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Paper Citation Record · LEDGER

The Mira-Titan Universe IV. High Precision Power Spectrum Emulation

As of 22 July 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2207.12345.

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

pith.paper-citation-record.v1
2207.12345 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 2026-07-20T06:30:07.809122+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-06-30T15:08:32.960489Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-06-30T15:14:47.289634Z

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 0ae02476-5658-4b07-a9a5-994e4ca80121 · inbound

$4\times3$ Point Correlation Functions in Galaxy Surveys: Impact of Baryonic Feedback cites this paper.

$4\times3$ Point Correlation Functions in Galaxy Surveys: Impact of Baryonic Feedback The Mira-Titan Universe IV. High Precision Power Spectrum Emulation

Reference 75

Resolution
verified exact
arxiv_id, observed 2026-05-11T16:11:07.964874Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-07-20T06:30:07.809122+00:00.

source=pdf_text observed=2026-05-09T18:38:12.253954Z digest=sha256:c7c0e837f793c92b7541118f75963c43f7f1546cda0a7d89b08991ad7533c498

Observation 087802df-8203-4d71-bf7a-e18340046522 · inbound

Cosmological constraints from neighbor-density-weighted marked correlation functions cites this paper.

Cosmological constraints from neighbor-density-weighted marked correlation functions The Mira-Titan Universe IV. High Precision Power Spectrum Emulation

Reference 76

Resolution
verified exact
arxiv_id, observed 2026-05-25T03:30:17.361855Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-07-20T06:30:07.809122+00:00.

source=pdf_text observed=2026-05-25T03:27:13.896349Z digest=sha256:a82c37a81b41a2dc46d2886ab47af483839268a6922d86aea424f702cc70dd6d

Observation 0ccda00c-183a-4df3-adeb-f07b5cd5bcdf · inbound

Cosmological constraints from neighbor-density-weighted marked correlation functions cites this paper.

Cosmological constraints from neighbor-density-weighted marked correlation functions The Mira-Titan Universe IV. High Precision Power Spectrum Emulation

Reference 76

Resolution
verified exact
arxiv_id, observed 2026-06-30T15:14:47.291093Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-07-20T06:30:07.809122+00:00.

source=pdf_text observed=2026-06-30T15:08:32.960489Z digest=sha256:f97da31222d9743fbafca2206a1279e33eb6b9cf35ab74531ddc747b67fe5198