Pith. sign in

Paper Citation Record · LEDGER

Introducing Enzo, an AMR Cosmology Application

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/0403044.

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

pith.paper-citation-record.v1
astro-ph/0403044 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 2026-08-10T17:19:39.621926Z

measured 1 of 1 external citation measurements

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

Source: arxiv_reference, 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

36
arxiv_reference, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation ce153c98-1369-4e07-bbdc-c532b53ad108 · 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? Introducing Enzo, an AMR Cosmology Application

Reference 54

Resolution
unresolved
no resolver link, observed 2026-08-10T16:43:48.985450Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T16:43:48.985450Z digest=sha256:0cbc440f1d9c4a7e1a297689c8c7b4341aadc90c3830b9d0823e47055c2d97a3

Observation c1f002f3-72cf-40ba-9f5f-54da55985050 · 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 Introducing Enzo, an AMR Cosmology Application

Reference 26

Resolution
verified exact
arxiv_id, observed 2026-05-13T17:48:05.696583Z

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=sha256:4a9bf8e06ffbbccfbe086cbf3ffadb85929093c8970904ec6e0311196e1dbeae

Observation 6279a792-9475-4997-9f3c-6aa95c8b0821 · inbound

Smoothed particle magnetohydrodynamics for simulations of galaxy and cosmic structure formation cites this paper.

Smoothed particle magnetohydrodynamics for simulations of galaxy and cosmic structure formation Introducing Enzo, an AMR Cosmology Application

Reference 33

Resolution
unresolved
no resolver link, observed 2026-08-10T17:19:39.621926Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T17:19:39.621926Z digest=sha256:48638c31f28b3cebceef3fa3bea0d798659c705108a57af071f83c35272434fd