Built on

W. D. Kenworthy, D. Scolnic, and A. Riess, “The Local Perspective on the Hubble Tension: Local Structure Does Not Impact Measurement of the Hubble Constant,” Astrophys. J
Original
1901
Earlier work this paper cites.
C. D. Kreisch, F.-Y. Cyr-Racine, and O. Doré, “Neutrino puzzle: Anomalies, interactions, and cosmological tensions,” Phys. Rev. D
Original
1902
Earlier work this paper cites.
R. Jimenez, A. Cimatti, L. Verde, M. Moresco, and B. Wandelt, “The local and distant Universe: stellar ages and H 0 H_{0} ,” JCAP
Original
1902
Earlier work this paper cites.
A. G. Riess, S. Casertano, W. Yuan, L. M. Macri, and D. Scolnic, “Large Magellanic Cloud Cepheid Standards Provide a 1% Foundation for the Determination of the Hubble Constant and Stronger Evidence for Physics Beyond LambdaCDM,” Astrophys. J
Original
1903
Earlier work this paper cites.
A. Domínguez, R. Wojtak, J. Finke, M. Ajello, K. Helgason, F. Prada, A. Desai, V. Paliya, L. Marcotulli, and D. Hartmann, “A new measurement of the Hubble constant and matter content of the Universe using extragalactic background light γ \gamma -ray attenuation,” Astrophys. J
Original
1903
Earlier work this paper cites.
P. Agrawal, F.-Y. Cyr-Racine, D. Pinner, and L. Randall, “Rock ’n’ Roll Solutions to the Hubble Tension,” arXiv:1904.01016 [astro-ph.CO]
Original
1904
Earlier work this paper cites.
V. de Sainte Agathe et al
Original
1904
Earlier work this paper cites.
M. Blomqvist et al
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
Original
1905
Earlier work this paper cites.
A. Cuceu, J. Farr, P. Lemos, and A. Font-Ribera, “Baryon Acoustic Oscillations and the Hubble Constant: Past, Present and Future,” JCAP
Original
1906
Earlier work this paper cites.
J.-M. Wang, Y.-Y. Songsheng, Y.-R. Li, P. Du, and Z.-X. Zhang, “A parallax distance to 3C 273 through spectroastrometry and reverberation mapping,” Nature Astron
Original
1906
Earlier work this paper cites.
N. Schöneberg, J. Lesgourgues, and D. C. Hooper, “The BAO+BBN take on the Hubble tension,” JCAP
Original
1907
Earlier work this paper cites.
W. L. Freedman et al
Original
1907
Earlier work this paper cites.
K. C. Wong et al
Original
1907
Earlier work this paper cites.
V. V. Luković, B. S. Haridasu, and N. Vittorio, “Exploring the evidence for a large local void with supernovae Ia data,” Mon. Not. Roy. Astron. Soc
Original
1907
Earlier work this paper cites.
J. Sakstein, H. Desmond, and B. Jain, “Screened Fifth Forces Mediated by Dark Matter–Baryon Interactions: Theory and Astrophysical Probes,” Phys. Rev. D
Original
1907
Earlier work this paper cites.
S. Vagnozzi, “New physics in light of the H 0 H_{0} tension: An alternative view,” Phys. Rev
Original
1907
Earlier work this paper cites.
L. Knox and M. Millea, “Hubble constant hunter’s guide,” Phys. Rev
Original
1908
Earlier work this paper cites.
W. Yuan, A. G. Riess, L. M. Macri, S. Casertano, and D. Scolnic, “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,” Astrophys. J
Original
1908
Earlier work this paper cites.
C. D. Huang, A. G. Riess, W. Yuan, L. M. Macri, N. L. Zakamska, S. Casertano, P. A. Whitelock, S. L. Hoffmann, A. V. Filippenko, and D. Scolnic, “Hubble Space Telescope Observations of Mira Variables in the Type Ia Supernova Host NGC 1559: An Alternative Candle to Measure the Hubble Constant,” Astrophys. J
Original
1908
Earlier work this paper cites.
LIGO Scientific, Virgo
Original
1908
Earlier work this paper cites.
T. L. Smith, V. Poulin, and M. A. Amin, “Oscillating scalar fields and the Hubble tension: a resolution with novel signatures,” Phys. Rev. D
Original
1908
Earlier work this paper cites.
S. Mukherjee, G. Lavaux, F. R. Bouchet, J. Jasche, B. D. Wandelt, S. M. Nissanke, F. Leclercq, and K. Hotokezaka, “Velocity correction for Hubble constant measurements from standard sirens,” Astron. Astrophys
Original
1909
Earlier work this paper cites.
N. Arendse et al
Original
1909
Earlier work this paper cites.
J. Solà Peracaula, A. Gomez-Valent, J. de Cruz Pérez, and C. Moreno-Pulido, “Brans–Dicke Gravity with a Cosmological Constant Smoothes Out Λ \Lambda CDM Tensions,” Astrophys. J. Lett
Original
1909
Earlier work this paper cites.
F. Niedermann and M. S. Sloth, “New early dark energy,” Phys. Rev. D
Original
1910
Earlier work this paper cites.
K. V. Berghaus and T. Karwal, “Thermal Friction as a Solution to the Hubble Tension,” Phys. Rev. D
Original
1911
Earlier work this paper cites.
J. Sakstein and M. Trodden, “Early Dark Energy from Massive Neutrinos as a Natural Resolution of the Hubble Tension,” Phys. Rev. Lett
Original
1911
Earlier work this paper cites.
L. Hart and J. Chluba, “Updated fundamental constant constraints from Planck 2018 data and possible relations to the Hubble tension,” Mon. Not. Roy. Astron. Soc
Original
1912
Earlier work this paper cites.
M. Liu, Z. Huang, X. Luo, H. Miao, N. K. Singh, and L. Huang, “Can Non-standard Recombination Resolve the Hubble Tension?,” Sci. China Phys. Mech. Astron
Original
1912
Earlier work this paper cites.
G. Schwarz, “Estimating the Dimension of a Model,” Annals Statist
1978
Earlier work this paper cites.
D. W. Pesce et al
Original
2001
Earlier work this paper cites.
A. G. Riess, “The Expansion of the Universe is Faster than Expected,” Nature Rev. Phys
Original
2001
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
Original
2001
Earlier work this paper cites.
S. Dhawan, D. Brout, D. Scolnic, A. Goobar, A. G. Riess, and V. Miranda, “Cosmological Model Insensitivity of Local H 0 H_{0} from the Cepheid Distance Ladder,” Astrophys. J
Original
2001
Earlier work this paper cites.
Z. Huang, “Supernova Magnitude Evolution and PAge Approximation,” Astrophys. J. Lett
Original
2001
Earlier work this paper cites.
M. Chevallier and D. Polarski, “Accelerating universes with scaling dark matter,” Int. J. Mod. Phys. D
2001
Earlier work this paper cites.
O. H. E. Philcox, M. M. Ivanov, M. Simonović, and M. Zaldarriaga, “Combining Full-Shape and BAO Analyses of Galaxy Power Spectra: A 1.6% CMB-independent constraint on H 0 ,” JCAP
Original
2002
Earlier work this paper cites.
W. L. Freedman, B. F. Madore, T. Hoyt, I. S. Jang, R. Beaton, M. G. Lee, A. Monson, J. Neeley, and J. Rich, “Calibration of the Tip of the Red Giant Branch (TRGB),” Astrophys. J
Original
2002
Earlier work this paper cites.
G. Benevento, W. Hu, and M. Raveri, “Can Late Dark Energy Transitions Raise the Hubble constant?,” Phys. Rev
Original
2002
Earlier work this paper cites.
R. Jimenez and A. Loeb, “Constraining cosmological parameters based on relative galaxy ages,” Astrophys. J
2002
Earlier work this paper cites.
G. D’Amico, L. Senatore, and P. Zhang, “Limits on w w CDM from the EFTofLSS with the PyBird code,” JCAP
Original
2003
Earlier work this paper cites.
J. C. Hill, E. McDonough, M. W. Toomey, and S. Alexander, “Early dark energy does not restore cosmological concordance,” Phys. Rev
Original
2003
Earlier work this paper cites.
E. V. Linder, “Exploring the expansion history of the universe,” Phys. Rev. Lett
2003
Earlier work this paper cites.
G. Bruzual and S. Charlot, “Stellar population synthesis at the resolution of 2003,” Mon. Not. Roy. Astron. Soc
2003
Earlier work this paper cites.
J.-F. Le Borgne, G. Bruzual A., R. Pello, A. Lancon, B. Rocca-Volmerange, B. Sanahuja, D. Schaerer, C. Soubiran, and R. Vilchez-Gomez, “STELIB: A Library of stellar spectra at R~2000,” Astron. Astrophys
2003
Earlier work this paper cites.
H. Desmond and J. Sakstein, “Screened fifth forces lower the TRGB-calibrated Hubble constant too,” Phys. Rev. D
Original
2003
Earlier work this paper cites.
E. Kourkchi, R. B. Tully, G. S. Anand, H. M. Courtois, A. Dupuy, J. D. Neill, L. Rizzi, and M. Seibert, “Cosmicflows-4: The Calibration of Optical and Infrared Tully–Fisher Relations,” Astrophys. J
Original
2004
Earlier work this paper cites.
A. Chudaykin, D. Gorbunov, and N. Nedelko, “Combined analysis of Planck and SPTPol data favors the early dark energy models,” JCAP
Original
2004
Earlier work this paper cites.
K. Jedamzik and L. Pogosian, “Relieving the Hubble tension with primordial magnetic fields,” Phys. Rev. Lett
Original
2004
Earlier work this paper cites.

Similar

M. Visser, “Jerk and the cosmological equation of state,” Class. Quant. Grav
2004
Cited alongside, same era.
J. Schombert, S. McGaugh, and F. Lelli, “Using the Baryonic Tully–Fisher Relation to Measure H o,” Astron. J
Original
2006
Cited alongside, same era.
M. Gonzalez, M. P. Hertzberg, and F. Rompineve, “Ultralight Scalar Decay and the Hubble Tension,” JCAP
Original
2006
Cited alongside, same era.
M. M. Ivanov, E. McDonough, J. C. Hill, M. Simonović, M. W. Toomey, S. Alexander, and M. Zaldarriaga, “Constraining Early Dark Energy with Large-Scale Structure,” Phys. Rev
Original
2006
Cited alongside, same era.
G. D’Amico, L. Senatore, P. Zhang, and H. Zheng, “The Hubble Tension in Light of the Full-Shape Analysis of Large-Scale Structure Data,” JCAP
Original

Then

I. Odderskov, S. Hannestad, and T. Haugbølle, “On the local variation of the Hubble constant,” JCAP
Original
2014
Later among the works it cites.
E. Aubourg et al
Original
2015
Later among the works it cites.
A. J. Cuesta, L. Verde, A. Riess, and R. Jimenez, “Calibrating the cosmic distance scale ladder: the role of the sound horizon scale and the local expansion rate as distance anchors,” Mon. Not. Roy. Astron. Soc
Original
2015
Later among the works it cites.
A. J. Ross, L. Samushia, C. Howlett, W. J. Percival, A. Burden, and M. Manera, “The clustering of the SDSS DR7 main Galaxy sample – I. A 4 per cent distance measure at z = 0.15 z=0.15 ,” Mon. Not. Roy. Astron. Soc
Original
2015
Later among the works it cites.
M. Moresco, “Raising the bar: new constraints on the Hubble parameter with cosmic chronometers at z ∼ \sim 2,” Mon. Not. Roy. Astron. Soc

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

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2021

No-go guide for the Hubble tension : Late-time solutions

Cai, Rong-Gen, Guo, Zong-Kuan, Wang, Shao-Jiang et al.

Understand

The Hubble tension, if not caused by any systematics, could be relieved or even resolved from modifying either the early-time or late-time Universe.

The early-time modifications are usually in tension with either galaxy clustering or galaxy lensing constraints.
The late-time modifications are also in conflict with the constraint from the inverse distance ladder, which, however, is weakened by the dependence on a sound-horizon prior and some particular approximation for the late-time expansion history.
To achieve a more general no-go argument for the late-time scenarios, we propose to use a global parametrizationbased on the cosmic age (PAge) to consistently use the cosmic chronometers data beyond the Taylor expansion domain and without the input of a sound-horizon prior.

Built on

W. D. Kenworthy, D. Scolnic, and A. Riess, “The Local Perspective on the Hubble Tension: Local Structure Does Not Impact Measurement of the Hubble Constant,” Astrophys. J
Original
1901
Earlier work this paper cites.
C. D. Kreisch, F.-Y. Cyr-Racine, and O. Doré, “Neutrino puzzle: Anomalies, interactions, and cosmological tensions,” Phys. Rev. D
Original
1902
Earlier work this paper cites.
R. Jimenez, A. Cimatti, L. Verde, M. Moresco, and B. Wandelt, “The local and distant Universe: stellar ages and H 0 H_{0} ,” JCAP
Original
1902
Earlier work this paper cites.
A. G. Riess, S. Casertano, W. Yuan, L. M. Macri, and D. Scolnic, “Large Magellanic Cloud Cepheid Standards Provide a 1% Foundation for the Determination of the Hubble Constant and Stronger Evidence for Physics Beyond LambdaCDM,” Astrophys. J
Original
1903
Earlier work this paper cites.
A. Domínguez, R. Wojtak, J. Finke, M. Ajello, K. Helgason, F. Prada, A. Desai, V. Paliya, L. Marcotulli, and D. Hartmann, “A new measurement of the Hubble constant and matter content of the Universe using extragalactic background light γ \gamma -ray attenuation,” Astrophys. J
Original
1903
Earlier work this paper cites.
P. Agrawal, F.-Y. Cyr-Racine, D. Pinner, and L. Randall, “Rock ’n’ Roll Solutions to the Hubble Tension,” arXiv:1904.01016 [astro-ph.CO]
Original
1904
Earlier work this paper cites.
V. de Sainte Agathe et al
Original
1904
Earlier work this paper cites.
M. Blomqvist et al
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
Original
1905
Earlier work this paper cites.
A. Cuceu, J. Farr, P. Lemos, and A. Font-Ribera, “Baryon Acoustic Oscillations and the Hubble Constant: Past, Present and Future,” JCAP
Original
1906
Earlier work this paper cites.
J.-M. Wang, Y.-Y. Songsheng, Y.-R. Li, P. Du, and Z.-X. Zhang, “A parallax distance to 3C 273 through spectroastrometry and reverberation mapping,” Nature Astron
Original
1906
Earlier work this paper cites.
N. Schöneberg, J. Lesgourgues, and D. C. Hooper, “The BAO+BBN take on the Hubble tension,” JCAP
Original
1907
Earlier work this paper cites.
W. L. Freedman et al
Original
1907
Earlier work this paper cites.
K. C. Wong et al
Original
1907
Earlier work this paper cites.
V. V. Luković, B. S. Haridasu, and N. Vittorio, “Exploring the evidence for a large local void with supernovae Ia data,” Mon. Not. Roy. Astron. Soc
Original
1907
Earlier work this paper cites.
J. Sakstein, H. Desmond, and B. Jain, “Screened Fifth Forces Mediated by Dark Matter–Baryon Interactions: Theory and Astrophysical Probes,” Phys. Rev. D
Original
1907
Earlier work this paper cites.
S. Vagnozzi, “New physics in light of the H 0 H_{0} tension: An alternative view,” Phys. Rev
Original
1907
Earlier work this paper cites.
L. Knox and M. Millea, “Hubble constant hunter’s guide,” Phys. Rev
Original
1908
Earlier work this paper cites.
W. Yuan, A. G. Riess, L. M. Macri, S. Casertano, and D. Scolnic, “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,” Astrophys. J
Original
1908
Earlier work this paper cites.
C. D. Huang, A. G. Riess, W. Yuan, L. M. Macri, N. L. Zakamska, S. Casertano, P. A. Whitelock, S. L. Hoffmann, A. V. Filippenko, and D. Scolnic, “Hubble Space Telescope Observations of Mira Variables in the Type Ia Supernova Host NGC 1559: An Alternative Candle to Measure the Hubble Constant,” Astrophys. J
Original
1908
Earlier work this paper cites.
LIGO Scientific, Virgo
Original
1908
Earlier work this paper cites.
T. L. Smith, V. Poulin, and M. A. Amin, “Oscillating scalar fields and the Hubble tension: a resolution with novel signatures,” Phys. Rev. D
Original
1908
Earlier work this paper cites.
S. Mukherjee, G. Lavaux, F. R. Bouchet, J. Jasche, B. D. Wandelt, S. M. Nissanke, F. Leclercq, and K. Hotokezaka, “Velocity correction for Hubble constant measurements from standard sirens,” Astron. Astrophys
Original
1909
Earlier work this paper cites.
N. Arendse et al
Original
1909
Earlier work this paper cites.
J. Solà Peracaula, A. Gomez-Valent, J. de Cruz Pérez, and C. Moreno-Pulido, “Brans–Dicke Gravity with a Cosmological Constant Smoothes Out Λ \Lambda CDM Tensions,” Astrophys. J. Lett
Original
1909
Earlier work this paper cites.
F. Niedermann and M. S. Sloth, “New early dark energy,” Phys. Rev. D
Original
1910
Earlier work this paper cites.
K. V. Berghaus and T. Karwal, “Thermal Friction as a Solution to the Hubble Tension,” Phys. Rev. D
Original
1911
Earlier work this paper cites.
J. Sakstein and M. Trodden, “Early Dark Energy from Massive Neutrinos as a Natural Resolution of the Hubble Tension,” Phys. Rev. Lett
Original
1911
Earlier work this paper cites.
L. Hart and J. Chluba, “Updated fundamental constant constraints from Planck 2018 data and possible relations to the Hubble tension,” Mon. Not. Roy. Astron. Soc
Original
1912
Earlier work this paper cites.
M. Liu, Z. Huang, X. Luo, H. Miao, N. K. Singh, and L. Huang, “Can Non-standard Recombination Resolve the Hubble Tension?,” Sci. China Phys. Mech. Astron
Original
1912
Earlier work this paper cites.
G. Schwarz, “Estimating the Dimension of a Model,” Annals Statist
1978
Earlier work this paper cites.
D. W. Pesce et al
Original
2001
Earlier work this paper cites.
A. G. Riess, “The Expansion of the Universe is Faster than Expected,” Nature Rev. Phys
Original
2001
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
Original
2001
Earlier work this paper cites.
S. Dhawan, D. Brout, D. Scolnic, A. Goobar, A. G. Riess, and V. Miranda, “Cosmological Model Insensitivity of Local H 0 H_{0} from the Cepheid Distance Ladder,” Astrophys. J
Original
2001
Earlier work this paper cites.
Z. Huang, “Supernova Magnitude Evolution and PAge Approximation,” Astrophys. J. Lett
Original
2001
Earlier work this paper cites.
M. Chevallier and D. Polarski, “Accelerating universes with scaling dark matter,” Int. J. Mod. Phys. D
2001
Earlier work this paper cites.
O. H. E. Philcox, M. M. Ivanov, M. Simonović, and M. Zaldarriaga, “Combining Full-Shape and BAO Analyses of Galaxy Power Spectra: A 1.6% CMB-independent constraint on H 0 ,” JCAP
Original
2002
Earlier work this paper cites.
W. L. Freedman, B. F. Madore, T. Hoyt, I. S. Jang, R. Beaton, M. G. Lee, A. Monson, J. Neeley, and J. Rich, “Calibration of the Tip of the Red Giant Branch (TRGB),” Astrophys. J
Original
2002
Earlier work this paper cites.
G. Benevento, W. Hu, and M. Raveri, “Can Late Dark Energy Transitions Raise the Hubble constant?,” Phys. Rev
Original
2002
Earlier work this paper cites.
R. Jimenez and A. Loeb, “Constraining cosmological parameters based on relative galaxy ages,” Astrophys. J
2002
Earlier work this paper cites.
G. D’Amico, L. Senatore, and P. Zhang, “Limits on w w CDM from the EFTofLSS with the PyBird code,” JCAP
Original
2003
Earlier work this paper cites.
J. C. Hill, E. McDonough, M. W. Toomey, and S. Alexander, “Early dark energy does not restore cosmological concordance,” Phys. Rev
Original
2003
Earlier work this paper cites.
E. V. Linder, “Exploring the expansion history of the universe,” Phys. Rev. Lett
2003
Earlier work this paper cites.
G. Bruzual and S. Charlot, “Stellar population synthesis at the resolution of 2003,” Mon. Not. Roy. Astron. Soc
2003
Earlier work this paper cites.
J.-F. Le Borgne, G. Bruzual A., R. Pello, A. Lancon, B. Rocca-Volmerange, B. Sanahuja, D. Schaerer, C. Soubiran, and R. Vilchez-Gomez, “STELIB: A Library of stellar spectra at R~2000,” Astron. Astrophys
2003
Earlier work this paper cites.
H. Desmond and J. Sakstein, “Screened fifth forces lower the TRGB-calibrated Hubble constant too,” Phys. Rev. D
Original
2003
Earlier work this paper cites.
E. Kourkchi, R. B. Tully, G. S. Anand, H. M. Courtois, A. Dupuy, J. D. Neill, L. Rizzi, and M. Seibert, “Cosmicflows-4: The Calibration of Optical and Infrared Tully–Fisher Relations,” Astrophys. J
Original
2004
Earlier work this paper cites.
A. Chudaykin, D. Gorbunov, and N. Nedelko, “Combined analysis of Planck and SPTPol data favors the early dark energy models,” JCAP
Original
2004
Earlier work this paper cites.
K. Jedamzik and L. Pogosian, “Relieving the Hubble tension with primordial magnetic fields,” Phys. Rev. Lett
Original
2004
Earlier work this paper cites.

Similar

M. Visser, “Jerk and the cosmological equation of state,” Class. Quant. Grav
2004
Cited alongside, same era.
J. Schombert, S. McGaugh, and F. Lelli, “Using the Baryonic Tully–Fisher Relation to Measure H o,” Astron. J
Original
2006
Cited alongside, same era.
M. Gonzalez, M. P. Hertzberg, and F. Rompineve, “Ultralight Scalar Decay and the Hubble Tension,” JCAP
Original
2006
Cited alongside, same era.
M. M. Ivanov, E. McDonough, J. C. Hill, M. Simonović, M. W. Toomey, S. Alexander, and M. Zaldarriaga, “Constraining Early Dark Energy with Large-Scale Structure,” Phys. Rev
Original
2006
Cited alongside, same era.
G. D’Amico, L. Senatore, P. Zhang, and H. Zheng, “The Hubble Tension in Light of the Full-Shape Analysis of Large-Scale Structure Data,” JCAP
Original

Then

I. Odderskov, S. Hannestad, and T. Haugbølle, “On the local variation of the Hubble constant,” JCAP
Original
2014
Later among the works it cites.
E. Aubourg et al
Original
2015
Later among the works it cites.
A. J. Cuesta, L. Verde, A. Riess, and R. Jimenez, “Calibrating the cosmic distance scale ladder: the role of the sound horizon scale and the local expansion rate as distance anchors,” Mon. Not. Roy. Astron. Soc
Original
2015
Later among the works it cites.
A. J. Ross, L. Samushia, C. Howlett, W. J. Percival, A. Burden, and M. Manera, “The clustering of the SDSS DR7 main Galaxy sample – I. A 4 per cent distance measure at z = 0.15 z=0.15 ,” Mon. Not. Roy. Astron. Soc
Original
2015
Later among the works it cites.
M. Moresco, “Raising the bar: new constraints on the Hubble parameter with cosmic chronometers at z ∼ \sim 2,” Mon. Not. Roy. Astron. Soc

Beyond the bibliography

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

Open on alphaXiv

alphaXiv is searching for related work…

2006

Cited alongside, same era.

X. Zhang and Q.-G. Huang, “Hubble constant and sound horizon from the late-time Universe,” Phys. Rev. D

Original

2006

Cited alongside, same era.

P. Sanchez-Blazquez, R. Peletier, J. Jimenez-Vicente, N. Cardiel, A. J. Cenarro, J. Falcon-Barroso, J. Gorgas, S. Selam, and A. Vazdekis, “Medium-resolution Isaac Newton Telescope library of empirical spectra,” Mon. Not. Roy. Astron. Soc

2006

Cited alongside, same era.

J. Solà Peracaula, A. Gómez-Valent, J. de Cruz Pérez, and C. Moreno-Pulido, “Brans–Dicke cosmology with a Λ \Lambda -term: a possible solution to Λ \Lambda CDM tensions,” Class. Quant. Grav

Original

2006

Cited alongside, same era.

S. Birrer et al

Original

2007

Cited alongside, same era.

T. Sekiguchi and T. Takahashi, “Early recombination as a solution to the H 0 H_{0} tension,” Phys. Rev. D

Original