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Paper Citation Record · LEDGER

One Solution to the Mass Budget Problem for Planet Formation: Optically Thick Disks with Dust Scattering

As of 5 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:1904.02127.

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

pith.paper-citation-record.v1
1904.02127 v2

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 2026-08-04T06:34:03.388597+00:00

measured 4 of 4 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-01T23:20:44.110151Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-10T06:15:00.866473Z

Reference resolution

0 of 0 outbound references displayed

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  • verified fuzzy0
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  • malformed identifier0
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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 e9f1d970-f3b4-4020-aa32-9d0d1386d2cd · inbound

Millimeter dust continuum and polarization in protoplanetary disks with scattering: A slab model cites this paper.

Millimeter dust continuum and polarization in protoplanetary disks with scattering: A slab model One Solution to the Mass Budget Problem for Planet Formation: Optically Thick Disks with Dust Scattering

Reference 12

Resolution
metadata mismatch
local_arxiv, observed 2026-05-15T03:14:52.164851Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:90ca935479c91ec0c63d292e389d660efb6abcc958f723cad0a8b6a8919e2195

Observation 5ad10d59-cb56-4bb3-85cf-6e0997ae68d1 · inbound

Data assimilation for subsurface flow using latent diffusion model parameterization: performance of ensemble-Kalman and Monte Carlo techniques cites this paper.

Data assimilation for subsurface flow using latent diffusion model parameterization: performance of ensemble-Kalman and Monte Carlo techniques One Solution to the Mass Budget Problem for Planet Formation: Optically Thick Disks with Dust Scattering

Reference 5

Resolution
metadata mismatch
local_arxiv, observed 2026-06-27T10:40:50.179032Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

source=pdf_text observed=2026-06-27T10:35:43.483712Z digest=sha256:34ec3eef34d7cc5b4da0ed6733e6858bb36b84a927820e389ac4e14535b060af

Observation 469a63cd-a1f2-451a-bdea-ed357ec6c3e0 · inbound

DiskMINT-GARDEN: Self-consistent Models to Estimate Disk Masses cites this paper.

DiskMINT-GARDEN: Self-consistent Models to Estimate Disk Masses One Solution to the Mass Budget Problem for Planet Formation: Optically Thick Disks with Dust Scattering

Reference 35

Resolution
metadata mismatch
local_arxiv, observed 2026-06-26T01:28:51.306519Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:06b1494711a5cff8e65a9040d24c55ecbe82d04bbad6866110d2a4be66eb9859

Observation 1a75bba9-c46c-46a1-9e53-8802e17bfb23 · inbound

A JWST, ALMA and VLA survey of the Ophiuchus-A star-forming region: Unveiling hidden dust mass and connecting infrared outflows to their radio origins cites this paper.

A JWST, ALMA and VLA survey of the Ophiuchus-A star-forming region: Unveiling hidden dust mass and connecting infrared outflows to their radio origins One Solution to the Mass Budget Problem for Planet Formation: Optically Thick Disks with Dust Scattering

Reference 7

Resolution
unresolved
no resolver link, observed 2026-08-01T23:20:44.110151Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T23:20:44.110151Z digest=sha256:423c1a7098ca27a6d2e93f2ca56c268be401b1ce887781aa9ce5549febcdef8f