Paper Citation Record · LEDGER

The Large Scale Bias of Dark Matter Halos: Numerical Calibration and Model Tests

As of 12 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 30 inbound Pith citation observations for arXiv:1001.3162.

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

pith.paper-citation-record.v1
1001.3162 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 30 of 30 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-11T06:34:44.6726+00:00

measured 30 of 30 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-12T00:58:57.673091Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-02T11:06:53.095115Z

Reference resolution

0 of 0 outbound references displayed

verified exact0
verified fuzzy0
unresolved0
parse uncertain0
malformed identifier0
metadata mismatch0

External citation measurements

No source-named external measurement is stored.

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 54c3b638-0247-4ee7-a273-88ca9c7a0937 · inbound

The Millennium and Astrid galaxies in effective field theory: comparison with galaxy-halo connection models at the field level cites this paper.

The Millennium and Astrid galaxies in effective field theory: comparison with galaxy-halo connection models at the field level The Large Scale Bias of Dark Matter Halos: Numerical Calibration and Model Tests

Reference 130

Resolution: unresolved; no resolver link, observed 2026-08-12T00:58:57.673091Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 5463b89a-7325-49a0-a323-a85f6eccc78c · inbound

Towards a multi-tracer neutrino mass measurement with line-intensity mapping cites this paper.

Towards a multi-tracer neutrino mass measurement with line-intensity mapping The Large Scale Bias of Dark Matter Halos: Numerical Calibration and Model Tests

Reference 115

Resolution: unresolved; no resolver link, observed 2026-08-11T21:53:33.766783Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 4f2c5a37-5286-4279-a1a6-1c4211bc6ca9 · inbound

DEMNUni: the Sunyaev-Zel'dovich effect in the presence of massive neutrinos and dynamical dark energy cites this paper.

DEMNUni: the Sunyaev-Zel'dovich effect in the presence of massive neutrinos and dynamical dark energy The Large Scale Bias of Dark Matter Halos: Numerical Calibration and Model Tests

Reference 52

Resolution: verified exact; local_arxiv, observed 2026-05-22T23:07:13.976035Z

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 5ef307d1-0589-4861-be3a-3ff755b3a53a · inbound

Scale-dependent bias and mode coupling in redshift-space clustering near the BAO scale cites this paper.

Scale-dependent bias and mode coupling in redshift-space clustering near the BAO scale The Large Scale Bias of Dark Matter Halos: Numerical Calibration and Model Tests

Reference 52

Resolution: unresolved; no resolver link, observed 2026-08-07T05:29:08.941478Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 3b40e9d0-d3fe-45fd-9903-492ca799375a · inbound

Patchy Helium and Hydrogen Reionization from the Kinetic Sunyaev-Zel'dovich Effect and Galaxies cites this paper.

Patchy Helium and Hydrogen Reionization from the Kinetic Sunyaev-Zel'dovich Effect and Galaxies The Large Scale Bias of Dark Matter Halos: Numerical Calibration and Model Tests

Reference 104

Resolution: unresolved; no resolver link, observed 2026-08-07T04:24:07.644697Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 22f92cd0-bbc9-4071-a266-265d78b69233 · inbound

Comparison of Halo Model and Simulation Predictions for Projected-Field Kinematic Sunyaev-Zel'dovich Cross-Correlations cites this paper.

Comparison of Halo Model and Simulation Predictions for Projected-Field Kinematic Sunyaev-Zel'dovich Cross-Correlations The Large Scale Bias of Dark Matter Halos: Numerical Calibration and Model Tests

Reference 28

Resolution: verified exact; local_arxiv, observed 2026-05-21T22:34:23.857671Z

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 469ae10a-e61a-4075-96f9-3b3694d20c73 · inbound

Impact of projection-induced optical selection bias on the weak lensing mass calibration of galaxy clusters cites this paper.

Impact of projection-induced optical selection bias on the weak lensing mass calibration of galaxy clusters The Large Scale Bias of Dark Matter Halos: Numerical Calibration and Model Tests

Reference 52

Resolution: verified exact; local_arxiv, observed 2026-05-18T10:56:17.526942Z

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 e33d0caa-08d8-4a3c-ae61-c5496279d9a1 · inbound

Sahyadri: A simulation suite for the cosmology dependence of the Cosmic Web cites this paper.

Sahyadri: A simulation suite for the cosmology dependence of the Cosmic Web The Large Scale Bias of Dark Matter Halos: Numerical Calibration and Model Tests

Reference 73

Resolution: unresolved; no resolver link, observed 2026-08-03T11:05:46.218696Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c8581e0d-8ff5-4c3b-bbb3-666e07b8e201 · inbound

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 The Large Scale Bias of Dark Matter Halos: Numerical Calibration and Model Tests

Reference 141

Resolution: unresolved; no resolver link, observed 2026-07-15T14:51:12.413085Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 85d36ca3-c10f-465a-b2f3-afdb996072b2 · inbound

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

An Improved Fit for Linear Halo Bias at High Redshift The Large Scale Bias of Dark Matter Halos: Numerical Calibration and Model Tests

Reference 15

Resolution: verified exact; arxiv_id, observed 2026-05-10T12:00:21.891669Z

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 763dea76-8766-4b87-bc31-7db97ffd1fcd · inbound

FLAMINGO: The thermal history of the Universe from tSZ effect cross-correlations and its dependencies on cosmology and baryon physics cites this paper.

FLAMINGO: The thermal history of the Universe from tSZ effect cross-correlations and its dependencies on cosmology and baryon physics The Large Scale Bias of Dark Matter Halos: Numerical Calibration and Model Tests

Reference 26

Resolution: metadata mismatch; local_arxiv, observed 2026-05-14T21:07:58.819076Z

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 5c3709a5-c0f3-4072-a7f7-340bfe4106a8 · inbound

Probing nonlinear structure formation beyond $\Lambda$CDM with the LSS bootstrap: a joint power spectrum and bispectrum analysis cites this paper.

Probing nonlinear structure formation beyond $\Lambda$CDM with the LSS bootstrap: a joint power spectrum and bispectrum analysis The Large Scale Bias of Dark Matter Halos: Numerical Calibration and Model Tests

Reference 66

Resolution: verified exact; local_arxiv, observed 2026-05-14T17:42:32.784727Z

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 43343d74-262e-446c-916b-fc774d201481 · inbound

Cosmological Constraints from Bias-Robust Wavelet Scattering Statistics for Stage-IV Galaxy Surveys cites this paper.

Cosmological Constraints from Bias-Robust Wavelet Scattering Statistics for Stage-IV Galaxy Surveys The Large Scale Bias of Dark Matter Halos: Numerical Calibration and Model Tests

Reference 21

Resolution: verified exact; local_arxiv, observed 2026-06-29T16:33:39.553918Z

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 17242095-2cb3-48ba-a288-df36027c9b2f · inbound

Reduced Incidence of Little Red Dots at z < 3 from Number Density and Halo Mass Evolution cites this paper.

Reduced Incidence of Little Red Dots at z < 3 from Number Density and Halo Mass Evolution The Large Scale Bias of Dark Matter Halos: Numerical Calibration and Model Tests

Reference 98

Resolution: verified exact; local_arxiv, observed 2026-06-28T13:22:14.961134Z

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 8056be6a-9266-4afc-a516-85582c0934c8 · inbound

Reduced Incidence of Little Red Dots at z < 3 from Number Density and Halo Mass Evolution cites this paper.

Reduced Incidence of Little Red Dots at z < 3 from Number Density and Halo Mass Evolution The Large Scale Bias of Dark Matter Halos: Numerical Calibration and Model Tests

Reference 98

Resolution: unresolved; no resolver link, observed 2026-08-02T12:34:34.361410Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d57e2ed6-01bf-4430-b16f-0a4f8b281cc8 · inbound

Full Nonlinear Velocity Reconstruction With Transformer and Ensemble Tree Machine Learning cites this paper.

Full Nonlinear Velocity Reconstruction With Transformer and Ensemble Tree Machine Learning The Large Scale Bias of Dark Matter Halos: Numerical Calibration and Model Tests

Reference 70

Resolution: verified exact; local_arxiv, observed 2026-07-02T11:06:53.096633Z

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 774aa51c-1a45-4d10-a0e5-91e03ecf465f · 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 The Large Scale Bias of Dark Matter Halos: Numerical Calibration and Model Tests

Reference 37

Resolution: verified exact; local_arxiv, observed 2026-06-27T09:40:48.030297Z

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 ab21196a-151e-4d13-9e3f-dce86ecd7f62 · 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 The Large Scale Bias of Dark Matter Halos: Numerical Calibration and Model Tests

Reference 78

Resolution: verified exact; local_arxiv, observed 2026-06-26T10:09:17.901455Z

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 cf0766ec-9e69-4f7b-8605-9799bb680b46 · inbound

Anisotropic quenching beyond $z=1$ and its implications for preprocessing around high-redshift galaxy clusters cites this paper.

Anisotropic quenching beyond $z=1$ and its implications for preprocessing around high-redshift galaxy clusters The Large Scale Bias of Dark Matter Halos: Numerical Calibration and Model Tests

Reference 280

Resolution: verified exact; local_arxiv, observed 2026-06-26T07:59:08.869850Z

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 926e90e4-5b79-4aa4-850d-4a4ddfb049f6 · inbound

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

Using SKAO to Understand the Clustering of Gravitational Wave Sources The Large Scale Bias of Dark Matter Halos: Numerical Calibration and Model Tests

Reference 130

Resolution: metadata mismatch; local_arxiv, observed 2026-06-25T23:08:41.077638Z

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 4ced6b0d-e18e-4615-ad1c-ed3c480c866c · inbound

Thermal Sunyaev-Zel'dovich cross-correlations with unWISE galaxies: disentangling radio contamination, dust properties, and electron pressure cites this paper.

Thermal Sunyaev-Zel'dovich cross-correlations with unWISE galaxies: disentangling radio contamination, dust properties, and electron pressure The Large Scale Bias of Dark Matter Halos: Numerical Calibration and Model Tests

Reference 129

Resolution: verified exact; local_arxiv, observed 2026-06-29T03:03:03.752847Z

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 ff562044-37a3-470b-a734-f4640c039eae · inbound

Searching for primordial features with radio surveys: synergy between the power spectrum and bispectrum cites this paper.

Searching for primordial features with radio surveys: synergy between the power spectrum and bispectrum The Large Scale Bias of Dark Matter Halos: Numerical Calibration and Model Tests

Reference 112

Resolution: verified exact; local_arxiv, observed 2026-07-01T17:55:52.351457Z

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 05e36827-47fd-4a9b-924e-9c3251d79f6e · inbound

Cosmology-dependent covariance in galaxy cluster number counts: consequences for parameter inference cites this paper.

Cosmology-dependent covariance in galaxy cluster number counts: consequences for parameter inference The Large Scale Bias of Dark Matter Halos: Numerical Calibration and Model Tests

Reference 60

Resolution: verified exact; local_arxiv, observed 2026-06-30T16:04:53.420819Z

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 596de688-1897-4770-ba11-d930bba2fc15 · 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? The Large Scale Bias of Dark Matter Halos: Numerical Calibration and Model Tests

Reference 205

Resolution: verified exact; local_arxiv, observed 2026-07-01T04:05:20.589045Z

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 335e1cfe-79b7-4b1a-88ae-f116cb20532f · inbound

Assembly bias and the redshift evolution of intrinsic alignments for LRGs cites this paper.

Assembly bias and the redshift evolution of intrinsic alignments for LRGs The Large Scale Bias of Dark Matter Halos: Numerical Calibration and Model Tests

Reference 117

Resolution: verified exact; local_arxiv, observed 2026-07-02T06:46:43.843303Z

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 be782cc9-0d2a-4d5d-88a0-a2ed061c7872 · inbound

Constraints on Annihilating Dark Matter from Gamma-Ray Background-Galaxy Shape Correlations: Model-independent Null Results and Moderate Template-based Signals cites this paper.

Constraints on Annihilating Dark Matter from Gamma-Ray Background-Galaxy Shape Correlations: Model-independent Null Results and Moderate Template-based Signals The Large Scale Bias of Dark Matter Halos: Numerical Calibration and Model Tests

Reference 36

Resolution: unresolved; no resolver link, observed 2026-07-14T07:56:20.592048Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c1ec83ff-9bcb-468b-9795-2e5166a3fec1 · inbound

Simulation-Based Priors for HI Bias from Halo Occupation Physics cites this paper.

Simulation-Based Priors for HI Bias from Halo Occupation Physics The Large Scale Bias of Dark Matter Halos: Numerical Calibration and Model Tests

Reference 59

Resolution: unresolved; no resolver link, observed 2026-08-02T02:52:38.804765Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 5f82f34b-da9e-4fd2-9af8-1c7601c9a7aa · 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 The Large Scale Bias of Dark Matter Halos: Numerical Calibration and Model Tests

Reference 59

Resolution: unresolved; no resolver link, observed 2026-08-01T07:53:24.293468Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 0419044b-ce2b-41dd-ba8c-2c8956ea1a99 · 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 The Large Scale Bias of Dark Matter Halos: Numerical Calibration and Model Tests

Reference 160

Resolution: unresolved; no resolver link, observed 2026-07-31T05:29:30.132412Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f54b96b4-3653-436b-839b-eb7bd063af2f · inbound

Emulating the nonlinear effects of modified gravity on the matter power spectrum for reconstruction cites this paper.

Emulating the nonlinear effects of modified gravity on the matter power spectrum for reconstruction The Large Scale Bias of Dark Matter Halos: Numerical Calibration and Model Tests

Reference 73

Resolution: unresolved; no resolver link, observed 2026-08-03T01:55:16.837830Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.