Paper Citation Record · LEDGER

Reanalyzing DESI DR1: 5. Cosmological Constraints with Simulation-Based Priors

As of 4 August 2026, this Paper Citation Record lists 100 of 131 outbound references and 10 inbound Pith citation observations for arXiv:2602.18554.

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pith.paper-citation-record.v1
2602.18554 v2

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Outbound references

Observation 4068ea9a-8de5-4efc-8ab7-8ad6daadbe09 · outbound

This paper cites an unresolved cited work.

Reanalyzing DESI DR1: 5. Cosmological Constraints with Simulation-Based Priors Unresolved cited work

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Reanalyzing DESI DR1: 5. Cosmological Constraints with Simulation-Based Priors Unresolved cited work

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Reanalyzing DESI DR1: 5. Cosmological Constraints with Simulation-Based Priors Unresolved cited work

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Reanalyzing DESI DR1: 5. Cosmological Constraints with Simulation-Based Priors decorated

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Reanalyzing DESI DR1: 5. Cosmological Constraints with Simulation-Based Priors kitchen sink

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Reanalyzing DESI DR1: 5. Cosmological Constraints with Simulation-Based Priors kitchen sink

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This paper cites Redshift Space Distortions in the Effective Field Theory of Large Scale Structures.

Reanalyzing DESI DR1: 5. Cosmological Constraints with Simulation-Based Priors Redshift Space Distortions in the Effective Field Theory of Large Scale Structures

Reference 7

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Reanalyzing DESI DR1: 5. Cosmological Constraints with Simulation-Based Priors Cosmological Non-Linearities as an Effective Fluid

Reference 8

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Reanalyzing DESI DR1: 5. Cosmological Constraints with Simulation-Based Priors The Effective Field Theory of Cosmological Large Scale Structures

Reference 9

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Reanalyzing DESI DR1: 5. Cosmological Constraints with Simulation-Based Priors Effective Field Theory for Large Scale Structure

Reference 10

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Reanalyzing DESI DR1: 5. Cosmological Constraints with Simulation-Based Priors Renormalized Halo Bias

Reference 11

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Reanalyzing DESI DR1: 5. Cosmological Constraints with Simulation-Based Priors Biased Tracers and Time Evolution

Reference 12

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Reanalyzing DESI DR1: 5. Cosmological Constraints with Simulation-Based Priors Bias in the Effective Field Theory of Large Scale Structures

Reference 13

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Reanalyzing DESI DR1: 5. Cosmological Constraints with Simulation-Based Priors Time-Sliced Perturbation Theory for Large Scale Structure I: General Formalism

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Reanalyzing DESI DR1: 5. Cosmological Constraints with Simulation-Based Priors The IR-resummed Effective Field Theory of Large Scale Structures

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This paper cites Equivalence Principle and the Baryon Acoustic Peak.

Reanalyzing DESI DR1: 5. Cosmological Constraints with Simulation-Based Priors Equivalence Principle and the Baryon Acoustic Peak

Reference 16

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This paper cites A Lagrangian effective field theory.

Reanalyzing DESI DR1: 5. Cosmological Constraints with Simulation-Based Priors A Lagrangian effective field theory

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Reanalyzing DESI DR1: 5. Cosmological Constraints with Simulation-Based Priors Perturbation theory, effective field theory, and oscillations in the power spectrum

Reference 18

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Reanalyzing DESI DR1: 5. Cosmological Constraints with Simulation-Based Priors The Gaussian streaming model and Lagrangian effective field theory

Reference 19

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Reanalyzing DESI DR1: 5. Cosmological Constraints with Simulation-Based Priors Exploring redshift-space distortions in large-scale structure

Reference 20

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Reanalyzing DESI DR1: 5. Cosmological Constraints with Simulation-Based Priors The Cosmological Analysis of the SDSS/BOSS data from the Effective Field Theory of Large-Scale Structure

Reference 21

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Reanalyzing DESI DR1: 5. Cosmological Constraints with Simulation-Based Priors Time-Sliced Perturbation Theory II: Baryon Acoustic Oscillations and Infrared Resummation

Reference 22

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Reanalyzing DESI DR1: 5. Cosmological Constraints with Simulation-Based Priors Infrared Resummation for Biased Tracers in Redshift Space

Reference 23

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This paper cites Time-sliced perturbation theory with primordial non-Gaussianity and effects of large bulk flows on inflationary oscillating features.

Reanalyzing DESI DR1: 5. Cosmological Constraints with Simulation-Based Priors Time-sliced perturbation theory with primordial non-Gaussianity and effects of large bulk flows on inflationary oscillating features

Reference 24

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Reanalyzing DESI DR1: 5. Cosmological Constraints with Simulation-Based Priors Consistent Modeling of Velocity Statistics and Redshift-Space Distortions in One-Loop Perturbation Theory

Reference 25

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Reanalyzing DESI DR1: 5. Cosmological Constraints with Simulation-Based Priors Redshift-Space Distortions in Lagrangian Perturbation Theory

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Reanalyzing DESI DR1: 5. Cosmological Constraints with Simulation-Based Priors Cosmological Parameters from the BOSS Galaxy Power Spectrum

Reference 27

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Reanalyzing DESI DR1: 5. Cosmological Constraints with Simulation-Based Priors Chudaykin, M

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Reanalyzing DESI DR1: 5. Cosmological Constraints with Simulation-Based Priors Combining Full-Shape and BAO Analyses of Galaxy Power Spectra: A 1.6% CMB-independent constraint on H0

Reference 29

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Reanalyzing DESI DR1: 5. Cosmological Constraints with Simulation-Based Priors The BOSS DR12 Full-Shape Cosmology: $\Lambda$CDM Constraints from the Large-Scale Galaxy Power Spectrum and Bispectrum Monopole

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Reanalyzing DESI DR1: 5. Cosmological Constraints with Simulation-Based Priors A new analysis of galaxy 2-point functions in the BOSS survey, including full-shape information and post-reconstruction BAO

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Reanalyzing DESI DR1: 5. Cosmological Constraints with Simulation-Based Priors Cosmological Analysis of Three-Dimensional BOSS Galaxy Clustering and Planck CMB Lensing Cross Correlations via Lagrangian Perturbation Theory

Reference 32

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Reanalyzing DESI DR1: 5. Cosmological Constraints with Simulation-Based Priors Suppression without Thawing: Constraining Structure Formation and Dark Energy with Galaxy Clustering

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Reanalyzing DESI DR1: 5. Cosmological Constraints with Simulation-Based Priors DESI 2024 VII: Cosmological Constraints from the Full-Shape Modeling of Clustering Measurements

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Reanalyzing DESI DR1: 5. Cosmological Constraints with Simulation-Based Priors An analysis of parameter compression and full-modeling techniques with Velocileptors for DESI 2024 and beyond

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Reanalyzing DESI DR1: 5. Cosmological Constraints with Simulation-Based Priors Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses

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Reanalyzing DESI DR1: 5. Cosmological Constraints with Simulation-Based Priors Chudaykin, M

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Reanalyzing DESI DR1: 5. Cosmological Constraints with Simulation-Based Priors Reanalyzing DESI DR1: 4. Percent-Level Cosmological Constraints from Combined Probes and Robust Evidence for the Normal Neutrino Mass Hierarchy

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Reanalyzing DESI DR1: 5. Cosmological Constraints with Simulation-Based Priors Large-Scale Galaxy Bias

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Reanalyzing DESI DR1: 5. Cosmological Constraints with Simulation-Based Priors The Connection between Galaxies and their Dark Matter Halos

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Reanalyzing DESI DR1: 5. Cosmological Constraints with Simulation-Based Priors Non-linear perturbation theory extension of the Boltzmann code CLASS

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Reanalyzing DESI DR1: 5. Cosmological Constraints with Simulation-Based Priors Modeling Galaxy Surveys with Hybrid SBI

Reference 42

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Reanalyzing DESI DR1: 5. Cosmological Constraints with Simulation-Based Priors Unresolved cited work

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Reanalyzing DESI DR1: 5. Cosmological Constraints with Simulation-Based Priors Full-shape analysis with simulation-based priors: constraints on single field inflation from BOSS

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Reanalyzing DESI DR1: 5. Cosmological Constraints with Simulation-Based Priors Full-shape analysis with simulation-based priors: cosmological parameters and the structure growth anomaly

Reference 45

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Reanalyzing DESI DR1: 5. Cosmological Constraints with Simulation-Based Priors The Millennium and Astrid galaxies in effective field theory: comparison with galaxy-halo connection models at the field level

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Reanalyzing DESI DR1: 5. Cosmological Constraints with Simulation-Based Priors BOSS Constraints on Massive Particles during Inflation: The Cosmological Collider in Action

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Reanalyzing DESI DR1: 5. Cosmological Constraints with Simulation-Based Priors Mapping the galaxy-halo connection to the galaxy bias: implication to the HOD-informed prior

Reference 48

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Reanalyzing DESI DR1: 5. Cosmological Constraints with Simulation-Based Priors Simulation-Based Priors without Simulations: an Analytic Perspective on EFT Parameters of Galaxies

Reference 49

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Reanalyzing DESI DR1: 5. Cosmological Constraints with Simulation-Based Priors Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors

Reference 50

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Reanalyzing DESI DR1: 5. Cosmological Constraints with Simulation-Based Priors HOD-informed prior for EFT-based full-shape analyses of LSS

Reference 51

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Reanalyzing DESI DR1: 5. Cosmological Constraints with Simulation-Based Priors An Analytic Hybrid Halo + Perturbation Theory Model for Small-scale Correlators: Baryons, Halos, and Galaxies

Reference 52

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Reanalyzing DESI DR1: 5. Cosmological Constraints with Simulation-Based Priors Extending the modeling of the anisotropic galaxy power spectrum to $k = 0.4 \ h\mathrm{Mpc}^{-1}$

Reference 53

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Observation 146023d4-16c6-4419-bba9-ec606c16c348 · outbound

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Reanalyzing DESI DR1: 5. Cosmological Constraints with Simulation-Based Priors Enhancing DESI DR1 Full-Shape analyses using HOD-informed priors

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Reanalyzing DESI DR1: 5. Cosmological Constraints with Simulation-Based Priors Data Release 1 of the Dark Energy Spectroscopic Instrument

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Reanalyzing DESI DR1: 5. Cosmological Constraints with Simulation-Based Priors SUNBIRD: A simulation-based model for full-shape density-split clustering

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Reanalyzing DESI DR1: 5. Cosmological Constraints with Simulation-Based Priors The DESI One-Percent Survey: Exploring the Halo Occupation Distribution of Luminous Red Galaxies and Quasi-Stellar Objects with AbacusSummit

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Reanalyzing DESI DR1: 5. Cosmological Constraints with Simulation-Based Priors The DESI One-Percent survey: exploring the Halo Occupation Distribution of Emission Line Galaxies with AbacusSummit simulations

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Reanalyzing DESI DR1: 5. Cosmological Constraints with Simulation-Based Priors Mauset al., JCAP11, 077 (2025), arXiv:2505.20656 [astro-ph.CO]

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Reanalyzing DESI DR1: 5. Cosmological Constraints with Simulation-Based Priors NuFit-6.0: Updated global analysis of three-flavor neutrino oscillations

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Reanalyzing DESI DR1: 5. Cosmological Constraints with Simulation-Based Priors Planck intermediate results. XVI. Profile likelihoods for cosmological parameters

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Reanalyzing DESI DR1: 5. Cosmological Constraints with Simulation-Based Priors Updated results on neutrino mass and mass hierarchy from cosmology with Planck 2018 likelihoods

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Reanalyzing DESI DR1: 5. Cosmological Constraints with Simulation-Based Priors No $\nu$s is Good News

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Reanalyzing DESI DR1: 5. Cosmological Constraints with Simulation-Based Priors Massive neutrinos and cosmic composition

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Reanalyzing DESI DR1: 5. Cosmological Constraints with Simulation-Based Priors The Cosmological Preference for Negative Neutrino Mass

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Reanalyzing DESI DR1: 5. Cosmological Constraints with Simulation-Based Priors Negative neutrino masses as a mirage of dark energy

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Reanalyzing DESI DR1: 5. Cosmological Constraints with Simulation-Based Priors Blinded challenge for precision cosmology with large-scale structure: results from effective field theory for the redshift-space galaxy power spectrum

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Reanalyzing DESI DR1: 5. Cosmological Constraints with Simulation-Based Priors Constraints on the curvature of the Universe and dynamical dark energy from the Full-shape and BAO data

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Reanalyzing DESI DR1: 5. Cosmological Constraints with Simulation-Based Priors Precision analysis of the redshift-space galaxy bispectrum

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Reanalyzing DESI DR1: 5. Cosmological Constraints with Simulation-Based Priors Cosmological constraints without fingers of God

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Reanalyzing DESI DR1: 5. Cosmological Constraints with Simulation-Based Priors Optimizing large-scale structure data analysis with the theoretical error likelihood

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Reanalyzing DESI DR1: 5. Cosmological Constraints with Simulation-Based Priors Cosmological constraints from the power spectrum of eBOSS quasars

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Reanalyzing DESI DR1: 5. Cosmological Constraints with Simulation-Based Priors DESI DR2 Results II: Measurements of Baryon Acoustic Oscillations and Cosmological Constraints

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Reanalyzing DESI DR1: 5. Cosmological Constraints with Simulation-Based Priors DESI DR2 Results I: Baryon Acoustic Oscillations from the Lyman Alpha Forest

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Reanalyzing DESI DR1: 5. Cosmological Constraints with Simulation-Based Priors An analytic approximation to the covariance between pre- and post-reconstruction galaxy two-point statistics

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Reanalyzing DESI DR1: 5. Cosmological Constraints with Simulation-Based Priors Planck 2018 results. I. Overview and the cosmological legacy of Planck

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Reanalyzing DESI DR1: 5. Cosmological Constraints with Simulation-Based Priors CMB lensing from Planck PR4 maps

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Reanalyzing DESI DR1: 5. Cosmological Constraints with Simulation-Based Priors The Atacama Cosmology Telescope: DR6 Gravitational Lensing Map and Cosmological Parameters

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Reanalyzing DESI DR1: 5. Cosmological Constraints with Simulation-Based Priors The Atacama Cosmology Telescope: A Measurement of the DR6 CMB Lensing Power Spectrum and its Implications for Structure Growth

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Reanalyzing DESI DR1: 5. Cosmological Constraints with Simulation-Based Priors The Pantheon+ Analysis: Cosmological Constraints

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Reanalyzing DESI DR1: 5. Cosmological Constraints with Simulation-Based Priors Chudaykin, M

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Reanalyzing DESI DR1: 5. Cosmological Constraints with Simulation-Based Priors Sailer, G

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Reanalyzing DESI DR1: 5. Cosmological Constraints with Simulation-Based Priors Sch¨ oneberg, JCAP06, 006 (2024), arXiv:2401.15054 [astro-ph.CO]

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Reanalyzing DESI DR1: 5. Cosmological Constraints with Simulation-Based Priors Conservative Constraints on Early Cosmology: an illustration of the Monte Python cosmological parameter inference code

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Reanalyzing DESI DR1: 5. Cosmological Constraints with Simulation-Based Priors MontePython 3: boosted MCMC sampler and other features

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Reanalyzing DESI DR1: 5. Cosmological Constraints with Simulation-Based Priors GetDist: a Python package for analysing Monte Carlo samples

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Reanalyzing DESI DR1: 5. Cosmological Constraints with Simulation-Based Priors Gelman and D

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Reanalyzing DESI DR1: 5. Cosmological Constraints with Simulation-Based Priors Kaiser, Mon

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Reanalyzing DESI DR1: 5. Cosmological Constraints with Simulation-Based Priors Bernardeau, S

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Reanalyzing DESI DR1: 5. Cosmological Constraints with Simulation-Based Priors Fingers of God

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Reanalyzing DESI DR1: 5. Cosmological Constraints with Simulation-Based Priors Chudaykin, M

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Reanalyzing DESI DR1: 5. Cosmological Constraints with Simulation-Based Priors The simple way to measure evolving dark energy without prior-volume effects

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Reanalyzing DESI DR1: 5. Cosmological Constraints with Simulation-Based Priors Reducing nuisance prior sensitivity via non-linear reparameterization, with application to EFT analyses of large-scale structure

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Reanalyzing DESI DR1: 5. Cosmological Constraints with Simulation-Based Priors Theoretical Models of the Halo Occupation Distribution: Separating Central and Satellite Galaxies

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Effective Field Theory of Large Scale Structure and Newtonian Motion Gauges Reanalyzing DESI DR1: 5. Cosmological Constraints with Simulation-Based Priors

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Observation ebf8028e-f6c5-4b98-b8c0-dea9335ff9cc · inbound

Galaxy Power Spectrum at Two-Loop Order: Implications for Weak Lensing Surveys and New Physics cites this paper.

Galaxy Power Spectrum at Two-Loop Order: Implications for Weak Lensing Surveys and New Physics Reanalyzing DESI DR1: 5. Cosmological Constraints with Simulation-Based Priors

Reference 38

Resolution: verified exact; arxiv_id, observed 2026-07-21T02:20:35.328941Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation f4855c79-a053-4b37-8f9a-a27a3844ac3e · inbound

Intertwined Constraints in Extended Cosmologies: Dark Energy, Curvature, Neutrinos, and Inflation cites this paper.

Intertwined Constraints in Extended Cosmologies: Dark Energy, Curvature, Neutrinos, and Inflation Reanalyzing DESI DR1: 5. Cosmological Constraints with Simulation-Based Priors

Reference 159

Resolution: verified exact; arxiv_id, observed 2026-07-21T02:20:35.328941Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation 104e459c-75f4-4efc-8aa9-8c65526c9f8e · inbound

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

Simulation-Based Priors for HI Bias from Halo Occupation Physics Reanalyzing DESI DR1: 5. Cosmological Constraints with Simulation-Based Priors

Reference 30

Resolution: unresolved; no resolver link, observed 2026-08-02T02:52:34.392211Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.