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Paper Citation Record · LEDGER

Reconstructing Cosmological Initial Conditions from Late-Time Structure with Convolutional Neural Networks

As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:2207.12511.

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

pith.paper-citation-record.v1
2207.12511 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 5 of 5 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 5 of 5 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-04T11:25:28.655317Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-12T00:31:19.703195Z

Reference resolution

0 of 0 outbound references displayed

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  • 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 373cefd7-f549-49e2-814f-1faa9ea8092d · inbound

DISCO-DJ II: a differentiable particle-mesh code for cosmology cites this paper.

DISCO-DJ II: a differentiable particle-mesh code for cosmology Reconstructing Cosmological Initial Conditions from Late-Time Structure with Convolutional Neural Networks

Reference 41

Resolution
unresolved
no resolver link, observed 2026-08-04T11:25:28.655317Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-04T11:25:28.655317Z digest=sha256:da05f01275fd0f1ea43de2dbc13d83bdb6fac0ba63030ab6a9f23ea6e92b5bea

Observation bc792777-78e4-4058-83d6-74b1a561121c · inbound

Non-Gaussian Galaxy Stochasticity and the Noise-Field Formulation cites this paper.

Non-Gaussian Galaxy Stochasticity and the Noise-Field Formulation Reconstructing Cosmological Initial Conditions from Late-Time Structure with Convolutional Neural Networks

Reference 15

Resolution
unresolved
no resolver link, observed 2026-08-03T23:38:16.444472Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-03T23:38:16.444472Z digest=sha256:88399dd70d198306f4ba72ad8fc8f9b38670968e1d12fa41d6be82b347909ea2

Observation 480ab389-2af9-47b8-8594-13d5fb0ff97e · inbound

The Linear Point Standard Ruler with DESI DR1 and DR2 Data cites this paper.

The Linear Point Standard Ruler with DESI DR1 and DR2 Data Reconstructing Cosmological Initial Conditions from Late-Time Structure with Convolutional Neural Networks

Reference 60

Resolution
unresolved
no resolver link, observed 2026-08-04T06:27:22.038477Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-04T06:27:22.038477Z digest=sha256:18c0300a6724c56b34cc2c184ac6955e616fd8046fd884333764118518102c39

Observation 2165150b-67fd-463e-9512-a39c41833082 · inbound

On the Relation Between Field-Level Posteriors, Correlators, and their Likelihoods cites this paper.

On the Relation Between Field-Level Posteriors, Correlators, and their Likelihoods Reconstructing Cosmological Initial Conditions from Late-Time Structure with Convolutional Neural Networks

Reference 12

Resolution
verified exact
arxiv_id, observed 2026-05-12T00:31:19.707397Z

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=2026-05-07T15:04:42.546535Z digest=sha256:8881430b60c4991671ab588e6024ffc10570f0139f35e7c5e7a9a8f577bafc2f

Observation 7b09de8b-2bf2-4917-9ef5-23b1920bccb6 · inbound

Standard Reconstruction Shifts the Optimal Input Scale for CNN-Based Density-Field Reconstruction cites this paper.

Standard Reconstruction Shifts the Optimal Input Scale for CNN-Based Density-Field Reconstruction Reconstructing Cosmological Initial Conditions from Late-Time Structure with Convolutional Neural Networks

Reference 12

Resolution
unresolved
no resolver link, observed 2026-08-01T22:12:35.451394Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T22:12:35.451394Z digest=sha256:4a83ff9642e29a75e4fb66f88043b0c72e97a08f6fa14dc7497da09dae59429e