Paper Citation Record · LEDGER

SE3D: Building a radiative transfer emulator to fit panchromatic resolved galaxy observations with 3D models of dust and stars

As of 17 August 2026, this Paper Citation Record lists 5 of 5 outbound references and 1 inbound Pith citation observation for arXiv:2511.19623.

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

pith.paper-citation-record.v1
2511.19623 v2

Coverage vector

measured 5 of 5 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links, observed 2026-05-21T19:14:44.551439Z

measured 6 of 6 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-17T06:30:58.91139+00:00

measured 1 of 1 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-02T00:50:15.421972Z

measured 1 of 1 external citation measurements

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

Source: pith, observed 2026-08-05T02:28:24.338817Z

Reference resolution

5 of 5 outbound references displayed

verified exact0
verified fuzzy0
unresolved4
parse uncertain0
malformed identifier1
metadata mismatch0

External citation measurements

0
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

Observation 7dc670da-6d2d-4342-88dc-6345d53d5ccd · outbound

This paper cites an unresolved cited work.

SE3D: Building a radiative transfer emulator to fit panchromatic resolved galaxy observations with 3D models of dust and stars Unresolved cited work

Reference 1

Resolution: unresolved; raw_fallback, observed 2026-05-21T19:15:31.260277Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

Observation 0de0f51b-96d7-494d-b44e-273752fd1935 · outbound

This paper cites an unresolved cited work.

SE3D: Building a radiative transfer emulator to fit panchromatic resolved galaxy observations with 3D models of dust and stars Unresolved cited work

Reference 2

Resolution: unresolved; raw_fallback, observed 2026-05-21T19:15:31.254876Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

Observation e77bd09a-c641-4fe1-9957-42206614f933 · outbound

This paper cites an unresolved cited work.

SE3D: Building a radiative transfer emulator to fit panchromatic resolved galaxy observations with 3D models of dust and stars Unresolved cited work

Reference 3

Resolution: unresolved; raw_fallback, observed 2026-05-21T19:15:31.249146Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

Observation 15306af2-f6fc-4ade-92c9-0c70ec504580 · outbound

This paper cites an unresolved cited work.

SE3D: Building a radiative transfer emulator to fit panchromatic resolved galaxy observations with 3D models of dust and stars Unresolved cited work

Reference 4

Resolution: unresolved; raw_fallback, observed 2026-05-21T19:15:31.252142Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

Observation f27883bf-cd43-4d47-a03e-86fffb872d8b · outbound

This paper cites Figure A1.Validation of model predicting whether a toy model galaxy is physical or unphysical, as evaluated on an unseen testing set.

SE3D: Building a radiative transfer emulator to fit panchromatic resolved galaxy observations with 3D models of dust and stars Figure A1.Validation of model predicting whether a toy model galaxy is physical or unphysical, as evaluated on an unseen testing set

Reference 5

Resolution: malformed identifier; raw_fallback, observed 2026-05-21T19:15:31.257650Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

Pith citing papers

Observation 8343ac0b-cdce-47df-a30f-70b2bdc60448 · inbound

The COLIBRE-SKIRT pipeline: Calibration-free dust radiative transfer postprocessing for cosmological simulations cites this paper.

The COLIBRE-SKIRT pipeline: Calibration-free dust radiative transfer postprocessing for cosmological simulations SE3D: Building a radiative transfer emulator to fit panchromatic resolved galaxy observations with 3D models of dust and stars

Reference 158

Resolution: metadata mismatch; local_arxiv, observed 2026-08-02T00:53:29.348152Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.