Paper Citation Record · LEDGER

Formation of planetary systems by pebble accretion and migration: How the radial pebble flux determines a terrestrial-planet or super-Earth growth mode

As of 16 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 9 inbound Pith citation observations for arXiv:1902.08694.

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

pith.paper-citation-record.v1
1902.08694 v1

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measured 9 of 9 standing notices

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Source: scholarly_work_events, retraction_status_cache, observed 2026-08-16T06:30:59.297886+00:00

measured 9 of 9 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-14T14:51:18.393850Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-06-29T01:22:56.301285Z

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Outbound references

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Pith citing papers

Observation 8b771237-a5c5-4c70-af2f-cba1241cd2bd · inbound

Linking planetesimal and dust content in protoplanetary disks via a local toy model cites this paper.

Linking planetesimal and dust content in protoplanetary disks via a local toy model Formation of planetary systems by pebble accretion and migration: How the radial pebble flux determines a terrestrial-planet or super-Earth growth mode

Reference 62

Resolution: unresolved; no resolver link, observed 2026-08-14T14:51:18.393850Z

Source-reported events for the cited work

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Observation 2eb1dca3-e2ae-401f-a3d7-916da4f4d9f9 · inbound

Super-Earth ingestion can explain the anomalously high metal abundances of M67 Y2235 cites this paper.

Super-Earth ingestion can explain the anomalously high metal abundances of M67 Y2235 Formation of planetary systems by pebble accretion and migration: How the radial pebble flux determines a terrestrial-planet or super-Earth growth mode

Reference 28

Resolution: unresolved; no resolver link, observed 2026-08-14T12:38:18.318980Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 25a46432-8b5c-43e8-a9ee-ccae2bb35410 · inbound

Super-Earth masses sculpted by pebble isolation around stars of different masses cites this paper.

Super-Earth masses sculpted by pebble isolation around stars of different masses Formation of planetary systems by pebble accretion and migration: How the radial pebble flux determines a terrestrial-planet or super-Earth growth mode

Reference 87

Resolution: unresolved; no resolver link, observed 2026-08-14T05:45:39.506312Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 4e6e8288-2356-4a32-a719-093279079268 · inbound

Accretion of Uranus and Neptune: confronting different giant impact scenarios cites this paper.

Accretion of Uranus and Neptune: confronting different giant impact scenarios Formation of planetary systems by pebble accretion and migration: How the radial pebble flux determines a terrestrial-planet or super-Earth growth mode

Reference 2019

Resolution: unresolved; no resolver link, observed 2026-08-11T23:13:10.647559Z

Source-reported events for the cited work

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Observation 02512f08-caa9-457b-8640-765ed0fbb6f7 · inbound

Chemical Divergence and Water Depletion: Gas Properties of Evolved Upper Scorpius Disks Revealed by JWST/MIRI cites this paper.

Chemical Divergence and Water Depletion: Gas Properties of Evolved Upper Scorpius Disks Revealed by JWST/MIRI Formation of planetary systems by pebble accretion and migration: How the radial pebble flux determines a terrestrial-planet or super-Earth growth mode

Reference 100

Resolution: metadata mismatch; local_arxiv, observed 2026-06-29T01:12:56.127651Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

Observation 9a47d08a-b32c-4316-9989-96bc0a3f434b · 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 Formation of planetary systems by pebble accretion and migration: How the radial pebble flux determines a terrestrial-planet or super-Earth growth mode

Reference 117

Resolution: verified exact; local_arxiv, observed 2026-06-29T01:22:56.302846Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

Observation 5d2903ad-924e-4691-b91d-d501d8080f37 · inbound

The GAPS Programme with HARPS-N at TNG LXXVII. Occurrence rates of small close-in planets in the presence of cold Jupiters cites this paper.

The GAPS Programme with HARPS-N at TNG LXXVII. Occurrence rates of small close-in planets in the presence of cold Jupiters Formation of planetary systems by pebble accretion and migration: How the radial pebble flux determines a terrestrial-planet or super-Earth growth mode

Reference 258

Resolution: unresolved; no resolver link, observed 2026-07-13T03:54:36.358098Z

Source-reported events for the cited work

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Observation 326a0d13-1b23-4ccf-bedf-5bde63dfb39c · inbound

The GAPS Programme with HARPS-N at TNG LXXVII. Occurrence rates of small close-in planets in the presence of cold Jupiters cites this paper.

Reference 258

Resolution: unresolved; no resolver link, observed 2026-07-14T15:15:28.911413Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 918d628a-bebc-4c2d-9950-a6e78614329b · inbound

Searching for Habitable Exoplanets with Relative Astrometry (SHERA). I. The Case for Searching for Planets in Binary Star Systems cites this paper.

Searching for Habitable Exoplanets with Relative Astrometry (SHERA). I. The Case for Searching for Planets in Binary Star Systems Formation of planetary systems by pebble accretion and migration: How the radial pebble flux determines a terrestrial-planet or super-Earth growth mode

Reference 47

Resolution: unresolved; no resolver link, observed 2026-08-08T00:10:25.866555Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.