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Paper Citation Record · LEDGER

Population Synthesis Models Indicate a Need for Early and Ubiquitous Disk Substructures

As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:2405.14501.

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

pith.paper-citation-record.v1
2405.14501 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 5 of 5 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 5 of 5 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-09T23:55:07.949506Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-08-07T05:53:04.462081Z

Reference resolution

0 of 0 outbound references displayed

  • verified exact0
  • verified fuzzy0
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  • 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 ddb2efe9-3735-439c-8360-30cb044a5c85 · inbound

Characterising the multiple protostellar system VLA 1623-2417 with JWST, ALMA and VLA: outflow origins, dust growth and an unsettled disk cites this paper.

Characterising the multiple protostellar system VLA 1623-2417 with JWST, ALMA and VLA: outflow origins, dust growth and an unsettled disk Population Synthesis Models Indicate a Need for Early and Ubiquitous Disk Substructures

Reference 30

Resolution
unresolved
no resolver link, observed 2026-08-09T23:55:07.949506Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-09T23:55:07.949506Z digest=sha256:beb2e7b037e5fde022b9b1f3b812b22f8d80c15eef533e376d37d4c6d6785dfe

Observation 0d309b4c-460e-401f-b90f-60837226f67d · inbound

On Linking Planet Formation Models, Protoplanetary Disk Properties, and Mature Gas Giant Exoplanet Atmospheres cites this paper.

On Linking Planet Formation Models, Protoplanetary Disk Properties, and Mature Gas Giant Exoplanet Atmospheres Population Synthesis Models Indicate a Need for Early and Ubiquitous Disk Substructures

Reference 118

Resolution
unresolved
no resolver link, observed 2026-08-07T12:04:37.893896Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T12:04:37.893896Z digest=sha256:14d774b6e875d168287afd82276ba40a551624bf8e0695b7437835a2f0639308

Observation eb76e5f5-eb14-4b76-be38-90dc5970a677 · inbound

FAUST XXVI. The dust opacity spectral indices of protostellar envelopes bridge the gap between interstellar medium and disks cites this paper.

FAUST XXVI. The dust opacity spectral indices of protostellar envelopes bridge the gap between interstellar medium and disks Population Synthesis Models Indicate a Need for Early and Ubiquitous Disk Substructures

Reference 32

Resolution
metadata mismatch
local_arxiv, observed 2026-08-07T05:53:04.465597Z

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=2026-08-07T05:53:04.057439Z digest=sha256:8c6da3a699a54e680c98f1f6d17cd6fd655adc681e7d733446f97a536f3ee4f0

Observation 5a4004f3-28e3-4cdc-9aea-8b916595ed27 · inbound

Preferential alignment of Class 0, Class I protostellar disks in multiple systems across nine nearby molecular clouds cites this paper.

Preferential alignment of Class 0, Class I protostellar disks in multiple systems across nine nearby molecular clouds Population Synthesis Models Indicate a Need for Early and Ubiquitous Disk Substructures

Reference 132

Resolution
unresolved
no resolver link, observed 2026-08-02T02:36:30.350667Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T02:36:30.350667Z digest=sha256:e49e85c58e80dc20e328d8aba9dbee233db01ea1c27635e588ee18676662edbb

Observation 80ee988e-48d7-47c5-913c-47b790dbff68 · inbound

SMA 200-400 GHz Survey for 10 faint Class II Disks in the Taurus Molecular Cloud cites this paper.

SMA 200-400 GHz Survey for 10 faint Class II Disks in the Taurus Molecular Cloud Population Synthesis Models Indicate a Need for Early and Ubiquitous Disk Substructures

Reference 80

Resolution
unresolved
no resolver link, observed 2026-08-08T13:01:49.661929Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-08T13:01:49.661929Z digest=sha256:b43c19c806f361772f2c89057385ef4b0e6ffa1c4b5411e5a372aa3055925ef1