Fig. 4 from New Constraints on ΩM, ΩΛ, and w from an Independent Set of 11 High‐Redshift Supernovae Observed with the Hubble Space Telescope

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New Constraints on Ω_M, Ω_Λ, and w from an Independent Set of 11 High‐Redshift Supernovae Observed with the Hubble Space Telescope

Authors: R. A. Knop, G. Aldering, R. Amanullah, P. Astier, G. Blanc, M. S. Burns, A. Conley, S. E. Deustua, M. Doi, R. Ellis, S. Fabbro, G. Folatelli, A. S. Fruchter, G. Garavini, S. Garmond, K. Garton, R. Gibbons, G. Goldhaber, A. Goobar, D. E. Groom, D. Hardin, I. Hook, D. A. Howell, A. G. Kim, B. C. Lee, C. Lidman, J. Mendez, S. Nobili, P. E. Nugent, R. Pain, N. Panagia, C. R. Pennypacker, S. Perlmutter, R. Quimby, J. Raux, N. Regnault, P. Ruiz-Lapuente, G. Sainton, B. Schaefer, K. Schahmaneche, E. Smith, A. L. Spadafora, V. Stanishev, M. Sullivan, N. A. Walton, L. Wang, W. M. Wood-Vasey, N. Yasuda, and (The Supernova Cosmology Project)

Knop et al. 2003 The Astrophysical Journal 598 102.

Provider: AAS Journals

Caption: Fig. 4.

Hubble diagram of effective K‐ and stretch‐corrected m_B vs. redshift for the SNe in the primary low‐extinction subset. Filled circles represent the HST SNe of this paper. Inner error bars show just the measurement uncertainties; outer error bars include 0.17 mag of intrinsic dispersion. The solid line is the best‐fit flat‐universe cosmology from the low‐extinction subset; the dashed and dotted lines represent the indicated cosmologies.

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