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Paper Citation Record · LEDGER

Non-universal star formation efficiency in turbulent ISM

As of 15 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:1512.03101.

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

pith.paper-citation-record.v1
1512.03101 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 2026-08-15T06:32:42.880941+00:00

measured 5 of 5 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-11T11:37:18.588956Z

measured 1 of 1 external citation measurements

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

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

Reference resolution

0 of 0 outbound references displayed

  • verified exact0
  • verified fuzzy0
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  • malformed identifier0
  • metadata mismatch0

External citation measurements

110
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 0125f96d-9610-426c-b636-aaab946badf7 · inbound

The effects of different cooling and heating function models on a simulated analog of NGC300 cites this paper.

The effects of different cooling and heating function models on a simulated analog of NGC300 Non-universal star formation efficiency in turbulent ISM

Reference 26

Resolution
unresolved
no resolver link, observed 2026-08-11T11:37:18.588956Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-11T11:37:18.588956Z digest=sha256:3b413b15ca9d26ae77c2265a429fe207b5596ae0f99ca1773840021a6c48c577

Observation 79d64767-faa5-473f-830e-ed3cfa62cdc9 · inbound

Cosmological Simulations of Galaxies cites this paper.

Cosmological Simulations of Galaxies Non-universal star formation efficiency in turbulent ISM

Reference 268

Resolution
unresolved
no resolver link, observed 2026-08-06T18:16:17.267911Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-06T18:16:17.267911Z digest=sha256:95aee0d762f4babbc20315f7b097161e7d956dc94fed8928216fa026c67f6cb6

Observation 2fc34c7f-90c6-469d-920a-6725d9e4c106 · inbound

The role of major mergers in triggering super-Eddington accretion cites this paper.

The role of major mergers in triggering super-Eddington accretion Non-universal star formation efficiency in turbulent ISM

Reference 122

Resolution
verified exact
local_arxiv, observed 2026-06-28T09:01:48.459592Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:8b73b720b1733be6e7dfb5475198bd103bada05da077051b79683c9cd97c69ec

Observation ba74d649-797f-4681-87d0-4e88e3128005 · inbound

mitigating the overcooling problem with sink-based bursty star formation in a high-z dwarf galaxy cites this paper.

mitigating the overcooling problem with sink-based bursty star formation in a high-z dwarf galaxy Non-universal star formation efficiency in turbulent ISM

Reference 23

Resolution
unresolved
no resolver link, observed 2026-07-13T06:20:04.707661Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-13T06:20:04.707661Z digest=sha256:830b5ec38b58347e24e6b3673ff2bbe5b7d9da07a9ee1ae194bfd79e4e779df0

Observation 7fb63c04-d638-4ab4-bcf8-cfd4dddcdbfc · inbound

Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity cites this paper.

Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity Non-universal star formation efficiency in turbulent ISM

Reference 235

Resolution
unresolved
no resolver link, observed 2026-08-01T14:10:57.199748Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T14:10:57.199748Z digest=sha256:a7ce63b03bb3b2f8e1b18866ebce9be630e0a20b21c251d4c80162371ad60879