Void spin distribution as a powerful probe of $\sigma_{8}$ | Paper Citation Record

Observation 56a0739d-6d39-4295-ba80-b9858b52fdf8 · outbound

This paper cites Voids in the PSCz Survey and the Updated Zwicky Catalog.

Void spin distribution as a powerful probe of $\sigma_{8}$ Voids in the PSCz Survey and the Updated Zwicky Catalog

Reference 1

Resolution: unresolved; no resolver link, observed 2026-08-10T20:04:03.397239Z

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Observation b64e1c17-2c40-46bb-bd7d-3e9298e7f2d4 · outbound

This paper cites AbacusSummit: A Massive Set of High-Accuracy, High-Resolution $N$-Body Simulations.

Void spin distribution as a powerful probe of $\sigma_{8}$ AbacusSummit: A Massive Set of High-Accuracy, High-Resolution $N$-Body Simulations

Reference 2

Resolution: unresolved; no resolver link, observed 2026-08-10T20:04:03.400747Z

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Observation 41b416be-7fe9-4c86-b7f6-25a0f6ce8a62 · outbound

This paper cites Planck 2013 results. XVI. Cosmological parameters.

Void spin distribution as a powerful probe of $\sigma_{8}$ Planck 2013 results. XVI. Cosmological parameters

Reference 3

Resolution: unresolved; no resolver link, observed 2026-08-10T20:04:03.403875Z

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Observation 2e17b64b-5fc2-4151-b609-b6a369b318b6 · outbound

This paper cites A 2.4% Determination of the Local Value of the Hubble Constant.

Void spin distribution as a powerful probe of $\sigma_{8}$ A 2.4% Determination of the Local Value of the Hubble Constant

Reference 4

Resolution: unresolved; no resolver link, observed 2026-08-10T20:04:03.406928Z

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Observation 7f5e5a1d-b8c5-4313-b88b-5b93c91728e3 · outbound

This paper cites The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Cosmological Implications from two Decades of Spectroscopic Surveys at the Apache Point observatory.

Void spin distribution as a powerful probe of $\sigma_{8}$ The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Cosmological Implications from two Decades of Spectroscopic Surveys at the Apache Point observatory

Reference 5

Resolution: unresolved; no resolver link, observed 2026-08-10T20:04:03.409916Z

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Observation 83d0d798-b921-4c6e-8eec-f35615652ea5 · outbound

This paper cites In the Realm of the Hubble tension $-$ a Review of Solutions.

Void spin distribution as a powerful probe of $\sigma_{8}$ In the Realm of the Hubble tension $-$ a Review of Solutions

Reference 6

Resolution: unresolved; no resolver link, observed 2026-08-10T20:04:03.412851Z

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Observation 2b3084c3-3d54-4b4b-8d5a-2812d16b65cd · outbound

This paper cites CFHTLenS revisited: assessing concordance with Planck including astrophysical systematics.

Void spin distribution as a powerful probe of $\sigma_{8}$ CFHTLenS revisited: assessing concordance with Planck including astrophysical systematics

Reference 7

Resolution: unresolved; no resolver link, observed 2026-08-10T20:04:03.416124Z

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Observation 76123c2f-7c1e-4de4-8b89-4c1de9505e5f · outbound

This paper cites KiDS-450: Cosmological parameter constraints from tomographic weak gravitational lensing.

Void spin distribution as a powerful probe of $\sigma_{8}$ KiDS-450: Cosmological parameter constraints from tomographic weak gravitational lensing

Reference 8

Resolution: unresolved; no resolver link, observed 2026-08-10T20:04:03.418636Z

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Observation cb9041ef-4003-47d9-8084-4b18d5d71886 · outbound

This paper cites Hints, neutrino bounds and WDM constraints from SDSS DR14 Lyman-$\alpha$ and Planck full-survey data.

Void spin distribution as a powerful probe of $\sigma_{8}$ Hints, neutrino bounds and WDM constraints from SDSS DR14 Lyman-$\alpha$ and Planck full-survey data

Reference 9

Resolution: unresolved; no resolver link, observed 2026-08-10T20:04:03.422143Z

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Observation 145951c6-1c40-48a5-8c21-aabb1d2ce0e8 · outbound

This paper cites KiDS+VIKING-450 and DES-Y1 combined: Mitigating baryon feedback uncertainty with COSEBIs.

Void spin distribution as a powerful probe of $\sigma_{8}$ KiDS+VIKING-450 and DES-Y1 combined: Mitigating baryon feedback uncertainty with COSEBIs

Reference 10

Resolution: unresolved; no resolver link, observed 2026-08-10T20:04:03.424815Z

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Observation e31e55a6-bfae-4efb-9ab8-761774dd1cb7 · outbound

This paper cites KiDS-1000 Cosmology: Multi-probe weak gravitational lensing and spectroscopic galaxy clustering constraints.

Void spin distribution as a powerful probe of $\sigma_{8}$ KiDS-1000 Cosmology: Multi-probe weak gravitational lensing and spectroscopic galaxy clustering constraints

Reference 11

Resolution: unresolved; no resolver link, observed 2026-08-10T20:04:03.428610Z

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Observation 577b0d0d-600b-49a0-8df8-d0ff0c6d9d7e · outbound

This paper cites an unresolved cited work.

Void spin distribution as a powerful probe of $\sigma_{8}$ Unresolved cited work

Reference 12

Resolution: unresolved; no resolver link, observed 2026-08-10T20:04:03.431799Z

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Observation de7e58f8-bb5f-4b13-a34a-19eac9dc6e36 · outbound

This paper cites Hyper Suprime-Cam Year 3 Results: Cosmology from Cosmic Shear Two-point Correlation Functions.

Void spin distribution as a powerful probe of $\sigma_{8}$ Hyper Suprime-Cam Year 3 Results: Cosmology from Cosmic Shear Two-point Correlation Functions

Reference 13

Resolution: unresolved; no resolver link, observed 2026-08-10T20:04:03.435134Z

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Observation 32b29872-4bc7-438d-ad07-657b48706a41 · outbound

This paper cites Cosmology Intertwined: A Review of the Particle Physics, Astrophysics, and Cosmology Associated with the Cosmological Tensions and Anomalies.

Void spin distribution as a powerful probe of $\sigma_{8}$ Cosmology Intertwined: A Review of the Particle Physics, Astrophysics, and Cosmology Associated with the Cosmological Tensions and Anomalies

Reference 14

Resolution: unresolved; no resolver link, observed 2026-08-10T20:04:03.437744Z

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Observation 3a78d08a-67f3-4385-a91c-768ea3786ecd · outbound

This paper cites Planck 2018 results. VI. Cosmological parameters.

Void spin distribution as a powerful probe of $\sigma_{8}$ Planck 2018 results. VI. Cosmological parameters

Reference 15

Resolution: unresolved; no resolver link, observed 2026-08-10T20:04:03.441449Z

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Observation df526bbf-52e3-437d-bf6f-67078f276d05 · outbound

This paper cites A Comprehensive Measurement of the Local Value of the Hubble Constant with 1 km/s/Mpc Uncertainty from the Hubble Space Telescope and the SH0ES Team.

Void spin distribution as a powerful probe of $\sigma_{8}$ A Comprehensive Measurement of the Local Value of the Hubble Constant with 1 km/s/Mpc Uncertainty from the Hubble Space Telescope and the SH0ES Team

Reference 16

Resolution: unresolved; no resolver link, observed 2026-08-10T20:04:03.444155Z

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Observation 8f6f8887-f15c-4627-8d97-e0004c823933 · outbound

This paper cites KiDS-1000 Cosmology: Cosmic shear constraints and comparison between two point statistics.

Void spin distribution as a powerful probe of $\sigma_{8}$ KiDS-1000 Cosmology: Cosmic shear constraints and comparison between two point statistics

Reference 17

Resolution: unresolved; no resolver link, observed 2026-08-10T20:04:03.447627Z

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Observation a1cc4e7a-a87e-447b-aae9-8e6d2c082362 · outbound

This paper cites GAIA Cepheid parallaxes and 'Local Hole' relieve $H_0$ tension.

Void spin distribution as a powerful probe of $\sigma_{8}$ GAIA Cepheid parallaxes and 'Local Hole' relieve $H_0$ tension

Reference 18

Resolution: unresolved; no resolver link, observed 2026-08-10T20:04:03.450234Z

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Observation 2ce0d11c-e9b1-4cdf-a8eb-f76dc432bae0 · outbound

This paper cites How does an incomplete sky coverage affect the Hubble Constant variance?.

Void spin distribution as a powerful probe of $\sigma_{8}$ How does an incomplete sky coverage affect the Hubble Constant variance?

Reference 19

Resolution: verified exact; local_arxiv, observed 2026-08-10T20:04:04.521779Z

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No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

Observation 36beef6c-8db6-4083-be68-7e0258f1c865 · outbound

This paper cites Sensitivity of the Hubble Constant Determination to Cepheid Calibration.

Void spin distribution as a powerful probe of $\sigma_{8}$ Sensitivity of the Hubble Constant Determination to Cepheid Calibration

Reference 20

Resolution: unresolved; no resolver link, observed 2026-08-10T20:04:03.454725Z

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Observation c91e996a-dd6f-426f-9895-10dbb508fc4c · outbound

This paper cites $\Lambda$CDM is alive and well.

Void spin distribution as a powerful probe of $\sigma_{8}$ $\Lambda$CDM is alive and well

Reference 21

Resolution: unresolved; no resolver link, observed 2026-08-10T20:04:03.457104Z

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Observation bc4f5b35-a673-4f31-abfb-866eba0e7ba0 · outbound

This paper cites The axis of systematic bias in SN~Ia cosmology and implications for DESI 2024 results.

Void spin distribution as a powerful probe of $\sigma_{8}$ The axis of systematic bias in SN~Ia cosmology and implications for DESI 2024 results

Reference 22

Resolution: unresolved; no resolver link, observed 2026-08-10T20:04:03.459301Z

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Observation 2a257ed6-4204-476b-84f7-a0876c355b58 · outbound

This paper cites Evolving Dark Energy or Supernovae Systematics?.

Void spin distribution as a powerful probe of $\sigma_{8}$ Evolving Dark Energy or Supernovae Systematics?

Reference 23

Resolution: unresolved; no resolver link, observed 2026-08-10T20:04:03.462276Z

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Observation db2e7704-7976-4426-96a9-d6d6959b5409 · outbound

This paper cites The $H_0$ Olympics: A fair ranking of proposed models.

Void spin distribution as a powerful probe of $\sigma_{8}$ The $H_0$ Olympics: A fair ranking of proposed models

Reference 24

Resolution: unresolved; no resolver link, observed 2026-08-10T20:04:03.465141Z

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Observation ae5ef287-28f5-420b-a0a5-f3a3b0d694f8 · outbound

This paper cites Review of Hubble tension solutions with new SH0ES and SPT-3G data.

Void spin distribution as a powerful probe of $\sigma_{8}$ Review of Hubble tension solutions with new SH0ES and SPT-3G data

Reference 25

Resolution: unresolved; no resolver link, observed 2026-08-10T20:04:03.467918Z

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Observation 929fed9c-4465-4049-b4b8-ae7488e1ec12 · outbound

This paper cites DESI 2024 VI: Cosmological Constraints from the Measurements of Baryon Acoustic Oscillations.

Void spin distribution as a powerful probe of $\sigma_{8}$ DESI 2024 VI: Cosmological Constraints from the Measurements of Baryon Acoustic Oscillations

Reference 26

Resolution: unresolved; no resolver link, observed 2026-08-10T20:04:03.470392Z

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Observation ab52f646-da38-4f42-9819-9a7fc4e12274 · outbound

This paper cites Implications of a transition in the dark energy equation of state for the $H_0$ and $\sigma_8$ tensions.

Void spin distribution as a powerful probe of $\sigma_{8}$ Implications of a transition in the dark energy equation of state for the $H_0$ and $\sigma_8$ tensions

Reference 27

Resolution: unresolved; no resolver link, observed 2026-08-10T20:04:03.473063Z

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Observation edacb007-34eb-4246-a29b-4d0bbc6297e2 · outbound

This paper cites Why reducing the cosmic sound horizon alone can not fully resolve the Hubble tension.

Void spin distribution as a powerful probe of $\sigma_{8}$ Why reducing the cosmic sound horizon alone can not fully resolve the Hubble tension

Reference 28

Resolution: unresolved; no resolver link, observed 2026-08-10T20:04:03.475404Z

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Observation 4bf47154-87c8-487a-b4c8-d0cede31e662 · outbound

This paper cites Extensions to $\Lambda$CDM at Intermediate Redshifts to Solve the Tensions ?.

Void spin distribution as a powerful probe of $\sigma_{8}$ Extensions to $\Lambda$CDM at Intermediate Redshifts to Solve the Tensions ?

Reference 29

Resolution: verified exact; local_arxiv, observed 2026-08-10T20:04:04.460941Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

Observation e16a996a-daec-4687-9e56-e2ad5aaf9fd0 · outbound

This paper cites $\Lambda$CDM Tensions: Localising Missing Physics through Consistency Checks.

Void spin distribution as a powerful probe of $\sigma_{8}$ $\Lambda$CDM Tensions: Localising Missing Physics through Consistency Checks

Reference 30

Resolution: unresolved; no resolver link, observed 2026-08-10T20:04:03.480097Z

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Observation 4c054800-f764-4e48-bc61-6fbea28f99fb · outbound

This paper cites The $H_0$ and $S_8$ tensions necessitate early and late time changes to $\Lambda$CDM.

Void spin distribution as a powerful probe of $\sigma_{8}$ The $H_0$ and $S_8$ tensions necessitate early and late time changes to $\Lambda$CDM

Reference 31

Resolution: unresolved; no resolver link, observed 2026-08-10T20:04:03.482536Z

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Observation abecbf71-0082-4f98-8f79-1002363a3eaa · outbound

This paper cites Heisenberg, H.

Void spin distribution as a powerful probe of $\sigma_{8}$ Heisenberg, H

Reference 32

Resolution: unresolved; no resolver link, observed 2026-08-10T20:04:03.484852Z

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Observation 9c22f156-4134-4fb8-82cf-c9c6a30a1557 · outbound

This paper cites Seven hints that early-time new physics alone is not sufficient to solve the Hubble tension.

Void spin distribution as a powerful probe of $\sigma_{8}$ Seven hints that early-time new physics alone is not sufficient to solve the Hubble tension

Reference 33

Resolution: unresolved; no resolver link, observed 2026-08-10T20:04:03.487497Z

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Observation 72ed4681-c9b7-4cb3-ad1b-893384ae82aa · outbound

This paper cites Using the Evolution of Clusters to Constrain Omega.

Void spin distribution as a powerful probe of $\sigma_{8}$ Using the Evolution of Clusters to Constrain Omega

Reference 34

Resolution: unresolved; no resolver link, observed 2026-08-10T20:04:03.489751Z

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Observation d1050796-366b-4bbc-b232-95022fe5953a · outbound

This paper cites Cluster Abundance Constraints on Quintessence Models.

Void spin distribution as a powerful probe of $\sigma_{8}$ Cluster Abundance Constraints on Quintessence Models

Reference 35

Resolution: unresolved; no resolver link, observed 2026-08-10T20:04:03.491990Z

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Observation fff66a64-24ba-4ac9-a875-c14753eb6d8b · outbound

This paper cites Massive neutrinos and cosmology.

Void spin distribution as a powerful probe of $\sigma_{8}$ Massive neutrinos and cosmology

Reference 36

Resolution: unresolved; no resolver link, observed 2026-08-10T20:04:03.494217Z

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Observation 84c2c96c-3d04-4df7-baf3-00f76a6efdf7 · outbound

This paper cites The X-ray Cluster Normalization of the Matter Power Spectrum.

Void spin distribution as a powerful probe of $\sigma_{8}$ The X-ray Cluster Normalization of the Matter Power Spectrum

Reference 37

Resolution: unresolved; no resolver link, observed 2026-08-10T20:04:03.496811Z

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Observation 600d8cdf-9355-4df7-83a2-91ebc8223fc6 · outbound

This paper cites Unveiling the Universe with Emerging Cosmological Probes.

Void spin distribution as a powerful probe of $\sigma_{8}$ Unveiling the Universe with Emerging Cosmological Probes

Reference 38

Resolution: unresolved; no resolver link, observed 2026-08-10T20:04:03.498979Z

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Observation d06583fe-5a9a-4365-90de-5562736c977e · outbound

This paper cites A Parameter-Masked Mock Data Challenge for Beyond-Two-Point Galaxy Clustering Statistics.

Void spin distribution as a powerful probe of $\sigma_{8}$ A Parameter-Masked Mock Data Challenge for Beyond-Two-Point Galaxy Clustering Statistics

Reference 39

Resolution: unresolved; no resolver link, observed 2026-08-10T20:04:03.501421Z

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Observation 9f3ed765-2b14-44f8-bc0e-ff4f93d802ae · outbound

This paper cites Constraining the Dark Energy Equation of State with Cosmic Voids.

Void spin distribution as a powerful probe of $\sigma_{8}$ Constraining the Dark Energy Equation of State with Cosmic Voids

Reference 40

Resolution: verified exact; local_arxiv, observed 2026-08-10T20:04:04.335957Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

Observation 04d1d919-f550-4211-9802-263782d6f1b0 · outbound

This paper cites Voids as a Precision Probe of Dark Energy.

Void spin distribution as a powerful probe of $\sigma_{8}$ Voids as a Precision Probe of Dark Energy

Reference 41

Resolution: verified exact; local_arxiv, observed 2026-08-10T20:04:04.326036Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

Observation cde4db30-bff4-4592-887c-538d69532b0a · outbound

This paper cites an unresolved cited work.

Void spin distribution as a powerful probe of $\sigma_{8}$ Unresolved cited work

Reference 42

Resolution: unresolved; no resolver link, observed 2026-08-10T20:04:03.509346Z

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Observation 8015a823-bee2-43ef-83bf-205c3c838b39 · outbound

This paper cites Precision cosmography with stacked voids.

Void spin distribution as a powerful probe of $\sigma_{8}$ Precision cosmography with stacked voids

Reference 43

Resolution: unresolved; no resolver link, observed 2026-08-10T20:04:03.511608Z

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Observation ddee7319-f6eb-4a4f-ac40-9510377ced06 · outbound

This paper cites Voids in massive neutrino cosmologies.

Void spin distribution as a powerful probe of $\sigma_{8}$ Voids in massive neutrino cosmologies

Reference 44

Resolution: unresolved; no resolver link, observed 2026-08-10T20:04:03.514278Z

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Observation c26f0fd9-5266-4873-b261-7fcb10e50a3e · outbound

This paper cites Voids in the Cosmic Web as a probe of dark energy.

Void spin distribution as a powerful probe of $\sigma_{8}$ Voids in the Cosmic Web as a probe of dark energy

Reference 45

Resolution: verified exact; local_arxiv, observed 2026-08-10T20:04:04.238727Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

Observation b14e126d-941d-48cb-9187-2b0c4d1b1cf7 · outbound

This paper cites The Void Size Function in Dynamical Dark Energy Cosmologies.

Void spin distribution as a powerful probe of $\sigma_{8}$ The Void Size Function in Dynamical Dark Energy Cosmologies

Reference 46

Resolution: verified exact; local_arxiv, observed 2026-08-10T20:04:04.229623Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

Observation 01d65831-e097-434a-8a97-688a4df9761d · outbound

This paper cites Precision cosmology with voids in the final BOSS data.

Void spin distribution as a powerful probe of $\sigma_{8}$ Precision cosmology with voids in the final BOSS data

Reference 47

Resolution: unresolved; no resolver link, observed 2026-08-10T20:04:03.522037Z

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Observation 0e7d1fec-3be7-4a04-8190-8e159f1267b9 · outbound

This paper cites Rezaei,Dark Matter-Dark Energy Interaction and the Shape of Cosmic Voids, Astrophys.

Void spin distribution as a powerful probe of $\sigma_{8}$ Rezaei,Dark Matter-Dark Energy Interaction and the Shape of Cosmic Voids, Astrophys

Reference 48

Resolution: unresolved; no resolver link, observed 2026-08-10T20:04:03.524049Z

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Observation dd2ccf34-52cd-44e1-bf41-07c721d9a0d9 · outbound

This paper cites an unresolved cited work.

Void spin distribution as a powerful probe of $\sigma_{8}$ Unresolved cited work

Reference 49

Resolution: verified exact; raw_fallback, observed 2026-08-10T20:04:04.158369Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

Observation 7fd34d16-c628-4921-84b0-54ab8c9f16bc · outbound

This paper cites Euclid: Cosmological forecasts from the void size function.

Void spin distribution as a powerful probe of $\sigma_{8}$ Euclid: Cosmological forecasts from the void size function

Reference 50

Resolution: unresolved; no resolver link, observed 2026-08-10T20:04:03.528843Z

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Observation 2cd2d71b-0635-4566-bc39-8b86cd606741 · outbound

This paper cites DEMNUni: disentangling dark energy from massive neutrinos with the void size function.

Void spin distribution as a powerful probe of $\sigma_{8}$ DEMNUni: disentangling dark energy from massive neutrinos with the void size function

Reference 51

Resolution: unresolved; no resolver link, observed 2026-08-10T20:04:03.531713Z

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Observation b9dc5d2e-7ec6-4fda-97b8-c9d9ec814307 · outbound

This paper cites Ebrahimi,Phenomenological emergent dark energy versus theΛCDM: ellipticity of cosmic voids, Mon.

Void spin distribution as a powerful probe of $\sigma_{8}$ Ebrahimi,Phenomenological emergent dark energy versus theΛCDM: ellipticity of cosmic voids, Mon

Reference 52

Resolution: verified exact; doi, observed 2026-08-10T20:04:03.704234Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

Observation 63df568a-66f2-4f51-929f-6946325f010b · outbound

This paper cites Void Ellipticity Distribution as a Probe of Cosmology.

Void spin distribution as a powerful probe of $\sigma_{8}$ Void Ellipticity Distribution as a Probe of Cosmology

Reference 53

Resolution: verified exact; local_arxiv, observed 2026-08-10T20:04:04.090158Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

Observation ba8a17ba-f0b9-4215-b32b-0cc5651992ec · outbound

This paper cites Constraining cosmological parameters using void statistics from the SDSS survey.

Void spin distribution as a powerful probe of $\sigma_{8}$ Constraining cosmological parameters using void statistics from the SDSS survey

Reference 54

Resolution: unresolved; no resolver link, observed 2026-08-10T20:04:03.539920Z

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Observation 38cebf06-1c3e-4bf9-b527-52b8cbd96030 · outbound

This paper cites Rotation of Cosmic Voids and Void-Spin Statistics.

Void spin distribution as a powerful probe of $\sigma_{8}$ Rotation of Cosmic Voids and Void-Spin Statistics

Reference 55

Resolution: verified exact; local_arxiv, observed 2026-08-10T20:04:04.073467Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

Observation 64466a50-25bd-4457-b8ce-ed2c632a9740 · outbound

This paper cites The $\texttt{Abacus}$ Cosmological $N$-body Code.

Void spin distribution as a powerful probe of $\sigma_{8}$ The $\texttt{Abacus}$ Cosmological $N$-body Code

Reference 56

Resolution: unresolved; no resolver link, observed 2026-08-10T20:04:03.545423Z

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Observation f00bdefc-2846-477c-a709-bcf6039d23d7 · outbound

This paper cites an unresolved cited work.

Void spin distribution as a powerful probe of $\sigma_{8}$ Unresolved cited work

Reference 57

Resolution: unresolved; no resolver link, observed 2026-08-10T20:04:03.548009Z

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Observation ca8c28b0-b2ef-49e9-89ed-54e196223012 · outbound

This paper cites The Cosmic Linear Anisotropy Solving System (CLASS) I: Overview.

Void spin distribution as a powerful probe of $\sigma_{8}$ The Cosmic Linear Anisotropy Solving System (CLASS) I: Overview

Reference 58

Resolution: unresolved; no resolver link, observed 2026-08-10T20:04:03.550037Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 7ec78c0c-374b-44fd-94e7-ea93854944c2 · outbound

This paper cites Weak Deflection angle and Shadow by Tidal Charged Black Hole.

Void spin distribution as a powerful probe of $\sigma_{8}$ Weak Deflection angle and Shadow by Tidal Charged Black Hole

Reference 59

Resolution: verified exact; local_arxiv, observed 2026-08-10T20:04:04.057554Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

Observation 5ea9d500-cf21-42b0-9680-0b1cbcb33898 · outbound

This paper cites \textsc{CompaSO}: A new halo finder for competitive assignment to spherical overdensities.

Void spin distribution as a powerful probe of $\sigma_{8}$ \textsc{CompaSO}: A new halo finder for competitive assignment to spherical overdensities

Reference 60

Resolution: unresolved; no resolver link, observed 2026-08-10T20:04:03.554447Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 2361f225-b313-45ab-8f66-26eb9f083812 · outbound

This paper cites Algebraic Properties of Blackwell's Order and A Cardinal Measure of Informativeness.

Void spin distribution as a powerful probe of $\sigma_{8}$ Algebraic Properties of Blackwell's Order and A Cardinal Measure of Informativeness

Reference 61

Resolution: verified exact; local_arxiv, observed 2026-08-10T20:04:04.041960Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

Observation cea8a0ce-742e-467e-8f4d-1a2cc7a9d1b4 · outbound

This paper cites an unresolved cited work.

Void spin distribution as a powerful probe of $\sigma_{8}$ Unresolved cited work

Reference 62

Resolution: unresolved; no resolver link, observed 2026-08-10T20:04:03.559766Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 2de1ec84-799b-471f-939c-0fcee16b6178 · outbound

This paper cites Voids in the Large-Scale Structure.

Void spin distribution as a powerful probe of $\sigma_{8}$ Voids in the Large-Scale Structure

Reference 63

Resolution: verified exact; local_arxiv, observed 2026-08-10T20:04:04.032804Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

Observation d91fd116-2a66-4549-baac-d7e5ff7b6a5c · outbound

This paper cites Multivariate analysis of cosmic void characteristics.

Void spin distribution as a powerful probe of $\sigma_{8}$ Multivariate analysis of cosmic void characteristics

Reference 64

Resolution: verified exact; local_arxiv, observed 2026-08-10T20:04:04.023881Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

Observation 92703033-912d-4cb8-829a-efa3c1f0584e · outbound

This paper cites Euclid: Forecasts from redshift-space distortions and the Alcock-Paczynski test with cosmic voids.

Void spin distribution as a powerful probe of $\sigma_{8}$ Euclid: Forecasts from redshift-space distortions and the Alcock-Paczynski test with cosmic voids

Reference 65

Resolution: unresolved; no resolver link, observed 2026-08-10T20:04:03.567985Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 06c9d531-7b82-4126-a53f-fe5df5c964ba · outbound

This paper cites Verza, G.

Void spin distribution as a powerful probe of $\sigma_{8}$ Verza, G

Reference 66

Resolution: unresolved; no resolver link, observed 2026-08-10T20:04:03.570192Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a0504d10-0081-4a40-bb1f-3fcbb9cc0c30 · outbound

This paper cites Simulating nonlinear cosmological structure formation with massive neutrinos.

Void spin distribution as a powerful probe of $\sigma_{8}$ Simulating nonlinear cosmological structure formation with massive neutrinos

Reference 67

Resolution: unresolved; no resolver link, observed 2026-08-10T20:04:03.572703Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c351a574-701e-4eca-a9c8-209faea1d8f6 · outbound

This paper cites an unresolved cited work.

Void spin distribution as a powerful probe of $\sigma_{8}$ Unresolved cited work

Reference 68

Resolution: unresolved; no resolver link, observed 2026-08-10T20:04:03.574981Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation b26d3d60-940b-4b54-8a7b-410c45208c1c · outbound

This paper cites Clues on void evolution III: Structure and dynamics in void shells.

Void spin distribution as a powerful probe of $\sigma_{8}$ Clues on void evolution III: Structure and dynamics in void shells

Reference 69

Resolution: unresolved; no resolver link, observed 2026-08-10T20:04:03.577747Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 83808ac4-7ec9-45b6-a0ef-93da30bcc628 · outbound

This paper cites Guess the cheese flavour by the size of its holes: A cosmological test using the abundance of Popcorn voids.

Void spin distribution as a powerful probe of $\sigma_{8}$ Guess the cheese flavour by the size of its holes: A cosmological test using the abundance of Popcorn voids

Reference 70

Resolution: verified exact; local_arxiv, observed 2026-08-10T20:04:03.945756Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

Observation 272a9c25-4fbe-4e46-a5ef-e9d2e6624cab · outbound

This paper cites an unresolved cited work.

Void spin distribution as a powerful probe of $\sigma_{8}$ Unresolved cited work

Reference 71

Resolution: unresolved; no resolver link, observed 2026-08-10T20:04:03.582990Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 5f0425d4-2be7-4556-a8f2-423409fd1e9f · outbound

This paper cites VIDE: The Void IDentification and Examination toolkit.

Void spin distribution as a powerful probe of $\sigma_{8}$ VIDE: The Void IDentification and Examination toolkit

Reference 72

Resolution: unresolved; no resolver link, observed 2026-08-10T20:04:03.585578Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 9ab90bf5-a193-4799-acad-187e4175ed8e · outbound

This paper cites Nadathur, P.

Void spin distribution as a powerful probe of $\sigma_{8}$ Nadathur, P

Reference 73

Resolution: verified fuzzy; raw_fallback, observed 2026-08-10T20:04:04.689751Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

Observation 13735c6b-9de0-4ea1-8034-a9ea4eb0cdfa · outbound

This paper cites An Observed Transition of Galaxy Spins on the Void Surfaces.

Void spin distribution as a powerful probe of $\sigma_{8}$ An Observed Transition of Galaxy Spins on the Void Surfaces

Reference 74

Resolution: unresolved; no resolver link, observed 2026-08-10T20:04:03.589815Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 6803a9cd-ef80-4451-8f18-78e431adb650 · outbound

This paper cites A universal angular momentum profile for galactic halos.

Void spin distribution as a powerful probe of $\sigma_{8}$ A universal angular momentum profile for galactic halos

Reference 75

Resolution: unresolved; no resolver link, observed 2026-08-10T20:04:03.592393Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 5c74fc5f-f299-4539-ac39-92b4f6a9dce9 · outbound

This paper cites Mutual information between galaxy properties and the initial predisposition.

Void spin distribution as a powerful probe of $\sigma_{8}$ Mutual information between galaxy properties and the initial predisposition

Reference 76

Resolution: verified exact; local_arxiv, observed 2026-08-10T20:04:03.857033Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

Observation 2ede085f-b5ad-4e6a-87f0-885c3842e2e8 · outbound

This paper cites Disentangling Modified Gravity and Massive Neutrinos with Intrinsic Shape Alignments of Massive Halos.

Void spin distribution as a powerful probe of $\sigma_{8}$ Disentangling Modified Gravity and Massive Neutrinos with Intrinsic Shape Alignments of Massive Halos

Reference 77

Resolution: verified exact; local_arxiv, observed 2026-08-10T20:04:03.848074Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

Observation fd429b91-5029-4615-bed2-97f56c55ea41 · outbound

This paper cites Possible observational evidence that cosmic filaments spin.

Void spin distribution as a powerful probe of $\sigma_{8}$ Possible observational evidence that cosmic filaments spin

Reference 78

Resolution: verified exact; local_arxiv, observed 2026-08-10T20:04:03.837786Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

Observation 7413e7c9-bf90-4537-8c82-891c30b652a5 · outbound

This paper cites Shandarin, H.

Void spin distribution as a powerful probe of $\sigma_{8}$ Shandarin, H

Reference 79

Resolution: unresolved; no resolver link, observed 2026-08-10T20:04:03.601786Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f480ec92-52e5-493b-92bd-29c74122d4f8 · outbound

This paper cites How Filaments are Woven into the Cosmic Web.

Void spin distribution as a powerful probe of $\sigma_{8}$ How Filaments are Woven into the Cosmic Web

Reference 80

Resolution: unresolved; no resolver link, observed 2026-08-10T20:04:03.603874Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 460d674e-8154-47c3-a677-8e24bd7cd146 · outbound

This paper cites Shannon,A Mathematical Theory of Communication, The Bell Sys.

Void spin distribution as a powerful probe of $\sigma_{8}$ Shannon,A Mathematical Theory of Communication, The Bell Sys

Reference 81

Resolution: unresolved; no resolver link, observed 2026-08-10T20:04:03.606243Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Outbound references

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