Optical Spectroscopy of High-Redshift Supernovae Used in Determination of Cosmological Parameters

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

Optical Spectroscopy of High-Redshift Supernovae Used in Determination of Cosmological Parameters

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

Research School of Astronomy & Astrophysics

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Abstract

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 Ω _M, Ω _Λ, 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.

Original language	English
Pages	45.05
Publication status	Published - 1 Dec 2003

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https://ui.adsabs.harvard.edu/abs/2003AAS...203.4505S

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Smith, E., Aldering, G., Amanullah, R., Antilogus, P., Astier, P., Blanc, G., Burns, M. S., Conley, A., Deustua, S. E., Doi, M., Ellis, R., Fabbro, S., Fadeyev, V., Folatelli, G., Fruchter, A. S., Garavini, G., Gibbons, R., Goldhaber, G., Goobar, A., ... Collaboration, S. C. P. (2003). Optical Spectroscopy of High-Redshift Supernovae Used in Determination of Cosmological Parameters. 45.05. https://ui.adsabs.harvard.edu/abs/2003AAS...203.4505S

@conference{f365d6f252f74b1ca5ca456b62f47e6f,

title = "Optical Spectroscopy of High-Redshift Supernovae Used in Determination of Cosmological Parameters",

abstract = "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 Ω M, Ω Λ , 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.",

author = "E. Smith and G. Aldering and R. Amanullah and P. Antilogus and P. Astier and G. Blanc and Burns, {M. S.} and A. Conley and Deustua, {S. E.} and M. Doi and R. Ellis and S. Fabbro and V. Fadeyev and G. Folatelli and Fruchter, {A. S.} and G. Garavini and R. Gibbons and G. Goldhaber and A. Goobar and D. Groom and D. Hardin and I. Hook and Howell, {D. A.} and M. Irwin and D. Kasen and Kim, {A. G.} and Knop, {R. A.} and Lee, {B. C.} and C. Lidman and R. McMahon and J. Mendez and S. Nobili and Nugent, {P. E.} and R. Pain and N. Panagia and Pennypacker, {C. R.} and S. Perlmutter and V. Prasad and R. Quimby and J. Raux and N. Regnault and P. Ruiz-Lapuente and G. Sainton and B. Schaefer and K. Schahmaneche and Spadafora, {A. L.} and V. Stanishev and M. Sullivan and N. Walton and L. Wang and Wood-Vasey, {W. M.} and N. Yasuda and Collaboration, {Supernova Cosmology Project}",

year = "2003",

month = dec,

day = "1",

language = "English",

pages = "45.05",

}

Smith, E, Aldering, G, Amanullah, R, Antilogus, P, Astier, P, Blanc, G, Burns, MS, Conley, A, Deustua, SE, Doi, M, Ellis, R, Fabbro, S, Fadeyev, V, Folatelli, G, Fruchter, AS, Garavini, G, Gibbons, R, Goldhaber, G, Goobar, A, Groom, D, Hardin, D, Hook, I, Howell, DA, Irwin, M, Kasen, D, Kim, AG, Knop, RA, Lee, BC, Lidman, C, McMahon, R, Mendez, J, Nobili, S, Nugent, PE, Pain, R, Panagia, N, Pennypacker, CR, Perlmutter, S, Prasad, V, Quimby, R, Raux, J, Regnault, N, Ruiz-Lapuente, P, Sainton, G, Schaefer, B, Schahmaneche, K, Spadafora, AL, Stanishev, V, Sullivan, M, Walton, N, Wang, L, Wood-Vasey, WM, Yasuda, N & Collaboration, SCP 2003, 'Optical Spectroscopy of High-Redshift Supernovae Used in Determination of Cosmological Parameters', pp. 45.05. <https://ui.adsabs.harvard.edu/abs/2003AAS...203.4505S>

TY - CONF

T1 - Optical Spectroscopy of High-Redshift Supernovae Used in Determination of Cosmological Parameters

AU - Smith, E.

AU - Aldering, G.

AU - Amanullah, R.

AU - Antilogus, P.

AU - Astier, P.

AU - Blanc, G.

AU - Burns, M. S.

AU - Conley, A.

AU - Deustua, S. E.

AU - Doi, M.

AU - Ellis, R.

AU - Fabbro, S.

AU - Fadeyev, V.

AU - Folatelli, G.

AU - Fruchter, A. S.

AU - Garavini, G.

AU - Gibbons, R.

AU - Goldhaber, G.

AU - Goobar, A.

AU - Groom, D.

AU - Hardin, D.

AU - Hook, I.

AU - Howell, D. A.

AU - Irwin, M.

AU - Kasen, D.

AU - Kim, A. G.

AU - Knop, R. A.

AU - Lee, B. C.

AU - Lidman, C.

AU - McMahon, R.

AU - Mendez, J.

AU - Nobili, S.

AU - Nugent, P. E.

AU - Pain, R.

AU - Panagia, N.

AU - Pennypacker, C. R.

AU - Perlmutter, S.

AU - Prasad, V.

AU - Quimby, R.

AU - Raux, J.

AU - Regnault, N.

AU - Ruiz-Lapuente, P.

AU - Sainton, G.

AU - Schaefer, B.

AU - Schahmaneche, K.

AU - Spadafora, A. L.

AU - Stanishev, V.

AU - Sullivan, M.

AU - Walton, N.

AU - Wang, L.

AU - Wood-Vasey, W. M.

AU - Yasuda, N.

AU - Collaboration, Supernova Cosmology Project

PY - 2003/12/1

Y1 - 2003/12/1

N2 - 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 Ω M, Ω Λ , 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.

AB - 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 Ω M, Ω Λ , 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.

M3 - Paper

SP - 45.05

ER -

Optical Spectroscopy of High-Redshift Supernovae Used in Determination of Cosmological Parameters

Abstract

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