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Paper Citation Record · LEDGER

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

As of 8 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 6 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 6 of 6 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-08T06:32:00.761636+00:00

measured 6 of 6 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-07T04:48:07.683143Z

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 469b96fb-b4d5-45c4-b4fc-ddc15da92bc7 · inbound

CSST Cosmological Emulator II: Generalized Accurate Halo Mass Function Emulation cites this paper.

CSST Cosmological Emulator II: Generalized Accurate Halo Mass Function Emulation The Mira-Titan Universe IV. High Precision Power Spectrum Emulation

Reference 63

Resolution
unresolved
no resolver link, observed 2026-08-07T04:48:07.683143Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T04:48:07.683143Z digest=sha256:7cb0d4b6a0a3176324bbbb584eddc4ce5573685f0b894d3c8cccc04dbcf66f69

Observation 51eafe6a-ad29-4095-b101-f17c3893a726 · inbound

Extending CSST Emulator to post-DESI era cites this paper.

Extending CSST Emulator to post-DESI era The Mira-Titan Universe IV. High Precision Power Spectrum Emulation

Reference 35

Resolution
unresolved
no resolver link, observed 2026-08-04T10:39:32.397228Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-04T10:39:32.397228Z digest=sha256:08751df0aa71bdbacc72a8bb6a151f280e3617a8c2078d92e93168c8c2d8696c

Observation 7ce56c3a-79e2-4e8e-9c44-02742c2b8873 · inbound

CLiENT: A new tool for emulating cosmological likelihoods using deep neural networks cites this paper.

CLiENT: A new tool for emulating cosmological likelihoods using deep neural networks The Mira-Titan Universe IV. High Precision Power Spectrum Emulation

Reference 14

Resolution
unresolved
no resolver link, observed 2026-08-03T15:17:37.676487Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-03T15:17:37.676487Z digest=sha256:ac29acc40b8f64d89595e94f5ad0375ef6b243f1ff052d847493a92c0e0ea785

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 2026-08-08T06:32:00.761636+00:00.

source=pdf_text observed=2026-05-09T18:38:12.253954Z digest=sha256:c8d70fc19267fc39646762945f68ba90bc924e21993846a842d6bef0d4c8d59c

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 2026-08-08T06:32:00.761636+00:00.

source=pdf_text observed=2026-05-25T03:27:13.896349Z digest=sha256:ac00e485cfc83e9ce4a52ffc589b3e1abb9a2e30475eb121a3b4a02c34d9e414

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 2026-08-08T06:32:00.761636+00:00.

source=pdf_text observed=2026-06-30T15:08:32.960489Z digest=sha256:54589628379a286afc7ed616fac898968183021f7f36ed8927b7221c6bcea64d