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Paper Citation Record · LEDGER

The Galactic 3D large-scale dust distribution via Gaussian process regression on spherical coordinates

As of 19 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2204.11715.

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

pith.paper-citation-record.v1
2204.11715 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 2026-08-19T06:32:44.657259+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-16T12:39:03.565410Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-08-12T17:50:36.467698Z

Reference resolution

0 of 0 outbound references displayed

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  • verified fuzzy0
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  • 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 f4a9764b-d9bd-4f92-b1f7-cefb10da0831 · inbound

Kinetic tomography of the Galactic plane within 1.25 kiloparsecs from the Sun. The interstellar flows revealed by HI and CO line emission and 3D dust cites this paper.

Kinetic tomography of the Galactic plane within 1.25 kiloparsecs from the Sun. The interstellar flows revealed by HI and CO line emission and 3D dust The Galactic 3D large-scale dust distribution via Gaussian process regression on spherical coordinates

Reference 111

Resolution
metadata mismatch
local_arxiv, observed 2026-08-12T17:50:36.475190Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

source=arxiv_source observed=2026-08-12T17:50:35.932726Z digest=sha256:43e926a080e7260f5e2c2428387c8d90eff58ca519389d1ddb49a46e02c0e4f2

Observation 6628b110-5717-44ff-aa6f-bee0299e1120 · inbound

Origin of the IRAS Vela Shell: New Insights from 3D Dust Mapping cites this paper.

Origin of the IRAS Vela Shell: New Insights from 3D Dust Mapping The Galactic 3D large-scale dust distribution via Gaussian process regression on spherical coordinates

Reference 45

Resolution
unresolved
no resolver link, observed 2026-08-16T12:39:03.565410Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-16T12:39:03.565410Z digest=sha256:179f4c5b8e1bf5cfc89a9ff882feee1d6d6b8ea1ba71b6e9c62b27023b6cc027

Observation 3bca5a87-0faa-496c-a5a3-d0ed32809e5d · inbound

Massive Acquisition of Ultraviolet Color Excess Information from GALEX and UVOT Bands cites this paper.

Massive Acquisition of Ultraviolet Color Excess Information from GALEX and UVOT Bands The Galactic 3D large-scale dust distribution via Gaussian process regression on spherical coordinates

Reference 23

Resolution
unresolved
no resolver link, observed 2026-08-15T23:56:01.184049Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-15T23:56:01.184049Z digest=sha256:455628d064bb7031019d05d34f429abf6ac76dbd458e23f2e90b74fb7052798f