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Paper Citation Record · LEDGER

The Planet Nine Hypothesis

As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:1902.10103.

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

pith.paper-citation-record.v1
1902.10103 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 2026-08-10T06:31:04.303077+00:00

measured 4 of 4 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-06T11:57:56.763579Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-04T18:40:02.517038Z

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 55644519-e806-4b1b-98e0-91cf2d35afe9 · inbound

The Radius, Composition, Albedo, and Absolute Magnitude of Planet Nine Based on Exoplanets with Teq less than 600 K and the Planet Nine Reference Population 3.0 cites this paper.

The Radius, Composition, Albedo, and Absolute Magnitude of Planet Nine Based on Exoplanets with Teq less than 600 K and the Planet Nine Reference Population 3.0 The Planet Nine Hypothesis

Reference 1

Resolution
unresolved
no resolver link, observed 2026-08-06T11:57:56.763579Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T11:57:56.763579Z digest=sha256:84dc5d937a1a37cf2775409b603e3478e73cfebbeaf17249f109b5831f813d23

Observation 17f43a57-698e-4fec-a9a9-f121e6b311cc · inbound

Planet or brown dwarf? Constraints on the formation of H-type objects in IC348 cites this paper.

Planet or brown dwarf? Constraints on the formation of H-type objects in IC348 The Planet Nine Hypothesis

Reference 88

Resolution
metadata mismatch
local_arxiv, observed 2026-06-28T02:31:30.732252Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:b383904b3041b83bc03cf250cf9791092f26e198f78fa5d577c42b2abd077476

Observation ee84943b-94c6-463e-a30e-edeb5c7970b5 · inbound

A Solar-System Window for Hidden Stellar Companions cites this paper.

A Solar-System Window for Hidden Stellar Companions The Planet Nine Hypothesis

Reference 4

Resolution
verified exact
local_arxiv, observed 2026-07-04T18:40:02.518278Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=pdf_text observed=2026-06-25T22:44:08.738991Z digest=sha256:28869d8bce2d236bc9225f365d9df1ef76e47bdf6b9a22ce33acf69ef175fef7

Observation 3e22a4f4-f0f5-48ef-a818-866331338607 · inbound

White dwarf planets in star clusters: gravitational scattering versus mass-loss effects cites this paper.

White dwarf planets in star clusters: gravitational scattering versus mass-loss effects The Planet Nine Hypothesis

Reference 88

Resolution
metadata mismatch
local_arxiv, observed 2026-07-02T17:47:17.318573Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:dc86841acdf035785a487e09e195cd9ad09aa1bb90dc35973b4341b55238cf86