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Paper Citation Record · LEDGER

A Comparison of Deep Learning Architectures for Optical Galaxy Morphology Classification

As of 16 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2111.04353.

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

pith.paper-citation-record.v1
2111.04353 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 2 of 2 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-16T06:30:59.297886+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-02T08:46:54.783692Z

measured 0 of 1 external citation measurements

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

Source: cited_works

Reference resolution

0 of 0 outbound references displayed

  • verified exact0
  • verified fuzzy0
  • unresolved0
  • 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 543b85a7-91d2-445d-a997-d54e52365c03 · inbound

Star-forming clump detection in nearby galaxies using Faster R-CNN and $ugrizy$ imaging data from CLAUDS and HSC-SSP cites this paper.

Star-forming clump detection in nearby galaxies using Faster R-CNN and $ugrizy$ imaging data from CLAUDS and HSC-SSP A Comparison of Deep Learning Architectures for Optical Galaxy Morphology Classification

Reference 28

Resolution
unresolved
no resolver link, observed 2026-07-11T21:10:16.126324Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-11T21:10:16.126324Z digest=sha256:bf97bf4f11d0cb2ad6a7778af9b02798f1ddfdb3bde17634c0ed0e34e4c926bc

Observation 6a722708-9d4f-41bc-85b2-03fa0e3b7ba6 · inbound

Star-forming clump detection in nearby galaxies using Faster R-CNN and $ugrizy$ imaging data from CLAUDS and HSC-SSP cites this paper.

Star-forming clump detection in nearby galaxies using Faster R-CNN and $ugrizy$ imaging data from CLAUDS and HSC-SSP A Comparison of Deep Learning Architectures for Optical Galaxy Morphology Classification

Reference 28

Resolution
unresolved
no resolver link, observed 2026-08-02T08:46:54.783692Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T08:46:54.783692Z digest=sha256:bfa9c0a5184a416960d34392f772bf11497de6c7d78bb9f59ad3177d9212f5a4