Paper Citation Record · LEDGER

The WiggleZ Dark Energy Survey: the growth rate of cosmic structure since redshift z=0.9

As of 4 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 11 inbound Pith citation observations for arXiv:1104.2948.

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pith.paper-citation-record.v1
1104.2948 v1

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measured 11 of 11 standing notices

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Source: scholarly_work_events, retraction_status_cache, observed 2026-08-04T06:34:03.388597+00:00

measured 11 of 11 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-03T07:07:18.855675Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-06-30T15:14:47.132215Z

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Outbound references

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Pith citing papers

Observation fb94383a-95fd-4f43-80c7-4ae4bef7094e · inbound

Modified Gravity and Cosmology cites this paper.

Modified Gravity and Cosmology The WiggleZ Dark Energy Survey: the growth rate of cosmic structure since redshift z=0.9

Reference 165

Resolution: verified exact; arxiv_id, observed 2026-05-13T13:08:19.787093Z

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MUltiplexed Survey Telescope (MUST) Science White Paper I: Overview of Large-Scale Structure Cosmology in the Era of Stage-V Spectroscopic Surveys cites this paper.

MUltiplexed Survey Telescope (MUST) Science White Paper I: Overview of Large-Scale Structure Cosmology in the Era of Stage-V Spectroscopic Surveys The WiggleZ Dark Energy Survey: the growth rate of cosmic structure since redshift z=0.9

Reference 298

Resolution: verified exact; local_arxiv, observed 2026-05-23T17:45:45.801452Z

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Observation a1c8bbb8-a39e-4cd7-b5cd-97ab61d50576 · inbound

Tomographic Alcock-Paczynski Test with Marked Correlation Functions cites this paper.

Tomographic Alcock-Paczynski Test with Marked Correlation Functions The WiggleZ Dark Energy Survey: the growth rate of cosmic structure since redshift z=0.9

Reference 8

Resolution: verified exact; local_arxiv, observed 2026-05-22T18:56:57.894283Z

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Observation c343f49e-c33a-4465-9e4d-3bde5fc102ce · inbound

Modeling nonlinear scales for dynamical dark energy cosmologies with COLA cites this paper.

Modeling nonlinear scales for dynamical dark energy cosmologies with COLA The WiggleZ Dark Energy Survey: the growth rate of cosmic structure since redshift z=0.9

Reference 61

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Observation c6672995-81e9-4d78-b979-5c60738f446c · inbound

Realizing the phantom-divide crossing with vector and scalar fields cites this paper.

Realizing the phantom-divide crossing with vector and scalar fields The WiggleZ Dark Energy Survey: the growth rate of cosmic structure since redshift z=0.9

Reference 115

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Observation af9cabe8-6376-46f6-909a-0e7c7385b0c5 · inbound

Signatures of Modified Gravity on Linear Scales in a Dynamical Dark Energy Background cites this paper.

Signatures of Modified Gravity on Linear Scales in a Dynamical Dark Energy Background The WiggleZ Dark Energy Survey: the growth rate of cosmic structure since redshift z=0.9

Reference 110

Resolution: verified exact; local_arxiv, observed 2026-05-22T05:41:08.976862Z

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Observation fb983d51-962e-45c0-9fa7-37cdc34ab411 · inbound

Signatures of Modified Gravity on Linear Scales in a Dynamical Dark Energy Background cites this paper.

Signatures of Modified Gravity on Linear Scales in a Dynamical Dark Energy Background The WiggleZ Dark Energy Survey: the growth rate of cosmic structure since redshift z=0.9

Reference 110

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Observation 570e99fb-985d-4de0-a82a-4a92ffa7b1bc · inbound

Cosmological constraints from neighbor-density-weighted marked correlation functions cites this paper.

Cosmological constraints from neighbor-density-weighted marked correlation functions The WiggleZ Dark Energy Survey: the growth rate of cosmic structure since redshift z=0.9

Reference 26

Resolution: verified exact; local_arxiv, observed 2026-05-25T03:30:17.265427Z

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Observation 60d49ea0-b673-4fe3-bba4-09a620cb47af · inbound

Cosmological constraints from neighbor-density-weighted marked correlation functions cites this paper.

Cosmological constraints from neighbor-density-weighted marked correlation functions The WiggleZ Dark Energy Survey: the growth rate of cosmic structure since redshift z=0.9

Reference 26

Resolution: verified exact; local_arxiv, observed 2026-06-30T15:14:47.133379Z

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Observation 8896f70d-a104-48fb-a6f6-1166affce3f3 · inbound

Cosmological Constraints from Bias-Robust Wavelet Scattering Statistics for Stage-IV Galaxy Surveys cites this paper.

Cosmological Constraints from Bias-Robust Wavelet Scattering Statistics for Stage-IV Galaxy Surveys The WiggleZ Dark Energy Survey: the growth rate of cosmic structure since redshift z=0.9

Reference 9

Resolution: verified exact; local_arxiv, observed 2026-06-29T16:33:39.561136Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation 2bfe305b-ece7-4364-a184-21aae11f5ede · inbound

Late-time cosmological constraints on three holographic dark energy models with DESI DR2 BAO and Type Ia supernovae cites this paper.

Late-time cosmological constraints on three holographic dark energy models with DESI DR2 BAO and Type Ia supernovae The WiggleZ Dark Energy Survey: the growth rate of cosmic structure since redshift z=0.9

Reference 94

Resolution: unresolved; no resolver link, observed 2026-07-14T16:44:02.461654Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.