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Paper Citation Record · LEDGER

A Hybrid AMR Application for Cosmology and Astrophysics

As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:astro-ph/9710187.

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

pith.paper-citation-record.v1
astro-ph/9710187 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 2026-08-11T06:34:44.6726+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-10T16:43:48.854850Z

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
  • unresolved0
  • parse uncertain0
  • malformed identifier0
  • metadata mismatch0

External citation measurements

11
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation d376100d-420c-4f94-ab6a-ee04c289cb6a · inbound

Can supermassive stars form in protogalaxies due to internal Lyman-Werner feedback? cites this paper.

Can supermassive stars form in protogalaxies due to internal Lyman-Werner feedback? A Hybrid AMR Application for Cosmology and Astrophysics

Reference 19

Resolution
unresolved
no resolver link, observed 2026-08-10T16:43:48.854850Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T16:43:48.854850Z digest=sha256:6652f6b5996d665a32ef01c836881282201808e9fe17910c7401c43a8cd3b702

Observation f6847fbd-4c24-4d61-85cd-0dd8dbbe5cd1 · inbound

ArkenstoneBH. A model for high-specific energy black hole feedback in cosmological simulations cites this paper.

ArkenstoneBH. A model for high-specific energy black hole feedback in cosmological simulations A Hybrid AMR Application for Cosmology and Astrophysics

Reference 27

Resolution
verified exact
arxiv_id, observed 2026-05-13T17:53:03.217442Z

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=2026-05-08T17:26:07.513278Z digest=sha256:7184dea153f6dd0504ddc1c46b25f213921c5a6038af6338e45b2c0b843973f1

Observation 9b59c8b4-6b79-4db0-9cdc-7c30b6990397 · inbound

Variability in Cosmological Hydrodynamical Simulations: how Stochastic Processes, Numerical Effects, and Reproducibility Limits impact Predictability cites this paper.

Variability in Cosmological Hydrodynamical Simulations: how Stochastic Processes, Numerical Effects, and Reproducibility Limits impact Predictability A Hybrid AMR Application for Cosmology and Astrophysics

Reference 185

Resolution
verified exact
local_arxiv, observed 2026-06-27T00:30:16.823224Z

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=2026-06-27T00:10:27.498005Z digest=sha256:e18596884c458d5b3b21a72b86166f12a5e6a5a5ce73c499f148bdb49529acfb