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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
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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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Wagner, C., Müller, V., & Steinmetz, M. (2008) · Springer Link (Chiba Institute of Technology) · doi:10.1051/0004-6361:20077688/pdf · Cited by 15
Constraints on C.D.M. cosmology from galaxy power spectrum, CMB and SNIa evolution
Ferramacho, L., Blanchard, A., & Zolnierowski, Y. (2009) · Springer Link (Chiba Institute of Technology) · doi:10.1051/0004-6361/200810693/pdf · Cited by 15
Observational tests of a two parameter power-law class modified gravity in Palatini formalism
Baghram, S., Movahed, M. S., & Rahvar, S. (2009) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.80.064003 · Cited by 15
Beck, C., & Mackey, M. C. (2008) · International Journal of Modern Physics D · doi:10.1142/s0218271808011870 · Cited by 15
A model independent measure of the large scale curvature of the UniversePreprint
Mörtsell, E., & Jonsson, J. (2011) · arXiv (Cornell University) · doi:10.48550/arxiv.1102.4485 · Cited by 15
Barnard, M., Abrahamse, A., Albrecht, A., Bozek, B., & Yashar, M. (2008) · Physical Review D · doi:10.1103/physrevd.78.043528 · Cited by 17
Constraints on dark energy models using late Universe probes
Barua, S., & Desai, S. (2025) · Physics of the Dark Universe · doi:10.1016/j.dark.2025.101995 · Cited by 14
Late time cosmic acceleration of a flat matter dominated universe with constant vacuum energy
Kalita, S., Duorah, H. L., & Duorah, K. (2010) · Indian Journal of Physics · doi:10.1007/s12648-010-0062-7 · Cited by 14
Analysis of f(R) Theory Corresponding to NADE and NHDE
Sharif, M., & Zubair, M. (2013) · Advances in High Energy Physics · doi:10.1155/2013/790967 · Cited by 14
The bouncing cosmic behavior with logarithmic law f(G,T) model
Yousaf, Z., Bhatti, M. Z. U. H., & Aman, H. (2022) · Chinese Journal of Physics · doi:10.1016/j.cjph.2022.07.006 · Cited by 14
Clocchiatti, A., Rodríguez, Ó., Morales, Á. L., & Cuevas-Tapia, B. (2024) · The Astrophysical Journal · doi:10.3847/1538-4357/ad51ff · Cited by 14
“…the deceleration parameter as if the universe had switched from deceleration to acceleration rather recently, as it has been actually observed (e.g. Riess et al. 2007), the other is that they will detect a dipolar anisotropy of the deceleration parameter if they measure its full-sky distribution.”
MethodDhawan, S., Pierel, J. D. R., Gu, M., Newman, A. B., Larison, C., Siebert, M. R., Petrushevska, T., Poidevin, F., Jha, S. W., Chen, W., et al. (2024) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stae2434 · Cited by 14
Self-citationField-theoretic construction of complexity-free anisotropic stars via extended decoupling
Farwa, U., Abbas, A., & Yousaf, M. (2025) · Nuclear Physics B · doi:10.1016/j.nuclphysb.2025.117086 · Cited by 14
Revisiting the screening mechanism in f(R) gravity
He, J.-H., Li, B., Hawken, A. J., & Granett, B. R. (2014) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.90.103505 · Cited by 14
Warped de Sitter compactifications
Minamitsuji, M., & Uzawa, K. (2012) · Journal of High Energy Physics · doi:10.1007/jhep01(2012)142 · Cited by 14
Constraints on small-scale cosmological fluctuations from SNe lensing dispersion
Ben-Dayan, I., & Takahashi, R. (2015) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stv2356 · Cited by 14
“Several SNe surveys have set strong constraints on cosmological models from the distance-redshift relation (e.g. Riess et al. 1998; Perlmutter et al. 1999; Riess et al. 2007; Sullivan et al. 2011; Campbell et al.2013).”
BackgroundCosmological tests with the joint lightcurve analysis
Melia, F., Wei, J.-J., Maier, R. S., & Wu, X.-F. (2018) · Europhysics Letters (EPL) · doi:10.1209/0295-5075/123/59002 · Cited by 14
Dark sector evolution in Horndeski models
Pace, F., Battye, R. A., Bolliet, B., & Trinh, D. (2019) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2019/09/018 · Cited by 14
Scalar field theory description of the running vacuum model: the vacuumon
Basilakos, S., Mavromatos, N. E., & Solà, J. (2019) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2019/12/025 · Cited by 14
An FLRW interacting dark energy model of the Universe
Pradhan, A., Goswami, G. K., Beesham, A., & Dixit, A. (2020) · New Astronomy · doi:10.1016/j.newast.2020.101368 · Cited by 14
Probing dark energy with the next generation X-ray surveys of galaxy clusters
Sartoris, B., Borgani, S., Rosati, P., & Weller, J. (2012) · MPG.PuRe (Max Planck Society) · Cited by 14
Quasi static evolution of compact objects in modified gravity
Yousaf, Z., Bamba, K., Bhatti, M. Z. U. H., & Farwa, U. (2022) · General Relativity and Gravitation · doi:10.1007/s10714-021-02887-z · Cited by 14
Barrow entropic quintessence and dilation dark energy models with generalized HDE cut-off
Garg, P., Bhardwaj, V. K., & Pradhan, A. (2022) · International Journal of Modern Physics A · doi:10.1142/s0217751x22502177 · Cited by 14
Is there a standard measuring rod in the Universe?
Jackson, J. C. (2008) · Monthly Notices of the Royal Astronomical Society Letters · doi:10.1111/j.1745-3933.2008.00509.x · Cited by 14
“…(Dunkley et al. 2008; Komatsu et al. 2008), in combination with observations of Type Ia supernovae (SNe Ia) (Riess et al. 2004; Astier et al. 2006; Riess et al. 2007; Wood-Vasey et al. 2007), and the imprint of Baryon Accoustic Oscillations (BAO) on the distribution of galaxies (Blake &…”
BackgroundConstraining the Parameters of Modified Chaplygin Gas in Einstein-Aether Gravity
Debnath, U. (2014) · Advances in High Energy Physics · doi:10.1155/2014/653630 · Cited by 14
Rainbow Gravity Corrections to the Entropic Force
Feng, Z.-W., & Yang, S.-Z. (2018) · Advances in High Energy Physics · doi:10.1155/2018/5968284 · Cited by 14
Transit cosmological models in FRW universe under the two-fluid scenario
Garg, P., Zia, R., & Pradhan, A. (2018) · International Journal of Geometric Methods in Modern Physics · doi:10.1142/s0219887819500075 · Cited by 14
On the distribution of Bayesian evidence
Keeley, R. E., & Shafieloo, A. (2022) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stac1851 · Cited by 14
The k-essence scalar field in the context of Supernova Ia observations
Bandyopadhyay, A., Gangopadhyay, D., & Moulik, A. (2012) · The European Physical Journal C · doi:10.1140/epjc/s10052-012-1943-z · Cited by 15
Implications of Two Type Ia Supernova Populations for Cosmological Measurements
Sarkar, D., Amblard, A., Cooray, A. R., & HOLZ, D. E. (2008) · The Astrophysical Journal · doi:10.1086/592019 · Cited by 14
“…existing data may be affected by a residual systematic in the luminosity difference betwen prompt and delayed SNe, we model fit a combined data set of 192 SNe (Davis et al. 2007; Wood-Vasey et al. 2007; Riess et al. 2007; Astier et al. 2006; Hamuy et al. 1996a; Riess et al. 1999; Jha et al. 2006).”
MethodOptical Observations of the Rapidly Expanding Type Ia Supernova 2007giPreprint
Zhang, T., Wang, X., Li, W., Filippenko, A. V., Wang, L., Zhou, X., Brown, P. J., Silverman, J. M., Steele, T. N., Ganeshalingam, M., et al. (2010) · Cited by 14
Self-citationSome Bianchi type-V accelerating cosmological models in f(R,T) = f1(R) + f2(T) formalism
Bhardwaj, V. K., & Yadav, A. K. (2020) · International Journal of Geometric Methods in Modern Physics · doi:10.1142/s0219887820501595 · Cited by 13
Late time cosmological evolution of the DBI model with collisional matter
Mavoa, F., Ganiou, M. G., Houndjo, M. J. S., Kanfon, A. D., & Salako, I. G. (2022) · Indian Journal of Physics · doi:10.1007/s12648-021-02271-2 · Cited by 13
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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