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Paper Citation Record · LEDGER

The baryonic Tully-Fisher relation of HI-bearing low-surface brightness galaxies implies their formation mechanism

As of 20 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:2403.16754.

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pith.paper-citation-record.v1
2403.16754 v4

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 4 of 4 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 4 of 4 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-12T18:36:54.252944Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-08-11T15:44:10.123092Z

Reference resolution

0 of 0 outbound references displayed

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Outbound references

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Pith citing papers

Observation d18daeba-41d2-4907-a171-fbe1647534de · inbound

Strong Correlation between Galactic HI-to-stellar Mass Ratio And Halo Spin Explored by HI-rich Galaxies cites this paper.

Strong Correlation between Galactic HI-to-stellar Mass Ratio And Halo Spin Explored by HI-rich Galaxies The baryonic Tully-Fisher relation of HI-bearing low-surface brightness galaxies implies their formation mechanism

Reference 37

Resolution
unresolved
no resolver link, observed 2026-08-12T18:36:54.252944Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation f1ca267f-5e6b-43e5-9735-f282c237a976 · inbound

Moderate Influence of Halo Spin on Stellar Mass Distributions in Dwarf and Massive Galaxies cites this paper.

Moderate Influence of Halo Spin on Stellar Mass Distributions in Dwarf and Massive Galaxies The baryonic Tully-Fisher relation of HI-bearing low-surface brightness galaxies implies their formation mechanism

Reference 28

Resolution
unresolved
no resolver link, observed 2026-08-12T17:54:54.585722Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation 330a6da5-44cd-493d-a9e0-4ab47d5e051d · inbound

Halo Spin Dependence on Environment for HI-bearing galaxies cites this paper.

Halo Spin Dependence on Environment for HI-bearing galaxies The baryonic Tully-Fisher relation of HI-bearing low-surface brightness galaxies implies their formation mechanism

Reference 15

Resolution
unresolved
no resolver link, observed 2026-08-12T17:53:29.377829Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation dadc9abf-6de9-4098-a141-ae5f138606a2 · inbound

Ultra Diffuse Dwarf Galaxies Hosting Pseudo-bulges cites this paper.

Ultra Diffuse Dwarf Galaxies Hosting Pseudo-bulges The baryonic Tully-Fisher relation of HI-bearing low-surface brightness galaxies implies their formation mechanism

Reference 34

Resolution
metadata mismatch
local_arxiv, observed 2026-08-11T15:44:10.130124Z

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=2026-08-11T15:44:09.898596Z digest=sha256:c7dec5dc1113b4812aaa5fecb417b8984d7cb0d291b65964572123116f70e4af