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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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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
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“…et al. 1998; Perlmutter et al. 1999), as well as to measure cosmological parameters with increasing accuracy and precision (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; Sullivan et al. 2011; Suzuki et al. 2012).”
BackgroundSelf-citationBasilakos, S., Sánchez, J. C. B., & Perivolaropoulos, L. (2009) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.80.043530 · Cited by 56
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“Further indications in the same directionc me from the study performed by Riess et al. (2007).”
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“ompilation [53]. It contains a set of 740 spectroscopically confirmed SNe Ia compiled by the SDSS-IIsupernova survey [54], SNLS survey [55] and a few from Hubble Space Telescope (HST) SNe observations [56] in the redshift region 0.01 < z < 1.3. The distance modulus of a SNe Ia is obtained by a linear relation fro…”
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“The current sample of SN distances at z > 1 is dominated by events measured with NIR instruments (NICMOS and WFC3) on the HST (Riess et al. 2007; Suzuki et al. 2012; Rodney et al. 2012; Rubin et al. 2013) and amounts to less than 40 such events.”
BackgroundHow to distinguish dark energy and modified gravity?
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High-redshift cosmography: new results and implications for dark energy
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“Thus, in principle, we could extend the series up to the redshift of decoupling, and one could place CMB related constraints within the cosmographic approach 2.”
ResultInfluentialK-inflationary power spectra at second order
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Crittenden, R., Majerotto, E., & Piazza, F. (2007) · Physical Review Letters · doi:10.1103/physrevlett.98.251301 · Cited by 54
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Xia, J., Li, H., Zhao, G., & Zhang, X. (2008) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.78.083524 · Cited by 53
Type Ia supernova spectral features in the context of their host galaxy properties
Pan, Y. C., Sullivan, M., Maguire, K., Gal‐Yam, A., Hook, I., Howell, D. A., Nugent, P., & Mazzali, P. A. (2014) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stu2121 · Cited by 53
“A better understanding of SN Ia progenitors would likely strengthen their continuing use as cosmological probes (e.g., Riess et al. 1998; Perlmutter et al. 1999; Kessler et al. 2009; Riess et al. 2007; Sullivan et al. 2011; Rest et al. 2013; Betoule et al. 2014).”
BackgroundSPECTROSCOPY OF HIGH-REDSHIFT SUPERNOVAE FROM THE ESSENCE PROJECT: THE FIRST FOUR YEARS
Foley, R. J., Matheson, T., Blondin, S., Chornock, R., Silverman, J. M., Challis, P., Clocchiatti, A., Filippenko, A. V., Kirshner, R., LEIBUNDGUT, B., et al. (2009) · The Astronomical Journal · doi:10.1088/0004-6256/137/4/3731 · Cited by 53
“…highredshift SN Ia surveys, using the large and normalized peak luminosities of SNe Ia, have focused on measuring the equation-of-state parameter of the dark energy, w = P/(ρc2), currently constraining it to ∼10% (Astier et al. 2006; Riess et al. 2007; Wood-Vasey et al. 2007; Kowalski et al. 2008).”
BackgroundSelf-citationRodney, S., Riess, A. G., Scolnic, D. M., Jones, D. O., Hemmati, S., Molino, A., McCully, C., Mobasher, B., Strolger, L.-G., Graur, O., et al. (2015) · The Astronomical Journal · doi:10.1088/0004-6256/150/5/156 · Cited by 53
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Quercellini, C., Bruni, M., Balbi, A., & Pietrobon, D. (2008) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.78.063527 · Cited by 52
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“Despite being in agreement with supernova observations (Riess et al. 1998; Perlmutter et al. 1999; Riess et al. 2007; Amanullah et al. 2010), data from the cosmic microwave background (CMB) (Fixsen & Mather 2002; Jarosik et al. 2011), including the recent Planck data (Planck Collaboration et al.…”
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“Since it is possible, although difficult (see figure 3), to obtain the Hubble parameter by differentiating distances, which would give us q(z) directly, we can try to compare ȧ = (1 + z)/H(z) at different redshifts [6].”
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Bordalo, V., & Telles, E. (2011) · The Astrophysical Journal · doi:10.1088/0004-637x/735/1/52 · Cited by 52
“On the other hand, light curves of Supernovae Type Ia (SNIa), which are today the most used technique to obtain such cosmological distances encounters lack of target objects at redshifts above ∼ 1.2 (Riess et al. 2007).”
MethodInfluentialAccelerating universe in hybrid and logarithmic teleparallel gravity
Mandal, S., Bhattacharjee, S., Pacif, S. K. J., & Sahoo, P. K. (2020) · Physics of the Dark Universe · doi:10.1016/j.dark.2020.100551 · Cited by 55
Tracing Dark Energy History with Gamma-Ray Bursts
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Measuring Dark Energy with Gamma‐Ray Bursts and Other Cosmological Probes
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“This led to a sample known as the ‘‘gold’’ sample containing 157 SNe Ia. Recently, Riess et al. (2007) added 25 SNe Ia to this sample.”
BackgroundDark energy, induced gravity and broken scale invariance
Finelli, F., Tronconi, A., & Venturi, G. (2007) · Physics Letters B · doi:10.1016/j.physletb.2007.11.053 · Cited by 55
Accelerating cosmologies tested by distance measures
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Transient cosmic acceleration from interacting fluids
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Foley, R. J., Kromer, M., Marion, G. H. H., Pignata, G., Stritzinger, M. D., Taubenberger, S., Challis, P., Filippenko, A. V., Folatelli, G., Hillebrandt, W., et al. (2012) · The Astrophysical Journal Letters · doi:10.1088/2041-8205/753/1/l5 · Cited by 50
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BackgroundSelf-citationLinden, S., & Virey, J.-M. (2008) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.78.023526 · Cited by 50
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de Jesus, J. F., Santos, R. C., Alcaniz, J. S., & Lima, J. A. S. (2008) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.78.063514 · Cited by 57
“We also include, as in [12], 30 new released SNe Ia, classified as “gold” supernovae by Riess et al. (2007) [16].”
BackgroundOscillations in the dark energy equation of state: New MCMC lessons
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“…ESSENCE survey (Miknaitis et al. 2007; Wood-Vasey et al. 2007), the Supernova Legacy Survey (SNLS)(Astier et al. 2006), the Hubble Space Telescope Page 5 of 7 (HST) (Garnavich et al. 1998; Knop et al. 2003; Riess et al. 2004, 2007), and a compilation of nearby SN Ia measurements (Jha et al. 2007).”
BackgroundStudy of gravastars in Rastall gravity
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Casarini, L., Macciò, A. V., & Bonometto, S. A. (2009) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2009/03/014 · Cited by 49
“7 is now required by CMB and LSS data and this implies that the gap between Ωm and unity is to be filled by a smooth non-particle component (Ωm, Ωb: matter, baryon present density parameters; h: present Hubble parameter in units of 100 km/s/Mpc; CMB: cosmic microwave background; LSS: large scale structure; for SNIa da…”
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Hilton, M., Collins, C. A., Stanford, S. A., Lidman, C. E., Dawson, K. S., Davidson, M., Kay, S. T., Liddle, A. R., Mann, R. G., Miller, C. J., et al. (2007) · The Astrophysical Journal · doi:10.1086/522827 · Cited by 49
“…obtained from cosmic microwave background observations (e.g., Spergel et al. 2007), or surveys using type Ia supernovae as standard candles (e.g., Astier et al. 2006; Riess et al. 2007; WoodVasey et al. 2007, for a compilation of all supernova surveys see Kowalski et al. 2007, in preparation).”
Does the Universe accelerate equally in all directions?
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“Using the Gold SNe sample (Riess et al. 2007), Leith, Ng & Wiltshire (2008) demonstrated that this model ⋆ E-mail: rcooke@ast.cam.ac.uk; dlb@ast.cam.ac.uk provides a possible alternative to dark energy, although this model fails to provide a consistent fit to the Union (Kowalski et al. 2008) and…”
MethodΛ(t) cosmology induced by a slowly varying Elko field
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“…a huge increment of data up to redshift z ∼ 1 (Riess et al. 1998,Perlmutter et al. 1999,Astier et al. 2006,Wood-Vasey et al. 2007, Riess et al. 2004, Riess et al. 2007, Dawson et al. 2009; Riess et al. 2011) The current precision and accuracy required to obtain deeper insight on the cosmological…”
BackgroundGal‐Yam, A., Maoz, D., Guhathakurta, P., & Filippenko, A. V. (2008) · The Astrophysical Journal · doi:10.1086/587680 · Cited by 48
“…2005a; A. V. Filippenko & W. Li 2008, in preparation) out to high redshifts (e.g., the SN legacy survey, Astier et al. 2006; ESSENCE, Wood-Vasey et al. 2007) and very high redshifts (e.g., GOODS,Riess et al. 2007; SDFSNS, Poznanski SNe IN LOW-REDSHIFT GALAXY CLUSTERS 561No. 1, 2008 et al. 2007).”
BackgroundSelf-citationAnisotropic universe with anisotropic sources
Aluri, P. K., Panda, S., Sharma, M., & Thakur, S. (2013) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2013/12/003 · Cited by 48
Cross-correlatingWMAP5 with 1.5 million LRGs: a new test for the ISW effect
Sawangwit, U., Shanks, T., Cannon, R., Croom, S. M., Ross, N. P., & Wake, D. A. (2009) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2009.16054.x · Cited by 48
“…(US); tom.shanks@durham. ac.uk (TS) 1 IN T RO D U C T I O N Many observations now suggest that we live in a spatially flat, dark-energy-dominated Universe (e.g. Perlmutter et al. 1999; Cole et al. 2005; Tegmark et al. 2006; Riess et al. 2007; Dunkley et al. C© 2009 The Authors.”
BackgroundFoley, R. J., Filippenko, A. V., Kessler, R., Bassett, B., Frieman, J. A., Garnavich, P. M., Jha, S. W., Konishi, K., Lampeitl, H., Riess, A. G., et al. (2012) · The Astronomical Journal · doi:10.1088/0004-6256/143/5/113 · Cited by 48
“…et al. 1998; Perlmutter et al. 1999), and that the equationof-state parameter of the dark energy, w = P/(ρc2), is consistent with the cosmological constant, w = −1 (e.g., Riess et al. 2007; Wood-Vasey et al. 2007; Hicken et al. 2009b; Kessler et al. 2009a; Conley et al. 2011; Sullivan et al. 2011).”
Self-citationGravastars in f(R,T,RμνTμν) gravity
Yousaf, Z., Bhatti, M. Z., & Asad, H. (2020) · Physics of the Dark Universe · doi:10.1016/j.dark.2020.100527 · Cited by 48
Inhomogeneity-Induced Cosmic Acceleration in a Dust Universe
Chuang, C.-H., Gu, J. A., & Hwang, W.-Y. P. (2005) · CERN Document Server (European Organization for Nuclear Research) · Cited by 48
Do spectra improve distance measurements of Type Ia supernovae?
Blondin, S., Mandel, K. S., & Kirshner, R. (2010) · Springer Link (Chiba Institute of Technology) · doi:10.1051/0004-6361/201015792/pdf · Cited by 48
Self-citationThe ΛCDM Model in the Lead—A Bayesian Cosmological Model Comparison
Kurek, A., & Marek Szydlowski, A. (2008) · The Astrophysical Journal · doi:10.1086/526333 · Cited by 48
“Here we treated posterior probabilities evaluated in the analysis with SNIa data as prior probabilities.”
MethodInfluentialLensed Type Ia supernovae as probes of cluster mass models
Nordin, J., Rubin, D., Richard, J., Rykoff, E. S., Aldering, G. S., Amanullah, R., Atek, H., Barbary, K., Deustua, S. E., Fakhouri, H., et al. (2014) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stu376 · Cited by 47
“…HST observations of the parallel fields were used for a search for field SNe by the CLASH team (see e.g. Rodney et al. 2012), where lensing effects are small and SNe Ia can be used for probing dark energy and SN rate studies (Riess et al. 2007; Dahlen et al. 2008; Barbary et al. 2012).”
MethodFoley, R. J. (2012) · The Astrophysical Journal · doi:10.1088/0004-637x/748/2/127 · Cited by 47
“…is accelerating (Riess et al. 1998; Perlmutter et al. 1999) and constrain the equation-of-state parameter of dark energy, w (Wood-Vasey et al. 2007; Riess et al. 2007; Hicken et al. 2009b; Kessler et al. 2009; Amanullah et al. 1 Harvard-Smithsonian Center for Astrophysics, 60 Garden Street,…”
BackgroundSelf-citationThe search for dark matter particles
Ryabov, V. A., Tsarev, V. A., & Tskhovrebov, A. M. (2008) · Physics-Uspekhi · doi:10.1070/pu2008v051n11abeh006599 · Cited by 44
Interpreting the near-infrared spectra of the ‘golden standard’ Type Ia supernova 2005cf
Gall, E. E. E., Taubenberger, S., Kromer, M., Sim, S. A., Benetti, S., Blanc, G., Elias-Rosa, N., & Hillebrandt, W. (2012) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2012.21999.x · Cited by 47
“This was in turn interpreted as evidence for the existence of ‘dark energy’ (e.g. Riess et al. 2007).”
Shabani, H., & Ziaie, A. H. (2017) · The European Physical Journal C · doi:10.1140/epjc/s10052-017-4844-3 · Cited by 47
Testable dark energy predictions from current data
Mortonson, M. J., Hu, W., & Dragan Huterer, A. (2010) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.81.063007 · Cited by 47
Cosmological constraints on invisible decay of dark matter
Gong, Y., & Chen, X. (2008) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.77.103511 · Cited by 47
Meyers, J. M., Aldering, G., Barbary, K., Barrientos, L. F., Brodwin, M., Dawson, K. S., Deustua, S., Doi, M., Eisenhardt, P., Faccioli, L., et al. (2012) · The Astrophysical Journal · doi:10.1088/0004-637x/750/1/1 · Cited by 47
“Riess et al. (2007) classifies the hosts of all of these but SN2003az as elliptical.”
BackgroundMethodInfluentialOn the Past Asymptotic Dynamics of Non-minimally Coupled Dark EnergyPreprint
León, G. (2008) · Cited by 47
A new approach on the stability analysis in ELKO cosmology
Souza, A. P. D. S., Pereira, S. H., & de Jesus, J. F. (2015) · The European Physical Journal C · doi:10.1140/epjc/s10052-015-3260-9 · Cited by 46
The growth of linear perturbations in the DGP model
Fu, X., Wu, P., & Yu, H. (2009) · Physics Letters B · doi:10.1016/j.physletb.2009.05.007 · Cited by 47
Entropic cosmology in a dissipative universe
KOMATSU, N., & KIMURA, S. (2014) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.90.123516 · Cited by 46
Revisiting the parametrization of equation of state of dark energy via SNIa data
Liu, D.-J., Li, X.-Z., Hao, J., & Jin, X.-H. (2008) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2008.13380.x · Cited by 46
“Current observations, such as those of CMB anisotropy (Spergel et al. 2007), Supernovae type Ia (Riess et al. 2004, 2007; Davis et al. 2007) and large scale structure (Tegmark et al. 2004; Eisenstein et al. 2007), converge on the fact that a spatially homogeneous and gravitationally repulsive…”
BackgroundModel independent constraints on transition redshift
Jesus, J. F., Holanda, R. F. L., & Pereira, S. H. (2018) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2018/05/073 · Cited by 46
Rivero, A. D., Dvorkin, C., Cyr-Racine, F.-Y., Zavala, J., & Vogelsberger, M. (2018) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.98.103517 · Cited by 45
Dark energy parametrizations and the curvature of the universe
Ichikawa, K., & Takahashi, T. (2007) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2007/02/001 · Cited by 46
THE MEAN TYPE IA SUPERNOVA SPECTRUM OVER THE PAST NINE GIGAYEARS
Sullivan, M., Ellis, R. S., Howell, D. A., Riess, A. G., Nugent, P., & Gal‐Yam, A. (2009) · The Astrophysical Journal · doi:10.1088/0004-637x/693/2/l76 · Cited by 46
“In this Letter, we examine the rest-frame λ 4500 Å spectrum of SNe Ia over 0 < z < 1.3 by combining data gathered using Keck at z 0.5 (E08) and Hubble Space Telescope (HST) at z > 1 (Riess et al. 2007, hereafter R07).”
MethodInfluentialSelf-citationK-inflationary Power Spectra at Second OrderPreprint
Ringevalb, A. C., & Vennina, V. (2016) · Cited by 46
Rubin, D., Knop, R. A., Rykoff, E. S., Aldering, G., Amanullah, R., Barbary, K., Burns, M. S., Conley, A., Connolly, N., Deustua, S. E., et al. (2013) · The Astrophysical Journal · doi:10.1088/0004-637x/763/1/35 · Cited by 45
“…18 CENTRA - Centro Multidisciplinar de Astrof́ısica, Instituto Superior Técnico, Av. Rovisco Pais 1, 1049-001 Lisbon, Portugal 19 Department of Physics, Texas A & M University, College Station, TX 77843, USA 20 Deceased 2003; Riess et al. 2004, 2007; Amanullah et al. 2010; Suzuki et al. 2012).”
BackgroundSalazar-Albornoz, S., Sánchez, A. G., Grieb, J. N., Crocce, M., Scoccimarro, R., Alam, S., Beutler, F., Brownstein, J. R., Chuang, C.-H., Kitaura, F.-S., et al. (2017) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stx633 · Cited by 45
Ruppin, F., Adam, R., Comis, B., Ade, P. A. R., André, P., Arnaud, M., Beelen, A., Benoit, A. D., Bideaud, A., Billot, N., et al. (2016) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201629405 · Cited by 45
“…2016) brings constraints on the cosmological parameters that are complementary to those derived with other probes such as type Ia supernovae (e.g., Riess et al. 2007), the CMB temperature and polarization angular power spectra (e.g., Planck Collaboration XIII 2016), or baryonic acoustic…”
BackgroundInflation and reheating in scale-invariant scalar-tensor gravity
Tambalo, G., & Rinaldi, M. (2017) · General Relativity and Gravitation · doi:10.1007/s10714-017-2217-8 · Cited by 47
Consistency tests in cosmology using relative entropy
Nicola, A., Amara, A., & Refregier, A. R. (2019) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2019/01/011 · Cited by 45
Thermal stability of Tsallis holographic dark energy in nonflat universe
Zadeh, M. A., Sheykhi, A., & Moradpour, H. (2019) · General Relativity and Gravitation · doi:10.1007/s10714-018-2497-7 · Cited by 44
The need for accurate redshifts in supernova cosmology
Calcino, J., & Davis, T. M. (2017) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2017/01/038 · Cited by 45
Complexity for self-gravitating fluid distributions in f(G, T) gravity
Yousaf, Z., Bhatti, M. Z. U. H., & Hassan, K. (2020) · The European Physical Journal Plus · doi:10.1140/epjp/s13360-020-00408-6 · Cited by 45
Liu, Y., Cao, S., Liu, T., Li, X., Geng, S., Lian, Y., & Guo, W. (2020) · The Astrophysical Journal · doi:10.3847/1538-4357/abb0e4 · Cited by 45
“Compared with the previous SNe Ia samples extensively discussed in the previous works, i.e., highz data (z>1.0) from the SCP survey (Suzuki et al. 2012), the GOODS (Riess et al. 2007) and CAN-DELS/CLASH surveys (Graur et al. 2014; Rodney et al. 2014; Riess et al. 2018), the Pantheon catalog extends the Hubble diagram…”
BackgroundInfluentialThe matter distribution in the local Universe as derived from galaxy groups in SDSS DR12 and 2MRS
Saulder, C., Kampen, E. V., Chilingarian, I., Mieske, S., & Zeilinger, W. W. (2016) · Springer Link (Chiba Institute of Technology) · doi:10.1051/0004-6361/201526711/pdf · Cited by 45
Inhomogeneity-induced cosmic acceleration in a dust universe
Chuang, C.-H., Gu, J.-A., & Hwang, W.-Y. P. (2008) · Classical and Quantum Gravity · doi:10.1088/0264-9381/25/17/175001 · Cited by 45
The three-loop Yang–Mills condensate dark energy model and its cosmological constraints
Wang, S., Zhang, Y., & Xia, T. Y. (2008) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2008/10/037 · Cited by 44
Xu, X., Wang, B., Zhang, P., & Atrio-Barandela, F. (2013) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2013/12/001 · Cited by 45
Constraints on growth index parameters from current and future observations
Dossett, J. N., Ishak, M., Moldenhauer, J., Gong, Y., & Wang, A. (2010) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2010/04/022 · Cited by 49
“lected by multiple experiments including the ESSENCE Survey [41, 42], Supernova Legacy Survey [43], an extended dataset of distant SNe observed with the Hubble space telescope, and older observed SNe data, [28] as well as 90 Type Ia SNe from the CFA3 survey [27].”
Anisotropic Viscous Fluid Cosmological Models from Deceleration to Acceleration in String Cosmology
Mishra, R. K., Pradhan, A., & Chawla, C. (2013) · International Journal of Theoretical Physics · doi:10.1007/s10773-013-1540-4 · Cited by 44
The effect of baryons in the cosmological lensing PDFs
Castro, T., Quartin, M., Giocoli, C., Borgani, S., & Dolag, K. (2018) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/sty1117 · Cited by 44
“The former is the mysterious energy density component responsible for the ongoing accelerated expansion of the Universe (Perlmutter et al. 1998; Riess et al. 1998; Riess et al. 2004, 2007; Betoule et al. 2014), while the latter is a weakly interactive form of matter.”
BackgroundSahoo, P. K., Moraes, P. H. R. S., Sahoo, P., & Bishi, B. K. (2018) · The European Physical Journal C · doi:10.1140/epjc/s10052-018-6211-4 · Cited by 47
Mustafa, G., Abbas, G., & Xia, T. (2019) · Chinese Journal of Physics · doi:10.1016/j.cjph.2019.05.025 · Cited by 44
Exploring the evidence for a large local void with supernovae Ia data
Luković, V. V., Haridasu, B. S., & Vittorio, N. (2019) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stz3070 · Cited by 44
“Indeed, calibrating SN Ia absolute magnitude with the use of Cepheid variable stars and fixing the local distance-redshift relation (at z ≤ 0.15) leads to a remarkable cosmology-independent measurement of H0 (Riess et al. 2005, 2007, 2009, 2011, 2016, 2018).”
MethodInfluentialHigh-redshift cosmography: Application and comparison with different methods
Hu, J.-P., & Wang, F. Y. (2022) · Astronomy and Astrophysics · doi:10.1051/0004-6361/202142162 · Cited by 44
A parametrization for the growth index of linear matter perturbations
Wu, P., Yu, H., & Fu, X. (2009) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2009/06/019 · Cited by 44
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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