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Cited by 18,062Cosmology and Gravitation TheoriesGamma-ray bursts and supernovaeGalaxies: Formation, Evolution, Phenomena

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

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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, The Supernova Cosmology·1999·The Astrophysical Journal
DOI 10.1086/307221
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Abstract

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.

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  1. 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
  2. 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
  3. 10.1086/305129 · DOI
  4. Kantowski R., 1998, ApJ, 88, 285
  5. Kayser R., 1996, A&A, 318, 680
  6. Maddox S. J., 1990, MNRAS, 247, 1P
  7. Malmquist K. G., 1924, Medd. Lund Astron. Obs. Ser., 64
  8. Perlmutter S., 1997, BAAS, 29, 1351
  9. 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
  10. Tripp R., 1998, A&A, 331, 815

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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
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
DOI
10.1086/307221
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
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

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