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Paper Citation Record · LEDGER

Invisible Accretion: Ionized Envelopes of TNG50 HVCs can Sustain Star Formation

As of 6 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 1 inbound Pith citation observation for arXiv:2507.18687.

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

pith.paper-citation-record.v1
2507.18687 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 1 of 1 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-06T06:34:29.942622+00:00

measured 1 of 1 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-01T10:03:33.184997Z

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

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  • malformed identifier0
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External citation measurements

No source-named external measurement is stored.

Outbound references

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Pith citing papers

Observation e0cde568-d0de-46d1-af11-f8032a91a20f · inbound

Gas accretion onto the Milky Way: high-velocity cloud survival and the revival of the terminal-velocity paradigm cites this paper.

Gas accretion onto the Milky Way: high-velocity cloud survival and the revival of the terminal-velocity paradigm Invisible Accretion: Ionized Envelopes of TNG50 HVCs can Sustain Star Formation

Reference 56

Resolution
unresolved
no resolver link, observed 2026-08-01T10:03:33.184997Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T10:03:33.184997Z digest=sha256:53a4bee9e2f6ee1ca27fe723339f48bb0a2d5e50edda17c3ea83196c7f0bc2be