Paper Citation Record · LEDGER

Is $\omega_0 \omega_a$CDM a good model for the clumpy Universe?

As of 22 August 2026, this Paper Citation Record lists 71 of 71 outbound references and 1 inbound Pith citation observation for arXiv:2507.00779.

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

pith.paper-citation-record.v1
2507.00779 v1

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Outbound references

Observation 20d00154-9df6-4ad1-8dc5-e479f2490e08 · outbound

This paper cites write newline.

Is $\omega_0 \omega_a$CDM a good model for the clumpy Universe? write newline

Reference 1

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

Is $\omega_0 \omega_a$CDM a good model for the clumpy Universe? Planck 2018 results. VI. Cosmological parameters

Reference 2

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This paper cites , year 1974.

Is $\omega_0 \omega_a$CDM a good model for the clumpy Universe? , year 1974

Reference 3

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This paper cites Linear matter density perturbations in the $\Lambda_{\rm s}$CDM model: Examining growth dynamics and addressing the $S_8$ tension.

Is $\omega_0 \omega_a$CDM a good model for the clumpy Universe? Linear matter density perturbations in the $\Lambda_{\rm s}$CDM model: Examining growth dynamics and addressing the $S_8$ tension

Reference 4

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This paper cites The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Cosmological Implications from two Decades of Spectroscopic Surveys at the Apache Point observatory.

Is $\omega_0 \omega_a$CDM a good model for the clumpy Universe? The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Cosmological Implications from two Decades of Spectroscopic Surveys at the Apache Point observatory

Reference 5

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Observation a9d5f381-30fc-416b-aa4c-8ca68ff91277 · outbound

This paper cites Inferring $S_8(z)$ and $\gamma(z)$ with cosmic growth rate measurements using machine learning.

Is $\omega_0 \omega_a$CDM a good model for the clumpy Universe? Inferring $S_8(z)$ and $\gamma(z)$ with cosmic growth rate measurements using machine learning

Reference 6

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This paper cites The growth rate of cosmic structures in the local Universe with the ALFALFA survey.

Is $\omega_0 \omega_a$CDM a good model for the clumpy Universe? The growth rate of cosmic structures in the local Universe with the ALFALFA survey

Reference 7

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Observation 924bdb7c-c0d0-4bfc-bc94-c351d36dfbcf · outbound

This paper cites The homogeneity scale and the growth rate of cosmic structures.

Is $\omega_0 \omega_a$CDM a good model for the clumpy Universe? The homogeneity scale and the growth rate of cosmic structures

Reference 8

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Observation 974b9bf4-cb81-4236-8e1c-3c0c8fb8abde · outbound

This paper cites Revisiting the temperature evolution law of the CMB with gaussian processes.

Is $\omega_0 \omega_a$CDM a good model for the clumpy Universe? Revisiting the temperature evolution law of the CMB with gaussian processes

Reference 9

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Observation df1fc3e6-f821-4468-b08a-74414beeea67 · outbound

This paper cites Conjoined constraints on modified gravity from the expansion history and cosmic growth.

Is $\omega_0 \omega_a$CDM a good model for the clumpy Universe? Conjoined constraints on modified gravity from the expansion history and cosmic growth

Reference 10

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Observation 1dfcf052-823e-417c-a7f7-fe47019ea744 · outbound

This paper cites Exploring the $H_0$ tension and the evidence of dark sector interaction from 2D BAO measurements.

Is $\omega_0 \omega_a$CDM a good model for the clumpy Universe? Exploring the $H_0$ tension and the evidence of dark sector interaction from 2D BAO measurements

Reference 11

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This paper cites Observational constraints on Starobinsky $f(R)$ cosmology from cosmic expansion and structure growth data.

Is $\omega_0 \omega_a$CDM a good model for the clumpy Universe? Observational constraints on Starobinsky $f(R)$ cosmology from cosmic expansion and structure growth data

Reference 12

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This paper cites Introduction to Early Universe Cosmology.

Is $\omega_0 \omega_a$CDM a good model for the clumpy Universe? Introduction to Early Universe Cosmology

Reference 13

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Is $\omega_0 \omega_a$CDM a good model for the clumpy Universe? , year 2011

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Observation 2610fa74-a08a-4eea-8b4d-2feec7775bfc · outbound

This paper cites Extended Theories of Gravity.

Is $\omega_0 \omega_a$CDM a good model for the clumpy Universe? Extended Theories of Gravity

Reference 15

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This paper cites Accelerating Universes with Scaling Dark Matter.

Is $\omega_0 \omega_a$CDM a good model for the clumpy Universe? Accelerating Universes with Scaling Dark Matter

Reference 16

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This paper cites Core Cosmology Library: Precision Cosmological Predictions for LSST.

Is $\omega_0 \omega_a$CDM a good model for the clumpy Universe? Core Cosmology Library: Precision Cosmological Predictions for LSST

Reference 17

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This paper cites Modified Gravity and Cosmology.

Is $\omega_0 \omega_a$CDM a good model for the clumpy Universe? Modified Gravity and Cosmology

Reference 18

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Is $\omega_0 \omega_a$CDM a good model for the clumpy Universe? , year 1996

Reference 19

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This paper cites Does DESI 2024 Confirm $\Lambda$CDM?.

Is $\omega_0 \omega_a$CDM a good model for the clumpy Universe? Does DESI 2024 Confirm $\Lambda$CDM?

Reference 20

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This paper cites The Dark Energy Survey: Cosmology Results With ~1500 New High-redshift Type Ia Supernovae Using The Full 5-year Dataset.

Is $\omega_0 \omega_a$CDM a good model for the clumpy Universe? The Dark Energy Survey: Cosmology Results With ~1500 New High-redshift Type Ia Supernovae Using The Full 5-year Dataset

Reference 21

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This paper cites DES Y3 + KiDS-1000: Consistent cosmology combining cosmic shear surveys.

Is $\omega_0 \omega_a$CDM a good model for the clumpy Universe? DES Y3 + KiDS-1000: Consistent cosmology combining cosmic shear surveys

Reference 22

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

Is $\omega_0 \omega_a$CDM a good model for the clumpy Universe? DESI DR2 Results II: Measurements of Baryon Acoustic Oscillations and Cosmological Constraints

Reference 23

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Is $\omega_0 \omega_a$CDM a good model for the clumpy Universe? COLOSSUS: A python toolkit for cosmology, large-scale structure, and dark matter halos

Reference 24

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Is $\omega_0 \omega_a$CDM a good model for the clumpy Universe? Model independent bounds on Type Ia supernova absolute peak magnitude

Reference 25

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Is $\omega_0 \omega_a$CDM a good model for the clumpy Universe? Model-independent reconstruction of the Interacting Dark Energy Kernel: Binned and Gaussian process

Reference 26

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Is $\omega_0 \omega_a$CDM a good model for the clumpy Universe? The Atacama Cosmology Telescope: Cosmology from cross-correlations of unWISE galaxies and ACT DR6 CMB lensing

Reference 27

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Is $\omega_0 \omega_a$CDM a good model for the clumpy Universe? , author Bamba , K

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Is $\omega_0 \omega_a$CDM a good model for the clumpy Universe? , author Avila , F

Reference 29

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Is $\omega_0 \omega_a$CDM a good model for the clumpy Universe? Measuring the matter fluctuations in the Local Universe with the ALFALFA catalog

Reference 30

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Is $\omega_0 \omega_a$CDM a good model for the clumpy Universe? The growth of density perturbations in the last $\sim$10 billion years from tomographic large-scale structure data

Reference 31

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Is $\omega_0 \omega_a$CDM a good model for the clumpy Universe? $H_0$ from cosmic chronometers and Type Ia supernovae, with Gaussian Processes and the novel Weighted Polynomial Regression method

Reference 32

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Is $\omega_0 \omega_a$CDM a good model for the clumpy Universe? Distinguishing between $\Lambda$CDM and modified gravity with future observations of cosmic growth rate

Reference 33

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Is $\omega_0 \omega_a$CDM a good model for the clumpy Universe? How to use GP: Effects of the mean function and hyperparameter selection on Gaussian Process regression

Reference 34

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Is $\omega_0 \omega_a$CDM a good model for the clumpy Universe? Gaussian Process Estimation of Transition Redshift

Reference 35

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Is $\omega_0 \omega_a$CDM a good model for the clumpy Universe? The DESI Experiment, a whitepaper for Snowmass 2013

Reference 36

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Is $\omega_0 \omega_a$CDM a good model for the clumpy Universe? Defying the laws of Gravity I: model-independent reconstruction of the Universe expansion from growth data

Reference 37

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Is $\omega_0 \omega_a$CDM a good model for the clumpy Universe? Exploring the Expansion History of the Universe

Reference 38

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Is $\omega_0 \omega_a$CDM a good model for the clumpy Universe? , author Fu , X

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Is $\omega_0 \omega_a$CDM a good model for the clumpy Universe? Extended Dark Energy analysis using DESI DR2 BAO measurements

Reference 40

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Is $\omega_0 \omega_a$CDM a good model for the clumpy Universe? Tomographic analyses of the CMB lensing and galaxy clustering to probe the linear structure growth

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Is $\omega_0 \omega_a$CDM a good model for the clumpy Universe? Cosmology from weak lensing peaks and minima with Subaru Hyper Suprime-Cam survey first-year data

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Is $\omega_0 \omega_a$CDM a good model for the clumpy Universe? First Identification of a CMB Lensing Signal Produced by $1.5$ Million Galaxies at $z\sim$4: Constraints on Matter Density Fluctuations at High Redshift

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Is $\omega_0 \omega_a$CDM a good model for the clumpy Universe? , author Li, E.K

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Is $\omega_0 \omega_a$CDM a good model for the clumpy Universe? , author Feldman , H.A

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Is $\omega_0 \omega_a$CDM a good model for the clumpy Universe? , author Mukherjee , A

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Is $\omega_0 \omega_a$CDM a good model for the clumpy Universe? To CPL, or not to CPL? What we have not learned about the dark energy equation of state

Reference 47

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Is $\omega_0 \omega_a$CDM a good model for the clumpy Universe? Tension and constraints on modified gravity parametrizations of $G_{\textrm{eff}}(z)$ from growth rate and Planck data

Reference 48

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Is $\omega_0 \omega_a$CDM a good model for the clumpy Universe? Cosmology from HSC Y1 Weak Lensing with Combined Higher-Order Statistics and Simulation-based Inference

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Is $\omega_0 \omega_a$CDM a good model for the clumpy Universe? Elucidating cosmological model dependence with $H_0$

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Is $\omega_0 \omega_a$CDM a good model for the clumpy Universe? Reconstructing the growth index $\gamma$ with Gaussian Processes

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Is $\omega_0 \omega_a$CDM a good model for the clumpy Universe? , author Ribeiro , B

Reference 52

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Observation f65a2f77-eba2-41d6-9bbb-af0388ec41d6 · outbound

This paper cites , author Paul , S.

Is $\omega_0 \omega_a$CDM a good model for the clumpy Universe? , author Paul , S

Reference 53

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Unavailable: canonical work link unavailable.

Observation c90f2d5b-50f7-4dd3-9d7d-c7152aaec4c6 · outbound

This paper cites Using non-DESI data to confirm and strengthen the DESI 2024 spatially-flat $w_0w_a$CDM cosmological parameterization result.

Is $\omega_0 \omega_a$CDM a good model for the clumpy Universe? Using non-DESI data to confirm and strengthen the DESI 2024 spatially-flat $w_0w_a$CDM cosmological parameterization result

Reference 54

Resolution: unresolved; no resolver link, observed 2026-08-06T21:15:09.949198Z

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Observation 5c10109e-69df-4618-a985-627f6592e237 · outbound

This paper cites Optimising growth of structure constraints on modified gravity.

Is $\omega_0 \omega_a$CDM a good model for the clumpy Universe? Optimising growth of structure constraints on modified gravity

Reference 55

Resolution: unresolved; no resolver link, observed 2026-08-06T21:15:09.991770Z

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Observation 71d32476-4a3c-4e97-8477-57efb7e75e34 · outbound

This paper cites , author Skara , F.

Is $\omega_0 \omega_a$CDM a good model for the clumpy Universe? , author Skara , F

Reference 56

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Observation 63bfcf07-b45b-408a-812e-c274b8ddfd63 · outbound

This paper cites Growth history and quasar bias evolution at z < 3 from Quaia.

Is $\omega_0 \omega_a$CDM a good model for the clumpy Universe? Growth history and quasar bias evolution at z < 3 from Quaia

Reference 57

Resolution: unresolved; no resolver link, observed 2026-08-06T21:15:10.060852Z

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Observation f89894ac-ea3b-4d2e-b048-1ee6f3b54b73 · outbound

This paper cites , author Williams, C.K.I.

Is $\omega_0 \omega_a$CDM a good model for the clumpy Universe? , author Williams, C.K.I

Reference 58

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Observation 7cdb8510-53bb-4135-9957-0acd17b2d4c4 · outbound

This paper cites Cosmological constraints on $R^2$-corrected Appleby-Battye model.

Is $\omega_0 \omega_a$CDM a good model for the clumpy Universe? Cosmological constraints on $R^2$-corrected Appleby-Battye model

Reference 59

Resolution: unresolved; no resolver link, observed 2026-08-06T21:15:10.091687Z

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Observation f8cd5f60-ed28-480a-9f3a-9a7aee401990 · outbound

This paper cites Exploring new physics in the late Universe's expansion through non-parametric inference.

Is $\omega_0 \omega_a$CDM a good model for the clumpy Universe? Exploring new physics in the late Universe's expansion through non-parametric inference

Reference 60

Resolution: unresolved; no resolver link, observed 2026-08-06T21:15:10.137016Z

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Observation 8eabc9c1-ee68-469c-9f73-ed795e3d6dbf · outbound

This paper cites , author Alfedeel , A.H.A.

Is $\omega_0 \omega_a$CDM a good model for the clumpy Universe? , author Alfedeel , A.H.A

Reference 61

Resolution: unresolved; no resolver link, observed 2026-08-06T21:15:10.171724Z

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Observation 4aa7cdfd-549e-4ca2-af9b-d2350fc4f5ba · outbound

This paper cites Optimising Gaussian processes for reconstructing dark energy dynamics from supernovae.

Is $\omega_0 \omega_a$CDM a good model for the clumpy Universe? Optimising Gaussian processes for reconstructing dark energy dynamics from supernovae

Reference 62

Resolution: unresolved; no resolver link, observed 2026-08-06T21:15:10.226162Z

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Observation 57d79625-40a0-462d-a688-2aa401ffd2ce · outbound

This paper cites Reconstruction of dark energy and expansion dynamics using Gaussian processes.

Is $\omega_0 \omega_a$CDM a good model for the clumpy Universe? Reconstruction of dark energy and expansion dynamics using Gaussian processes

Reference 63

Resolution: unresolved; no resolver link, observed 2026-08-06T21:15:10.247918Z

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Observation e989e9ea-69b3-47ab-927e-be3565b17c39 · outbound

This paper cites Efficient Compression of Redshift-Space Distortion Data for Late-Time Modified Gravity Models.

Is $\omega_0 \omega_a$CDM a good model for the clumpy Universe? Efficient Compression of Redshift-Space Distortion Data for Late-Time Modified Gravity Models

Reference 64

Resolution: unresolved; no resolver link, observed 2026-08-06T21:15:10.284319Z

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Observation 274e21be-e318-442d-b263-c2b5465a1ce9 · outbound

This paper cites , year 2010.

Is $\omega_0 \omega_a$CDM a good model for the clumpy Universe? , year 2010

Reference 65

Resolution: unresolved; no resolver link, observed 2026-08-06T21:15:10.332627Z

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Unavailable: canonical work link unavailable.

Observation 314e5b9f-84b9-4ee9-81b2-f14253ef7493 · outbound

This paper cites , author Vanzan , E.

Is $\omega_0 \omega_a$CDM a good model for the clumpy Universe? , author Vanzan , E

Reference 66

Resolution: verified exact; doi, observed 2026-08-06T21:15:10.646593Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

Observation 60d0cf7e-983f-4528-89a4-4c01c9c1d63f · outbound

This paper cites Dark Matter and Dark Energy Interactions: Theoretical Challenges, Cosmological Implications and Observational Signatures.

Is $\omega_0 \omega_a$CDM a good model for the clumpy Universe? Dark Matter and Dark Energy Interactions: Theoretical Challenges, Cosmological Implications and Observational Signatures

Reference 67

Resolution: unresolved; no resolver link, observed 2026-08-06T21:15:10.379019Z

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Unavailable: canonical work link unavailable.

Observation 6bf1b1e9-4cd3-41cb-b5dc-ddb22afaf74b · outbound

This paper cites Reconstructing the interaction between dark energy and dark matter using Gaussian Processes.

Is $\omega_0 \omega_a$CDM a good model for the clumpy Universe? Reconstructing the interaction between dark energy and dark matter using Gaussian Processes

Reference 68

Resolution: unresolved; no resolver link, observed 2026-08-06T21:15:10.399522Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation ea9c48c5-572b-4ed6-9f94-5414e288a218 · outbound

This paper cites Cosmology with the Large Synoptic Survey Telescope: an Overview.

Is $\omega_0 \omega_a$CDM a good model for the clumpy Universe? Cosmology with the Large Synoptic Survey Telescope: an Overview

Reference 69

Resolution: unresolved; no resolver link, observed 2026-08-06T21:15:10.434765Z

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Unavailable: canonical work link unavailable.

Observation 2332b109-90d2-4f44-b605-edc120682d96 · outbound

This paper cites Kernel Selection for Gaussian Process in Cosmology: with Approximate Bayesian Computation Rejection and Nested Sampling.

Is $\omega_0 \omega_a$CDM a good model for the clumpy Universe? Kernel Selection for Gaussian Process in Cosmology: with Approximate Bayesian Computation Rejection and Nested Sampling

Reference 70

Resolution: unresolved; no resolver link, observed 2026-08-06T21:15:10.471496Z

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Observation eeaa6796-dfb0-402e-a357-828b35af7118 · outbound

This paper cites 2015, , 579, A101.

Is $\omega_0 \omega_a$CDM a good model for the clumpy Universe? 2015, , 579, A101

Reference 71

Resolution: unresolved; no resolver link, observed 2026-08-06T21:15:10.504924Z

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Pith citing papers

Observation 2d3cb364-834c-4e49-9870-063e76252996 · inbound

Probing the Cosmic Distance Duality Relation via Non-Parametric Reconstruction for High Redshifts cites this paper.

Probing the Cosmic Distance Duality Relation via Non-Parametric Reconstruction for High Redshifts Is $\omega_0 \omega_a$CDM a good model for the clumpy Universe?

Reference 86

Resolution: verified exact; local_arxiv, observed 2026-08-15T16:14:11.843992Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.