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Paper Citation Record · LEDGER

Compaction during fragmentation and bouncing produces realistic dust grain porosities in protoplanetary discs

As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2406.15622.

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

pith.paper-citation-record.v1
2406.15622 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 3 of 3 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-11T06:34:44.6726+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-10T21:34:15.735878Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-08-10T21:34:15.923711Z

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 db00bd59-5081-46f8-8d45-e6887abb04aa · inbound

Chondrule dust rim growth: Influence of restructuring using molecular dynamics simulations cites this paper.

Chondrule dust rim growth: Influence of restructuring using molecular dynamics simulations Compaction during fragmentation and bouncing produces realistic dust grain porosities in protoplanetary discs

Reference 19

Resolution
verified exact
local_arxiv, observed 2026-08-10T21:34:15.931588Z

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.

source=pdf_text observed=2026-08-10T21:34:15.735878Z digest=sha256:79b129d0d12f3362200c77495d3573ee7dc960596cd3718b6d62108743ee7c7c

Observation c8883ba6-6692-4e71-84ba-b3655d0fc8ea · inbound

Circumstellar and circumbinary discs in multiple stellar systems cites this paper.

Circumstellar and circumbinary discs in multiple stellar systems Compaction during fragmentation and bouncing produces realistic dust grain porosities in protoplanetary discs

Reference 183

Resolution
unresolved
no resolver link, observed 2026-08-09T20:51:30.716049Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-09T20:51:30.716049Z digest=sha256:0e406fa33ee2c2a6868f81994ffcdcdc5f06209f0d4ea90035fc8e17909ac564

Observation cdaf4fec-6b6e-4821-9e56-5713e97c7b74 · inbound

Dust Growth in Binary Systems: Inhibition of dust settling and growth in circumbinary discs cites this paper.

Dust Growth in Binary Systems: Inhibition of dust settling and growth in circumbinary discs Compaction during fragmentation and bouncing produces realistic dust grain porosities in protoplanetary discs

Reference 185

Resolution
unresolved
no resolver link, observed 2026-08-02T01:07:56.743445Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T01:07:56.743445Z digest=sha256:de67cc1abcdee79e601d0878757c6b826ec830a710a3a38dcb788ad2ab0940e3