Paper Citation Record · LEDGER

How Filaments are Woven into the Cosmic Web

As of 12 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 42 inbound Pith citation observations for arXiv:astro-ph/9512141.

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pith.paper-citation-record.v1
astro-ph/9512141 v1

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measured 42 of 42 inbound itemization

Pith citing papers itemized under the disclosed page cap.

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Outbound references

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Pith citing papers

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Galaxy and halo angular clustering in LCDM and Modified Gravity cosmologies cites this paper.

Galaxy and halo angular clustering in LCDM and Modified Gravity cosmologies How Filaments are Woven into the Cosmic Web

Reference 6

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Tracing cosmic gas in filaments and halos: Low-redshift insights from the kinematic Sunyaev-Zel'dovich effect cites this paper.

Tracing cosmic gas in filaments and halos: Low-redshift insights from the kinematic Sunyaev-Zel'dovich effect How Filaments are Woven into the Cosmic Web

Reference 33

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Void spin distribution as a powerful probe of $\sigma_{8}$ cites this paper.

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

Reference 80

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Observation a9063798-177b-4ab6-9668-8c91c1d2b55a · inbound

Cosmic filaments confirm unexplained CMB temperature decrements in two independent redshift ranges cites this paper.

Cosmic filaments confirm unexplained CMB temperature decrements in two independent redshift ranges How Filaments are Woven into the Cosmic Web

Reference 3

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Disentangling the growth rate of perturbations from the HI bias using only clustering data from galaxy surveys cites this paper.

Disentangling the growth rate of perturbations from the HI bias using only clustering data from galaxy surveys How Filaments are Woven into the Cosmic Web

Reference 2

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Observation 6619f740-8ec7-420f-ac9b-de222ae30252 · inbound

Artifacts in Halo Shapes: Imprints of the Initial Condition cites this paper.

Artifacts in Halo Shapes: Imprints of the Initial Condition How Filaments are Woven into the Cosmic Web

Reference 3

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Observation b8aed006-f8c2-4e02-a491-da3cf970dfe9 · inbound

The impact of cosmic filaments on the abundance of satellite galaxies cites this paper.

The impact of cosmic filaments on the abundance of satellite galaxies How Filaments are Woven into the Cosmic Web

Reference 4

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Observation 6b74c44c-67ba-4d10-9e06-f8e0f888f8a2 · inbound

Weak-Lensing Analysis of the Galaxy Cluster Abell 85: Constraints on the Merger Scenarios of Its Southern Subcluster cites this paper.

Weak-Lensing Analysis of the Galaxy Cluster Abell 85: Constraints on the Merger Scenarios of Its Southern Subcluster How Filaments are Woven into the Cosmic Web

Reference 13

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Counting voids and filaments: Betti Curves as a Powerful Probe for Cosmology cites this paper.

Counting voids and filaments: Betti Curves as a Powerful Probe for Cosmology How Filaments are Woven into the Cosmic Web

Reference 11

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Observation a784600a-d6cf-40ae-af75-ea0e69127803 · inbound

Galaxy evolution in the cosmic web: the relative impact of nodes and filaments in the EAGLE simulation cites this paper.

Galaxy evolution in the cosmic web: the relative impact of nodes and filaments in the EAGLE simulation How Filaments are Woven into the Cosmic Web

Reference 6

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Observation f7cccf8f-d7b8-4ceb-8040-48382e563cd7 · inbound

Universal Dark-matter Density Profiles of Cosmic Filaments cites this paper.

Universal Dark-matter Density Profiles of Cosmic Filaments How Filaments are Woven into the Cosmic Web

Reference 3

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Weak-lensing Analysis of Intracluster Filaments in Abell 2744: Matched-filter Scans and Stepwise 2D Tracing cites this paper.

Weak-lensing Analysis of Intracluster Filaments in Abell 2744: Matched-filter Scans and Stepwise 2D Tracing How Filaments are Woven into the Cosmic Web

Reference 11

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Galaxy Populations in the IllustrisTNG Caustic Skeleton cites this paper.

Galaxy Populations in the IllustrisTNG Caustic Skeleton How Filaments are Woven into the Cosmic Web

Reference 27

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Caught in the Cosmic Web: Environmental Impacts on the Halo Substructure Boosts to Dark Matter Annihilation Signals cites this paper.

Caught in the Cosmic Web: Environmental Impacts on the Halo Substructure Boosts to Dark Matter Annihilation Signals How Filaments are Woven into the Cosmic Web

Reference 21

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Observation 95f15341-096a-405e-8ef4-79d7aefd21e7 · inbound

Non-Equilibrium Ionisation in Photoionised Haloes: Implications for Shock Stability and Absorption-Line Signatures cites this paper.

Non-Equilibrium Ionisation in Photoionised Haloes: Implications for Shock Stability and Absorption-Line Signatures How Filaments are Woven into the Cosmic Web

Reference 186

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Observation a122510c-a636-41bc-bbbf-949fedb25767 · inbound

Baryons in the Darkest Sites of the Universe cites this paper.

Baryons in the Darkest Sites of the Universe How Filaments are Woven into the Cosmic Web

Reference 8

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A statistical look on kinematic planes of satellite galaxies II: The physics behind their early formation in TNG50 MW/M31-like galaxies cites this paper.

A statistical look on kinematic planes of satellite galaxies II: The physics behind their early formation in TNG50 MW/M31-like galaxies How Filaments are Woven into the Cosmic Web

Reference 105

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TopoFisher: Learning Topological Summary Statistics by Maximizing Fisher Information cites this paper.

TopoFisher: Learning Topological Summary Statistics by Maximizing Fisher Information How Filaments are Woven into the Cosmic Web

Reference 49

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Information Content of the Cosmic Web cites this paper.

Information Content of the Cosmic Web How Filaments are Woven into the Cosmic Web

Reference 1

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Information Content of the Cosmic Web cites this paper.

Information Content of the Cosmic Web How Filaments are Woven into the Cosmic Web

Reference 1

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Observation e2cfa05e-e9f3-4ee4-b34d-6f03f85e2635 · inbound

Cosmic web stripping and starvation of low-mass filament galaxies in TNG50 cites this paper.

Cosmic web stripping and starvation of low-mass filament galaxies in TNG50 How Filaments are Woven into the Cosmic Web

Reference 129

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Observation ca54cdde-4f69-477a-b988-88627a49fce0 · inbound

Cosmography of the Sloan Basin of Attraction and Neighborhood cites this paper.

Cosmography of the Sloan Basin of Attraction and Neighborhood How Filaments are Woven into the Cosmic Web

Reference 4

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A series of unfortunate events: CHIME/FRB misclassification of a Galactic pulsar as a periodic fast radio burst cites this paper.

A series of unfortunate events: CHIME/FRB misclassification of a Galactic pulsar as a periodic fast radio burst How Filaments are Woven into the Cosmic Web

Reference 167

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The X-ray-to-UV relation does not evolve in homogeneous quasar samples cites this paper.

The X-ray-to-UV relation does not evolve in homogeneous quasar samples How Filaments are Woven into the Cosmic Web

Reference 237

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A local Universe catalogue of structures and voids dynamically identified using Cosmic-Flows4++ZOA peculiar velocities cites this paper.

A local Universe catalogue of structures and voids dynamically identified using Cosmic-Flows4++ZOA peculiar velocities How Filaments are Woven into the Cosmic Web

Reference 191

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Chemical hints of Population III stars from silicon abundances in massive galaxies cites this paper.

Chemical hints of Population III stars from silicon abundances in massive galaxies How Filaments are Woven into the Cosmic Web

Reference 22

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The impact of evolving cosmic filaments on mass and spin evolution of dark matter halos cites this paper.

The impact of evolving cosmic filaments on mass and spin evolution of dark matter halos How Filaments are Woven into the Cosmic Web

Reference 6

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Analytical and fitting formulae for solutions to Lyman-alpha radiative transfer equations: the effects of geometry, recoil, and velocity gradients cites this paper.

Analytical and fitting formulae for solutions to Lyman-alpha radiative transfer equations: the effects of geometry, recoil, and velocity gradients How Filaments are Woven into the Cosmic Web

Reference 9

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ScaleAware-JEPA: Latent Representation for Discovery in Multiscale Physical Fields cites this paper.

ScaleAware-JEPA: Latent Representation for Discovery in Multiscale Physical Fields How Filaments are Woven into the Cosmic Web

Reference 35

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Observation f91edfae-8887-4618-b0a7-5ba22dbd1ad8 · inbound

Cosmology with Intensity Mapping via Statistics Beyond the Power Spectrum in the SKAO Era cites this paper.

Cosmology with Intensity Mapping via Statistics Beyond the Power Spectrum in the SKAO Era How Filaments are Woven into the Cosmic Web

Reference 242

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Observation a99aa84f-58c3-4640-932c-833da40b05b4 · inbound

Cosmology with Multi-Wavelength Line Intensity Mapping Synergies in the SKAO Era cites this paper.

Cosmology with Multi-Wavelength Line Intensity Mapping Synergies in the SKAO Era How Filaments are Woven into the Cosmic Web

Reference 238

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The Large-Scale Structure of the Universe through the SKA lenses cites this paper.

The Large-Scale Structure of the Universe through the SKA lenses How Filaments are Woven into the Cosmic Web

Reference 79

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Hot or Cold? Radial Redistribution of Stars in FIRE Simulations of Milky Way-Mass Galaxies and the Asymmetry of Inward versus Outward Migrators cites this paper.

Hot or Cold? Radial Redistribution of Stars in FIRE Simulations of Milky Way-Mass Galaxies and the Asymmetry of Inward versus Outward Migrators How Filaments are Woven into the Cosmic Web

Reference 138

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Disentangling modified gravity and galaxy bias with field-level inference cites this paper.

Disentangling modified gravity and galaxy bias with field-level inference How Filaments are Woven into the Cosmic Web

Reference 20

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Quantifying Environmental Effects on Galaxy Properties using Non-spherical Voids Identified from SDSS DR7 cites this paper.

Quantifying Environmental Effects on Galaxy Properties using Non-spherical Voids Identified from SDSS DR7 How Filaments are Woven into the Cosmic Web

Reference 5

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Observation 8e5f8a98-ef04-4b57-b41b-d1f2605fe7e4 · inbound

Mass--size evolution and the emerging passive--density relation revealed by JWST/NIRCam in the Spiderweb protocluster cites this paper.

Mass--size evolution and the emerging passive--density relation revealed by JWST/NIRCam in the Spiderweb protocluster How Filaments are Woven into the Cosmic Web

Reference 189

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Web-Halo Model Peak-Background Split (WHM-PBS): halo bias as a distribution, not a number cites this paper.

Web-Halo Model Peak-Background Split (WHM-PBS): halo bias as a distribution, not a number How Filaments are Woven into the Cosmic Web

Reference 20

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Weighted Webs: Morphology-Informed Marked Fields cites this paper.

Weighted Webs: Morphology-Informed Marked Fields How Filaments are Woven into the Cosmic Web

Reference 3

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Tracing the Cosmic web across Cosmic time through SKA observations of radio galaxies cites this paper.

Tracing the Cosmic web across Cosmic time through SKA observations of radio galaxies How Filaments are Woven into the Cosmic Web

Reference 42

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A study of the large-scale formation in the environment of A3266: Infalling groups, filaments, and a premerger cold front cites this paper.

A study of the large-scale formation in the environment of A3266: Infalling groups, filaments, and a premerger cold front How Filaments are Woven into the Cosmic Web

Reference 31

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Cosmic Velocity Flows: from Theory to Observations cites this paper.

Cosmic Velocity Flows: from Theory to Observations How Filaments are Woven into the Cosmic Web

Reference 93

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Observation 0863c26c-b025-44c4-a5e6-372a1f2f91c9 · inbound

Multi-tracer mass bias in matched cosmic voids from SDSS DR7 and the ELUCID constrained simulation cites this paper.

Multi-tracer mass bias in matched cosmic voids from SDSS DR7 and the ELUCID constrained simulation How Filaments are Woven into the Cosmic Web

Reference 13

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