Pith. sign in

Paper Citation Record · LEDGER

Effective cosmic density field reconstruction with convolutional neural network

As of 15 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:2306.10538.

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

pith.paper-citation-record.v1
2306.10538 v1

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 2026-08-15T06:32:42.880941+00:00

measured 5 of 5 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-12T04:54:06.382311Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-12T00:31:19.422201Z

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 939f7a6a-17fe-4192-b72e-690e2c87b238 · inbound

Probing primordial non-Gaussianity by reconstructing the initial conditions cites this paper.

Probing primordial non-Gaussianity by reconstructing the initial conditions Effective cosmic density field reconstruction with convolutional neural network

Reference 59

Resolution
unresolved
no resolver link, observed 2026-08-12T04:54:06.382311Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-12T04:54:06.382311Z digest=sha256:1196822e81eee35a1fb9a5f3077e195789663721123793417f1a25e1c831c050

Observation 1cd9a077-7481-47fe-8bc8-accd1a748683 · inbound

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

Non-Gaussian Galaxy Stochasticity and the Noise-Field Formulation Effective cosmic density field reconstruction with convolutional neural network

Reference 16

Resolution
unresolved
no resolver link, observed 2026-08-03T23:38:16.512394Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-03T23:38:16.512394Z digest=sha256:78942e8235c996a792d1acd7b516726cec3a1f40881953004505ab2a3a9a9262

Observation 16e4a4a7-63cc-448f-be0c-17c2697b9977 · 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 Effective cosmic density field reconstruction with convolutional neural network

Reference 59

Resolution
unresolved
no resolver link, observed 2026-08-04T06:27:21.951729Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-04T06:27:21.951729Z digest=sha256:45eff5972c803ece2baf2c52da35336d2ed28dd7fc3c47384411c6a43828d1fa

Observation c9c3501d-81d6-4a2f-976b-886de237e49b · 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 Effective cosmic density field reconstruction with convolutional neural network

Reference 13

Resolution
verified exact
arxiv_id, observed 2026-05-12T00:31:19.426083Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

source=pdf_text observed=2026-05-07T15:04:42.546535Z digest=sha256:8744ee1b58e62c63582cc25ace24f3f5b46c5bb0d052d675522cd9a5051063e9

Observation d7dc32f3-3cc2-4232-bf66-8370bde9ff97 · 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 Effective cosmic density field reconstruction with convolutional neural network

Reference 31

Resolution
unresolved
no resolver link, observed 2026-08-01T22:12:37.125654Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T22:12:37.125654Z digest=sha256:21b42f04dc966f8bd84c2be3c552b0a4507dfac64ac27460c1e69ae697639b39