Paper Citation Record · LEDGER

Measuring the galaxy power spectrum with future redshift surveys

As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:astro-ph/9708020.

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

pith.paper-citation-record.v1
astro-ph/9708020 v2

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measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 3 of 3 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-10T06:31:04.303077+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-10T06:07:09.906689Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-11T12:31:06.943365Z

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0 of 0 outbound references displayed

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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 a8bb0736-e7f9-4600-85f9-deda71b14e51 · inbound

Sound Mode and Scale-Dependent Growth in Two-Fluid Dynamical Dark Energy cites this paper.

Sound Mode and Scale-Dependent Growth in Two-Fluid Dynamical Dark Energy Measuring the galaxy power spectrum with future redshift surveys

Reference 131

Resolution: unresolved; no resolver link, observed 2026-07-15T14:51:12.413085Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 02678276-266a-4c91-a26d-59f2e8b2bdbd · inbound

If at First You Don't Succeed, Trispectrum: I. Estimating the Matter Power Spectrum Covariance with Higher-Order Statistics cites this paper.

If at First You Don't Succeed, Trispectrum: I. Estimating the Matter Power Spectrum Covariance with Higher-Order Statistics Measuring the galaxy power spectrum with future redshift surveys

Reference 69

Resolution: verified exact; arxiv_id, observed 2026-07-04T15:53:45.688770Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

Observation 578949ef-e3eb-44c6-9e30-c56794b20e9e · inbound

Sample Variance Cancellation for Future Spectroscopic Surveys cites this paper.

Sample Variance Cancellation for Future Spectroscopic Surveys Measuring the galaxy power spectrum with future redshift surveys

Reference 31

Resolution: unresolved; no resolver link, observed 2026-08-10T06:07:09.906689Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.