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Quasar cosmology II: joint analyses with Cosmic Microwave Background

As of 7 August 2026, this Paper Citation Record lists 100 of 121 outbound references and 1 inbound Pith citation observation for arXiv:2506.21477.

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Outbound references

Observation 1709f158-f442-43ec-87d8-bcf28fcd0e34 · outbound

This paper cites Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant.

Quasar cosmology II: joint analyses with Cosmic Microwave Background Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant

Reference 1

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Observation 91aec2e3-c172-4e93-8581-28cd5869b6e9 · outbound

This paper cites Measurements of Omega and Lambda from 42 High-Redshift Supernovae.

Quasar cosmology II: joint analyses with Cosmic Microwave Background Measurements of Omega and Lambda from 42 High-Redshift Supernovae

Reference 2

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Observation 12ac138d-871f-40f4-8551-e6e3e7d4f0d1 · outbound

This paper cites The Complete Light-curve Sample of Spectroscopically Confirmed Type Ia Supernovae from Pan-STARRS1 and Cosmological Constraints from The Combined Pantheon Sample.

Quasar cosmology II: joint analyses with Cosmic Microwave Background The Complete Light-curve Sample of Spectroscopically Confirmed Type Ia Supernovae from Pan-STARRS1 and Cosmological Constraints from The Combined Pantheon Sample

Reference 3

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Observation 3dd87333-9fcb-4be6-8cb3-7e1fe9fa10a3 · 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.

Quasar cosmology II: joint analyses with Cosmic Microwave 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 a2e230ef-59a0-4be4-9942-b76ef69a2429 · outbound

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

Quasar cosmology II: joint analyses with Cosmic Microwave Background Planck 2018 results. VI. Cosmological parameters

Reference 5

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Observation a808ede6-2db3-4237-89f7-ca86c1dc4004 · outbound

This paper cites Nine-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Parameter Results.

Quasar cosmology II: joint analyses with Cosmic Microwave Background Nine-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Parameter Results

Reference 6

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Observation 1cd85767-7a3d-4b4e-a966-31cd56e7ba47 · outbound

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.

Quasar cosmology II: joint analyses with Cosmic Microwave Background The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Cosmological Implications from two Decades of Spectroscopic Surveys at the Apache Point observatory

Reference 7

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Observation aee29177-8a8f-40df-97a0-aace6574a544 · outbound

This paper cites The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample: First measurement of Baryon Acoustic Oscillations between redshift 0.8 and 2.2.

Quasar cosmology II: joint analyses with Cosmic Microwave Background The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample: First measurement of Baryon Acoustic Oscillations between redshift 0.8 and 2.2

Reference 8

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Observation 2699a2ff-5229-4982-a90b-9fefdb743363 · outbound

This paper cites The 6dF Galaxy Survey: Baryon Acoustic Oscillations and the Local Hubble Constant.

Quasar cosmology II: joint analyses with Cosmic Microwave Background The 6dF Galaxy Survey: Baryon Acoustic Oscillations and the Local Hubble Constant

Reference 9

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Observation 0204a97a-81d1-41b8-91ce-1cb99fb2c9fd · outbound

This paper cites The Clustering of the SDSS DR7 Main Galaxy Sample I: A 4 per cent Distance Measure at z=0.15.

Quasar cosmology II: joint analyses with Cosmic Microwave Background The Clustering of the SDSS DR7 Main Galaxy Sample I: A 4 per cent Distance Measure at z=0.15

Reference 10

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Observation a5180e2d-3644-448a-b9f4-907f7264b1e2 · outbound

This paper cites The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological analysis of the DR12 galaxy sample.

Quasar cosmology II: joint analyses with Cosmic Microwave Background The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological analysis of the DR12 galaxy sample

Reference 11

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This paper cites The Cosmological Constant.

Quasar cosmology II: joint analyses with Cosmic Microwave Background The Cosmological Constant

Reference 12

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Quasar cosmology II: joint analyses with Cosmic Microwave Background Weinberg, The cosmological constant problem, Reviews of Modern Physics 61 (1) (1989) 1–23.doi:10.1103/RevModPhys.61.1

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Quasar cosmology II: joint analyses with Cosmic Microwave Background One-Loop Analysis of the Electroweak Breaking in Supersymmetric Models and the Fine-Tuning Problems

Reference 14

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This paper cites A review of indirect searches for particle dark matter.

Quasar cosmology II: joint analyses with Cosmic Microwave Background A review of indirect searches for particle dark matter

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Quasar cosmology II: joint analyses with Cosmic Microwave Background Effective Field Theory of Dark Energy: a Review

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Quasar cosmology II: joint analyses with Cosmic Microwave Background Using the tilted flat-$\Lambda$CDM and the untilted non-flat $\Lambda$CDM inflation models to measure cosmological parameters from a compilation of observational data

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Quasar cosmology II: joint analyses with Cosmic Microwave Background Planck evidence for a closed Universe and a possible crisis for cosmology

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Quasar cosmology II: joint analyses with Cosmic Microwave Background Curvature tension: evidence for a closed universe

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Quasar cosmology II: joint analyses with Cosmic Microwave Background Investigating Cosmic Discordance

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Quasar cosmology II: joint analyses with Cosmic Microwave Background 2021-$H_0$ Odyssey: Closed, Phantom and Interacting Dark Energy Cosmologies

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Quasar cosmology II: joint analyses with Cosmic Microwave Background Non-parametric spatial curvature inference using late-universe cosmological probes

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Quasar cosmology II: joint analyses with Cosmic Microwave Background The galaxy power spectrum take on spatial curvature and cosmic concordance

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Quasar cosmology II: joint analyses with Cosmic Microwave Background In the Realm of the Hubble tension $-$ a Review of Solutions

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Quasar cosmology II: joint analyses with Cosmic Microwave Background Looking for interactions in the cosmological dark sector

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Quasar cosmology II: joint analyses with Cosmic Microwave Background J-PAS: forecasts on interacting vacuum energy models

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Quasar cosmology II: joint analyses with Cosmic Microwave Background Cosmology Intertwined: A Review of the Particle Physics, Astrophysics, and Cosmology Associated with the Cosmological Tensions and Anomalies

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Quasar cosmology II: joint analyses with Cosmic Microwave Background Large Magellanic Cloud Cepheid Standards Provide a 1% Foundation for the Determination of the Hubble Constant and Stronger Evidence for Physics Beyond LambdaCDM

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Quasar cosmology II: joint analyses with Cosmic Microwave Background Local determination of the Hubble constant and the deceleration parameter

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Quasar cosmology II: joint analyses with Cosmic Microwave Background H0LiCOW XIII. A 2.4% measurement of $H_{0}$ from lensed quasars: $5.3\sigma$ tension between early and late-Universe probes

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Quasar cosmology II: joint analyses with Cosmic Microwave Background $H_0$ from cosmic chronometers and Type Ia supernovae, with Gaussian Processes and the novel Weighted Polynomial Regression method

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Quasar cosmology II: joint analyses with Cosmic Microwave Background Cosmic chronometers to calibrate the ladders and measure the curvature of the Universe. A model-independent study

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Quasar cosmology II: joint analyses with Cosmic Microwave Background A model-independent determination of the Hubble constant from lensed quasars and supernovae using Gaussian process regression

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Quasar cosmology II: joint analyses with Cosmic Microwave Background Unresolved cited work

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Quasar cosmology II: joint analyses with Cosmic Microwave Background Measurements of the Hubble Constant: Tensions in Perspective

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Quasar cosmology II: joint analyses with Cosmic Microwave Background An updated Gamma Ray Bursts Hubble diagram

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This paper cites Non-parametric study of the evolution of the cosmological equation of state with SNeIa, BAO and high redshift GRBs.

Quasar cosmology II: joint analyses with Cosmic Microwave Background Non-parametric study of the evolution of the cosmological equation of state with SNeIa, BAO and high redshift GRBs

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Quasar cosmology II: joint analyses with Cosmic Microwave Background On the evolution of the Hubble constant with the SNe Ia Pantheon Sample and Baryon Acoustic Oscillations: a feasibility study for GRB-cosmology in 2030

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Observation 51eb302a-25da-4eda-976c-8ba4b65dcfdf · outbound

This paper cites Capozziello, M.

Quasar cosmology II: joint analyses with Cosmic Microwave Background Capozziello, M

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This paper cites Gamma-Ray Bursts, Supernovae Ia and Baryon Acoustic Oscillations: a binned cosmological analysis.

Quasar cosmology II: joint analyses with Cosmic Microwave Background Gamma-Ray Bursts, Supernovae Ia and Baryon Acoustic Oscillations: a binned cosmological analysis

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Quasar cosmology II: joint analyses with Cosmic Microwave Background Precision cosmology with Pad\'e rational approximations: theoretical predictions versus observational limits

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This paper cites Cosmographic analysis with Chebyshev polynomials.

Quasar cosmology II: joint analyses with Cosmic Microwave Background Cosmographic analysis with Chebyshev polynomials

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Quasar cosmology II: joint analyses with Cosmic Microwave Background Cosmology with gamma-ray bursts: II Cosmography challenges and cosmological scenarios for the accelerated Universe

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Observation 043c5c83-7b0d-42f4-baa9-3a85a8405b98 · outbound

This paper cites Inverse Cosmography: testing the effectiveness of cosmographic polynomials using machine learning.

Quasar cosmology II: joint analyses with Cosmic Microwave Background Inverse Cosmography: testing the effectiveness of cosmographic polynomials using machine learning

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This paper cites Risaliti, E.

Quasar cosmology II: joint analyses with Cosmic Microwave Background Risaliti, E

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Quasar cosmology II: joint analyses with Cosmic Microwave Background Cosmography by orthogonalized logarithmic polynomials

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Observation a3b7bee9-7b17-4962-a6ba-a1ed60709121 · outbound

This paper cites Connecting early and late epochs by f(z)CDM cosmography.

Quasar cosmology II: joint analyses with Cosmic Microwave Background Connecting early and late epochs by f(z)CDM cosmography

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This paper cites Extended Gravity Cosmography.

Quasar cosmology II: joint analyses with Cosmic Microwave Background Extended Gravity Cosmography

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This paper cites Addressing the cosmological $H_0$ tension by the Heisenberg uncertainty.

Quasar cosmology II: joint analyses with Cosmic Microwave Background Addressing the cosmological $H_0$ tension by the Heisenberg uncertainty

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Observation e5f1380c-d10b-4b5e-8410-b2b77b370555 · outbound

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Quasar cosmology II: joint analyses with Cosmic Microwave Background Cosmological model insensitivity of local $H_0$ from the Cepheid distance ladder

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Observation 2a2204e7-a38c-4c2a-906f-e2ba13a1dbf3 · outbound

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Quasar cosmology II: joint analyses with Cosmic Microwave Background A $w-M$ phantom transition at $z_t<0.1$ as a resolution of the Hubble tension

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Observation 7688fe39-eb90-4a68-96fa-3774571b9db6 · outbound

This paper cites $H_0$ Tension, Phantom Dark Energy and Cosmological Parameter Degeneracies.

Quasar cosmology II: joint analyses with Cosmic Microwave Background $H_0$ Tension, Phantom Dark Energy and Cosmological Parameter Degeneracies

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Observation 77738fb5-4dae-4a9e-808c-2213bc2dba20 · outbound

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Quasar cosmology II: joint analyses with Cosmic Microwave Background A look at the Hubble speed from first principles

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Quasar cosmology II: joint analyses with Cosmic Microwave Background On the Hubble constant tension in the SNe Ia Pantheon sample

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Quasar cosmology II: joint analyses with Cosmic Microwave Background $f(R)$ gravity in the Jordan Frame as a Paradigm for the Hubble Tension

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This paper cites Questioning the $H_0$ tension via the look-back time.

Quasar cosmology II: joint analyses with Cosmic Microwave Background Questioning the $H_0$ tension via the look-back time

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Quasar cosmology II: joint analyses with Cosmic Microwave Background Unresolved cited work

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Quasar cosmology II: joint analyses with Cosmic Microwave Background A Luminous Quasar at Redshift 7.642

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Quasar cosmology II: joint analyses with Cosmic Microwave Background The X-ray-to-Optical Properties of Optically-Selected Active Galaxies Over Wide Luminosity and Redshift Ranges

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Quasar cosmology II: joint analyses with Cosmic Microwave Background The X-ray Properties of the Most-Luminous Quasars from the Sloan Digital Sky Survey

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Quasar cosmology II: joint analyses with Cosmic Microwave Background Lusso, et al., The X-ray to optical-UV luminosity ratio of X-ray selected type 1 AGN in XMM-COSMOS, A&A512 (2010) A34.arXiv:0912

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Observation a7e1e4a8-ebd1-425b-97b0-4c197b2f559d · outbound

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Quasar cosmology II: joint analyses with Cosmic Microwave Background The tight relation between X-ray and ultraviolet luminosity of quasars

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Observation 8dac9e2f-b2d9-4439-abd2-3a8b0c4ae907 · outbound

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Quasar cosmology II: joint analyses with Cosmic Microwave Background Quasars as standard candles III. Validation of a new sample for cosmological studies

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Quasar cosmology II: joint analyses with Cosmic Microwave Background The Chandra view of the relation between X-ray and UV emission in quasars

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Quasar cosmology II: joint analyses with Cosmic Microwave Background The High-z Quasar Hubble Diagram

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Quasar cosmology II: joint analyses with Cosmic Microwave Background Tension with the flat {\Lambda}CDM model from a high redshift Hubble Diagram of supernovae, quasars and gamma-ray bursts

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Observation 707d51d8-610f-42d7-914c-53575b1ac3e5 · outbound

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Quasar cosmology II: joint analyses with Cosmic Microwave Background Quasar cosmology: dark energy evolution and spatial curvature

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Observation 7bf60655-c9fc-4441-90d9-56acfe913e09 · outbound

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Quasar cosmology II: joint analyses with Cosmic Microwave Background Quasars: standard candles up to z=7.5 with the precision of Supernovae Ia

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Observation 3bd65e0e-7f7e-42c2-9713-5dbadaccc261 · outbound

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Quasar cosmology II: joint analyses with Cosmic Microwave Background Gamma-Ray Bursts, Quasars, Baryonic Acoustic Oscillations, and Supernovae Ia: new statistical insights and cosmological constraints

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Observation b0fb2209-c0f4-4f23-a060-dadfd1034dcf · outbound

This paper cites Reducing the uncertainty on the Hubble constant up to 35\% with an improved statistical analysis: different best-fit likelihoods for Supernovae Ia, Baryon Acoustic Oscillations, Quasars, and Gamma-Ray Bursts.

Quasar cosmology II: joint analyses with Cosmic Microwave Background Reducing the uncertainty on the Hubble constant up to 35\% with an improved statistical analysis: different best-fit likelihoods for Supernovae Ia, Baryon Acoustic Oscillations, Quasars, and Gamma-Ray Bursts

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Observation 11b140cf-f8b0-4d40-9a48-3be8868e8ed2 · outbound

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Quasar cosmology II: joint analyses with Cosmic Microwave Background Eppur \`e piatto? The cosmic chronometer take on spatial curvature and cosmic concordance

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Observation 0605edce-6c27-448b-bdc3-0cb18502be72 · outbound

This paper cites Dark sector interactions and the curvature of the Universe in light of Planck's 2018 data.

Quasar cosmology II: joint analyses with Cosmic Microwave Background Dark sector interactions and the curvature of the Universe in light of Planck's 2018 data

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This paper cites Testing the growth rate in homogeneous and inhomogeneous interacting vacuum models.

Quasar cosmology II: joint analyses with Cosmic Microwave Background Testing the growth rate in homogeneous and inhomogeneous interacting vacuum models

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Quasar cosmology II: joint analyses with Cosmic Microwave Background Non-adiabatic Chaplygin gas

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Quasar cosmology II: joint analyses with Cosmic Microwave Background Observational tests of non-adiabatic Chaplygin gas

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Quasar cosmology II: joint analyses with Cosmic Microwave Background Cobaya: Code for Bayesian Analysis of hierarchical physical models

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Quasar cosmology II: joint analyses with Cosmic Microwave Background Planck 2018 results. V. CMB power spectra and likelihoods

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Quasar cosmology II: joint analyses with Cosmic Microwave Background Planck 2018 results. VIII. Gravitational lensing

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This paper cites Cosmic Distances Calibrated to 1% Precision with Gaia EDR3 Parallaxes and Hubble Space Telescope Photometry of 75 Milky Way Cepheids Confirm Tension with LambdaCDM.

Quasar cosmology II: joint analyses with Cosmic Microwave Background Cosmic Distances Calibrated to 1% Precision with Gaia EDR3 Parallaxes and Hubble Space Telescope Photometry of 75 Milky Way Cepheids Confirm Tension with LambdaCDM

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Observation 5250c78b-8469-4c9d-be5c-a37a61fd6324 · outbound

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Quasar cosmology II: joint analyses with Cosmic Microwave Background Are quasars reliable standard candles?

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Observation 66f42a26-d0b5-4491-8545-1746c7604aed · outbound

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Quasar cosmology II: joint analyses with Cosmic Microwave Background emcee: The MCMC Hammer

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Quasar cosmology II: joint analyses with Cosmic Microwave Background A Hubble Diagram for Quasars

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Quasar cosmology II: joint analyses with Cosmic Microwave Background Dark Energy Survey Year 1 Results: Cosmological Constraints from Galaxy Clustering and Weak Lensing

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Observation 019afc3f-a8d0-43f8-a7e5-62df1d71d593 · outbound

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Quasar cosmology II: joint analyses with Cosmic Microwave Background Dark Energy Survey Year 1 Results: Multi-Probe Methodology and Simulated Likelihood Analyses

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Quasar cosmology II: joint analyses with Cosmic Microwave Background Dark Energy Survey Year 1 Results: Cosmological Constraints from Cosmic Shear

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Observation 18462c2c-8525-46d5-bb5e-56d424ca6f07 · outbound

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Quasar cosmology II: joint analyses with Cosmic Microwave Background Accelerating Universes with Scaling Dark Matter

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This paper cites Exploring the Expansion History of the Universe.

Quasar cosmology II: joint analyses with Cosmic Microwave Background Exploring the Expansion History of the Universe

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Quasar cosmology II: joint analyses with Cosmic Microwave Background Density perturbations in an Universe dominated by the Chaplygin gas

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Quasar cosmology II: joint analyses with Cosmic Microwave Background Generalized Chaplygin Gas, Accelerated Expansion and Dark Energy-Matter Unification

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Quasar cosmology II: joint analyses with Cosmic Microwave Background The end of unified dark matter?

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Quasar cosmology II: joint analyses with Cosmic Microwave Background Generalized Chaplygin Gas Model: Dark Energy - Dark Matter Unification and CMBR Constraints

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This paper cites Does a generalized Chaplygin gas correctly describe the cosmological dark sector?.

Quasar cosmology II: joint analyses with Cosmic Microwave Background Does a generalized Chaplygin gas correctly describe the cosmological dark sector?

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Quasar cosmology II: joint analyses with Cosmic Microwave Background Cosmological constraints on parametrized interacting dark energy

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Quasar cosmology II: joint analyses with Cosmic Microwave Background Unification of Dark Matter and Dark Energy: the Inhomogeneous Chaplygin Gas

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Quasar cosmology II: joint analyses with Cosmic Microwave Background Constraints on Chaplygin quartessence from the CLASS gravitational lens statistics and supernova data

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Quasar cosmology II: joint analyses with Cosmic Microwave Background Cosmological constraints on a decomposed Chaplygin gas

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Quasar cosmology II: joint analyses with Cosmic Microwave Background The Revival of the Unified Dark Energy-Dark Matter Model ?

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Quasar cosmology II: joint analyses with Cosmic Microwave Background Dynamical system analysis of interacting models

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Quasar cosmology II: joint analyses with Cosmic Microwave Background On the concordance of cosmological data in the case of the generalized Chaplygin gas

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BAO miscalibration cannot rescue late-time solutions to the Hubble tension cites this paper.

BAO miscalibration cannot rescue late-time solutions to the Hubble tension Quasar cosmology II: joint analyses with Cosmic Microwave Background

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