The DOI matches its Crossref record; 87 of the 87 references it cites were found in a registry or an index.
Measurements of Ω and Λ from 42 High‐Redshift Supernovae
Open accessAbstract
We report measurements of the mass density, Ω M , and cosmological-constant energy density, Ω Λ , of the universe based on the analysis of 42 type Ia supernovae discovered by the Supernova Cosmology Project. The magnitude-redshift data for these supernovae, at redshifts between 0.18 and 0.83, are fitted jointly with a set of supernovae from the Calán/Tololo Supernova Survey, at redshifts below 0.1, to yield values for the cosmological parameters. All supernova peak magnitudes are standardized using a SN Ia light-curve width-luminosity relation. The measurement yields a joint probability distribution of the cosmological parameters that is approximated by the relation 0.8Ω M -0.6Ω Λ ≈-0.2±0.1 in the region of interest (Ω M ≲1.5). For a flat (Ω M +Ω Λ =1) cosmology we find Ω M flat =0.28 +0.09 -0.08 (1 σ statistical) +0.05 -0.04 (identified systematics). The data are strongly inconsistent with a Λ=0 flat cosmology, the simplest inflationary universe model. An open, Λ=0 cosmology also does not fit the data well: the data indicate that the cosmological constant is nonzero and positive, with a confidence of P (Λ>0)=99%, including the identified systematic uncertainties. The best-fit age of the universe relative to the Hubble time is t 0 flat =14.9 +1.4 -1.1 (0.63/ h ) Gyr for a flat cosmology. The size of our sample allows us to perform a variety of statistical tests to check for possible systematic errors and biases. We find no significant differences in either the host reddening distribution or Malmquist bias between the low-redshift Calán/Tololo sample and our high-redshift sample. Excluding those few supernovae that are outliers in color excess or fit residual does not significantly change the results. The conclusions are also robust whether or not a width-luminosity relation is used to standardize the supernova peak magnitudes. We discuss and constrain, where possible, hypothetical alternatives to a cosmological constant.
Overview
The claims and statistics of this paper haven’t been checked yet.
Run the check — free, no account needed. It reads the open-access text and checks the sources it cites.
Integrity signals
Registry
Cites
Statistics
Verification
Claims the paper makes
The claims and statistics of this paper haven’t been checked yet.
Run the check — free, no account needed. It reads the open-access text and checks the sources it cites.
Claims other papers make about this one
Each is checked against this paper’s own text: does it say what the citing paper says it does?
The source backs part of the claim, not all of it — or backs it for a different population, condition or comparison.
In the citing paper
“the dark energy (DE) [6,7] component, introduced to explain the current stage of accelerated expansion, in the standard model is the cosmological constant term Λ, without any strong physical basis.”
From Challenges of the Standard Cosmological Model (2022) · cites this paper as [7]
Experimental — accuracy not yet measuredThe cited source says what the claim attributes to it.
In the citing paper
“Two decades ago, two independent groups using supernova measurements found that the universe’s expansion is speeding up rather than slowing down (Riess et al. 1998; Perlmutter et al. 1999).”
From Testing general relativity in cosmology (2019) · cites this paper as Perlmutter et al. 1999
The cited source says what the claim attributes to it.
In the citing paper
“One of the first compelling evidences for cosmic acceleration came from Supernovae type Ia (SN Ia) observations (Riess et al. 1998; Perlmutter et al. 1999).”
From Testing general relativity in cosmology (2019) · cites this paper as Perlmutter et al. 1999
The cited source says what the claim attributes to it.
In the citing paper
“In the presence of a small positive vacuum energy (such as seems to exist in our universe [16, 17, 18]), systems will tend to initially empty out to an approximate de Sitter vacuum.”
From Spontaneous inflation and the origin of the arrow of time (2004) · cites this paper as [17]
The cited source says what the claim attributes to it.
In the citing paper
“A mechanism for such an instability may be provided by the small positive cosmological constant that has apparently been discovered [16, 17, 18].”
From Spontaneous inflation and the origin of the arrow of time (2004) · cites this paper as [17]
In the citing paper
“SNe Ia provided the fi rst robust evidence that the expansion of the universe is accelerating”
From LSST: From Science Drivers to Reference Design and Anticipated Data Products (2019) · cites this paper as Perlmutter et al. 1999
Self-check
Percentages, sums and reported differences re-computed from the paper’s own numbers.
The self-check needs the paper’s full text.
Citations
Cites
1 retracted
Erratum: Discovery of a supernova explosion at half the age of the Universe
Perlmutter, S., Aldering, G., Valle, M. D., Deustua, S., Ellis, R. S., Fabbro, S., Fruchter, A. S., Goldhaber, G., Goobar, A., Groom, D. E., et al. (1998) · Nature · doi:10.1038/32711 · Cited by 21
Self-citationRetractedObservational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
Riess, A. G., Filippenko, A. V., Challis, P., Clocchiatti, A., Diercks, A., Garnavich, P. M., Gilliland, R. L., Hogan, C. J., Jha, S., Kirshner, R. P., et al. (1998) · The Astronomical Journal · doi:10.1086/300499 · Cited by 19,704
Self-citationSchlegel, D. J., Finkbeiner, D. P., & Davis, M. (1998) · The Astrophysical Journal · doi:10.1086/305772 · Cited by 15,126
The relationship between infrared, optical, and ultraviolet extinction
Cardelli, J. A., Clayton, G. C., & Mathis, J. S. (1989) · The Astrophysical Journal · doi:10.1086/167900 · Cited by 11,794
Cosmological Imprint of an Energy Component with General Equation of State
Caldwell, R. R., Dave, R., & Steinhardt, P. J. (1998) · Physical Review Letters · doi:10.1103/physrevlett.80.1582 · Cited by 3,697
Unified approach to the classical statistical analysis of small signals
Feldman, G. J., & Cousins, R. D. (1998) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.57.3873 · Cited by 3,123
Quintessence, Cosmic Coincidence, and the Cosmological Constant
Zlatev, I. S., Wang, L.-M., & Steinhardt, P. J. (1999) · Physical Review Letters · doi:10.1103/physrevlett.82.896 · Cited by 2,678
Discovery of a supernova explosion at half the age of the Universe
Perlmutter, S., Aldering, G., Valle, M. D., Deustua, S. E., Ellis, R. S., Fabbro, S., Fruchter, A. S., Goldhaber, G., Groom, D. E., Hook, I., et al. (1998) · Nature · doi:10.1038/34124 · Cited by 2,542
Self-citationThe absolute magnitudes of Type IA supernovae
Phillips, M. M. (1993) · The Astrophysical Journal · doi:10.1086/186970 · Cited by 2,111
The Keck Low-Resolution Imaging Spectrometer
Oke, J. B., Cohen, J., Carr, M., Cromer, J. L., Dingizian, A., Harris, F. H., Labrecque, S., Lucinio, R., Schaal, W., Epps, H. W., et al. (1995) · Publications of the Astronomical Society of the Pacific · doi:10.1086/133562 · Cited by 2,100
Research works printed but not linked: 10
- Carlberg, R. G., etal 1998, in Proc. 33d Recontres de Moriond, Fundamental Parameters in Cosmology, ed. J. Tran Thanh Vang & Y. Giraud-Heraud (Paris: Editions frontieres), in press
- Freedman, W. L., Mould, J. R., Kennicut, R. C. & Madore, B. F. 1998, in IAU Symp. 183, Cosmological Parameters and the Evolution of the Universe, ed. K. Sato (Dordrecht: Kluwer) (astro-ph/9801080) · arXiv
- 10.1086/305129 · DOI
- Kantowski R., 1998, ApJ, 88, 285
- Kayser R., 1996, A&A, 318, 680
- Maddox S. J., 1990, MNRAS, 247, 1P
- Malmquist K. G., 1924, Medd. Lund Astron. Obs. Ser., 64
- Perlmutter S., 1997, BAAS, 29, 1351
- Tammann, G. A. 1979, in ESA/ESO Workshop on Astronomical Uses of the Space Telescope, ed. F. Macchetto, F. Pacini, and M. Tarenghi (Geneva: ESO), 329
- Tripp R., 1998, A&A, 331, 815
Cited by
Sorted by citations
Planck 2018 results: VI. Cosmological parameters
Planck Collaboration, Aghanim, N., Akrami, Y., Ashdown, M., Aumont, J., Baccigalupi, C., Ballardini, M., Banday, A. J., Barreiro, R. B., Bartolo, N., et al. (2020) · Astronomy & Astrophysics · doi:10.1051/0004-6361/201833910 · Cited by 14,258
Spergel, D. N., Verde, L., Peiris, H. V., Komatsu, E., Nolta, M. R., Bennett, C. L., Halpern, M., Hinshaw, G., Jarosik, N., Kogut, A., et al. (2003) · The Astrophysical Journal Supplement Series · doi:10.1086/377226 · Cited by 10,976
Ade, P. A. R., Aghanim, N., Arnaud, M., Ashdown, M., Aumont, J., Baccigalupi, C., Banday, A. J., Barreiro, R. B., Bartlett, J. G., Bartolo, N., et al. (2016) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201525830 · Cited by 10,685
SEVEN-YEAR WILKINSON MICROWAVE ANISOTROPY PROBE(WMAP) OBSERVATIONS: COSMOLOGICAL INTERPRETATION
Komatsu, E., Smith, K. M., Dunkley, J., Bennett, C. L., Gold, B., Hinshaw, G., Jarosik, N., Larson, D., Nolta, M. R., Page, L., et al. (2011) · The Astrophysical Journal Supplement Series · doi:10.1088/0067-0049/192/2/18 · Cited by 8,802
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
Three‐Year Wilkinson Microwave Anisotropy Probe ( WMAP ) Observations: Implications for Cosmology
Spergel, D. N., Bean, R., Dore, O., Nolta, M. R., Bennett, C. L., Dunkley, J., Hinshaw, G., Jarosik, N., Komatsu, E., Page, L., et al. (2007) · The Astrophysical Journal Supplement Series · doi:10.1086/513700 · Cited by 6,778
Copeland, E. J., Sami, M., & Tsujikawa, S. (2006) · International Journal of Modern Physics D · doi:10.1142/s021827180600942x · Cited by 6,733
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
Ade, P. A. R., Aghanim, N., Arnaud, M., Ashdown, M., Aumont, J., Baccigalupi, C., Banday, A. J., Barreiro, R. B., Bartlett, J. G., Bartolo, N., et al. (2016) · Research at the University of Copenhagen (University of Copenhagen) · doi:10.17863/cam.32861 · Cited by 5,299
The cosmological constant and dark energy
Peebles, P. J. E., & Ratra, B. (2003) · Reviews of Modern Physics · doi:10.1103/revmodphys.75.559 · Cited by 5,624
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
Simulations of the formation, evolution and clustering of galaxies and quasars
Springel, V., White, S. D. M., Jenkins, A. R., Frenk, C. S., Yoshida, N., Gao, L., Navarro, J. F., Thacker, R. J., Croton, D., Helly, J. C., et al. (2005) · Nature · doi:10.1038/nature03597 · Cited by 5,060
Eisenstein, D. J., Zehavi, I., Hogg, D. W., Scoccimarro, R., Blanton, M. R., Nichol, R. C., Scranton, R., Seo, H., Tegmark, M., Zheng, Z., et al. (2005) · The Astrophysical Journal · doi:10.1086/466512 · Cited by 4,641
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
Self-citationModified gravity and cosmology
Clifton, T., Ferreira, P. G., Padilla, A., & Skordis, C. (2012) · Physics Reports · doi:10.1016/j.physrep.2012.01.001 · Cited by 4,575
Felice, A. D., & Tsujikawa, S. (2010) · Living Reviews in Relativity · doi:10.12942/lrr-2010-3 · Cited by 4,327
Croton, D. J., Springel, V., White, S. D. M., Lucia, G. D., Frenk, C. S., Gao, L., Jenkins, A., Kauffmann, G., Navarro, J. F., & Yoshida, N. (2005) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2005.09675.x · Cited by 3,686
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
Self-citationFinal Results from the Hubble Space Telescope Key Project to Measure the Hubble Constant
Freedman, W. L., Madore, B. F., Gibson, B. K., Ferrarese, L., Kelson, D. D., Sakai, S., Mould, J. R., Robert C. Kennicutt, Jr., Ford, H. C., Graham, J. A., et al. (2001) · The Astrophysical Journal · doi:10.1086/320638 · Cited by 3,543
Cosmological parameters from CMB and other data: A Monte Carlo approach
Lewis, A., & Bridle, S. (2002) · Physical Review D · doi:10.1103/physrevd.66.103511 · Cited by 3,495
Caldwell, R. R. (2002) · Physics Letters B · doi:10.1016/s0370-2693(02)02589-3 · Cited by 3,458
Planck 2018 results. VI. Cosmological parametersPreprint
Planck Collaboration, Aghanim, N., Akrami, Y., Ashdown, M., Aumont, J., Baccigalupi, C., Ballardini, M., Banday, A. J., Barreiro, R. B., Bartolo, N., et al. (2018) · arXiv (Cornell University) · doi:10.48550/arxiv.1807.06209 · Cited by 3,364
de Sitter vacua in string theory
Shamit Kachru, A., Каллош, Р., Linde, A. D., & Trivedi, S. P. (2003) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.68.046005 · Cited by 3,869
Capozzıello, S., & Laurentis, M. D. (2011) · Physics Reports · doi:10.1016/j.physrep.2011.09.003 · Cited by 3,560
Alam, S., Ata, M., Bailey, S., Beutler, F., Bizyaev, D., Blazek, J. A., Bolton, A. S., Brownstein, J. R., Burden, A., Chuang, C.-H., et al. (2017) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stx721 · Cited by 3,056
Harko, T., Lobo, F. S. N., Nojiri, S., & Odintsov, S. D. (2011) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.84.024020 · Cited by 2,888
THE CASE FOR A POSITIVE COSMOLOGICAL Λ-TERM
SAHNI, V., & STAROBINSKY, A. (2000) · International Journal of Modern Physics D · doi:10.1142/s0218271800000542 · Cited by 2,767
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
The Universe in a Helium Droplet
Volovik, G. E. (2009) · doi:10.1093/acprof:oso/9780199564842.001.0001 · Cited by 2,632
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
Carroll, S. M. (2001) · Living Reviews in Relativity · doi:10.12942/lrr-2001-1 · Cited by 2,650
Eisenstein, D. J., Zehavi, I., Hogg, D. W., Scoccimarro, R., Blanton, M. R., Nichol, R. C., Scranton, R., Seo, H., Tegmark, M., Zheng, Z., et al. (2005) · Cited by 2,568
A flat Universe from high-resolution maps of the cosmic microwave background radiation
de Bernardis, P., Ade, P. A. R., Bock, J. J., Bond, J. R., Borrill, J., Boscaleri, A., Coble, K., Crill, B. P., de Gasperis, G., Farese, P. C., et al. (2000) · Nature · doi:10.1038/35010035 · Cited by 2,614
Astier, P., Guy, J., Regnault, N., Pain, R., Aubourg, É., Balam, D. D., Basa, S., Carlberg, R. G., Fabbro, S., Fouchez, D., et al. (2006) · Astronomy and Astrophysics · doi:10.1051/0004-6361:20054185 · Cited by 2,438
Self-citationBamba, K., Capozzıello, S., Nojiri, S., & Odintsov, S. D. (2012) · Astrophysics and Space Science · doi:10.1007/s10509-012-1181-8 · Cited by 2,502
Is cosmic speed-up due to new gravitational physics?
Carroll, S. M., Duvvuri, V., Trodden, M., & Turner, M. S. (2004) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.70.043528 · Cited by 2,438
Vogelsberger, M., Genel, S., Springel, V., Torrey, P., Sijacki, D., Xu, D., Snyder, G., Nelson, D., & Hernquist, L. (2014) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stu1536 · Cited by 2,251
Eisenstein, D. J., Weinberg, D. H., Agol, E., Aihara, H., Prieto, C. A., Anderson, S. F., Arns, J. A., Aubourg, É., Bailey, S., Balbinot, E., et al. (2011) · The Astronomical Journal · doi:10.1088/0004-6256/142/3/72 · Cited by 2,143
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
Self-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
Self-citationPhantom Energy: Dark Energy with w < − 1 Causes a Cosmic Doomsday
Caldwell, R. R., Kamionkowski, M., & Weinberg, N. N. (2003) · Physical Review Letters · doi:10.1103/physrevlett.91.071301 · Cited by 2,258
Nojiri, S., & Odintsov, S. D. (2003) · Physical Review D · doi:10.1103/physrevd.68.123512 · Cited by 2,183
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 2,100
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 1,910
Self-citationA model of holographic dark energy
Li, M. (2004) · Physics Letters B · doi:10.1016/j.physletb.2004.10.014 · Cited by 1,893
Hopkins, P. F., Hernquist, L., Cox, T. J., Matteo, T. D., Robertson, B. E., & Springel, V. (2006) · The Astrophysical Journal Supplement Series · doi:10.1086/499298 · Cited by 1,872
Galileon as a local modification of gravity
Nicolis, A., Rattazzi, R., & Trincherini, E. (2009) · Physical Review D · doi:10.1103/physrevd.79.064036 · Cited by 1,863
Anderson, L., Aubourg, É., Bailey, S., Beutler, F., Bhardwaj, V., Blanton, M. R., Bolton, A. S., Brinkmann, J., Brownstein, J. R., Burden, A., et al. (2014) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stu523 · Cited by 1,908
Amendola, L. (2000) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.62.043511 · Cited by 1,841
Cosmological Constant - the Weight of the VacuumPreprint
Padmanabhan, Τ. (2002) · Cited by 2,196
The clustering of the SDSS DR7 main Galaxy sample – I. A 4 per cent distance measure at z=0.15
Ross, A. J., Samushia, L., Howlett, C., Percival, W. J., Burden, A., & Manera, M. (2015) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stv154 · Cited by 1,745
Riess, A. G., Strolger, L., Casertano, S., Ferguson, H. C., Mobasher, B., Gold, B., Challis, P. J., Filippenko, A. V., Jha, S., Li, W., et al. (2007) · The Astrophysical Journal · doi:10.1086/510378 · Cited by 1,758
Self-citationCosmological Results from High‐zSupernovae
Tonry, J. L., Schmidt, B. P., Barris, B. J., Candia, P., Challis, P., Clocchiatti, A., Coil, A. L., Filippenko, A. V., Garnavich, P., Hogan, C. J., et al. (2003) · The Astrophysical Journal · doi:10.1086/376865 · Cited by 1,750
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
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 1,799
Self-citationBousso, R. (2002) · Reviews of Modern Physics · doi:10.1103/revmodphys.74.825 · Cited by 1,741
Aghanim, N., Akrami, Y., Arroja, F. M. A., Ashdown, M., Aumont, J., Baccigalupi, C., Ballardini, M., Banday, A. J., Barreiro, R. B., Bartolo, N., et al. (2019) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201833880 · Cited by 2,386
Knop, R. A., Aldering, G., Amanullah, R., Astier, P., Blanc, G., Burns, M. S., Conley, A., Deustua, S. E., Doi, M., Ellis, R. S., et al. (2003) · The Astrophysical Journal · doi:10.1086/378560 · Cited by 1,639
Self-citationCroton, D., Springel, V., White, S. D. M., Lucia, G. D., Frenk, C. S., Gao, L., Jenkins, A. R., Kauffmann, G., Navarro, J. F., & Yoshida, N. (2006) · Max Planck Digital Library · doi:10.25916/sut.26253068.v1 · Cited by 1,611
Sloan Digital Sky Survey IV: Mapping the Milky Way, Nearby Galaxies, and the Distant Universe
Blanton, M. R., Bershady, M. A., Abolfathi, B., Albareti, F. D., Prieto, C. A., Almeida, A., Alonso-García, J., Anders, F., Anderson, S. F., Andrews, B. H., et al. (2017) · The Astronomical Journal · doi:10.3847/1538-3881/aa7567 · Cited by 1,588
Search for new physics with atoms and molecules
Safronova, M. S., Budker, D., DeMille, D. P., Kimball, D. F. J., Derevianko, A., & Clark, C. W. (2018) · Reviews of Modern Physics · doi:10.1103/revmodphys.90.025008 · Cited by 1,642
A Flat Universe from High-Resolution Maps of the Cosmic Microwave Background \nRadiation
de Bernardis, P., Ade, P. A. R., Bock, J. J., Bond, J. R., Borrill, J., Boscaleri, A., Coble, K., Crill, B. P., de Gasperis, G., Farese, P. C., et al. (2000) · eScholarship (California Digital Library) · Cited by 1,562
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
Self-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
Self-citationf ( T ) teleparallel gravity and cosmology
Cai, Y.-F., Capozzıello, S., Laurentis, M. D., & Saridakis, E. N. (2016) · Reports on Progress in Physics · doi:10.1088/0034-4885/79/10/106901 · Cited by 1,647
Statefinder—A new geometrical diagnostic of dark energy
Varun Sahni, B., Saini, T. D., Starobinsky, A. A., & Ujjaini Alam, A. (2003) · Journal of Experimental and Theoretical Physics Letters · doi:10.1134/1.1574831 · Cited by 1,564
Dark Matter Candidates from Particle Physics and Methods of Detection
Feng, J. L. (2010) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev-astro-082708-101659 · Cited by 1,475
Khoury, J., & Weltman, A. (2004) · Physical Review D · doi:10.1103/physrevd.69.044026 · Cited by 1,634
Kinetically driven quintessence
Chiba, T., Okabe, T., & Yamaguchi, M. (2000) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.62.023511 · Cited by 1,434
Iwamoto, K., Brachwitz, F., Nomoto, K., Kishimoto, N., Umeda, H., Hix, W. R., & Thielemann, F. ‐. (1999) · The Astrophysical Journal Supplement Series · doi:10.1086/313278 · Cited by 1,419
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 1,520
In the beginning: the first sources of light and the reionization of the universe
Barkana, R., & Loeb, A. (2001) · Physics Reports · doi:10.1016/s0370-1573(01)00019-9 · Cited by 1,470
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
Self-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
Self-citationAlam, 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
Recent progress and new challenges in isospin physics with heavy-ion reactions
Li, B.-A., Chen, L.-W., & Ko, C. M. (2008) · Physics Reports · doi:10.1016/j.physrep.2008.04.005 · Cited by 1,340
Dark energy constraints from the cosmic age and supernova
Feng, B., Wang, X.-L., & Zhang, X.-M. (2004) · Physics Letters B · doi:10.1016/j.physletb.2004.12.071 · Cited by 1,182
Extended Theories of GravityPreprint
Capozzıello, S., Lobod, C. F. S. N., P, F. J., & Cinthia, A. E. G. V. (2010) · Cited by 1,672
Science case for the Einstein telescope
Maggiore, M., Broeck, C. V. D., Bartolo, N., Belgacem, E., Bertacca, D., Bizouard, M. A., Branchesi, M., Clesse, S., Foffa, S., García-Bellido, J., et al. (2020) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2020/03/050 · Cited by 1,257
Can the dark energy equation-of-state parameterwbe less than −1?
Carroll, S. M., Hoffman, M. B., & Trodden, M. (2003) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.68.023509 · Cited by 1,347
Bertone, G., & Hooper, D. (2018) · Reviews of Modern Physics · doi:10.1103/revmodphys.90.045002 · Cited by 1,241
Cosmic chronometers: constraining the equation of state of dark energy. I: H(z) measurements
Stern, D., Jimenez, R., Verde, L., Kamionkowski, M., & Stanford, S. A. (2010) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2010/02/008 · Cited by 1,232
Dark Energy Survey year 1 results: Cosmological constraints from galaxy clustering and weak lensing
Abbott, T. M. C., Abdalla, F. B., Alarcon, A., Aleksić, J., Allam, S., Allen, S., Amara, A., Annis, J., Asorey, J., Avila, S., et al. (2018) · Physical Review D · doi:10.1103/physrevd.98.043526 · Cited by 1,213
Self-citationType Ia Supernova Explosion Models
Hillebrandt, W., & Niemeyer, J. C. (2000) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev.astro.38.1.191 · Cited by 1,219
Dark torsion as the cosmic speed-up
Bengochea, G. R., & Ferraro, R. (2009) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.79.124019 · Cited by 1,244
DESI 2024 VI: cosmological constraints from the measurements of baryon acoustic oscillations
Adame, A. G., Aguilar, J., Ahlen, S. P., Alam, S., Alexander, D. M., Alvarez, M. A., Alves, O., Anand, A., Andrade, U., Armengaud, E., et al. (2025) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2025/02/021 · Cited by 1,156
The Palomar Transient Factory: System Overview, Performance, and First Results
Law, N. M., Kulkarni, S. R., Dekany, R. G., Ofek, E. O., Quimby, R. M., Nugent, P. E., Surace, J., Grillmair, C. C., Bloom, J. S., Kasliwal, M. M., et al. (2009) · Publications of the Astronomical Society of the Pacific · doi:10.1086/648598 · Cited by 1,141
Self-citationMoresco, 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
Dark Energy Survey Year 3 results: Cosmological constraints from galaxy clustering and weak lensing
Abbott, T. M. C., Aguena, M., Alarcon, A., Allam, S., Alves, O., Amon, A., Andrade-Oliveira, F., Annis, J., Avila, S., Bacon, D., et al. (2022) · Physical Review D · doi:10.1103/physrevd.105.023520 · Cited by 1,124
Self-citationCappellari, M., Emsellem, É., Krajnović, D., McDermid, R. M., Scott, N., Kleijn, G. A. V., Young, L. M., Alatalo, K., Bacon, R. M., Blitz, L., et al. (2011) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2010.18174.x · Cited by 1,128
Beyond the cosmological standard model
Joyce, A., Jain, B., Khoury, J., & Trodden, M. (2015) · Physics Reports · doi:10.1016/j.physrep.2014.12.002 · Cited by 1,231
Theoretical aspects of massive gravity
Hinterbichler, K. (2012) · Reviews of Modern Physics · doi:10.1103/revmodphys.84.671 · Cited by 1,088
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
The 6dF Galaxy Survey: final redshift release (DR3) and southern large-scale structures
Jones, D. H. P., Read, M., Saunders, W., Colless, M., Jarrett, T. H., Parker, Q. A., Fairall, A. P., Mauch, T., Sadler, E. M., Watson, F. G., et al. (2009) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2009.15338.x · Cited by 1,052
Thermodynamical aspects of gravity: new insights
Padmanabhan, Τ. (2010) · Reports on Progress in Physics · doi:10.1088/0034-4885/73/4/046901 · Cited by 1,188
Non-conventional cosmology from a brane universe
Binétruy, P., Deffayet, C., & Langlois, D. (2000) · Nuclear Physics B · doi:10.1016/s0550-3213(99)00696-3 · Cited by 1,036
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
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
Self-citationRaising the bar: new constraints on the Hubble parameter with cosmic chronometers at z ∼ 2
Moresco, M. (2015) · Monthly Notices of the Royal Astronomical Society Letters · doi:10.1093/mnrasl/slv037 · Cited by 1,011
Constraining Cosmological Parameters Based on Relative Galaxy Ages
Jiménez, R., & Loeb, A. (2002) · The Astrophysical Journal · doi:10.1086/340549 · Cited by 986
Metadata
- Authors
- Perlmutter, S., Aldering, G., Goldhaber, G., Knop, R. A., Nugent, P., Castro, P. G., Deustua, S., Fabbro, S., Goobar, A., Groom, D. E., Hook, I. M., Kim, A. G., Kim, M. Y., Lee, J. C., Nunes, N. J., Pain, R., Pennypacker, C. R., Quimby, R., Lidman, C., Ellis, R. S., Irwin, M., McMahon, R. G., Ruiz‐Lapuente, P., Walton, N., Schaefer, B., Boyle, B. J., Filippenko, A. V., Matheson, T., Fruchter, A. S., Panagia, N., Newberg, H. J. M., Couch, W. J., & Project, T. S. C.
- Affiliations
- Lawrence Berkeley National Laboratory (US)
- Centre National de la Recherche Scientifique (FR)
- European Southern Observatory (DE)
- University of Cambridge (GB)
- Isaac Newton Group (ES)
- Yale University (US)
- Australian Astronomical Observatory (AU)
- University of California, Berkeley (US)
- Space Telescope Science Institute (US)
- Fermi National Accelerator Laboratory (US)
- UNSW Sydney (AU)
- ORCID
- Perlmutter, S.
- Aldering, G.
- Goldhaber, G.
- Knop, R. A.
- Nugent, P.
- Castro, P. G.
- Deustua, S.
- Fabbro, S.
- Goobar, A.
- Groom, D. E.
- Hook, I. M.
- Kim, A. G.
- Lee, J. C.
- Nunes, N. J.
- Pain, R.
- Quimby, R.
- Lidman, C.
- Ellis, R. S.
- Irwin, M.
- McMahon, R. G.
- Walton, N.
- Schaefer, B.
- Filippenko, A. V.
- Matheson, T.
- Fruchter, A. S.
- Panagia, N.
- Newberg, H. J. M.
- Couch, W. J.
- Venue
- The Astrophysical Journal
- Publisher
- American Astronomical Society
- Published
- 1999-06
- Volume
- 517
- Issue
- 2
- Pages
- 565-586
- ISSN
- 0004-637X (ISSN-L)
- 1538-4357
- OpenAlex
- W1853767801
- Cited by
- 18,062
- References
- 83
- Citations by year
- 2026: 700 · 2025: 976 · 2024: 989 · 2023: 863 · 2022: 759 · 2021: 778 · 2020: 744 · 2019: 784 · 2018: 718 · 2017: 725 · 2016: 819 · 2015: 741 · 2014: 757 · 2013: 894 · 2012: 822
- FWCI
- 271.14
- Type
- journal article
- Language
- en
- Open access
- bronze
- doi.org
- Locations
- The Astrophysical Journal (publishedVersion)
- arXiv (Cornell University) (submittedVersion)
- OSTI OAI (U.S. Department of Energy Office of Scientific and Technical Information) (submittedVersion)
- Civil War Book Review (submittedVersion)
- HAL (submittedVersion)
- eScholarship (California Digital Library) (submittedVersion)
- ANU Open Research (Australian National University) (submittedVersion)
- Funders
- National Science Foundation (9417213)
- France-Berkeley Fund
- 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, cosmological constant, matter density parameter, high-redshift supernovae, flat universe, age of the universe, Malmquist bias, systematic errors, inflationary universe
About these checks
Registry, retraction, Cites and statistics results are computed, not judged, with one exception: a printed reference that no index lists is read once by a model before it counts as a citation error. Claims are extracted by a model and kept only when their quote appears verbatim in the text; each cited source is then checked, with a model’s help, for whether it says what the claim relies on. Those verdicts can be wrong — read the claim’s quote and the cited source before relying on one.
Statistics and arithmetic are recomputed, not judged.
Confidence bands are shown only for fields calibrated on our annotated test set. None is calibrated yet, so no band is shown.
What counts as a claim ›How we measure confidence ›How we check this ›
Are you an author, or do you see a problem with this page? Request a review
