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Paper Citation Record · LEDGER

RMS asymmetry: a robust metric of galaxy shapes in images with varied depth and resolution

As of 5 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:2404.05792.

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

pith.paper-citation-record.v1
2404.05792 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 5 of 5 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-05T06:32:48.257954+00:00

measured 5 of 5 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-02T08:46:56.967656Z

measured 1 of 1 external citation measurements

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

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

Reference resolution

0 of 0 outbound references displayed

  • verified exact0
  • verified fuzzy0
  • unresolved0
  • parse uncertain0
  • malformed identifier0
  • metadata mismatch0

External citation measurements

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

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 235a5b51-0027-49d3-abf5-dff834f28fb0 · inbound

Resolved Ages and Stellar Metallicities in Progenitors of Milky Way Analogs: A Closer Look at their Star Formation Histories since $z=5$ cites this paper.

Resolved Ages and Stellar Metallicities in Progenitors of Milky Way Analogs: A Closer Look at their Star Formation Histories since $z=5$ RMS asymmetry: a robust metric of galaxy shapes in images with varied depth and resolution

Reference 76

Resolution
verified exact
arxiv_id, observed 2026-06-26T13:39:31.122849Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-06-26T13:33:19.791535Z digest=sha256:565e5ead10de1039b4cd8faa3c7107b8356dc7c7f7e657015e4c1ef1787bc14c

Observation 70744714-a3d7-4738-a399-120e0d222ef1 · 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 RMS asymmetry: a robust metric of galaxy shapes in images with varied depth and resolution

Reference 275

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=sha256:4e344bd655d6bfccdbee018da70643f90d08e94fa95b60c8ff5533afa4a3bcd8

Observation 1721d31e-7210-4be8-8608-8eed3db1efcb · 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 RMS asymmetry: a robust metric of galaxy shapes in images with varied depth and resolution

Reference 275

Resolution
unresolved
no resolver link, observed 2026-08-02T08:46:56.967656Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T08:46:56.967656Z digest=sha256:c56f53e3b40f29acb1a9fd050b3ac260f7c566c739fe7a973c479bb8dc0869c3

Observation e5f27b19-c080-44f4-9795-4525669cc3ea · inbound

Performance of morphological classifiers for galaxy mergers compared to current machine learning methods cites this paper.

Performance of morphological classifiers for galaxy mergers compared to current machine learning methods RMS asymmetry: a robust metric of galaxy shapes in images with varied depth and resolution

Reference 27

Resolution
unresolved
no resolver link, observed 2026-07-13T04:41:12.165957Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-13T04:41:12.165957Z digest=sha256:d0f5f1230bc8dea6d1dfceb90bf956b355103f9bdb3fe5fc73f1d57684a48a7f

Observation 952645bd-23ce-4089-b87e-7154cfaa38b8 · inbound

Morphologies of SAGAbg low-mass galaxies in Legacy Survey multi-band imaging: dependence on stellar masses, star-formation rates and low-redshift evolution cites this paper.

Morphologies of SAGAbg low-mass galaxies in Legacy Survey multi-band imaging: dependence on stellar masses, star-formation rates and low-redshift evolution RMS asymmetry: a robust metric of galaxy shapes in images with varied depth and resolution

Reference 16

Resolution
unresolved
no resolver link, observed 2026-08-01T21:11:56.874572Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T21:11:56.874572Z digest=sha256:75b9c2d62440e161470e4d00e8db7932424338de6e2d4ee85af3b5d4e3aab5fd