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Large scale bias and the peak background split

As of 19 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 41 inbound Pith citation observations for arXiv:astro-ph/9901122.

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astro-ph/9901122 v2

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Pith citing papers itemized under the disclosed page cap.

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Source: pith, observed 2026-07-04T14:19:54.142489Z

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Pith citing papers

Observation 713ce630-9af0-45ba-9c18-96e9b64db706 · inbound

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

Modelling the matter bispectrum at small scales in modified gravity Large scale bias and the peak background split

Reference 94

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Observation 38b682b9-c79c-44e3-a5d6-94b4e13db8c8 · inbound

The Gravitational Wave Bias Parameter from Angular Power Spectra: Bridging Between Galaxies and Binary Black Holes cites this paper.

The Gravitational Wave Bias Parameter from Angular Power Spectra: Bridging Between Galaxies and Binary Black Holes Large scale bias and the peak background split

Reference 57

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Observation b6124c52-4385-40d9-982a-9841b4da903a · inbound

Cosmic Structure Formation in the Non-linear Regime: Beyond Gaussian Statistics and Standard Cosmologies cites this paper.

Cosmic Structure Formation in the Non-linear Regime: Beyond Gaussian Statistics and Standard Cosmologies Large scale bias and the peak background split

Reference 72

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Accelerating HI density predictions during the Epoch of Reionization using a GPR-based emulator on N-body simulations cites this paper.

Accelerating HI density predictions during the Epoch of Reionization using a GPR-based emulator on N-body simulations Large scale bias and the peak background split

Reference 32

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Observation 3ad8b362-986a-42c3-ab5d-11ff216a1565 · inbound

The ACCEL2 Project: Precision Measurements of EFT Parameters and BAO Peak Shifts for the Lyman-$\alpha$ Forest cites this paper.

The ACCEL2 Project: Precision Measurements of EFT Parameters and BAO Peak Shifts for the Lyman-$\alpha$ Forest Large scale bias and the peak background split

Reference 127

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Observation d0c98e5a-656e-48e3-8ac9-a77b9f64eb54 · inbound

Simulation-based inference on warm dark matter from HERA forecasts cites this paper.

Simulation-based inference on warm dark matter from HERA forecasts Large scale bias and the peak background split

Reference 63

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Observation d3ae9f00-1abc-4dc3-a49b-0fcb6eb89124 · inbound

Impact of light sterile neutrinos on cosmological large scale structure cites this paper.

Impact of light sterile neutrinos on cosmological large scale structure Large scale bias and the peak background split

Reference 59

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Observation 0d0c2b36-a741-44bb-8e85-f4f9d4ebd6ae · inbound

The Irrelevance of Primordial Black Hole Clustering in the LVK mass range cites this paper.

The Irrelevance of Primordial Black Hole Clustering in the LVK mass range Large scale bias and the peak background split

Reference 112

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Observation e48a07a2-e2f1-4a4f-835f-b56040cbea26 · inbound

Joint 21-cm and CMB Forecasts for Constraining Self-Interacting Massive Neutrinos cites this paper.

Joint 21-cm and CMB Forecasts for Constraining Self-Interacting Massive Neutrinos Large scale bias and the peak background split

Reference 113

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Vlasov Perturbation Theory applied to $\Lambda$CDM cites this paper.

Vlasov Perturbation Theory applied to $\Lambda$CDM Large scale bias and the peak background split

Reference 31

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Observation 68a4e059-23f1-4432-b200-4ddb38db15c1 · inbound

Modeling Gravitational Wave Bias from 3D Power Spectra of Spectroscopic Surveys cites this paper.

Modeling Gravitational Wave Bias from 3D Power Spectra of Spectroscopic Surveys Large scale bias and the peak background split

Reference 42

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Observation e5979869-fcf2-406b-91ee-7ddaed312508 · inbound

Not-quite-primordial black holes cites this paper.

Not-quite-primordial black holes Large scale bias and the peak background split

Reference 65

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Observation b61408b2-2c64-4635-8cc9-70aeeecf0266 · inbound

Cosmological Remapping for Efficient Generation of 21 cm Intensity Mapping Mocks cites this paper.

Cosmological Remapping for Efficient Generation of 21 cm Intensity Mapping Mocks Large scale bias and the peak background split

Reference 41

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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 Large scale bias and the peak background split

Reference 61

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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 Large scale bias and the peak background split

Reference 47

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Influence of supermassive primordial black holes on ultraviolet luminosity of high-redshift galaxies cites this paper.

Influence of supermassive primordial black holes on ultraviolet luminosity of high-redshift galaxies Large scale bias and the peak background split

Reference 82

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Conditioning halos on the tidal environment for fast and accurate HI power spectra during reionization cites this paper.

Conditioning halos on the tidal environment for fast and accurate HI power spectra during reionization Large scale bias and the peak background split

Reference 24

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Direct Collapse Black Hole Candidates from Decaying Dark Matter cites this paper.

Direct Collapse Black Hole Candidates from Decaying Dark Matter Large scale bias and the peak background split

Reference 135

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Dark Secrets of Baryons: Illuminating Dark Matter-Baryon Interactions with JWST cites this paper.

Dark Secrets of Baryons: Illuminating Dark Matter-Baryon Interactions with JWST Large scale bias and the peak background split

Reference 277

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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 Large scale bias and the peak background split

Reference 34

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21 cm Cosmology Sensitivity to Small-Scale Structure: Warm vs Neutrino-Interacting Dark Matter cites this paper.

21 cm Cosmology Sensitivity to Small-Scale Structure: Warm vs Neutrino-Interacting Dark Matter Large scale bias and the peak background split

Reference 80

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

An essential building block for cosmological zoom-in perturbation theory Large scale bias and the peak background split

Reference 20

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A Variable-Slope Smooth-$k$ Filter for Modeling Halo Abundances with Damped and Oscillatory Power Spectra cites this paper.

A Variable-Slope Smooth-$k$ Filter for Modeling Halo Abundances with Damped and Oscillatory Power Spectra Large scale bias and the peak background split

Reference 51

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Sound Mode and Scale-Dependent Growth in Two-Fluid Dynamical Dark Energy cites this paper.

Sound Mode and Scale-Dependent Growth in Two-Fluid Dynamical Dark Energy Large scale bias and the peak background split

Reference 140

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Reionization Topology as a Probe of Self-Interacting Dark Matter cites this paper.

Reionization Topology as a Probe of Self-Interacting Dark Matter Large scale bias and the peak background split

Reference 35

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

An Improved Fit for Linear Halo Bias at High Redshift Large scale bias and the peak background split

Reference 12

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Breaking the UV Luminosity Function Degeneracy:Self-Interacting Dark Matter Constraints from Reionization Topology cites this paper.

Breaking the UV Luminosity Function Degeneracy:Self-Interacting Dark Matter Constraints from Reionization Topology Large scale bias and the peak background split

Reference 28

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

Anisotropy of Cosmic Background Photons from Annihilating/Decaying Dark Matter Large scale bias and the peak background split

Reference 51

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Primordial Magnetic Fields at Cosmic Dawn: 21-cm Forecasts with HERA and SKA cites this paper.

Primordial Magnetic Fields at Cosmic Dawn: 21-cm Forecasts with HERA and SKA Large scale bias and the peak background split

Reference 60

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Spherical collapse and cluster number counts in DHOST theories that pass the constraints from gravitational waves cites this paper.

Spherical collapse and cluster number counts in DHOST theories that pass the constraints from gravitational waves Large scale bias and the peak background split

Reference 21

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Supermassive black hole seeds from direct collapse of CDM-curvature peaks cites this paper.

Supermassive black hole seeds from direct collapse of CDM-curvature peaks Large scale bias and the peak background split

Reference 145

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Optimal Transport Reconstruction of Biased Tracers in Primordial Non-Gaussian Fields cites this paper.

Optimal Transport Reconstruction of Biased Tracers in Primordial Non-Gaussian Fields Large scale bias and the peak background split

Reference 13

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Too Heavy to Hide: Gamma-Ray Constraints on Annihilating Dark Matter beyond Unitarity cites this paper.

Too Heavy to Hide: Gamma-Ray Constraints on Annihilating Dark Matter beyond Unitarity Large scale bias and the peak background split

Reference 150

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Non-linear Structure Formation in Planck+DESI Favoured Interacting Dark Energy Cosmologies cites this paper.

Non-linear Structure Formation in Planck+DESI Favoured Interacting Dark Energy Cosmologies Large scale bias and the peak background split

Reference 103

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Probing the fate of large primordial perturbations with exoplanets cites this paper.

Probing the fate of large primordial perturbations with exoplanets Large scale bias and the peak background split

Reference 95

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Spherical Collapse and Halo Formation in a Cosmology with Decaying Dark Matter and a Semi-Cosmographic Dark Energy cites this paper.

Spherical Collapse and Halo Formation in a Cosmology with Decaying Dark Matter and a Semi-Cosmographic Dark Energy Large scale bias and the peak background split

Reference 70

Resolution
verified exact
local_arxiv, observed 2026-07-04T14:19:54.143728Z

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.

source=pdf_text observed=2026-06-26T04:08:17.208050Z digest=sha256:b01643598a7fc0971572e19a08bac247e8a576addee1bc40fda557129f8b72e4

Observation 717cb920-50da-4407-b1e6-5409b4df3a40 · inbound

Core-Halo Mass Relation in Cosmological Vector Dark Matter cites this paper.

Core-Halo Mass Relation in Cosmological Vector Dark Matter Large scale bias and the peak background split

Reference 52

Resolution
unresolved
no resolver link, observed 2026-08-01T16:24:14.621460Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T16:24:14.621460Z digest=sha256:b76e375d2ee5067d677194dbe35c1069335dffb89501bc0eb16fecc5f1ac13c6

Observation ad9c2180-96df-473d-b5a6-11a0edd8f3af · 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 Large scale bias and the peak background split

Reference 13

Resolution
unresolved
no resolver link, observed 2026-08-01T07:53:19.875370Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T07:53:19.875370Z digest=sha256:3777e90bf996ebd1703dd769d584cf85815983178257c7d339fd79658f229bd2

Observation 5b7975cd-60f9-45f7-80c7-e68bfbae31f6 · inbound

Interlopers as Signal in Line Intensity Mapping cites this paper.

Interlopers as Signal in Line Intensity Mapping Large scale bias and the peak background split

Reference 27

Resolution
unresolved
no resolver link, observed 2026-07-31T06:02:18.691975Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-07-31T06:02:18.691975Z digest=sha256:fce30f4cd4d3d6d6ab2ccb6ec86f765e002812d2619d4207b6b8a9432583754b

Observation 65b2ca2f-704b-4de7-9918-42fc7dea782b · inbound

Searching for Population III stars with line intensity mapping cross-correlations cites this paper.

Searching for Population III stars with line intensity mapping cross-correlations Large scale bias and the peak background split

Reference 94

Resolution
unresolved
no resolver link, observed 2026-08-03T00:21:45.505892Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-03T00:21:45.505892Z digest=sha256:0c046e74e2370e1f71a838d6805056e591219a3e136988ff09893f24c3b64f72

Observation 128c9a3a-8610-4505-b459-d445bca8e4b7 · inbound

The One-Loop Power Spectrum of Fast Radio Burst Dispersion Measures cites this paper.

The One-Loop Power Spectrum of Fast Radio Burst Dispersion Measures Large scale bias and the peak background split

Reference 128

Resolution
unresolved
no resolver link, observed 2026-08-05T23:03:10.196081Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-05T23:03:10.196081Z digest=sha256:9608dacdfa69dc4dd57fc78c79f7db00272bd352a2653323e2bd16a0ef8836cc