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A Quantitative Framework for Testing the Hubble Tension in a Bianchi Type I Cosmological Background

As of 17 August 2026, this Paper Citation Record lists 100 of 104 outbound references and 0 inbound Pith citation observations for arXiv:2607.29197.

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pith.paper-citation-record.v1
2607.29197 v1

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Outbound references

Observation b69644a0-e265-4e5c-80d8-c7d7139ee9d7 · outbound

This paper cites A class of homogeneous cosmological models,.

A Quantitative Framework for Testing the Hubble Tension in a Bianchi Type I Cosmological Background A class of homogeneous cosmological models,

Reference 1

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Observation 9b3e843f-bab7-4f21-a095-f6ad1ead8377 · outbound

This paper cites Cosmological models,.

A Quantitative Framework for Testing the Hubble Tension in a Bianchi Type I Cosmological Background Cosmological models,

Reference 2

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Observation dce004fd-fa73-4b5c-b0fa-46550e25785d · outbound

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

A Quantitative Framework for Testing the Hubble Tension in a Bianchi Type I Cosmological Background Planck 2018 results. VI. Cosmological parameters

Reference 3

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Observation f4f7f0c3-6dc0-479b-875a-e9fe68d686d6 · outbound

This paper cites A Comprehensive Measurement of the Local Value of the Hubble Constant with 1 km/s/Mpc Uncertainty from the Hubble Space Telescope and the SH0ES Team.

A Quantitative Framework for Testing the Hubble Tension in a Bianchi Type I Cosmological Background A Comprehensive Measurement of the Local Value of the Hubble Constant with 1 km/s/Mpc Uncertainty from the Hubble Space Telescope and the SH0ES Team

Reference 4

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Observation faa6d886-6bdd-43ae-b121-3c54896c804c · outbound

This paper cites JWST Observations Reject Unrecognized Crowding of Cepheid Photometry as an Explanation for the Hubble Tension at 8 sigma Confidence.

A Quantitative Framework for Testing the Hubble Tension in a Bianchi Type I Cosmological Background JWST Observations Reject Unrecognized Crowding of Cepheid Photometry as an Explanation for the Hubble Tension at 8 sigma Confidence

Reference 5

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Observation d1dbb047-f758-491f-ad30-11fa389d7052 · outbound

This paper cites Status Report on the Chicago-Carnegie Hubble Program (CCHP): Measurement of the Hubble Constant Using the Hubble and James Webb Space Telescopes.

A Quantitative Framework for Testing the Hubble Tension in a Bianchi Type I Cosmological Background Status Report on the Chicago-Carnegie Hubble Program (CCHP): Measurement of the Hubble Constant Using the Hubble and James Webb Space Telescopes

Reference 6

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Observation c9d2d4c8-7f6e-4e72-a135-ed45be43be62 · outbound

This paper cites The Chicago-Carnegie Hubble Program: The JWST J-region Asymptotic Giant Branch (JAGB) Extragalactic Distance Scale.

A Quantitative Framework for Testing the Hubble Tension in a Bianchi Type I Cosmological Background The Chicago-Carnegie Hubble Program: The JWST J-region Asymptotic Giant Branch (JAGB) Extragalactic Distance Scale

Reference 7

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Observation 285ef10f-3295-4dab-b566-cc70a9e40385 · outbound

This paper cites The Chicago Carnegie Hubble Program: Improving the Calibration of SNe Ia with JWST Measurements of the Tip of the Red Giant Branch.

A Quantitative Framework for Testing the Hubble Tension in a Bianchi Type I Cosmological Background The Chicago Carnegie Hubble Program: Improving the Calibration of SNe Ia with JWST Measurements of the Tip of the Red Giant Branch

Reference 8

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Observation ecb9a3fa-4ae1-4cae-ba58-bd4aadecec39 · outbound

This paper cites The Perfect Host: JWST Cepheid Observations in a Background-Free SN Ia Host Confirm No Bias in Hubble-Constant Measurements.

A Quantitative Framework for Testing the Hubble Tension in a Bianchi Type I Cosmological Background The Perfect Host: JWST Cepheid Observations in a Background-Free SN Ia Host Confirm No Bias in Hubble-Constant Measurements

Reference 9

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This paper cites The Complete Sample of Available SNe Ia Luminosity Calibrations from the TRGB Observed with either HST or JWST.

A Quantitative Framework for Testing the Hubble Tension in a Bianchi Type I Cosmological Background The Complete Sample of Available SNe Ia Luminosity Calibrations from the TRGB Observed with either HST or JWST

Reference 10

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Observation 0a5b01cc-8463-427c-8ec7-f3cab4139396 · outbound

This paper cites The Hubble Tension in our own Backyard: DESI and the Nearness of the Coma Cluster.

A Quantitative Framework for Testing the Hubble Tension in a Bianchi Type I Cosmological Background The Hubble Tension in our own Backyard: DESI and the Nearness of the Coma Cluster

Reference 11

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Observation d5f8ad30-f220-40f4-9af7-fe265b9dfd17 · outbound

This paper cites Tensions between the Early and the Late Universe.

A Quantitative Framework for Testing the Hubble Tension in a Bianchi Type I Cosmological Background Tensions between the Early and the Late Universe

Reference 12

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This paper cites The Hubble Hunter's Guide.

A Quantitative Framework for Testing the Hubble Tension in a Bianchi Type I Cosmological Background The Hubble Hunter's Guide

Reference 13

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This paper cites A buyer's guide to the Hubble Constant.

A Quantitative Framework for Testing the Hubble Tension in a Bianchi Type I Cosmological Background A buyer's guide to the Hubble Constant

Reference 14

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Observation 25e2d737-7cfd-4000-b63e-5b7a51aa4276 · outbound

This paper cites In the Realm of the Hubble tension $-$ a Review of Solutions.

A Quantitative Framework for Testing the Hubble Tension in a Bianchi Type I Cosmological Background In the Realm of the Hubble tension $-$ a Review of Solutions

Reference 15

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This paper cites Cosmology Intertwined: A Review of the Particle Physics, Astrophysics, and Cosmology Associated with the Cosmological Tensions and Anomalies.

A Quantitative Framework for Testing the Hubble Tension in a Bianchi Type I Cosmological Background Cosmology Intertwined: A Review of the Particle Physics, Astrophysics, and Cosmology Associated with the Cosmological Tensions and Anomalies

Reference 16

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This paper cites Challenges to the Lambda CDM Cosmology.

A Quantitative Framework for Testing the Hubble Tension in a Bianchi Type I Cosmological Background Challenges to the Lambda CDM Cosmology

Reference 17

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This paper cites Hubble Tension: The Evidence of New Physics.

A Quantitative Framework for Testing the Hubble Tension in a Bianchi Type I Cosmological Background Hubble Tension: The Evidence of New Physics

Reference 18

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This paper cites Dissecting the Hubble tension: insights from a diverse set of sound-horizon-freeH0 measurements,.

A Quantitative Framework for Testing the Hubble Tension in a Bianchi Type I Cosmological Background Dissecting the Hubble tension: insights from a diverse set of sound-horizon-freeH0 measurements,

Reference 19

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This paper cites Difficulties with late-time solutions for the Hubble tension,.

A Quantitative Framework for Testing the Hubble Tension in a Bianchi Type I Cosmological Background Difficulties with late-time solutions for the Hubble tension,

Reference 20

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This paper cites Impact of ACT DR6 and DESI DR2 for Early Dark Energy and the Hubble tension.

A Quantitative Framework for Testing the Hubble Tension in a Bianchi Type I Cosmological Background Impact of ACT DR6 and DESI DR2 for Early Dark Energy and the Hubble tension

Reference 21

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This paper cites What it takes to solve the Hubble tension through Modifications of Cosmological Recombination II: in light of ACT DR6 and DESI DR2.

A Quantitative Framework for Testing the Hubble Tension in a Bianchi Type I Cosmological Background What it takes to solve the Hubble tension through Modifications of Cosmological Recombination II: in light of ACT DR6 and DESI DR2

Reference 22

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A Quantitative Framework for Testing the Hubble Tension in a Bianchi Type I Cosmological Background The isotropy of the Universe,

Reference 23

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This paper cites Asymptotic behavior of homogeneous cosmological models in the presence of a positive cosmological constant,.

A Quantitative Framework for Testing the Hubble Tension in a Bianchi Type I Cosmological Background Asymptotic behavior of homogeneous cosmological models in the presence of a positive cosmological constant,

Reference 24

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A Quantitative Framework for Testing the Hubble Tension in a Bianchi Type I Cosmological Background Constraints on a Bianchi type I spacetime extension of the standard $\Lambda$CDM model

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A Quantitative Framework for Testing the Hubble Tension in a Bianchi Type I Cosmological Background Hubble Diagrams in Statistically Homogeneous, Anisotropic Universes

Reference 26

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A Quantitative Framework for Testing the Hubble Tension in a Bianchi Type I Cosmological Background Hubble tension in an anisotropic Universe,

Reference 27

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A Quantitative Framework for Testing the Hubble Tension in a Bianchi Type I Cosmological Background Anisotropic Generalization of the {\Lambda}CDM Universe Model with Application to the Hubble Tension

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A Quantitative Framework for Testing the Hubble Tension in a Bianchi Type I Cosmological Background Anisotropic universes in light of background cosmological observations,

Reference 29

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A Quantitative Framework for Testing the Hubble Tension in a Bianchi Type I Cosmological Background Isotropy of Hubble expansion in the early and late Universe,

Reference 30

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A Quantitative Framework for Testing the Hubble Tension in a Bianchi Type I Cosmological Background Ellipsoidal Universe Can Solve The CMB Quadrupole Problem

Reference 31

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A Quantitative Framework for Testing the Hubble Tension in a Bianchi Type I Cosmological Background Cosmic Microwave Background Quadrupole and Ellipsoidal Universe

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A Quantitative Framework for Testing the Hubble Tension in a Bianchi Type I Cosmological Background Ellipsoidal Universe induces large scale CMB polarization,

Reference 33

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A Quantitative Framework for Testing the Hubble Tension in a Bianchi Type I Cosmological Background On the Large Scale CMB Polarization

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A Quantitative Framework for Testing the Hubble Tension in a Bianchi Type I Cosmological Background The Ellipsoidal Universe in the Planck Satellite Era

Reference 35

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A Quantitative Framework for Testing the Hubble Tension in a Bianchi Type I Cosmological Background The Ellipsoidal Universe and the Hubble tension

Reference 36

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Observation 069011c4-2cb0-46ce-8f70-1973a81f7a3c · outbound

This paper cites The Atacama Cosmology Telescope: DR6 Power Spectra, Likelihoods and $\Lambda$CDM Parameters.

A Quantitative Framework for Testing the Hubble Tension in a Bianchi Type I Cosmological Background The Atacama Cosmology Telescope: DR6 Power Spectra, Likelihoods and $\Lambda$CDM Parameters

Reference 37

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Observation 436f94d9-1bed-4de0-9b1d-4e6dbb61b825 · outbound

This paper cites The Atacama Cosmology Telescope: DR6 Constraints on Extended Cosmological Models.

A Quantitative Framework for Testing the Hubble Tension in a Bianchi Type I Cosmological Background The Atacama Cosmology Telescope: DR6 Constraints on Extended Cosmological Models

Reference 38

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Observation 1d1dfd4d-9f65-451e-b771-76d70879cc29 · outbound

This paper cites The Atacama Cosmology Telescope: Multi-probe cosmology with unWISE galaxies and ACT DR6 CMB lensing.

A Quantitative Framework for Testing the Hubble Tension in a Bianchi Type I Cosmological Background The Atacama Cosmology Telescope: Multi-probe cosmology with unWISE galaxies and ACT DR6 CMB lensing

Reference 39

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Observation 523f689e-c43c-4f2a-b4c7-b5c7af0119ee · outbound

This paper cites Towards constraining cosmological parameters with SPT-3G observations of 25% of the sky.

A Quantitative Framework for Testing the Hubble Tension in a Bianchi Type I Cosmological Background Towards constraining cosmological parameters with SPT-3G observations of 25% of the sky

Reference 40

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Observation 6ed17b54-3c42-4691-a9a1-aca13304e735 · outbound

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A Quantitative Framework for Testing the Hubble Tension in a Bianchi Type I Cosmological Background The Dark Energy Survey: Cosmology Results With ~1500 New High-redshift Type Ia Supernovae Using The Full 5-year Dataset

Reference 41

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Observation 9bf3d1e4-5242-4d17-b1dc-d15a69ca2896 · outbound

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A Quantitative Framework for Testing the Hubble Tension in a Bianchi Type I Cosmological Background The Dark Energy Survey Supernova Program: A Reanalysis Of Cosmology Results And Evidence For Evolving Dark Energy With An Updated Type Ia Supernova Calibration

Reference 42

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Observation ebfeb88e-a1b8-4d60-a7f3-cf3b1e1dd077 · outbound

This paper cites Union Through UNITY: Cosmology with 2,000 SNe Using a Unified Bayesian Framework.

A Quantitative Framework for Testing the Hubble Tension in a Bianchi Type I Cosmological Background Union Through UNITY: Cosmology with 2,000 SNe Using a Unified Bayesian Framework

Reference 43

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Observation 63a8d009-c0d4-4b50-a7ae-a5fb3fe72bff · outbound

This paper cites Detection of the baryon acoustic peak in the large-scale correlation function of SDSS luminous red galaxies,.

A Quantitative Framework for Testing the Hubble Tension in a Bianchi Type I Cosmological Background Detection of the baryon acoustic peak in the large-scale correlation function of SDSS luminous red galaxies,

Reference 44

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Observation d7025548-8ba3-4392-8cc5-b772b223f4fb · outbound

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A Quantitative Framework for Testing the Hubble Tension in a Bianchi Type I Cosmological Background The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Cosmological Implications from two Decades of Spectroscopic Surveys at the Apache Point observatory

Reference 45

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Observation 2760d518-2a53-42ad-a5b3-96a3661519b1 · outbound

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

A Quantitative Framework for Testing the Hubble Tension in a Bianchi Type I Cosmological Background DESI 2024 VI: Cosmological Constraints from the Measurements of Baryon Acoustic Oscillations

Reference 46

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Observation 7e0267e9-2b35-4087-8279-e772ae27bce9 · outbound

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A Quantitative Framework for Testing the Hubble Tension in a Bianchi Type I Cosmological Background DESI DR2 Results II: Measurements of Baryon Acoustic Oscillations and Cosmological Constraints

Reference 47

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Observation 8889698c-feba-4750-be55-92b876cc8bf7 · outbound

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A Quantitative Framework for Testing the Hubble Tension in a Bianchi Type I Cosmological Background DESI DR2 Results I: Baryon Acoustic Oscillations from the Lyman Alpha Forest

Reference 48

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Observation 9be453d2-657c-42bc-9437-6d8f99b1c48f · outbound

This paper cites The Hubble tension resolved by the DESI baryon acoustic oscillations measurements,.

A Quantitative Framework for Testing the Hubble Tension in a Bianchi Type I Cosmological Background The Hubble tension resolved by the DESI baryon acoustic oscillations measurements,

Reference 49

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Observation 2aca292a-4007-49c9-890e-96fd9ebe22de · outbound

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A Quantitative Framework for Testing the Hubble Tension in a Bianchi Type I Cosmological Background Probing potential redshift-dependent systematics in the Hubble tension: model-independent H0 constraints from DESI R2,

Reference 50

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Observation 1b226246-bb29-4708-a64f-1b270e219b4f · outbound

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A Quantitative Framework for Testing the Hubble Tension in a Bianchi Type I Cosmological Background Updated cosmological constraints from 2D BAO measurements: a new compilation and comparison with DESI DR2,

Reference 51

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Observation 3b006061-cb02-453a-a408-60c2c0db035d · outbound

This paper cites Cosmological constraints from a joint DESI DR1 Full-Shape and DR2 BAO,.

A Quantitative Framework for Testing the Hubble Tension in a Bianchi Type I Cosmological Background Cosmological constraints from a joint DESI DR1 Full-Shape and DR2 BAO,

Reference 52

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Observation d526a852-970d-45c2-9d72-144a9ed25b93 · outbound

This paper cites An anisotropic model for the Universe,.

A Quantitative Framework for Testing the Hubble Tension in a Bianchi Type I Cosmological Background An anisotropic model for the Universe,

Reference 53

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Observation 09455a5b-9cb9-4d12-9476-e9fac000d055 · outbound

This paper cites Constraints on an Anisotropic Universe.

A Quantitative Framework for Testing the Hubble Tension in a Bianchi Type I Cosmological Background Constraints on an Anisotropic Universe

Reference 54

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Observation d1ec9f84-03cd-4666-bd26-a05e8512edb5 · outbound

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A Quantitative Framework for Testing the Hubble Tension in a Bianchi Type I Cosmological Background Constraining Axially Symmetric Bianchi Type I Model with Self-Consistent Recombination History and Observables

Reference 55

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Observation 2828fe56-61bf-4a6d-ad5e-e3943fe82603 · outbound

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A Quantitative Framework for Testing the Hubble Tension in a Bianchi Type I Cosmological Background Bianchi Type I Model Cannot Explain the Observed CMB Angular Acoustic Scale Directional Variation

Reference 56

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Observation ef34a6b3-5c61-425e-a330-d770f262d759 · outbound

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A Quantitative Framework for Testing the Hubble Tension in a Bianchi Type I Cosmological Background Anisotropic Dark Energy: Dynamics of Background and Perturbations

Reference 57

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Observation 398e3580-f770-480d-a986-efbb24bf00c0 · outbound

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A Quantitative Framework for Testing the Hubble Tension in a Bianchi Type I Cosmological Background Anisotropic Cosmological Constant and the CMB Quadrupole Anomaly

Reference 58

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Observation 6664020e-f7e6-43b5-af97-8515f46c3e36 · outbound

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A Quantitative Framework for Testing the Hubble Tension in a Bianchi Type I Cosmological Background Probing Dark Energy Anisotropy

Reference 59

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Observation bcf7b97d-614d-4648-b33f-25978f01be18 · outbound

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A Quantitative Framework for Testing the Hubble Tension in a Bianchi Type I Cosmological Background Anisotropic universe with anisotropic dark energy

Reference 60

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Observation 2e7c549e-5bb1-4234-ba45-9e552b7e9c3a · outbound

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A Quantitative Framework for Testing the Hubble Tension in a Bianchi Type I Cosmological Background Ellipsoidal Universe and Cosmic Shear

Reference 61

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Observation 7483f5ab-d0c0-4f01-86a8-a22c38ce82ac · outbound

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A Quantitative Framework for Testing the Hubble Tension in a Bianchi Type I Cosmological Background Testing spatial curvature and anisotropic expansion on top of the $\Lambda$CDM model

Reference 62

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Observation 17adb886-c1fa-4179-9885-c8d1a54281d7 · outbound

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A Quantitative Framework for Testing the Hubble Tension in a Bianchi Type I Cosmological Background On the definition of distance in general relativity,

Reference 63

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Observation b0bf9e4e-b891-4836-9cd4-2b7bccab20a3 · outbound

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A Quantitative Framework for Testing the Hubble Tension in a Bianchi Type I Cosmological Background Republication of: Relativistic cosmology,

Reference 64

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Observation 84fbbc4f-f716-4170-a49d-841220bf3eaa · outbound

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A Quantitative Framework for Testing the Hubble Tension in a Bianchi Type I Cosmological Background Observations in cosmology,

Reference 65

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Observation a158d3d6-2092-48ae-9e2f-04d9c9f95ed0 · outbound

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A Quantitative Framework for Testing the Hubble Tension in a Bianchi Type I Cosmological Background Gravitational waves in general relativity. VI. The outgoing radiation condi- tion,

Reference 66

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Observation 5207efd2-e841-4c2b-9043-5cf7218d05e9 · outbound

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A Quantitative Framework for Testing the Hubble Tension in a Bianchi Type I Cosmological Background Geodesic-light-cone coordinates and the Bianchi I spacetime

Reference 67

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Observation 8b9b9887-8d59-4fee-a93c-28d775919247 · outbound

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A Quantitative Framework for Testing the Hubble Tension in a Bianchi Type I Cosmological Background Light-cone averaging in cosmology: formalism and applications

Reference 68

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Observation ee151661-d537-43e4-9856-f394c1e8dfc2 · outbound

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A Quantitative Framework for Testing the Hubble Tension in a Bianchi Type I Cosmological Background An exact Jacobi map in the geodesic light-cone gauge

Reference 69

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Observation 492e20d1-c006-4ff1-b628-774587d29c70 · outbound

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A Quantitative Framework for Testing the Hubble Tension in a Bianchi Type I Cosmological Background A new approach to the propagation of light-like signals in perturbed cosmological backgrounds

Reference 70

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Observation 0131b881-0967-4377-9e47-fd548015765c · outbound

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A Quantitative Framework for Testing the Hubble Tension in a Bianchi Type I Cosmological Background Cosmic Parallax: possibility of detecting anisotropic expansion of the universe by very accurate astrometry measurements

Reference 71

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Observation 72c24b24-364a-455f-81d2-d97dd48a9101 · outbound

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A Quantitative Framework for Testing the Hubble Tension in a Bianchi Type I Cosmological Background Can Cosmic Parallax Distinguish Between Anisotropic Cosmologies?

Reference 72

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Observation c2c65172-2a66-44c3-b285-6dcf40574b9c · outbound

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A Quantitative Framework for Testing the Hubble Tension in a Bianchi Type I Cosmological Background Cosmic Parallax in Ellipsoidal Universe

Reference 73

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Observation 2d8d0e46-c8f1-4aa5-8aaf-d3f2d0be4678 · outbound

This paper cites Anisotropy of Cosmic Acceleration.

A Quantitative Framework for Testing the Hubble Tension in a Bianchi Type I Cosmological Background Anisotropy of Cosmic Acceleration

Reference 74

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Observation 130a1c8f-c393-4aa9-a4af-a5c80ce77051 · outbound

This paper cites Testing the isotropy of the Universe by using the JLA compilation of type-Ia supernovae.

A Quantitative Framework for Testing the Hubble Tension in a Bianchi Type I Cosmological Background Testing the isotropy of the Universe by using the JLA compilation of type-Ia supernovae

Reference 75

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Observation 320e25e2-0456-4438-afe3-4daf9f72e85e · outbound

This paper cites Probing the isotropy of cosmic acceleration traced by Type Ia supernovae.

A Quantitative Framework for Testing the Hubble Tension in a Bianchi Type I Cosmological Background Probing the isotropy of cosmic acceleration traced by Type Ia supernovae

Reference 76

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Observation 7b0fb58c-3454-4337-ac29-bbdc03a5f446 · outbound

This paper cites Evidence for anisotropy of cosmic acceleration.

A Quantitative Framework for Testing the Hubble Tension in a Bianchi Type I Cosmological Background Evidence for anisotropy of cosmic acceleration

Reference 77

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Observation baf52c40-8b8f-45f3-8987-e52562263ea9 · outbound

This paper cites Percent-Level Test of Isotropic Expansion Using Type Ia Supernovae.

A Quantitative Framework for Testing the Hubble Tension in a Bianchi Type I Cosmological Background Percent-Level Test of Isotropic Expansion Using Type Ia Supernovae

Reference 78

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Observation 97410c05-2e6f-4438-a8af-14dbf06556cb · outbound

This paper cites Determining the Hubble constant from gravitational wave observations,.

A Quantitative Framework for Testing the Hubble Tension in a Bianchi Type I Cosmological Background Determining the Hubble constant from gravitational wave observations,

Reference 79

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Observation 457ba705-adb0-4e4b-97a3-e910f9b94e07 · outbound

This paper cites A gravitational-wave standard siren measurement of the Hubble constant.

A Quantitative Framework for Testing the Hubble Tension in a Bianchi Type I Cosmological Background A gravitational-wave standard siren measurement of the Hubble constant

Reference 80

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Observation 1ca7783f-ce95-45a0-9b42-011a44c32029 · outbound

This paper cites Probing cosmic anisotropy with gravitational waves as standard sirens.

A Quantitative Framework for Testing the Hubble Tension in a Bianchi Type I Cosmological Background Probing cosmic anisotropy with gravitational waves as standard sirens

Reference 81

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Observation 17860aeb-f377-4de7-920c-5812360fde97 · outbound

This paper cites Big-Bang Nucleosynthesis After Planck.

A Quantitative Framework for Testing the Hubble Tension in a Bianchi Type I Cosmological Background Big-Bang Nucleosynthesis After Planck

Reference 82

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Observation 49a2ad37-af2f-4770-9974-2dbbbaad3861 · outbound

This paper cites Precision big bang nucleosynthesis with improved Helium-4 predictions.

A Quantitative Framework for Testing the Hubble Tension in a Bianchi Type I Cosmological Background Precision big bang nucleosynthesis with improved Helium-4 predictions

Reference 83

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Observation 3f8e0442-5fa6-4559-acb4-cb862bfb0251 · outbound

This paper cites Planck 2018 results. VII. Isotropy and Statistics of the CMB.

A Quantitative Framework for Testing the Hubble Tension in a Bianchi Type I Cosmological Background Planck 2018 results. VII. Isotropy and Statistics of the CMB

Reference 84

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Observation 81602e4e-f07d-495a-891d-3b58e07926b4 · outbound

This paper cites Is the Observable Universe Consistent with the Cosmological Principle?.

A Quantitative Framework for Testing the Hubble Tension in a Bianchi Type I Cosmological Background Is the Observable Universe Consistent with the Cosmological Principle?

Reference 85

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Observation 4ef88c3c-cf0e-4af2-8416-7ad29fcccb09 · outbound

This paper cites Anisotropic Distance Ladder in Pantheon+ Supernovae.

A Quantitative Framework for Testing the Hubble Tension in a Bianchi Type I Cosmological Background Anisotropic Distance Ladder in Pantheon+ Supernovae

Reference 86

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Observation 134da76d-7fbf-474f-b5a4-a567f19c4081 · outbound

This paper cites The Dipole of the Pantheon+SH0ES Data.

A Quantitative Framework for Testing the Hubble Tension in a Bianchi Type I Cosmological Background The Dipole of the Pantheon+SH0ES Data

Reference 87

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Observation 16a51349-df44-47c1-8e01-da3adf68bff1 · outbound

This paper cites Potential signature of a quadrupolar Hubble expansion in Pantheon+ supernovae.

A Quantitative Framework for Testing the Hubble Tension in a Bianchi Type I Cosmological Background Potential signature of a quadrupolar Hubble expansion in Pantheon+ supernovae

Reference 88

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Observation a3036166-5651-4a43-a7e5-454ead1339b8 · outbound

This paper cites Testing the cosmological principle with the Pantheon+ sample and the region-fitting method.

A Quantitative Framework for Testing the Hubble Tension in a Bianchi Type I Cosmological Background Testing the cosmological principle with the Pantheon+ sample and the region-fitting method

Reference 89

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Observation 15a34094-10e3-4604-9ebf-d7377076ca9e · outbound

This paper cites Testing the isotropy of cosmic acceleration with Pantheon+ and SH0ES: A cosmographic analysis.

A Quantitative Framework for Testing the Hubble Tension in a Bianchi Type I Cosmological Background Testing the isotropy of cosmic acceleration with Pantheon+ and SH0ES: A cosmographic analysis

Reference 90

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Observation ab048a13-3b2b-43bd-b560-31e5ee81696d · outbound

This paper cites Anisotropy in Pantheon+ supernovae.

A Quantitative Framework for Testing the Hubble Tension in a Bianchi Type I Cosmological Background Anisotropy in Pantheon+ supernovae

Reference 91

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Observation 0f910db0-a0bb-46b8-9b4a-6f42a7bff08b · outbound

This paper cites Constraining Cosmological Parameters Based on Relative Galaxy Ages.

A Quantitative Framework for Testing the Hubble Tension in a Bianchi Type I Cosmological Background Constraining Cosmological Parameters Based on Relative Galaxy Ages

Reference 92

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Observation 0d52df2c-2337-4ba6-8501-eeaf6068b901 · outbound

This paper cites A 6% measurement of the Hubble parameter at $z\sim0.45$: direct evidence of the epoch of cosmic re-acceleration.

A Quantitative Framework for Testing the Hubble Tension in a Bianchi Type I Cosmological Background A 6% measurement of the Hubble parameter at $z\sim0.45$: direct evidence of the epoch of cosmic re-acceleration

Reference 93

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Observation 557c6408-e3fe-4138-8b58-dc01a3b1cb24 · outbound

This paper cites Unveiling the Universe with Emerging Cosmological Probes.

A Quantitative Framework for Testing the Hubble Tension in a Bianchi Type I Cosmological Background Unveiling the Universe with Emerging Cosmological Probes

Reference 94

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Observation 676fc4d8-8b03-4eab-8274-fa83e7c3ae79 · outbound

This paper cites Testing anisotropic Hubble expansion.

A Quantitative Framework for Testing the Hubble Tension in a Bianchi Type I Cosmological Background Testing anisotropic Hubble expansion

Reference 95

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Observation 1d083b03-0356-48c4-a515-b8b8aae8be5c · outbound

This paper cites Bayes in the sky: Bayesian inference and model selection in cosmology.

A Quantitative Framework for Testing the Hubble Tension in a Bianchi Type I Cosmological Background Bayes in the sky: Bayesian inference and model selection in cosmology

Reference 96

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Observation e2d98bbb-cb38-40c1-bc6f-0e1bd1b6cb6d · outbound

This paper cites Information criteria for astrophysical model selection.

A Quantitative Framework for Testing the Hubble Tension in a Bianchi Type I Cosmological Background Information criteria for astrophysical model selection

Reference 97

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Observation 45cc4088-38c5-45e1-8028-785a6edbc19e · outbound

This paper cites Ellipsoidal Expansion of the Universe, Cosmic Shear, Acceleration and Jerk Parameter.

A Quantitative Framework for Testing the Hubble Tension in a Bianchi Type I Cosmological Background Ellipsoidal Expansion of the Universe, Cosmic Shear, Acceleration and Jerk Parameter

Reference 98

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Observation bdd90726-7b45-4cc1-ae32-e5a2a208a139 · outbound

This paper cites CMB Anomalies after Planck.

A Quantitative Framework for Testing the Hubble Tension in a Bianchi Type I Cosmological Background CMB Anomalies after Planck

Reference 99

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Observation 723d0107-4c03-4aa9-87f7-1f6c6d15317f · outbound

This paper cites Anisotropic dark energy and ellipsoidal universe.

A Quantitative Framework for Testing the Hubble Tension in a Bianchi Type I Cosmological Background Anisotropic dark energy and ellipsoidal universe

Reference 100

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