New Hubble Space Telescope Discoveries of Type Ia Supernovae at z≥ 1: Narrowing Constraints on the Early Behavior of Dark Energy

Riess, Adam G.; Strolger, Louis‐Gregory; Casertano, Stefano; Ferguson, Henry C.; Mobasher, Bahram; Gold, Ben; Challis, Peter J.; Filippenko, Alexei V.; Jha, Saurabh; Li, Weidong; Tonry, John; Foley, Ryan; Kirshner, Robert P.; Dickinson, Mark; MacDonald, Emily; Eisenstein, Daniel; Livio, Mario; Younger, Josh; Xu, Chun; Dahlen, Tomas; Stern, Daniel

doi:10.1086/510378

Cited by 1,758Cosmology and Gravitation TheoriesGamma-ray bursts and supernovaeGalaxies: Formation, Evolution, Phenomena

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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Riess, Adam G., Strolger, Louis‐Gregory, Casertano, Stefano, Ferguson, Henry C., Mobasher, Bahram, Gold, Ben, Challis, Peter J., Filippenko, Alexei V. +13 more·2007·The Astrophysical Journal

DOI 10.1086/510378

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Abstract

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 cosmological models need both dark matter and dark energy to fit observational constraints.
“Current models of cosmology require the existence of both dark matter and dark energy to match observational constraints”
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Riess, A. G., Strolger, L.-G., Tonry, J. L., Tsvetanov, Z., Casertano, S., Ferguson, H. C., Mobasher, B., Challis, P., Panagia, N., Filippenko, A. V., et al. (2004) · The Astrophysical Journal · doi:10.1086/378311 · Cited by 75 · see citing works
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Cosmological Constant or Intergalactic Dust? Constraints from the Cosmic Far‐Infrared Background
Aguirre, A. N., & Haiman, Z. (2000) · The Astrophysical Journal · doi:10.1086/308557 · Cited by 74 · see citing works
The Age of the Universe and the Cosmological Constant Determined from Cosmic Microwave Background Anisotropy Measurements
Knox, L., Christensen, N. L., & Skordis, C. (2001) · CERN Document Server (European Organization for Nuclear Research) · Cited by 74 · see citing works
Quintessential Cosmology Novel Models of Cosmological Structure Formation
Caldwell, R. R., Dave, R., & Steinhardt, P. J. (1998) · Astrophysics and Space Science · doi:10.1023/a:1002028230277 · Cited by 69 · see citing works
Measuring the properties of extragalactic dust and implications for the Hubble diagram
Goobar, A., Bergström, L., & Mörtsell, E. (2002) · Astronomy and Astrophysics · doi:10.1051/0004-6361:20020002 · Cited by 64 · see citing works
The Magnification of SN 1997[CLC]ff[/CLC], the Farthest Known Supernova
Benítez, N., Riess, A. G., Nugent, P., Dickinson, M., Chornock, R., & Filippenko, A. V. (2002) · The Astrophysical Journal · doi:10.1086/344048 · Cited by 63 · see citing works
Self-citation
Spectra of High-Redshift Type Ia Supernovae and a Comparison with Their Low-Redshift Counterparts
Hook, I., Howell, D. A., Aldering, G., Amanullah, R., Burns, M. S., Conley, A., Deustua, S. E., Ellis, R. S., Fabbro, S., Fadeyev, V., et al. (2005) · The Astronomical Journal · doi:10.1086/497635 · Cited by 60 · see citing works
Limiting the dimming of distant type Ia supernovae
Östman, L., & Mörtsell, E. (2005) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2005/02/005 · Cited by 59 · see citing works
Nonlinear Decline‐Rate Dependence and Intrinsic Variation of Type Ia Supernova Luminosities
Wang, L., Strovink, M., Conley, A., Goldhaber, G., Kowalski, M. P., Perlmutter, S., & Siegrist, J. L. (2006) · The Astrophysical Journal · doi:10.1086/500422 · Cited by 58 · see citing works
Optical Spectra of Type I[CLC]a[/CLC] Supernovae at [CLC][ITAL]z[/ITAL][/CLC] = 0.46 and [CLC][ITAL]z[/ITAL][/CLC] = 1.2
Coil, A. L., Matheson, T., Filippenko, A. V., Leonard, D. C., Tonry, J. L., Riess, A. G., Challis, P., Clocchiatti, A., Garnavich, P., Hogan, C. J., et al. (2000) · The Astrophysical Journal · doi:10.1086/317311 · Cited by 58 · see citing works
Self-citation
The First Type Ia Supernovae: An Empirical Approach to Taming Evolutionary Effects in Dark Energy Surveys from SNe Ia atz > 2
Riess, A. G., & Livio, M. (2006) · The Astrophysical Journal · doi:10.1086/504791 · Cited by 53 · see citing works
Self-citation
Hubble Space TelescopeObservations of Nine High-Redshift ESSENCE Supernovae
Krisciunas, K., Garnavich, P., Challis, P., Prieto, J. L., Riess, A. G., Barris, B. J., Aguilera, C., Becker, A. C., Blondin, S., Chornock, R., et al. (2005) · The Astronomical Journal · doi:10.1086/497640 · Cited by 45 · see citing works
Self-citation
Lensing Magnification of Supernovae in the GOODS Fields
Jonsson, J., Dahlen, T., Goobar, A., Gunnarsson, C., Mortsell, E., & Lee, K. (2006) · The Astrophysical Journal · doi:10.1086/499396 · Cited by 37 · see citing works
Self-citation
Exploring dark energy with SNAP
Aldering, G. (2005) · New Astronomy Reviews · doi:10.1016/j.newar.2005.08.002 · Cited by 34 · see citing works
A Light Echo from Type Ia SN 1995E?
Quinn, J., Garnavich, P., Li, W., Panagia, N., Riess, A. G., Schmidt, B. P., & Valle, M. D. (2006) · The Astrophysical Journal · doi:10.1086/507826 · Cited by 33 · see citing works
Self-citation
Cardassian expansion: dark energy density from modified Friedmann equations
Freese, K. (2005) · New Astronomy Reviews · doi:10.1016/j.newar.2005.01.007 · Cited by 32 · see citing works
Cardassian Expansion: Dark Energy Density from Modified Friedmann Equations
Freese, K. (2005) · CERN Document Server (European Organization for Nuclear Research) · Cited by 26 · see citing works
Lensing magnification of supernovae in the GOODS-fields
Jonsson, J., Dahlen, T., Goobar, A., Gunnarsson, C., Mortsell, E., & Lee, K. (2005) · CERN Document Server (European Organization for Nuclear Research) · Cited by 24 · see citing works
Self-citation
Absorption effects of intergalactic natural graphite whiskers on observations at microwave and radio frequencies
Rana, N. (1979) · Astrophysics and Space Science · doi:10.1007/bf00648369 · Cited by 23 · see citing works
Absorption effects due to intergalactic long whiskers of pyrolytic graphite and the cosmic microwave background
Rana, N. (1980) · Astrophysics and Space Science · doi:10.1007/bf00646913 · Cited by 19 · see citing works
Spectroscopy of twelve type Ia supernovae at intermediate redshift
Balland, C., Mouchet, M., Pain, R., Walton, N. A., Amanullah, R., Astier, P., Ellis, R. S., Fabbro, S., Goobar, A., Hardin, D., et al. (2005) · Astronomy and Astrophysics · doi:10.1051/0004-6361:20053552 · Cited by 15 · see citing works
A Direct Upper Limit on the Density of Cosmological Dust from the Absence of an X‐Ray Scattering Halo around thez = 4.3 Quasar QSO 1508 \documentclass{aastex} \usepackage{amsbsy} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{bm} \usepackage{mathrsfs} \usepackage{pifont} \usepackage{stmaryrd} \usepackage{textcomp} \usepackage{portland,xspace} \usepackage{amsmath,amsxtra} \usepackage[OT2,OT1]{fontenc} \newcommand\cyr{ \renewcommand\rmdefault{wncyr} \renewcommand\sfdefault{wncyss} \renewcommand\encodingdefault{OT2} \normalfont \selectfont} \DeclareTextFontCommand{\textcyr}{\cyr} \pagestyle{empty} \DeclareMathSizes{10}{9}{7}{6} \begin{document} \landscape $+$ \end{document} 5714
Petric, A. O., Telis, G. A., Paerels, F. B. S., & Helfand, D. J. (2006) · The Astrophysical Journal · doi:10.1086/507667 · Cited by 14 · see citing works
Methanol in the L1551 Circumbinary Torus
White, G. J., Fridlund, C. V. M., Bergman, P., Beardsmore, A., Liseau, R., Price, M. C., & Phillips, R. R. (2006) · The Astrophysical Journal · doi:10.1086/509570 · Cited by 10 · see citing works
Spectroscopy of twelve Type Ia supernovae at intermediate redshift
Balland, C., Mouchet, M., Pain, R., Walton, N. A., Amanullah, R., Astier, P., Ellis, R. S., Fabbro, S., Goobar, A., Hardin, D., et al. (2005) · Springer Link (Chiba Institute of Technology) · doi:10.1051/0004-6361:20053552/pdf · Cited by 10 · see citing works
NICMOS Count Rate Dependent Non-Linearity in G096 and G141
Bohlin, R. C., Riess, A. G., & de Jong, R. (2006) · Cited by 9 · see citing works
Self-citation
Dark energy search with supernovae
Wang, Y. (2005) · New Astronomy Reviews · doi:10.1016/j.newar.2005.01.034 · Cited by 6 · see citing works
4 Dark Energy Search with SupernovaePreprint
Wang, Y. (2004) · Cited by 4 · see citing works

Flagged first, then by citations

Research works printed but not linked: 8

Albrecht, A., & Bernstein, G. 2006, preprint (astro-ph /0608269)
de Jong, R. S., et al. 2006, in The 2005 HST Calibration Workshop, ed.
---. 2004, in Measuring and Modeling the Universe, ed. W. L. Freedman (Cambridge: Cambridge Univ. Press), 270
---. 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
Riess, A. G., Press, W. H., & Kirshner, R. P. 1995, ApJ, 438, L17
Wood-Vasey, W. M., et al. 2007, ApJ, in press (astro-ph/0701041) · arXiv

Sorted by citations

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 6,875 · see citing works
FIVE-YEARWILKINSON MICROWAVE ANISOTROPY PROBEOBSERVATIONS: 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 · see citing works
“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-citation
NINE-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 · see citing works
“…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-citation
LSST: 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 · see citing works
“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-citation
The Complete Light-curve Sample of Spectroscopically Confirmed SNe Ia from Pan-STARRS1 and Cosmological Constraints from the Combined Pantheon Sample
Scolnic, 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 · see citing works
“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-citation
Nine-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 · see citing works
Dark energy cosmology: the equivalent description via different theoretical models and cosmography tests
Bamba, K., Capozzıello, S., Nojiri, S., & Odintsov, S. D. (2012) · Astrophysics and Space Science · doi:10.1007/s10509-012-1181-8 · Cited by 2,400 · see citing works
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 · see citing works
“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-citation
CANDELS: 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 · see citing works
“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-citation
CANDELS: THE COSMIC ASSEMBLY NEAR-INFRARED DEEP EXTRAGALACTIC LEGACY SURVEY—THE HUBBLE SPACE TELESCOPE OBSERVATIONS, IMAGING DATA PRODUCTS, AND MOSAICS
Koekemoer, 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 · see citing works
“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-citation
Dark 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 1,948 · see citing works
“…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).”
Influential
Improved 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 1,912 · see citing works
“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-citation
FIVE-YEAR WILKINSON MICROWAVE ANISOTROPY PROBE OBSERVATIONS: DATA PROCESSING, SKY MAPS, AND BASIC RESULTS
Hinshaw, 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 · see citing works
“…(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-citation
FIVE-YEAR WILKINSON MICROWAVE ANISOTROPY PROBE OBSERVATIONS: LIKELIHOODS AND PARAMETERS FROM THE WMAP DATA
Dunkley, 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 · see citing works
Self-citation
THEHUBBLE SPACE TELESCOPECLUSTER SUPERNOVA SURVEY. V. IMPROVING THE DARK-ENERGY CONSTRAINTS ABOVEz> 1 AND BUILDING AN EARLY-TYPE-HOSTED SUPERNOVA SAMPLE
Suzuki, 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 1,721 · see citing works
“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-citation
Improved 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 · see citing works
“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-citation
A 3% SOLUTION: DETERMINATION OF THE HUBBLE CONSTANT WITH THEHUBBLE SPACE TELESCOPEAND WIDE FIELD CAMERA 3
Riess, 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 · see citing works
“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-citation
Observational 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 1,393 · see citing works
Self-citation
The 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 · see citing works
“…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-citation
SPECTRA AND HUBBLE SPACE TELESCOPE LIGHT CURVES OF SIX TYPE Ia SUPERNOVAE AT 0.511 < z < 1.12 AND THE UNION2 COMPILATION
Amanullah, 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 · see citing works
“Revised HST zero-points and filter curves Since Riess et al. (2007), the reported zero-points of both NICMOS and ACS were revised.”
BackgroundMethodInfluential
Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Cosmological implications from two decades of spectroscopic surveys at the Apache Point Observatory
Alam, 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 · see citing works
“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.”
BackgroundInfluential
UV 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 · see citing works
“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).”
Method
Progenitors 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 · see citing works
“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).”
Background
A 6% measurement of the Hubble parameter at z∼0.45: direct evidence of the epoch of cosmic re-acceleration
Moresco, 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 · see citing works
“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].”
Background
CHANDRACLUSTER 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 · see citing works
“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.…”
Method
Encyclopædia Inflationaris
Martin, J., Ringeval, C., & Vennin, V. (2024) · Physics of the Dark Universe · doi:10.1016/j.dark.2014.01.003 · Cited by 396 · see citing works
Improved constraints on the expansion rate of the Universe up to z ∼ 1.1 from the spectroscopic evolution of cosmic chronometers
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 · see citing works
Self-citation
The WiggleZ Dark Energy Survey: mapping the distance-redshift relation with baryon acoustic oscillations
Blake, 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 · see citing works
“…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).”
BackgroundMethodInfluential
The 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 · see citing works
Self-citation
The 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 · see citing works
“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).”
Method
Observational Constraints on the Nature of Dark Energy: First Cosmological Results from the ESSENCE Supernova Survey
Wood‐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 · see citing works
Self-citation
SUPERNOVA CONSTRAINTS AND SYSTEMATIC UNCERTAINTIES FROM THE FIRST THREE YEARS OF THE SUPERNOVA LEGACY SURVEY
Conley, 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 · see citing works
“Altogether, we are left with a sample of 14 HST SNe from z = 0.7− 1.4.”
BackgroundMethodInfluential
IMPROVED 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 · see citing works
“On the time-evolution of 1+w, Riess et al. (2007) rule out rapidly evolving dark energy.”
BackgroundMethodSelf-citation
Quintom 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 · see citing works
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 849 · see citing works
“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-citation
Dark Energy
Li, M., Li, X.-D., Wang, S., & Wang, Y. (2011) · Communications in Theoretical Physics · doi:10.1088/0253-6102/56/3/24 · Cited by 838 · see citing works
A REDETERMINATION OF THE HUBBLE CONSTANT WITH THE HUBBLE SPACE TELESCOPE FROM A DIFFERENTIAL DISTANCE LADDER
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 · see citing works
“This method was used by Riess et al. (2007) and Sullivan et al. (2007) to constrain multiple independent measures of w(z).”
BackgroundMethodResultInfluentialSelf-citation
Cosmological 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 · see citing works
Self-citation
Two 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 710 · see citing works
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 · see citing works
“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-citation
Dark matter and dark energy interactions: theoretical challenges, cosmological implications and observational signatures
Wang, 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 · see citing works
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 · see citing works
Self-citation
Improved constraints on dark energy from Chandra X-ray observations of the largest relaxed galaxy clusters
Allen, 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 630 · see citing works
“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).”
BackgroundMethodResultInfluential
Scrutinizing Exotic Cosmological Models Using ESSENCE Supernova Data Combined with Other Cosmological Probes
Davis, 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 · see citing works
“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-citation
UV Luminosity Functions atz∼4, 5, and 6 from the Hubble Ultra Deep Field and Other DeepHubble Space TelescopeACS Fields: Evolution and Star Formation History
Bouwens, R. J., Illingworth, G. D., Franx, M., & Ford, H. C. (2007) · The Astrophysical Journal · doi:10.1086/521811 · Cited by 588 · see citing works
“…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.”
Method
ULTRAVIOLET LUMINOSITY FUNCTIONS FROM 132z∼ 7 ANDz∼ 8 LYMAN-BREAK GALAXIES IN THE ULTRA-DEEP HUDF09 AND WIDE-AREA EARLY RELEASE SCIENCE WFC3/IR OBSERVATIONS
Bouwens, 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 · see citing works
“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).”
MethodInfluential
The Supernova Legacy Survey 3-year sample: Type Ia supernovae photometric distances and cosmological constraints
Guy, 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 571 · see citing works
“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…”
MethodInfluential
CANDELS 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 · see citing works
“…(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-citation
The 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 517 · see citing works
“…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.”
BackgroundInfluential
Holographic dark energy
Wang, S., Wang, Y., & Li, M. (2017) · Physics Reports · doi:10.1016/j.physrep.2017.06.003 · Cited by 500 · see citing works
“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.”
UV-CONTINUUM SLOPES AT z ∼ 4-7 FROM THE HUDF09+ERS+CANDELS OBSERVATIONS: DISCOVERY OF A WELL-DEFINED UV COLOR-MAGNITUDE RELATIONSHIP FOR z ⩾ 4 STAR-FORMING GALAXIES
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 · see citing works
“We included all F814W observations from the ERS+CANDELS programs over the CDF-South.”
BackgroundInfluential
Supernova remnants: the X-ray perspective
Vink, J. (2011) · The Astronomy and Astrophysics Review · doi:10.1007/s00159-011-0049-1 · Cited by 473 · see citing works
Finite-time future singularities in modified Gauss–Bonnet and ℱ(R,G) gravity and singularity avoidance
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 · see citing works
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 · see citing works
“Hubble Space Telescope pilot programs in the z > 1 regime are in progress (Riess et al. 2007; Barbary et al. 2006).”
Self-citation
The Dark Energy Survey: Cosmology Results with ∼1500 New High-redshift Type Ia Supernovae Using the Full 5 yr Data Set
Acevedo, 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 · see citing works
Self-citation
CARNEGIE 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 · see citing works
“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.”
Method
SNLS3: CONSTRAINTS ON DARK ENERGY COMBINING THE SUPERNOVA LEGACY SURVEY THREE-YEAR DATA WITH OTHER PROBES
Sullivan, 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 · see citing works
“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…”
BackgroundInfluential
The 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 · see citing works
“We also use the HST -discovered sample of Riess et al. (2004) and Riess et al. (2007), hereafter the R07 sample.”
Method
UV CONTINUUM SLOPE AND DUST OBSCURATION FROMz∼ 6 TOz∼ 2: THE STAR FORMATION RATE DENSITY AT HIGH REDSHIFT
Bouwens, 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 · see citing works
“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).”
Method
Quintom Cosmology: theoretical implications and observationsPreprint
Cai, Y.-F., Saridakis, E. N., & Setare, M. R. (2016) · Cited by 413 · see citing works
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 · see citing works
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 · see citing works
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 · see citing works
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 384 · see citing works
“In more recent years, distant SNe with redshifts up to z ∼ 1.7 have been observed by the Hubble space telescope (HST) [17, 18].”
BackgroundInfluential
Thermodynamics 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 379 · see citing works
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 · see citing works
“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-citation
Evidence 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 · see citing works
Nonlocal Cosmology
Deser, S., & Woodard, R. P. (2007) · Physical Review Letters · doi:10.1103/physrevlett.99.111301 · Cited by 425 · see citing works
“PACS numbers: 95.36.+x, 98.80.”
Influential
The 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 352 · see citing works
“…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.…”
Background
THE 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 · see citing works
“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-citation
Berkeley Supernova Ia Program - I. Observations, data reduction and spectroscopic sample of 582 low-redshift Type Ia supernovae
Silverman, 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 347 · see citing works
“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-citation
Dark 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 · see citing works
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 · see citing works
“⋆ 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).”
Background
The 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 · see citing works
“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-citation
A 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 · see citing works
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 · see citing works
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 · see citing works
“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-citation
z∼ 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 · see citing works
“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.”
BackgroundInfluential
Cosmography of f(R) gravity
Capozzıello, 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 281 · see citing works
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 259 · see citing works
CLUMPY GALAXIES IN CANDELS. I. THE DEFINITION OF UV CLUMPS AND THE FRACTION OF CLUMPY GALAXIES AT 0.5 < z < 3
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 · see citing works
“…(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-citation
From 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 253 · see citing works
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 251 · see citing works
Type Ia Supernova Distances at Redshift >1.5 from the Hubble Space Telescope Multi-cycle Treasury Programs: The Early Expansion Rate
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 · see citing works
“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-citation
Observational 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 · see citing works
VERY BLUE UV-CONTINUUM SLOPE β OF LOW LUMINOSITY z ∼ 7 GALAXIES FROM WFC3/IR: EVIDENCE FOR EXTREMELY LOW METALLICITIES?
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 · see citing works
“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).”
BackgroundInfluential
The WiggleZ Dark Energy Survey: testing the cosmological model with baryon acoustic oscillations at z= 0.6
Blake, 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 · see citing works
“…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…”
Method
RESULTS OF THE LICK OBSERVATORY SUPERNOVA SEARCH FOLLOW-UP PHOTOMETRY PROGRAM: BVRI LIGHT CURVES OF 165 TYPE Ia SUPERNOVAE
Ganeshalingam, 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 · see citing works
“…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-citation
THEORETICAL MODELS OF DARK ENERGY
Yoo, J., & Watanabe, Y. (2012) · International Journal of Modern Physics D · doi:10.1142/s0218271812300029 · Cited by 232 · see citing works
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 · see citing works
“…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-citation
Constraints on holographic dark energy from the latest supernovae, galaxy clustering, and cosmic microwave background anisotropy observations
Zhang, 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 232 · see citing works
“[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.”
BackgroundMethodInfluential
Cluster 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 · see citing works
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 226 · see citing works
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 · see citing works
“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-citation
CfA4: 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 · see citing works
“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-citation
Confronting 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 · see citing works
Untitled work
(2018) · doi:10.1103/physrevd.97.103503 · Cited by 233 · see citing works
Thawing quintessence with a nearly flat potential
Scherrer, R., & Sen, A. A. (2007) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.77.083515 · Cited by 175 · see citing works
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 · see citing works
“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.”
ResultInfluential
Cosmography 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 210 · see citing works

NEW HUBBLE SPACE TELESCOPE DISCOVERIES OF TYPE Ia SUPERNOVAE AT z 1: NARROWING CONSTRAINTS ON THE EARLY BEHAVIOR OF DARK ENERGY1
(2006) · Cited by 51 · see citing works
Type Ia Supernova Discoveries at z > 1 from the Hubble Space Telescope : Evidence for Past Deceleration and Constraints on Dark Energy Evolution
Riess, 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 · see citing works
Self-citation
New hubble space telescope discoveries of type ia supernovae at z > 1: Narrowing constraints on the early behavior of dark energy. Available at arXiv:astro-ph/0611572Preprint
Riess, A. G., Strolger, L.-G., Ferguson, H. C., Mobasher, B., Gold, B., Challis, P., Jha, S. W., Li, W., Tonry, J. L., Foley, R., et al. (2006)
Self-citation
Confirming Cosmic Acceleration in the Decade that Followed from SNe Ia at z > 1
Riess, A. G. (2016) · Springer eBooks · doi:10.1007/978-3-319-20794-0_105-1 · Cited by 2 · see citing works
Self-citation
TYPE Ia SUPERNOVA DISCOVERIES AT Z> 1 FROM THE HUBBLE SPACE TELESCOPE: EVIDENCE FOR PAST DECELERATION AND CONSTRAINTS ON DARK ENERGY EVOLUTION1
(2004)

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: Riess, Adam G.
Ferguson, Henry C.
Mobasher, Bahram
Filippenko, Alexei V.
Jha, Saurabh
Li, Weidong
Tonry, John
Foley, Ryan
Kirshner, Robert P.
Dickinson, Mark
Eisenstein, Daniel
Stern, Daniel
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
DOI: 10.1086/510378
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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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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