Pith. sign in

Paper Citation Record · LEDGER

DEUS Full Observable {\Lambda}CDM Universe Simulation: the numerical challenge

As of 12 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1206.2838.

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

pith.paper-citation-record.v1
1206.2838 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 2 of 2 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-12T06:34:41.77262+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-03T04:06:12.482885Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-05-20T15:53:33.648281Z

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 bcea5e19-c565-448d-ad4e-0ac3f09d266a · inbound

Dynamic Zoom Simulations of structure formation beyond standard cosmology cites this paper.

Dynamic Zoom Simulations of structure formation beyond standard cosmology DEUS Full Observable {\Lambda}CDM Universe Simulation: the numerical challenge

Reference 4

Resolution
unresolved
no resolver link, observed 2026-08-03T04:06:12.482885Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-03T04:06:12.482885Z digest=sha256:dbd0b9b4852b39d74f4fe9a012d00f499de2da2720194d2879e7d3ff58b8288d

Observation c4e03de8-2b35-4088-ac9b-7fb87c93a8d5 · inbound

Feedback driven interactions between dark and luminous matter to explain tight galaxy scaling relations cites this paper.

Feedback driven interactions between dark and luminous matter to explain tight galaxy scaling relations DEUS Full Observable {\Lambda}CDM Universe Simulation: the numerical challenge

Reference 47

Resolution
metadata mismatch
local_arxiv, observed 2026-05-20T15:53:33.649876Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

source=arxiv_source observed=2026-05-20T15:53:21.021477Z digest=sha256:29de3075f7bf960cce61b2b621401db54e2e731e18fe229ee2062bb1d09560da