Paper Citation Record · LEDGER

Gigaparsec structures are nowhere to be seen in $\Lambda$CDM: an enhanced analysis of LSS in FLAMINGO-10K simulations

As of 21 August 2026, this Paper Citation Record lists 22 of 22 outbound references and 3 inbound Pith citation observations for arXiv:2504.14940.

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

pith.paper-citation-record.v1
2504.14940 v1

Coverage vector

measured 22 of 22 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links, observed 2026-08-16T11:41:06.584967Z

measured 25 of 25 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-21T06:32:19.484+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-07T13:18:44.240925Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-11T11:41:06.268020Z

Reference resolution

22 of 22 outbound references displayed

verified exact7
verified fuzzy2
unresolved13
parse uncertain0
malformed identifier0
metadata mismatch0

External citation measurements

No source-named external measurement is stored.

Outbound references

Observation 52aa8e3b-fd5c-4ee7-944a-5076da136974 · outbound

This paper cites The Emperor's New Arc: gigaparsec patterns abound in a $\Lambda$CDM universe.

Gigaparsec structures are nowhere to be seen in $\Lambda$CDM: an enhanced analysis of LSS in FLAMINGO-10K simulations The Emperor's New Arc: gigaparsec patterns abound in a $\Lambda$CDM universe

Reference 1

Resolution: unresolved; no resolver link, observed 2026-08-16T11:41:06.500967Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a84e3f85-581d-480b-9086-14ce9b4d9744 · outbound

This paper cites A Giant Arc on the Sky.

Gigaparsec structures are nowhere to be seen in $\Lambda$CDM: an enhanced analysis of LSS in FLAMINGO-10K simulations A Giant Arc on the Sky

Reference 2

Resolution: unresolved; no resolver link, observed 2026-08-16T11:41:06.505838Z

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Unavailable: canonical work link unavailable.

Observation 0cee7f50-435d-463c-96e9-b73f13f1b4d8 · outbound

This paper cites A Big Ring on the Sky.

Gigaparsec structures are nowhere to be seen in $\Lambda$CDM: an enhanced analysis of LSS in FLAMINGO-10K simulations A Big Ring on the Sky

Reference 3

Resolution: unresolved; no resolver link, observed 2026-08-16T11:41:06.509739Z

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Unavailable: canonical work link unavailable.

Observation 91b33f4a-d661-449f-b83c-701fa9a2ef90 · outbound

This paper cites A structure in the early universe at z ~ 1.3 that exceeds the homogeneity scale of the R-W concordance cosmology.

Gigaparsec structures are nowhere to be seen in $\Lambda$CDM: an enhanced analysis of LSS in FLAMINGO-10K simulations A structure in the early universe at z ~ 1.3 that exceeds the homogeneity scale of the R-W concordance cosmology

Reference 4

Resolution: unresolved; no resolver link, observed 2026-08-16T11:41:06.513779Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 788ecd62-6a2e-40de-a00c-6d249efc8487 · outbound

This paper cites Two close Large Quasar Groups of size ~ 350 Mpc at z ~ 1.2.

Gigaparsec structures are nowhere to be seen in $\Lambda$CDM: an enhanced analysis of LSS in FLAMINGO-10K simulations Two close Large Quasar Groups of size ~ 350 Mpc at z ~ 1.2

Reference 5

Resolution: unresolved; no resolver link, observed 2026-08-16T11:41:06.518179Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 576b2ca8-d57c-42cb-987a-1fda36d0f6dd · outbound

This paper cites Seeing patterns in noise: Gigaparsec-scale `structures' that do not violate homogeneity.

Gigaparsec structures are nowhere to be seen in $\Lambda$CDM: an enhanced analysis of LSS in FLAMINGO-10K simulations Seeing patterns in noise: Gigaparsec-scale `structures' that do not violate homogeneity

Reference 6

Resolution: unresolved; no resolver link, observed 2026-08-16T11:41:06.522529Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 66b66bc0-7281-4fec-97ca-0abb7690f59c · outbound

This paper cites The Challenge of the Largest Structures in the Universe to Cosmology.

Gigaparsec structures are nowhere to be seen in $\Lambda$CDM: an enhanced analysis of LSS in FLAMINGO-10K simulations The Challenge of the Largest Structures in the Universe to Cosmology

Reference 7

Resolution: unresolved; no resolver link, observed 2026-08-16T11:41:06.527326Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 14f7b1af-a878-4bee-8ced-e56ed38f63b7 · outbound

This paper cites Large SDSS quasar groups and their statistical significance.

Gigaparsec structures are nowhere to be seen in $\Lambda$CDM: an enhanced analysis of LSS in FLAMINGO-10K simulations Large SDSS quasar groups and their statistical significance

Reference 8

Resolution: unresolved; no resolver link, observed 2026-08-16T11:41:06.531143Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 0c6f05d9-75be-4556-96e0-fa304cf6e342 · outbound

This paper cites Compatibility of the Large Quasar Groups with the Concordance Cosmological Model.

Gigaparsec structures are nowhere to be seen in $\Lambda$CDM: an enhanced analysis of LSS in FLAMINGO-10K simulations Compatibility of the Large Quasar Groups with the Concordance Cosmological Model

Reference 9

Resolution: verified exact; local_arxiv, observed 2026-08-16T11:41:06.749148Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

Observation be911dd1-ce90-4ae3-9145-06cfd6724437 · outbound

This paper cites Murtagh, A.

Gigaparsec structures are nowhere to be seen in $\Lambda$CDM: an enhanced analysis of LSS in FLAMINGO-10K simulations Murtagh, A

Reference 10

Resolution: verified fuzzy; raw_fallback, observed 2026-08-16T11:41:06.837704Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

Observation 58dd8a8f-9555-43a0-9ca2-ad4914f49142 · outbound

This paper cites Pilipenko,The space distribution of quasars, Astron.

Gigaparsec structures are nowhere to be seen in $\Lambda$CDM: an enhanced analysis of LSS in FLAMINGO-10K simulations Pilipenko,The space distribution of quasars, Astron

Reference 11

Resolution: verified fuzzy; raw_fallback, observed 2026-08-16T11:41:06.828991Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

Observation b17f364d-2d16-4d77-887b-2d538fda8bfc · outbound

This paper cites The Clustering of MgII Absorption Systems at z=0.5 and Detection of Cold Gas in Massive Halos.

Gigaparsec structures are nowhere to be seen in $\Lambda$CDM: an enhanced analysis of LSS in FLAMINGO-10K simulations The Clustering of MgII Absorption Systems at z=0.5 and Detection of Cold Gas in Massive Halos

Reference 12

Resolution: verified exact; local_arxiv, observed 2026-08-16T11:41:06.733895Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

Observation 22cc84df-c72e-4f4e-9e1d-bb1b009d3683 · outbound

This paper cites A Cross-Correlation Analysis of Mg II Absorption Line Systems and Luminous Red Galaxies from the SDSS DR5.

Gigaparsec structures are nowhere to be seen in $\Lambda$CDM: an enhanced analysis of LSS in FLAMINGO-10K simulations A Cross-Correlation Analysis of Mg II Absorption Line Systems and Luminous Red Galaxies from the SDSS DR5

Reference 13

Resolution: verified exact; local_arxiv, observed 2026-08-16T11:41:06.719438Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

Observation 7ea8808d-c854-4a65-a8fc-7cd2e3238663 · outbound

This paper cites The Cross-correlation of MgII Absorption and Galaxies in BOSS.

Gigaparsec structures are nowhere to be seen in $\Lambda$CDM: an enhanced analysis of LSS in FLAMINGO-10K simulations The Cross-correlation of MgII Absorption and Galaxies in BOSS

Reference 14

Resolution: verified exact; local_arxiv, observed 2026-08-16T11:41:06.706256Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

Observation 5dbea673-1350-41ea-b7a4-741bf78e1870 · outbound

This paper cites Determine the galaxy bias factors on large scales using bispectrum method.

Gigaparsec structures are nowhere to be seen in $\Lambda$CDM: an enhanced analysis of LSS in FLAMINGO-10K simulations Determine the galaxy bias factors on large scales using bispectrum method

Reference 15

Resolution: verified exact; local_arxiv, observed 2026-08-16T11:41:06.693386Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

Observation 98cbc15d-1a11-4b30-b1d7-24b64bde6e99 · outbound

This paper cites Clustering of MgII absorption line systems around massive galaxies: an important constraint on feedback processes in galaxy formation.

Gigaparsec structures are nowhere to be seen in $\Lambda$CDM: an enhanced analysis of LSS in FLAMINGO-10K simulations Clustering of MgII absorption line systems around massive galaxies: an important constraint on feedback processes in galaxy formation

Reference 16

Resolution: verified exact; local_arxiv, observed 2026-08-16T11:41:06.679989Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

Observation 99c20da8-dd9c-459e-bda1-756ba514a012 · outbound

This paper cites HBT+: an improved code for finding subhalos and building merger trees in cosmological simulations.

Gigaparsec structures are nowhere to be seen in $\Lambda$CDM: an enhanced analysis of LSS in FLAMINGO-10K simulations HBT+: an improved code for finding subhalos and building merger trees in cosmological simulations

Reference 17

Resolution: unresolved; no resolver link, observed 2026-08-16T11:41:06.565245Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c5b142d3-345e-4989-b35b-44dd620b2dd6 · outbound

This paper cites Assessing subhalo finders in cosmological hydrodynamical simulations.

Gigaparsec structures are nowhere to be seen in $\Lambda$CDM: an enhanced analysis of LSS in FLAMINGO-10K simulations Assessing subhalo finders in cosmological hydrodynamical simulations

Reference 18

Resolution: unresolved; no resolver link, observed 2026-08-16T11:41:06.568906Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 76f364ca-1c07-423e-9284-ccf54685de0d · outbound

This paper cites Fractal Dimension as a measure of the scale of Homogeneity.

Gigaparsec structures are nowhere to be seen in $\Lambda$CDM: an enhanced analysis of LSS in FLAMINGO-10K simulations Fractal Dimension as a measure of the scale of Homogeneity

Reference 19

Resolution: unresolved; no resolver link, observed 2026-08-16T11:41:06.573623Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 56d22dff-4d63-45cd-8ca7-600fdd687d49 · outbound

This paper cites A Map of the Universe.

Gigaparsec structures are nowhere to be seen in $\Lambda$CDM: an enhanced analysis of LSS in FLAMINGO-10K simulations A Map of the Universe

Reference 20

Resolution: unresolved; no resolver link, observed 2026-08-16T11:41:06.577383Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 8333e411-4942-4673-8140-708dd9746b8a · outbound

This paper cites Cosmicflows-3: The South Pole Wall.

Gigaparsec structures are nowhere to be seen in $\Lambda$CDM: an enhanced analysis of LSS in FLAMINGO-10K simulations Cosmicflows-3: The South Pole Wall

Reference 21

Resolution: verified exact; local_arxiv, observed 2026-08-16T11:41:06.629655Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

Observation 1ea6fd45-0e00-47f4-9a5c-107c7daaa025 · outbound

This paper cites Unveiling the largest structures in the nearby Universe: Discovery of the Quipu superstructure.

Gigaparsec structures are nowhere to be seen in $\Lambda$CDM: an enhanced analysis of LSS in FLAMINGO-10K simulations Unveiling the largest structures in the nearby Universe: Discovery of the Quipu superstructure

Reference 22

Resolution: unresolved; no resolver link, observed 2026-08-16T11:41:06.584967Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Pith citing papers

Observation 7ccaf758-ef92-4c88-b3cd-1bd489f572c5 · inbound

Constraining the Hubble parameter with the 21 cm brightness temperature signal in a universe with inhomogeneities cites this paper.

Constraining the Hubble parameter with the 21 cm brightness temperature signal in a universe with inhomogeneities Gigaparsec structures are nowhere to be seen in $\Lambda$CDM: an enhanced analysis of LSS in FLAMINGO-10K simulations

Reference 16

Resolution: unresolved; no resolver link, observed 2026-08-07T13:18:44.240925Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 89336781-50a8-4e26-addc-887a0791b1f8 · inbound

Optical depth to reionization in a Universe with multiple inhomogeneous domains cites this paper.

Optical depth to reionization in a Universe with multiple inhomogeneous domains Gigaparsec structures are nowhere to be seen in $\Lambda$CDM: an enhanced analysis of LSS in FLAMINGO-10K simulations

Reference 27

Resolution: verified exact; arxiv_id, observed 2026-05-11T11:41:06.269823Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

Observation b83cdae0-57c2-4099-9a01-c2d73daefa92 · inbound

Optical depth to reionization in a Universe with multiple inhomogeneous domains cites this paper.

Optical depth to reionization in a Universe with multiple inhomogeneous domains Gigaparsec structures are nowhere to be seen in $\Lambda$CDM: an enhanced analysis of LSS in FLAMINGO-10K simulations

Reference 27

Resolution: unresolved; no resolver link, observed 2026-07-12T20:37:56.268361Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.