Paper Citation Record · LEDGER

Trans-Neptunian Binaries as Evidence for Planetesimal Formation by the Streaming Instability

As of 15 August 2026, this Paper Citation Record lists 19 of 19 outbound references and 2 inbound Pith citation observations for arXiv:1906.11344.

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

pith.paper-citation-record.v1
1906.11344 v1

Coverage vector

measured 19 of 19 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links, observed 2026-05-25T14:51:41.872962Z

measured 21 of 21 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-15T06:32:42.880941+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-14T14:51:18.509971Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-08-11T22:22:54.904883Z

Reference resolution

19 of 19 outbound references displayed

verified exact2
verified fuzzy13
unresolved4
parse uncertain0
malformed identifier0
metadata mismatch0

External citation measurements

No source-named external measurement is stored.

Outbound references

Observation 1ec7d60c-34d9-45b8-a3e5-56c8f9aa5c1c · outbound

This paper cites Multidimensional upwind methods for hyperbolic conservation laws, J.

Trans-Neptunian Binaries as Evidence for Planetesimal Formation by the Streaming Instability Multidimensional upwind methods for hyperbolic conservation laws, J

Reference 1

Resolution: verified fuzzy; raw_fallback, observed 2026-05-25T14:57:03.675469Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Observation 7c2a4933-d0e7-497f-85c3-7f30937ba829 · outbound

This paper cites an unresolved cited work.

Trans-Neptunian Binaries as Evidence for Planetesimal Formation by the Streaming Instability Unresolved cited work

Reference 2

Resolution: unresolved; raw_fallback, observed 2026-05-25T14:57:03.664808Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Observation 29d1d37d-baa6-4009-969a-a337f6a901ac · outbound

This paper cites F.Riemann Solvers and Numerical Models for Fluid Dynamics, Springer-Verlag: Berlin, Heidelberg (1999).

Trans-Neptunian Binaries as Evidence for Planetesimal Formation by the Streaming Instability F.Riemann Solvers and Numerical Models for Fluid Dynamics, Springer-Verlag: Berlin, Heidelberg (1999)

Reference 3

Resolution: verified fuzzy; raw_fallback, observed 2026-05-25T14:57:03.661666Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Observation 00f027ca-6b28-4008-8995-0807f4f72cdd · outbound

This paper cites an unresolved cited work.

Trans-Neptunian Binaries as Evidence for Planetesimal Formation by the Streaming Instability Unresolved cited work

Reference 4

Resolution: unresolved; raw_fallback, observed 2026-05-25T14:57:03.668469Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Observation 14543d5e-404f-4bf9-be98-6fb2c02e9169 · outbound

This paper cites W., Eastwood, J.

Trans-Neptunian Binaries as Evidence for Planetesimal Formation by the Streaming Instability W., Eastwood, J

Reference 5

Resolution: verified fuzzy; raw_fallback, observed 2026-05-25T14:57:03.672211Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Observation b795c875-3139-4148-87fe-49fc90641c1b · outbound

This paper cites Protoplanetary disk turbulence driven by the streaming insta- bility: linear evolution and numerical methods.

Trans-Neptunian Binaries as Evidence for Planetesimal Formation by the Streaming Instability Protoplanetary disk turbulence driven by the streaming insta- bility: linear evolution and numerical methods

Reference 6

Resolution: verified fuzzy; raw_fallback, observed 2026-05-25T14:57:03.679138Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Observation 02021ee0-cbf6-4d3d-97ba-5947a98efda8 · outbound

This paper cites F., Gammie, C.

Trans-Neptunian Binaries as Evidence for Planetesimal Formation by the Streaming Instability F., Gammie, C

Reference 7

Resolution: verified fuzzy; raw_fallback, observed 2026-05-25T14:57:03.712938Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Observation 94314408-c8c8-42c5-8bf7-165296ee8c48 · outbound

This paper cites B., Armitage, P.

Trans-Neptunian Binaries as Evidence for Planetesimal Formation by the Streaming Instability B., Armitage, P

Reference 8

Resolution: verified fuzzy; raw_fallback, observed 2026-05-25T14:57:03.702549Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Observation 288f2323-4568-46b4-9d03-45e8dc29eed0 · outbound

This paper cites FARGO: A fast eulerian transport algorithm for diﬀerentially rotating disks.

Trans-Neptunian Binaries as Evidence for Planetesimal Formation by the Streaming Instability FARGO: A fast eulerian transport algorithm for diﬀerentially rotating disks

Reference 9

Resolution: verified fuzzy; raw_fallback, observed 2026-05-25T14:57:03.699216Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Observation 1d915fca-a16b-40db-9d3b-5706aadd61ae · outbound

This paper cites M., Gardiner, T.

Trans-Neptunian Binaries as Evidence for Planetesimal Formation by the Streaming Instability M., Gardiner, T

Reference 10

Resolution: verified fuzzy; raw_fallback, observed 2026-05-25T14:57:03.706214Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Observation a40e5c82-2a89-428b-92b0-d0b9ba4a349f · outbound

This paper cites an unresolved cited work.

Trans-Neptunian Binaries as Evidence for Planetesimal Formation by the Streaming Instability Unresolved cited work

Reference 11

Resolution: unresolved; raw_fallback, observed 2026-05-25T14:57:03.709776Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Observation f4cf69c7-23bb-4b4d-9b75-aa20f724430e · outbound

This paper cites The Mass and Size Distribution of Planetesimals Formed by the Streaming Instability. II. The Effect of the Radial Gas Pressure Gradient.

Trans-Neptunian Binaries as Evidence for Planetesimal Formation by the Streaming Instability The Mass and Size Distribution of Planetesimals Formed by the Streaming Instability. II. The Effect of the Radial Gas Pressure Gradient

Reference 12

Resolution: verified exact; arxiv_id, observed 2026-05-25T14:55:57.298744Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Observation 88a1b2b7-99fa-488a-b66d-60512dab9b8c · outbound

This paper cites an unresolved cited work.

Trans-Neptunian Binaries as Evidence for Planetesimal Formation by the Streaming Instability Unresolved cited work

Reference 13

Resolution: unresolved; raw_fallback, observed 2026-05-25T14:57:03.720369Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Observation 710a925d-db5f-416d-ada6-6c907ab91df8 · outbound

This paper cites an unresolved cited work.

Trans-Neptunian Binaries as Evidence for Planetesimal Formation by the Streaming Instability Unresolved cited work

Reference 14

Resolution: verified exact; doi, observed 2026-05-25T14:55:56.909479Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Observation 8c57bb93-0989-4357-bcca-958b2820dc1f · outbound

This paper cites J., Hut, P.

Trans-Neptunian Binaries as Evidence for Planetesimal Formation by the Streaming Instability J., Hut, P

Reference 15

Resolution: verified fuzzy; raw_fallback, observed 2026-05-25T14:57:03.682474Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Observation 636ab67e-09a7-449b-b688-828c32598c3c · outbound

This paper cites M., A Computer Oriented Geodetic Data Base and a New Technique in File Sequencing, International Business Machines Co.

Trans-Neptunian Binaries as Evidence for Planetesimal Formation by the Streaming Instability M., A Computer Oriented Geodetic Data Base and a New Technique in File Sequencing, International Business Machines Co

Reference 16

Resolution: verified fuzzy; raw_fallback, observed 2026-05-25T14:57:03.687660Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Observation 85fc3326-172c-4a3e-b947-0e1e39fe7dd6 · outbound

This paper cites A hierarchical O(N log N) force-calculation algorithm.

Trans-Neptunian Binaries as Evidence for Planetesimal Formation by the Streaming Instability A hierarchical O(N log N) force-calculation algorithm

Reference 17

Resolution: verified fuzzy; raw_fallback, observed 2026-05-25T14:57:03.695388Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Observation 57cc56e9-47e8-4757-96fc-9c07b08bf181 · outbound

This paper cites J., Kary, D.

Trans-Neptunian Binaries as Evidence for Planetesimal Formation by the Streaming Instability J., Kary, D

Reference 18

Resolution: verified fuzzy; raw_fallback, observed 2026-05-25T14:57:03.691430Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Observation 597d7e95-2889-415f-bd58-7a9aab60beba · outbound

This paper cites On the origin of planetary spins.

Trans-Neptunian Binaries as Evidence for Planetesimal Formation by the Streaming Instability On the origin of planetary spins

Reference 19

Resolution: verified fuzzy; raw_fallback, observed 2026-05-25T14:57:03.715775Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Pith citing papers

Observation 0cdbc30c-5049-42e2-8725-fa385a9387f2 · 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 Trans-Neptunian Binaries as Evidence for Planetesimal Formation by the Streaming Instability

Reference 75

Resolution: unresolved; no resolver link, observed 2026-08-14T14:51:18.509971Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 27fbe4fa-7e51-481a-a69f-9ed41b1ff82c · inbound

Angular Momentum Drain: Despinning Embedded Planetesimals cites this paper.

Angular Momentum Drain: Despinning Embedded Planetesimals Trans-Neptunian Binaries as Evidence for Planetesimal Formation by the Streaming Instability

Reference 2019

Resolution: metadata mismatch; local_arxiv, observed 2026-08-11T22:22:54.909306Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.