Paper Citation Record · LEDGER

Chemical enrichment of giant planets and discs due to pebble drift

As of 19 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:1705.03305.

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

pith.paper-citation-record.v1
1705.03305 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 2026-08-19T06:32:44.657259+00:00

measured 4 of 4 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-11T21:00:08.544515Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-10T23:07:43.560525Z

Reference resolution

0 of 0 outbound references displayed

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verified fuzzy0
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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 5db6fa5f-e8ce-417a-be2b-ad475f2e453e · inbound

C/O ratios in self-gravitating protoplanetary discs with dust evolution cites this paper.

C/O ratios in self-gravitating protoplanetary discs with dust evolution Chemical enrichment of giant planets and discs due to pebble drift

Reference 2017

Resolution: unresolved; no resolver link, observed 2026-08-11T21:00:08.544515Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 06d0067f-3f84-4f29-ad7d-ee85b3aa72d5 · inbound

From Young to Older Disks: JWST/MIRI Evidence for Fading Molecular Emission and Hints for Elevated C/O in Upper Scorpius cites this paper.

From Young to Older Disks: JWST/MIRI Evidence for Fading Molecular Emission and Hints for Elevated C/O in Upper Scorpius Chemical enrichment of giant planets and discs due to pebble drift

Reference 149

Resolution: verified exact; local_arxiv, observed 2026-06-29T01:22:56.270746Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation 2001b81b-996e-4a37-831b-8707031130ef · inbound

Mitigating Charge Migration in JWST NIRISS Reveals That KELT-7 b is a Metal-enriched Ultra-hot Jupiter Orbiting a Young Metal-rich Star cites this paper.

Mitigating Charge Migration in JWST NIRISS Reveals That KELT-7 b is a Metal-enriched Ultra-hot Jupiter Orbiting a Young Metal-rich Star Chemical enrichment of giant planets and discs due to pebble drift

Reference 213

Resolution: verified exact; local_arxiv, observed 2026-07-10T23:07:43.574716Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation 6fb6a2e5-222b-4abc-aa4d-e6010ee441a5 · inbound

The majority of hot Jupiters formed beyond the water ice line cites this paper.

The majority of hot Jupiters formed beyond the water ice line Chemical enrichment of giant planets and discs due to pebble drift

Reference 24

Resolution: unresolved; no resolver link, observed 2026-08-02T00:06:49.396821Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.