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Paper Citation Record · LEDGER

Thermal and Fragmentation Properties of Star-forming Clouds in Low-metallicity Environments

As of 12 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:astro-ph/0503010.

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

pith.paper-citation-record.v1
astro-ph/0503010 v1

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 2026-08-11T06:34:44.6726+00:00

measured 5 of 5 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-10T22:18:28.241277Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-06-28T21:02:38.386889Z

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 a87bf9a4-baf6-4692-917d-c33d9a6f4e83 · inbound

Abundant Water from Early Supernovae at Cosmic Dawn cites this paper.

Abundant Water from Early Supernovae at Cosmic Dawn Thermal and Fragmentation Properties of Star-forming Clouds in Low-metallicity Environments

Reference 48

Resolution
unresolved
no resolver link, observed 2026-08-10T22:18:28.241277Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T22:18:28.241277Z digest=sha256:5f04b0ca39ef82dc392682b5cd0b0925ccc00c93a5401f34a2502a78376b4cf8

Observation 248971ca-3c44-4400-aa8a-4f61e0668b42 · inbound

Introducing the Lumina project: large-volume radiation-hydrodynamic simulations of the epochs of hydrogen and helium reionization cites this paper.

Introducing the Lumina project: large-volume radiation-hydrodynamic simulations of the epochs of hydrogen and helium reionization Thermal and Fragmentation Properties of Star-forming Clouds in Low-metallicity Environments

Reference 46

Resolution
verified exact
local_arxiv, observed 2026-05-19T16:17:39.273520Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:00db0aed61b583b67527298c0de79eaba1add8971aa67731488ff23b01e1a476

Observation 668e69b3-0645-43a0-bef0-17ee86e87a1e · inbound

Numerical simulations of shock-driven, supersonic turbulence in colliding three-temperature laboratory plasmas cites this paper.

Numerical simulations of shock-driven, supersonic turbulence in colliding three-temperature laboratory plasmas Thermal and Fragmentation Properties of Star-forming Clouds in Low-metallicity Environments

Reference 199

Resolution
metadata mismatch
local_arxiv, observed 2026-05-22T08:11:16.198465Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:b503795f34cc98bdfd16ef1f89e78c22854dfc366381c563011002bd04df0b22

Observation 3c097f0c-715c-405d-af5c-e2da241a9279 · inbound

21cmEMUv3: a hybrid diffusion-LSTM emulator of 21cmFAST summary observables cites this paper.

21cmEMUv3: a hybrid diffusion-LSTM emulator of 21cmFAST summary observables Thermal and Fragmentation Properties of Star-forming Clouds in Low-metallicity Environments

Reference 31

Resolution
verified exact
local_arxiv, observed 2026-06-28T21:02:38.388184Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:ad4ae4354630e03820b76a5bfb6ab738b0a9481d46d822d45ba604a9bb888b6d

Observation 5a544148-fabc-4ac7-81fc-965b782bb75d · inbound

The evolution of the galaxy gas-phase mass-metallicity relation from $z=15$ to $z=0$ in the COLIBRE cosmological simulations cites this paper.

The evolution of the galaxy gas-phase mass-metallicity relation from $z=15$ to $z=0$ in the COLIBRE cosmological simulations Thermal and Fragmentation Properties of Star-forming Clouds in Low-metallicity Environments

Reference 72

Resolution
verified exact
local_arxiv, observed 2026-06-27T04:20:32.810510Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:d81b45650d7ac6b0666b8321c8493d4cda64eaaaee83c9b2004f43d9df64d336