Paper Citation Record · LEDGER

Halo Models of Large Scale Structure

As of 17 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 33 inbound Pith citation observations for arXiv:astro-ph/0206508.

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

pith.paper-citation-record.v1
astro-ph/0206508 v1

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measured 0 of 0 reference resolution

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measured 33 of 33 standing notices

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Source: scholarly_work_events, retraction_status_cache, observed 2026-08-17T06:30:58.91139+00:00

measured 33 of 33 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-15T22:13:49.578529Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-01T04:05:20.597611Z

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Outbound references

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Pith citing papers

Observation 6c5af142-048c-4ea5-ad20-1e0bce7db6d2 · inbound

Parametrizations for tests of gravity cites this paper.

Parametrizations for tests of gravity Halo Models of Large Scale Structure

Reference 156

Resolution: unresolved; no resolver link, observed 2026-08-14T11:57:58.865353Z

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Unavailable: canonical work link unavailable.

Observation d77b6e4a-5df8-49cc-b138-e6a696defb9f · inbound

Modelling the matter bispectrum at small scales in modified gravity cites this paper.

Modelling the matter bispectrum at small scales in modified gravity Halo Models of Large Scale Structure

Reference 80

Resolution: unresolved; no resolver link, observed 2026-08-14T04:55:19.477383Z

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Unavailable: canonical work link unavailable.

Observation 71706d7b-e0b9-4611-8369-fabcae646c1f · inbound

Cosmology with HI cites this paper.

Cosmology with HI Halo Models of Large Scale Structure

Reference 21

Resolution: unresolved; no resolver link, observed 2026-08-12T22:02:03.934758Z

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Unavailable: canonical work link unavailable.

Observation 1c83408e-bcee-4cff-9c90-0cc14abf387d · inbound

Analytical modeling of the one-dimensional power spectrum of 21-cm forest based on a halo model method cites this paper.

Analytical modeling of the one-dimensional power spectrum of 21-cm forest based on a halo model method Halo Models of Large Scale Structure

Reference 43

Resolution: unresolved; no resolver link, observed 2026-08-12T12:42:56.859387Z

Source-reported events for the cited work

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Observation 8f5f6c83-4246-4920-a345-53ca2b7a3e43 · inbound

Cosmology with Galaxy Clusters cites this paper.

Cosmology with Galaxy Clusters Halo Models of Large Scale Structure

Reference 28

Resolution: unresolved; no resolver link, observed 2026-08-15T22:13:49.578529Z

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Observation 331abfa0-de3d-4fd7-9314-663c2f6cff52 · inbound

Perturbative Likelihoods for Large-Scale Structure of the Universe cites this paper.

Perturbative Likelihoods for Large-Scale Structure of the Universe Halo Models of Large Scale Structure

Reference 12

Resolution: unresolved; no resolver link, observed 2026-08-07T12:48:14.725094Z

Source-reported events for the cited work

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Observation f7c62442-bc3e-454b-b45f-caa4e5c87ff6 · inbound

Gravitational redshift from large-scale structure: nonlinearities, antisymmetries, and the dipole cites this paper.

Gravitational redshift from large-scale structure: nonlinearities, antisymmetries, and the dipole Halo Models of Large Scale Structure

Reference 82

Resolution: unresolved; no resolver link, observed 2026-08-06T22:10:41.706285Z

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Unavailable: canonical work link unavailable.

Observation 5888e94a-d54b-4cd7-8222-304a42dcad73 · inbound

Baryonification II: Constraining feedback with X-ray and kinematic Sunyaev-Zel'dovich observations cites this paper.

Baryonification II: Constraining feedback with X-ray and kinematic Sunyaev-Zel'dovich observations Halo Models of Large Scale Structure

Reference 90

Resolution: unresolved; no resolver link, observed 2026-08-06T18:36:06.329693Z

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Unavailable: canonical work link unavailable.

Observation 7211a8e0-5fb6-4e5a-b430-8c3793a4968a · inbound

Risk-based framework to determine climate-informed design storms for road drainage infrastructure cites this paper.

Risk-based framework to determine climate-informed design storms for road drainage infrastructure Halo Models of Large Scale Structure

Reference 51

Resolution: unresolved; no resolver link, observed 2026-08-05T20:39:32.831733Z

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Observation 66615914-876e-4a02-89af-5bd666460336 · inbound

Where does non-Universality in Assembly Bias come from? cites this paper.

Where does non-Universality in Assembly Bias come from? Halo Models of Large Scale Structure

Reference 50

Resolution: unresolved; no resolver link, observed 2026-08-15T17:30:09.624844Z

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Unavailable: canonical work link unavailable.

Observation c372fbc3-803d-4d0b-becc-2230cc630e85 · inbound

Periodic orbits and their gravitational waves in EMRIs: supermassive black hole affected by galactic dark matter halos cites this paper.

Periodic orbits and their gravitational waves in EMRIs: supermassive black hole affected by galactic dark matter halos Halo Models of Large Scale Structure

Reference 11

Resolution: unresolved; no resolver link, observed 2026-08-15T15:48:18.762044Z

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Observation ad929c06-2c80-4ebf-9590-a64440bf73ea · inbound

Statistics Meet Systematics: Resolution of the Massive Early JWST Galaxy Tension cites this paper.

Statistics Meet Systematics: Resolution of the Massive Early JWST Galaxy Tension Halo Models of Large Scale Structure

Reference 29

Resolution: verified exact; local_arxiv, observed 2026-05-17T21:45:18.334915Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

Observation 10ac55fa-9bc7-4618-b4a0-8b355b2f6f6e · inbound

An essential building block for cosmological zoom-in perturbation theory cites this paper.

An essential building block for cosmological zoom-in perturbation theory Halo Models of Large Scale Structure

Reference 22

Resolution: verified exact; local_arxiv, observed 2026-05-16T10:50:51.595069Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

Observation de5fefbe-b248-4b0b-820c-d0debfc70b01 · inbound

Seeing Wiggles without Seeing Wiggles: BAO Recovery in 21 cm Intensity Mapping with Deep Learning cites this paper.

Seeing Wiggles without Seeing Wiggles: BAO Recovery in 21 cm Intensity Mapping with Deep Learning Halo Models of Large Scale Structure

Reference 38

Resolution: unresolved; no resolver link, observed 2026-08-03T05:10:22.674524Z

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Observation f0d39d7f-d2e6-40f6-9d0d-ab36508e0e3d · inbound

A unified harmonic framework for dark siren cosmology cites this paper.

A unified harmonic framework for dark siren cosmology Halo Models of Large Scale Structure

Reference 51

Resolution: verified exact; local_arxiv, observed 2026-05-15T11:30:31.017116Z

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No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

Observation 05ee9e65-c910-4886-ada6-66599c3def68 · inbound

An Improved Fit for Linear Halo Bias at High Redshift cites this paper.

An Improved Fit for Linear Halo Bias at High Redshift Halo Models of Large Scale Structure

Reference 3

Resolution: verified exact; arxiv_id, observed 2026-05-10T12:00:21.838938Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

Observation 11e8efa3-96d9-4ac4-9114-0f4b5c6b03c7 · inbound

Anisotropy of Cosmic Background Photons from Annihilating/Decaying Dark Matter cites this paper.

Anisotropy of Cosmic Background Photons from Annihilating/Decaying Dark Matter Halo Models of Large Scale Structure

Reference 50

Resolution: verified exact; arxiv_id, observed 2026-05-11T15:56:11.280532Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

Observation 4f16b0e6-5c3d-4910-a219-e5e66aa820c6 · inbound

New constraints on primordial non-Gaussianity from large-scale cross-correlations of CMB lensing and the cosmic infrared background cites this paper.

New constraints on primordial non-Gaussianity from large-scale cross-correlations of CMB lensing and the cosmic infrared background Halo Models of Large Scale Structure

Reference 66

Resolution: verified exact; arxiv_id, observed 2026-05-12T08:51:25.069981Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

Observation a3eecee6-09ad-4b91-8e13-887fb6d3e310 · inbound

Gravitational wave emission from nonspherical collapse in an early matter-dominated era using N-body simulations cites this paper.

Gravitational wave emission from nonspherical collapse in an early matter-dominated era using N-body simulations Halo Models of Large Scale Structure

Reference 6

Resolution: verified exact; arxiv_id, observed 2026-05-11T17:21:07.201750Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

Observation e27aa086-e562-45f7-989c-503bf2d4552d · inbound

UNIONS-3500 Weak Lensing: III. 2D Cosmological Constraints in Configuration Space cites this paper.

UNIONS-3500 Weak Lensing: III. 2D Cosmological Constraints in Configuration Space Halo Models of Large Scale Structure

Reference 67

Resolution: verified exact; local_arxiv, observed 2026-05-14T18:19:22.079956Z

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No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

Observation 563acadf-9edb-44b6-9e51-d597a0fc1107 · inbound

Accretion Effects on Primordial Black Hole Reheating Constraints cites this paper.

Accretion Effects on Primordial Black Hole Reheating Constraints Halo Models of Large Scale Structure

Reference 42

Resolution: verified exact; local_arxiv, observed 2026-05-20T17:08:41.852262Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

Observation a96de297-64a2-44ab-b5de-fc5e8fe5135c · inbound

A Designer's Guide to Lunar Far-Side Interferometer Array: Power Spectrum Measurement and Cosmological Constraints from the Dark Ages cites this paper.

A Designer's Guide to Lunar Far-Side Interferometer Array: Power Spectrum Measurement and Cosmological Constraints from the Dark Ages Halo Models of Large Scale Structure

Reference 41

Resolution: verified exact; local_arxiv, observed 2026-06-29T06:23:09.275205Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

Observation c92389ec-87c5-4d38-92c7-ad2a167a65d2 · inbound

A Unified Halo Mass Function Across Dark Matter Models from High-Resolution Multi-Scale Simulations cites this paper.

A Unified Halo Mass Function Across Dark Matter Models from High-Resolution Multi-Scale Simulations Halo Models of Large Scale Structure

Reference 53

Resolution: verified exact; local_arxiv, observed 2026-06-27T09:40:47.975457Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

Observation b0018bc5-3bd9-42d1-9d7c-c03cca18d0f1 · inbound

Tracing Large-scale Structure with the MeerKLASS On-the-Fly Survey: Angular Clustering of Radio Sources at 816 MHz cites this paper.

Tracing Large-scale Structure with the MeerKLASS On-the-Fly Survey: Angular Clustering of Radio Sources at 816 MHz Halo Models of Large Scale Structure

Reference 1

Resolution: verified exact; local_arxiv, observed 2026-06-26T10:09:17.888162Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

Observation 5d1a1c8b-352b-42b4-bfc5-04e6aa01f418 · inbound

Revisiting the 'Lensing is Low' Problem with UNIONS cites this paper.

Revisiting the 'Lensing is Low' Problem with UNIONS Halo Models of Large Scale Structure

Reference 28

Resolution: verified exact; local_arxiv, observed 2026-06-26T07:19:07.244518Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

Observation c204f390-8bbd-4f9e-9883-7d0307aa0434 · inbound

Using SKAO to Understand the Clustering of Gravitational Wave Sources cites this paper.

Using SKAO to Understand the Clustering of Gravitational Wave Sources Halo Models of Large Scale Structure

Reference 132

Resolution: verified exact; local_arxiv, observed 2026-06-25T23:08:41.073997Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

Observation 93f08225-f2ee-4fa5-8136-e862dfb66dfa · inbound

Large-scale structures of the Universe: physics, phenomenology, statistics cites this paper.

Large-scale structures of the Universe: physics, phenomenology, statistics Halo Models of Large Scale Structure

Reference 57

Resolution: metadata mismatch; local_arxiv, observed 2026-06-29T03:13:04.008653Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

Observation 13ff647b-241f-4623-b035-ec89adfaab08 · inbound

COSMOS-Web: does halo mass alone shape the clustering of star-forming and quiescent galaxies? cites this paper.

COSMOS-Web: does halo mass alone shape the clustering of star-forming and quiescent galaxies? Halo Models of Large Scale Structure

Reference 33

Resolution: verified exact; local_arxiv, observed 2026-07-01T04:05:20.598766Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

Observation a93e7202-accc-4b61-aa63-97b660d2b49f · inbound

Decaying Dark Matter Halo Abundance from a Revised Spherical Collapse Model cites this paper.

Decaying Dark Matter Halo Abundance from a Revised Spherical Collapse Model Halo Models of Large Scale Structure

Reference 70

Resolution: unresolved; no resolver link, observed 2026-08-01T13:07:52.282091Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 85586321-684e-4415-9401-d1569dbd5802 · inbound

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 Halo Models of Large Scale Structure

Reference 14

Resolution: unresolved; no resolver link, observed 2026-08-01T07:53:19.986383Z

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Unavailable: canonical work link unavailable.

Observation 2ddcc08d-c82d-48e5-8892-daa686f825fd · inbound

Interpreting the stacked kinetic SZ effect I: velocity reconstruction and non-linear velocity effects cites this paper.

Interpreting the stacked kinetic SZ effect I: velocity reconstruction and non-linear velocity effects Halo Models of Large Scale Structure

Reference 100

Resolution: unresolved; no resolver link, observed 2026-07-31T23:49:26.021303Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e2502fa8-9823-466b-862b-24af4917ee1d · inbound

Primordial Physics in the Nonlinear Universe: Revealing the oscillating halo bias from cosmological collider models cites this paper.

Primordial Physics in the Nonlinear Universe: Revealing the oscillating halo bias from cosmological collider models Halo Models of Large Scale Structure

Reference 188

Resolution: unresolved; no resolver link, observed 2026-07-31T05:29:30.281546Z

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Unavailable: canonical work link unavailable.

Observation e560b16b-a7c3-4ac8-8a1c-950628b55c73 · inbound

GGI Lectures on Large-Scale Structure Perturbation Theory (Effective Field Theory) cites this paper.

GGI Lectures on Large-Scale Structure Perturbation Theory (Effective Field Theory) Halo Models of Large Scale Structure

Reference 55

Resolution: unresolved; no resolver link, observed 2026-07-31T11:32:39.389414Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.