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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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Cites
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Demiański, M., Piedipalumbo, E., Sawant, D., & Amati, L. (2021) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stab1669 · Cited by 43
Early dark energy at high redshifts: status and perspectives
Xia, J., & Viel, M. (2009) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2009/04/002 · Cited by 43
“dw/dz ≫ 1) seems to be ruled out by high-redshift SNIa [23].”
Testing the distance-duality relation with a combination of cosmological distance observations
Cao, S., & Liang, N. (2011) · Research in Astronomy and Astrophysics · doi:10.1088/1674-4527/11/10/008 · Cited by 43
“The first direct evid nce for cosmic acceleration came from Type Ia Supernave (SNe Ia) (Riess, 1998; Perlmutter et al., 1999), which have provided the strongest constraints on the cosmological parameters (Riess et al., 2004, 2007; Astier et al., 2006; Wood-Vasey et al., 2007; Kowalski et al., 2008).”
BackgroundDynamics of a magnetized Bianchi I universe with vacuum energy
King, E. J., & Coles, P. (2007) · Classical and Quantum Gravity · doi:10.1088/0264-9381/24/8/008 · Cited by 43
f(R) gravity theories in the Palatini formalism constrained from strong lensing
Yang, X.-J., & Chen, D.-M. (2009) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2008.14318.x · Cited by 43
“…results that support this discovery are: the luminosity-redshift relationship from SNIa surveys (Astier et al. 2006; Perlmutter et al. 1999; Riess et al. 1998, 2004, 2007),the CMB anisotropy spectrum (de Bernardis et al. 2000; Spergel et al. 2003, 2007; Hinshaw et al. 2007), the large…”
ResultBEYOND H 0 AND q 0 : COSMOLOGY IS NO LONGER JUST TWO NUMBERS
Neben, A. R., & Turner, M. S. (2013) · The Astrophysical Journal · doi:10.1088/0004-637x/769/2/133 · Cited by 43
“…velocity scatter to the redshift data, giving the mock measurement of redshift: (z + 1)(zpec + 1) − 1, where each zpec is chosen from a Gaussian distribution centered at zero with σpec = 300 km s−1 (e.g., Riess et al. 2004, 2007; Rapetti et al. 2007; Hicken et al. 2009b; Lampeitl et al. 2010).”
BackgroundConstraining chameleon field driven warm inflation with Planck 2018 data
Sheikhahmadi, H., Mohammadi, A., Aghamohammadi, A., Harko, T., Herrera, R., Corda, C., Abebe, A., & Saaidi, K. (2019) · The European Physical Journal C · doi:10.1140/epjc/s10052-019-7571-0 · Cited by 46
Physical properties of class I compact star model for linear and Starobinsky − f ( R , T ) functions
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Testing the DGP model with ESSENCE
Rydbeck, S., Fairbairn, M., & Goobar, A. (2007) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2007/05/003 · Cited by 43
“The Riess et al 07 gold sample contains supernovae from the Supernova Cosmology Project, SNLS, the High-Z Team, the GOODS transient survey, and includes 21 new supernovae at extremely high redshift obtained with the Hubble Space Telescope.”
The ESO/VLT 3rd year Type Ia supernova data set from the supernova legacy survey
Balland, C., Baumont, S., Basa, S., Mouchet, M., Howell, D. A., Astier, P., Carlberg, R. G., Conley, A., Fouchez, D., Guy, J., et al. (2009) · Springer Link (Chiba Institute of Technology) · doi:10.1051/0004-6361/200912246/pdf · Cited by 43
Bayesian Evidence for a cosmological constant using new high-redshift supernova data
Serra, P., Heavens, A., & MELCHIORRI, A. (2007) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2007.11924.x · Cited by 43
“In particular we compare the luminosity distance at redshift z of each model given by dL(z) = c(1 + z) Z z 0 dz′ H(z′) (11) with the SN-Ia luminosity distances from the latest catalogue of Riess et al. (2007).”
MethodResultInfluentialSauer, D., Mazzali, P. A., Blondin, S., Stehle, M., Benetti, S., Challis, P., Filippenko, A. V., Kirshner, R., Li, W., & Matheson, T. (2008) · Cited by 43
Self-citationTension in the recent Type Ia supernovae datasets
Wei, H. (2010) · Physics Letters B · doi:10.1016/j.physletb.2010.03.015 · Cited by 42
Casimir effect in de Sitter space–time with compactified dimension
SAHARIAN, A. A., & Setare, M. R. (2007) · Physics Letters B · doi:10.1016/j.physletb.2007.10.050 · Cited by 43
Emergent physics: Fermi-point scenario
Воловик, Г. Е. (2008) · Philosophical Transactions of the Royal Society A Mathematical Physical and Engineering Sciences · doi:10.1098/rsta.2008.0070 · Cited by 42
Supernovae as seen by off-center observers in a local void
Blomqvist, M., & Mörtsell, E. (2010) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2010/05/006 · Cited by 42
“The data set consists of 397 SNe Ia and extends the previously available Union set [31] (which includes many SNe Ia from ESSENCE, SNLS and HST) by adding 90 SNe Ia at low reshifts discovered by the CfA3 [32].”
GLOBAL AND LOCAL EFFECTS OF ROTATION: OBSERVATIONAL ASPECTS
Godłowski, W. (2011) · International Journal of Modern Physics D · doi:10.1142/s0218271811019475 · Cited by 41
“For Ωm,0 = 0.30 (Perlmutter et al. 1998, 1999, Riess et al. 1998, 2004, 2007) the value of the Hubble constant is H0 = 65 kms −1Mpc−1, but then for the flat Universe in the classic scenario of dark cold matter with a cosmological constant (ΛCDM) there is a discrepancy between the theoretical…”
BackgroundInfluentialLennarz, D., Altmann, D., & Wiebusch, C. H. (2011) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201117666 · Cited by 41
“About 300 SNe from high-redshift surveys are not covered (Riess et al. 2007; Guy et al. 2010).”
BackgroundTesting dynamical vacuum models with CMB power spectrum from Planck
Tsiapi, P., & Basilakos, S. (2019) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stz540 · Cited by 41
Berkeley supernova Ia program: data release of 637 spectra from 247 Type Ia supernovae
Stahl, B. E., Zheng, W., de Jaeger, T., Brink, T. G., Filippenko, A. V., Silverman, J. M., Cenko, S. B., Clubb, K. I., Graham, M. L., Halevi, G., et al. (2020) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/staa102 · Cited by 41
“SNe Ia have since been used to place increasingly stringent constraints on cosmological parameters (Astier et al. 2006; Riess et al. 2007; Hicken et al. 2009; Suzuki et al. 2012; Betoule et al. 2014; Jones et al. 2018; Scolnic et al. 2018) and continue to provide precise measurements of the Hubble…”
BackgroundSelf-citationBounce cosmology in $$f({\mathcal {R}})$$ gravity
Ilyas, M., & Rahman, W. U. (2021) · The European Physical Journal C · doi:10.1140/epjc/s10052-021-08955-7 · Cited by 41
Chemical potential and the nature of dark energy: The case of a phantom field
Lima, J. A. S., & Pereira, S. H. (2008) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.78.083504 · Cited by 41
USING A PHENOMENOLOGICAL MODEL TO TEST THE COINCIDENCE PROBLEM OF DARK ENERGY
Chen, Y., Zhu, Z., Alcaniz, J. S., & Gong, Y. (2010) · The Astrophysical Journal · doi:10.1088/0004-637x/711/1/439 · Cited by 41
“…SNeIa (Riess et al. 1998; Perlmutter et al. 1999), and they have provided the strongest constraints on the cosmic equation of state and other cosmological parameters (Riess et al. 2004, 2007; Astier et al. 2006; Wood-Vasey et al. 2007; Davis et al. 2007; Kowalski et al. 2008; Hicken et al. 2009).”
BackgroundCONSTRAINING THE DARK ENERGY EQUATION OF STATE WITH COSMIC VOIDSPreprint
Lee, J., & Park, D. (2013) · Cited by 41
Casertano, S., Anand, G., Anderson, R. I., Beaton, R. L., Bhardwaj, A., Blakeslee, J. P., Boubel, P., Breuval, L., Brout, D., Cantiello, M., et al. (2026) · Astronomy and Astrophysics · doi:10.1051/0004-6361/202557993 · Cited by 40
Self-citationCasimir effect for parallel plates in de Sitter spacetime
Elizalde, E., SAHARIAN, A. A., & Vardanyan, T. (2010) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.81.124003 · Cited by 40
Measuring dark energy spatial inhomogeneity with supernova data
Cooray, A. R., HOLZ, D. E., & Caldwell, R. R. (2010) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2010/11/015 · Cited by 40
COSMIC CONSTRAINTS ON DECELERATION PARAMETER WITH Sne Ia AND CMB
Xu, L., & Lu, J. (2009) · Modern Physics Letters A · doi:10.1142/s0217732309027212 · Cited by 40
Non-minimal derivative coupling gravity in cosmology
Gumjudpai, B., & Rangdee, P. (2015) · General Relativity and Gravitation · doi:10.1007/s10714-015-1985-2 · Cited by 40
Transition redshift: new constraints from parametric and nonparametric methods
Rani, N., Jain, D., Mahajan, S., Mukherjee, A., & Pires, N. (2015) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2015/12/045 · Cited by 40
Mukherjee, P., & Banerjee, N. (2022) · Physics of the Dark Universe · doi:10.1016/j.dark.2022.100998 · Cited by 49
Brane assisted quintessential inflation with transient acceleration
Bento, M. C., Felipe, R. G., & Santos, N. M. C. (2008) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.77.123512 · Cited by 41
Dark energy, gravitation and supernovae
Ruiz-Lapuente, P. (2007) · Classical and Quantum Gravity · doi:10.1088/0264-9381/24/11/r01 · Cited by 40
Observational constraints of modified Chaplygin gas in loop quantum cosmology
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Dossett, J., Moldenhauer, J., & Ishak, M. (2011) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.84.023012 · Cited by 28
Cooke, J., Ellis, R. S., Sullivan, M., Nugent, P., Howell, D. A., Gal-Yam, A., Lidman, C. E., Bloom, J. S., Cenko, S. B., Kasliwal, M. M., et al. (2011) · The Astrophysical Journal Letters · doi:10.1088/2041-8205/727/2/l35 · Cited by 39
“Measures of distant events are being used to distinguish between Einstein’s cosmological constant, Λ, and a scalar field whose equation of state parameter w 6=−1 (Astier et al. 2006; Riess et al. 2007; Kessler et al. 2009; Amanullah et al. 2010).”
MethodThe periodic universe with varying deceleration parameter of the second degree
Bakry, M. A., & Shafeek, A. T. (2019) · Astrophysics and Space Science · doi:10.1007/s10509-019-3625-x · Cited by 39
“…or independent analyses of the cosmological observations, the transition redshift of the accelerating expansion is given by zt = 0.43 ± 0.07 (Riess et al. 2007), the accelerating expansion in our model at ta1 = 0.18, and za1 = 0.43, our model enters into a strongexponential tse = 0.42,…”
MethodInfluentialEffects of Supernova Redshift Uncertainties on the Determination of Cosmological Parameters
Steinhardt, C. L., Sneppen, A., & Sen, B. (2020) · The Astrophysical Journal · doi:10.3847/1538-4357/abb140 · Cited by 40
“…about the necessity of obtaining additional spectra and the most suitable telescopes, exposure times, and resolutions for follow-up spectroscopy (Riess et al. 1999, 2007, 2018b; Pritchet & SNLS Collaboration 2004; Jha et al. 2006; Hicken et al. 2009, 2012; Contreras et al. 2010; Morokuma et al.…”
BackgroundAstronomical Distance Determination in the Space Age
Czerny, B., Beaton, R. L., Bejger, M., Cackett, E. M., Dall’Ora, M., Holanda, R. F. L., Jensen, J. B., Jha, S. W., Lusso, E., Minezaki, T., et al. (2018) · Space Science Reviews · doi:10.1007/s11214-018-0466-9 · Cited by 39
Self-citationCosmological perturbations in models of coupled dark energy
Chongchitnan, S. (2009) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.79.043522 · Cited by 39
Near-IR search for lensed supernovae behind galaxy clusters
Goobar, A., Paech, K., Stanishev, V., Amanullah, R., Dahlén, T., Jönsson, J., Kneib, J., Lidman, C. E., Limousin, M., Mörtsell, E., et al. (2009) · Astronomy and Astrophysics · doi:10.1051/0004-6361/200811254 · Cited by 39
“For higher redshifts, Riess et al. (2007) demonstrated the power f space measurements by reporting the discovery and analysisof 23 Type Ia SNe withz ≥ 1, although not without significant effort.”
BackgroundGALEX Spectroscopy of SN 2005ay Suggests Ultraviolet Spectral Uniformity among Type II-P Supernovae
Gal‐Yam, A., Bufano, F., Barlow, T. A., Baron, E., Benetti, S., Cappellaro, E., Challis, P. J., Ellis, R. S., Filippenko, A. V., Foley, R. J., et al. (2008) · The Astrophysical Journal · doi:10.1086/592744 · Cited by 39
“These include both samples currently assembled using the Hubble Space Telescope (HST; e.g., GOODS, Dahlen et al. 2004; Riess et al. 2007) and from the ground (e.g., Poznanski et al. 2007a), and future datasets expected to emerge from a possible JDEM mission that includes a SN component and from…”
MethodSelf-citationComparison of recent SnIa datasets
Sánchez, J. C. B., Nesseris, S., & Perivolaropoulos, L. (2009) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2009/11/029 · Cited by 38
Gauss-Bonnet chameleon mechanism of dark energy
Ito, Y., & Nojiri, S. (2009) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.79.103008 · Cited by 38
Bouncing universe and reconstructing vector field
Sadeghi, J., Setare, M. R., Amani, A., & Noorbakhsh, S. M. (2010) · Physics Letters B · doi:10.1016/j.physletb.2010.01.071 · Cited by 38
Cosmological constraints on neutrino plus axion hot dark matterPreprint
Hannestad, S., Mirizzi, A., Raffelt, G. G., & Wong, Y. Y. Y. (2007) · Cited by 38
Li, H., Xia, J., Zhao, G., Fan, Z., & Zhang, X. (2008) · The Astrophysical Journal · doi:10.1086/591082 · Cited by 37
“Since the purpose of this paper is not to make a global analysis, in order to see the effects of the other cosmological data, we include the gold sample of 182 SN Ia (Riess et al. 2007) for a joint constraint on EoS of dark energy in the combination with the WMAP5 data.”
MethodPERTURBATIONS OF SNe Ia LIGHT CURVES, COLORS, AND SPECTRAL FEATURES BY CIRCUMSTELLAR DUST
Amanullah, R., & Goobar, A. (2011) · The Astrophysical Journal · doi:10.1088/0004-637x/735/1/20 · Cited by 37
“SNe Ia remain among the best tools to investigate the energy content of the universe, as demonstrated by recent very successful surveys of highz SNe (Astier et al. 2006; Wood-Vasey et al. 2007; Riess et al. 2007; Kowalski et al. 2008; Kessler et al. 2009; Amanullah et al. 2010).”
BackgroundWeak lensing signal in unified dark matter models
Camera, S., Bertacca, D., Diaferio, A., Bartolo, N., & Matarrese, S. (2009) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2009.15326.x · Cited by 38
“However, a number of independent data sets, the distance modulus from Supernovæ Ia used as standard candles (Riess et al. 1998; Knop et al. 2003; Riess et al. 2004, 2007), the Cosmic Microwave Background (CMB) anisotropies (de Bernardis et al. 2000; Bennett et al. 2003; Spergel et al. 2003; Hinshaw…”
MethodA simultaneous search for high-z LAEs and LBGs in the SHARDS survey
Haro, P. A., Rodríguez-Espinosa, J. M., Muñoz-Tuñón, C., Pérez‐González, P. G., Dannerbauer, H., Bongiovanni, A. M., Barro, G., Cava, A., Lumbreras-Calle, A., Hernán-Caballero, A., et al. (2018) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/sty1106 · Cited by 37
“We have also made use of additional public data from HST/ACS (Giavalisco et al. 2004b; Riess et al. 2007), MNRAS 000, 1–18 (2018) HST/WFC3 (Grogin et al. 2011; Koekemoer et al. 2011), Subaru/Suprime-Cam (as a part of the Hawaii Hubble Deep Field North project, Capak et al. 2004), Subaru/MOIRCS…”
MethodSupernova tests of the timescape cosmology
Smale, P. R., & Wiltshire, D. L. (2011) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2010.18142.x · Cited by 37
“Leith, Ng & Wiltshire (2008) considered some preliminary quantitative tests of the TS model, concentrating in particular on the fit of the 182 SN Ia distance moduli in the Gold dataset of Riess et al. (2007) (Riess07).”
BackgroundMethodResultInfluentialNew parametrization for the scale dependent growth function in general relativity
Dent, J. B., Dutta, S., & Perivolaropoulos, L. (2009) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.80.023514 · Cited by 37
Spatially Hyperbolic Gravitating Sources in Λ-Dominated Era
Yousaf, Z. (2022) · Universe · doi:10.3390/universe8020131 · Cited by 36
THE CHANGING FRACTIONS OF TYPE IA SUPERNOVA NUV–OPTICAL SUBCLASSES WITH REDSHIFT
Milne, P. A., Foley, R. J., Brown, P. J., & Narayan, G. (2015) · The Astrophysical Journal · doi:10.1088/0004-637x/803/1/20 · Cited by 36
“Riess et al. (2007) obtained HST photometry and spectra of high-z SNe Ia with redshifts exceeding z ≥ 0.6.”
BackgroundInfluentialSelf-citationConstraining non-minimally coupled tachyon fields by the Noether symmetry
de Souza, R. C., & Kremer, G. M. (2009) · Classical and Quantum Gravity · doi:10.1088/0264-9381/26/13/135008 · Cited by 36
Chand, A., Mishra, R. K., & Pradhan, A. (2016) · Astrophysics and Space Science · doi:10.1007/s10509-015-2579-x · Cited by 35
“(Riess et al. 2007).”
Waheed, S. (2020) · The European Physical Journal Plus · doi:10.1140/epjp/s13360-019-00028-9 · Cited by 36
Two-fluid atmosphere from decelerating to accelerating Friedmann–Robertson–Walker dark energy models
Pradhan, A. (2013) · Indian Journal of Physics · doi:10.1007/s12648-013-0399-9 · Cited by 36
A PRELIMINARY ANALYSIS OF THE ENERGY TRANSFER BETWEEN THE DARK SECTORS OF THE UNIVERSE
Zhou, J., Wang, B., Pavón, D., & Elcio Abdalla, A. (2009) · Modern Physics Letters A · doi:10.1142/s0217732309030308 · Cited by 36
Affine parametrization of the dark sector: Constraints from WMAP5 and SDSS
Pietrobon, D., Balbi, A., Bruni, M., & Quercellini, C. (2008) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.78.083510 · Cited by 36
Constraining the evolution of dark energy with type Ia supernovae and gamma-ray bursts
Qi, S., Wang, F.-Y., & Lu, T. (2008) · Astronomy and Astrophysics · doi:10.1051/0004-6361:20079329 · Cited by 36
“This approach was proposed by Huterer & Starkman (2003) and Huterer & Cooray (2005) and has been adopted in previous analyses using SNe Ia (Riess et al. 2007; Sullivan et al. 2007a).”
BackgroundMethodResultInfluentialThe fermionic Casimir effect in toroidally compactified de Sitter spacetime
Saharian, A. A. (2008) · Classical and Quantum Gravity · doi:10.1088/0264-9381/25/16/165012 · Cited by 37
Beyond Two Dark Energy Parameters
Sarkar, D., Sullivan, S. T., Joudaki, S., Amblard, A., HOLZ, D. E., & Cooray, A. R. (2008) · Physical Review Letters · doi:10.1103/physrevlett.100.241302 · Cited by 36
Lectures on Dark Energy and Cosmic AccelerationPreprint
Frieman, J. A. (2013) · Cited by 36
Narrowing Constraints with Type Ia Supernovae: Converging on a Cosmological ConstantPreprint
Sullivan, S., Cooray, A. R., & HOLZ, D. E. (2012) · Cited by 36
Probing the existence of the ZTF Casimir wormholes in the framework of f(R) gravity
Sokoliuk, O., Baransky, A., & Sahoo, P. K. (2022) · Nuclear Physics B · doi:10.1016/j.nuclphysb.2022.115845 · Cited by 35
The crossing statistic: dealing with unknown errors in the dispersion of Type Ia supernovae
Shafieloo, A., Clifton, T., & Ferreira, P. G. (2011) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2011/08/017 · Cited by 35
Constraints on w0 and wa of dark energy from high-redshift gamma-ray bursts
Tsutsui, R., Nakamura, T., Yonetoku, D., Murakami, T., Tanabe, S., Kodama, Y., & Takahashi, K. (2009) · Monthly Notices of the Royal Astronomical Society Letters · doi:10.1111/j.1745-3933.2008.00604.x · Cited by 35
“In our previous paper (Kodama et al. 2008), we calibrated the peak energy-peak luminosity relation of GRBs with 33 nearby events (z < 1.62) whose luminosity distances were estimated from those of large amount of SNeIa (Riess et al. 2007; Wood-Vasey et al. 2007; Davis et al. 2007).”
BackgroundMethodInfluentialThermonuclear explosions of rapidly rotating white dwarfs
Pfannes, J. M. M., Niemeyer, J. C., Schmidt, W., & Klingenberg, C. (2009) · Astronomy and Astrophysics · doi:10.1051/0004-6361/200912032 · Cited by 35
Hybrid star model with quark matter and baryonic matter in minimally coupled f ( R ) gravity
Abbas, G., & Nazar, H. (2020) · Annals of Physics · doi:10.1016/j.aop.2020.168336 · Cited by 35
Cosmic age, statefinder, and O m diagnostics in the decaying vacuum cosmology
Tong, M., & Zhang, Y. (2009) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.80.023503 · Cited by 35
Hybrid natural inflation from non-Abelian discrete symmetry
Ross, G. G., & Germán, G. (2010) · Physics Letters B · doi:10.1016/j.physletb.2010.01.003 · Cited by 38
Reconstruction of k-essence model
Matsumoto, J., & Nojiri, S. (2010) · Physics Letters B · doi:10.1016/j.physletb.2010.03.030 · Cited by 35
Gravitational lensing in the supernova legacy survey (SNLS)
Kronborg, T., Hardin, D., Guy, J., Astier, P., Balland, C., Basa, S., Carlberg, R. G., Conley, A., Fouchez, D., Hook, I., et al. (2010) · Astronomy and Astrophysics · doi:10.1051/0004-6361/200913618 · Cited by 35
“C O Riess et al., 2007; Freedman et al., 2009; Kessler et al., 2009).”
Couplings between holographic dark energy and dark matter
Ma, Y.-Z., Gong, Y., & Chen, X. (2010) · The European Physical Journal C · doi:10.1140/epjc/s10052-010-1408-1 · Cited by 35
Dynamics of holographic vacuum energy in the DGP model
Wu, X., Cai, R.-G., & Zhu, Z. (2008) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.77.043502 · Cited by 37
Direction dependence and non-Gaussianity in the high-redshift supernova data
Gupta, S., Saini, T. D., & Laskar, T. (2008) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2008.13377.x · Cited by 35
“The combined analysis of high-redshift supernova data (Riess et al. 1998, 2002; Perlmutter et al. 1999; Riess et al. 2004, hereafter GD04; Riess et al. 2007, hereafter GD07), along with observations of cosmic microwave background (Benoit et al. 2003; Page et al. 2007) or large-scale structure…”
BackgroundQuantifying systematic uncertainties in supernova cosmology
Nordin, J., Goobar, A., & Jönsson, J. (2008) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2008/02/008 · Cited by 35
“…of this paper is twofold: to present a method to investigate the impact on the estimation of cosmological parameters due to a number of systematic effects and, as an example, investigate the potential impact of systematic uncertainties in the cosmology fits of the Gold data-set of Riess et al 2007.”
MethodDES Collaboration, Abbott, T. M. C., Acevedo, M., Aguena, M., Alarcon, A., Allam, S., Alves, O., Amon, A., Andrade-Oliveira, F., Annis, J., et al. (2024) · arXiv (Cornell University) · doi:10.48550/arxiv.2401.02929 · Cited by 35
Self-citationAn updated measurement of the Hubble constant from near-infrared observations of Type Ia supernovae
Galbany, L., de Jaeger, T., Riess, A. G., Müller-Bravo, T. E., Dhawan, S., Phan, K., Stritzinger, M. D., Karamehmetoglu, E., LEIBUNDGUT, B., Burns, C. R., et al. (2023) · Astronomy and Astrophysics · doi:10.1051/0004-6361/202244893 · Cited by 34
Self-citationEvolution of non-static fluid for irreversible gravitational radiation in Palatini F(R) gravity
Asad, H., Yousaf, M., Almutairi, B. N., Zahid, L., & Khan, A. S. (2024) · Physics of the Dark Universe · doi:10.1016/j.dark.2024.101666 · Cited by 34
Demiański, M., & Piedipalumbo, E. (2011) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2011.18975.x · Cited by 34
“Parameters of this model are fixed by fitting appropriate estimates to the set of type Ia supernovae data, the power spectrum of CMB temperature anisotropies and parameters of the observed large scale structure (see (Demianski et al. 2005)), which has been recently referred as fiducial model to standardize the GRBs an…”
ResultCosmological models with viscous fluid and variable deceleration parameter
Tiwari, R. K., Beesham, A., & Shukla, B. K. (2017) · The European Physical Journal Plus · doi:10.1140/epjp/i2017-11289-y · Cited by 34
Bayesian comparison of interacting scenarios
Cid, A., Santos, B., Pigozzo, C., Ferreira, T., & Alcaniz, J. S. (2019) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2019/03/030 · Cited by 34
Measure of complexity in self-gravitating systems using structure scalars
Yousaf, Z., Bamba, K., Bhatti, M. Z. U. H., & Hassan, K. (2020) · New Astronomy · doi:10.1016/j.newast.2020.101541 · Cited by 34
“Baryon Acoustic oscillations, clusters of galaxies and Type Ia supernovae are some of the most important confirmations for the accelerated expansion of universe [29–31].”
BackgroundThe Lyman Continuum Escape Fraction of Galaxies and AGN in the GOODS Fields
Smith, B. M., Windhorst, R. A., Cohen, S. H., Koekemoer, A. M., Jansen, R. A., White, C., Borthakur, S., Hathi, N. P., Jiang, L., Rutkowski, M. J., et al. (2020) · The Astrophysical Journal · doi:10.3847/1538-4357/ab8811 · Cited by 34
Luminosity distance and anisotropic sky-sampling at low redshifts: A numerical relativity study
Macpherson, H. J., & Heinesen, A. (2021) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.104.023525 · Cited by 34
Kazantzidis, L., & Perivolaropoulos, L. (2021) · Springer eBooks · doi:10.1007/978-3-030-83715-0_33 · Cited by 41
Elcio Abdalla, A., Graef, L. L., & Wang, B. (2013) · Physics Letters B · doi:10.1016/j.physletb.2013.08.011 · Cited by 34
Tsutsui, R., Nakamura, T., Yonetoku, D., Murakami, T., Kodama, Y., & Takahashi, K. (2009) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2009/08/015 · Cited by 34
“In our previous papers (Kodama et al. 2008; Tsutsui et al. 2009), we calibrated the relation between peak energy Ep and peak luminosity Lp of prompt GRB emission (so called Yonetoku relation (Yonetoku et al. 2004)) by 33 low-redshift GRBs (z < 1.62) whose luminosity distances were estimated from SNeIa (Riess et al. 20…”
MethodInfluentialStatefinder diagnosis for holographic dark energy models in modified f ( R , T ) $f(R,T)$ gravity
Singh, C. P., & Kumar, P. (2016) · Astrophysics and Space Science · doi:10.1007/s10509-016-2740-1 · Cited by 34
“…believed that the Universe has entered a phase of the accelerated expansion which has been confirmed by the recent observations like supernovae Ia (Riess et al. 2007; Suzuki et al. 2012), cosmic microwave background radiation (Bennett et al. 2003; Komatsu et al. 2011), baryon acoustic B C.P.…”
BackgroundDiversity of Decline Rate–corrected Type Ia Supernova Rise Times: One Mode or Two?
Strovink, M. (2007) · The Astrophysical Journal · doi:10.1086/523089 · Cited by 34
“In cosmological studies, SNe Ia are prized for their use as standardizable candles to trace the history of cosmic expansion (Riess et al. 1998, 2007; Perlmutter et al. 1999; for a review, see Perlmutter & Schmidt 2003); in this context, periods of greater SN uniformity are of greater value.”
BackgroundHow strong is the evidence for accelerated expansion?
Seikel, M., & Schwarz, D. J. (2008) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2008/02/007 · Cited by 34
“For the analysis we take the following SN Ia data sets: Gold 2007 (MLCS2k2): the Gold sample by Riess et al. (2007) [5], which was obtained by using the MLCS2k2 fitting method ESSENCE (MLCS2k2): the set given by Wood-Vasey et al. (2007) [6], which includes data from ESSENCE, SNLS [4] and nearby SNe…”
MethodAditya, Y., & Reddy, D. R. K. (2019) · Astrophysics and Space Science · doi:10.1007/s10509-018-3491-y · Cited by 33
Cosmography with cluster strong lensing
Gilmore, J. B., & Natarajan, P. (2009) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2009.14612.x · Cited by 33
“…expansion of the Universe inferred from the Hubble diagram for SN type Ia (Riess et al. 1998; Perlmutter et al. 1999; Tonry et al. 2003; Riess et al. 2004, 2007) combined with constraints from Cosmic Microwave Background Radiation from the Wilkinson Microwave Anisotropy Probe (Spergel…”
On the nature of dark energy: the lattice Universe
Villata, M. (2013) · Astrophysics and Space Science · doi:10.1007/s10509-013-1388-3 · Cited by 33
“Due to the various well-known problems affecting low-redshift SNe Ia (see e.g. Riess et al. 2007; Kessler et al. 2009; Conley et al. 8 2011), we excluded events withz < 0.02 (36 out of 472, cyan symbols in the figure) from the fitting procedure.”
BackgroundInfluentialInduced cosmological constant and other features of asymmetric brane embedding
Shtanov, Y., Varun Sahni, A., Shafieloo, A., & TOPORENSKY, A. V. (2009) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2009/04/023 · Cited by 36
The growth factor of matter perturbations in f(R) gravity
Fu, X., Wu, P., & Yu, H. (2010) · The European Physical Journal C · doi:10.1140/epjc/s10052-010-1324-4 · Cited by 36
Supernovae data and perturbative deviation from homogeneity
Enqvist, K., Mattsson, M., & Rigopoulos, G. (2009) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2009/09/022 · Cited by 33
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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