-
[1]
D. Hutsemekers, R. Cabanac, H. Lamy et al., Astron. Astrophys. 441, 915 (2005)
-
[2]
J. A. King, J. K. Webb, M. T. Murphy et al., Mon. Not. Roy. Astron. Soc. 422, 3370 (2012)
-
[3]
A. Mariano and L. Perivolaropoulos, Phys. Rev. D 86, 083517 (2012)
-
[4]
C. H. Lineweaver, L. Tenorio, G. F. Smoot et al., Astrophys. J. 470, 38 (1996)
-
[5]
M. Tegmark, A. de Oliveira-Costa, and A. Hamilton, Phys. Rev. D 68, 123523 (2003)
-
[6]
M. Frommert and T. A. Enßlin, PoS Cosmology 2009, 015 (2009)
-
[7]
A. G. Riess et al., Astrophys. J. 855(2), 136 (2018)
-
[8]
A. G. Riess et al., Astrophys. J. Lett. 934(1), L7 (2022)
-
[9]
N. Aghanim et al. (Planck Collaboration), Astron. Astrophys. 641 , A6 (2020) [Erratum: Astron. Astrophys. 652 , C4 (2021)]
-
[10]
E. Aubourg et al., Phys. Rev. D 92(12), 123516 (2015)
-
[11]
A. Cuceu, J. Farr, P. Lemos et al., Present and Future, JCAP 2019(10), 044 (2019)
-
[12]
O. H. E. Philcox, M. M. Ivanov, M. Simonović et al., JCAP 2020(05), 032 (2020)
-
[13]
A. G. Riess, S. Casertano, W. Yuan et al., Astrophys. J. 876(1), 85 (2019)
-
[14]
T. M. C. Abbott et al., Phys. Rev. D 98(4), 043526 (2018)
-
[15]
B. P. Abbott et al., Nature 551(7678), 85 (2017)
-
[16]
A. Kozmanyan, H. Bourdin, P. Mazzotta et al., Astron. Astrophys. 621, A34 (2019)
-
[17]
A. Domínguez, R. Wojtak, J. Finke et al., A new measurement of the Hubble constant and matter content of the Universe using extragalactic background light γ-ray attenuation
-
[18]
M. Soares-Santos et al., Astrophys. J. Lett. 876(1), L7 (2019)
-
[19]
S. H. Suyu et al., Mon. Not. Roy. Astron. Soc. 468(3), 2590 (2017)
-
[20]
S. Birrer et al., Mon. Not. Roy. Astron. Soc. 484, 4726 (2019)
-
[21]
K. C. Wong et al., Mon. Not. Roy. Astron. Soc. 498(1), 1420 (2020)
-
[22]
S. H. Suyu, P. J. Marshall, M. W. Auger et al., Astrophys. J. 711, 201 (2010)
-
[23]
S. H. Suyu et al., Astrophys. J. Lett. 788, L35 (2014)
-
[24]
K. C. Wong et al., Mon. Not. Roy. Astron. Soc. 465(4), 4895 (2017)
-
[25]
I. Jee, S. Suyu, E. Komatsu, C. D. Fassnacht et al., A measurement of the Hubble constant from angular diameter distances to two gravitational lenses
-
[26]
G. C. F. Chen et al., Mon. Not. Roy. Astron. Soc. 490(2), 1743 (2019)
-
[27]
C. E. Rusu et al., Mon. Not. Roy. Astron. Soc. 498(1), 1440 (2020)
-
[28]
A. Agnello et al., Mon. Not. Roy. Astron. Soc. 472(4), 4038 (2017)
-
[29]
A. J. Shajib et al., Mon. Not. Roy. Astron. Soc. 494(4), 6072 (2020)
-
[30]
L. F. Wang, J. H. Zhang, D. Z. He et al., Mon. Not. Roy. Astron. Soc. 514(1), 1433 (2022)
-
[31]
M. Millon et al., Astron. Astrophys. 639, A101 (2020)
-
[32]
S. Birrer et al., Astron. Astrophys. 643, A165 (2020)
-
[33]
T. Collett, F. Montanari, and S. Rasanen, Phys. Rev. Lett. 123(23), 231101 (2019)
-
[34]
K. Liao, A. Shafieloo, R. E. Keeley et al., Astrophys. J. Lett. 886(1), L23 (2019)
-
[35]
K. Liao, A. Shafieloo, R. E. Keeley et al., Astrophys. J. Lett. 895(2), L29 (2020)
-
[36]
C. Escamilla-Rivera, M. A. C. Quintero, and S. Capozziello, JCAP 2020(03), 008 (2020)
-
[37]
L. Tang, X. Li, H. N. Lin et al., Astrophys. J. 907(2), 121 (2021)
-
[38]
L. Liu, L. J. Hu, L. Tang et al., Res. Astron. Astrophys. 23(12), 125012 (2023)
-
[39]
J. Z. Qi, P. Meng, J. F. Zhang et al., Phys. Rev. D 108(6), 063522 (2023)
-
[40]
D. M. Scolnic et al., Astrophys. J. 859(2), 101 (2018)
-
[41]
S. Refsdal, Mon. Not. Roy. Astron. Soc. 128(4), 307 (1964)
-
[42]
M. Bartelmann and P. Schneider, Phys. Rept. 340, 291 (2001)
-
[43]
L. Tang, H. N. Lin, and Y. Wu, Chin. Phys. C 49, 015104 (2025)
-
[44]
D. Scolnic et al., Astrophys. J. 938(2), 113 (2022)
-
[45]
Y. Gal and Z. Ghahramani, Dropout as a Bayesian Approximation: Representing Model Uncertainty in Deep Learning, arXiv: 1506.02142
-
[46]
G. J. Wang, X. J. Ma, S. Y. Li et al., Astrophys. J. Suppl. 246(1), 13 (2020)
-
[47]
F. Pedregosa, G. Varoquaux, A. Gramfort et al., Journal of Machine Learning Research 12, 2825 (2011)
-
[48]
D. Foreman-Mackey, D. W. Hogg, D. Lang et al., Publ. Astron. Soc. Pac. 125, 306 (2013)
-
[49]
X. Li, R. E. Keeley, A. Shafieloo et al., Astrophys. J. 960(2), 103 (2024)
-
[50]
M. Oguri and P. J. Marshall, Mon. Not. Roy. Astron. Soc. 405, 2579 (2010)