The DOI matches its Crossref record; 104 of the 104 references it cites were found in a registry or an index.
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.
Overview
The claims and statistics of this paper haven’t been checked yet.
Run the check — free, no account needed. It reads the open-access text and checks the sources it cites.
Integrity signals
Registry
Cites
Statistics
Verification
Claims the paper makes
The claims and statistics of this paper haven’t been checked yet.
Run the check — free, no account needed. It reads the open-access text and checks the sources it cites.
Claims other papers make about this one
Each is checked against this paper’s own text: does it say what the citing paper says it does?
In the citing paper
“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
Self-check
Percentages, sums and reported differences re-computed from the paper’s own numbers.
The self-check needs the paper’s full text.
Citations
Cites
Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
Riess, A. G., Filippenko, A. V., Challis, P., Clocchiatti, A., Diercks, A., Garnavich, P. M., Gilliland, R. L., Hogan, C. J., Jha, S., Kirshner, R. P., et al. (1998) · The Astronomical Journal · doi:10.1086/300499 · Cited by 19,704
Self-citationMeasurements of Ω and Λ from 42 High‐Redshift Supernovae
Perlmutter, S., Aldering, G., Goldhaber, G., Knop, R. A., Nugent, P., Castro, P. G., Deustua, S., Fabbro, S., Goobar, A., Groom, D. E., et al. (1999) · The Astrophysical Journal · doi:10.1086/307221 · Cited by 18,062
Self-citationThe cosmological constant and dark energy
Peebles, P. J. E., & Ratra, B. (2003) · Reviews of Modern Physics · doi:10.1103/revmodphys.75.559 · Cited by 5,624
Eisenstein, D. J., Zehavi, I., Hogg, D. W., Scoccimarro, R., Blanton, M. R., Nichol, R. C., Scranton, R., Seo, H., Tegmark, M., Zheng, Z., et al. (2005) · The Astrophysical Journal · doi:10.1086/466512 · Cited by 4,641
Self-citationRiess, A. G., Strolger, L., Tonry, J., Casertano, S., Ferguson, H. C., Mobasher, B., Challis, P., Filippenko, A. V., Jha, S., Li, W., et al. (2004) · The Astrophysical Journal · doi:10.1086/383612 · Cited by 4,315 · cited 3×
“These half-dozen SNe Ia, all at z > 1:25, helped confirm the reality of cosmic acceleration by delineating the transition from preceding cosmic deceleration during the matter-dominated phase and by ruling out simple sources of astrophysical dimming (Riess et al. 2004b, hereafter R04).”
BackgroundMethodSelf-citationUBVRI photometric standard stars in the magnitude range 11.5-16.0 around the celestial equator
Landolt, A. U. (1992) · The Astronomical Journal · doi:10.1086/116242 · Cited by 4,184
Final Results from the Hubble Space Telescope Key Project to Measure the Hubble Constant
Freedman, W. L., Madore, B. F., Gibson, B. K., Ferrarese, L., Kelson, D. D., Sakai, S., Mould, J. R., Robert C. Kennicutt, Jr., Ford, H. C., Graham, J. A., et al. (2001) · The Astrophysical Journal · doi:10.1086/320638 · Cited by 3,543
Eisenstein, D. J., Zehavi, I., Hogg, D. W., Scoccimarro, R., Blanton, M. R., Nichol, R. C., Scranton, R., Seo, H., Tegmark, M., Zheng, Z., et al. (2005) · Cited by 2,568
Self-citationExploring the Expansion History of the Universe
Linder, E. V. (2003) · Physical Review Letters · doi:10.1103/physrevlett.90.091301 · Cited by 2,526
ACCELERATING UNIVERSES WITH SCALING DARK MATTER
CHEVALLIER, M., & POLARSKI, D. (2001) · International Journal of Modern Physics D · doi:10.1142/s0218271801000822 · Cited by 2,490
Research works printed but not linked: 12
- Albrecht, A. & Bernstein, G. 2006, preprint (astro-ph/0608269) · arXiv
- Bond J. R., 1997, MNRAS, 291, L33
- de Jong, R. S., etal 2006, in The 2005 HST Calibration Workshop, ed. A. Koekemoer, P. Goudfrooij, & L. Dressel (Greenbelt: GSFC), 121
- Filippenko, A. V. 2004, in Measuring and Modeling the Universe, ed. W. L. Freedman (Cambridge: Cambridge Univ. Press), 270
- Filippenko, A. V. 2005, in White Dwarfs: Cosmological and Galactic Probes, ed. E. M. Sion, S. Vennes, & H. L. Shipman (Dordrecht: Springer), 97
- Jha, S. 2002, Ph.D. thesis, Harvard Univ.
- Jha, S., Riess, A. G. & Kirshner, R. P. 2007, ApJ, in press
- 10.1086/322348 · DOI
- Spergel, D. N., etal 2006, ApJ, submitted (astro-ph/0603449) · arXiv
- Wetterich C., 1995, A&A, 301, 321
- Wood-Vasey, W. M., etal 2007, ApJ, in press (astro-ph/0701041) · arXiv
- Wright E. L., 2002, BAAS, 34, 174
Cited by
Sorted by citations
Items 301–400 of 1,000
TYPE II-P SUPERNOVAE FROM THE SDSS-II SUPERNOVA SURVEY AND THE STANDARDIZED CANDLE METHOD
D’Andrea, C. B., Sako, M., Dilday, B., Frieman, J. A., Holtzman, J. A., Kessler, R., Konishi, K., Schneider, D. P., Sollerman, J., Wheeler, J. C., et al. (2009) · The Astrophysical Journal · doi:10.1088/0004-637x/708/1/661 · Cited by 82
“…years over a wide range of redshifts, lowering statistical uncertainties with the volume of their discoveries (For high redshift SN programs, see Riess et al. 2004, 2007; Astier et al. 2006; Wood-Vasey et al. 2007; Miknaitis et al. 2007; Kessler et al. 2009a; Frieman et al. 2008; for low…”
BackgroundSelf-citationObservational constraints on holographic tachyonic dark energy in interaction with dark matter
Micheletti, S. M. R. (2010) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2010/05/009 · Cited by 82
Gravitational Energy as Dark Energy: Concordance of Cosmological Tests
Leith, B. M., Ng, S. C. C., & Wiltshire, D. L. (2007) · The Astrophysical Journal · doi:10.1086/527034 · Cited by 82
“We have tested the luminosity distance of the FB model against the Riess et al. (2007) (Riess07) gold data set of SneIa and find that for 182 data points and two degrees of freedom the best–fit χ2 = 162.7, i.e., a χ2 of approximately 0.9 per degree of freedom, which is a good fit.”
MethodInfluentialChasing the phantom: A closer look at type Ia supernovae and the dark energy equation of state
Shafer, D. L., & Dragan Huterer, A. (2014) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.89.063510 · Cited by 81
Gaussian process estimation of transition redshift
de Jesus, J. F., Valentim, R., Escobal, A. A., & Pereira, S. H. (2020) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2020/04/053 · Cited by 81
Gluonic vacuum, q -theory, and the cosmological constant
Klinkhamer, F. R., & Воловик, Г. Е. (2009) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.79.063527 · Cited by 86
LRS Bianchi type-I cosmological model in f(R,T) theory of gravity with Λ(T)
Sahoo, P. K., & Sivakumar, M. (2015) · Astrophysics and Space Science · doi:10.1007/s10509-015-2264-0 · Cited by 81
“…(Bennet et al. 2003, Spergel et al. 2003, 2007) observations, cosmic microwave background (CMB) anisotropies (Perlmutter et al. 1997, 1999, Riess et al. 2004, 2007) and large scale structure (Tegmark et al. 2004; Cole et al. 2005) indicate that most of the cosmic energy density is…”
Apparent cosmic acceleration from Type Ia supernovae
Dam, L., Heinesen, A., & Wiltshire, D. L. (2017) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stx1858 · Cited by 80
“In fact, SneIa analyses using the MLCS method have typically excluded SneIa below a cutoff at z = 0.024 (Riess et al. 2007).”
MethodInfluentialMoresco, M., Jiménez, R., Verde, L., Cimatti, A., Pozzetti, L., Maraston, C., & Thomas, D. (2016) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2016/12/039 · Cited by 80
“Type 1A supernovae (standard candles) We consider the latest “joint light curves” (JLA) sample [11], comprising 740 SNe Ia from the three year Sloan Digital Sky Survey, Supernova Legacy Survey [17, 18], Hubble Space Telescope [19, 20] and other local experiments (see [21]).”
MethodThe Hubble series: Convergence properties and redshift variables
Cattoën, C., & Visser, M. (2007) · Cited by 80
The evidence of cosmic acceleration and observational constraints
Yang, Y., & Gong, Y. (2020) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2020/06/059 · Cited by 83
Dark energy, inflation, and extra dimensions
Steinhardt, P. J., & Wesley, D. (2009) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.79.104026 · Cited by 79
Cosmological models and gamma-ray bursts calibrated by using Padé method
Liu, J., & Wei, H. (2015) · General Relativity and Gravitation · doi:10.1007/s10714-015-1986-1 · Cited by 79
The reliability of the Akaike information criterion method in cosmological model selection
Tan, M. Y. J., & Biswas, R. (2011) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2011.19969.x · Cited by 78
“For our calculation, we use data from the Constitution compilation (Hicken et al. 2009b) of the Center for Astrophysics (CFA3) sample (Hicken et al. 2009a) ESSENCE (Miknaitis et al. 2007), Supernova Legacy Survey (SNLS) (Astier et al. 2006) and ‘High-z’ samples (Riess et al. 2007).”
MethodProbing the cosmographic parameters to distinguish between dark energy and modified gravity models
Wang, F. Y., Dai, Z.-G., & Qi, S. (2009) · Astronomy and Astrophysics · doi:10.1051/0004-6361/200911998 · Cited by 78
“Davis et al. (2007) fitted the SNe Ia dataset that includes 60 ESSENCE SNe Ia (WoodVasey et al. 2007), 57 SNe Ia from Super-Nova Legacy Survey (SNLS) (Astier et al. 2006), 45 nearby SNe Ia and 30 SNe Ia detected by HST (Riess et al. 2007) with the MCLS2K2 method.”
MethodReconstruction and stability of f(R,T) gravity with Ricci and modified Ricci dark energy
Sharif, M., & Zubair, M. (2013) · Astrophysics and Space Science · doi:10.1007/s10509-013-1623-y · Cited by 77
“Contemporary observational data on the cosmic expansion history (Fedeli et al. 2009; Perlmutter et al. 1999; Riess et al. 2007; Spergel et al. 2003; Tegmark et al. 2004) affirm the expanding paradigm of the universe.”
BackgroundMartin, J., Ringeval, C., & Vennin, V. (2024) · Physics of the Dark Universe · doi:10.1016/j.dark.2024.101653 · Cited by 105
Tests of gravity from imaging and spectroscopic surveys
Guzik, J., Jain, B., & Takada, M. (2010) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.81.023503 · Cited by 77
Phantom dark energy models with a nearly flat potential
Scherrer, R. J., & Sen, A. A. (2008) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.78.067303 · Cited by 76
Thermodynamics in f ( R ) gravity in the Palatini formalism
Bamba, K., & Geng, C.-Q. (2010) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2010/06/014 · Cited by 83
Bayesian optimization for likelihood-free cosmological inference
Leclercq, F. (2018) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.98.063511 · Cited by 76
“4) observed by the Hubble Space Telescope (HST Riess et al ., 2007).”
MethodViscous cosmology with matter creation in modified f(R,T) gravity
Kumar, P., & Singh, C. P. (2015) · Astrophysics and Space Science · doi:10.1007/s10509-015-2348-x · Cited by 73
PS1-10afx ATz= 1.388: PAN-STARRS1 DISCOVERY OF A NEW TYPE OF SUPERLUMINOUS SUPERNOVA
Chornock, R., Berger, E., Rest, A., Milisavljevic, D., Lunnan, R., Foley, R. J., Soderberg, A. M., Smartt, S. J., Burgasser, A. J., Challis, P., et al. (2013) · The Astrophysical Journal · doi:10.1088/0004-637x/767/2/162 · Cited by 75
“One of the most distant spectroscopically confirmed SNe Ia known, HST04Sas, is at z = 1.39 (Riess et al. 2007), consistent with the redshift of PS1-10afx.”
BackgroundInfluentialSelf-citationEstimation of primordial spectrum with post-WMAP 3-year data
Shafieloo, A., & Souradeep, T. (2008) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.78.023511 · Cited by 74
SPACE: the spectroscopic all-sky cosmic explorer
Cimatti, A., Robberto, M., Baugh, C. M., Beckwith, S., Robert Content, A., Daddi, E., Lucia, G. D., Garilli, B., Guzzo, L., Kauffmann, G., et al. (2008) · Experimental Astronomy · doi:10.1007/s10686-008-9096-7 · Cited by 74
Self-citationObserving the clustering properties of galaxy clusters in dynamical dark-energy cosmologies
Fedeli, C., Moscardini, L., & Bartelmann, M. (2009) · Astronomy and Astrophysics · doi:10.1051/0004-6361/200811477 · Cited by 74
“While the evidence of its presence has became compelling in the past decade (Astier et al. 2006; Riess et al. 2007; Dunkley et al. 2008; Komatsu et al. 2008; Rubin et al. 2008; Kilbinger et al. 2008), its nature remains entirely unexplained.”
BackgroundFalsifying paradigms for cosmic acceleration
Mortonson, M. J., Hu, W., & Dragan Huterer, A. (2009) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.79.023004 · Cited by 74
Do spectra improve distance measurements of Type Ia supernovae?
Blondin, S., Mandel, K. S., & Kirshner, R. P. (2010) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201015792 · Cited by 74
“Constraints on the variation of w with redshift come from from high-redshift observations with the Hubble Space Telescope (Riess et al. 2004, 2007).”
MethodSelf-citationGrowth index of DGP model and current growth rate data
Wei, H. (2008) · Physics Letters B · doi:10.1016/j.physletb.2008.04.060 · Cited by 76
Genetic algorithms and supernovae type Ia analysis
Bogdanos, C., & Nesseris, S. (2009) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2009/05/006 · Cited by 73
“Early SNIa data put together with more recent such data through the Gold dataset [1, 14] have been used to reconstruct w(z), and have demonstrated a mild preference for a w(z) that crossed the phantom divide line [11, 15].”
MethodInfluence of $$f\,(R)$$ f ( R ) models on the existence of anisotropic self-gravitating systems
Yousaf, Z., Sharif, M., Ilyas, M., & Bhatti, M. Z. (2017) · The European Physical Journal C · doi:10.1140/epjc/s10052-017-5280-0 · Cited by 73
Spherical collapse in f(R) gravity
Borisov, A., Jain, B., & Zhang, P. (2012) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.85.063518 · Cited by 72
Mattsson, T. (2009) · General Relativity and Gravitation · doi:10.1007/s10714-009-0873-z · Cited by 72
“onstrated in Eq. (3.27), the same optical phenomenon is already inherent to the non-linear structure formation with no dark energy. Here we use the Riess et. al. gold sample of 182 type Ia supernovae [16] to study how the nonlinear CHDM model fits the actual data. For this, we use the conventional χ2 test: χ2 ≡ X182 n=…”
MethodInfluentialAN INTENSIVEHUBBLE SPACE TELESCOPESURVEY FORz>1 TYPE Ia SUPERNOVAE BY TARGETING GALAXY CLUSTERS
Dawson, K., Aldering, G., Amanullah, R., Barbary, K., Barrientos, L. F., Brodwin, M., Connolly, N., Dey, A. T., Doi, M., Donahue, M. E., et al. (2009) · The Astronomical Journal · doi:10.1088/0004-6256/138/5/1271 · Cited by 72
“Six SNe with early-type hosts were discovered at z > 0.9 (Riess et al. 2007).”
BackgroundInfluentialSelf-citationCosmological evolution in f(R,T) theory with collisional matter
Baffou, E., Houndjo, M. J. S., Rodrigues, M. E., Kpadonou, A. V., & Tossa, J. (2015) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.92.084043 · Cited by 72
Observational constraints on the deceleration parameter in a tilted universe
Asvesta, K., Kazantzidis, L., Perivolaropoulos, L., & Tsagas, C. G. (2022) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stac922 · Cited by 71
Quasi-static evolution of axially and reflection symmetric large-scale configuration
Yousaf, Z., Bamba, K., Bhatti, M. Z. U. H., & Farwa, U. (2024) · International Journal of Geometric Methods in Modern Physics · doi:10.1142/s0219887824300058 · Cited by 71
Testing the copernican principle via cosmological observations
Bolejko, K., & Wyithe, J. S. B. (2009) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2009/02/020 · Cited by 71
“In addition we also present the constraints coming from the Riess gold data set [18], which until recently has been the most popular sample for testing inhomogeneous models.”
Constraining Cosmic Evolution of Type Ia Supernovae
Foley, R. J., Filippenko, A. V., Aguilera, C., Becker, A. C., Blondin, S., Challis, P., Clocchiatti, A., Covarrubias, R., Davis, T. M., Garnavich, P., et al. (2008) · The Astrophysical Journal · doi:10.1086/589612 · Cited by 71
“The meticulous measurement of several hundred SNe Ia at both low and high redshifts has shown that the expansion of the Universe is currently accelerating (Riess et al. 1998, 2007; Perlmutter et al. 1999; Astier et al. 2006; Wood-Vasey et al. 2007); see Filippenko (2005) for a recent review.”
BackgroundMethodInfluentialSelf-citationThe time evolution of cosmological redshift as a test of dark energy
Balbi, A., & Quercellini, C. (2007) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2007.12407.x · Cited by 71
Stability analysis of stellar radiating filaments
Yousaf, Z., Bhatti, M. Z.-U.-H., & Farwa, U. (2017) · Classical and Quantum Gravity · doi:10.1088/1361-6382/aa73b9 · Cited by 70
Kocevski, D. D. (2016) · Texas ScholarWorks (Texas Digital Library) · doi:10.15781/t2vn58 · Cited by 70
Kuznetsova, N., Barbary, K., Connolly, B. M., Kim, A., Pain, R., Roe, N. A., Aldering, G., Amanullah, R., Dawson, K., Doi, M., et al. (2008) · The Astrophysical Journal · doi:10.1086/524881 · Cited by 70
“The tables specify the supernova names and classifications (gold, silver, or bronze) for the candidates that were also found in Riess et al. (2004a) and in Riess et al. (2007).”
BackgroundThe rate of supernovae at redshift 0.1–1.0
Melinder, J., Dahlén, T., Trinchant, L. M., Östlin, G., Mattila, S., Sollerman, J., Fransson, C., Hayes, M., Kankare, E., & Nasoudi-Shoar, S. (2012) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201219364 · Cited by 70
“…large programmes targeting type Ia supernovae at intermediate and high (& 0.1) redshifts have been conducted to measure the expansion of the universe and do precision cosmology (e.g. Perlmutter et al. 1997; Schmidt et al. 1998; Astier et al. 2006; Riess et al. 2007; Miknaitis et al. 2007).”
BackgroundInfluentialStellar filaments with Minkowskian core in the Einstein- $\Lambda$ Λ gravity
Yousaf, Z. (2017) · The European Physical Journal Plus · doi:10.1140/epjp/i2017-11547-0 · Cited by 69
On redshift evolution and negative dark energy density in Pantheon + Supernovae
Malekjani, M., Conville, R. M., Colgáin, E. Ó., Pourojaghi, S., & Sheikh-Jabbari, M. M. (2024) · The European Physical Journal C · doi:10.1140/epjc/s10052-024-12667-z · Cited by 68
Mustafa, G., Maurya, S. K., & Ray, S. (2022) · The Astrophysical Journal · doi:10.3847/1538-4357/ac9b00 · Cited by 67
“…pushing out the phenomenon of spacetime as well as the existence of dark matter, have raised awkward situation to the success of the Einsteinian GR (Riess et al. 1998, 2007; Perlmutter et al. 1999; Hanany et al. 2000; de Bernardis et al. 2002; Peebles & Ratra 2003; Tegmark et al. 2004; Amanullah…”
BackgroundRapetti, D., Allen, S. W., Mantz, A. B., & Ebeling, H. (2010) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2010.16799.x · Cited by 67
“…have continuously corroborated these results (Garnavich et al. 1998; Schmidt et al. 1998; Knop et al. 2003; Tonry et al. 2003; ⋆ Email: drapetti@slac.stanford.edu Barris et al. 2004; Riess et al. 2004, 2007; Astier et al. 2006; Wood-Vasey et al. 2007; Kowalski et al. 2008; Hicken et al. 2009).”
ResultSapone, D. (2010) · International Journal of Modern Physics A · doi:10.1142/s0217751x10050743 · Cited by 66
Non-commutative wormholes exhibiting conformal motion in Rastall gravity
Mustafa, G., Waheed, S., Zubair, M., & Xia, T. (2020) · Chinese Journal of Physics · doi:10.1016/j.cjph.2020.02.008 · Cited by 66
Probing dark matter substructure with pulsar timing
Siegel, E. R., Hertzberg, M. P., & Fry, J. N. (2007) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2007.12435.x · Cited by 66
EXTRAORDINARY MAGNIFICATION OF THE ORDINARY TYPE Ia SUPERNOVA PS1-10afx
Quimby, R. M., Werner, M. C., Oguri, M., More, S., More, A., Tanaka, M., Nomoto, K., Moriya, T. J., Folatelli, G., Maeda, K., et al. (2013) · The Astrophysical Journal Letters · doi:10.1088/2041-8205/768/1/l20 · Cited by 66
“C13 note that PS1-10afx is 3.8 magnitudes brighter than HST04Sas, a spectroscopically confirmed SNIa at z = 1.39 (Riess et al. 2007).”
BackgroundInfluentialCosmological equivalence principle and the weak-field limit
Wiltshire, D. L. (2008) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.78.084032 · Cited by 66
Reconstruction of f(T) gravity according to holographic dark energy
Daouda, M. H., Rodrigues, M. E., & Houndjo, M. J. S. (2012) · The European Physical Journal C · doi:10.1140/epjc/s10052-012-1893-5 · Cited by 65
Confronting dark energy models using galaxy cluster number counts
Basilakos, S., Plionis, M., & Lima, J. A. S. (2010) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.82.083517 · Cited by 65
Can dark matter decay in dark energy?
Pereira, S. H., & de Jesus, J. F. (2009) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.79.043517 · Cited by 64
Chawla, C., Mishra, R. K., & Pradhan, A. (2012) · The European Physical Journal Plus · doi:10.1140/epjp/i2012-12137-4 · Cited by 64
REAL-TIME ANALYSIS AND SELECTION BIASES IN THE SUPERNOVA LEGACY SURVEY
Perrett, K., Balam, D., Sullivan, M., Pritchet, C. J., Conley, A., Carlberg, R. G., Astier, P., Balland, C., Basa, S., Fouchez, D., et al. (2010) · The Astronomical Journal · doi:10.1088/0004-6256/140/2/518 · Cited by 64
“Subsequent searches have led to SN Ia discoveries over a wide range of redshifts (e.g., Astier et al. 2006; Miknaitis et al. 2007; Sako et al. 2008; Riess et al. 2007).”
BackgroundObservational constraints to Ricci dark energy model by using: SN, BAO, OHD, fgas data sets
Xu, L., & Wang, Y. (2010) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2010/06/002 · Cited by 64
The Peculiar Velocities of Local Type Ia Supernovae and Their Impact on Cosmology
Neill, J. D., Hudson, M. J., & Conley, A. (2007) · The Astrophysical Journal · doi:10.1086/518808 · Cited by 64
“Current analyses (e.g., Astier et al. 2006; Riess et al. 2007; Wood-Vasey et al. 2007) of the cosmological parameters do not attempt to correct for the effect of local peculiar velocities.”
BackgroundEffects of shear and rotation on the spherical collapse model for clustering dark energy
Pace, F., Batista, R. C., & Popolo, A. D. (2014) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stu1782 · Cited by 63
“…latest observations of Supernovae type Ia (Riess et al. 1998; Perlmutter et al. 1999; Knop et al. 2003; Riess et al. 2004; Astier et al. 2006; Riess et al. 2007; Amanullah et al. 2010), together with the cosmic microwave background (CMB) (Komatsu et al. 2011; Jarosik et al. 2011; Planck…”
BackgroundInstability of meridional axial system in f(R) gravity
Sharif, M., & Yousaf, Z. (2015) · The European Physical Journal C · doi:10.1140/epjc/s10052-015-3415-8 · Cited by 63
Viscous fluid cosmology: A path to cosmic acceleration
Yousaf, Z. (2025) · Physics of the Dark Universe · doi:10.1016/j.dark.2025.101884 · Cited by 63
Bandpass Dependence of X‐Ray Temperatures in Galaxy Clusters
Cavagnolo, K. W., Donahue, M. E., Voit, G. M., & Sun, M. (2008) · The Astrophysical Journal · doi:10.1086/588630 · Cited by 63
“In particular, the evolution of large-scale structure formation provides a complementary and distinct constraint on cosmological parameters to those tests which constrain them geometrically, such as supernovae (Riess et al. 1998, 2007) and baryon acoustic oscillations (Eisenstein et al. 2005).”
A review of type Ia supernova spectra
Parrent, J., Friesen, B., & Parthasarathy, M. (2014) · Astrophysics and Space Science · doi:10.1007/s10509-014-1830-1 · Cited by 63
“There have been ∼110 high-z (1 < z < 2) SN Ia discoveries since SN 1997ff (Riess et al. 2004, 2007; Suzuki et al. 2012), with the most recent and and one of the most distant SN Ia known being “SN UDS10Wil” at z = 1.914 (Jones et al. 2013).”
BackgroundInfluentialTHE FUNDAMENTAL METALLICITY RELATION REDUCES TYPE Ia SN HUBBLE RESIDUALS MORE THAN HOST MASS ALONE
Hayden, B. T., Gupta, R. R., Garnavich, P., Mannucci, F., Nichol, R. C., & Sako, M. (2013) · The Astrophysical Journal · doi:10.1088/0004-637x/764/2/191 · Cited by 63
“…studies have shifted from confirming acceleration to constraining the properties of dark energy (Garnavich et al. 1998a; Astier et al. 2006; Riess et al. 2007; Wood-Vasey et al. 2007; Miknaitis et al. 2007; Eisenstein et al. 2007; Conley et al. 2011; Sullivan et al. 2011; Suzuki et al.…”
BackgroundThe matter distribution in the local Universe as derived from galaxy groups in SDSS DR12 and 2MRS
Saulder, C., van Kampen, E., Chilingarian, I., Mieske, S., & Zeilinger, W. W. (2016) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201526711 · Cited by 63
“This renormalized critical density is about 61% of the critical density in the Λ-CDM model according to the best fits for this alternative cosmology (the Hubble parameter10 for the wall environment (inside finite infinity regions) is expected to be 48.2 km s−1 Mpc−1 and void environment (outside finite infinity region…”
BackgroundInfluentialOvercoming the Circular Problem for Gamma‐Ray Bursts in Cosmological Global‐Fitting Analysis
Li, H., Xia, J., Liu, J., Zhao, G., Fan, Z., & Zhang, X. (2008) · The Astrophysical Journal · doi:10.1086/529582 · Cited by 62
“Li et al. (2008), for the first time, performed global fitting on the GRB data with the Markov chain Monte Carlo (MCMC) technique together with SNe Ia data (Riess et al. 2007) and data fromWMAP (Spergel et al. 2007), SDSS (Tegmark et al. 2004), and 2dFGRS (Cole et al. 2005).”
MethodThe imprint of the interaction between dark sectors in galaxy clusters
He, J.-H., Wang, B., Elcio Abdalla, A., & Pavón, D. (2010) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2010/12/022 · Cited by 62
Stefano, R. D. (2010) · The Astrophysical Journal · doi:10.1088/0004-637x/719/1/474 · Cited by 62
“The results have been exciting, indicating epochs of deceleration and acceleration, and suggesting the presence of dark energy (see, e.g., Riess et al. 2007; Kuznetsova et al. 2008).”
Charged Adiabatic LTB Gravitational Collapse in f (R) Gravity
Sharif, M., & Yousaf, Z. (2015) · International Journal of Theoretical Physics · doi:10.1007/s10773-015-2681-4 · Cited by 62
THREE GRAVITATIONALLY LENSED SUPERNOVAE BEHIND CLASH GALAXY CLUSTERS
Patel, B., McCully, C., Jha, S. W., Rodney, S. A., Jones, D. O., Graur, O., Merten, J., Zitrin, A., Riess, A. G., Matheson, T., et al. (2014) · The Astrophysical Journal · doi:10.1088/0004-637x/786/1/9 · Cited by 62
“Both plots also show a comparison sample of 18 field SNe Ia from Riess et al. (2007) and Suzuki et al. (2012) in the range 1.14 ≤ z ≤ 1.41, fit in exactly the same manner as SN CLO12Car.”
MethodInfluentialSelf-citationThe growth of matter perturbations in some scalar-tensor DE modelsPreprint
Gannouji, R., & Polarski, D. (2008) · Cited by 71
A comparison of structure formation in minimally and non-minimally coupled quintessence models
Pace, F., Moscardini, L., Crittenden, R., Bartelmann, M., & Pettorino, V. (2013) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stt1907 · Cited by 62
“1 IN T RO D U C T I O N In recent years, data ranging from observations of Type Ia supernovae (Riess et al. 1998, 2004, 2007; Perlmutter et al. 1999), cosmic microwave background (CMB) and the integrated Sachs–Wolfe effect (Jaffe et al. 2001; Giannantonio et al. 2008; Ho et al. 2008; Jarosik et al.…”
BackgroundBerkeley Supernova Ia Program – V. Late-time spectra of Type Ia Supernovae
Silverman, J. M., Ganeshalingam, M., & Filippenko, A. V. (2013) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/sts674 · Cited by 61
“Type Ia supernovae (SNe Ia) can be used to accurately measure cosmological parameters (e.g., Astier et al. 2006; 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. 2012), and they led to the discovery of the…”
BackgroundSelf-citationIsocurvature, non-Gaussianity, and the curvaton model
Beltrán, M. T. (2008) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.78.023530 · Cited by 63
Kim, Y.-L., Smith, M., Sullivan, M., & Lee, Y. (2018) · The Astrophysical Journal · doi:10.3847/1538-4357/aaa127 · Cited by 61
“…et al. 2011), the SDSS-II SN survey (hereafter SDSS; Sako et al. 2014), the ESSENCE survey (Miknaitis et al. 2007), the first three years of the Canada–France–Hawaii Telescope Supernova Legacy Survey (hereafter SNLS; Guy et al. 2010), and the Hubble Space Telescope sample of Riess et al. (2007).”
BackgroundObservational bounds on the cosmic radiation density
Hamann, J., Hannestad, S., Raffelt, G. G., & Wong, Y. Y. Y. (2007) · Max Planck Institute for Plasma Physics · Cited by 61
Affine equation of state from quintessence and k-essence fields
Quercellini, C., Bruni, M., & Balbi, A. (2007) · Classical and Quantum Gravity · doi:10.1088/0264-9381/24/22/006 · Cited by 62
The age problem in ΛCDM modelPreprint
Yang, R.-J., & Zhang, S. (2016) · Cited by 72
Pereira, S. H., & Lima, J. A. S. (2008) · Physics Letters B · doi:10.1016/j.physletb.2008.10.006 · Cited by 61
The Absolute Magnitudes of Type Ia Supernovae in the UltravioletPreprint
Brown, P., Roming, P., Milne, P., Bufano, F., Ciardullo, R., Elias-Rosa, N., Filippenko, A. V., Foley, R., Gehrels, N., Gronwall, C., et al. (2010) · Cited by 60
Self-citationInfluence of electric charge and modified gravity on density irregularities
Bhatti, M. Z. U. H., & Yousaf, Z. (2016) · The European Physical Journal C · doi:10.1140/epjc/s10052-016-4064-2 · Cited by 59
Alleviation of cosmic age problem in interacting dark energy model
Wang, S., & Zhang, Y. (2008) · Physics Letters B · doi:10.1016/j.physletb.2008.09.055 · Cited by 59
On the Magnitude of Dark Energy Voids and Overdensities
Mota, D. F., Shaw, D. J., & Silk, J. I. (2008) · The Astrophysical Journal · doi:10.1086/524401 · Cited by 59
A Detailed Study of Photometric Redshifts for GOODS-South GalaxiesPreprint
Dahlén, T., Mobasher, B., Dickinson, M., Ferguson, H. C., Dahlén, T., Mobasher, B., Dickinson, M., Ferguson, H. C., Grogin, G. N. A., Lee, S.-K., et al. (2010) · Cited by 59
Self-citationImpact of f(ℜ) functions on the dynamical evolution of axially symmetric collapsing stars
Yousaf, M. (2025) · Chinese Journal of Physics · doi:10.1016/j.cjph.2025.02.017 · Cited by 58
Hachinger, S., Mazzali, P. A., Sullivan, M., Ellis, R. S., Maguire, K., Gal‐Yam, A., Howell, D. A., Nugent, P., Baron, E., Cooke, J., et al. (2013) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/sts492 · Cited by 58
“…produce most of the iron-group elements in the cosmos (Iwamoto et al. 1999), and can be used as ‘standardizable candles’ to probe the expansion history of the Universe (e.g. Riess et al. 1998; Perlmutter et al. 1999; Riess et al. 2007; Kessler et al. 2009; Sullivan et al. 2011; Suzuki et al. 2012).”
BackgroundCosmological model with non-minimally coupled fermionic field
Ribas, M. O., Devecchi, F. P., & Kremer, G. M. (2007) · Europhysics Letters (EPL) · doi:10.1209/0295-5075/81/19001 · Cited by 58
Stefano, R. D. (2010) · Cited by 58
Dynamics of linear perturbations in the hybrid metric-Palatini gravity
Lima, N. A. (2014) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.89.083527 · Cited by 57
Dynamics and cosmological evolution in $$\Lambda $$-varying cosmology
Papagiannopoulos, G., Tsiapi, P., Basilakos, S., & Paliathanasis, A. (2019) · The European Physical Journal C · doi:10.1140/epjc/s10052-019-7600-z · Cited by 40
Exact dark energy star solutions
Yazadjiev, S. S. (2011) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.83.127501 · Cited by 57
Cosmological model with interactions in the dark sector
Chimento, L. P., Forte, M., & Kremer, G. M. (2008) · General Relativity and Gravitation · doi:10.1007/s10714-008-0694-5 · Cited by 57
“The circles in Fig. 6 are observational data for super-novae of type Ia taken from the work [ 44 ].”
MethodZhao, W. K. (2007) · Physics Letters B · doi:10.1016/j.physletb.2007.08.083 · Cited by 57
PTF10ops - a subluminous, normal-width light curve Type Ia supernova in the middle of nowhere
Maguire, K., Sullivan, M., Thomas, R. C., Nugent, P., Howell, D. A., Gal‐Yam, A., Arcavi, I., Ben-Ami, S., Blake, S., Botyanszki, J., et al. (2011) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2011.19526.x · Cited by 57
“…and since then major advances have been made in further standardising their lightcurves to produce a very successful method of determining the cosmological parametersof the universe (e.g. Riess et al. 1998; Perlmutter et al. 1999; Riess et al. 2007; Kessler et al. 2009; Sullivan et al. 2011b).”
MethodThe 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) · Astronomy and Astrophysics · doi:10.1051/0004-6361/200912246 · Cited by 57
“When combined with other probes, the picture of a universe dominated by dark energy emerges (Tonry et al. 2003; Astier et al. 2006; Riess et al. 2007; Wood-Vasey et al. 2007; Kowalski et al. 2008).”
BackgroundPlionis, M., Terlevich, R. J., Basilakos, S., Bresolin, F., Terlevich, E., Melnick, J., & Chávez, R. (2011) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2011.19247.x · Cited by 56
“To this end we have decided to re-analyse two recently compiled SNIa samples, the Davis et al. (2007) [hereafter D07] compilation of 192 SNIa (based on data from Wood-Vasey et al. 2007, Riess et al. 2007 and Astier et al. 2007) and the Constitution compilation of 397 SNIa (Hicken et al. 2009).”
BackgroundMethodLiang, N., Wu, P., & Zhang, S. (2010) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.81.083518 · Cited by 56
Testing dark energy paradigms with weak gravitational lensing
Vanderveld, R. A., Mortonson, M. J., Hu, W., & Eifler, T. F. (2012) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.85.103518 · Cited by 56
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
About these checks
Registry, retraction, Cites and statistics results are computed, not judged, with one exception: a printed reference that no index lists is read once by a model before it counts as a citation error. Claims are extracted by a model and kept only when their quote appears verbatim in the text; each cited source is then checked, with a model’s help, for whether it says what the claim relies on. Those verdicts can be wrong — read the claim’s quote and the cited source before relying on one.
Statistics and arithmetic are recomputed, not judged.
Confidence bands are shown only for fields calibrated on our annotated test set. None is calibrated yet, so no band is shown.
What counts as a claim ›How we measure confidence ›How we check this ›
Are you an author, or do you see a problem with this page? Request a review
