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Paper Citation Record · LEDGER

Radiative Transfer Model of Dust Attenuation Curves in Clumpy, Galactic Environments

As of 23 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:1606.02030.

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

pith.paper-citation-record.v1
1606.02030 v1

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 2026-08-22T06:32:14.747728+00:00

measured 4 of 4 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-02T07:18:19.918400Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-06-30T03:34:12.803576Z

Reference resolution

0 of 0 outbound references displayed

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  • verified fuzzy0
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  • parse uncertain0
  • 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 bd6b816c-7192-4af7-8fed-0a4095e2d541 · inbound

Learning the Universe: The Structure of Dust Attenuation Curves in Galaxy Simulations cites this paper.

Learning the Universe: The Structure of Dust Attenuation Curves in Galaxy Simulations Radiative Transfer Model of Dust Attenuation Curves in Clumpy, Galactic Environments

Reference 164

Resolution
verified exact
local_arxiv, observed 2026-06-27T15:51:01.874757Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:d616db8e79c4d29e531fce68dc12aeea481c7cc040d0001f200b537a5ba8b84d

Observation 16b2551a-f231-4c25-b775-74331ebca9a0 · inbound

High-Resolution Spectroscopy of Raman-scattered He II Lines in the Symbiotic Nova RR Telescopii cites this paper.

High-Resolution Spectroscopy of Raman-scattered He II Lines in the Symbiotic Nova RR Telescopii Radiative Transfer Model of Dust Attenuation Curves in Clumpy, Galactic Environments

Reference 133

Resolution
verified exact
local_arxiv, observed 2026-06-30T03:34:12.805157Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:3cf7d7435f2ec851dc462c330bfdb1d4dc60b8796b59547446ada039eba75f5b

Observation 562c4a2b-a3cd-49a9-89a8-b88a60e0c575 · inbound

Mapping Dust Attenuation at Kiloparsec Scales. III. The 2175\AA\ Bump cites this paper.

Mapping Dust Attenuation at Kiloparsec Scales. III. The 2175\AA\ Bump Radiative Transfer Model of Dust Attenuation Curves in Clumpy, Galactic Environments

Reference 56

Resolution
unresolved
no resolver link, observed 2026-07-14T10:44:26.626236Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-14T10:44:26.626236Z digest=sha256:fe9d9bbcc27a1c32a20fb272de8c4f9b6eca699d8b1c40a97b2bc9be6c59d504

Observation 94ceba1f-fe4b-4cc4-9ae1-044ce3ef441f · inbound

Mapping Dust Attenuation at Kiloparsec Scales. III. The 2175\AA\ Bump cites this paper.

Mapping Dust Attenuation at Kiloparsec Scales. III. The 2175\AA\ Bump Radiative Transfer Model of Dust Attenuation Curves in Clumpy, Galactic Environments

Reference 56

Resolution
unresolved
no resolver link, observed 2026-08-02T07:18:19.918400Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T07:18:19.918400Z digest=sha256:f9d5b3b445028673b432780ff249956689e6016638043ea4ce76d36789627e92