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Paper Citation Record · LEDGER

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors

As of 19 August 2026, this Paper Citation Record lists 100 of 104 outbound references and 7 inbound Pith citation observations for arXiv:2507.00118.

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pith.paper-citation-record.v1
2507.00118 v1

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measured 100 of 104 reference resolution

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measured 7 of 7 inbound itemization

Pith citing papers itemized under the disclosed page cap.

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measured 0 of 1 external citation measurements

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Source: arxiv_reference, observed 2026-05-17T04:19:00.846851Z

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100 of 104 outbound references displayed

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Outbound references

Observation 7627e816-bdc8-473c-86ef-70ff4f90f75a · outbound

This paper cites Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors

Reference 1

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Observation b948eff6-c865-42fa-97a6-36cac3a48b2b · outbound

This paper cites For instance, even at the level of the power spec- trum alone, there are eleven EFT nuisance parameters that must be marginalized over to constrain cosmological parameters.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors For instance, even at the level of the power spec- trum alone, there are eleven EFT nuisance parameters that must be marginalized over to constrain cosmological parameters

Reference 2

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Observation 65f33602-5cde-4140-b847-19fa394a003a · outbound

This paper cites We will present the detail of each experiment here and explain the pa- rameters varied in this section.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors We will present the detail of each experiment here and explain the pa- rameters varied in this section

Reference 3

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Observation a7b177c1-a02c-4be8-a916-bd2e1570c49b · outbound

This paper cites Gaussian.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Gaussian

Reference 4

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Observation 1c695ac2-f751-4021-9798-8fcde43f4e3b · outbound

This paper cites an unresolved cited work.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Unresolved cited work

Reference 5

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Observation 859a32ee-f9e7-4e8d-8a01-585c5b411b1e · outbound

This paper cites DESI 2024 VI: Cosmological Constraints from the Measurements of Baryon Acoustic Oscillations.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors DESI 2024 VI: Cosmological Constraints from the Measurements of Baryon Acoustic Oscillations

Reference 6

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Observation 059a5092-64a5-47b4-b966-81424a55fa32 · outbound

This paper cites DESI 2024 III: Baryon Acoustic Oscillations from Galaxies and Quasars.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors DESI 2024 III: Baryon Acoustic Oscillations from Galaxies and Quasars

Reference 7

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Observation c6f8f6ad-b20f-4c34-9f71-bcbaa61ec642 · outbound

This paper cites DESI DR2 Results II: Measurements of Baryon Acoustic Oscillations and Cosmological Constraints.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors DESI DR2 Results II: Measurements of Baryon Acoustic Oscillations and Cosmological Constraints

Reference 8

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Observation 77796c6b-a2a1-4ae0-a30b-0afd3987f2e0 · outbound

This paper cites Extended Dark Energy analysis using DESI DR2 BAO measurements.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Extended Dark Energy analysis using DESI DR2 BAO measurements

Reference 9

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Observation 7ce3cee7-64de-410a-a3f1-ab12539422f0 · outbound

This paper cites Euclid Definition Study Report.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Euclid Definition Study Report

Reference 10

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Observation 65d0bdf3-da30-4182-8e37-a162fa87b3e5 · outbound

This paper cites LSST: from Science Drivers to Reference Design and Anticipated Data Products.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors LSST: from Science Drivers to Reference Design and Anticipated Data Products

Reference 11

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Observation 3be237c7-4291-478c-8f68-e8c26dc3b16c · outbound

This paper cites The Wide Field Infrared Survey Telescope: 100 Hubbles for the 2020s.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors The Wide Field Infrared Survey Telescope: 100 Hubbles for the 2020s

Reference 12

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Observation 841d6954-b332-4b65-bcf8-bf40391528ed · outbound

This paper cites The EAGLE simulations of galaxy formation: public release of halo and galaxy catalogues.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors The EAGLE simulations of galaxy formation: public release of halo and galaxy catalogues

Reference 13

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This paper cites First results from the IllustrisTNG simulations: matter and galaxy clustering.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors First results from the IllustrisTNG simulations: matter and galaxy clustering

Reference 14

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This paper cites The MillenniumTNG Project: High-precision predictions for matter clustering and halo statistics.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors The MillenniumTNG Project: High-precision predictions for matter clustering and halo statistics

Reference 15

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Observation 7244e37d-b665-4e7c-ab34-3e1ecb783b6b · outbound

This paper cites The Halo Occupation Distribution: Towards an Empirical Determination of the Relation Between Galaxies and Mass.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors The Halo Occupation Distribution: Towards an Empirical Determination of the Relation Between Galaxies and Mass

Reference 16

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Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors The Dark Side of the Halo Occupation Distribution

Reference 17

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This paper cites Zheng, A.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Zheng, A

Reference 18

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Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Introducing Decorated HODs: modeling assembly bias in the galaxy-halo connection

Reference 19

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Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors The Connection between Galaxies and their Dark Matter Halos

Reference 20

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This paper cites A Parameter-Masked Mock Data Challenge for Beyond-Two-Point Galaxy Clustering Statistics.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors A Parameter-Masked Mock Data Challenge for Beyond-Two-Point Galaxy Clustering Statistics

Reference 21

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Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological analysis of the DR12 galaxy sample

Reference 22

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This paper cites Full-shape cosmology analysis of SDSS-III BOSS galaxy power spectrum using emulator-based halo model: a $5\%$ determination of $\sigma_8$.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Full-shape cosmology analysis of SDSS-III BOSS galaxy power spectrum using emulator-based halo model: a $5\%$ determination of $\sigma_8$

Reference 23

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Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors SUNBIRD: A simulation-based model for full-shape density-split clustering

Reference 24

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Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Precise Cosmological Constraints from BOSS Galaxy Clustering with a Simulation-Based Emulator of the Wavelet Scattering Transform

Reference 25

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Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors ${\rm S{\scriptsize IM}BIG}$: The First Cosmological Constraints from the Non-Linear Galaxy Bispectrum

Reference 26

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Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors ${\rm S{\scriptsize IM}BIG}$: Cosmological Constraints from the Redshift-Space Galaxy Skew Spectra

Reference 27

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Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Cosmological Non-Linearities as an Effective Fluid

Reference 28

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Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors The Effective Field Theory of Cosmological Large Scale Structures

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Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Effective Field Theory for Large Scale Structure

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Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Large-Scale Galaxy Bias

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Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Cosmological Parameters from the BOSS Galaxy Power Spectrum

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Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors The Cosmological Analysis of the SDSS/BOSS data from the Effective Field Theory of Large-Scale Structure

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Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors A new analysis of galaxy 2-point functions in the BOSS survey, including full-shape information and post-reconstruction BAO

Reference 34

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Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors The BOSS DR12 Full-Shape Cosmology: $\Lambda$CDM Constraints from the Large-Scale Galaxy Power Spectrum and Bispectrum Monopole

Reference 35

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Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Cosmology with the Galaxy Bispectrum Multipoles: Optimal Estimation and Application to BOSS Data

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Observation 182c724b-6cb6-4312-9164-103bae84968d · outbound

This paper cites Suppression without Thawing: Constraining Structure Formation and Dark Energy with Galaxy Clustering.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Suppression without Thawing: Constraining Structure Formation and Dark Energy with Galaxy Clustering

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Observation b4923a69-91ba-418f-a76f-4265391df4ba · outbound

This paper cites Full-shape analysis with simulation-based priors: constraints on single field inflation from BOSS.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Full-shape analysis with simulation-based priors: constraints on single field inflation from BOSS

Reference 38

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source=pdf_text observed=2026-08-06T21:30:54.513122Z digest=sha256:3852997b1afbc37f0afafffe92891c74ab660aa03b8666bf2d3d6b9b93e3f059

Observation 7e63e80b-c6b4-4250-8c8b-6d7561b66e1d · outbound

This paper cites Full-shape analysis with simulation-based priors: cosmological parameters and the structure growth anomaly.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Full-shape analysis with simulation-based priors: cosmological parameters and the structure growth anomaly

Reference 39

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source=pdf_text observed=2026-08-06T21:30:54.521158Z digest=sha256:2554de567588d6b71c4eb141ae4b8041ea3593511541fc0ea6eb8cbe46425769

Observation 43e5637a-9167-4d1f-970d-37c0e4b33df5 · outbound

This paper cites BOSS Constraints on Massive Particles during Inflation: The Cosmological Collider in Action.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors BOSS Constraints on Massive Particles during Inflation: The Cosmological Collider in Action

Reference 40

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source=pdf_text observed=2026-08-06T21:30:54.527370Z digest=sha256:dd3333420820438a16f591adf4409a5f923d286023989cefb4da979212af459a

Observation 2c5c067b-d1c0-4b97-bc48-49935e6864ca · outbound

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

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors The Millennium and Astrid galaxies in effective field theory: comparison with galaxy-halo connection models at the field level

Reference 41

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source=pdf_text observed=2026-08-06T21:30:54.532095Z digest=sha256:1d451af533241075671ecf306a8bdeb980e4032a0b01997c71d146de1c6496ac

Observation 74198b84-c3a5-435c-be5e-fa10d082c97a · outbound

This paper cites Simulation-Based Priors without Simulations: an Analytic Perspective on EFT Parameters of Galaxies.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Simulation-Based Priors without Simulations: an Analytic Perspective on EFT Parameters of Galaxies

Reference 42

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Observation 94be9440-a4bb-4d81-9d0b-9de6642ff03d · outbound

This paper cites High-redshift Millennium and Astrid galaxies in effective field theory at the field level.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors High-redshift Millennium and Astrid galaxies in effective field theory at the field level

Reference 43

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source=pdf_text observed=2026-08-06T21:30:54.542883Z digest=sha256:81258456964b04068bdf51691151625549cafff2b30a0d42198d7d66cf14e2ee

Observation 896f3ed7-7609-45dc-a18e-d285c75a3e6f · outbound

This paper cites An Analytic Hybrid Halo + Perturbation Theory Model for Small-scale Correlators: Baryons, Halos, and Galaxies.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors An Analytic Hybrid Halo + Perturbation Theory Model for Small-scale Correlators: Baryons, Halos, and Galaxies

Reference 44

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source=pdf_text observed=2026-08-06T21:30:54.548679Z digest=sha256:d3f85ce8cec8b0415c437621a4f8700d1269951d7e460e372581e42ecc280a02

Observation 39d009c2-ccc9-4728-8e81-cf9683eea983 · outbound

This paper cites Modeling HI at the field level.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Modeling HI at the field level

Reference 45

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Observation c551da39-4a9f-4bf7-9ce2-f9ebe6e32f90 · outbound

This paper cites Hybrid SBI or How I Learned to Stop Worrying and Learn the Likelihood.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Hybrid SBI or How I Learned to Stop Worrying and Learn the Likelihood

Reference 46

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source=pdf_text observed=2026-08-06T21:30:54.561851Z digest=sha256:a578f92c432cc0c9f8b5633f86ae88502a50991893cc7bc4706deb1a3e5fe238

Observation 7f33f24b-94f7-46f1-bc80-b5f37e5c6751 · outbound

This paper cites Mapping the galaxy-halo connection to the galaxy bias: implication to the HOD-informed prior.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Mapping the galaxy-halo connection to the galaxy bias: implication to the HOD-informed prior

Reference 47

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source=pdf_text observed=2026-08-06T21:30:54.567911Z digest=sha256:c17e7d45b98065a2896a5bd99bfb7b157476a74efdaafe166ff798bf0910bcce

Observation e75f5742-3386-42f7-b8e1-8b40c8f6d9b7 · outbound

This paper cites HOD-informed prior for EFT-based full-shape analyses of LSS.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors HOD-informed prior for EFT-based full-shape analyses of LSS

Reference 48

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source=pdf_text observed=2026-08-06T21:30:54.574685Z digest=sha256:f7bbb9cfbddb89696c63bbb033e34fb2cfe2ca78b0746d9838c4d9b1270c7c3e

Observation 7f0724c3-f259-4c4c-9b22-79120d8e7404 · outbound

This paper cites Enhancing DESI DR1 Full-Shape analyses using HOD-informed priors.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Enhancing DESI DR1 Full-Shape analyses using HOD-informed priors

Reference 49

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source=pdf_text observed=2026-08-06T21:30:54.580118Z digest=sha256:a33151bc1d812ad20dd592032f1d9d0a8222afb5033f112452e748dd12552a65

Observation 3875fad6-16e4-4553-928a-bfe10ddb3f19 · outbound

This paper cites Modeling Galaxy Surveys with Hybrid SBI.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Modeling Galaxy Surveys with Hybrid SBI

Reference 50

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source=pdf_text observed=2026-08-06T21:30:54.585910Z digest=sha256:840f4e8b1def0deb7519af70bf274708e96a40b60f1933dcf28991f15b98b941

Observation 24c3fe6e-9c34-4c03-8e33-53a5387d221b · outbound

This paper cites Modeling Biased Tracers at the Field Level.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Modeling Biased Tracers at the Field Level

Reference 51

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source=pdf_text observed=2026-08-06T21:30:54.591396Z digest=sha256:97b5e1fe44b3268fdb37982057c9cebe2bb080b62f0a8e53971e9359ce4eacfd

Observation 33b44dfa-d6e4-4610-a6af-c6e8c12f7398 · outbound

This paper cites Modeling Galaxies in Redshift Space at the Field Level.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Modeling Galaxies in Redshift Space at the Field Level

Reference 52

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source=pdf_text observed=2026-08-06T21:30:54.597407Z digest=sha256:d9ecdb0d6cff3abc3579b442c27c1c7f9ff34883a823ff1db25fe64edfa76c62

Observation c9bb7fb0-d01e-44c3-aff0-38401457e8be · outbound

This paper cites Improving cosmological analyses of HI clustering by reducing stochastic noise.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Improving cosmological analyses of HI clustering by reducing stochastic noise

Reference 53

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source=pdf_text observed=2026-08-06T21:30:54.602992Z digest=sha256:966b242e6448d0199d5a21a60b378d6f380fa8298231e8533fd5e77ff0917e2a

Observation 268b9c65-657d-4f74-85d9-e5056529770f · outbound

This paper cites Near optimal bispectrum estimators for large-scale structure.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Near optimal bispectrum estimators for large-scale structure

Reference 54

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source=pdf_text observed=2026-08-06T21:30:54.609055Z digest=sha256:c3de28855ffa9cbb18b7ff0fd8ba4a6ff2c554c50607e01fa646231867425369

Observation 24fbea34-bc86-405f-a819-f387abd02e52 · outbound

This paper cites Beyond LIMD bias: a measurement of the complete set of third-order halo bias parameters.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Beyond LIMD bias: a measurement of the complete set of third-order halo bias parameters

Reference 55

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Observation 60d97db2-4312-4cb7-bd71-9cee67f2db23 · outbound

This paper cites Cubic Halo Bias in Eulerian and Lagrangian Space.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Cubic Halo Bias in Eulerian and Lagrangian Space

Reference 56

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source=pdf_text observed=2026-08-06T21:30:54.621796Z digest=sha256:12d9d83036dfc3b1142dab54d1c2ba47c059bdb579a547a1fd4dbe304e000439

Observation 4dd19cb1-89c5-4a66-a8ec-bc15004b4f04 · outbound

This paper cites A rigorous EFT-based forward model for large-scale structure.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors A rigorous EFT-based forward model for large-scale structure

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Observation 9bbe2620-422f-4e3e-b8c4-3c14ecbb01a3 · outbound

This paper cites Cosmology Inference from Biased Tracers using the EFT-based Likelihood.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Cosmology Inference from Biased Tracers using the EFT-based Likelihood

Reference 58

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Observation f8508abd-69d8-4873-814f-a3efc9a84c0a · outbound

This paper cites The EFT Likelihood for Large-Scale Structure.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors The EFT Likelihood for Large-Scale Structure

Reference 59

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Observation 3fc4b614-45fa-4ed0-b210-5b2a58ed17a4 · outbound

This paper cites Simulations and symmetries.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Simulations and symmetries

Reference 60

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Observation ee59ae21-c76f-4542-a9f4-8b72315fccce · outbound

This paper cites Sigma-Eight at the Percent Level: The EFT Likelihood in Real Space.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Sigma-Eight at the Percent Level: The EFT Likelihood in Real Space

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Observation 97896322-91fb-4021-aabe-08260ee25bb3 · outbound

This paper cites Unbiased Cosmology Inference from Biased Tracers using the EFT Likelihood.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Unbiased Cosmology Inference from Biased Tracers using the EFT Likelihood

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Observation 1b0303b6-899e-4907-b62e-e77ce9613cd5 · outbound

This paper cites Assembly bias in quadratic bias parameters of dark matter halos from forward modeling.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Assembly bias in quadratic bias parameters of dark matter halos from forward modeling

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local_arxiv, observed 2026-08-06T21:30:56.904024Z

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Observation ebb1a074-51bf-4296-99a9-0fe0f4c4d64c · outbound

This paper cites Cosmology inference at the field level from biased tracers in redshift-space.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Cosmology inference at the field level from biased tracers in redshift-space

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Observation c7e36254-7807-48ed-b316-6b70830a3760 · outbound

This paper cites How much information can be extracted from galaxy clustering at the field level?.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors How much information can be extracted from galaxy clustering at the field level?

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Observation dc0cc32c-601e-4caa-ac83-26a2141b1c88 · outbound

This paper cites Constraints on the curvature of the Universe and dynamical dark energy from the Full-shape and BAO data.

Constraining Dynamical Dark Energy from Galaxy Clustering 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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Observation fa74b654-37d8-4dce-9900-b53cf2b137fb · outbound

This paper cites Fewer Mocks and Less Noise: Reducing the Dimensionality of Cosmological Observables with Subspace Projections.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Fewer Mocks and Less Noise: Reducing the Dimensionality of Cosmological Observables with Subspace Projections

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Observation 5c13206e-b906-4b19-8100-7f81b66174d7 · outbound

This paper cites Planck 2018 results. VI. Cosmological parameters.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Planck 2018 results. VI. Cosmological parameters

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Observation 10738bcc-2e83-4a36-8f49-a8a94afecda7 · outbound

This paper cites The Pantheon+ Analysis: The Full Dataset and Light-Curve Release.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors The Pantheon+ Analysis: The Full Dataset and Light-Curve Release

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source=pdf_text observed=2026-08-06T21:30:54.721619Z digest=sha256:8c475fe65ff43198e8ed992f3dafe1fa5593408e36970e657fbfd62b4c250c87

Observation e97eae9b-02e2-47cc-969a-9532b57029a0 · outbound

This paper cites The Pantheon+ Analysis: Cosmological Constraints.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors The Pantheon+ Analysis: Cosmological Constraints

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source=pdf_text observed=2026-08-06T21:30:54.731173Z digest=sha256:2d5da35ce1acb7b29b0e40b7c3c56a043643b7705e7e89cf581dd811762702e3

Observation d7274eac-984c-423f-9ba1-db78ab7cd6c9 · outbound

This paper cites Cosmological Parameters and Neutrino Masses from the Final Planck and Full-Shape BOSS Data.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Cosmological Parameters and Neutrino Masses from the Final Planck and Full-Shape BOSS Data

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Observation 471ea66b-8d38-4fdf-a939-27ea97bfef10 · outbound

This paper cites Optimizing large-scale structure data analysis with the theoretical error likelihood.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Optimizing large-scale structure data analysis with the theoretical error likelihood

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Observation 8a9bd3e4-f1f0-4674-81d4-7586b88a5637 · outbound

This paper cites Precision analysis of the redshift-space galaxy bispectrum.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Precision analysis of the redshift-space galaxy bispectrum

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Observation 4335c02e-2b44-4be0-b32f-2a9e0b4c9093 · outbound

This paper cites Bernardeau, S.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Bernardeau, S

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Observation 4a6035af-076d-4dd6-8c24-1d27a0bf4f8d · outbound

This paper cites Non-linear perturbation theory extension of the Boltzmann code CLASS.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Non-linear perturbation theory extension of the Boltzmann code CLASS

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Observation 60615dd3-48a2-4e3c-9fd8-73ed8c313026 · outbound

This paper cites The two-loop power spectrum in redshift space.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors The two-loop power spectrum in redshift space

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Observation 24ea5e24-4408-4f56-b870-b761f369dc1e · outbound

This paper cites Fingers of God.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Fingers of God

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Observation d4e5bc7f-97e2-45f3-a19e-503163d0b5d6 · outbound

This paper cites Biased Tracers in Redshift Space in the EFT of Large-Scale Structure.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Biased Tracers in Redshift Space in the EFT of Large-Scale Structure

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Observation 07eab98a-09c6-4136-9572-3ba60e69d0b3 · outbound

This paper cites The Baryon Oscillation Spectroscopic Survey of SDSS-III.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors The Baryon Oscillation Spectroscopic Survey of SDSS-III

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Observation 16c4482b-0daa-4204-b43e-394505bff32a · outbound

This paper cites Cosmological constraints without fingers of God.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Cosmological constraints without fingers of God

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Observation aea6ea0a-5e8f-44c1-9603-e1d8b2fb390c · outbound

This paper cites Combining Full-Shape and BAO Analyses of Galaxy Power Spectra: A 1.6% CMB-independent constraint on H0.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Combining Full-Shape and BAO Analyses of Galaxy Power Spectra: A 1.6% CMB-independent constraint on H0

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Observation 7d2b3e01-f1f3-426e-9a74-1aacf2d8e193 · outbound

This paper cites Chudaykin, M.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Chudaykin, M

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Observation feb42ea7-1112-41c4-9b90-4b6c4baf9870 · outbound

This paper cites Cosmology Without Windows: Quadratic Estimators for the Galaxy Power Spectrum.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Cosmology Without Windows: Quadratic Estimators for the Galaxy Power Spectrum

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Observation e9cbe3ab-4b42-4b37-bea1-3bc084944636 · outbound

This paper cites Cosmology Without Window Functions: Cubic Estimators for the Galaxy Bispectrum.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Cosmology Without Window Functions: Cubic Estimators for the Galaxy Bispectrum

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source=pdf_text observed=2026-08-06T21:30:54.838718Z digest=sha256:f9be483b958c4af71278efb8d23ac0412ca0fd07c60ec56aebb62e6c309de4ff

Observation 1955ea4f-5e9b-41b3-bac6-e9d22992b121 · outbound

This paper cites DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars

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Observation 0f0ef580-eb69-4d93-a027-d070f2668a19 · outbound

This paper cites Planck 2018 results. V. CMB power spectra and likelihoods.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Planck 2018 results. V. CMB power spectra and likelihoods

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Observation a361211a-4f7e-4633-b3cd-beb865f8577f · outbound

This paper cites Planck 2018 results. I. Overview and the cosmological legacy of Planck.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Planck 2018 results. I. Overview and the cosmological legacy of Planck

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Observation 06a98ab0-a570-4f88-b815-401737bf7649 · outbound

This paper cites Report of the Dark Energy Task Force.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Report of the Dark Energy Task Force

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Observation dceb52c2-cde5-4240-afc1-e657ca23729c · outbound

This paper cites Uniting the Observed Dynamical Dark Energy Preference with the Discrepancies in $\Omega_m$ and $H_0$ Across Cosmological Probes.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Uniting the Observed Dynamical Dark Energy Preference with the Discrepancies in $\Omega_m$ and $H_0$ Across Cosmological Probes

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Observation af26d374-4a05-41cc-b922-e983d4d7cd4e · outbound

This paper cites Sailer, G.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Sailer, G

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Observation 25d43ac1-3d9a-4c54-b1e1-9f92b853261e · outbound

This paper cites Cosmological Constraints on Light (but Massive) Relics.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Cosmological Constraints on Light (but Massive) Relics

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source=pdf_text observed=2026-08-06T21:30:54.897815Z digest=sha256:93c03ef9b6f7ff5433ba9f99fd213ea0f920d040225e24f720100fd458f6a199

Observation 6776c901-a329-4d7f-ab84-35a47692929f · outbound

This paper cites Ultra-light axions and the $S_8$ tension: joint constraints from the cosmic microwave background and galaxy clustering.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Ultra-light axions and the $S_8$ tension: joint constraints from the cosmic microwave background and galaxy clustering

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Observation 2936a765-fc6b-48a2-a874-9b2b431f128c · outbound

This paper cites $S_8$ Tension in the Context of Dark Matter-Baryon Scattering.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors $S_8$ Tension in the Context of Dark Matter-Baryon Scattering

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Observation ae889dbe-7ed5-4ee6-9d98-eb51b08a0ad5 · outbound

This paper cites Self-Interacting Neutrinos in Light of Large-Scale Structure Data.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Self-Interacting Neutrinos in Light of Large-Scale Structure Data

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Observation aa32c113-7843-4f99-a6af-2dca5d223134 · outbound

This paper cites Bounds on Velocity-Dependent Dark Matter-Baryon Scattering from Large-Scale Structure.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Bounds on Velocity-Dependent Dark Matter-Baryon Scattering from Large-Scale Structure

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Observation 6ee0b670-4b72-4528-9c04-e3036eef26df · outbound

This paper cites Constraining Early Dark Energy with Large-Scale Structure.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Constraining Early Dark Energy with Large-Scale Structure

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Observation c5a782d2-dd8c-4258-ab35-7e6311778b24 · outbound

This paper cites Observational constraints on early dark energy.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Observational constraints on early dark energy

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Observation 324792a2-152c-4057-895a-97f1ad8f17a5 · outbound

This paper cites Learning Theory Informed Priors for Bayesian Inference: A Case Study with Early Dark Energy.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Learning Theory Informed Priors for Bayesian Inference: A Case Study with Early Dark Energy

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Observation d1435927-83d1-465f-84b0-039d03b1b317 · outbound

This paper cites Don't miss the forest for the trees: the Lyman alpha forest power spectrum in effective field theory.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Don't miss the forest for the trees: the Lyman alpha forest power spectrum in effective field theory

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Observation 34a3ceae-d536-4fed-a7b0-6d2733582732 · outbound

This paper cites Fundamental physics with the Lyman-alpha forest: constraints on the growth of structure and neutrino masses from SDSS with effective field theory.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Fundamental physics with the Lyman-alpha forest: constraints on the growth of structure and neutrino masses from SDSS with effective field theory

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Observation 7627e816-bdc8-473c-86ef-70ff4f90f75a · inbound

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Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors

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Observation 92a54218-4e62-4b03-abfc-0497aee76a41 · inbound

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Low-redshift constraints on structure growth from CMB lensing tomography Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors

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Observation 6fe91a3a-8e3a-4a4c-9803-22430536034f · inbound

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Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors

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Observation c73080c8-c333-41d7-94bd-bea54d664cfa · inbound

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Reanalyzing DESI DR1: 4. Percent-Level Cosmological Constraints from Combined Probes and Robust Evidence for the Normal Neutrino Mass Hierarchy Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors

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Observation 33633291-b3c8-4815-8f7b-1db39fa99e55 · inbound

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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

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Observation 3915240b-d39b-4c0c-97f4-5097f27d6bd2 · inbound

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Simulation-Based Priors for HI Bias from Halo Occupation Physics Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors

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Observation 6c098446-e334-4594-8221-dd37cccb6e3e · inbound

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GGI Lectures on Large-Scale Structure Perturbation Theory (Effective Field Theory) Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors

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