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Paper Citation Record · LEDGER

exoALMA III: Line-intensity Modeling and System Property Extraction from Protoplanetary Disks

As of 6 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2504.19986.

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

pith.paper-citation-record.v1
2504.19986 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 2026-08-06T06:34:29.942622+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-04T01:36:12.712106Z

measured 0 of 1 external citation measurements

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

Source: cited_works

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 dde729df-95fc-4bb0-b36d-98b44b140674 · inbound

Extending dynamical mass measurements: probing GI as a possible origin of mm-dust spirals cites this paper.

Extending dynamical mass measurements: probing GI as a possible origin of mm-dust spirals exoALMA III: Line-intensity Modeling and System Property Extraction from Protoplanetary Disks

Reference 189

Resolution
unresolved
no resolver link, observed 2026-08-01T22:01:35.286321Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T22:01:35.286321Z digest=sha256:8ec290afe29f7c8984fc36db0d15bdc0b728fc9cb11001d105b4ead1ea6bf1fe

Observation 2200ac1b-3d26-41dc-b9b2-744b3c3fa626 · inbound

Angular Momentum of Planet-Forming Disks: Implications for Infall Driven Misalignments cites this paper.

Angular Momentum of Planet-Forming Disks: Implications for Infall Driven Misalignments exoALMA III: Line-intensity Modeling and System Property Extraction from Protoplanetary Disks

Reference 53

Resolution
unresolved
no resolver link, observed 2026-07-30T14:23:16.815396Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-30T14:23:16.815396Z digest=sha256:65de293c2adc4ce7776485a3a9df49fa270deb9827c22d6efc9c0ed23cc7aa94

Observation 06e9aa91-5a6b-4f89-a44c-26b99d714be7 · inbound

Angular Momentum of Planet-Forming Disks: Implications for Infall Driven Misalignments cites this paper.

Angular Momentum of Planet-Forming Disks: Implications for Infall Driven Misalignments exoALMA III: Line-intensity Modeling and System Property Extraction from Protoplanetary Disks

Reference 53

Resolution
unresolved
no resolver link, observed 2026-08-04T01:36:12.712106Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-04T01:36:12.712106Z digest=sha256:70edd2fbb041c239e2f24ede97b074e373ba960bd2ffdd33e4fe3479b4495447