Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links, observed 2026-08-16T11:41:06.584967Z
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 20 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.
Coverage vector
One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-19T06:32:44.657259+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-07T13:18:44.240925Z
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
Source-reported events for the cited work
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
Source-reported events for the cited work
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 2026-08-19T06:32:44.657259+00:00.
Observation be911dd1-ce90-4ae3-9145-06cfd6724437 · outbound
This paper cites 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 2026-08-19T06:32:44.657259+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 2026-08-19T06:32:44.657259+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 2026-08-19T06:32:44.657259+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 2026-08-19T06:32:44.657259+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 2026-08-19T06:32:44.657259+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 2026-08-19T06:32:44.657259+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 2026-08-19T06:32:44.657259+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 2026-08-19T06:32:44.657259+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 2026-08-19T06:32:44.657259+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.