Fig. 1 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. 1.

Light curves and images from the PC CCD on WFPC2 for the HST SNe reported in this paper. The left‐hand column shows the R‐band light curves (including F675W HST data), and the middle column shows I‐band light curves (including F814W HST data). Open circles represent ground‐based data points, and filled circles represent WFPC2 data points. Note that there are correlated errors between all of the ground‐based points for each SN in these figures, as a single ground‐based zero point was used to scale each of them together with the HST photometry. The right‐hand column shows ﹩6^{\prime \prime }\times 6^{\prime \prime }﹩ images, summed from all HST images of the SN in the indicated filter.

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