrier cites this paper.

Size limits on tidal debris around white dwarfs: the km-size barrier Can Planets survive Stellar Evolution?

Reference 177

Resolution: verified exact; local_arxiv, observed 2026-06-28T12:42:09.285913Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

Observation f88f9d09-1c95-4ddb-b2f7-45b707c9037d · 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 Can Planets survive Stellar Evolution?

Reference 6

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

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c4d25e3c-1e1e-40d7-8984-533dc65f0c6a · 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 Can Planets survive Stellar Evolution?

Reference 186

Resolution: unresolved; no resolver link, observed 2026-08-01T13:29:20.983151Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.