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Paper Citation Record · LEDGER

Iterative initial condition reconstruction

As of 15 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 7 inbound Pith citation observations for arXiv:1704.06634.

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

pith.paper-citation-record.v1
1704.06634 v3

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 7 of 7 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 7 of 7 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-11T21:56:23.356264Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-02T10:26:52.050083Z

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External citation measurements

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Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 89d8ade7-fc57-4b03-add1-fbdc6f452abd · inbound

DESI 2024 III: Baryon Acoustic Oscillations from Galaxies and Quasars cites this paper.

DESI 2024 III: Baryon Acoustic Oscillations from Galaxies and Quasars Iterative initial condition reconstruction

Reference 107

Resolution
verified exact
arxiv_id, observed 2026-05-17T06:34:54.619174Z

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.

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Observation dc295b45-6c09-440c-98ea-518fb9db5bd7 · inbound

Restoring Missing Modes of 21cm Intensity Mapping with Deep Learning: Impact on BAO Reconstruction cites this paper.

Restoring Missing Modes of 21cm Intensity Mapping with Deep Learning: Impact on BAO Reconstruction Iterative initial condition reconstruction

Reference 73

Resolution
unresolved
no resolver link, observed 2026-08-11T21:56:23.356264Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation 538fc89c-4d58-4b21-bdcb-45e7a1d31bb1 · inbound

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

DISCO-DJ II: a differentiable particle-mesh code for cosmology Iterative initial condition reconstruction

Reference 37

Resolution
unresolved
no resolver link, observed 2026-08-04T11:25:28.286327Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-04T11:25:28.286327Z digest=sha256:65c76963bfddf604f6f41a20a59371aaf8300309cbddb9d9652637a0d24c0def

Observation 980a7d62-0d75-475a-bc54-40efd1fa7ddb · 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 Iterative initial condition reconstruction

Reference 55

Resolution
unresolved
no resolver link, observed 2026-08-04T06:27:21.711382Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-04T06:27:21.711382Z digest=sha256:b92b64e03a0bf3ec98b2f0dfa62c31f872290d439d947763cfe29670cf16c311

Observation 15e26064-edac-41b1-a73e-636815dc5c6a · inbound

Cosmic variance or galaxy bias? Disentangling finite-volume and galaxy formation effects in cosmological analysis cites this paper.

Cosmic variance or galaxy bias? Disentangling finite-volume and galaxy formation effects in cosmological analysis Iterative initial condition reconstruction

Reference 31

Resolution
verified exact
arxiv_id, observed 2026-07-02T10:26:52.051411Z

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=2026-06-28T05:03:06.464090Z digest=sha256:ba0280ea866e18fdeb9aacfc8fcac172d41347a4fc9f7c506cd6dd4b6306e6d5

Observation 4ad1452b-7bcd-4808-b686-702ac4a865cb · inbound

Cosmic variance or galaxy bias? Disentangling finite-volume and galaxy formation effects in cosmological analysis cites this paper.

Cosmic variance or galaxy bias? Disentangling finite-volume and galaxy formation effects in cosmological analysis Iterative initial condition reconstruction

Reference 31

Resolution
unresolved
no resolver link, observed 2026-07-12T15:09:49.195956Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-07-12T15:09:49.195956Z digest=sha256:59c9389c0f8447994ff896cc307bbe9e961f1bf1e8fc022f02fec3f5bcac96e1

Observation 8083e3f4-5e73-4711-8e80-55f77e076b97 · 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 Iterative initial condition reconstruction

Reference 39

Resolution
unresolved
no resolver link, observed 2026-08-01T22:12:37.867388Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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