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The Hubble constant tension with next-generation galaxy surveys

As of 15 August 2026, this Paper Citation Record lists 43 of 43 outbound references and 0 inbound Pith citation observations for arXiv:1908.04619.

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1908.04619 v2

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Outbound references

Observation 8b50e1f6-efed-4404-961e-d3294e52dec0 · outbound

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

The Hubble constant tension with next-generation galaxy surveys Planck 2018 results. VI. Cosmological parameters

Reference 1

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Observation 32adee23-51e2-4d03-8a88-39be01225aea · outbound

This paper cites Planck 2015 results. XIII. Cosmological parameters.

The Hubble constant tension with next-generation galaxy surveys Planck 2015 results. XIII. Cosmological parameters

Reference 2

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Observation a12083d4-42c6-4c88-b2a4-db04925db543 · outbound

This paper cites Large Magellanic Cloud Cepheid Standards Provide a 1% Foundation for the Determination of the Hubble Constant and Stronger Evidence for Physics Beyond LambdaCDM.

The Hubble constant tension with next-generation galaxy surveys Large Magellanic Cloud Cepheid Standards Provide a 1% Foundation for the Determination of the Hubble Constant and Stronger Evidence for Physics Beyond LambdaCDM

Reference 3

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Observation cdba0c49-b47d-4dbc-8508-c9b119144d37 · outbound

This paper cites Milky Way Cepheid Standards for Measuring Cosmic Distances and Application to Gaia DR2: Implications for the Hubble Constant.

The Hubble constant tension with next-generation galaxy surveys Milky Way Cepheid Standards for Measuring Cosmic Distances and Application to Gaia DR2: Implications for the Hubble Constant

Reference 4

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Observation db090d89-edf7-48b6-af39-9b927e8b0b34 · outbound

This paper cites A 2.4% Determination of the Local Value of the Hubble Constant.

The Hubble constant tension with next-generation galaxy surveys A 2.4% Determination of the Local Value of the Hubble Constant

Reference 5

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Observation 52b99a01-8e73-4bd3-b717-92db91538a9e · outbound

This paper cites H0LiCOW XIII. A 2.4% measurement of $H_{0}$ from lensed quasars: $5.3\sigma$ tension between early and late-Universe probes.

The Hubble constant tension with next-generation galaxy surveys H0LiCOW XIII. A 2.4% measurement of $H_{0}$ from lensed quasars: $5.3\sigma$ tension between early and late-Universe probes

Reference 6

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Observation b29a1791-a6cf-48a6-92d7-99fdc3fef464 · outbound

This paper cites The Carnegie-Chicago Hubble Program. VIII. An Independent Determination of the Hubble Constant Based on the Tip of the Red Giant Branch.

The Hubble constant tension with next-generation galaxy surveys The Carnegie-Chicago Hubble Program. VIII. An Independent Determination of the Hubble Constant Based on the Tip of the Red Giant Branch

Reference 7

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Observation 9ac6b5e5-f875-4dd3-82d1-bfb1f2eaf251 · outbound

This paper cites Consistent Calibration of the Tip of the Red Giant Branch in the Large Magellanic Cloud on the Hubble Space Telescope Photometric System and a Re-determination of the Hubble Constant.

The Hubble constant tension with next-generation galaxy surveys Consistent Calibration of the Tip of the Red Giant Branch in the Large Magellanic Cloud on the Hubble Space Telescope Photometric System and a Re-determination of the Hubble Constant

Reference 8

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Observation 1751e9e3-5141-44d2-96cc-7252eea13ed4 · outbound

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

The Hubble constant tension with next-generation galaxy surveys Tensions between the Early and the Late Universe

Reference 9

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Observation bd8936ac-859c-48c6-bf04-e6e52da4ef0b · outbound

This paper cites Measuring the Homogeneity of the Universe Using Polarization Drift.

The Hubble constant tension with next-generation galaxy surveys Measuring the Homogeneity of the Universe Using Polarization Drift

Reference 10

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Observation 7a6c272a-cdb0-4d80-bcc4-82acb3e7dae3 · outbound

This paper cites The Alcock Paczynski test with Baryon Acoustic Oscillations: systematic effects for future surveys.

The Hubble constant tension with next-generation galaxy surveys The Alcock Paczynski test with Baryon Acoustic Oscillations: systematic effects for future surveys

Reference 11

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Observation 9b641a45-95c1-4f3a-8e4f-40025c603aab · outbound

This paper cites Model independent $H(z)$ reconstruction using the cosmic inverse distance ladder.

The Hubble constant tension with next-generation galaxy surveys Model independent $H(z)$ reconstruction using the cosmic inverse distance ladder

Reference 12

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Observation a6b98857-1ba7-40a1-9ec2-e7b910605139 · outbound

This paper cites Cosmology and Fundamental Physics with the Euclid Satellite.

The Hubble constant tension with next-generation galaxy surveys Cosmology and Fundamental Physics with the Euclid Satellite

Reference 13

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This paper cites Cosmology with Phase 1 of the Square Kilometre Array; Red Book 2018: Technical specifications and performance forecasts.

The Hubble constant tension with next-generation galaxy surveys Cosmology with Phase 1 of the Square Kilometre Array; Red Book 2018: Technical specifications and performance forecasts

Reference 14

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This paper cites Extending cosmological tests of General Relativity with the Square Kilometre Array.

The Hubble constant tension with next-generation galaxy surveys Extending cosmological tests of General Relativity with the Square Kilometre Array

Reference 15

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Observation 2ec75991-d6b1-40c8-9331-10163c47d153 · outbound

This paper cites Baryonic acoustic oscillations from 21cm intensity mapping: the Square Kilometre Array case.

The Hubble constant tension with next-generation galaxy surveys Baryonic acoustic oscillations from 21cm intensity mapping: the Square Kilometre Array case

Reference 16

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Observation 898adc03-b2e6-4641-a430-c43be8d7d6c3 · outbound

This paper cites Evidence for a Lower Value for $H_0$ from Cosmic Chronometers Data?.

The Hubble constant tension with next-generation galaxy surveys Evidence for a Lower Value for $H_0$ from Cosmic Chronometers Data?

Reference 17

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Observation fdbc4bc8-dec9-4ada-9a88-3afd822749db · outbound

This paper cites Model-independent determination on $H_0$ using the latest $H(z)$ data.

The Hubble constant tension with next-generation galaxy surveys Model-independent determination on $H_0$ using the latest $H(z)$ data

Reference 18

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This paper cites $H_0$ from cosmic chronometers and Type Ia supernovae, with Gaussian Processes and the novel Weighted Polynomial Regression method.

The Hubble constant tension with next-generation galaxy surveys $H_0$ from cosmic chronometers and Type Ia supernovae, with Gaussian Processes and the novel Weighted Polynomial Regression method

Reference 19

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The Hubble constant tension with next-generation galaxy surveys Reconstruction of dark energy and expansion dynamics using Gaussian processes

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The Hubble constant tension with next-generation galaxy surveys Gaussian Process Cosmography

Reference 21

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The Hubble constant tension with next-generation galaxy surveys Null tests of the cosmological constant using supernovae

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The Hubble constant tension with next-generation galaxy surveys Non-parametric reconstruction of cosmological matter perturbations

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The Hubble constant tension with next-generation galaxy surveys Model-independent reconstruction of the linear anisotropic stress $\eta$

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The Hubble constant tension with next-generation galaxy surveys Null test for interactions in the dark sector

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The Hubble constant tension with next-generation galaxy surveys The impact of the cosmic variance on $H_0$ on cosmological analyses

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The Hubble constant tension with next-generation galaxy surveys How does an incomplete sky coverage affect the Hubble Constant variance?

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The Hubble constant tension with next-generation galaxy surveys A 2 per cent Hubble constant measurement from standard sirens within 5 years

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The Hubble constant tension with next-generation galaxy surveys Measuring the Hubble constant: Gravitational wave observations meet galaxy clustering

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The Hubble constant tension with next-generation galaxy surveys Measuring the Hubble constant with neutron star black hole mergers

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The Hubble constant tension with next-generation galaxy surveys Unbiased Hubble constant estimation from binary neutron star mergers

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The Hubble constant tension with next-generation galaxy surveys Will Gravitational Wave Sirens Determine the Hubble Constant?

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The Hubble constant tension with next-generation galaxy surveys Gravitational wave standard sirens and cosmological parameter measurement

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This paper cites Prospects for resolving the Hubble constant tension with standard sirens.

The Hubble constant tension with next-generation galaxy surveys Prospects for resolving the Hubble constant tension with standard sirens

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This paper cites A new measurement of the Hubble constant and matter content of the Universe using extragalactic background light $\gamma$-ray attenuation.

The Hubble constant tension with next-generation galaxy surveys A new measurement of the Hubble constant and matter content of the Universe using extragalactic background light $\gamma$-ray attenuation

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The Hubble constant tension with next-generation galaxy surveys An independent determination of the local Hubble constant

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The Hubble constant tension with next-generation galaxy surveys Dark Energy Survey Year 1 Results: A Precise H0 Measurement from DES Y1, BAO, and D/H Data

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The Hubble constant tension with next-generation galaxy surveys A measurement of the Hubble constant using galaxy redshift surveys

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Observation 89b564f2-b34e-4ad3-8ce5-cce88d6a64b4 · outbound

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

The Hubble constant tension with next-generation galaxy surveys A gravitational-wave standard siren measurement of the Hubble constant

Reference 39

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This paper cites Debiasing Cosmic Gravitational Wave Sirens.

The Hubble constant tension with next-generation galaxy surveys Debiasing Cosmic Gravitational Wave Sirens

Reference 40

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Observation 9b6ac58e-e158-4ba6-8dd0-c9a4f9318604 · outbound

This paper cites The DESI Experiment Part I: Science,Targeting, and Survey Design.

The Hubble constant tension with next-generation galaxy surveys The DESI Experiment Part I: Science,Targeting, and Survey Design

Reference 41

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This paper cites MeerKLASS: MeerKAT Large Area Synoptic Survey.

The Hubble constant tension with next-generation galaxy surveys MeerKLASS: MeerKAT Large Area Synoptic Survey

Reference 42

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The Hubble constant tension with next-generation galaxy surveys Unresolved cited work

Reference 43

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