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Paper Citation Record · LEDGER

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

As of 10 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 2026-08-09T06:31:02.800959+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:ad189b6c8d1acf22fb28d67e3db0164e64ff850b4fb5505f01a9b8af714ef13c

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:e020e85ca623488b2b01e18557aac32e137bf06e805834d8c615d44c135e6eff

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=sha256:274cc809a650e474eb2b260b18f0f035e933a173bb629b4ca8295f66c18565b4

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 2026-08-09T06:31:02.800959+00:00.

source=pdf_text observed=2026-05-09T18:38:12.253954Z digest=sha256:3ffee5b28ecb0686f5294636e43ffd77a9081623e5b6eddb1efada91b889c2c6

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 2026-08-09T06:31:02.800959+00:00.

source=pdf_text observed=2026-05-25T03:27:13.896349Z digest=sha256:2bb22c9409eb1ba3387298e287cb381f6ed0b324f86c056fcfb3b046b5d05a98

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 2026-08-09T06:31:02.800959+00:00.

source=pdf_text observed=2026-06-30T15:08:32.960489Z digest=sha256:356bf5b564b3216412195ed78a356d9f2ccf8490e341b6a3e426f3d9959e9e25