Pith. sign in

Paper Citation Record · LEDGER

Cosmological SPH simulations: A hybrid multi-phase model for star formation

As of 22 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:astro-ph/0206393.

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

pith.paper-citation-record.v1
astro-ph/0206393 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 3 of 3 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-22T06:32:14.747728+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-12T00:58:57.623600Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-08-07T15:44:32.943239Z

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 666d3848-1aba-4381-a011-5a68d68a1ae0 · inbound

The Millennium and Astrid galaxies in effective field theory: comparison with galaxy-halo connection models at the field level cites this paper.

The Millennium and Astrid galaxies in effective field theory: comparison with galaxy-halo connection models at the field level Cosmological SPH simulations: A hybrid multi-phase model for star formation

Reference 116

Resolution
unresolved
no resolver link, observed 2026-08-12T00:58:57.623600Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-12T00:58:57.623600Z digest=sha256:026f81c298dc6af936e38bd3d6a47bd92fc8f2e5a81ec0fb285526e8be4bfb02

Observation 038aa66b-45b6-4245-b055-a83480c2bc26 · inbound

3D matter power spectrum correspondence to 1D Lyman-alpha flux power spectrum cites this paper.

3D matter power spectrum correspondence to 1D Lyman-alpha flux power spectrum Cosmological SPH simulations: A hybrid multi-phase model for star formation

Reference 22

Resolution
verified exact
local_arxiv, observed 2026-08-07T15:44:33.119284Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

source=pdf_text observed=2026-08-07T15:44:29.364916Z digest=sha256:da420616c09d14d12ea658d97ff00e9f239202462c1e6b4b1265ddb0adbd29b3

Observation b11752f2-7063-44f5-9b4e-c6ebddaa2025 · inbound

CRESCENDO II: Spectral cosmic rays with improved energy losses and realistic supernova seeding cites this paper.

CRESCENDO II: Spectral cosmic rays with improved energy losses and realistic supernova seeding Cosmological SPH simulations: A hybrid multi-phase model for star formation

Reference 134

Resolution
unresolved
no resolver link, observed 2026-08-02T02:26:46.955787Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T02:26:46.955787Z digest=sha256:1ae4e6520a9388733f7826a603471daa19aa77b1b674747853053ef1e31c4119