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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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Taubenberger, S., Benetti, S., Childress, M., Pakmor, R., Hachinger, S., Mazzali, P. A., Stanishev, V., Elias-Rosa, N., Agnoletto, I., Bufano, F., et al. (2011) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2010.18107.x · Cited by 205
“In particular, with sufficiently precise observations of SNe Ia at low and high redshift, the expansion history of the Universe can be reconstructed and a possible time evolution of Dark Energy can be probed (e.g. Riess et al. 2007).”
BackgroundTransition redshift: new kinematic constraints from supernovae
Cunha, J. V., & Lima, J. A. S. (2008) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2008.13640.x · Cited by 204
“The supernovae span the redshift range 0.2 < z < 1.8 (Riess et al. 2007).”
BackgroundMethodInfluentialTotal mass biases in X-ray galaxy clusters
Piffaretti, R., & Valdarnini, R. (2008) · Astronomy and Astrophysics · doi:10.1051/0004-6361:200809739 · Cited by 199
“…evolution will provide independent tests with which to compare constraints on cosmological models extracted from observations of the cosmic background radiation (e.g. Spergel et al. 2007) and distance measurements of high redshift supernovae (e.g. Tonry et al. 2003; Riess et al. 2004, 2007).”
BackgroundWang, X., Li, W., Filippenko, A. V., Krisciunas, K., Suntzeff, N. B., Li, J., Zhang, T., Deng, J.-S., Foley, R. J., Ganeshalingam, M., et al. (2008) · The Astrophysical Journal · doi:10.1086/526413 · Cited by 194
“…of mysterious dark energy, was subsequently confirmed by more studies using SNe Ia (Barris et al. 2003; Tonry et al. 2003; Knop et al. 2003; Riess et al. 2004, 2007; Astier et al. 2006; Wood-Vasey et al. 2007), and by independent methods such as the power spectrum of fluctuations in the…”
ResultSelf-citationLi, M., Li, X.-D., Wang, S., & Wang, Y. (2013) · Frontiers of Physics · doi:10.1007/s11467-013-0300-5 · Cited by 203
Kinematic constraints to the transition redshift from supernovae type Ia union data
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Simulations of the WFIRST Supernova Survey and Forecasts of Cosmological Constraints
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Self-citationRevisiting a Negative Cosmological Constant from Low-Redshift Data
Visinelli, L., Vagnozzi, S., & Danielsson, U. (2019) · Symmetry · doi:10.3390/sym11081035 · Cited by 183
Quantifying the effect of baryon physics on weak lensing tomography
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HOST GALAXY PROPERTIES AND HUBBLE RESIDUALS OF TYPE Ia SUPERNOVAE FROM THE NEARBY SUPERNOVA FACTORY
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“…providing the tightest possible constraints on the matter and dark energy densities as well as the dark energy equation of state parameter w (e.g. Riess et al. 1998; Perlmutter et al. 1999; Garnavich et al. 1998; Knop et al. 2003; Riess et al. 2004, 2007; Sullivan et al. 2011; Suzuki et al. 2012).”
BackgroundRodney, S., Riess, A. G., Strolger, L.-G., Dahlen, T., Graur, O., Casertano, S., Dickinson, M. E., Ferguson, H. C., Garnavich, P., Hayden, B., et al. (2014) · The Astronomical Journal · doi:10.1088/0004-6256/148/1/13 · Cited by 185
“To that end, we have applied the STARDUST classifier to the “Gold” sample of 31 SN from the GOODS and PANS surveys (Strolger et al. 2004; Riess et al. 2007) that have spectroscopic classifications.”
MethodSelf-citationBarro, G., Pérez‐González, P. G., Cava, A., Brammer, G., Pandya, V., Eliche-Moral, M. C., Esquej, P., Sánchez, H. D., Pampliega, B. A., Guo, Y., et al. (2019) · The Astrophysical Journal Supplement Series · doi:10.3847/1538-4365/ab23f2 · Cited by 182
Self-citationSollerman, J., Mörtsell, E., Davis, T. M., Blomqvist, M., Bassett, B. A., Becker, A. C., Cinabro, D., Filippenko, A. V., Foley, R. J., Frieman, J. A., et al. (2009) · The Astrophysical Journal · doi:10.1088/0004-637x/703/2/1374 · Cited by 183
“This technique was used to great effect by Riess et al. (2007).”
BackgroundMethodSelf-citationCosmology with gamma-ray bursts
Demiański, M., Piedipalumbo, E., Sawant, D., & Amati, L. (2016) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201628909 · Cited by 183
Interacting agegraphic dark energy
Wei, H., & Cai, R.-G. (2008) · The European Physical Journal C · doi:10.1140/epjc/s10052-008-0799-8 · Cited by 179
The ESSENCE Supernova Survey: Survey Optimization, Observations, and Supernova Photometry
Miknaitis, G. A., Pignata, G., Rest, A., Wood‐Vasey, W. M., Blondin, S., Challis, P., Smith, R. C., Stubbs, C. W., Suntzeff, N. B., Foley, R. J., et al. (2006) · University of North Texas Digital Library (University of North Texas) · Cited by 180
Self-citationThe Hubble series: convergence properties and redshift variables
Cattoën, C., & Visser, M. (2007) · Classical and Quantum Gravity · doi:10.1088/0264-9381/24/23/018 · Cited by 179
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Wang, X., Li, W., Filippenko, A. V., Foley, R. J., Kirshner, R., Modjaz, M., Bloom, J. S., Brown, P. J., Carter, D., Friedman, A. S., et al. (2009) · The Astrophysical Journal · doi:10.1088/0004-637x/697/1/380 · Cited by 175
“…for the acceleration expansion from SNe Ia improved markedly with follow-up studies (Barris et al. 2004; Tonry et al. 2003; Knop et al. 2003; Riess et al. 2004, 2007; Astier et al. 2006; Wood-Vasey et al. 2007a), suggesting that ∼70% of the universe is composed of a mysterious dark energy…”
BackgroundSelf-citationA Cosmology‐Independent Calibration of Gamma‐Ray Burst Luminosity Relations and the Hubble Diagram
Liang, N., Xiao, W. K., Liu, Y., & Zhang, S. (2008) · The Astrophysical Journal · doi:10.1086/590903 · Cited by 173
“However, Riess et al. (2007) failed to reveal the direct evidence for SN Ia evolution from analysis of thez > 1 sampleaveraged spectrum.”
BackgroundMethodInteracting models may be key to solve the cosmic coincidence problem
del Campo, S., Herrera, R., & Pavón, D. (2009) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2009/01/020 · Cited by 169
Mazzali, P. A., Sullivan, M., Hachinger, S., Ellis, R. S., Nugent, P., Howell, D. A., Gal‐Yam, A., Maguire, K., Cooke, J., Thomas, R. C., et al. (2014) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stu077 · Cited by 168
“energy (e.g. Riess et al. 1998, 2007; Perlmutter et al. 1999; Kessler et al. 2009; Sullivan et al. 2011; Suzuki et al. 2012).”
Bamba, K., Nojiri, S., & Odintsov, S. D. (2008) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.77.123532 · Cited by 167
MEASURING EJECTA VELOCITY IMPROVES TYPE Ia SUPERNOVA DISTANCES
Foley, R. J., & Kasen, D. (2011) · The Astrophysical Journal · doi:10.1088/0004-637x/729/1/55 · Cited by 166
“…to determine that the expansion of the Universe is accelerating (Riess et al. 1998; Perlmutter et al. 1999), and constrain the equation-of-state parameter of Dark Energy (Astier et al. 2006; Wood-Vasey et al. 2007; Riess et al. 2007; Hicken et al. 2009b; Kessler et al. 2009; Amanullah et al. 2010).”
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Bamba, K., Ilyas, M., Bhatti, M. Z., & Yousaf, Z. (2017) · General Relativity and Gravitation · doi:10.1007/s10714-017-2276-x · Cited by 170
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“…by 0.068 mag and F160W fainter by 0.023 mag as the result of three net changes: (1) updated NICMOS zero-points over the original calibration of Riess et al. (2007), used (2) Rubin et al. (2015) to check the low count-rate zero-points, and (3) provide an update to Rubin et al. (2015) based on…”
InfluentialSelf-citationSupernovae in Early‐Type Galaxies: Directly Connecting Age and Metallicity with Type Ia Luminosity
Gallagher, J. S., Garnavich, P., Caldwell, N., Kirshner, R. P., Jha, S. W., Li, W., Ganeshalingam, M., & Filippenko, A. V. (2008) · The Astrophysical Journal · doi:10.1086/590659 · Cited by 164
Self-citationIMPROVED STANDARDIZATION OF TYPE II-P SUPERNOVAE: APPLICATION TO AN EXPANDED SAMPLE
Poznanski, D., Butler, N., Filippenko, A. V., Ganeshalingam, M., Li, W., Bloom, J. S., Chornock, R., Foley, R. J., Nugent, P., Silverman, J. M., et al. (2009) · The Astrophysical Journal · doi:10.1088/0004-637x/694/2/1067 · Cited by 165
“Compelling evidence for cosmic acceleration comes from distance measurements to Type Ia supernovae (SNe Ia; e.g., Astier et al. 2006; Wood-Vasey et al. 2007; Riess et al. 2007; Kowalski et al. 2008, see Filippenko 2005b for a review of earlier studies).”
BackgroundSelf-citationNew constraints on dark energy from the observed growth of the most X-ray luminous galaxy clusters
Mantz, A. B., Allen, S. W., Ebeling, H., & Rapetti, D. (2008) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2008.13311.x · Cited by 186
“…2008 RAS, MNRAS 000, 1–15 the SNLS first year data (57 targets; Astier et al. 2006), 45 nearby supernovae (Jha et al. 2007) and the 30 highredshift supernovae discovered by the Hubble Space Telescope and reported by Riess et al. (2007) for which a ‘gold’ rating was awarded (192 SNIa in total).”
BackgroundType Ia Supernovae Are Good Standard Candles in the Near Infrared: Evidence from PAIRITEL
Wood‐Vasey, W. M., Friedman, A. S., Bloom, J. S., Hicken, M., Modjaz, M., Kirshner, R., Starr, D., Blake, C. H., Falco, E. E., Szentgyorgyi, A. H., et al. (2008) · The Astrophysical Journal · doi:10.1086/592374 · Cited by 164
“The predicted turnover to the matterdominated era and the corresponding deceleration at z > 1 have been seen in space-based work from theHubble Space Telescope (HST ) (Riess et al. 2007).”
Self-citationBenítez, N., GAZTAÑAGA, E., Miquel, R., Castander, F. J., Moles, M., Crocce, M., Fernández-Soto, A., Fosalba, P., Ballesteros, F., Campa, J., et al. (2009) · The Astrophysical Journal · doi:10.1088/0004-637x/691/1/241 · Cited by 163
“…al. 2008; Dickinson et al. 2004) with distancescale measurements at increasingly higher redshifts (e.g., WoodVasey et al. 2007; Astier et al. 2006; Riess et al. 2007) and probes of large-scale structure (Cole et al. 2005; Tegmark et al. 2004, 2006; Percival et al. 2007; Hütsi 2006b) yields a…”
BackgroundNon-perturbative and self-consistent models of neutron stars in R -squared gravity
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Schmidt, F. (2008) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.78.043002 · Cited by 161
Constraining Interactions in Cosmology's Dark Sector
Bean, R., Flanagan, E., László, I., & Trodden, M. (2008) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.78.123514 · Cited by 122
SPECTROSCOPY OF TYPE Ia SUPERNOVAE BY THE CARNEGIE SUPERNOVA PROJECT
Folatelli, G., Morrell, N., Phillips, M. M., Hsiao, E. Y., Campillay, A. R., Contreras, C., Castellón, S., Hamuy, M., Krzemiński, W., Roth, M. R., et al. (2013) · The Astrophysical Journal · doi:10.1088/0004-637x/773/1/53 · Cited by 160
“…the equation-of-state parameter, w, of dark energy to be constrained to within 10% by comparing low- and high-redshift SNe Ia samples (see, e.g. Riess et al. 2007; Freedman et al. 2009; 15 National Snow and Ice Data Center, University of Colorado, Boulder, CO 80309, USA 16 Max-Planck-Institute…”
BackgroundVARIABLE SODIUM ABSORPTION IN A LOW-EXTINCTION TYPE Ia SUPERNOVA,
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“These objects are thus the focus of many current and future dark-energy experiments (e.g., Astier et al. 2006; Riess et al. 2007; Wood-Vasey et al. 2007; Aldering 2005).”
BackgroundSelf-citationConley, A., Carlberg, R. G., Guy, J., Howell, D. A., Jha, S. W., Riess, A. G., & Sullivan, M. (2007) · The Astrophysical Journal · doi:10.1086/520625 · Cited by 160
“Note that SN cosmology analyses that restrict themselves to zmin & 0.015 such as Astier et al. (2006); Riess et al. (2007); Wood-Vasey et al. (2007) are not strongly affected by the existence of the bubble.”
BackgroundInfluentialSelf-citationFriedmann model with viscous cosmology in modified $$f(R,T)$$ f ( R , T ) gravity theory
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A Test of the Copernican Principle
Caldwell, R. R., & Stebbins, A. J. (2008) · Physical Review Letters · doi:10.1103/physrevlett.100.191302 · Cited by 158
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“This compilation of 557 supernovae includes data from Hamuy et al. (1996), Riess et al. (1999, 2007), Astier et al. (2006), Jha et al. (2006), Wood-Vasey et al. (2007), Holtzman et al. (2008), Hicken et al. (2009) and Kessler et al. (2009).”
MethodOPTICAL SPECTROSCOPY OF TYPE Ia SUPERNOVAE
Matheson, T., Kirshner, R., Challis, P., Jha, S. W., Garnavich, P., Berlind, P., Calkins, M. L., Blondin, S., Balog, Z., Bragg, A. E., et al. (2008) · The Astronomical Journal · doi:10.1088/0004-6256/135/4/1598 · Cited by 155
“Using SNe Ia as cosmological lighthouses led to a recent revolution in cosmology, with the discovery that the universe was accelerating (e.g., Riess et al. 1998, 2001, 2004, 2007; Perlmutter et al. ∗ Based in part on observations obtained at the F. L. Whipple Observatory, which is operated by the…”
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“…(Larson et al. 21 2011), the “Union 2” supernova dataset (hereafter SN), which includes 557 supernova from Hamuy et al. (1996); Riess et al. (1999); Riess et al. (2007); Astier et al. (2006); Jha et al. (2006); Wood-Vasey et al. (2007); Holtzman et al. (2008); Hicken et al. (2009); Kessler et…”
Self-citationBaryonic acoustic oscillations in 21-cm emission: a probe of dark energy out to high redshifts
Wyithe, J. S. B., Loeb, A., & Geil, P. M. (2007) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2007.12631.x · Cited by 155
“…have not incorporated additional sources of constraint on the dark energy equation of state at lower redshift, which could include observations of Type Ia supernovae (e.g. Riess et al. 2007; Zhao et al. 2007), or the BAO scale from galaxy redshift surveys (Cole et al. 2005; Eisenstein et al. 2005).”
BackgroundMethodBlake, C., Davis, T. M., Poole, G. B., Parkinson, D., Brough, S., Colless, M., Contreras, C., Couch, W. J., Croom, S. M., Drinkwater, M. J., et al. (2024) · doi:10.25916/sut.26215247.v1 · Cited by 155
Cosmological model from the holographic equipartition law with a modified Rényi entropy
KOMATSU, N. (2017) · The European Physical Journal C · doi:10.1140/epjc/s10052-017-4800-2 · Cited by 160
Confronting Lemaitre-Tolman-Bondi models with Observational CosmologyPreprint
García-Bellido, J., & Haugbølle, T. (2008) · Cited by 153
Influence of modification of gravity on the dynamics of radiating spherical fluids
Yousaf, Z., Bamba, K., & Bhatti, M. Z. U. H. (2016) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.93.064059 · Cited by 152
Jones, D. O., Scolnic, D. M., Riess, A. G., Rest, A., Kirshner, R., Berger, E., Kessler, R., Pan, Y. C., Foley, R. J., Chornock, R., et al. (2018) · The Astrophysical Journal · doi:10.3847/1538-4357/aab6b1 · Cited by 151
“D.S. is supported by NASA through Hubble Fellowship grant HST-HF2-51383.”
BackgroundInfluentialSelf-citationThe rise-time distribution of nearby Type Ia supernovae
Ganeshalingam, M., Li, W., & Filippenko, A. V. (2011) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2011.19213.x · Cited by 148
“…has led to the discovery of the accelerating expansion of the Universe (Riess et al. 1998; Perlmutter et al. 1999; see also Astier et al. 2006; Riess et al. 2007; Wood-Vasey et al. 2007; Kowalski et al. 2008; Hicken et al. 2009b; Amanullah et al. 2010), indicating either the presence of…”
BackgroundSelf-citationDISCOVERY OF A TIGHT CORRELATION FOR GAMMA-RAY BURST AFTERGLOWS WITH “CANONICAL” LIGHT CURVES
Dainotti, M. G., Willingale, R., Capozzıello, S., Cardone, V. F., & Ostrowski, M. (2010) · The Astrophysical Journal Letters · doi:10.1088/2041-8205/722/2/l215 · Cited by 148
“The detection of gamma-ray bursts (GRBs) up to high redshifts (z = 8.2; Salvaterra et al. 2009; Tanvir et al. 2009), larger than Type I supernovae Ia (SNeIa; zmax = 1.77; Riess et al. 2007), makes these objects appealing for possible use in cosmology.”
BackgroundInfluentialPHOTOMETRIC TYPE Ia SUPERNOVA CANDIDATES FROM THE THREE-YEAR SDSS-II SN SURVEY DATA
Sako, M., Bassett, B. A., Connolly, B., Dilday, B., Cambell, H., Frieman, J. A., Gladney, L., Kessler, R., Lampeitl, H., Marriner, J. P., et al. (2011) · The Astrophysical Journal · doi:10.1088/0004-637x/738/2/162 · Cited by 147
“1 by the Supernova Legacy Survey (SNLS; Astier et al. 2006; Guy et al. 2010; Conley et al. 2011), the ESSENCE SN Survey (Miknaitis et al. 2007; Wood-Vasey et al. 2007), the Carnegie Supernova Project High-z Program (Freedman et al. 2009); and finally 4) z & 1 SN Ia from space using the Hubble Space Telescope (Riess et…”
MethodCrossing of the phantom divide in modified gravity
Bamba, K., Geng, C.-Q., Nojiri, S., & Odintsov, S. D. (2009) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.79.083014 · Cited by 147
Dark Energy: Investigation and Modeling
Tsujikawa, S. (2011) · Astrophysics and space science library · doi:10.1007/978-90-481-8685-3_8 · Cited by 213
Daly, R. A., Djorgovski, S. G., Freeman, K. A., Mory, M. P., O’Dea, C. P., Kharb, P., & Baum, S. A. (2008) · The Astrophysical Journal · doi:10.1086/528837 · Cited by 146
“The recent data sets presented by Astier et al. (2006), Riess et al. (2007), Wood-Vasey et al. (2007), Davis et al. (2007), and Daly et al. (2008) have been analyzed by these groups and compared with models by other researchers.”
BackgroundResultInfluentialSelf-consistent cosmological simulations of DGP braneworld gravity
Schmidt, F. (2009) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.80.043001 · Cited by 146
THE EFFECT OF PECULIAR VELOCITIES ON SUPERNOVA COSMOLOGY
Davis, T. M., Hui, L., Frieman, J. A., Haugbølle, T., Kessler, R., Sinclair, B., Sollerman, J., Bassett, B. A., Marriner, J. P., Mörtsell, E., et al. (2011) · The Astrophysical Journal · doi:10.1088/0004-637x/741/1/67 · Cited by 156
“Since the SDSS sample concentrates on relatively nearby supernovae (0.05 <∼ z <∼ 0.4) the peculiar velocity contribution is a more significant proportion of the total redshift than in surveys that focus on higher redshifts such as ESSENCE (Wood-Vasey et al. 2007), SuperNova Legacy Survey (Astier et al. 2006), and High…”
BackgroundMethodInfluentialVERY EARLY ULTRAVIOLET AND OPTICAL OBSERVATIONS OF THE TYPE Ia SUPERNOVA 2009ig
Foley, R. J., Challis, P., Filippenko, A. V., Ganeshalingam, M., Landsman, W., Li, W., Marion, G. H. H., Silverman, J. M., Beaton, R. L., Bennert, V. N., et al. (2011) · The Astrophysical Journal · doi:10.1088/0004-637x/744/1/38 · Cited by 145
“Riess et al. 1998; Perlmutter et al. 1999; Riess et al. 2007; Wood-Vasey et al. 2007; Hicken et al. 2009; Kessler et al. 2009; Amanullah et al. 2010; Conley et al. 2011; Suzuki et al. 2011).”
BackgroundSelf-citationEntropic cosmology for a generalized black-hole entropy
KOMATSU, N., & KIMURA, S. (2013) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.88.083534 · Cited by 151
Anisotropic Dark Energy: Dynamics of Background and PerturbationsPreprint
Koivisto, T., & Mota, D. F. (2012) · Cited by 145
DARK MATTER INVESTIGATION BY DAMA AT GRAN SASSO
Bernabei, R., Belli, P., d'ANGELO, S., Marco, A. D., MONTECCHIA, F., Cappella, F., d'ANGELO, A., Incicchitti, A., Caracciolo, V., Castellano, S., et al. (2013) · International Journal of Modern Physics A · doi:10.1142/s0217751x13300226 · Cited by 143
Ellis, R. S., Sullivan, M., Nugent, P., Howell, D. A., Gal‐Yam, A., Astier, P., Balam, D., Balland, C., Basa, S., Carlberg, R. G., et al. (2008) · The Astrophysical Journal · doi:10.1086/524981 · Cited by 142
“However, very recently, as a result of a survey of high-redshift SNe Ia with the ACS grism onboard Hubble Space Telescope, Riess et al. (2007) have published the mean rest-frame UV spectrum of 13 SNe Ia more distant (z > 1) than those studied here; the average redshift of this sample is z=1.3.”
BackgroundMethodInfluentialLiving in a Void: Testing the Copernican Principle with Distant Supernovae
Clifton, T., Ferreira, P. G., & Land, K. (2008) · Physical Review Letters · doi:10.1103/physrevlett.101.131302 · Cited by 141
Cosmological evolution in exponential gravity
Bamba, K., Geng, C.-Q., & Lee, C.-C. (2010) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2010/08/021 · Cited by 148
Photometric calibration of the Supernova Legacy Survey fields
Regnault, N., Conley, A., Guy, J., Sullivan, M., Cuillandre, J., Astier, P., Balland, C., Basa, S., Carlberg, R. G., Fouchez, D., et al. (2009) · Astronomy and Astrophysics · doi:10.1051/0004-6361/200912446 · Cited by 138
Sánchez, A. G., Crocce, M., Cabré, A., Baugh, C. M., & GAZTAÑAGA, E. (2009) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2009.15572.x · Cited by 138
“…the Equation of State SupErNovae trace Cosmic Expansion (ESSENCE; Miknaitis et al. 2007), the high-redshift sample from the Hubble Space Telescope (Riess et al. 2004; Riess et al. 2007) as well as older data sets (Riess et al. 1998; Perlmutter et al. 1999; Tonry et al. 2003; Barris et al. 2004).”
BackgroundProbing Gravity with Spacetime Sirens
Deffayet, C., & Kristen Menou, A. (2007) · The Astrophysical Journal · doi:10.1086/522931 · Cited by 134
“A mea- surable dimming of distant type Ia supernovae (e.g., Astier et al. 2006; Riess et al. 2007; Wood-Vasey et al. 2007), CMB data (e.g., Spergel et al. 2007) and additional cosmological probes (e.g., Wright 2007) indicate that a repulsive ”dark energy” comprises 73% of the Universe’s content.”
BackgroundLocal void vs dark energy: confrontation with WMAP and type Ia supernovae
Alexander, S., Tirthabir Biswas, A., Notari, A., & Vaid, D. (2009) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2009/09/025 · Cited by 134
Establishing homogeneity of the universe in the shadow of dark energy
Clarkson, C. (2012) · Comptes Rendus Physique · doi:10.1016/j.crhy.2012.04.005 · Cited by 134
Differentiating dark energy and modified gravity with galaxy redshift surveys
Wang, Y. (2008) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2008/05/021 · Cited by 134
A measurement of the Hubble constant from Type II supernovae
de Jaeger, T., Stahl, B. E., Zheng, W., Filippenko, A. V., Riess, A. G., & Galbany, L. (2020) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/staa1801 · Cited by 165
“(6) As defined by Riess et al. (2007), q0 is the present acceleration (q0 = −0.55) and j0 is the prior deceleration ( j0 = 1).”
BackgroundInfluentialSelf-citationFigure of merit for dark energy constraints from current observational data
Wang, Y. (2008) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.77.123525 · Cited by 133
Testing the interaction between dark energy and dark matter via the latest observations
He, J.-H., Wang, B., & Elcio Abdalla, A. (2011) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.83.063515 · Cited by 132
The growth of matter perturbations inf(R) models
Gannouji, R., Moraes, B., & Polarski, D. (2009) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2009/02/034 · Cited by 139
The host galaxies of Type Ia supernovae discovered by the Palomar Transient Factory
Pan, Y. C., Sullivan, M., Maguire, K., Hook, I., Nugent, P., Howell, D. A., Arcavi, I., Botyanszki, J., Cenko, S. B., DeRose, J., et al. (2013) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stt2287 · Cited by 129
“…July 2018 1 IN T RO D U C T I O N Type Ia supernovae (SNe Ia) are remarkable cosmological standardizable candles that are routinely used to measure cosmological parameters (Riess et al. 1998; Perlmutter et al. 1999; Riess et al. 2007; Kessler et al. 2009; Sullivan et al. 2011b; Suzuki et al. 2012).”
BackgroundAverage observational quantities in the timescape cosmology
Wiltshire, D. L. (2009) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.80.123512 · Cited by 128
Lampeitl, H., Nichol, R. C., Seo, H., Giannantonio, T., Shapiro, C., Bassett, B. A., Percival, W. J., Davis, T. M., Dilday, B., Frieman, J. A., et al. (2009) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2009.15851.x · Cited by 125
“Recently, several dedicated SN surveys have been carried out to confirm and extend the earlier detections of an accelerating universe (HST, Riess et al. 2004, 2007; SNLS, Astier et al. 2006; ESSENCE, Wood-Vasey et al. 2007) as well as new compilations of existing SN datasets (Davis et al. 2007;…”
BackgroundSelf-citationScant evidence for thawing quintessence
Wolf, W. J., Garcia-Garcia, C., Bartlett, D., & Ferreira, P. G. (2024) · Physical Review D · doi:10.1103/physrevd.110.083528 · Cited by 106
Study of Bianchi I anisotropic model in f(R,T) gravity
Sharif, M., & Zubair, M. (2013) · Astrophysics and Space Science · doi:10.1007/s10509-013-1605-0 · Cited by 126
Supernova Cosmology: Legacy and Future
Goobar, A., & LEIBUNDGUT, B. (2011) · Annual Review of Nuclear and Particle Science · doi:10.1146/annurev-nucl-102010-130434 · Cited by 126
Model independentH(z) reconstruction using the cosmic inverse distance ladder
Lemos, P., Lee, E., Efstathiou, G., & Gratton, S. (2018) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/sty3082 · Cited by 126
“This dataset contains SNe spanning the redshift range 0.01 < z < 2.3 drawn from a number of surveys: The Pan-Starrs1 survey (Rest et al. 2014; Scolnic et al. 2014), CfA1-CfA4 (Riess et al. 1998; Jha et al. 2006; Hicken et al. 2009, 2012), CSP (Contreras et al. 2010; Folatelli et al. 2010; Stritzinger et al. 2011), SNL…”
BackgroundInfluentialTHE CHEMICAL ABUNDANCES OF TYCHO G IN SUPERNOVA REMNANT 1572
Hernández, J. I. G., Ruiz-Lapuente, P., Filippenko, A. V., Foley, R. J., Gal‐Yam, A., & Simon, J. D. (2009) · The Astrophysical Journal · doi:10.1088/0004-637x/691/1/1 · Cited by 124
“Larger, higher-quality samples of SNe Ia, together with other data, are now providing increasingly accurate and precise measurements of the dark energy equation-of-state parameter, w = P/(ρc2) (e.g., Astier et al. 2006; Riess et al. 2007; Wood-Vasey et al. 2007; Kowalski et al. 2008).”
BackgroundMethodSelf-citationObservational constraints on the dark energy and dark matter mutual coupling
Feng, C. Q., Wang, B., Elcio Abdalla, A., & Ru-keng Su, C. (2008) · Physics Letters B · doi:10.1016/j.physletb.2008.05.066 · Cited by 123
Simultaneous falsification of ΛCDM and quintessence with massive, distant clusters
Mortonson, M. J., Hu, W., & Dragan Huterer, A. (2011) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.83.023015 · Cited by 122
THE RISE AND FALL OF TYPE Ia SUPERNOVA LIGHT CURVES IN THE SDSS-II SUPERNOVA SURVEY
Hayden, B. T., Garnavich, P., Kessler, R., Frieman, J. A., Jha, S. W., Bassett, B. A., Cinabro, D., Dilday, B., Kasen, D., Marriner, J. P., et al. (2010) · The Astrophysical Journal · doi:10.1088/0004-637x/712/1/350 · Cited by 122
“…this result (Knop et al. 2003; Tonry et al. 2003; Barris et al. 2006; Riess et al. 2004), the focus has shifted to constraining the properties of dark energy (Garnavich et al. 1998b; Astier et al. 2006; Riess et al. 2007; Wood-Vasey et al. 2007; Miknaitis et al. 2007; Eisenstein et al. 2007).”
BackgroundSelf-citationTHE CARNEGIE SUPERNOVA PROJECT: FIRST NEAR-INFRARED HUBBLE DIAGRAM TOz∼ 0.7
Freedman, W. L., Burns, C. R., Phillips, M. M., Wyatt, P., Persson, S. E., Madore, B. F., Contreras, C., Folatelli, G., Gonzalez, E. S., Hamuy, M., et al. (2009) · The Astrophysical Journal · doi:10.1088/0004-637x/704/2/1036 · Cited by 122
Self-citationCDM accelerating cosmology as an alternative to ΛCDM model
Lima, J. A. S., de Jesus, J. F., & Oliveira, F. A. (2010) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2010/11/027 · Cited by 129
New Constraints on Dark Energy from the ObservedGrowth of the Most X-ray Luminous Galaxy Clusters
Mantz, A. B., Allen, S. W., Ebeling, H., & Rapetti, D. (2007) · OSTI OAI (U.S. Department of Energy Office of Scientific and Technical Information) · Cited by 121
Energy conditions in f (R, T, R μν T μν ) gravity
Sharif, M., & Zubair, M. (2013) · Journal of High Energy Physics · doi:10.1007/jhep12(2013)079 · Cited by 121
Accelerating cold dark matter cosmology (Ω Λ ≡ 0)
Lima, J. A. S., Silva, F. E., & Santos, R. C. (2008) · Classical and Quantum Gravity · doi:10.1088/0264-9381/25/20/205006 · Cited by 119
THE ABSOLUTE MAGNITUDES OF TYPE Ia SUPERNOVAE IN THE ULTRAVIOLET
Brown, P. J., Roming, P. W. A., Milne, P., Bufano, F., Ciardullo, R., Elias-Rosa, N., Filippenko, A. V., Foley, R. J., Gehrels, N., Gronwall, C. A., et al. (2010) · The Astrophysical Journal · doi:10.1088/0004-637x/721/2/1608 · Cited by 118
“…they have been used to constrain cosmological parameters such as H0, Ω, and Λ (Barris et al. 2004; Astier et al. 2006; Hicken et al. 2009b; Kessler et al. 2009; Riess et al. 2009) and the nature and evolution of dark energy (Riess et al. 2004, 2007; Wood-Vasey et al. 2007; Freedman et al. 2009).”
MethodSelf-citationCondensates in quantum chromodynamics and the cosmological constant
Brodsky, S. J., & Shrock, R. E. (2010) · Proceedings of the National Academy of Sciences · doi:10.1073/pnas.1010113107 · Cited by 117
A statistical analysis of circumstellar material in Type Ia supernovae
Maguire, K., Sullivan, M., Patat, F., Gal‐Yam, A., Hook, I., Dhawan, S., Howell, D. A., Mazzali, P. A., Nugent, P., Pan, Y. C., et al. (2013) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stt1586 · Cited by 117
“Type Ia supernovae (SNe Ia) are excellent standardisable candles and play an important role in constraining cosmological parameters (e.g., Riess et al. 1998, 2007; Perlmutter et al. 1999; Kessler et al. 2009; Sullivan et al. 2011; Suzuki et al. 2012).”
BackgroundImproved constraints on cosmological parameters from Type Ia supernova data
March, M. C., Trotta, R., Berkes, P., Starkman, G. D., & Vaudrevange, P. M. (2011) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2011.19584.x · Cited by 117
Self-tuning vacuum variable and cosmological constant
Klinkhamer, F. R., & Воловик, Г. Е. (2008) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.77.085015 · Cited by 131
“The homogeneity assumption is indeed supported by the observed flatness and smoothness of our universe [12, 13, 14].”
BackgroundInfluentialAn updated gamma-ray bursts Hubble diagram
Cardone, V. F., Capozziello, S., & Dainotti, M. G. (2009) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2009.15456.x · Cited by 130
“The astrophysical data coming from later SNeIa samples (Riess et al. 2007; Astier et al. 2006; Wood -Vasey et al. 2007; ?”
MethodThermodynamics in F(R) gravity with phantom crossing
Bamba, K., & Geng, C.-Q. (2009) · Physics Letters B · doi:10.1016/j.physletb.2009.07.039 · Cited by 116
Realistic stellar anisotropic model satisfying Karmarker condition in f(R, T) gravity
Mustafa, G., Zubair, M., Waheed, S., & Tiecheng, X. (2020) · The European Physical Journal C · doi:10.1140/epjc/s10052-019-7588-4 · Cited by 115
COSMOLOGY WITH PHOTOMETRICALLY CLASSIFIED TYPE Ia SUPERNOVAE FROM THE SDSS-II SUPERNOVA SURVEY
Campbell, H. C., D’Andrea, C. B., Nichol, R. C., Sako, M., Smith, M., Lampeitl, H., Olmstead, M. D., Bassett, B. A., Biswas, R., Brown, P. J., et al. (2013) · The Astrophysical Journal · doi:10.1088/0004-637x/763/2/88 · Cited by 114
“The Hubble Space Telescope Program (GOODS SN sample; Riess et al. 2004, 2007), Supernovae Cosmology Project (SCP or HST Clus- ter SN sample; Knop et al. 2003; Kowalski et al. 2008; Amanullah et al. 2010; Suzuki et al. 2011), the Supernova Legacy Survey (SNLS; Guy et al. 2010), and Equation of State: SupErNovae trace C…”
MethodInfluentialSelf-citationCuesta, A. J., Verde, L., Riess, A. G., & Jiménez, R. (2015) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stv261 · Cited by 113
“1 (e.g., Betoule et al. 2014; Riess et al. 2007; Hicken et al. 2009; Conley et al. 2011; Suzuki et al. 2012; Sako et al. 2014).”
Self-citation
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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