Open Access
Open access
volume 537 issue 2 pages 1818-1825

The Dark Energy Survey Supernova Program: An updated measurement of the Hubble constant using the Inverse Distance Ladder

R Camilleri 1
T.D Davis 1
S. R. Hinton 1
P. Armstrong 2
D. Brout 3, 4
L. Galbany 5, 6, 7, 8
K. Glazebrook 9, 10
J. Lee 11
C. Lidman 2, 12
A Möller 9, 10
R. C. Nichol 13
M. Sako 11
D. Scolnic 14
P. Shah 15, 16
M. Smith 17
M. Sullivan 17
B.O. Sánchez 14, 18, 19
M. Vincenzi 14
P. Wiseman 17
S. Allam 20
T. M. C. Abbott 21
M. Aguena 22, 23
F. Andrade-Oliveira 24
J. Asorey 25, 26
S. Avila 27, 28
D. Bacon 29
K. Bechtol 30
S Bocquet 31, 32
D. Brooks 15, 16
E. Buckley-Geer 20, 33
D. L. Burke 34, 35, 36
A. Carnero Rosell 22, 23, 37
D. Carollo 38
J. Carretero 27, 28
F. J. Castander 5, 6, 7, 8
C. Conselice 39, 40, 41
L. N. da Costa 22, 23
M. E. S. Pereira 42, 43
S. Desai 44
H. T. Diehl 20
S. Everett 45
I. Ferrero 46
B. Flaugher 20
J. Frieman 20, 47
J. García-Bellido 48, 49
E. Gaztanaga 5, 6, 7, 8, 29
G. Giannini 27, 28, 47
R. A. Gruendl 50, 51
K. Herner 20
D. L. Hollowood 52
K. Honscheid 53, 54
D. Huterer 24
D. J. James 3, 4
S. Kent 20, 47
K. Kuehn 55, 56
O. Lahav 15, 16
S ( Lee 45
G. F. Lewis 57
M. Lima 22, 23, 58
J. L. Marshall 59
J. Mena-Fernández 60, 61
R. Miquel 27, 28, 62
J. Myles 63
R. L. C. Ogando 64, 65
A. Palmese 66, 67
A. Pieres 22, 23, 64, 65
A. A. Plazas Malagón 34, 35
A. A. Plazas Malagón 35, 36
A. K. Romer 68
A. Roodman 34, 35, 36
S. Samuroff 69
E. Sanchez 70, 71
D Sanchez Cid 70
D. Sanchez Cid 71
M. Schubnell 24
I. Sevilla-Noarbe 70, 71
E. Suchyta 72
N. Suntzeff 59
M. E. C. Swanson 50
G. Tarle 24
B. E. Tucker 2
A. R. Walker 21
N. Weaverdyck 73, 74
8
 
Institute of Space Sciences (ICE, CSIC), Campus UAB, Carrer de Can Magrans , s/n, E-08193 Barcelona ,
21
 
Cerro Tololo Inter-American Observatory, NSF’s National Optical-Infrared Astronomy Research Laboratory , Casilla 603, La Serena ,
22
 
Laboratório Interinstitucional de e-Astronomia - LIneA , Rua Gal. José Cristino 77, Rio de Janeiro, RJ - 20921-400 ,
23
 
Laboratório Interinstitucional de e-Astronomia – LIneA , Rua Gal. José Cristino 77, Rio de Janeiro, RJ – 20921-400 ,
50
 
Center for Astrophysical Surveys, National Center for Supercomputing Applications , 1205 West Clark St., Urbana, IL 61801 ,
52
 
Santa Cruz Institute for Particle Physics , Santa Cruz, CA 95064 ,
56
 
Lowell Observatory , 1400 Mars Hill Rd, Flagstaff, AZ 86001 ,
60
 
LPSC Grenoble - 53 , Avenue des Martyrs 38026 Grenoble ,
61
 
LPSC Grenoble – 53 , Avenue des Martyrs, F-38026 Grenoble ,
64
 
Observatório Nacional , Rua Gal. José Cristino 77, Rio de Janeiro, RJ - 20921-400 ,
65
 
Observatório Nacional , Rua Gal. José Cristino 77, Rio de Janeiro, RJ – 20921-400 ,
Publication typeJournal Article
Publication date2025-01-23
scimago Q1
wos Q1
SJR1.702
CiteScore9.7
Impact factor4.8
ISSN00358711, 13652966, 13658711
Abstract
ABSTRACT

We measure the current expansion rate of the Universe, Hubble’s constant $H_0$, by calibrating the absolute magnitudes of supernovae to distances measured by baryon acoustic oscillations (BAO). This ‘inverse distance ladder’ technique provides an alternative to calibrating supernovae using nearby absolute distance measurements, replacing the calibration with a high-redshift anchor. We use the recent release of 1829 supernovae from the Dark Energy Survey spanning $0.01\lt z\lt 1.13$ anchored to the recent baryon acoustic oscillation measurements from Dark Energy Spectroscopic Instrument (DESI) spanning $0.30 \lt z_{\mathrm{eff}}\lt 2.33$. To trace cosmology to $z=0$, we use the third-, fourth-, and fifth-order cosmographic models, which, by design, are agnostic about the energy content and expansion history of the universe. With the inclusion of the higher redshift DESI-BAO data, the third-order model is a poor fit to both data sets, with the fourth-order model being preferred by the Akaike Information Criterion. Using the fourth-order cosmographic model, we find $H_0=67.19^{+0.66}_{-0.64}\mathrm{~km} \mathrm{~s}^{-1} \mathrm{~Mpc}^{-1}$, in agreement with the value found by Planck without the need to assume Flat-$\Lambda$CDM. However, the best-fitting expansion history differs from that of Planck, providing continued motivation to investigate these tensions.

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Camilleri R. et al. The Dark Energy Survey Supernova Program: An updated measurement of the Hubble constant using the Inverse Distance Ladder // Monthly Notices of the Royal Astronomical Society. 2025. Vol. 537. No. 2. pp. 1818-1825.
GOST all authors (up to 50) Copy
Camilleri R. et al. The Dark Energy Survey Supernova Program: An updated measurement of the Hubble constant using the Inverse Distance Ladder // Monthly Notices of the Royal Astronomical Society. 2025. Vol. 537. No. 2. pp. 1818-1825.
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@article{2025_Camilleri,
author = {R Camilleri and T.D Davis and S. R. Hinton and P. Armstrong and D. Brout and L. Galbany and K. Glazebrook and J. Lee and C. Lidman and A Möller and R. C. Nichol and M. Sako and D. Scolnic and P. Shah and M. Smith and M. Sullivan and B.O. Sánchez and M. Vincenzi and P. Wiseman and S. Allam and T. M. C. Abbott and M. Aguena and F. Andrade-Oliveira and J. Asorey and S. Avila and D. Bacon and K. Bechtol and S Bocquet and D. Brooks and E. Buckley-Geer and D. L. Burke and A. Carnero Rosell and D. Carollo and J. Carretero and F. J. Castander and C. Conselice and L. N. da Costa and M. E. S. Pereira and S. Desai and H. T. Diehl and S. Everett and I. Ferrero and B. Flaugher and J. Frieman and J. García-Bellido and E. Gaztanaga and G. Giannini and R. A. Gruendl and K. Herner and D. L. Hollowood and others},
title = {The Dark Energy Survey Supernova Program: An updated measurement of the Hubble constant using the Inverse Distance Ladder},
journal = {Monthly Notices of the Royal Astronomical Society},
year = {2025},
volume = {537},
publisher = {Oxford University Press},
month = {jan},
url = {https://academic.oup.com/mnras/advance-article/doi/10.1093/mnras/staf122/7994423},
number = {2},
pages = {1818--1825},
doi = {10.1093/mnras/staf122}
}
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Camilleri, R., et al. “The Dark Energy Survey Supernova Program: An updated measurement of the Hubble constant using the Inverse Distance Ladder.” Monthly Notices of the Royal Astronomical Society, vol. 537, no. 2, Jan. 2025, pp. 1818-1825. https://academic.oup.com/mnras/advance-article/doi/10.1093/mnras/staf122/7994423.