Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links, observed 2026-08-05T15:17:55.703509Z
Paper Citation Record · LEDGER
A unique solution to overcome the barriers to planetesimal formation at low dust-to-gas ratio
As of 11 August 2026, this Paper Citation Record lists 19 of 19 outbound references and 0 inbound Pith citation observations for arXiv:2508.20070.
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 2026-08-11T06:34:44.6726+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links
A source-named dated measurement, never combined with another source.
Source: cited_works
Reference resolution
19 of 19 outbound references displayed
- verified exact1
- verified fuzzy6
- unresolved11
- parse uncertain0
- malformed identifier0
- metadata mismatch1
External citation measurements
No source-named external measurement is stored.
Outbound references
Observation 90a646c6-3c5e-4e03-ae69-429c98198520 · outbound
This paper cites & Sommeria, J.
A unique solution to overcome the barriers to planetesimal formation at low dust-to-gas ratio & Sommeria, J
Reference 1
- Resolution
- unresolved
- no resolver link, observed 2026-08-05T15:17:55.623104Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation a142ae9a-e222-4fba-94af-c03669eec551 · outbound
This paper cites 2024, Annual Review of Astronomy and Astrophysics, 62, 157.
A unique solution to overcome the barriers to planetesimal formation at low dust-to-gas ratio 2024, Annual Review of Astronomy and Astrophysics, 62, 157
Reference 2
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-05T15:17:55.963036Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation a216256e-2c83-4a65-a284-8b6ccca3fa66 · outbound
This paper cites an unresolved cited work.
A unique solution to overcome the barriers to planetesimal formation at low dust-to-gas ratio Unresolved cited work
Reference 3
- Resolution
- unresolved
- raw_fallback, observed 2026-08-05T15:17:55.951616Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation 1b635091-df92-4fb6-a45a-89516df42e41 · outbound
This paper cites an unresolved cited work.
A unique solution to overcome the barriers to planetesimal formation at low dust-to-gas ratio Unresolved cited work
Reference 4
- Resolution
- unresolved
- raw_fallback, observed 2026-08-05T15:17:55.939456Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation c94efe49-a269-4d9c-8e58-7218738d84de · outbound
This paper cites A., Bec, J., M´ eheut, H., & Kapoor, A.
A unique solution to overcome the barriers to planetesimal formation at low dust-to-gas ratio A., Bec, J., M´ eheut, H., & Kapoor, A
Reference 5
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-05T15:17:55.926246Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation 367cea19-c064-4e60-b6d8-24958aeb500e · outbound
This paper cites Clusters of heavy particles in two-dimensional Keplerian turbulence.
A unique solution to overcome the barriers to planetesimal formation at low dust-to-gas ratio Clusters of heavy particles in two-dimensional Keplerian turbulence
Reference 6
- Resolution
- metadata mismatch
- local_arxiv, observed 2026-08-05T15:17:55.783030Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation 302c9187-0174-473d-a8d1-23eac5d26efd · outbound
This paper cites F., Gammie, C.
A unique solution to overcome the barriers to planetesimal formation at low dust-to-gas ratio F., Gammie, C
Reference 7
- Resolution
- unresolved
- no resolver link, observed 2026-08-05T15:17:55.651028Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 08f9620b-29ca-480c-8100-cfec7c870fd4 · outbound
This paper cites an unresolved cited work.
A unique solution to overcome the barriers to planetesimal formation at low dust-to-gas ratio Unresolved cited work
Reference 8
- Resolution
- unresolved
- raw_fallback, observed 2026-08-05T15:17:55.908145Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation 753e6c2a-f45b-44c0-909a-0044262e8b3c · outbound
This paper cites an unresolved cited work.
A unique solution to overcome the barriers to planetesimal formation at low dust-to-gas ratio Unresolved cited work
Reference 9
- Resolution
- unresolved
- raw_fallback, observed 2026-08-05T15:17:55.895890Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation 1e153366-677c-4e97-b987-6cc722362c64 · outbound
This paper cites & Longaretti, P.-Y.
A unique solution to overcome the barriers to planetesimal formation at low dust-to-gas ratio & Longaretti, P.-Y
Reference 10
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-05T15:17:55.883173Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation 9d8c04c1-59b4-4c3c-8fa5-42a67b38c257 · outbound
This paper cites 2015, A&A, 579, A117.
A unique solution to overcome the barriers to planetesimal formation at low dust-to-gas ratio 2015, A&A, 579, A117
Reference 11
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-05T15:17:55.869750Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation ed731255-775c-4efd-9de2-11699063fd9b · outbound
This paper cites an unresolved cited work.
A unique solution to overcome the barriers to planetesimal formation at low dust-to-gas ratio Unresolved cited work
Reference 12
- Resolution
- unresolved
- raw_fallback, observed 2026-08-05T15:17:55.855666Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation ad2067b0-27a9-49e3-ac31-15de32321160 · outbound
This paper cites 1986, Icarus, 67, 375.
A unique solution to overcome the barriers to planetesimal formation at low dust-to-gas ratio 1986, Icarus, 67, 375
Reference 13
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-05T15:17:55.841429Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation c0d08270-bb9e-4412-bc02-0d4c70f3b8f9 · outbound
This paper cites an unresolved cited work.
A unique solution to overcome the barriers to planetesimal formation at low dust-to-gas ratio Unresolved cited work
Reference 14
- Resolution
- unresolved
- raw_fallback, observed 2026-08-05T15:17:55.829230Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation 97acb899-dcad-47e2-bad6-2aaa9ad3655a · outbound
This paper cites Length and Velocity Scales in Protoplanetary Disk Turbulence.
A unique solution to overcome the barriers to planetesimal formation at low dust-to-gas ratio Length and Velocity Scales in Protoplanetary Disk Turbulence
Reference 15
- Resolution
- verified exact
- local_arxiv, observed 2026-08-05T15:17:55.763502Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation bc27269b-c0a2-4938-9880-aa1ae8ef6fa8 · outbound
This paper cites Comets and Planetesimal Formation.
A unique solution to overcome the barriers to planetesimal formation at low dust-to-gas ratio Comets and Planetesimal Formation
Reference 16
- Resolution
- unresolved
- no resolver link, observed 2026-08-05T15:17:55.690548Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 63e2b392-b889-4014-82a3-a22a1eef0699 · outbound
This paper cites 1996, Icarus, 121, 158.
A unique solution to overcome the barriers to planetesimal formation at low dust-to-gas ratio 1996, Icarus, 121, 158
Reference 17
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-05T15:17:55.816626Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation f0a8036a-44d5-4481-863a-4af85efa8381 · outbound
This paper cites an unresolved cited work.
A unique solution to overcome the barriers to planetesimal formation at low dust-to-gas ratio Unresolved cited work
Reference 18
- Resolution
- unresolved
- raw_fallback, observed 2026-08-05T15:17:55.804774Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation 3ea15a86-4ba5-4e04-bf53-cc7dd057d5bf · outbound
This paper cites an unresolved cited work.
A unique solution to overcome the barriers to planetesimal formation at low dust-to-gas ratio Unresolved cited work
Reference 19
- Resolution
- unresolved
- no resolver link, observed 2026-08-05T15:17:55.703509Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Pith citing papers
No inbound Pith citation observations are available.