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Paper Citation Record · LEDGER

The bending of the star-forming main sequence traces the cold- to hot-accretion transition mass over 0<z<4

As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2203.10880.

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

pith.paper-citation-record.v1
2203.10880 v2

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 2026-08-10T06:31:04.303077+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-02T02:50:46.131127Z

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 0371859f-6fef-4cc7-bde5-933e50a3e502 · inbound

Cold Stream Penetration of Virial Shocks: Fragmentation, Coagulation, and Disruption in the Hot Circumgalactic Medium cites this paper.

Cold Stream Penetration of Virial Shocks: Fragmentation, Coagulation, and Disruption in the Hot Circumgalactic Medium The bending of the star-forming main sequence traces the cold- to hot-accretion transition mass over 0<z<4

Reference 59

Resolution
unresolved
no resolver link, observed 2026-08-02T02:50:46.131127Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T02:50:46.131127Z digest=sha256:b703f964e12067a91601dd03b2d1c629d6098c652adcdc3a029953ed422cfc27

Observation 1c3415f1-cec7-4635-a6a5-c1c14d967717 · inbound

Cosmic ray heating of cold streams: Implications for the gas supply and growth of massive galaxies cites this paper.

Cosmic ray heating of cold streams: Implications for the gas supply and growth of massive galaxies The bending of the star-forming main sequence traces the cold- to hot-accretion transition mass over 0<z<4

Reference 36

Resolution
unresolved
no resolver link, observed 2026-07-31T14:25:21.927315Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-31T14:25:21.927315Z digest=sha256:f0b7e99bef9e212bcdccae3eee5ad9dcfe6575e8929c5d00dee01faa144aa103