Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Formation of planetary systems by pebble accretion and migration: Hot super-Earth systems from breaking compact resonant chains
As of 14 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:1902.08772.
A citation records a reference. It does not transfer a finding from one paper to another.
Coverage vector
One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-14T06:32:32.682623+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-14T12:38:18.288134Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-08-11T23:13:11.681328Z
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 60906666-60ed-4e19-be52-eb1b10b9b93a · 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: Hot super-Earth systems from breaking compact resonant chains
Reference 23
- Resolution
- unresolved
- no resolver link, observed 2026-08-14T12:38:18.288134Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation d6610051-d536-419a-a55e-97d0ccf332aa · inbound
How Flow Isolation May Set the Mass Scale for Super-Earth Planets cites this paper.
How Flow Isolation May Set the Mass Scale for Super-Earth Planets Formation of planetary systems by pebble accretion and migration: Hot super-Earth systems from breaking compact resonant chains
Reference 25
- Resolution
- unresolved
- no resolver link, observed 2026-08-14T12:35:52.618283Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 1a7de187-d398-40f8-a580-ab49234e7baf · 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: Hot super-Earth systems from breaking compact resonant chains
Reference 70
- Resolution
- unresolved
- no resolver link, observed 2026-08-14T05:45:39.445001Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 0fc466f0-33ce-4a95-b8dd-34c5092e426c · 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: Hot super-Earth systems from breaking compact resonant chains
Reference 19
- Resolution
- verified exact
- local_arxiv, observed 2026-08-11T23:13:11.686387Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.
Observation f778c5fd-c342-4319-a79f-0d8f18a91f11 · inbound
Dynamically Selected Mass-Radius Relationship for Low Mass Exoplanets cites this paper.
Dynamically Selected Mass-Radius Relationship for Low Mass Exoplanets Formation of planetary systems by pebble accretion and migration: Hot super-Earth systems from breaking compact resonant chains
Reference 54
- Resolution
- unresolved
- no resolver link, observed 2026-08-01T12:14:31.224051Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.