Paper Citation Record · LEDGER

Extrasolar Carbon Planets

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/0504214.

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

pith.paper-citation-record.v1
astro-ph/0504214 v2

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 2026-08-14T10:51:33.823809Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-11T00:25:50.081573Z

Reference resolution

0 of 0 outbound references displayed

verified exact0
verified fuzzy0
unresolved0
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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 0b7272e4-d2a3-4f23-bee8-77b7f8a98369 · inbound

Carbon, oxygen, and iron abundances in disk and halo stars. Implications of 3D non-LTE spectral line formation cites this paper.

Carbon, oxygen, and iron abundances in disk and halo stars. Implications of 3D non-LTE spectral line formation Extrasolar Carbon Planets

Reference 68

Resolution: unresolved; no resolver link, observed 2026-08-14T10:51:33.823809Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 8863be8f-8185-4850-b8d0-881f983203a1 · inbound

Chemical Abundances Shape History (CASH). I. A Link between Giant Planets Orbital Periods and Host Stellar C/O Ratios cites this paper.

Chemical Abundances Shape History (CASH). I. A Link between Giant Planets Orbital Periods and Host Stellar C/O Ratios Extrasolar Carbon Planets

Reference 23

Resolution: verified exact; arxiv_id, observed 2026-05-13T17:50:46.173256Z

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 0ac961c4-5a72-4931-9423-b7dda876e51a · inbound

Host--Non-host Differences in Stellar Chemistry, Activity, and Birth Radius: Hints of Distinct Formation Environments for Earth-like Planets and Sub-Neptunes cites this paper.

Host--Non-host Differences in Stellar Chemistry, Activity, and Birth Radius: Hints of Distinct Formation Environments for Earth-like Planets and Sub-Neptunes Extrasolar Carbon Planets

Reference 39

Resolution: unresolved; no resolver link, observed 2026-08-10T10:16:18.615570Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.