Built on

P. Agrawal, F.-Y. Cyr-Racine, D. Pinner, and L. Randall, Rock ‘n’ roll solutions to the Hubble tension, Phys. Dark Univ. 42
Original
1904
Earlier work this paper cites.
M.-X. Lin, G. Benevento, W. Hu, and M. Raveri, Acoustic Dark Energy: Potential Conversion of the Hubble Tension, Phys. Rev. D 100
Original
1905
Earlier work this paper cites.
R. Arcodia, A. Merloni, K. Nandra, and G. Ponti, Testing the disk-corona interplay in radiatively-efficient broad-line AGN, Astron. Astrophys. 628
Original
1907
Earlier work this paper cites.
E. Lusso, E. Piedipalumbo, G. Risaliti, M. Paolillo, S. Bisogni, E. Nardini, and L. Amati, Tension with the flat Λ \Lambda CDM model from a high-redshift Hubble diagram of supernovae, quasars, and gamma-ray bursts, Astron. Astrophys. 628
Original
1907
Earlier work this paper cites.
L. Knox and M. Millea, Hubble constant hunter’s guide, Phys. Rev. D 101
Original
1908
Earlier work this paper cites.
F. Salvestrini, G. Risaliti, S. Bisogni, E. Lusso, and C. Vignali, Quasars as standard candles II: The non linear relation between UV and X-ray emission at high redshifts, Astron. Astrophys. 631
Original
1909
Earlier work this paper cites.
F. Niedermann and M. S. Sloth, New early dark energy, Phys. Rev. D 103
Original
1910
Earlier work this paper cites.
A. Lewis, Getdist: a python package for analysing monte carlo samples (2019), arXiv:1910.13970 [astro-ph.IM]
Original
1910
Earlier work this paper cites.
T. Yang, A. Banerjee, and E. Ó Colgáin, Cosmography and flat Λ \Lambda CDM tensions at high redshift, Phys. Rev. D 102
Original
1911
Earlier work this paper cites.
H. Velten and S. Gomes, Is the Hubble diagram of quasars in tension with concordance cosmology?, Phys. Rev. D 101
Original
1911
Earlier work this paper cites.
S. S. Wilks, The Large-Sample Distribution of the Likelihood Ratio for Testing Composite Hypotheses, The Annals of Mathematical Statistics 9
1938
Earlier work this paper cites.
S. Weinberg, The Cosmological Constant Problem, Rev. Mod. Phys. 61
1989
Earlier work this paper cites.
G. J. Feldman and R. D. Cousins, A Unified approach to the classical statistical analysis of small signals, Phys. Rev. D 57
1998
Earlier work this paper cites.
R. K. Sheth and G. Tormen, Large scale bias and the peak background split, Mon. Not. Roy. Astron. Soc. 308
1999
Earlier work this paper cites.
G. Ye and Y.-S. Piao, Is the Hubble tension a hint of AdS phase around recombination?, Phys. Rev. D 101
Original
2001
Earlier work this paper cites.
L. Amati et al. , Intrinsic spectra and energetics of BeppoSAX gamma-ray bursts with known redshifts, Astron. Astrophys. 390
2002
Earlier work this paper cites.
C. Vignali, W. N. Brandt, and D. P. Schneider, X-ray emission from radio - quiet quasars in the SDSS Early Data Release. The Alpha(ox) dependence upon UV luminosity, Astron. J. 125
2003
Earlier work this paper cites.
N. Khadka and B. Ratra, Using quasar X-ray and UV flux measurements to constrain cosmological model parameters, Mon. Not. Roy. Astron. Soc. 497
Original
2004
Earlier work this paper cites.
D. W. Just, W. N. Brandt, O. Shemmer, A. T. Steffen, D. P. Schneider, G. Chartas, and G. P. Garmire, The X-ray Properties of the Most-Luminous Quasars from the Sloan Digital Sky Survey, Astrophys. J. 665
Original
2007
Earlier work this paper cites.
S. Alam et al. (eBOSS), Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Cosmological implications from two decades of spectroscopic surveys at the Apache Point Observatory, Phys. Rev. D 103
Original
2007
Earlier work this paper cites.
E. Lusso et al. , Quasars as standard candles III. Validation of a new sample for cosmological studies, Astron. Astrophys. 642
Original
2008
Earlier work this paper cites.
K. Jedamzik, L. Pogosian, and G.-B. Zhao, Why reducing the cosmic sound horizon alone can not fully resolve the Hubble tension, Commun. in Phys. 4
Original
2010
Earlier work this paper cites.
E. Lusso, A. Comastri, C. Vignali, G. Zamorani, M. Brusa, R. Gilli, K. Iwasawa, M. Salvato, F. Civano, M. Elvis, A. Merloni, A. Bongiorno, J. R. Trump, A. M. Koekemoer, E. Schinnerer, E. Le Floc’h, N. Cappelluti, K. Jahnke, M. Sargent, J. Silverman, V. Mainieri, F. Fiore, M. Bolzonella, O. Le Fèvre, B. Garilli, A. Iovino, J. P. Kneib, F. Lamareille, S. Lilly, M. Mignoli, M. Scodeggio, and D. Vergani, The x-ray to optical-uv luminosity ratio of x-ray selected type 1 agn in xmm-cosmos, Astronomy and Astrophysics 512
2010
Earlier work this paper cites.
O. Luongo and M. Muccino, Model-independent calibrations of gamma-ray bursts using machine learning, Mon. Not. Roy. Astron. Soc. 503
Original
2011
Earlier work this paper cites.
N. Khadka and B. Ratra, Determining the range of validity of quasar X-ray and UV flux measurements for constraining cosmological model parameters, Mon. Not. Roy. Astron. Soc. 502
Original
2012
Earlier work this paper cites.
D. Foreman-Mackey, D. W. Hogg, D. Lang, and J. Goodman, emcee: The MCMC Hammer, Publ. Astron. Soc. Pac. 125
Original
2013
Earlier work this paper cites.
G. Risaliti and E. Lusso, A Hubble Diagram for Quasars, Astrophys. J. 815
Original
2015
Earlier work this paper cites.
G. Dvali and C. Gomez, Quantum Exclusion of Positive Cosmological Constant?, Annalen Phys. 528
Original
2016
Earlier work this paper cites.
R. Trotta, Bayesian Methods in Cosmology (2017) arXiv:1701.01467 [astro-ph.CO]
Original
2017
Earlier work this paper cites.
E. Lusso and G. Risaliti, Quasars as standard candles I: The physical relation between disc and coronal emission, Astron. Astrophys. 602
Original
2017
Earlier work this paper cites.
G. Obied, H. Ooguri, L. Spodyneiko, and C. Vafa, De Sitter Space and the Swampland, arXiv e-prints , arXiv:1806.08362 (2018) , arXiv:1806.08362 [hep-th]
Original
2018
Earlier work this paper cites.
A. Kubota and C. Done, A physical model of the broad-band continuum of AGN and its implications for the UV/X relation and optical variability, Mon. Not. Roy. Astron. Soc. 480
Original
2018
Earlier work this paper cites.
V. Poulin, T. L. Smith, T. Karwal, and M. Kamionkowski, Early Dark Energy Can Resolve The Hubble Tension, Phys. Rev. Lett. 122
Original
2019
Earlier work this paper cites.
G. Risaliti and E. Lusso, Cosmological constraints from the Hubble diagram of quasars at high redshifts, Nature Astron. 3
Original
2019
Earlier work this paper cites.
G. Dvali and C. Gomez, On Exclusion of Positive Cosmological Constant, Fortsch. Phys. 67
Original
2019
Earlier work this paper cites.
E. Di Valentino, O. Mena, S. Pan, L. Visinelli, W. Yang, A. Melchiorri, D. F. Mota, A. G. Riess, and J. Silk, In the realm of the Hubble tension—a review of solutions, Class. Quant. Grav. 38
Original
2021
Earlier work this paper cites.
N. Aghanim et al. (Planck), Planck 2018 results. VI. Cosmological parameters, Astron. Astrophys. 641
Original
2021
Earlier work this paper cites.
S. Bisogni, E. Lusso, F. Civano, E. Nardini, G. Risaliti, M. Elvis, and G. Fabbiano, The Chandra view of the relation between X-ray and UV emission in quasars, Astron. Astrophys. 655
Original
2021
Earlier work this paper cites.
N. J. Adams, C. J. Conselice, L. Ferreira, D. Austin, J. A. A. Trussler, I. Juodžbalis, S. M. Wilkins, J. Caruana, P. Dayal, A. Verma, and A. P. Vijayan, Discovery and properties of ultra-high redshift galaxies ( 9 ≤ z ≤ 12 9\leq z\leq 12 ) in the JWST ERO SMACS 0723 Field, Monthly Notices of the Royal Astronomical Society 518
2022
Earlier work this paper cites.
R. P. Naidu, P. A. Oesch, P. van Dokkum, E. J. Nelson, K. A. Suess, G. Brammer, K. E. Whitaker, G. Illingworth, R. Bouwens, S. Tacchella, J. Matthee, N. Allen, R. Bezanson, C. Conroy, I. Labbe, J. Leja, E. Leonova, D. Magee, S. H. Price, D. J. Setton, V. Strait, M. Stefanon, S. Toft, J. R. Weaver, and A. Weibel, Two Remarkably Luminous Galaxy Candidates at z ≈ \approx 10-12 Revealed by JWST, apjl 940
Original
2022
Earlier work this paper cites.
C. C. Lovell, I. Harrison, Y. Harikane, S. Tacchella, and S. M. Wilkins, Extreme value statistics of the halo and stellar mass distributions at high redshift: are JWST results in tension with Λ \Lambda CDM?, Mon. Not. Roy. Astron. Soc. 518
Original
2022
Earlier work this paper cites.

Similar

B. Liu and V. Bromm, Accelerating Early Massive Galaxy Formation with Primordial Black Holes, Astrophys. J. Lett. 937
Original
2022
Cited alongside, same era.
M. Haslbauer, P. Kroupa, A. H. Zonoozi, and H. Haghi, Has JWST Already Falsified Dark-matter-driven Galaxy Formation?, Astrophys. J. Lett. 939
Original
2022
Cited alongside, same era.
P. Santini, N. Menci, and M. Castellano, CONSTRAINTS ON DARK ENERGY FROM THE ABUNDANCE OF MASSIVE GALAXIES, Frascati Phys. Ser. 74
Original
2022
Cited alongside, same era.
N. Menci, M. Castellano, P. Santini, E. Merlin, A. Fontana, and F. Shankar, High-redshift Galaxies from Early JWST Observations: Constraints on Dark Energy Models, Astrophys. J. Lett. 938
Original
2022
Cited alongside, same era.
L. Perivolaropoulos and F. Skara, Challenges for Λ \Lambda CDM: An update, New Astron. Rev. 95

Then

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Reading the bibliography…

2024

Do high redshift QSOs and GRBs corroborate JWST?

Colgáin, Eoin Ó, Sheikh-Jabbari, M. M., Yin, Lu

Understand

The James Webb Space Telescope (JWST) is reporting massive high redshift galaxies that appear challenging from the $\Lambda$CDM perspective.

Interpreted as a cosmological problem, this necessitates the Planck collaboration underestimating either matter density $\Omega_m$ or physical matter density $\Omega_m h^2$ at higher redshifts.
Through standard frequentist profile likelihoods, we identify corroborating quasar (QSO) and gamma-ray burst (GRB) data sets where $\Omega_m$ increases with effective redshift $z_{\textrm{eff}}$ and remains anomalously large at higher redshifts.
We relax the traditional priors by allowing for $\Omega_m > 1$, consistent with negative dark energy density, to locate profile likelihood peaks where possible.

Built on

P. Agrawal, F.-Y. Cyr-Racine, D. Pinner, and L. Randall, Rock ‘n’ roll solutions to the Hubble tension, Phys. Dark Univ. 42
Original
1904
Earlier work this paper cites.
M.-X. Lin, G. Benevento, W. Hu, and M. Raveri, Acoustic Dark Energy: Potential Conversion of the Hubble Tension, Phys. Rev. D 100
Original
1905
Earlier work this paper cites.
R. Arcodia, A. Merloni, K. Nandra, and G. Ponti, Testing the disk-corona interplay in radiatively-efficient broad-line AGN, Astron. Astrophys. 628
Original
1907
Earlier work this paper cites.
E. Lusso, E. Piedipalumbo, G. Risaliti, M. Paolillo, S. Bisogni, E. Nardini, and L. Amati, Tension with the flat Λ \Lambda CDM model from a high-redshift Hubble diagram of supernovae, quasars, and gamma-ray bursts, Astron. Astrophys. 628
Original
1907
Earlier work this paper cites.
L. Knox and M. Millea, Hubble constant hunter’s guide, Phys. Rev. D 101
Original
1908
Earlier work this paper cites.
F. Salvestrini, G. Risaliti, S. Bisogni, E. Lusso, and C. Vignali, Quasars as standard candles II: The non linear relation between UV and X-ray emission at high redshifts, Astron. Astrophys. 631
Original
1909
Earlier work this paper cites.
F. Niedermann and M. S. Sloth, New early dark energy, Phys. Rev. D 103
Original
1910
Earlier work this paper cites.
A. Lewis, Getdist: a python package for analysing monte carlo samples (2019), arXiv:1910.13970 [astro-ph.IM]
Original
1910
Earlier work this paper cites.
T. Yang, A. Banerjee, and E. Ó Colgáin, Cosmography and flat Λ \Lambda CDM tensions at high redshift, Phys. Rev. D 102
Original
1911
Earlier work this paper cites.
H. Velten and S. Gomes, Is the Hubble diagram of quasars in tension with concordance cosmology?, Phys. Rev. D 101
Original
1911
Earlier work this paper cites.
S. S. Wilks, The Large-Sample Distribution of the Likelihood Ratio for Testing Composite Hypotheses, The Annals of Mathematical Statistics 9
1938
Earlier work this paper cites.
S. Weinberg, The Cosmological Constant Problem, Rev. Mod. Phys. 61
1989
Earlier work this paper cites.
G. J. Feldman and R. D. Cousins, A Unified approach to the classical statistical analysis of small signals, Phys. Rev. D 57
1998
Earlier work this paper cites.
R. K. Sheth and G. Tormen, Large scale bias and the peak background split, Mon. Not. Roy. Astron. Soc. 308
1999
Earlier work this paper cites.
G. Ye and Y.-S. Piao, Is the Hubble tension a hint of AdS phase around recombination?, Phys. Rev. D 101
Original
2001
Earlier work this paper cites.
L. Amati et al. , Intrinsic spectra and energetics of BeppoSAX gamma-ray bursts with known redshifts, Astron. Astrophys. 390
2002
Earlier work this paper cites.
C. Vignali, W. N. Brandt, and D. P. Schneider, X-ray emission from radio - quiet quasars in the SDSS Early Data Release. The Alpha(ox) dependence upon UV luminosity, Astron. J. 125
2003
Earlier work this paper cites.
N. Khadka and B. Ratra, Using quasar X-ray and UV flux measurements to constrain cosmological model parameters, Mon. Not. Roy. Astron. Soc. 497
Original
2004
Earlier work this paper cites.
D. W. Just, W. N. Brandt, O. Shemmer, A. T. Steffen, D. P. Schneider, G. Chartas, and G. P. Garmire, The X-ray Properties of the Most-Luminous Quasars from the Sloan Digital Sky Survey, Astrophys. J. 665
Original
2007
Earlier work this paper cites.
S. Alam et al. (eBOSS), Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Cosmological implications from two decades of spectroscopic surveys at the Apache Point Observatory, Phys. Rev. D 103
Original
2007
Earlier work this paper cites.
E. Lusso et al. , Quasars as standard candles III. Validation of a new sample for cosmological studies, Astron. Astrophys. 642
Original
2008
Earlier work this paper cites.
K. Jedamzik, L. Pogosian, and G.-B. Zhao, Why reducing the cosmic sound horizon alone can not fully resolve the Hubble tension, Commun. in Phys. 4
Original
2010
Earlier work this paper cites.
E. Lusso, A. Comastri, C. Vignali, G. Zamorani, M. Brusa, R. Gilli, K. Iwasawa, M. Salvato, F. Civano, M. Elvis, A. Merloni, A. Bongiorno, J. R. Trump, A. M. Koekemoer, E. Schinnerer, E. Le Floc’h, N. Cappelluti, K. Jahnke, M. Sargent, J. Silverman, V. Mainieri, F. Fiore, M. Bolzonella, O. Le Fèvre, B. Garilli, A. Iovino, J. P. Kneib, F. Lamareille, S. Lilly, M. Mignoli, M. Scodeggio, and D. Vergani, The x-ray to optical-uv luminosity ratio of x-ray selected type 1 agn in xmm-cosmos, Astronomy and Astrophysics 512
2010
Earlier work this paper cites.
O. Luongo and M. Muccino, Model-independent calibrations of gamma-ray bursts using machine learning, Mon. Not. Roy. Astron. Soc. 503
Original
2011
Earlier work this paper cites.
N. Khadka and B. Ratra, Determining the range of validity of quasar X-ray and UV flux measurements for constraining cosmological model parameters, Mon. Not. Roy. Astron. Soc. 502
Original
2012
Earlier work this paper cites.
D. Foreman-Mackey, D. W. Hogg, D. Lang, and J. Goodman, emcee: The MCMC Hammer, Publ. Astron. Soc. Pac. 125
Original
2013
Earlier work this paper cites.
G. Risaliti and E. Lusso, A Hubble Diagram for Quasars, Astrophys. J. 815
Original
2015
Earlier work this paper cites.
G. Dvali and C. Gomez, Quantum Exclusion of Positive Cosmological Constant?, Annalen Phys. 528
Original
2016
Earlier work this paper cites.
R. Trotta, Bayesian Methods in Cosmology (2017) arXiv:1701.01467 [astro-ph.CO]
Original
2017
Earlier work this paper cites.
E. Lusso and G. Risaliti, Quasars as standard candles I: The physical relation between disc and coronal emission, Astron. Astrophys. 602
Original
2017
Earlier work this paper cites.
G. Obied, H. Ooguri, L. Spodyneiko, and C. Vafa, De Sitter Space and the Swampland, arXiv e-prints , arXiv:1806.08362 (2018) , arXiv:1806.08362 [hep-th]
Original
2018
Earlier work this paper cites.
A. Kubota and C. Done, A physical model of the broad-band continuum of AGN and its implications for the UV/X relation and optical variability, Mon. Not. Roy. Astron. Soc. 480
Original
2018
Earlier work this paper cites.
V. Poulin, T. L. Smith, T. Karwal, and M. Kamionkowski, Early Dark Energy Can Resolve The Hubble Tension, Phys. Rev. Lett. 122
Original
2019
Earlier work this paper cites.
G. Risaliti and E. Lusso, Cosmological constraints from the Hubble diagram of quasars at high redshifts, Nature Astron. 3
Original
2019
Earlier work this paper cites.
G. Dvali and C. Gomez, On Exclusion of Positive Cosmological Constant, Fortsch. Phys. 67
Original
2019
Earlier work this paper cites.
E. Di Valentino, O. Mena, S. Pan, L. Visinelli, W. Yang, A. Melchiorri, D. F. Mota, A. G. Riess, and J. Silk, In the realm of the Hubble tension—a review of solutions, Class. Quant. Grav. 38
Original
2021
Earlier work this paper cites.
N. Aghanim et al. (Planck), Planck 2018 results. VI. Cosmological parameters, Astron. Astrophys. 641
Original
2021
Earlier work this paper cites.
S. Bisogni, E. Lusso, F. Civano, E. Nardini, G. Risaliti, M. Elvis, and G. Fabbiano, The Chandra view of the relation between X-ray and UV emission in quasars, Astron. Astrophys. 655
Original
2021
Earlier work this paper cites.
N. J. Adams, C. J. Conselice, L. Ferreira, D. Austin, J. A. A. Trussler, I. Juodžbalis, S. M. Wilkins, J. Caruana, P. Dayal, A. Verma, and A. P. Vijayan, Discovery and properties of ultra-high redshift galaxies ( 9 ≤ z ≤ 12 9\leq z\leq 12 ) in the JWST ERO SMACS 0723 Field, Monthly Notices of the Royal Astronomical Society 518
2022
Earlier work this paper cites.
R. P. Naidu, P. A. Oesch, P. van Dokkum, E. J. Nelson, K. A. Suess, G. Brammer, K. E. Whitaker, G. Illingworth, R. Bouwens, S. Tacchella, J. Matthee, N. Allen, R. Bezanson, C. Conroy, I. Labbe, J. Leja, E. Leonova, D. Magee, S. H. Price, D. J. Setton, V. Strait, M. Stefanon, S. Toft, J. R. Weaver, and A. Weibel, Two Remarkably Luminous Galaxy Candidates at z ≈ \approx 10-12 Revealed by JWST, apjl 940
Original
2022
Earlier work this paper cites.
C. C. Lovell, I. Harrison, Y. Harikane, S. Tacchella, and S. M. Wilkins, Extreme value statistics of the halo and stellar mass distributions at high redshift: are JWST results in tension with Λ \Lambda CDM?, Mon. Not. Roy. Astron. Soc. 518
Original
2022
Earlier work this paper cites.

Similar

B. Liu and V. Bromm, Accelerating Early Massive Galaxy Formation with Primordial Black Holes, Astrophys. J. Lett. 937
Original
2022
Cited alongside, same era.
M. Haslbauer, P. Kroupa, A. H. Zonoozi, and H. Haghi, Has JWST Already Falsified Dark-matter-driven Galaxy Formation?, Astrophys. J. Lett. 939
Original
2022
Cited alongside, same era.
P. Santini, N. Menci, and M. Castellano, CONSTRAINTS ON DARK ENERGY FROM THE ABUNDANCE OF MASSIVE GALAXIES, Frascati Phys. Ser. 74
Original
2022
Cited alongside, same era.
N. Menci, M. Castellano, P. Santini, E. Merlin, A. Fontana, and F. Shankar, High-redshift Galaxies from Early JWST Observations: Constraints on Dark Energy Models, Astrophys. J. Lett. 938
Original
2022
Cited alongside, same era.
L. Perivolaropoulos and F. Skara, Challenges for Λ \Lambda CDM: An update, New Astron. Rev. 95

Then

Beyond the bibliography

alphaXiv searches the wider corpus for related work and actual follow-ups.

Open on alphaXiv

alphaXiv is searching for related work…

Original

2022

Cited alongside, same era.

E. Abdalla et al. , Cosmology intertwined: A review of the particle physics, astrophysics, and cosmology associated with the cosmological tensions and anomalies, JHEAp 34

Original

2022

Cited alongside, same era.

N. Khadka and B. Ratra, Do quasar X-ray and UV flux measurements provide a useful test of cosmological models?, Mon. Not. Roy. Astron. Soc. 510

Original

2022

Cited alongside, same era.

J. Singal, S. Mutchnick, and V. Petrosian, The X-Ray Luminosity Function Evolution of Quasars and the Correlation between the X-Ray and Ultraviolet Luminosities, Astrophys. J. 932

Original

2022

Cited alongside, same era.

V. Petrosian, J. Singal, and S. Mutchnick, Can the Distance-Redshift Relation be Determined from Correlations between Luminosities?, Astrophys. J. Lett. 935

Original

2022

Cited alongside, same era.

A. Gómez-Valent, Fast test to assess the impact of marginalization in Monte Carlo analyses and its application to cosmology, Phys. Rev. D 106

Original

2022

Cited alongside, same era.

L. Herold, E. G. M. Ferreira, and E. Komatsu, New Constraint on Early Dark Energy from Planck and BOSS Data Using the Profile Likelihood, Astrophys. J. Lett. 929

Original

2022

Cited alongside, same era.

E. Ó Colgáin, M. M. Sheikh-Jabbari, R. Solomon, G. Bargiacchi, S. Capozziello, M. G. Dainotti, and D. Stojkovic, Revealing intrinsic flat Λ \Lambda CDM biases with standardizable candles, Phys. Rev. D 106

Original

2022

Cited alongside, same era.

Later among the works it cites.

J. McCaffrey, S. Hardin, J. H. Wise, and J. A. Regan, No tension: Jwst galaxies at z > 10 z>10 consistent with cosmological simulations, The Open Journal of Astrophysics 6

2023

Later among the works it cites.

V. Poulin, T. L. Smith, and T. Karwal, The Ups and Downs of Early Dark Energy solutions to the Hubble tension: A review of models, hints and constraints circa 2023, Phys. Dark Univ. 42

Original

2023

Later among the works it cites.

M. Boylan-Kolchin, Stress testing Λ \Lambda CDM with high-redshift galaxy candidates, Nature Astron. 7

Original

2023

Later among the works it cites.

N. Khadka, M. Zajaček, R. Prince, S. Panda, B. Czerny, M. L. Martínez-Aldama, V. K. Jaiswal, and B. Ratra, Quasar UV/X-ray relation luminosity distances are shorter than reverberation-measured radius–luminosity relation luminosity distances, Mon. Not. Roy. Astron. Soc. 522

Original