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E. Smith (Vanderbilt), G. Aldering (LBNL), R. Amanullah (Stockholm), P. Antilogus, P. Astier (LPNHE Paris), G. Blanc (Padova), M.S. Burns (Colorado Col.), A. Conley, S.E. Deustua (LBNL), M. Doi (Tokyo), R. Ellis (CalTech), S. Fabbro (Lisbon), V. Fadeyev (LBNL), G. Folatelli (Stockholm), A.S. Fruchter (STScI), G. Garavini (Stockholm), R. Gibbons, G. Goldhaber (LBNL), A. Goobar (Stockholm), D. Groom (LBNL), D. Hardin (LPNHE Paris), I. Hook (Oxford), D.A. Howell (Toronto), M. Irwin (IOA Cambridge), D. Kasen, A.G. Kim (LBNL), R.A. Knop (Vanderbilt), B.C. Lee (LBNL), C. Lidman (ESO), R. McMahon (IOA Cambridge), J. Mendez (ING), S. Nobili (Stockholm), P.E. Nugent (LBNL), R. Pain (LPNHE Paris), N. Panagia (STScI), C.R. Pennypacker, S. Perlmutter, V. Prasad (LBNL), R. Quimby (Texas), J. Raux (LPNHE Paris), N. Regnault (LBNL), P. Ruiz-Lapuente (Barcelona), G. Sainton (LPNHE Paris), B. Schaefer (Texas), K. Schahmaneche (LPNHE Paris), A.L. Spadafora (LBNL), V. Stanishev (Stockholm), M. Sullivan (Toronto), N. Walton (IOA Cambridge), L. Wang, W.M. Wood-Vasey, N. Yasuda (LBNL), Supernova Cosmology Project Collaboration
We present the spectra of eleven supernovae with redshifts in the range of 0.35 < z < 0.86. These spectra were obtained at the Keck observatory and the European Southern Observatory between December 1997 and May 2000. These supernovae were discovered by the Supernova Cosmology Project; lightcurves and cosmological results appear in ``New Constraints on \OmegaM, \Omega\Lambda, and w from an Independent Set of Eleven High-Redshift Supernovae Observed with HST" (Knop, et. al, 2003.). Redshifts were obtained through the use of both galaxy lines and supernovae lines, and supernova type was determined through spectrum matching.
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Bulletin of the American Astronomical Society, 35#5
© 2003. The American Astronomical Soceity.