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Paper Citation Record · LEDGER

Architectures of Compact Multi-planet Systems: Diversity and Uniformity

As of 9 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 8 inbound Pith citation observations for arXiv:2203.10076.

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

pith.paper-citation-record.v1
2203.10076 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 8 of 8 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-09T06:31:02.800959+00:00

measured 8 of 8 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-07T10:34:42.568945Z

measured 1 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-08-05T02:28:24.338817Z

Reference resolution

0 of 0 outbound references displayed

  • verified exact0
  • verified fuzzy0
  • unresolved0
  • parse uncertain0
  • malformed identifier0
  • metadata mismatch0

External citation measurements

16
arxiv_reference, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 2a65e3e1-f7f3-4357-a06a-f7ef1e0b0f92 · inbound

Planets similar in size are often dissimilar in interior cites this paper.

Planets similar in size are often dissimilar in interior Architectures of Compact Multi-planet Systems: Diversity and Uniformity

Reference 70

Resolution
unresolved
no resolver link, observed 2026-08-07T10:34:42.568945Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T10:34:42.568945Z digest=sha256:f3cb51ed45ef6759cbbe8ed2202225119fcc799b296677d9243879c12b85077d

Observation 8d6f04c4-cb74-4496-b1ed-96d4c1816048 · inbound

Gas Pressure Driven Screening Forces and Pebble Aggregation: A Pathway for Growth in Planet Formation cites this paper.

Gas Pressure Driven Screening Forces and Pebble Aggregation: A Pathway for Growth in Planet Formation Architectures of Compact Multi-planet Systems: Diversity and Uniformity

Reference 38

Resolution
unresolved
no resolver link, observed 2026-08-06T20:36:05.507469Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T20:36:05.507469Z digest=sha256:0cf61e186ec6794cc87d086ab8a4e465bb36151fff14e92db6672cc3f284dddc

Observation 1f8775f6-7c8e-4b40-acfb-dc37e1f5985b · inbound

The formation of planetary systems: physics, populations, and architectures cites this paper.

The formation of planetary systems: physics, populations, and architectures Architectures of Compact Multi-planet Systems: Diversity and Uniformity

Reference 65

Resolution
verified exact
arxiv_id, observed 2026-05-10T17:50:40.684081Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

source=pdf_text observed=2026-05-10T17:49:00.258666Z digest=sha256:aa338ea5cca2a7ab9e204ae23d245e7110dbb2d016b1264b70545c073b29d651

Observation 8bf8bd63-9b6d-43db-bba5-3aa0c8835a78 · inbound

Peas and USPs: Can Stellar Spindown and Peas in a Pod Replicate Ultra-Short-Period Planet Characteristics? cites this paper.

Peas and USPs: Can Stellar Spindown and Peas in a Pod Replicate Ultra-Short-Period Planet Characteristics? Architectures of Compact Multi-planet Systems: Diversity and Uniformity

Reference 71

Resolution
metadata mismatch
arxiv_id, observed 2026-06-27T23:31:25.413391Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

source=pdf_text observed=2026-06-27T23:28:30.261149Z digest=sha256:9fba414d192797d7d7b7adee2b19bb7ea85b772aa4679f6c825c7942132091a1

Observation fa17c51d-5fd9-49ae-9492-1ab4d8094266 · inbound

Observing a 542-day transiting giant with large TTVs: The 2025 transit of HIP 41378 f and new constraints on the outer system cites this paper.

Observing a 542-day transiting giant with large TTVs: The 2025 transit of HIP 41378 f and new constraints on the outer system Architectures of Compact Multi-planet Systems: Diversity and Uniformity

Reference 286

Resolution
metadata mismatch
arxiv_id, observed 2026-06-26T17:29:38.750304Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

source=arxiv_source observed=2026-06-26T07:16:08.147760Z digest=sha256:74b3aa59e9a777d3759f918f7f167a5b12c7431a310adc0a59d654baf289867e

Observation b6ad0c13-0af7-4bd5-9ad2-11d6cd06f832 · inbound

Observing a 542-day transiting giant with large TTVs: The 2025 transit of HIP 41378 f and new constraints on the outer system cites this paper.

Observing a 542-day transiting giant with large TTVs: The 2025 transit of HIP 41378 f and new constraints on the outer system Architectures of Compact Multi-planet Systems: Diversity and Uniformity

Reference 286

Resolution
metadata mismatch
arxiv_id, observed 2026-06-30T10:24:35.597804Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

source=arxiv_source observed=2026-06-30T10:20:49.416445Z digest=sha256:f4b00fc6fa5b0140325a9abbeb17f06276e07293e8adebc99f665ddff222a99f

Observation f7a04927-3f5b-4b05-a291-447cdd2da359 · inbound

Architectures of Planetary Systems III: Excitation of Eccentricities and Inclinations cites this paper.

Architectures of Planetary Systems III: Excitation of Eccentricities and Inclinations Architectures of Compact Multi-planet Systems: Diversity and Uniformity

Reference 44

Resolution
verified exact
arxiv_id, observed 2026-06-26T03:38:58.450926Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

source=pdf_text observed=2026-06-26T01:21:43.804149Z digest=sha256:cf9ed41ac2fd07e62487104c8570caafbf0cbdd841bcdcc585145de9f02fd35b

Observation b8a46db1-536d-414f-bc6c-91b9504fec3b · inbound

Dynamically Selected Mass-Radius Relationship for Low Mass Exoplanets cites this paper.

Dynamically Selected Mass-Radius Relationship for Low Mass Exoplanets Architectures of Compact Multi-planet Systems: Diversity and Uniformity

Reference 138

Resolution
unresolved
no resolver link, observed 2026-08-01T12:14:31.459894Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T12:14:31.459894Z digest=sha256:06a2b2da29e31f46c4540587e19ed5f182ef61b5c94edc228d8c223a5663cfaf