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New Hubble Space Telescope Discoveries of Type Ia Supernovae at z≥ 1: Narrowing Constraints on the Early Behavior of Dark Energy
Open accessAbstract
We have discovered 21 new Type Ia supernovae (SNe Ia) with the Hubble Space Telescope ( HST ) and have used them to trace the history of cosmic expansion over the last 10 billion yr. These objects, which include 13 spectroscopically confirmed SNe Ia at z ≥ 1, were discovered during 14 epochs of reimaging of the GOODS fields North and South over 2 yr with the Advanced Camera for Surveys on HST . Together with a recalibration of our previous HST -discovered SNe Ia, the full sample of 23 SNe Ia at z ≥ 1 provides the highest redshift sample known. Combining these data with previous SN Ia data sets, we measured H ( z ) at discrete, uncorrelated epochs, reducing the uncertainty of H ( z > 1) from 50% to under 20%, strengthening the evidence for a cosmic jerk—the transition from deceleration in the past to acceleration in the present. The unique leverage of the HST high-redshift SNe Ia provides the first meaningful constraint on the dark energy equation-of-state parameter at z ≥ 1. The result remains consistent with a cosmological constant [ w ( z ) = −1] and rules out rapidly evolving dark energy ( dw / dz ≫ 1). The defining property of dark energy, its negative pressure, appears to be present at z > 1, in the epoch preceding acceleration, with ~98% confidence in our primary fit. Moreover, the z > 1 sample-averaged spectral energy distribution is consistent with that of the typical SN Ia over the last 10 Gyr, indicating that any spectral evolution of the properties of SNe Ia with redshift is still below our detection threshold.
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“Current models of cosmology require the existence of both dark matter and dark energy to match observational constraints”
From LSST: From Science Drivers to Reference Design and Anticipated Data Products (2019) · cites this paper as Riess et al. 2007
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“Combining these high-z and nearby SNe Ia, the Hubble diagram was established, allowing significant constraints on properties of Dark Energy and its equation of state (Riess et al. 2004, 2007).”
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“At present, SNe Ia are proposed to be cosmological probes for testing the evolution of the dark energy equation of state with time and testing the evolutionary history of the universe (Riess et al. 2007; Kuznetsova et al. 2008; Howell et al. 2009).”
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“…et al. 2007) target the redshift range 0.3 <∼ z <∼ 1.0 for SNe Ia. Finally, the highest redshift SNe currently used for cosmological constraints, those at z >∼ 1, are studied using the Hubble Space Telescope(HST) (Riess et al. 2004, 2007; Dawson et al. 2009; Suzuki et al. 2012; Rodney et al. 2012).”
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“…but also occurs with fits using dark energy EOS functions with a very limited number of best-fit coefficients—as demonstrated, for example, in Riess et al. (2007), and also by the “Mirage of w 1= - ” problem (Linder 2007) for fits with w z( ) models limited to a single, constant value…”
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“…(Miknaitis et al. 2007; Wood-Vasey et al. 2007; Krisciunas et al. 2005), Hubble Space Telescope (HST; Garnavich et al. 1998; Knop et al. 2003; Riess et al. 2004, 2007), Sloan Digital Sky Survey (SDSS; Frieman et al. 2008; Kessler et al. 2009; Holtzman et al. 2008; Betoule et al. 2014),…”
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Cosmological evolution of two-scalar fields cosmology in the Jordan frame
Giacomini, A., León, G., Paliathanasis, A., & Pan, S. (2020) · The European Physical Journal C · doi:10.1140/epjc/s10052-020-7730-3 · Cited by 18
Koo, H., Shafieloo, A., Keeley, R. E., & L’Huillier, B. (2020) · The Astrophysical Journal · doi:10.3847/1538-4357/ab9c9a · Cited by 18
Foundations of supernova cosmology
Kirshner, R. (2010) · Cambridge University Press eBooks · doi:10.1017/cbo9781139193627.006 · Cited by 18
Self-citationA brief review on cosmological analysis of galaxy surveys with multiple tracers
Wang, Y., & Zhao, G.-B. (2020) · Research in Astronomy and Astrophysics · doi:10.1088/1674-4527/20/10/158 · Cited by 18
“Being complementary to other probes including the supernovae (SNIa) (Riess et al. 1998; Perlmutter et al. 1999; Riess et al. 2007; Sullivan et al. 2011; Suzuki et al. 2012; Betoule et al. 2014; Scolnic et al. 2018; D’Andrea et al. 2018) and the cosmic microwave background (CMB) (Bennett et al.…”
BackgroundFermionic vacuum polarization by a cosmic string in anti-de Sitter spacetime
de Mello, E. R. B., Medeiros, E. R. F., & SAHARIAN, A. A. (2013) · Classical and Quantum Gravity · doi:10.1088/0264-9381/30/17/175001 · Cited by 19
Dynamics and chaos in the unified scalar field cosmology
Lukes-Gerakopoulos, G., Basilakos, S., & Contopoulos, G. (2008) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.77.043521 · Cited by 18
Statefinder diagnostic in a torsion cosmology
Li, X.-Z., Chang-bo, S., & Xi, P. (2009) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2009/04/015 · Cited by 26
“755 by the Hubble Space Telescope [24] as in ref.”
InfluentialThe Type Ia supernovae rate with Subaru/XMM-Newton Deep Survey
Okumura, J. E., Ihara, Y., Doi, M., Morokuma, T., Pain, R., Totani, T., Barbary, K., Takanashi, N., Yasuda, N., Aldering, G., et al. (2014) · Publications of the Astronomical Society of Japan · doi:10.1093/pasj/psu024 · Cited by 18
“…SN surveys have been carried out to accurately measure the cosmological parameters (e.g., Knop et al. 2003; Tonry et al. 2003; Astier et al. 2006; Riess et al. 2007; Wood-Vasey et al. 2007; Kowalski et al. 2008; Hicken et al. 2009; Amanullah et al. 2010; Sullivan et al. 2011; Suzuki et al. 2012).”
BackgroundDark energy from cosmological fluids obeying a Shan-Chen nonideal equation of state
Bini, D., Geralico, A., Gregoris, D., & Sauro Succi, A. (2013) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.88.063007 · Cited by 18
Dust Static Cylindrically Symmetric Solutions in f ( R ) Gravity
Shamir, M. F., & Raza, Z. (2014) · Communications in Theoretical Physics · doi:10.1088/0253-6102/62/3/10 · Cited by 18
Cosmological Constraints on Polytropic Gas Model
Asadzadeh, S., Safari, Z., Karami, K., & Abdolmaleki, A. (2013) · International Journal of Theoretical Physics · doi:10.1007/s10773-013-1922-7 · Cited by 18
Holwerda, B. W. (2008) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2008.13050.x · Cited by 18
“Models of a dusty universe (Goobar, Bergström & Mörtsell 2002; Robaina & Cepa 2007) find this grey dust explanation increasingly inconsistent with observational data (see also e.g. Riess et al. 2007).”
BackgroundMethodConstraints on the Physical Properties of SNe Ia from Photometry
Könyves-Tóth, R., Vinkó, J., Ordasi, A., Sárneczky, K., Bódi, A., Cseh, B., Csörnyei, G., Dencs, Z., Hanyecz, O., Ignácz, B., et al. (2020) · The Astrophysical Journal · doi:10.3847/1538-4357/ab76bb · Cited by 18
高, C. 超. G., 陈, Y. 云. C., & 郑, J. 接. Z. (2020) · Research in Astronomy and Astrophysics · doi:10.1088/1674-4527/20/9/151 · Cited by 18
“The popular samples include the “gold” 2004 (157 data;Riess et al. 2004) and “gold” 2007 (182 data; Riess et al. 2007) samples, the Supernova Legacy Survey (SNLS) 1-year (115 data;Astier et al. 2006) and 3-year (252 data;Guy et al. 2010) samples, the “Equation of State: SupErNovae trace Cosmic…”
BackgroundCosmological Implications of 5-dimensional Brans-Dicke Theory
Qiang, L.-E., Gong, Y., Ma, Y.-G., & Chen, X.-L. (2009) · Physics Letters B · doi:10.1016/j.physletb.2009.10.028 · Cited by 19
Beck, C., & MacKey, M. C. (2007) · CERN Document Server (European Organization for Nuclear Research) · Cited by 18
Dynamical 3-Space: A ReviewPreprint
Cahill, R. T. (2007) · arXiv (Cornell University) · doi:10.48550/arxiv.0705.4146 · Cited by 18
The Hubble Tension Resolved by the DESI Baryon Acoustic Oscillations Measurements
Jia, X. D., Hu, J.-P., Gao, D.-Y., Yi, S.-X., & Wang, F. Y. (2025) · The Astrophysical Journal Letters · doi:10.3847/2041-8213/ae1965 · Cited by 19
“In order to study w ( z ) model-independently, we use a non-parametric approach (Huterer & Cooray 2005; Riess et al. 2007; Lodha et al. 2025).”
Dynamics and constraints of the massive graviton dark matter flat cosmologies
Basilakos, S., Plionis, M., Alves, M. E. S., & Lima, J. A. S. (2011) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.83.103506 · Cited by 17
A probe of cosmological models in modified teleparallel gravity
Dixit, A., Pradhan, A., & Maurya, D. C. (2021) · International Journal of Geometric Methods in Modern Physics · doi:10.1142/s021988782150208x · Cited by 20
Prospects of Searching for Type Ia Supernovae with 2.5-m Wide Field Survey Telescope
Hu, M., Hu, L., Jiang, J.-A., Xiao, L., Fan, L., Wei, J.-J., & Wu, X.-F. (2022) · Universe · doi:10.3390/universe9010007 · Cited by 17
“For those SNe Ia at high-redshifts, they can be applied to constrain the property of dark energy [10], test the cosmic distance duality relation [76–78], constrain cosmic opacity [79], estimate the time variation of Newton’s constant G [80], and so on.”
EDSFD parameterization in f(R,T) gravity with linear curvature terms
Singh, J. K., Shaily, Balhara, H., Ghosh, S. G., & Maharaj, S. D. (2024) · Physics of the Dark Universe · doi:10.1016/j.dark.2024.101513 · Cited by 17
Hubble tension in a nonminimally coupled curvature-matter gravity model
Varela, M. B., & Orfeu Bertolami, A. (2024) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2024/06/025 · Cited by 17
Charged gravastar model in Rastall theory of gravity
Bhattacharjee, D., & Chattopadhyay, P. K. (2024) · Journal of High Energy Astrophysics · doi:10.1016/j.jheap.2024.08.001 · Cited by 17
Inhomogeneous Viscous Fluids in a Friedmann-Robertson-Walker (FRW) Universe
Myrzakulov, R., Sebastiani, L., & Zerbini, S. (2013) · Galaxies · doi:10.3390/galaxies1020083 · Cited by 17
“ence problem may be solved, and if the de Sitter solution is stable, the model is also protected against the Big Rip singularity. 1 Introduction Since the discovery of the current cosmic acceleration [1, 2, 3, 4, 5, 6, 7, 8], the dark energy issue has become one of the most interesting fields of research in modern cosm…”
BackgroundFrom model dynamics to oscillating dark energy parameterisation
Kurek, A., Hrycyna, O., & Marek Szydlowski, A. (2010) · Physics Letters B · doi:10.1016/j.physletb.2010.05.061 · Cited by 17
Revisiting the matter power spectra in f(R) gravity
He, J.-H., Li, B., & Jing, Y. (2013) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.88.103507 · Cited by 17
SNe Ia as a cosmological probe
Meng, X., Gao, Y., & Han, Z. (2015) · International Journal of Modern Physics D · doi:10.1142/s0218271815300293 · Cited by 17
QCD MODIFIED GHOST SCALAR FIELD DARK ENERGY MODELS
Karami, K., ASADZADEH, S., Mousivand, M., & Safari, Z. (2013) · International Journal of Modern Physics D · doi:10.1142/s0218271813500181 · Cited by 17
Probing dark energy with the next generation X-ray surveys of galaxy clusters
Sartoris, B., Borgani, S., Rosati, P., & Weller, J. (2012) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2012.21064.x · Cited by 17
“1 IN T RO D U C T I O N A number of independent cosmological observations, ranging from Type Ia supernova (SNIa) (e.g. Perlmutter et al. 1999; Riess et al. 2007) to cosmic microwave background (CMB) anisotropies (e.g. E-mail: sartoris@oats.inaf.it Komatsu et al. 2011; Larson et al. 2011) and…”
BackgroundThe velocity-density relation in the spherical model
Bilicki, M., & Chodorowski, M. J. (2008) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2008.13988.x · Cited by 17
“Since for small redshifts dark energy behaves similarly to the cosmological constant (e.g. Riess et al. 2007), and since only for such redshifts the weak dependence of equations of motion on cosmological parameters starts to play any role (because earlier we hadΩ<∼ 1; NuCo98), the velocity–density…”
Background
Metadata
- Authors
- Riess, A. G., Strolger, L., Casertano, S., Ferguson, H. C., Mobasher, B., Gold, B., Challis, P. J., Filippenko, A. V., Jha, S., Li, W., Tonry, J., Foley, R., Kirshner, R. P., Dickinson, M., MacDonald, E., Eisenstein, D., Livio, M., Younger, J., Xu, C., Dahlen, T., & Stern, D.
- Affiliations
- Space Telescope Science Institute (US)
- Western Kentucky University (US)
- Johns Hopkins University (US)
- Center for Astrophysics Harvard & Smithsonian (US)
- University of California, Berkeley (US)
- University of Hawaiʻi at Mānoa (US)
- University of Arizona (US)
- California Institute of Technology (US)
- ORCID
- Venue
- The Astrophysical Journal
- Publisher
- American Astronomical Society
- Published
- 2007-04-10
- Volume
- 659
- Issue
- 1
- Pages
- 98-121
- ISSN
- 0004-637X (ISSN-L)
- 1538-4357
- OpenAlex
- W2099827831
- Cited by
- 1,758
- References
- 101
- Citations by year
- 2026: 28 · 2025: 51 · 2024: 75 · 2023: 64 · 2022: 68 · 2021: 60 · 2020: 76 · 2019: 57 · 2018: 67 · 2017: 63 · 2016: 77 · 2015: 65 · 2014: 87 · 2013: 104 · 2012: 108
- FWCI
- 116.60
- Type
- journal article
- Language
- en
- Open access
- bronze
- doi.org
- Locations
- The Astrophysical Journal (publishedVersion)
- arXiv (Cornell University) (submittedVersion)
- Digital Access to Scholarship at Harvard (DASH) (Harvard University) (submittedVersion, cc-by)
- CERN Document Server (European Organization for Nuclear Research) (submittedVersion)
- arXiv (Cornell University)
- Funders
- National Aeronautics and Space Administration
- W. M. Keck Foundation
- California Institute of Technology
- McMaster University
- Space Telescope Science Institute
- Topics
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Cosmology and Gravitation Theories
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Gamma-ray bursts and supernovae
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Galaxies: Formation, Evolution, Phenomena
- Keywords
- Type Ia supernovae, high-redshift supernovae, dark energy, dark energy equation of state, cosmic acceleration, spectral energy distribution, GOODS fields, cosmological constant
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