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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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Model-independent reconstruction of the expansion history of the Universe from Type Ia supernovae
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BackgroundKaluza–Klein spacetime filled with barotropic fluid and dark energy
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“…measurement of the CMB shift parameter R = 1.71 ± 0.02 (Komatsu et al. 2009), including the correlation between R and ℓA, together with the latest supernovae data from the Essence, SNLS and HST observations (see Wood-Vasey et al. 2007, Astier et al. 2006, Riess et al. 2007, Davis et al. 2007).”
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BackgroundInfluentialA measure of complexity for axial self-gravitating static fluids
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“Moreover, the largest fraction of the energy budget in the present Universe is occupied by Dark Energy (DE), which seems to be accelerating the expansion of the Universe ⋆ E-mail: camera@ph.unito.it (SC); tdk@roe.ac.uk (TDK); afh@roe.ac.uk (AFH); bertacca@pd.infn.it (DB); diaferio@ph.unito.it (AD) † Istituto Nazionale…”
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MethodObservational constraints on interacting dark matter model without dark energy
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Limitations of Bayesian Evidence Applied to CosmologyPreprint
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CONFORMAL COSMOLOGICAL MODEL PARAMETERS WITH DISTANT SNe Ia DATA: "GOLD" AND "SILVER"
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Holographic Dark Energy Cosmological Models in f(G) Theory
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Investigating Dark Energy Equation of State With High Redshift Hubble Diagram
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Gamma-ray burst contributions to constraining the evolution of dark energy
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“0) of the data was released, which included the additional data acquired on the GOODS fields during HST Cycles 12 and 13 looking for high-redshift Type Ia supernovae (Program IDs 9727, 9728, 10339, 10340, Riess et al. 2007).”
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Self-citationConstraining the evolution of dark energy with type Ia supernovae and gamma-ray bursts
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“The cosmological data sets, especially the SNe Iadata(Riess et al., 2004; Riess et al., 2007; Astier et al., 2006), the three years WMAP data (Spergel et al., 2003) , the SDSS data(Eisenstein et al., 2005; Bamba et al., 2012) all indicate that the ɅCDM model or the model that reduces to ɅCDM serves…”
MethodCosmological singularities and analytical solutions in varying vacuum cosmologies
Basilakos, S., Paliathanasis, A., Barrow, J. D., & Papagiannopoulos, G. (2018) · The European Physical Journal C · doi:10.1140/epjc/s10052-018-6139-8 · Cited by 22
Lasker, J., Kessler, R., Scolnic, D. M., Brout, D., Burke, D. L., D’Andrea, C. B., Davis, T. M., Hinton, S. R., Kim, A., Li, T. S., et al. (2019) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stz619 · Cited by 22
“PS1 used repeated observations of many HST CalSpec (Bohlin et al. 2014) standard stars inside of the footprint to tie its photometry to the AB system (Scolnic et al. 2015).”
BackgroundInfluentialPradhan, A., Tiwari, R. K., Beesham, A., & Zia, R. (2019) · The European Physical Journal Plus · doi:10.1140/epjp/i2019-12583-4 · Cited by 22
Charged anisotropic collapsing stars with heat flux in f(R) gravity
Nazar, H., & Abbas, G. (2019) · Chinese Journal of Physics · doi:10.1016/j.cjph.2019.11.019 · Cited by 22
Kinematic constraints on spatial curvature from supernovae Ia and cosmic chronometers
de Jesus, J. F., Valentim, R., Moraes, P. H. R. S., & Malheiro, M. M. (2020) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/staa3426 · Cited by 26
A new well-behaved class of compact strange astrophysical model consistent with observational data
Errehymy, A., & Mohammed Daoud, A. (2021) · The European Physical Journal C · doi:10.1140/epjc/s10052-021-09330-2 · Cited by 22
Stable gravastar with large surface redshift in Einstein's gravity with two scalar fields
Nojiri, S., & NASHED, G. G. L. (2024) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2024/03/023 · Cited by 22
PARAMETERIZING AND MEASURING DARK ENERGY TRAJECTORIES FROM LATE INFLATONS
Huang, Z.-Q., Bond, J., & Kofman, L. (2010) · The Astrophysical Journal · doi:10.1088/0004-637x/726/2/64 · Cited by 17
“…samples with the data from the ESSENCE project (Miknaitis et al. 2007; Wood-Vasey et al. 2007), the Supernova Legacy Survey (SNLS) (Astier et al. 2006), the Hubble Space Telescope (HST) (Garnavich et al. 1998; Knop et al. 2003; Riess et al. 2004, 2007), and a compilation of nearby SN measurements.”
MethodDynamical analysis of radiating spherical collapse in Palatini f(R) gravity
Sharif, M., & Yousaf, Z. (2014) · Astrophysics and Space Science · doi:10.1007/s10509-014-2116-3 · Cited by 22
Probing dark energy inhomogeneities with supernovae
Blomqvist, M., Mörtsell, E., & Nobili, S. (2008) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2008/06/027 · Cited by 22
“(8) Since σ2X ≈ 1, we can define the n-standard deviation (n-σ) detection limit of the angular correlation to be Clim = n√ Np .”
BackgroundIs the universe simpler than ΛCDM?
Walker, M. G., & Loeb, A. (2014) · Contemporary Physics · doi:10.1080/00107514.2014.919741 · Cited by 21
LIGHT CURVES OF 213 TYPE Ia SUPERNOVAE FROM THE ESSENCE SURVEY
Narayan, G., Rest, A., Tucker, B. E., Foley, R. J., Wood-Vasey, W. M., Challis, P., Stubbs, C. W., Kirshner, R. P., Aguilera, C., Becker, A. C., et al. (2016) · The Astrophysical Journal Supplement Series · doi:10.3847/0067-0049/224/1/3 · Cited by 22
“High-redshift SNIa surveys (Riess et al. 2007; Wood-Vasey et al. 2007; Guy et al. 2010; Betoule et al. 2014; Sako et al. 2014) have independently reported measurements of w consistent with −1, in good agreement with a classical cosmological constant.”
BackgroundSelf-citationMaurya, D. C., Zia, R., & Pradhan, A. (2017) · International Journal of Geometric Methods in Modern Physics · doi:10.1142/s0219887817500773 · Cited by 22
The phenomenology of beyond Horndeski gravity
Traykova, D., Bellini, E., & Ferreira, P. G. (2019) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2019/08/035 · Cited by 26
LIGHT CURVES OF 213 TYPE Ia SUPERNOVAE FROM THE ESSENCE SURVEY
Narayan, G., Rest, A., Tucker, B. E., Foley, R. J., Wood‐Vasey, W. M., Challis, P., Stubbs, C. W., Kirshner, R., Aguilera, C., Becker, A. C., et al. (2016) · OakTrust (Texas A&M University Libraries) · Cited by 22
Self-citationFIRST RESULTS FROM THE La Silla-QUEST SUPERNOVA SURVEY AND THE CARNEGIE SUPERNOVA PROJECT
Walker, E., Baltay, C., Campillay, A., Citrenbaum, C., Contreras, C., Ellman, N., Feindt, U., González, C., Graham, M., Hadjiyska, E., et al. (2015) · eScholarship (California Digital Library) · Cited by 22
Stable charged radiating systems associated with tilted observers
Yousaf, Z. (2021) · The European Physical Journal Plus · doi:10.1140/epjp/s13360-021-01278-2 · Cited by 22
Thermodynamics of Spinor Quintom
Wang, J., Cui, S. W., & Zhang, C. (2009) · Physics Letters B · doi:10.1016/j.physletb.2009.11.064 · Cited by 22
RECONSTRUCTING COSMOLOGICAL MATTER PERTURBATIONS USING STANDARD CANDLES AND RULERS
Alam, U., Sahni, V., & Starobinsky, A. A. (2009) · The Astrophysical Journal · doi:10.1088/0004-637x/704/2/1086 · Cited by 21
“Over the last decade, observations of Type Ia supernovae (SNe) have shown that the expansion of the universe is currently accelerating (Perlmutter et al. 1998, 1999; Riess et al. 1998, 2005, 2007; Tonry et al. 2003; Astier et al. 2005; Wood-Vasey et al. 2007; Kowalski et al. 2008).”
BackgroundEntropic Cosmology from a Thermodynamics Viewpoint
KOMATSU, N. (2014) · Asia Pacific Physics Conference (APPC) · doi:10.7566/jpscp.1.013112 · Cited by 21
Interpretation of complexity associated with cylindrically symmetric configuration in f(R, G) theory
Rehman, A., Yousaf, M., Javed, F., & Channuie, P. (2025) · The European Physical Journal C · doi:10.1140/epjc/s10052-025-14624-w · Cited by 21
Type Ia supernovae: Non-standard candles of the universe
Богомазов, А. И., & Tutukov, A. V. (2011) · Astronomy Reports · doi:10.1134/s1063772911060023 · Cited by 21
ACCELERATION OF THE UNIVERSE DRIVEN BY THE CASIMIR FORCE
Marek Szydlowski, A., & Godłowski, W. (2008) · International Journal of Modern Physics D · doi:10.1142/s021827180801205x · Cited by 21
Application of Bayesian graphs to SN Ia data analysis and compression
Ma, C., Corasaniti, P.-S., & Bassett, B. A. (2016) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stw2069 · Cited by 21
“To date these systematic searches have detected about a thousand SN Ia across a large red-shift range (see Astier et al. 2006; Riess et al. 2007; Wood-Vasey et al. 2007; Frieman et al. 2008; Hicken et al. 2009; Contreras et al. 2010; Tonry et al. 2012; Suzuki et al. 2012; Campbell et al. 2013).”
BackgroundAnisotropic compact star models in f(T) gravity with Tolman–Kuchowicz spacetime
Zubair, M., Ditta, A., Güdekli, E., Bhar, P., & Azmat, H. (2021) · International Journal of Geometric Methods in Modern Physics · doi:10.1142/s0219887821500602 · Cited by 21
Corrected holographic dark energy with power-law entropy and Hubble Horizon cut-off in FRW Universe
Bhardwaj, V. K., Garg, P., Pradhan, A., & Krishnannair, S. (2022) · Chinese Journal of Physics · doi:10.1016/j.cjph.2022.06.028 · Cited by 21
Dynamical evolution of self-gravitating compact fluid with hyperbolic corrections
Yousaf, M., Asad, H., & Rehman, A. (2025) · Physics of the Dark Universe · doi:10.1016/j.dark.2025.101888 · Cited by 21
Consistency of ΛCDM with geometric and dynamical probes
Perivolaropoulos, L. (2010) · Journal of Physics Conference Series · doi:10.1088/1742-6596/222/1/012024 · Cited by 21
The birth rate of supernovae from double-degenerate and core-degenerate systems
Meng, X., & Yang, W. (2012) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201218810 · Cited by 21
“At present, SNe Ia are regarded as critical cosmological probes for testing both the evolution of the dark energy equation of state with time and the evolutionary history of the universe (Riess et al. 2007; Kuznetsova et al. 2008; Howell et al. 2009a).”
BackgroundGauging the cosmic acceleration with recent type Ia supernovae data sets
Velten, H. E. S., Gomes, S., & Busti, V. C. (2018) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.97.083516 · Cited by 21
Comparison of Observed Galaxy Properties with Semianalytic Model Predictions Using Machine Learning
Simet, M., Chartab, N., Lu, Y., & Mobasher, B. (2021) · The Astrophysical Journal · doi:10.3847/1538-4357/abd179 · Cited by 21
Self-citationPan, Y. C., Foley, R. J., Jones, D. O., Filippenko, A. V., & Kuin, N. P. M. (2019) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stz3391 · Cited by 21
“…cosmological standardizable candles that are consistently used to measure cosmological parameters (e.g. Riess et al. 1998; Perlmutter et al. 1999; Riess et al. 2007; Kessler et al. 2009; Suzuki et al. 2012; Betoule et al. 2014; Rest et al. 2014; Riess et al. 2016, 2018; Scolnic et al. 2018).”
BackgroundSelf-citationDifferences and similarities of stellar populations in LAEs and LBGs at z ∼ 3.4−6.8
Haro, P. A., Rodríguez-Espinosa, J. M., Muñoz-Tuñón, C., Sobral, D., Lumbreras-Calle, A., Boquien, M., Hernán-Caballero, A., Rodríguez-Muñoz, L., & Pampliega, B. A. (2020) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/staa1196 · Cited by 21
Interacting Tsallis and Rényi holographic dark energy with hybrid expansion law
Bhattacharjee, S. (2020) · Astrophysics and Space Science · doi:10.1007/s10509-020-03820-7 · Cited by 24
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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