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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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“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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Final Results from the Hubble Space Telescope Key Project to Measure the Hubble Constant
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Linder, E. V. (2003) · Physical Review Letters · doi:10.1103/physrevlett.90.091301 · Cited by 2,526
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Cited by
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Planck 2013 results. XVI. Cosmological parameters
Ade, P. A. R., Aghanim, N., Armitage-Caplan, C., Arnaud, M., Ashdown, M., Atrio-Barandela, F., Aumont, J., Baccigalupi, C., Banday, A. J., Barreiro, R. B., et al. (2014) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201321591 · Cited by 8,459
FIVE-YEAR WILKINSON MICROWAVE ANISOTROPY PROBE OBSERVATIONS: COSMOLOGICAL INTERPRETATION
Komatsu, E., Dunkley, J., Nolta, M. R., Bennett, C. L., Gold, B., Hinshaw, G., Jarosik, N., Larson, D., Limon, M., Page, L., et al. (2009) · The Astrophysical Journal Supplement Series · doi:10.1088/0067-0049/180/2/330 · Cited by 5,786
“The highz samples contain the Type Ia supernovae from the Hubble Space Telescope (Knop et al. 2003; Riess et al. 2004, 2007), the SuperNova Legacy Survey (SNLS) (Astier et al. 2006), the Equation of State: SupErNovae trace Cosmic Expansion (ESSENCE) survey (Wood-Vasey et al. 2007), as well as those used in the origina…”
InfluentialSelf-citationNINE-YEAR WILKINSON MICROWAVE ANISOTROPY PROBE ( WMAP ) OBSERVATIONS: COSMOLOGICAL PARAMETER RESULTS
Hinshaw, G., Larson, D., Komatsu, E., Spergel, D. N., Bennett, C. L., Dunkley, J., Nolta, M. R., Halpern, M., Hill, R. S., Odegard, N., et al. (2013) · The Astrophysical Journal Supplement Series · doi:10.1088/0067-0049/208/2/19 · Cited by 5,121
“…supernovae with 123 SNe at low redshift (Hamuy et al. 1996; Riess et al. 1999; Jha et al. 2006; Hicken et al. 2009; Contreras et al. 2010), 93 SNe from the SDSS supernovae search (Holtzman et al. 2008), and 14 SNe at z > 1 from HST measurements by Riess et al. (2007) to form a sample of 472 SNe.”
MethodSelf-citationLSST: From Science Drivers to Reference Design and Anticipated Data Products
Ivezić, Ž., Kahn, S. M., Tyson, J. A., Abel, B., Acosta, E., Allsman, R., Alonso, D., AlSayyad, Y., Anderson, S. F., Andrew, J., et al. (2019) · The Astrophysical Journal · doi:10.3847/1538-4357/ab042c · Cited by 4,357
“Probing Dark Energy and Dark Matter Current models of cosmology require the existence of both dark matter and dark energy to match observational constraints (Riess et al. 2007; Komatsu et al. 2009; Percival et al. 2010; LSST Dark Energy Science Collaboration 2012, and references therein).”
BackgroundSelf-citationScolnic, D. M., Jones, D. O., Rest, A., Pan, Y. C., Chornock, R., Foley, R. J., Huber, M. E., Kessler, R., Narayan, G., Riess, A. G., et al. (2018) · The Astrophysical Journal · doi:10.3847/1538-4357/aab9bb · Cited by 2,700
“The HST simulations are made in the same way as the PS1 and Low-z simulations, so that they directly represent the data in the SCP Cluster survey, GOODS, and CANDELS/CLASH surveys, but the spectroscopic selection efficiency was set equal to unity for these surveys.”
BackgroundMethodInfluentialSelf-citationNine-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Parameter Results
WRIGHT, E. L. (2016) · NASA STI Repository (National Aeronautics and Space Administration) · doi:10.15781/t2st7f05x · Cited by 2,604
Bamba, K., Capozzıello, S., Nojiri, S., & Odintsov, S. D. (2012) · Astrophysics and Space Science · doi:10.1007/s10509-012-1181-8 · Cited by 2,502
A 2.4% DETERMINATION OF THE LOCAL VALUE OF THE HUBBLE CONSTANT *
Riess, A. G., Macri, L. M., Hoffmann, S. L., Scolnic, D., Casertano, S., Filippenko, A. V., Tucker, B. E., Reid, M. J., Jones, D. O., Silverman, J. M., et al. (2016) · The Astrophysical Journal · doi:10.3847/0004-637x/826/1/56 · Cited by 2,250
“Together with the present acceleration q0=−0.55 and prior deceleration j0=1 which can be measured via high-redshift SNe Ia (Riess et al. 2007; Betoule et al. 2014) independently of the CMB or BAO, we find for the primary fit aB=0.71273±0.00176, with the uncertainty in q0 contributing 0.1%…”
MethodInfluentialSelf-citationCANDELS: THE COSMIC ASSEMBLY NEAR-INFRARED DEEP EXTRAGALACTIC LEGACY SURVEY
Grogin, N. A., Kocevski, D. D., Faber, S. M., Ferguson, H. C., Koekemoer, A. M., Riess, A. G., Acquaviva, V., Alexander, D. M., Almaini, O., Ashby, M. L. N., et al. (2011) · The Astrophysical Journal Supplement Series · doi:10.1088/0067-0049/197/2/35 · Cited by 2,137
“HST and ACS have played a unique role in the ongoing investigation of dark energy by enabling the discovery of 23 SNe Ia at z > 1, beyond the reach of ground-based telescopes (Riess et al. 2004, 2007).”
InfluentialSelf-citationKoekemoer, A., Faber, S., Ferguson, H., Grogin, N., Kocevski, D., Koo, D., Lai, K., Lotz, J., Lucas, R., McGrath, E., et al. (2011) · The Astrophysical Journal Supplement Series · doi:10.1088/0067-0049/197/2/36 · Cited by 1,812
“While SNe Ia at z. 1− 1.5 have already provided startling evidence of dark energy (Riess et al. 1998; Perlmutter et al. 1999; Riess et al. 2004, 2007), CANDELS now provides a direct probe of 1.5<z < 2.5 to test the nature of SNe Ia progenitors and their possible evolution (Ruiz-Lapuente & Canal…”
BackgroundInfluentialSelf-citationDark Energy and the Accelerating Universe
Frieman, J. A., Turner, M. S., & Dragan Huterer, A. (2008) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev.astro.46.060407.145243 · Cited by 2,100
“…have provided high-quality light curves (Knop et al. 2003) and have extended supernova measurements to redshift z + 1.8, providing evidence for the expected earlier epoch of deceleration and disfavoring dust extinction as an alternative explanation to acceleration (Riess et al. 2001, 2004, 2007).”
InfluentialImproved cosmological constraints from a joint analysis of the SDSS-II and SNLS supernova samples
Betoule, M., Kessler, R., Guy, J., Mosher, J., Hardin, D., Biswas, R., Astier, P., El-Hage, P., König, M., Kuhlmann, S. E., et al. (2014) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201423413 · Cited by 1,910
“In the most sensitive bands (g, r, i), the uncertainties introduced in the calibration transfer are now typically smaller than the uncertainty in the HST flux standards (∼3 mmag); in other words, our calibration is now limited by the precision in the CALSPEC flux calibration.”
MethodInfluentialSelf-citationHinshaw, G. F., Weiland, J. L., Hill, R., Odegard, N., Larson, D., Bennett, C. L., Dunkley, J., Gold, B., Greason, M. R., Jarosik, N., et al. (2009) · The Astrophysical Journal Supplement Series · doi:10.1088/0067-0049/180/2/225 · Cited by 1,769
“…(Percival et al. 2001; Tegmark et al. 2004; Cole et al. 2005; Tegmark et al. 2006; Eisenstein et al. 2005; Percival et al. 2007; Astier et al. 2006; Riess et al. 2007; Wood-Vasey et al. 2007) have established ΛCDM as the standard model of cosmology: a flat universe dominated by dark energy,…”
Self-citationDunkley, J., Komatsu, E., Nolta, M. R., Spergel, D. N., Larson, D., Hinshaw, G., Page, L., Bennett, C. L., Gold, B., Jarosik, N., et al. (2009) · The Astrophysical Journal Supplement Series · doi:10.1088/0067-0049/180/2/306 · Cited by 1,787
Self-citationSuzuki, N., Rubin, D., Lidman, C. E., Aldering, G., Amanullah, R., Barbary, K., Barrientos, L. F., Botyanszki, J., Brodwin, M., Connolly, N., et al. (2012) · The Astrophysical Journal · doi:10.1088/0004-637x/746/1/85 · Cited by 1,799
“Keck AO Photometry The photometry ofz > 1.2 SNe has been almost exclusively measured from HST images (Knop et al. 2003; Riess et al. 2004, 2007; Amanullah et al. 2010).”
BackgroundMethodInfluentialSelf-citationImproved Cosmological Constraints from New, Old, and Combined Supernova Data Sets
Kowalski, M. P., Rubin, D., Aldering, G., Agostinho, R., Amadon, A., Amanullah, R., Balland, C., Barbary, K., Blanc, G., Challis, P., et al. (2008) · The Astrophysical Journal · doi:10.1086/589937 · Cited by 1,541
“For comparison with previous work, Figure 13 shows our joint constraints on M and (statistical error only) and the Riess et al. (2007) constraints obtained from the Gold compilation of data primarily from the HZT, SCP, and SNLS (Riess et al. 2007) and a recent compilation of Davis et al. (2007),…”
BackgroundMethodResultInfluentialSelf-citationRiess, A. G., Macri, L. M., Casertano, S., Lampeitl, H., Ferguson, H. C., Filippenko, A. V., Jha, S. W., Li, W., & Chornock, R. (2011) · The Astrophysical Journal · doi:10.1088/0004-637x/730/2/119 · Cited by 1,513
“Together with the present acceleration q0 = −0.55 and prior deceleration j0 = 1 (Riess et al. 2007), we find av = 0.697 ± 0.00201.”
BackgroundInfluentialSelf-citationObservational probes of cosmic acceleration
Weinberg, D. H., Mortonson, M. J., Eisenstein, D. J., Hirata, C. M., Riess, A. G., & Rozo, E. (2013) · Physics Reports · doi:10.1016/j.physrep.2013.05.001 · Cited by 1,520
Self-citationThe Pantheon+ Analysis: Cosmological Constraints
Brout, D., Scolnic, D. M., Popovic, B., Riess, A. G., Carr, A., Zuntz, J., Kessler, R., Davis, T. M., Hinton, S. R., Jones, D. O., et al. (2022) · The Astrophysical Journal · doi:10.3847/1538-4357/ac8e04 · Cited by 1,369
“…Legacy Survey (SNLS; Betoule et al. 2014), Sloan Digital Sky Survey (SDSS; Sako et al. 2011), Hubble Space Telescope (HST; Gilliland et al. 1999; Riess et al. 2001, 2004, 2007; Suzuki et al. 2012; Riess et al. 2018), and Low-z (grouped together as LOSS_11; Ganeshalingam et al. 2010; LOSS_21;…”
BackgroundSelf-citationAmanullah, R., Lidman, C. E., Rubin, D., Aldering, G., Astier, P., Barbary, K., Burns, M. S., Conley, A., Dawson, K., Deustua, S. E., et al. (2010) · The Astrophysical Journal · doi:10.1088/0004-637x/716/1/712 · Cited by 1,368
“Revised HST zero-points and filter curves Since Riess et al. (2007), the reported zero-points of both NICMOS and ACS were revised.”
BackgroundMethodInfluentialAlam, S., Aubert, M., Avila, S., Balland, C., Bautista, J. E., Bershady, M. A., Bizyaev, D., Blanton, M. R., Bolton, A. S., Bovy, J., et al. (2021) · Physical Review D · doi:10.1103/physrevd.103.083533 · Cited by 1,337
“This high signal-to-noise spectrum, along with smaller aperture emission line measurements from Hubble Space Telescope and quasar absorption line observations, can all be explained by a selfconsistent outflow model.”
BackgroundInfluentialUV LUMINOSITY FUNCTIONS AT REDSHIFTS z ∼ 4 TO z ∼ 10: 10,000 GALAXIES FROM HST LEGACY FIELDS
Bouwens, R. J., Illingworth, G. D., Oesch, P. A., Trenti, M., Labbé, I., Bradley, L., Carollo, C. M., van Dokkum, P. G., Gonzalez, V., Holwerda, B. W., et al. (2015) · The Astrophysical Journal · doi:10.1088/0004-637x/803/1/34 · Cited by 1,298
“Optical observations are available over these fields as a result of the original ACS GOODS program (Giavalisco et al. 2004a) and extensive SNe search and follow-up observations (Riess et al. 2007).”
MethodProgenitors of Core-Collapse Supernovae
Smartt, S. J. (2009) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev-astro-082708-101737 · Cited by 1,235
“The analyses of data samples of such variable quality have often adopted subjective quality bins to describe the caliber of information available, such as using gold and silver categories (e.g. in designating the quality of high-z SNe Ia data sets, see Riess et al. 2007).”
BackgroundMoresco, M., Pozzetti, L., Cimatti, A., Jimenez, R., Maraston, C., Verde, L., Thomas, D., Citro, A., Tojeiro, R., & Wilkinson, D. (2016) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2016/05/014 · Cited by 1,182
“Moreover, the redshift range probed by BOSS proves to be fundamental to set cosmology independent constraints on the redshift at which the Universe expansion turns from decelerated to accelerated, which we refer to as the cosmological transition redshift [19, 20, 21, 22].”
BackgroundCHANDRACLUSTER COSMOLOGY PROJECT III: COSMOLOGICAL PARAMETER CONSTRAINTS
Vikhlinin, A., Kravtsov, A. V., Burenin, R., Ebeling, H., Forman, W. R., Hornstrup, A., Jones, C., Murray, S. S., Nagai, D., Quintana, H., et al. (2009) · The Astrophysical Journal · doi:10.1088/0004-637x/692/2/1060 · Cited by 1,081
“We use the distancemoduli estimated for the Type Ia supernovae from the HST sample of Riess et al. (2007), SNLS survey (Astier et al. 2006), and ESSENCE survey (Wood-Vasey et al. 2007), combined with the nearby supernova sample (we used a combination of all these samples compiled by Davis et al.…”
MethodMartin, J., Ringeval, C., & Vennin, V. (2014) · Physics of the Dark Universe · doi:10.1016/j.dark.2014.01.003 · Cited by 1,093
Moresco, M., Cimatti, A., Jimenez, R., Pozzetti, L., Zamorani, G., Bolzonella, M., Dunlop, J., Lamareille, F., Mignoli, M., Pearce, H., et al. (2012) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2012/08/006 · Cited by 1,012
Self-citationBlake, C., Kazin, E. A., Beutler, F., Davis, T. M., Parkinson, D., Brough, S., Colless, M., Contreras, C., Couch, W. J., Croom, S. M., et al. (2011) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2011.19592.x · Cited by 1,003
“…low-to-intermediate redshifts 0.1 < z < 0.3; the Supernova Legacy Survey (Astier et al. 2006) and ESSENCE (Wood-Vasey et al. 2007) projects at intermediate redshifts 0.3 < z < 1.0; and observations by the Hubble Space Telescope at high redshifts z > 1 (Riess et al. 2004, 2007; Dawson et al. 2009).”
BackgroundMethodInfluentialThe Pantheon+ Analysis: The Full Data Set and Light-curve Release
Scolnic, D. M., Brout, D., Carr, A., Riess, A. G., Davis, T. M., Dwomoh, A., Jones, D. O., Ali, N., Charvu, P., Chen, R. C., et al. (2022) · The Astrophysical Journal · doi:10.3847/1538-4357/ac8b7a · Cited by 957
Self-citationThe WiggleZ Dark Energy Survey: joint measurements of the expansion and growth history at z < 1
Blake, C., Brough, S., Colless, M., Contreras, C., Couch, W., Croom, S., Croton, D., Davis, T. M., Drinkwater, M. J., Forster, K., et al. (2012) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2012.21473.x · Cited by 929
“This compilation of 557 supernovae includes data from Hamuy et al. (1996), Riess et al. (1999, 2007), Astier et al. (2006), Jha et al. (2006), Wood-Vasey et al. (2007), Holtzman et al. (2008), Hicken et al. (2009) and Kessler et al. (2009).”
MethodWood‐Vasey, W. M., Miknaitis, G., Stubbs, C. W., Jha, S., Riess, A. G., Garnavich, P. M., Kirshner, R. P., Aguilera, C., Becker, A. C., Blackman, J. W., et al. (2007) · The Astrophysical Journal · doi:10.1086/518642 · Cited by 928
Self-citationConley, A., Guy, J., Sullivan, M., Regnault, N., Astier, P., Balland, C., Basa, S., Carlberg, R. G., Fouchez, D., Hardin, D., et al. (2010) · The Astrophysical Journal Supplement Series · doi:10.1088/0067-0049/192/1/1 · Cited by 910
“Altogether, we are left with a sample of 14 HST SNe from z = 0.7− 1.4.”
BackgroundMethodInfluentialIMPROVED DARK ENERGY CONSTRAINTS FROM ∼100 NEW CfA SUPERNOVA TYPE Ia LIGHT CURVES
Hicken, M., Wood‐Vasey, W. M., Blondin, S., Challis, P., Jha, S. W., Kelly, P. L., Rest, A., & Kirshner, R. (2009) · The Astrophysical Journal · doi:10.1088/0004-637x/700/2/1097 · Cited by 899
“On the time-evolution of 1+w, Riess et al. (2007) rule out rapidly evolving dark energy.”
BackgroundMethodSelf-citationQuintom Cosmology: theoretical implications and observations
Cai, Y., Saridakis, E., Setare, M., & Xia, J.-Q. (2009) · Physics Reports · doi:10.1016/j.physrep.2010.04.001 · Cited by 872
THE CLUSTER LENSING AND SUPERNOVA SURVEY WITH HUBBLE: AN OVERVIEW
Postman, M., Coe, D., Benítez, N., Bradley, L., Broadhurst, T. J., Donahue, M. E., Ford, H. C., Graur, O., Graves, G. J. M., Jouvel, S., et al. (2012) · The Astrophysical Journal Supplement Series · doi:10.1088/0067-0049/199/2/25 · Cited by 874
“From the 23 SNe Ia at z > 1 with HST data (Riess et al. 2004, 2007) we have learned: 1) that cosmic expansion was once decelerating before it recently began accelerating, 2) that dark energy, i.e., an energy density with w < 0, was already present during this prior decelerating phase, 3) that SNe…”
MethodSelf-citationLi, M., Li, X.-D., Wang, S., & Wang, Y. (2011) · Communications in Theoretical Physics · doi:10.1088/0253-6102/56/3/24 · Cited by 896
Riess, A. G., Macri, L. M., Casertano, S., Sosey, M., Lampeitl, H., Ferguson, H. C., Filippenko, A. V., Jha, S. W., Li, W., Chornock, R., et al. (2009) · The Astrophysical Journal · doi:10.1088/0004-637x/699/1/539 · Cited by 796
“This method was used by Riess et al. (2007) and Sullivan et al. (2007) to constrain multiple independent measures of w(z).”
BackgroundMethodResultInfluentialSelf-citationCosmological implications of baryon acoustic oscillation measurements
Aubourg, É., Bailey, S., Bautista, J., Beutler, F., Bhardwaj, V., Bizyaev, D., Blanton, M. R., Blomqvist, M., Bolton, A. S., Bovy, J., et al. (2015) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.92.123516 · Cited by 743
Self-citationTwo new diagnostics of dark energy
Varun Sahni, A., Shafieloo, A., & Starobinsky, A. A. (2008) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.78.103502 · Cited by 754
FIRST-YEAR SLOAN DIGITAL SKY SURVEY-II SUPERNOVA RESULTS: HUBBLE DIAGRAM AND COSMOLOGICAL PARAMETERS
Kessler, R., Becker, A. C., Cinabro, D., Vanderplas, J., Frieman, J. A., Marriner, J. P., Davis, T. M., Dilday, B., Holtzman, J. A., Jha, S. W., et al. (2009) · The Astrophysical Journal Supplement Series · doi:10.1088/0067-0049/185/1/32 · Cited by 695
“For SDSS-II, ESSENCE, SNLS, and HST, at least one measurement is required before peak brightness (Trest < 0 days); for the nearby sample, at least one measurement is required with Trest < +5 days.”
BackgroundMethodResultInfluentialSelf-citationWang, B., Abdalla, E., Atrio-Barandela, F., & Pavón, D. (2016) · Reports on Progress in Physics · doi:10.1088/0034-4885/79/9/096901 · Cited by 644
Baryon acoustic oscillations in the Ly α forest of BOSS quasars
Busca, N. G., Delubac, T., Rich, J., Bailey, S., Font-Ribera, A., Kirkby, D. P., Goff, J.-M. L., Pieri, M. M., Slosar, A., Aubourg, É., et al. (2013) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201220724 · Cited by 631
Self-citationAllen, S. W., Rapetti, D., Schmidt, R. W., Ebeling, H., Morris, R. G., & Fabian, A. C. (2007) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2007.12610.x · Cited by 636
“SNIa studies have established the presence of a systematic scatter of ∼ 7 per cent in distance measurements for individual SNIa using high quality data (Jha et al. 2007; see also e.g. Riess et al. 2004, 2007; Astier et al. 2006; WoodVasey et al. 2007).”
BackgroundMethodResultInfluentialDavis, T. M., Mörtsell, E., Sollerman, J., Becker, A. C., Blondin, S., Challis, P., Clocchiatti, A., Filippenko, A. V., Foley, R. J., Garnavich, P., et al. (2007) · The Astrophysical Journal · doi:10.1086/519988 · Cited by 605
“Giving an analytic form to the time evolution of w can act like a strong prior and may give misleading results (see Bassett et al. 2004; Riess et al. 2007, for further discussion).”
BackgroundMethodResultInfluentialSelf-citationBouwens, R. J., Illingworth, G. D., Franx, M., & Ford, H. C. (2007) · The Astrophysical Journal · doi:10.1086/521811 · Cited by 588
“…reductions not only take advantage of all the original data taken with ACS GOODS program, but also include all the ACS data associated with the SNe search (A. Riess et al. 2007, in preparation), GEMS (Rix et al. 2004), HUDF NICMOS (Thompson et al. 2005), and HUDF05 (Oesch et al. 2007) programs.”
MethodBouwens, R. J., Illingworth, G. D., Oesch, P. A., Labbé, I., Trenti, M., van Dokkum, P., Franx, M., Stiavelli, M., Carollo, C. M., Magee, D. K., et al. (2011) · The Astrophysical Journal · doi:10.1088/0004-637x/737/2/90 · Cited by 580
“0 reductions, but reach ∼0.1-0.3 mag deeper in the z850-band due to our inclusion of the SNe follow-up data (e.g., Riess et al. 2007).”
MethodInfluentialGuy, J., Sullivan, M., Conley, A., Regnault, N., Astier, P., Balland, C., Basa, S., Carlberg, R. G., Fouchez, D., Hardin, D., et al. (2010) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201014468 · Cited by 551
“On the contrary, the MLCS2k2 technique used in ESSENCE (Wood-Vasey et al. 2007), GOODS (Riess et al. 2004, 2007) and SDSS surveys (Kessler et al. 2009), assumes that the derived (B − V) colour offset primarily comes from extinction by dust, and therefore that theβ parameter should be identified…”
MethodInfluentialCANDELS MULTI-WAVELENGTH CATALOGS: SOURCE DETECTION AND PHOTOMETRY IN THE GOODS-SOUTH FIELD
Guo, Y.-C., Ferguson, H., Giavalisco, M., Barro, G., Willner, S., Ashby, M., Dahlén, T., Donley, J., Faber, S., Fontana, A., et al. (2013) · The Astrophysical Journal Supplement Series · doi:10.1088/0067-0049/207/2/24 · Cited by 372
“…(GO 9425 and 9583; see Giavalisco et al. 2004) and additional data acquired on the GOODS fields during the search for high redshift Type Ia supernovae carried out during Cycles 12 and 13 (Program ID 9727, P.I. Saul Perlmutter, and 9728, 10339, 10340, P.I. Adam Riess; see, e.g., Riess et al. 2007).”
BackgroundSelf-citationThe WiggleZ Dark Energy Survey: survey design and first data release
Drinkwater, M. J., Jurek, R. J., Blake, C., Woods, D., Pimbblet, K. A., Glazebrook, K., Sharp, R., Pracy, M., Brough, S., Colless, M., et al. (2009) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2009.15754.x · Cited by 528
“…and the latest supernova data from the supernova legacy survey (SNLS), HST and Equation of State: Supernovae Trace Cosmic Expansion (ESSENCE) projects (Astier et al. 2006; Riess et al. 2007; Wood-Vasey et al. 2007) to predict marginalized errors in our model of σ ( m) = 0.02 and σ (wconst) = 0.07.”
BackgroundInfluentialWang, S., Wang, Y., & Li, M. (2017) · Physics Reports · doi:10.1016/j.physrep.2017.06.003 · Cited by 530
“In recent years, several high quality supernova (SN) datasets have been released, such as “gold04” [59], “gold06” [60] “SNLS” [61], “ESSENCE” [62], “Union” [63], “Constitution” [64], “SDSS” [65], “Union2” [66], “SNLS3” [67] and “Union2.”
Bouwens, R. J., Illingworth, G. D., Oesch, P. A., Franx, M., Labbé, I., Trenti, M., van Dokkum, P., Carollo, C. M., González, V., Smit, R., et al. (2012) · The Astrophysical Journal · doi:10.1088/0004-637x/754/2/83 · Cited by 486
“We included all F814W observations from the ERS+CANDELS programs over the CDF-South.”
BackgroundInfluentialSupernova remnants: the X-ray perspective
Vink, J. (2011) · The Astronomy and Astrophysics Review · doi:10.1007/s00159-011-0049-1 · Cited by 473
Bamba, K., Odintsov, S. D., Sebastiani, L., & Zerbini, S. (2010) · The European Physical Journal C · doi:10.1140/epjc/s10052-010-1292-8 · Cited by 465
THE SLOAN DIGITAL SKY SURVEY-II SUPERNOVA SURVEY: TECHNICAL SUMMARY
Frieman, J. A., Bassett, B. A., Becker, A. C., Choi, C., Cinabro, D., DeJongh, F., DePoy, D. L., Dilday, B., Doi, M., Garnavich, P., et al. (2007) · The Astronomical Journal · doi:10.1088/0004-6256/135/1/338 · Cited by 462
“Hubble Space Telescope pilot programs in the z > 1 regime are in progress (Riess et al. 2007; Barbary et al. 2006).”
Self-citationAcevedo, M., Aguena, M., Alarcon, A., Allam, S., Alves, O., Amon, A., Andrade-Oliveira, F., Annis, J. T., Armstrong, P., Asorey, J., et al. (2024) · The Astrophysical Journal Letters · doi:10.3847/2041-8213/ad6f9f · Cited by 462
Self-citationCARNEGIE HUBBLE PROGRAM: A MID-INFRARED CALIBRATION OF THE HUBBLE CONSTANT
Freedman, W. L., Madore, B. F., Scowcroft, V., Burns, C. R., Monson, A. J., Persson, S. E., Seibert, M., & Rigby, J. R. (2012) · The Astrophysical Journal · doi:10.1088/0004-637x/758/1/24 · Cited by 460
“We use the SN Ia data from Sullivan et al. (2011), consisting of the SNLS 3 year sample, the SDSSII SN sample, the high-z sample from Riess et al. (2007), and several lowredshift samples from the literature.”
MethodSullivan, M., Guy, J., Conley, A., Regnault, N., Astier, P., Balland, C., Basa, S., Carlberg, R. G., Fouchez, D., Hardin, D., et al. (2011) · The Astrophysical Journal · doi:10.1088/0004-637x/737/2/102 · Cited by 455
“When combined together, recent SN Ia samples (Astier et al. 2006; Riess et al. 2007; Miknaitis et al. 2007; Holtzman et al. 2008; Hicken et al. 2009a; Contreras et al. 2010) provide measures of dark energy generally consistent with a cosmological constant of w = −1 with statistical uncertainties in…”
BackgroundInfluentialThe dependence of Type Ia Supernovae luminosities on their host galaxies
Sullivan, M., Conley, A., Howell, D. A., Neill, J. D., Astier, P., Balland, C., Basa, S., Carlberg, R. G., Fouchez, D., Guy, J., et al. (2010) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2010.16731.x · Cited by 439
“We also use the HST -discovered sample of Riess et al. (2004) and Riess et al. (2007), hereafter the R07 sample.”
MethodBouwens, R. J., Illingworth, G. D., Franx, M., Chary, R., Meurer, G. R., Conselice, C. J., Ford, H. C., Giavalisco, M., & van Dokkum, P. (2009) · The Astrophysical Journal · doi:10.1088/0004-637x/705/1/936 · Cited by 428
“These data were obtained as a result of the cumulative observations of many different HST programs (e.g., Dickinson 1999; Thompson et al. 1999; Thompson et al. 2005; Bouwens et al. 2005; Oesch et al. 2007; Riess et al. 2007; C. Conselice et al. 2009, in prep).”
MethodQuintom Cosmology: theoretical implications and observationsPreprint
Cai, Y.-F., Saridakis, E. N., & Setare, M. R. (2016) · Cited by 547
CFHTLenS: the Canada–France–Hawaii Telescope Lensing Survey – imaging data and catalogue products
Erben, T., Hildebrandt, H., Miller, L., Waerbeke, L. V., Heymans, C., Hoekstra, H., Kitching, T., Mellier, Y., Benjamin, J., Blake, C., et al. (2013) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stt928 · Cited by 412
HIGH-RESOLUTION CMB POWER SPECTRUM FROM THE COMPLETE ACBAR DATA SET
Reichardt, C. L., Ade, P. A. R., Bock, J. J., Bond, J. R., Brevik, J. A., Contaldi, C., Daub, M. D., Dempsey, J. T., Goldstein, J. H., Holzapfel, W. L., et al. (2009) · The Astrophysical Journal · doi:10.1088/0004-637x/694/2/1200 · Cited by 402
The WiggleZ Dark Energy Survey: joint measurements of the expansion and growth history at z 1Preprint
Blake, C., Brough, S., Colless, M., Contreras, C., Couch, W. J., Croom, S. M., Croton, D., Davis, T. M., Drinkwater, M. J., Förster, K., et al. (2024) · doi:10.25916/sut.26242559.v1 · Cited by 392
Approaches to understanding cosmic acceleration
Silvestri, A., & Trodden, M. (2009) · Reports on Progress in Physics · doi:10.1088/0034-4885/72/9/096901 · Cited by 405
“In more recent years, distant SNe with redshifts up to z ∼ 1.7 have been observed by the Hubble space telescope (HST) [17, 18].”
BackgroundInfluentialThermodynamics inf(R,T) theory of gravity
Sharif, M., & Zubair, M. (2012) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2012/03/028 · Cited by 391
HUBBLE RESIDUALS OF NEARBY TYPE Ia SUPERNOVAE ARE CORRELATED WITH HOST GALAXY MASSES
Kelly, P. L., Hicken, M., Burke, D. L., Mandel, K. S., & Kirshner, R. P. (2010) · The Astrophysical Journal · doi:10.1088/0004-637x/715/2/743 · Cited by 373
“SN Ia are useful probes of the cosmic expansion history (Astier et al. 2006; Wood-Vasey et al. 2007; Riess et al. 2007; Hicken et al. 2009b; Kessler et al. 2009a).”
Self-citationEvidence of the accelerated expansion of the Universe from weak lensing tomography with COSMOS
Schrabback, T., Hartlap, J., Joachimi, B., Kilbinger, M., Simon, P., Benabed, K., Bradač, M., Eifler, T. F., Erben, T., Fassnacht, C. D., et al. (2010) · Astronomy and Astrophysics · doi:10.1051/0004-6361/200913577 · Cited by 372
Deser, S., & Woodard, R. P. (2007) · Physical Review Letters · doi:10.1103/physrevlett.99.111301 · Cited by 425
“PACS numbers: 95.36.+x, 98.80.”
InfluentialThe observed growth of massive galaxy clusters - I. Statistical methods and cosmological constraints
Mantz, A. B., Allen, S. W., Rapetti, D., & Ebeling, H. (2010) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2010.16992.x · Cited by 391
“…Union compilation (Kowalski et al. 2008), which includes data from a variety of sources (307 SNIa in total; Hamuy et al. 1996; Garnavich et al. 1998; Riess et al. 1998, 1999, 2004, 2007; Schmidt et al. 1998; Perlmutter et al. 1999; Krisciunas et al. 2001, 2004a,b; Knop et al. 2003; Tonry et al.…”
BackgroundTHE CARNEGIE SUPERNOVA PROJECT: ANALYSIS OF THE FIRST SAMPLE OF LOW-REDSHIFT TYPE-Ia SUPERNOVAE
Folatelli, G., Phillips, M. M., Burns, C. R., Contreras, C., Hamuy, M., Freedman, W. L., Persson, S. E., Stritzinger, M. D., Suntzeff, N. B., Krisciunas, K., et al. (2009) · The Astronomical Journal · doi:10.1088/0004-6256/139/1/120 · Cited by 350
“In recent years, observations of SNe Ia to increasingly higher redshifts have confirmed this finding (e.g., Riess et al. 2007; Astier et al. 2006; Wood-Vasey et al. 2007).”
BackgroundSelf-citationSilverman, J. M., Foley, R. J., Filippenko, A. V., Ganeshalingam, M., Barth, A. J., Chornock, R., Griffith, C. V., Kong, J. J., Lee, N., Leonard, D. C., et al. (2012) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2012.21270.x · Cited by 356
“Type Ia supernovae (SNe Ia) have been particularly useful in recent years as a way to accurately measure cosmological parameters (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; Sullivan et al. 2011;…”
BackgroundSelf-citationDark energy two decades after: observables, probes, consistency tests
Dragan Huterer, A., & Shafer, D. L. (2017) · Reports on Progress in Physics · doi:10.1088/1361-6633/aa997e · Cited by 328
Quantifying the effect of baryon physics on weak lensing tomography
Semboloni, E., Hoekstra, H., Schaye, J., van Daalen, M. V., & McCarthy, I. (2011) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2011.19385.x · Cited by 268
“⋆ sembolon@strw.leidenuniv.nl Observations of type Ia supernovae provided the first evidence for the accelerated expansion (Perlmutter et al. 1999; Riess et al. 2007; Amanullah et al. 2010).”
BackgroundThe ESSENCE Supernova Survey: Survey Optimization, Observations, and Supernova Photometry
Miknaitis, G., Pignata, G., Rest, A., Wood‐Vasey, W. M., Blondin, S., Challis, P., Smith, R. C., Stubbs, C. W., Suntzeff, N. B., Foley, R. J., et al. (2007) · The Astrophysical Journal · doi:10.1086/519986 · Cited by 318
“The observation of acceleration from SNe Ia is the unique clue that indicates that this component must have negative pressure (Riess et al. 1998, 2001, 2004, 2007; Perlmutter et al. 1999; Tonry et al. 2003; Knop et al. 2003; Barris et al. 2004; Clocchiatti et al. 2006; Astier et al. 2006).”
BackgroundSelf-citationA candidate redshift z ≈ 10 galaxy and rapid changes in that population at an age of 500 Myr
Bouwens, R. J., Illingworth, G. D., Labbé, I., Oesch, P. A., Trenti, M., Carollo, C. M., van Dokkum, P., Franx, M., Stiavelli, M., González, V., et al. (2011) · Nature · doi:10.1038/nature09717 · Cited by 314
Towards an understanding of Type Ia supernovae from a synthesis of theory and observations
Hillebrandt, W., Kromer, M., Röpke, F. K., & Ruiter, A. J. (2013) · Frontiers of Physics · doi:10.1007/s11467-013-0303-2 · Cited by 291
THE CARNEGIE SUPERNOVA PROJECT: SECOND PHOTOMETRY DATA RELEASE OF LOW-REDSHIFT TYPE Ia SUPERNOVAE
Stritzinger, M. D., Phillips, M. M., Boldt, L., Burns, C. R., Campillay, A. R., Contreras, C., Gonzalez, S., Folatelli, G., Morrell, N., Krzemiński, W., et al. (2011) · The Astronomical Journal · doi:10.1088/0004-6256/142/5/156 · Cited by 286
“The current data have revealed that the equation-of- state parameter of the dark energy, w = P/(ρc2), is consistent with a cosmological constant, w = −1 (Astier et al. 2006; Wood-Vasey et al. 2007; Riess et al. 2007; Freedman et al. 2009; Sullivan et al. 2011).”
BackgroundSelf-citationz∼ 7–10 Galaxies in the HUDF and GOODS Fields: UV Luminosity Functions
Bouwens, R. J., Illingworth, G. D., Franx, M., & Ford, H. C. (2008) · The Astrophysical Journal · doi:10.1086/590103 · Cited by 281
“We estimated that there would be 0.0, 0.3, 0.2, and 0.3 low-redshift contaminants, respectively, for our z-dropout selections over the HUDF, NICPAR, HDFN, and GOODS parallel fields.”
BackgroundInfluentialCapozzıello, S., Cardone, V. F., & Salzano, V. (2008) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.78.063504 · Cited by 286
Union through UNITY: Cosmology with 2000 SNe Using a Unified Bayesian Framework
Rubin, D., Aldering, G., Betoule, M., Fruchter, A., Huang, X., Kim, A., Lidman, C. E., Linder, E. V., Perlmutter, S., Ruiz-Lapuente, P., et al. (2025) · The Astrophysical Journal · doi:10.3847/1538-4357/adc0a5 · Cited by 505
Guo, Y., Ferguson, H. C., Bell, E. F., Koo, D. C., Conselice, C. J., Giavalisco, M., Kassin, S. A., Lu, Y., Lucas, R., Mandelker, N., et al. (2015) · The Astrophysical Journal · doi:10.1088/0004-637x/800/1/39 · Cited by 258
“…(GO 9425 and 9583; see Giavalisco et al. 2004) and additional data acquired on the GOODS fields during the search for high redshift Type Ia supernovae carried out during Cycles 12 and 13 (Program ID 9727, P.I. Saul Perlmutter, and 9728, 10339, 10340, P.I. Adam Riess; see, e.g., Riess et al. 2007).”
BackgroundSelf-citationFrom cosmic deceleration to acceleration: new constraints from SN Ia and BAO/CMB
Giostri, R., dos Santos, M. V., Waga, I., Reis, R. R. R., Calvão, M. O., & Lago, B. L. (2012) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2012/03/027 · Cited by 261
Mimetic Gravity: A Review of Recent Developments and Applications to Cosmology and Astrophysics
Sebastiani, L., Vagnozzi, S., & Myrzakulov, R. (2017) · Advances in High Energy Physics · doi:10.1155/2017/3156915 · Cited by 274
Riess, A. G., Rodney, S., Scolnic, D. M., Shafer, D. L., Strolger, L.-G., Ferguson, H. C., Postman, M., Graur, O., Maoz, D., Jha, S. W., et al. (2018) · The Astrophysical Journal · doi:10.3847/1538-4357/aaa5a9 · Cited by 250
“We also require that the first epoch with >3σ detection must be no more than 10 days after the peak of the light curve in the rest-frame B band, consistent with the requirements used by Riess et al. (1996) and Riess et al. (2007).”
BackgroundMethodInfluentialSelf-citationObservational tests of modified gravity
Jain, B., & Zhang, P. (2008) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.78.063503 · Cited by 249
Bouwens, R. J., Illingworth, G. D., Oesch, P. A., Trenti, M., Stiavelli, M., Carollo, C. M., Franx, M., van Dokkum, P. G., Labbé, I., & Magee, D. K. (2009) · The Astrophysical Journal Letters · doi:10.1088/2041-8205/708/2/l69 · Cited by 243
“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).”
BackgroundInfluentialBlake, C., Davis, T. M., Poole, G. B., Parkinson, D., Brough, S., Colless, M., Contreras, C., Couch, W., Croom, S. M., Drinkwater, M. J., et al. (2011) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2011.19077.x · Cited by 238
“…those arising from type Ia supernovae data from the “Union2” compilation by Amanullah et al. (2010), which includes data from Hamuy et al. (1996), Riess et al. (1999, 2007), Astier et al. (2006), Jha et al. (2006), Wood-Vasey et al. (2007), Holtzman et al. (2008), Hicken et al. (2009) and…”
MethodGaneshalingam, M., Li, W., Filippenko, A. V., Anderson, C., Foster, G., Gates, E. L., Griffith, C. V., Grigsby, B. J., Joubert, N., Leja, J., et al. (2010) · The Astrophysical Journal Supplement Series · doi:10.1088/0067-0049/190/2/418 · Cited by 234
“…distance indicators, playing a critical role in the discovery and subsequent study of the accelerating expansion of the universe and dark energy (Riess et al. 1998, 2007; Perlmutter et al. 1999; Hamuy et al. 1996a; Wood-Vasey et al. 2007; Kowalski et al. 2008; Hicken et al. 2009a); see…”
BackgroundSelf-citationTHEORETICAL MODELS OF DARK ENERGY
Yoo, J., & Watanabe, Y. (2012) · International Journal of Modern Physics D · doi:10.1142/s0218271812300029 · Cited by 246
THE SLOAN DIGITAL SKY SURVEY-II SUPERNOVA SURVEY: SEARCH ALGORITHM AND FOLLOW-UP OBSERVATIONS
Sako, M., Bassett, B. A., Becker, A. C., Cinabro, D., DeJongh, F., DePoy, D. L., Dilday, B., Doi, M., Frieman, J. A., Garnavich, P., et al. (2007) · The Astronomical Journal · doi:10.1088/0004-6256/135/1/348 · Cited by 232
“…and the Equation of State: Supernovae Trace Cosmic Expansion (ESSENCE2; Wood-Vasey et al. 2007; Miknaitis et al. 2007) – and from space using the HST (Riess et al. 2004a, 2007; Barbary et al. 2006) have substantially increased the sample of high-z SNe, and have provided much-improved statistical…”
MethodSelf-citationZhang, X., & Wu, F. (2007) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.76.023502 · Cited by 254
“[68] lately released the up-to-date 182 “gold” data of SNIa from various sources analyzed in a consistent and robust mannor with reduced calibration errors arising from systematics.”
BackgroundMethodInfluentialCluster constraints on f(R) gravity
Schmidt, F., Vikhlinin, A. A., & Hu, W. (2009) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.80.083505 · Cited by 227
Cosmic clocks, cosmic variance and cosmic averages
Wiltshire, D. L. (2007) · New Journal of Physics · doi:10.1088/1367-2630/9/10/377 · Cited by 246
The Data Release of the Sloan Digital Sky Survey-II Supernova Survey
Sako, M., Bassett, B. A., Becker, A. C., Brown, P. J., Campbell, H. C., Wolf, R. C., Cinabro, D., D’Andrea, C. B., Dawson, K., DeJongh, F., et al. (2018) · Publications of the Astronomical Society of the Pacific · doi:10.1088/1538-3873/aab4e0 · Cited by 225
“At higher redshift, new surveys included ESSENCE (Miknaitis et al. 2007), the Supernova Legacy Survey (SNLS; Astier et al. 2006), and dedicated HST observations by Riess et al. (2007).”
BackgroundSelf-citationCfA4: LIGHT CURVES FOR 94 TYPE Ia SUPERNOVAE
Hicken, M., Challis, P., Kirshner, R., Rest, A., Cramer, C. E., Wood‐Vasey, W. M., Bakos, G. Á., Berlind, P., Brown, W. R., Caldwell, N., et al. (2012) · The Astrophysical Journal Supplement Series · doi:10.1088/0067-0049/200/2/12 · Cited by 223
“Sullivan et al. (2011) combine all three years of the Supernova Legacy Survey data with the nearby, first-year SDSS-II and Higher-z (Riess et al. 2007) samples to measure 1+w = 0.061+0.069−0.068, where a flat universe is assumed and the uncertainties include all statistical and SN Ia systematic…”
MethodInfluentialSelf-citationConfronting Lemaitre–Tolman–Bondi models with observational cosmology
García-Bellido, J., & Haugbølle, T. (2008) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2008/04/003 · Cited by 220
(2018) · doi:10.1103/physrevd.97.103503 · Cited by 233
Thawing quintessence 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.77.083515 · Cited by 237
Evidence for anisotropy of cosmic acceleration
Colin, J., Mohayaee, R., Rameez, M., & Sarkar, S. (2019) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201936373 · Cited by 213
“It is stated that the inclusion of these corrections allow SNe Ia with redshifts down to 0.01 to be included in the cosmological analysis, in contrast to earlier analyses (Riess et al. 2007) which employed only SNe Ia down to z = 0.023.”
ResultInfluentialCosmography in f ( Q ) gravity
Mandal, S., Wang, D., & Sahoo, P. K. (2020) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.102.124029 · Cited by 229
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 ›
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