Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links, observed 2026-08-14T13:42:33.118270Z
Paper Citation Record · LEDGER
The Hubble constant tension with next-generation galaxy surveys
As of 23 August 2026, this Paper Citation Record lists 43 of 43 outbound references and 0 inbound Pith citation observations for arXiv:1908.04619.
A citation records a reference. It does not transfer a finding from one paper to another.
Coverage vector
One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-22T06:32:14.747728+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links
A source-named dated measurement, never combined with another source.
Source: cited_works
Reference resolution
43 of 43 outbound references displayed
- verified exact3
- verified fuzzy0
- unresolved40
- parse uncertain0
- malformed identifier0
- metadata mismatch0
External citation measurements
No source-named external measurement is stored.
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
- Resolution
- unresolved
- no resolver link, observed 2026-08-14T13:42:32.991338Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
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
- Resolution
- unresolved
- no resolver link, observed 2026-08-14T13:42:32.995074Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
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
- Resolution
- unresolved
- no resolver link, observed 2026-08-14T13:42:32.998559Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
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
- Resolution
- unresolved
- no resolver link, observed 2026-08-14T13:42:33.001955Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
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
- Resolution
- unresolved
- no resolver link, observed 2026-08-14T13:42:33.005351Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
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
- Resolution
- unresolved
- no resolver link, observed 2026-08-14T13:42:33.008707Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
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
- Resolution
- unresolved
- no resolver link, observed 2026-08-14T13:42:33.012157Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
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
- Resolution
- unresolved
- no resolver link, observed 2026-08-14T13:42:33.015063Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
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
- Resolution
- unresolved
- no resolver link, observed 2026-08-14T13:42:33.018014Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
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
- Resolution
- unresolved
- no resolver link, observed 2026-08-14T13:42:33.020863Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
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
- Resolution
- verified exact
- local_arxiv, observed 2026-08-14T13:42:33.382797Z
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 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
- Resolution
- unresolved
- no resolver link, observed 2026-08-14T13:42:33.026622Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
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
- Resolution
- unresolved
- no resolver link, observed 2026-08-14T13:42:33.029696Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 01a509d7-bd45-4aad-9737-a8ce6d46cf76 · outbound
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
- Resolution
- unresolved
- no resolver link, observed 2026-08-14T13:42:33.032601Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 1a8a8f1f-9fe4-493f-9537-6f2279050653 · outbound
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
- Resolution
- unresolved
- no resolver link, observed 2026-08-14T13:42:33.035586Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
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
- Resolution
- unresolved
- no resolver link, observed 2026-08-14T13:42:33.038546Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
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
- Resolution
- unresolved
- no resolver link, observed 2026-08-14T13:42:33.041411Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
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
- Resolution
- unresolved
- no resolver link, observed 2026-08-14T13:42:33.044357Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 90f89aa4-2158-4382-b097-08b8d2251fc7 · outbound
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
- Resolution
- unresolved
- no resolver link, observed 2026-08-14T13:42:33.047219Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 011802d3-3174-47ad-9d93-43fc95bd2dd9 · outbound
This paper cites Reconstruction of dark energy and expansion dynamics using Gaussian processes.
The Hubble constant tension with next-generation galaxy surveys Reconstruction of dark energy and expansion dynamics using Gaussian processes
Reference 20
- Resolution
- unresolved
- no resolver link, observed 2026-08-14T13:42:33.049983Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation c43e6dec-ea7c-4e6e-b41a-61a9edf72c37 · outbound
This paper cites Gaussian Process Cosmography.
The Hubble constant tension with next-generation galaxy surveys Gaussian Process Cosmography
Reference 21
- Resolution
- unresolved
- no resolver link, observed 2026-08-14T13:42:33.053083Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 3c105e43-e2da-4db5-90f0-1cc478c5e8ae · outbound
This paper cites Null tests of the cosmological constant using supernovae.
The Hubble constant tension with next-generation galaxy surveys Null tests of the cosmological constant using supernovae
Reference 22
- Resolution
- unresolved
- no resolver link, observed 2026-08-14T13:42:33.056050Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 452b990f-04b4-44de-b90d-82a9ab756a58 · outbound
This paper cites Non-parametric reconstruction of cosmological matter perturbations.
The Hubble constant tension with next-generation galaxy surveys Non-parametric reconstruction of cosmological matter perturbations
Reference 23
- Resolution
- verified exact
- local_arxiv, observed 2026-08-14T13:42:33.289349Z
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 2b121c74-e80d-46b4-b9bd-e38b6cc718a9 · outbound
This paper cites Model-independent reconstruction of the linear anisotropic stress $\eta$.
The Hubble constant tension with next-generation galaxy surveys Model-independent reconstruction of the linear anisotropic stress $\eta$
Reference 24
- Resolution
- unresolved
- no resolver link, observed 2026-08-14T13:42:33.062018Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 1f0928dd-616f-4209-8029-cb35eeb9e0ff · outbound
This paper cites Null test for interactions in the dark sector.
The Hubble constant tension with next-generation galaxy surveys Null test for interactions in the dark sector
Reference 25
- Resolution
- unresolved
- no resolver link, observed 2026-08-14T13:42:33.064954Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation a2c2319f-e340-487c-ab9f-17e240561894 · outbound
This paper cites The impact of the cosmic variance on $H_0$ on cosmological analyses.
The Hubble constant tension with next-generation galaxy surveys The impact of the cosmic variance on $H_0$ on cosmological analyses
Reference 26
- Resolution
- unresolved
- no resolver link, observed 2026-08-14T13:42:33.068055Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 49794afe-a283-4562-8ae9-d8de34614a28 · outbound
This paper cites How does an incomplete sky coverage affect the Hubble Constant variance?.
The Hubble constant tension with next-generation galaxy surveys How does an incomplete sky coverage affect the Hubble Constant variance?
Reference 27
- Resolution
- unresolved
- no resolver link, observed 2026-08-14T13:42:33.071052Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 561e5cd2-718b-458a-bc18-1fd61f88ecd4 · outbound
This paper cites A 2 per cent Hubble constant measurement from standard sirens within 5 years.
The Hubble constant tension with next-generation galaxy surveys A 2 per cent Hubble constant measurement from standard sirens within 5 years
Reference 28
- Resolution
- unresolved
- no resolver link, observed 2026-08-14T13:42:33.074326Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 32adf742-3b1a-4e3f-a484-2ff6a86a833d · outbound
This paper cites Measuring the Hubble constant: Gravitational wave observations meet galaxy clustering.
The Hubble constant tension with next-generation galaxy surveys Measuring the Hubble constant: Gravitational wave observations meet galaxy clustering
Reference 29
- Resolution
- unresolved
- no resolver link, observed 2026-08-14T13:42:33.077387Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation eeb7043f-c5c0-4f81-8283-9f3fc2cb67e6 · outbound
This paper cites Measuring the Hubble constant with neutron star black hole mergers.
The Hubble constant tension with next-generation galaxy surveys Measuring the Hubble constant with neutron star black hole mergers
Reference 30
- Resolution
- unresolved
- no resolver link, observed 2026-08-14T13:42:33.080198Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 0c83b4f5-4ae4-4cea-9e99-6fa18abc3a16 · outbound
This paper cites Unbiased Hubble constant estimation from binary neutron star mergers.
The Hubble constant tension with next-generation galaxy surveys Unbiased Hubble constant estimation from binary neutron star mergers
Reference 31
- Resolution
- unresolved
- no resolver link, observed 2026-08-14T13:42:33.083096Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation edc2e001-3de8-479e-9541-7a85dabb10c3 · outbound
This paper cites Will Gravitational Wave Sirens Determine the Hubble Constant?.
The Hubble constant tension with next-generation galaxy surveys Will Gravitational Wave Sirens Determine the Hubble Constant?
Reference 32
- Resolution
- unresolved
- no resolver link, observed 2026-08-14T13:42:33.085929Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 333d42fa-4c44-47da-aefc-725449a45d32 · outbound
This paper cites Gravitational wave standard sirens and cosmological parameter measurement.
The Hubble constant tension with next-generation galaxy surveys Gravitational wave standard sirens and cosmological parameter measurement
Reference 33
- Resolution
- unresolved
- no resolver link, observed 2026-08-14T13:42:33.088871Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation e03ab12c-23a5-4380-9ccf-44e2329854b3 · outbound
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
Reference 34
- Resolution
- unresolved
- no resolver link, observed 2026-08-14T13:42:33.091714Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 64f342f8-0b88-45e9-86ce-dc97d1a46a26 · outbound
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
Reference 35
- Resolution
- unresolved
- no resolver link, observed 2026-08-14T13:42:33.094691Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation ae0d7093-560a-43d3-8ace-c124b1747c13 · outbound
This paper cites An independent determination of the local Hubble constant.
The Hubble constant tension with next-generation galaxy surveys An independent determination of the local Hubble constant
Reference 36
- Resolution
- unresolved
- no resolver link, observed 2026-08-14T13:42:33.097661Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 9480866b-3714-4977-9de0-1fe0cb609699 · outbound
This paper cites Dark Energy Survey Year 1 Results: A Precise H0 Measurement from DES Y1, BAO, and D/H Data.
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
Reference 37
- Resolution
- unresolved
- no resolver link, observed 2026-08-14T13:42:33.100689Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 07f820ef-cf40-42ab-a84e-0e82d4660c6f · outbound
This paper cites A measurement of the Hubble constant using galaxy redshift surveys.
The Hubble constant tension with next-generation galaxy surveys A measurement of the Hubble constant using galaxy redshift surveys
Reference 38
- Resolution
- verified exact
- local_arxiv, observed 2026-08-14T13:42:33.175101Z
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 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
- Resolution
- unresolved
- no resolver link, observed 2026-08-14T13:42:33.106268Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 9f36a042-da64-4485-aa45-48ef86fe6400 · outbound
This paper cites Debiasing Cosmic Gravitational Wave Sirens.
The Hubble constant tension with next-generation galaxy surveys Debiasing Cosmic Gravitational Wave Sirens
Reference 40
- Resolution
- unresolved
- no resolver link, observed 2026-08-14T13:42:33.109100Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
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
- Resolution
- unresolved
- no resolver link, observed 2026-08-14T13:42:33.112153Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation f2831f9e-3d3d-43e6-bcd1-828d79e1888a · outbound
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
- Resolution
- unresolved
- no resolver link, observed 2026-08-14T13:42:33.115197Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 28f81bce-2a8a-4e4c-a340-8346cc168c77 · outbound
This paper cites an unresolved cited work.
The Hubble constant tension with next-generation galaxy surveys Unresolved cited work
Reference 43
- Resolution
- unresolved
- raw_fallback, observed 2026-08-14T13:42:33.467659Z
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.
Pith citing papers
No inbound Pith citation observations are available.