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Paper Citation Record · LEDGER

MaLeFiSenta: Machine Learning for FilamentS Identification and orientation in the ISM

As of 20 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2205.00683.

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

pith.paper-citation-record.v1
2205.00683 v2

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 2026-08-20T06:33:59.587034+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-16T00:44:22.494857Z

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

2
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 7f3a01a0-116d-48f9-99a5-1d56ee05ef74 · inbound

Fuzzy Galaxies or Cirrus? Decomposition of Galactic Cirrus in Deep Wide-Field Images cites this paper.

Fuzzy Galaxies or Cirrus? Decomposition of Galactic Cirrus in Deep Wide-Field Images MaLeFiSenta: Machine Learning for FilamentS Identification and orientation in the ISM

Reference 7

Resolution
unresolved
no resolver link, observed 2026-08-12T04:57:47.093660Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-12T04:57:47.093660Z digest=sha256:778ff0e8c41f11995f984cdb8e0626288ddb21c295055981b5c612a349bbc324

Observation a5782e36-2af1-4cd0-8ccb-cf6e6884c3a1 · inbound

The role of magnetic field and stellar feedback in the evolution of filamentary structures in collapsing star-forming clouds cites this paper.

The role of magnetic field and stellar feedback in the evolution of filamentary structures in collapsing star-forming clouds MaLeFiSenta: Machine Learning for FilamentS Identification and orientation in the ISM

Reference 3

Resolution
unresolved
no resolver link, observed 2026-08-16T00:44:22.494857Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:44:22.494857Z digest=sha256:3d2ebc18142a88fc9e2769b614e72aa1daa09bf30e265f865d19ff7dd221aa0b

Observation 95fa339d-d320-4f25-a79c-468e0d52cba9 · inbound

Automated void identification by Blendmask: from hierarchical molecular gas to hierarchical voids in NGC 628 cites this paper.

Automated void identification by Blendmask: from hierarchical molecular gas to hierarchical voids in NGC 628 MaLeFiSenta: Machine Learning for FilamentS Identification and orientation in the ISM

Reference 3

Resolution
verified exact
arxiv_id, observed 2026-06-29T06:23:08.557207Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=pdf_text observed=2026-06-29T06:05:22.636697Z digest=sha256:ac1fd38e5862b9da430ca826b9ffb424d6015d6718a21587172a5bb9e5d86e2f