Paper Citation Record · LEDGER

Perturbative Likelihoods for Large-Scale Structure of the Universe

As of 8 August 2026, this Paper Citation Record lists 51 of 51 outbound references and 1 inbound Pith citation observation for arXiv:2505.23750.

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

pith.paper-citation-record.v1
2505.23750 v1

Coverage vector

measured 51 of 51 reference resolution

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Source: paper_references, paper_reference_links, observed 2026-08-07T12:48:18.438527Z

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measured 1 of 1 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-03T23:38:16.389133Z

measured 0 of 1 external citation measurements

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

Source: cited_works

Reference resolution

51 of 51 outbound references displayed

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External citation measurements

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Outbound references

Observation b03f882e-4a68-4c06-a836-ded5e82e42e3 · outbound

This paper cites Large-Scale Structure of the Universe and Cosmological Perturbation Theory.

Perturbative Likelihoods for Large-Scale Structure of the Universe Large-Scale Structure of the Universe and Cosmological Perturbation Theory

Reference 1

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Observation 12ecb25b-37d6-4ec0-a507-3b4a3262d056 · outbound

This paper cites Resumming Cosmological Perturbations via the Lagrangian Picture: One-loop Results in Real Space and in Redshift Space.

Perturbative Likelihoods for Large-Scale Structure of the Universe Resumming Cosmological Perturbations via the Lagrangian Picture: One-loop Results in Real Space and in Redshift Space

Reference 2

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Observation 9bd3ba11-5b9f-48ef-acb3-946f2416f4f0 · outbound

This paper cites Matsubara,Recursive solutions of Lagrangian perturbation theory, Phys.

Perturbative Likelihoods for Large-Scale Structure of the Universe Matsubara,Recursive solutions of Lagrangian perturbation theory, Phys

Reference 3

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Observation 3e057197-049b-451f-b6c8-91befc454731 · outbound

This paper cites Renormalized Cosmological Perturbation Theory.

Perturbative Likelihoods for Large-Scale Structure of the Universe Renormalized Cosmological Perturbation Theory

Reference 4

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Observation 3f4bb464-4d53-499d-8a65-fafa7c68d26b · outbound

This paper cites A Consistent Effective Theory of Long-Wavelength Cosmological Perturbations.

Perturbative Likelihoods for Large-Scale Structure of the Universe A Consistent Effective Theory of Long-Wavelength Cosmological Perturbations

Reference 5

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Observation fd98bb50-2fa8-455e-8937-06426b468701 · outbound

This paper cites Large-Scale Galaxy Bias.

Perturbative Likelihoods for Large-Scale Structure of the Universe Large-Scale Galaxy Bias

Reference 6

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Observation 126e7b89-b379-49d0-9086-1856394266f5 · outbound

This paper cites Large-scale dark matter simulations.

Perturbative Likelihoods for Large-Scale Structure of the Universe Large-scale dark matter simulations

Reference 7

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Observation 1f939d50-b06d-4b70-921d-90652d6f9739 · outbound

This paper cites Cosmological Simulations of Galaxy Formation.

Perturbative Likelihoods for Large-Scale Structure of the Universe Cosmological Simulations of Galaxy Formation

Reference 8

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Observation fe45e93d-9ef1-4973-ba8b-7b3392ac2c63 · outbound

This paper cites Revising the Halofit Model for the Nonlinear Matter Power Spectrum.

Perturbative Likelihoods for Large-Scale Structure of the Universe Revising the Halofit Model for the Nonlinear Matter Power Spectrum

Reference 9

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Observation e97a6095-94fc-406e-b5ba-9cb710c05db7 · outbound

This paper cites The cosmological simulation code GADGET-2.

Perturbative Likelihoods for Large-Scale Structure of the Universe The cosmological simulation code GADGET-2

Reference 10

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Observation 905fb0c1-5c02-436b-9b57-176421d55ac9 · outbound

This paper cites Cosmological Hydrodynamics with Adaptive Mesh Refinement: a new high resolution code called RAMSES.

Perturbative Likelihoods for Large-Scale Structure of the Universe Cosmological Hydrodynamics with Adaptive Mesh Refinement: a new high resolution code called RAMSES

Reference 11

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

This paper cites Halo Models of Large Scale Structure.

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

Reference 12

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Observation ab345c63-4c9d-43d3-ab0a-2aa85ea2445a · outbound

This paper cites The Halo Void (Dust) Model of Large Scale Structure.

Perturbative Likelihoods for Large-Scale Structure of the Universe The Halo Void (Dust) Model of Large Scale Structure

Reference 13

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Observation 34303863-9666-4953-9a68-06882e77f8ba · outbound

This paper cites Simulations and symmetries.

Perturbative Likelihoods for Large-Scale Structure of the Universe Simulations and symmetries

Reference 14

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Observation 4caae374-c322-4072-8e34-30b4045e9f5b · outbound

This paper cites Zennaro, R.

Perturbative Likelihoods for Large-Scale Structure of the Universe Zennaro, R

Reference 15

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Observation c41fb412-7bc0-415b-9f47-9b103990065d · outbound

This paper cites Modelling galaxy clustering in redshift space with a Lagrangian bias formalism and $N$-body simulations.

Perturbative Likelihoods for Large-Scale Structure of the Universe Modelling galaxy clustering in redshift space with a Lagrangian bias formalism and $N$-body simulations

Reference 16

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Observation 55e92472-8c72-4624-a270-4f85863823f7 · outbound

This paper cites Blinded challenge for precision cosmology with large-scale structure: results from effective field theory for the redshift-space galaxy power spectrum.

Perturbative Likelihoods for Large-Scale Structure of the Universe Blinded challenge for precision cosmology with large-scale structure: results from effective field theory for the redshift-space galaxy power spectrum

Reference 17

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Observation 29a1415e-8fcb-43c1-898d-5c78e35e7dd1 · outbound

This paper cites A critical look at cosmological perturbation theory techniques.

Perturbative Likelihoods for Large-Scale Structure of the Universe A critical look at cosmological perturbation theory techniques

Reference 18

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Observation c4b6d1be-bd9a-47ba-8f12-bfd0aa608c09 · outbound

This paper cites The Effective Field Theory of Large Scale Structure at Three Loops.

Perturbative Likelihoods for Large-Scale Structure of the Universe The Effective Field Theory of Large Scale Structure at Three Loops

Reference 19

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Observation 2f75c6fc-59ce-4e08-a2f1-783e53201d1d · outbound

This paper cites The Effective Field Theory and Perturbative Analysis for Log-Density Fields.

Perturbative Likelihoods for Large-Scale Structure of the Universe The Effective Field Theory and Perturbative Analysis for Log-Density Fields

Reference 20

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Observation d0e096e6-93d9-4e70-aefb-5ceb6a19ce70 · outbound

This paper cites The One-Loop Matter Bispectrum in the Effective Field Theory of Large Scale Structures.

Perturbative Likelihoods for Large-Scale Structure of the Universe The One-Loop Matter Bispectrum in the Effective Field Theory of Large Scale Structures

Reference 21

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Observation a69a2337-8c0a-4b03-a214-751dd460ec55 · outbound

This paper cites Bertolini, K.

Perturbative Likelihoods for Large-Scale Structure of the Universe Bertolini, K

Reference 22

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Observation cbde0395-1e10-4f1e-8830-e2ed2bb50dbc · outbound

This paper cites an unresolved cited work.

Perturbative Likelihoods for Large-Scale Structure of the Universe Unresolved cited work

Reference 23

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Observation fc5efccd-4ae9-4716-a8c4-32d01668379a · outbound

This paper cites Perturbation theory approach to predict the covariance matrices of the galaxy power spectrum and bispectrum in redshift space.

Perturbative Likelihoods for Large-Scale Structure of the Universe Perturbation theory approach to predict the covariance matrices of the galaxy power spectrum and bispectrum in redshift space

Reference 24

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Observation 7eddf521-29ff-4d9c-8f40-3b2233dc859f · outbound

This paper cites Galaxy Power Spectrum Multipoles Covariance in Perturbation Theory.

Perturbative Likelihoods for Large-Scale Structure of the Universe Galaxy Power Spectrum Multipoles Covariance in Perturbation Theory

Reference 25

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Observation c13c042f-f28e-4738-b40d-49e71c8821c2 · outbound

This paper cites The Effective Field Theory of Large-Scale Structure and Multi-tracer.

Perturbative Likelihoods for Large-Scale Structure of the Universe The Effective Field Theory of Large-Scale Structure and Multi-tracer

Reference 26

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Observation 8ddbf6e1-f196-41a4-9229-0acca3712e97 · outbound

This paper cites The Effective Field Theory of Large-Scale Structure and Multi-tracer II: redshift space and realistic tracers.

Perturbative Likelihoods for Large-Scale Structure of the Universe The Effective Field Theory of Large-Scale Structure and Multi-tracer II: redshift space and realistic tracers

Reference 27

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Observation 79cfaf31-3cd0-411a-bcb7-e99c735ee92d · outbound

This paper cites Priors on Lagrangian bias parameters from galaxy formation modelling.

Perturbative Likelihoods for Large-Scale Structure of the Universe Priors on Lagrangian bias parameters from galaxy formation modelling

Reference 28

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Observation 641aa878-e817-402b-b26d-aefb2cfed151 · outbound

This paper cites Cosmology with the EFTofLSS and BOSS: dark energy constraints and a note on priors.

Perturbative Likelihoods for Large-Scale Structure of the Universe Cosmology with the EFTofLSS and BOSS: dark energy constraints and a note on priors

Reference 29

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Observation 815ba93a-ea07-42f5-93be-e4f73e1eb9cd · outbound

This paper cites BOSS full-shape analysis from the EFTofLSS with exact time dependence.

Perturbative Likelihoods for Large-Scale Structure of the Universe BOSS full-shape analysis from the EFTofLSS with exact time dependence

Reference 30

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Observation b319aff0-1399-4ef5-838e-17aaf32c6872 · outbound

This paper cites The BOSS bispectrum analysis at one loop from the Effective Field Theory of Large-Scale Structure.

Perturbative Likelihoods for Large-Scale Structure of the Universe The BOSS bispectrum analysis at one loop from the Effective Field Theory of Large-Scale Structure

Reference 31

Resolution: unresolved; no resolver link, observed 2026-08-07T12:48:16.464027Z

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Observation 5e2e4042-a7c2-41cd-a108-cf62203b1d6b · outbound

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

Perturbative Likelihoods for Large-Scale Structure of the Universe The EFT Likelihood for Large-Scale Structure

Reference 32

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Observation e8bb79ea-09bb-49dc-adaa-86ac4d9c13b2 · outbound

This paper cites The Likelihood for LSS: Stochasticity of Bias Coefficients at All Orders.

Perturbative Likelihoods for Large-Scale Structure of the Universe The Likelihood for LSS: Stochasticity of Bias Coefficients at All Orders

Reference 33

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Observation 785ce7af-1bfd-440f-8b6e-b6007ab50895 · outbound

This paper cites Schmidt, F.

Perturbative Likelihoods for Large-Scale Structure of the Universe Schmidt, F

Reference 34

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Observation 5981718b-445c-48a7-bbed-bc7a77f8ee21 · outbound

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

Perturbative Likelihoods for Large-Scale Structure of the Universe Sigma-Eight at the Percent Level: The EFT Likelihood in Real Space

Reference 35

Resolution: unresolved; no resolver link, observed 2026-08-07T12:48:16.990191Z

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Observation 1b426146-c302-4fde-a5ba-9b2dd1bb51b5 · outbound

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

Perturbative Likelihoods for Large-Scale Structure of the Universe Cosmology inference at the field level from biased tracers in redshift-space

Reference 36

Resolution: unresolved; no resolver link, observed 2026-08-07T12:48:17.137198Z

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Observation 143ecdd0-e366-4dd3-a70b-16b8109b17d7 · outbound

This paper cites The Cosmological Analysis of the SDSS/BOSS data from the Effective Field Theory of Large-Scale Structure.

Perturbative Likelihoods for Large-Scale Structure of the Universe The Cosmological Analysis of the SDSS/BOSS data from the Effective Field Theory of Large-Scale Structure

Reference 37

Resolution: unresolved; no resolver link, observed 2026-08-07T12:48:17.243030Z

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Observation bdf073f4-1b61-4a4f-9c67-0cd999304610 · outbound

This paper cites Comparing approximate methods for mock catalogues and covariance matrices II: Power spectrum multipoles.

Perturbative Likelihoods for Large-Scale Structure of the Universe Comparing approximate methods for mock catalogues and covariance matrices II: Power spectrum multipoles

Reference 38

Resolution: unresolved; no resolver link, observed 2026-08-07T12:48:17.345197Z

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Observation 1f2c0b75-2510-45e9-ac26-fa34e54b0979 · outbound

This paper cites Dark Energy Survey Year 3 Results: Cosmological Constraints from Galaxy Clustering and Weak Lensing.

Perturbative Likelihoods for Large-Scale Structure of the Universe Dark Energy Survey Year 3 Results: Cosmological Constraints from Galaxy Clustering and Weak Lensing

Reference 39

Resolution: unresolved; no resolver link, observed 2026-08-07T12:48:17.427105Z

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Observation 22edd82a-ca50-4591-becb-a5b9aca11990 · outbound

This paper cites Cosmological Parameters from the BOSS Galaxy Power Spectrum.

Perturbative Likelihoods for Large-Scale Structure of the Universe Cosmological Parameters from the BOSS Galaxy Power Spectrum

Reference 40

Resolution: unresolved; no resolver link, observed 2026-08-07T12:48:17.515184Z

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Observation 325d7caa-13b0-4181-a7ab-789051741f12 · outbound

This paper cites BOSS Correlation Function Analysis from the Effective Field Theory of Large-Scale Structure.

Perturbative Likelihoods for Large-Scale Structure of the Universe BOSS Correlation Function Analysis from the Effective Field Theory of Large-Scale Structure

Reference 41

Resolution: unresolved; no resolver link, observed 2026-08-07T12:48:17.523326Z

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Observation e6505523-0792-4b92-bda3-992458a8aa4f · outbound

This paper cites Constraints on primordial non-Gaussianity from 800,000 photometric quasars.

Perturbative Likelihoods for Large-Scale Structure of the Universe Constraints on primordial non-Gaussianity from 800,000 photometric quasars

Reference 42

Resolution: unresolved; no resolver link, observed 2026-08-07T12:48:17.577017Z

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Observation f5762013-04cd-47d0-87fa-ec8dc7dc5d16 · outbound

This paper cites Planck 2018 results. IX. Constraints on primordial non-Gaussianity.

Perturbative Likelihoods for Large-Scale Structure of the Universe Planck 2018 results. IX. Constraints on primordial non-Gaussianity

Reference 43

Resolution: unresolved; no resolver link, observed 2026-08-07T12:48:17.689904Z

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Observation ebbf91d5-ea14-4125-ac12-b328372a7b9d · outbound

This paper cites Constraining Primordial Non-Gaussianity with Post-reconstructed Galaxy Bispectrum in Redshift Space.

Perturbative Likelihoods for Large-Scale Structure of the Universe Constraining Primordial Non-Gaussianity with Post-reconstructed Galaxy Bispectrum in Redshift Space

Reference 44

Resolution: verified exact; local_arxiv, observed 2026-08-07T12:48:18.958346Z

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Observation dda61db5-a551-4b81-9fbf-5add2f03291a · outbound

This paper cites Schmidt,On the Connection between Field-Level Inference andn-point Correlation Functions, arXiv e-prints (Apr., 2025) arXiv:2504.15351, [2504.15351].

Perturbative Likelihoods for Large-Scale Structure of the Universe Schmidt,On the Connection between Field-Level Inference andn-point Correlation Functions, arXiv e-prints (Apr., 2025) arXiv:2504.15351, [2504.15351]

Reference 45

Resolution: unresolved; no resolver link, observed 2026-08-07T12:48:18.085864Z

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Observation 3e7b3f86-de57-43c7-95a9-585530dceca4 · outbound

This paper cites Renormalized Halo Bias.

Perturbative Likelihoods for Large-Scale Structure of the Universe Renormalized Halo Bias

Reference 46

Resolution: unresolved; no resolver link, observed 2026-08-07T12:48:18.169591Z

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Observation d1f7a325-6b08-46ae-865e-24b55c32fe17 · outbound

This paper cites Excursion Set Halos -- ExSHalos: A New Parameter Free Method for Fast Generation of Halo Catalogues.

Perturbative Likelihoods for Large-Scale Structure of the Universe Excursion Set Halos -- ExSHalos: A New Parameter Free Method for Fast Generation of Halo Catalogues

Reference 47

Resolution: unresolved; no resolver link, observed 2026-08-07T12:48:18.240476Z

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Observation 9d9db600-52b8-4098-8ba3-0d8c81bdbf7d · outbound

This paper cites emcee: The MCMC Hammer.

Perturbative Likelihoods for Large-Scale Structure of the Universe emcee: The MCMC Hammer

Reference 48

Resolution: unresolved; no resolver link, observed 2026-08-07T12:48:18.325962Z

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Observation fd5c2f15-5bbf-4077-afdc-825afae78310 · outbound

This paper cites Rubira and F.

Perturbative Likelihoods for Large-Scale Structure of the Universe Rubira and F

Reference 49

Resolution: unresolved; no resolver link, observed 2026-08-07T12:48:18.438527Z

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Observation 6d07a0e3-6603-4214-af5c-1b3a4efc7dfa · outbound

This paper cites Recursive Solutions of Lagrangian Perturbation Theory.

Perturbative Likelihoods for Large-Scale Structure of the Universe Recursive Solutions of Lagrangian Perturbation Theory

Reference 2015

Resolution: unresolved; no resolver link, observed 2026-08-07T12:48:13.899388Z

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Observation 51c869b5-caf3-45a8-93dc-bc188b40d6a5 · outbound

This paper cites The BACCO simulation project: biased tracers in real space.

Perturbative Likelihoods for Large-Scale Structure of the Universe The BACCO simulation project: biased tracers in real space

Reference 2023

Resolution: unresolved; no resolver link, observed 2026-08-07T12:48:15.087368Z

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Pith citing papers

Observation 4f931b32-cce7-4629-ad60-3f6b88d31dba · inbound

Non-Gaussian Galaxy Stochasticity and the Noise-Field Formulation cites this paper.

Non-Gaussian Galaxy Stochasticity and the Noise-Field Formulation Perturbative Likelihoods for Large-Scale Structure of the Universe

Reference 7

Resolution: unresolved; no resolver link, observed 2026-08-03T23:38:16.389133Z

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