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New Hubble Space Telescope Discoveries of Type Ia Supernovae at z≥ 1: Narrowing Constraints on the Early Behavior of Dark Energy
Open accessAbstract
We have discovered 21 new Type Ia supernovae (SNe Ia) with the Hubble Space Telescope ( HST ) and have used them to trace the history of cosmic expansion over the last 10 billion yr. These objects, which include 13 spectroscopically confirmed SNe Ia at z ≥ 1, were discovered during 14 epochs of reimaging of the GOODS fields North and South over 2 yr with the Advanced Camera for Surveys on HST . Together with a recalibration of our previous HST -discovered SNe Ia, the full sample of 23 SNe Ia at z ≥ 1 provides the highest redshift sample known. Combining these data with previous SN Ia data sets, we measured H ( z ) at discrete, uncorrelated epochs, reducing the uncertainty of H ( z > 1) from 50% to under 20%, strengthening the evidence for a cosmic jerk—the transition from deceleration in the past to acceleration in the present. The unique leverage of the HST high-redshift SNe Ia provides the first meaningful constraint on the dark energy equation-of-state parameter at z ≥ 1. The result remains consistent with a cosmological constant [ w ( z ) = −1] and rules out rapidly evolving dark energy ( dw / dz ≫ 1). The defining property of dark energy, its negative pressure, appears to be present at z > 1, in the epoch preceding acceleration, with ~98% confidence in our primary fit. Moreover, the z > 1 sample-averaged spectral energy distribution is consistent with that of the typical SN Ia over the last 10 Gyr, indicating that any spectral evolution of the properties of SNe Ia with redshift is still below our detection threshold.
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“Current models of cosmology require the existence of both dark matter and dark energy to match observational constraints”
From LSST: From Science Drivers to Reference Design and Anticipated Data Products (2019) · cites this paper as Riess et al. 2007
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“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).”
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Self-citationExploring the Expansion History of the Universe
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ACCELERATING UNIVERSES WITH SCALING DARK MATTER
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Note on Tsallis holographic dark energy
Zadeh, M. A., Sheykhi, A., Moradpour, H., & Bamba, K. (2018) · The European Physical Journal C · doi:10.1140/epjc/s10052-018-6427-3 · Cited by 120
Sánchez, A. G., Crocce, M., Cabre, A., Baugh, C. M., & GAZTAÑAGA, E. (2009) · Max Planck Digital Library · Cited by 113
Avelino, A., & Nucamendi, U. (2009) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2009/04/006 · Cited by 120
“We use the definition of luminosity distance dL [3, 5, 85]–[87] in a flat cosmology, it is”
THE DEEP3 GALAXY REDSHIFT SURVEY: KECK/DEIMOS SPECTROSCOPY IN THE GOODS-N FIELD
Cooper, M. C., Aird, J., Coil, A. L., Davis, M., Faber, S. M., Juneau, S., Lotz, J. M., Nandra, K., Newman, J. A., Willmer, C. N. A., et al. (2011) · The Astrophysical Journal Supplement Series · doi:10.1088/0067-0049/193/1/14 · Cited by 112
“Altogether, the TKRS observed nearly 3000 sources, yielding secure spectroscopic redshifts for ∼ 1500 objects and enabling numerous studies of galaxy evolution and cosmology (e.g., Kobulnicky & Kewley 2004; Weiner et al. 2006; Riess et al. 2007; Juneau et al. 2010).”
BackgroundParsa, S., Dunlop, J., McLure, R., & Mortlock, A. (2015) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stv2857 · Cited by 82
“…(CANDELS) (Grogin et al. 2011; Koekemoer et al. 2011; Windhorst et al. 2011), and the associated pre-existing HST optical (Giavalisco et al. 2004; Riess et al. 2007), ground-based VLT U band (Nonino et al. 2009) and Ks band (Retzlaff et al. 2010; Fontana et al. 2014), and Spitzer IRAC imaging…”
BackgroundFuture Cosmological Constraints From Fast Radio Bursts
Walters, A., Weltman, A., Gaensler, B. M., Ma, Y.-Z., & Witzemann, A. (2018) · The Astrophysical Journal · doi:10.3847/1538-4357/aaaf6b · Cited by 111
“…galaxy power spectrum (Beutler et al. 2011; Anderson et al. 2014; Ross et al. 2015), luminosity distance–redshift relation of TypeIa supernovae (SNIa; Riess et al. 2004, 2007; Kowalski et al. 2008; Betoule et al. 2014), local distance ladder (Riess et al. 2016), galaxy clustering and weak lensing…”
BackgroundAn accelerating cosmology without dark energy
Steigman, G., Santos, R. C., & Lima, J. A. S. (2009) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2009/06/033 · Cited by 109
WRIGHT, E. L. (2007) · The Astrophysical Journal · doi:10.1086/519274 · Cited by 110
“Wood-Vasey et al. (2007) recently published supernova data from the ESSENCE project, while Riess et al. (2007) have published a large sample of supernovae from the SNLS project (Astier et al. 2006), the HST, and Hi-z Supernova Team.”
BackgroundMethodInfluentialRubin, D., Aldering, G., Barbary, K., Boone, K., Chappell, G., Currie, M. H., Deustua, S., Fagrelius, P., Fruchter, A. S., Hayden, B., et al. (2015) · The Astrophysical Journal · doi:10.1088/0004-637x/813/2/137 · Cited by 109
“Some distant SN surveys (Tonry et al. 2003; Riess et al. 2007; Amanullah et al. 2010; Suzuki et al. 2012; Rubin et al. 2013) had selections that were different (bluer) than rest-frame B-band.”
BackgroundCosmographic Hubble fits to the supernova data
Cattoën, C., & Visser, M. (2008) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.78.063501 · Cited by 109
Some issues concerning holographic dark energy
Li, M., Lin, C., & Wang, Y. (2008) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2008/05/023 · Cited by 118
Measuring cosmic bulk flows with Type Ia supernovae from the Nearby Supernova Factory
Feindt, U., Kerschhaggl, M., Kowalski, M. P., Aldering, G., Antilogus, P. E., Aragon, C., Bailey, S., Baltay, C., Bongard, S., Buton, C., et al. (2013) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201321880 · Cited by 108
“Additionally we analyzed the Union2 compilation (Amanullah et al. 2010) of 577 SNe of which 165 are at redshifts below z = 0.1 (Hamuy et al. 1996; Riess et al. 1998, 1999, 2007; Perlmutter et al. 1999; Knop et al. 2003; Tonry et al. 2003; Barris et al. 2004; Krisciunas et al. 2005; Astier et al.…”
MethodInfluentialHints of FLRW breakdown from supernovae
Krishnan, C., Mohayaee, R., Colgáin, E. Ó., Sheikh-Jabbari, M. M., & Yin, L. (2022) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.105.063514 · Cited by 111
Predicted and Observed Evolution in the Mean Properties of Type Ia Supernovae with Redshift
Howell, D. A., Sullivan, M., Conley, A., & Carlberg, R. G. (2007) · The Astrophysical Journal · doi:10.1086/522030 · Cited by 108
“We then compare the predicted evolution in lightcurve stretch to SN distributions from the SNLS and the Higher-z SN Search (Riess et al. 2007).”
BackgroundMethodInfluentialGorini, V., Kamenshchik, A. Y., Moschella, U., Piattella, O. F., & Starobinsky, A. A. (2008) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2008/02/016 · Cited by 111
He, J.-H., Wang, B., & Zhang, P. (2009) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.80.063530 · Cited by 108
Maguire, K., Sullivan, M., Ellis, R. S., Nugent, P., Howell, D. A., Gal-Yam, A., Cooke, J., Mazzali, P. A., Pan, Y.-C., Dilday, B., et al. (2012) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2012.21909.x · Cited by 107
“…(SNe Ia) as cosmological probes is now well established; significant advancements in constraining the cosmological parameters using distant SNe Ia (Riess et al. 2007; Kessler et al. 2009; Sullivan et al. 2011) have been made since the initial discovery of the accelerating Universe at the end of…”
BackgroundTHE EXTENDEDHUBBLE SPACE TELESCOPESUPERNOVA SURVEY: THE RATE OF CORE COLLAPSE SUPERNOVAE TOz∼ 1
Dahlén, T., Strolger, L.-G., Riess, A. G., Mattila, S., Kankare, E., & Mobasher, B. (2012) · The Astrophysical Journal · doi:10.1088/0004-637x/757/1/70 · Cited by 107
“Observations The data used in this investigation were obtained during HST Cycles 11–13 (2002–2005) and consist of 1 reference and 13 search images in the GOODS-North and 1 reference and 9 search images in the GOODS-South fields (Giavalisco et al. 2004; Riess et al. 2004, 2007).”
MethodSelf-citationAHubble Space Telescopesurvey of the host galaxies of Superluminous Supernovae
Angus, C. R., Levan, A. J., Perley, D. A., Tanvir, N. R., Lyman, J. D., Stanway, E. R., & Fruchter, A. S. (2016) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stw063 · Cited by 107
“Our CCSNe host sample is based on that detected in the rolling SNe searches of the GOODS field (Dahlen et al. 2003; Fruchter et al. 2006; Riess et al. 2007; Strolger, Dahlen & Riess 2010; Svensson et al. 2010).”
MethodHipólito-Ricaldi, W. S., Velten, H., & Zimdahl, W. (2010) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.82.063507 · Cited by 108
Cosmological reconstruction and stability in $$f(R,T)$$ f ( R , T ) gravity
Sharif, M., & Zubair, M. (2014) · General Relativity and Gravitation · doi:10.1007/s10714-014-1723-1 · Cited by 106
Growth factor parametrization and modified gravity
Gong, Y. (2008) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.78.123010 · Cited by 116
Dynamical instability of the charged expansion-free spherical collapse in f(R) gravity
Sharif, M., & Yousaf, Z. (2013) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.88.024020 · Cited by 106
Taubenberger, S., Benetti, S., Childress, M. J., Pakmor, R., Hachinger, S., Mazzali, P. A., Stanishev, V., Elias-Rosa, N., Agnoletto, I., Bufano, F., et al. (2011) · Max Planck Digital Library · Cited by 105
Testing the isotropy of the Universe with type Ia supernovae
Campanelli, L., Paolo Cea, A., Fogli, G. L., & Marrone, A. (2011) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.83.103503 · Cited by 105
Dark energy model with spinor matter and its quintom scenario
Cai, Y.-F., & Wang, J. (2008) · Classical and Quantum Gravity · doi:10.1088/0264-9381/25/16/165014 · Cited by 113
Features of holographic dark energy under combined cosmological constraints
Ma, Y.-Z., Gong, Y., & Chen, X. (2009) · The European Physical Journal C · doi:10.1140/epjc/s10052-009-0876-7 · Cited by 104
Noether symmetry approach in phantom quintessence cosmology
Capozzıello, S., Piedipalumbo, E., Rubano, C., & Scudellaro, P. (2009) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.80.104030 · Cited by 109
Dynamical analysis of self-gravitating stars in f(R,T) gravity
Sharif, M., & Yousaf, Z. (2014) · Astrophysics and Space Science · doi:10.1007/s10509-014-2113-6 · Cited by 103
Bianchi Type-I Anisotropic Dark Energy Model with Constant Deceleration Parameter
Pradhan, A., Amirhashchi, H., & Saha, B. (2011) · International Journal of Theoretical Physics · doi:10.1007/s10773-011-0793-z · Cited by 114
Studying the diversity of Type Ia supernovae in the ultraviolet: comparing models with observations
Walker, E. S., Hachinger, S., Mazzali, P. A., Ellis, R. S., Sullivan, M., Gal‐Yam, A., & Howell, D. A. (2012) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2012.21928.x · Cited by 102
“SNe Ia studies have measured that w, the dark energy equation of state parameter is consistent with w = −1 to 6.5% with some studies at high-z even beginning to place constraints on whether w = w(z) (Riess et al. 2007).”
ResultInfluentialVELOCITY EVOLUTION AND THE INTRINSIC COLOR OF TYPE Ia SUPERNOVAE
Foley, R. J., Sanders, N. E., & Kirshner, R. P. (2011) · The Astrophysical Journal · doi:10.1088/0004-637x/742/2/89 · Cited by 102
“…expansion of the Universe is accelerating (Riess et al. 1998; Perlmutter et al. 1999), and constrain the equation-of-state parameter of dark energy (Wood-Vasey et al. 2007; Riess et al. 2007; Hicken et al. 2009b; Kessler et al. 2009; Amanullah et al. 2010; Conley et al. 2011; Sullivan et al. 2011).”
BackgroundSelf-citationThe Beginning and Evolution of the Universe
Ratra, B., & Vogeley, M. S. (2008) · Publications of the Astronomical Society of the Pacific · doi:10.1086/529495 · Cited by 118
Maguire, K., Sullivan, M., Pan, Y. C., Gal‐Yam, A., Hook, I., Howell, D. A., Nugent, P., Mazzali, P. A., Chotard, N., Clubb, K. I., et al. (2014) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stu1607 · Cited by 101
“The use of Type Ia supernovae (SNe Ia) as cosmological probes is firmly established (e.g., Riess et al. 1998, 2007; Perlmutter et al. c© 0000 RAS 1999; Kessler et al. 2009; Sullivan et al. 2011; Suzuki et al.2012; Ganeshalingam et al. 2013; Rest et al. 2013; Betoule et al. 2014).”
BackgroundSelf-citationCharged gravastars in modified gravity
Yousaf, Z., Bamba, K., Bhatti, M. Z. U. H., & Ghafoor, U. (2019) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.100.024062 · Cited by 100
Spherical collapse and the halo model in braneworld gravity
Schmidt, F., Hu, W., & Lima, M. (2010) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.81.063005 · Cited by 101
MEASURING COSMOLOGICAL PARAMETERS WITH GAMMA RAY BURSTS
Amati, L., & Valle, M. D. (2013) · International Journal of Modern Physics D · doi:10.1142/s0218271813300280 · Cited by 101
THE PROGENITORS OF TYPE Ia SUPERNOVAE. I. ARE THEY SUPERSOFT SOURCES?
Stefano, R. D. (2010) · The Astrophysical Journal · doi:10.1088/0004-637x/712/1/728 · Cited by 100
“Type Ia supernovae (SNe Ia) help us to explore the history of the cosmos (see, e.g., Riess et al. 2007; Kuznetsova et al. 2008).”
BackgroundEvidence for Emergent Dark Energy
Li, X., & Shafieloo, A. (2020) · The Astrophysical Journal · doi:10.3847/1538-4357/abb3d0 · Cited by 100
Cosmology with gamma-ray bursts
Demiański, M., Piedipalumbo, E., Sawant, D., & Amati, L. (2016) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201628911 · Cited by 100
“…past dozen years a huge and diverse set of observational data revealed that the Universe is now expanding at an accelerated rate, see for instance ( Riess et al. 2007), (Astier et al. 2006), ( Riess et al. 2011), ( Suzuki et al. 2012), ( Planck Collaboration 2013), and (Planck Collaboration 2015).”
BackgroundVitagliano, V. M., Xia, J., Liberati, S., & Viel, M. (2010) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2010/03/005 · Cited by 100
Model-independent distance measurements from gamma-ray bursts and constraints on dark energy
Wang, Y. (2008) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.78.123532 · Cited by 100
Jones, D. O., Scolnic, D. M., Foley, R. J., Rest, A., Kessler, R., Challis, P., Chambers, K. C., Coulter, D. A., Dettman, K., Foley, M. M., et al. (2019) · The Astrophysical Journal · doi:10.3847/1538-4357/ab2bec · Cited by 99
“…of the dark energy equation-of-state parameter, w, have been steadily improving (Garnavich et al. 1998; Knop et al. 2003; Tonry et al. 2003; Riess et al. 2004, 2007; Astier et al. 2006; Wood-Vasey et al. 2007; Kowalski et al. 2008; Kessler et al. 2009; Sullivan et al. 2011; Betoule et al.…”
BackgroundSelf-citationInteracting ghost dark energy in non-flat universe
Sheykhi, A., & Movahed, M. S. (2011) · General Relativity and Gravitation · doi:10.1007/s10714-011-1286-3 · Cited by 98
Evolution of the universe in entropic cosmologies via different formulations
KOMATSU, N., & KIMURA, S. (2014) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.89.123501 · Cited by 106
Observational bounds on the cosmic radiation density
Hamann, J., Hannestad, S., Raffelt, G. G., & Wong, Y. Y. Y. (2007) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2007/08/021 · Cited by 98
“This sample is a compilation of supernovae measured by the Supernova Legacy Survey (SNLS) [30], the ESSENCE project [31], and the Hubble Space Telescope [ 32 ], as well as a set of 45 nearby supernovae.”
MethodBerkeley Supernova Ia Program - II. Initial analysis of spectra obtained near maximum brightness
Silverman, J. M., Kong, J. J., & Filippenko, A. V. (2012) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2012.21269.x · Cited by 98
“…supernovae (SNe Ia) have been particularly useful in recent years as a way 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; Suzuki et al. 2012), and led to the…”
BackgroundSelf-citationDilday, B., Smith, M., Bassett, B. A., Becker, A. C., Bender, R., Castander, F. J., Cinabro, D., Filippenko, A. V., Frieman, J. A., Galbany, L., et al. (2010) · The Astrophysical Journal · doi:10.1088/0004-637x/713/2/1026 · Cited by 98
“…distances to SNe Ia and thereby place important constraints on cosmological models (e.g., Riess et al. 1998; Perlmutter et al. 1999; Riess et al. 2004; Astier et al. 2006; Wood-Vasey et al. 2007; Riess et al. 2007; Hicken et al. 2009; Riess et al. 2009; Freedman et al. 2009; Kessler et al. 2009).”
BackgroundSelf-citationEffects of dark sectors' mutual interaction on the growth of structures
He, J.-H., Wang, B., & Jing, Y. (2009) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2009/07/030 · Cited by 98
TYPE Ia SUPERNOVA CARBON FOOTPRINTS
Thomas, R. C., Aldering, G., Antilogus, P. E., Aragon, C., Bailey, S., Baltay, C., Bongard, S., Buton, C., Canto, A., Childress, M., et al. (2011) · The Astrophysical Journal · doi:10.1088/0004-637x/743/1/27 · Cited by 97
“…itself is accelerating, in contrast to previous expectations that it would be found to be decelerating (Riess et al. 1998; Perlmutter et al. 1999; Astier et al. 2006; Riess et al. 2007; Wood-Vasey et al. 2007; Kowalski et al. 2008; Hicken et al. 2009; Sullivan et al. 2011; Suzuki et al. 2011).”
ResultBaltic Sea biodiversity status vs. cumulative human pressures
Andersen, J. H., Halpern, B. S., Korpinen, S., Murray, C., & Reker, J. (2015) · Estuarine Coastal and Shelf Science · doi:10.1016/j.ecss.2015.05.002 · Cited by 103
Avelino, A., & Nucamendi, U. (2010) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2010/08/009 · Cited by 101
“We use the definition of luminosity distance dL (see [3, 5, 66]–[68]) in a flat cosmology,”
The ExtendedHSTSupernova Survey: The Rate of SNe Ia atz> 1.4 Remains Low
Dahlén, T., Strolger, L., & Riess, A. G. (2008) · The Astrophysical Journal · doi:10.1086/587978 · Cited by 97
“The SNe used in this investigation are described in detail in Riess et al. (2004, 2007) and Strolger et al. (2004; L. G. Strolger et al. 2008, in preparation).”
BackgroundMethodInfluentialSelf-citationScale dependence of cosmological backreaction
Li, N., & Schwarz, D. J. (2008) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.78.083531 · Cited by 97
Gamma-ray bursts in 1.8 < z < 5.6 suggest that the time variation of the dark energy is small
Kodama, Y., Yonetoku, D., Murakami, T., Tanabe, S., Tsutsui, R., & Nakamura, T. (2008) · Monthly Notices of the Royal Astronomical Society Letters · doi:10.1111/j.1745-3933.2008.00508.x · Cited by 97
“We found the empirical formula of the luminosity distance of Type Ia supernovae in Riess et al. (2007) with 0.359 < z < 1.755 as dL(z) 1027cm = 14.57 × z1.”
BackgroundMethodInfluentialNoether symmetry of F(T) cosmology with quintessence and phantom scalar fields
Jamil, M., Momeni, D., & Myrzakulov, R. (2012) · The European Physical Journal C · doi:10.1140/epjc/s10052-012-2137-4 · Cited by 96
Casimir wormholes in modified symmetric teleparallel gravity
Hassan, Z., Ghosh, S., Sahoo, P. K., & Bamba, K. (2022) · The European Physical Journal C · doi:10.1140/epjc/s10052-022-11107-0 · Cited by 95
Examining the cosmic acceleration with the latest Union2 supernova data
Li, Z., Wu, P., & Yu, H. (2010) · Physics Letters B · doi:10.1016/j.physletb.2010.10.044 · Cited by 95
DeterminingH0with Bayesian hyper-parameters
Cardona, W., Kunz, M., & Pettorino, V. (2017) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2017/03/056 · Cited by 94
Field theory model for dark matter and dark energy in interaction
Micheletti, S., Elcio Abdalla, A., & Wang, B. (2009) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.79.123506 · Cited by 94
Cosmological Constraints from Type Ia Supernovae Peculiar Velocity Measurements
Gordon, C., Land, K., & Slosar, A. (2007) · Physical Review Letters · doi:10.1103/physrevlett.99.081301 · Cited by 95
Lee, K.-S., Giavalisco, M., Conroy, C., Wechsler, R. H., Ferguson, H. C., Somerville, R. S., Dickinson, M., & Urry, C. M. (2009) · The Astrophysical Journal · doi:10.1088/0004-637x/695/1/368 · Cited by 93
“…of the B435V606i775z850 imaging data taken with the Advanced Camera for Surveys (ACS) on HST obtained as part of the Great Observatories Origins Deep Survey (GOODS: Giavalisco et al. 2004b) with a significant addition of exposure time taken as part of the supernovae search (Riess et al. 2007).”
MethodSelf-citationA DETAILED STUDY OF PHOTOMETRIC REDSHIFTS FOR GOODS-SOUTH GALAXIES
Dahlen, T., Mobasher, B., Dickinson, M., Ferguson, H. C., Giavalisco, M., Grogin, N. A., Guo, Y., Koekemoer, A. M., Lee, K.-S., Lee, S.-K., et al. (2010) · The Astrophysical Journal · doi:10.1088/0004-637x/724/1/425 · Cited by 93
“These images were then combined with further ACS exposures from the HST Supernovae search project (Riess et al. 2007), adding five more epochs, making these among the deepest HST data currently available.”
MethodSelf-citationReconstruction of cosmic history from a simple parametrization of H
Pacif, S. K. J., Myrzakulov, R., & Myrzakul, S. (2017) · International Journal of Geometric Methods in Modern Physics · doi:10.1142/s0219887817501110 · Cited by 94
Barotropic index w -singularities in cosmology
Da̧browski, M. P., & Denkiewicz, T. (2009) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.79.063521 · Cited by 93
Dynamics of an interacting dark energy model in Einstein and loop quantum cosmology
Chen, S., Wang, B., & Jing, J. (2008) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.78.123503 · Cited by 95
SOME ASPECTS OF GENERALIZED MODIFIED GRAVITY MODELS
MYRZAKULOV, R., SEBASTIANI, L., & Zerbini, S. (2013) · International Journal of Modern Physics D · doi:10.1142/s0218271813300176 · Cited by 96
Definition of complexity factor for self-gravitating systems in Palatini f(R) gravity
Yousaf, Z. (2020) · Physica Scripta · doi:10.1088/1402-4896/ab9479 · Cited by 92
Constraints on dark energy with the LOSS SN Ia sample
Ganeshalingam, M., Li, W., & Filippenko, A. V. (2013) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stt893 · Cited by 92
“Searching for SNe Ia at these redshifts is more feasible from a space-based telescope such as HST. Targeted searches for higher-z SNe have produced a sample in the redshift range 0.2 < z < 1.55 (Riess et al. 2007).”
BackgroundMethodInfluentialSelf-citationFinite-time singularities in f(R, T) gravity and the effect of conformal anomaly
Houndjo, M. J. S., Batista, C. E. M., Campos, J. P., & Piattella, O. F. (2013) · Canadian Journal of Physics · doi:10.1139/cjp-2013-0023 · Cited by 91
Onset of cosmological backreaction
Li, N., & Schwarz, D. J. (2007) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.76.083011 · Cited by 91
The DEEP3 galaxy redshift survey: Keck/DEIMOS spectroscopy in the GOODS-N field
Cooper, M., Aird, J., Coil, A., Davis, M., Faber, S. M., Juneau, S., Lotz, J., Nandra, K., Newman, J., Willmer, C., et al. (2011) · Max Planck Digital Library · Cited by 91
LINKING TYPE Ia SUPERNOVA PROGENITORS AND THEIR RESULTING EXPLOSIONS
Foley, R. J., Simon, J. D., Burns, C. R., Gal‐Yam, A., Hamuy, M., Kirshner, R., Morrell, N., Phillips, M. M., Shields, G. A., & Sternberg, A. (2012) · The Astrophysical Journal · doi:10.1088/0004-637x/752/2/101 · Cited by 90
“…(Riess et al. 1998; Perlmutter et al. 1999) and continue to be exquisite tools for constraining cosmological parameters (Wood-Vasey et al. 2007; Riess et al. 2007; Freedman et al. 2009; Hicken et al. 2009b; Kessler et al. 2009; Amanullah et al. 2010; Conley et al. 2011; Suzuki et al. 2012).”
BackgroundSelf-citationA divergence-free parametrization of deceleration parameter for scalar field dark energy
Mamon, A. A., & Das, S. (2016) · International Journal of Modern Physics D · doi:10.1142/s0218271816500322 · Cited by 96
Rodney, S., Patel, B., Scolnic, D. M., Foley, R. J., Molino, A., Brammer, G., Jauzac, M., Bradač, M., Broadhurst, T. J., Coe, D., et al. (2015) · The Astrophysical Journal · doi:10.1088/0004-637x/811/1/70 · Cited by 89
“Second, the value of 0.08 mag determined in Conley et al. (2011) is specific to the HST SN sample, from Riess et al. (2007) and Suzuki et al. (2012), which is the SN subset that is most similar to HFF14Tom in terms of redshift and data analysis.”
BackgroundMethodInfluentialSelf-citationSilverman, J. M., & Filippenko, A. V. (2012) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2012.21276.x · Cited by 89
“…to discover the accelerating expansion of the Universe (Riess et al. 1998; Perlmutter et al. 1999), as well as to 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; Suzuki et al. 2012).”
BackgroundSelf-citationBeyond Concordance Cosmology with Magnification of Gravitational-Wave Standard Sirens
Camera, S., & Nishizawa, A. (2013) · Physical Review Letters · doi:10.1103/physrevlett.110.151103 · Cited by 89
Dynamic vacuum variable and equilibrium approach in cosmology
Klinkhamer, F. R., & Воловик, Г. Е. (2008) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.78.063528 · Cited by 100
Electromagnetic field and cylindrical compact objects in modified gravity
Yousaf, Z., & Bhatti, M. Z. U. H. (2016) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stw423 · Cited by 88
“1 INTRODUCTION It seems established from direct observations (Perlmutter et al. 1999; Riess et al. 2007; Komatsu et al. 2011) of high red-shift supernovae as well as the cosmic microwave background fluctuations that the universe expands with acceleration at present state indicating the presence of…”
BackgroundL’Huillier, B., & Shafieloo, A. (2017) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2017/01/015 · Cited by 88
Construction of charged cylindrical gravastar-like structures
Yousaf, Z. (2020) · Physics of the Dark Universe · doi:10.1016/j.dark.2020.100509 · Cited by 88
CONSTRAINING THE DARK ENERGY EQUATION OF STATE WITH COSMIC VOIDS
Lee, J., & Park, D. (2009) · The Astrophysical Journal · doi:10.1088/0004-637x/696/1/l10 · Cited by 87
“The following observables have so far been suggested to discriminate the dark en- ergy models: the luminosity-distance measure of type Ia supernova (Riess et al. 2004, 2007; Davis et al. 2007; Kowalski et al. 2008); the abundance of galaxy clusters as a function of mass (Wang & Steinhardt 1998;…”
BackgroundThe growth of matter perturbations in some scalar–tensor DE models
Gannouji, R., & Polarski, D. (2008) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2008/05/018 · Cited by 93
Evidence of short-lived SN Ia progenitors
Aubourg, É., Tojeiro, R., Jiménez, R., Heavens, A., Strauss, M. A., & Spergel, D. N. (2008) · Astronomy and Astrophysics · doi:10.1051/0004-6361:200809796 · Cited by 85
“Current SN Ia surveys such as SNLS (Astier et al., 2006), ESSENCE (Wood-Vasey et al., 2007), and GOODS-SN (Riess et al., 2007) are contributing to current constraints on cosmological parameters, and SNe Ia will continue to be important for cosmological constraints in the next generation of surveys…”
BackgroundHOST GALAXIES OF TYPE Ia SUPERNOVAE FROM THE NEARBY SUPERNOVA FACTORY
Childress, M., Aldering, G., Antilogus, P. E., Aragon, C., Bailey, S., Baltay, C., Bongard, S., Buton, C., Canto, A., Cellier-Holzem, F., et al. (2013) · The Astrophysical Journal · doi:10.1088/0004-637x/770/2/107 · Cited by 85
“…constrain the energy content of the Universe (Riess et al. 1998; Perlmutter et al. 1999; Tonry et al. 2003; Knop et al. 2003; Wood-Vasey et al. 2007; Riess et al. 2007; Kowalski et al. 2008; Hicken et al. 2009; Kessler et al. 2009; Amanullah et al. 2010; Sullivan et al. 2011; Suzuki et al. 2012).”
BackgroundBouwens, R. J., Illingworth, G. D., González, V., Labbé, I., Franx, M., Conselice, C. J., Blakeslee, J. P., van Dokkum, P., Holden, B. P., Magee, D. K., et al. (2010) · The Astrophysical Journal · doi:10.1088/0004-637x/725/2/1587 · Cited by 85
“0 reductions, but reach ∼0.1-0.3 mag deeper in the z850-band due to the inclusion of the SNe follow-up data (Riess et al. 2007).”
BackgroundInfluentialExistence of compact structures in f(R, T) gravity
Yousaf, Z., Bhatti, M. Z.-U.-H., & Ilyas, M. (2018) · The European Physical Journal C · doi:10.1140/epjc/s10052-018-5797-x · Cited by 84
Sauer, D. N., Mazzali, P. A., Blondin, S., Stehle, M., Benetti, S., Challis, P., Filippenko, A. V., Kirshner, R. P., Li, W., & Matheson, T. (2008) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2008.14018.x · Cited by 84
“With the empirical calibration of their peak luminosity (Phillips 1993; Phillips et al. 1999; Jha, Riess & Kirshner 2007), it is feasible to probe the properties of the Universe out to a redshift of z ≈ 1 and higher (Goldhaber et al. 2001; Tonry et al. 2003; Riess et al. 2004, 2007).”
BackgroundSelf-citationArt of lattice and gravity waves from preheating
Huang, Z. (2011) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.83.123509 · Cited by 98
Testing general relativity at cosmological scales: Implementation and parameter correlations
Dossett, J. N., Ishak, M., & Moldenhauer, J. (2011) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.84.123001 · Cited by 83
Jackson, N. J. (2015) · Living Reviews in Relativity · doi:10.1007/lrr-2015-2 · Cited by 83
The updated luminosity correlations of gamma-ray bursts and cosmological implications
Wang, F. Y., Qi, S., & Dai, Z.-G. (2011) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2011.18961.x · Cited by 83
“A nearly model-independent approach in which uncorrelated estimates are made about discrete w(z) at different redshifts has been extensively discussed (Huterer & Cooray 2005; Riess et al. 2007; Sullivan et al. 2007; Qi, Wang & Lu 2008).”
BackgroundTHE DISCOVERY OF THE MOST DISTANT KNOWN TYPE Ia SUPERNOVA AT REDSHIFT 1.914
Jones, D. O., Rodney, S., Riess, A. G., Mobasher, B., Dahlén, T., McCully, C., Frederiksen, T. F., Casertano, S., Hjorth, J., Keeton, C. R., et al. (2013) · The Astrophysical Journal · doi:10.1088/0004-637x/768/2/166 · Cited by 83
“Over the past decade, measurements of Type Ia supernovae (SNe) at redshift z & 1 have extended the observed population to a time when the universe was matter dominated (Riess et al. 2001, 2004, 2007; Suzuki et al. 2012; Rodney et al. 2012; Rubin et al. 2013).”
BackgroundSelf-citationA model with interaction of dark components and recent observational data
Pan, S., & Sharov, G. S. (2017) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stx2278 · Cited by 83
The age problem in the ΛCDM model
Yang, R.-J., & Zhang, S. N. (2010) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2010.17020.x · Cited by 87
“SNIa, R, A, d, and H(z) To consider observational bounds on ΛCDM model for a flat Universe, we use the recently published 182 gold SNIa data with 23 SNIa at z & 1 obtained by imposing constraints Av < 0.5 (excluding high extinction) (Riess et al. 2007).”
MethodInfluentialAlimi, J., Füzfa, A., Boucher, V., Rasera, Y., Courtin, J., & Corasaniti, P.-S. (2009) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2009.15712.x · Cited by 83
“…et al. 1998, 2001; Perlmutter et al. 1999) which have been recently confirmed by more accurate detections (Knop et al. 2003; Astier et al. 2006; Riess et al. 2007), in combination with precise measurements of Cosmic Microwave Background (CMB) anisotropies (De Bernardis et al. 2000; Spergel et…”
BackgroundObservational evidence of the accelerated expansion of the universe
Astier, P., & Pain, R. (2012) · Comptes Rendus Physique · doi:10.1016/j.crhy.2012.04.009 · Cited by 93
A modified holographic dark energy model with infrared infinite extra dimension(s)
Gong, Y., & Li, T. (2009) · Physics Letters B · doi:10.1016/j.physletb.2009.12.040 · Cited by 86
Evidence of a decreasing trend for the Hubble constant
Jia, X., Hu, J.-P., & Wang, F. Y. (2023) · Astronomy and Astrophysics · doi:10.1051/0004-6361/202346356 · Cited by 85
Consistency among distance measurements: transparency, BAO scale and accelerated expansion
Avgoustidis, A., Verde, L., & Jiménez, R. (2009) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2009/06/012 · Cited by 82
“While the H(z) data of [30] and [13] for z = 0 yield f(z) directly, Supernovae-determined dL does not, and f(z) can be inferred only taking a derivative [9, 28, 31].”
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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