Interpretation of High-z SN Spectra

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

Interpretation of High-z SN Spectra

P. Nugent, G. Aldering, R. Amanullah, P. Antilogus, P. Astier, C. Balland, G. Blanc, M. S. Burns, A. Conley, S. Deustua, R. Ellis, S. Fabbro, G. Folatelli, A. Fruchter, G. Garavini, R. Gibbons, G. Goldhaber, A. Goobar, D. E. Groom, D. HardinI. M. Hook, D. A. Howell, M. Irwin, D. Kasen, A. Kim, R. A. Knop, J. -M. Levy, C. Lidman, R. McMahon, M. Mouchet, S. Nobili, R. Pain, N. Panagia, E. Pécontal, C. R. Pennypacker, S. Perlmutter, R. Quimby, J. Raux, N. Regnault, P. Ruiz-Lapuente, B. Schaefer, K. Schahmaneche, A. L. Spadafora, N. Walton, L. Wang, W. M. Wood-Vasey, Supernova Cosmology Project Collaboration

Research School of Astronomy & Astrophysics

Research output: Contribution to conference › Paper

Abstract

We present several quality spectra of high-redshift Type Ia Supernovae (SNe Ia) observed over the past 7 years by the Supernova Cosmology Project. These spectra are first and foremost used to classify the supernova type since non-Ia contamination can contribute a significant systematic error in the measurement of the cosmological parameters. A secondary effort is under way to use SNe Ia spectra at both high and low redshift as an independent tool to measure the intrinsic brightness of a supernova and to quantify/constrain possible evolutionary effects. PEN acknowledges ongoing support from the DOE and NASA.

Original language	English
Pages	84.01
Publication status	Published - 1 Dec 2001

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https://ui.adsabs.harvard.edu/abs/2001AAS...199.8401N

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Nugent, P., Aldering, G., Amanullah, R., Antilogus, P., Astier, P., Balland, C., Blanc, G., Burns, M. S., Conley, A., Deustua, S., Ellis, R., Fabbro, S., Folatelli, G., Fruchter, A., Garavini, G., Gibbons, R., Goldhaber, G., Goobar, A., Groom, D. E., ... Collaboration, S. C. P. (2001). Interpretation of High-z SN Spectra. 84.01. https://ui.adsabs.harvard.edu/abs/2001AAS...199.8401N

@conference{d43b36c4937843dea9954a7abb252dfc,

title = "Interpretation of High-z SN Spectra",

abstract = "We present several quality spectra of high-redshift Type Ia Supernovae (SNe Ia) observed over the past 7 years by the Supernova Cosmology Project. These spectra are first and foremost used to classify the supernova type since non-Ia contamination can contribute a significant systematic error in the measurement of the cosmological parameters. A secondary effort is under way to use SNe Ia spectra at both high and low redshift as an independent tool to measure the intrinsic brightness of a supernova and to quantify/constrain possible evolutionary effects. PEN acknowledges ongoing support from the DOE and NASA.",

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

year = "2001",

month = dec,

day = "1",

language = "English",

pages = "84.01",

}

Nugent, P, Aldering, G, Amanullah, R, Antilogus, P, Astier, P, Balland, C, Blanc, G, Burns, MS, Conley, A, Deustua, S, Ellis, R, Fabbro, S, Folatelli, G, Fruchter, A, Garavini, G, Gibbons, R, Goldhaber, G, Goobar, A, Groom, DE, Hardin, D, Hook, IM, Howell, DA, Irwin, M, Kasen, D, Kim, A, Knop, RA, Levy, J-M, Lidman, C, McMahon, R, Mouchet, M, Nobili, S, Pain, R, Panagia, N, Pécontal, E, Pennypacker, CR, Perlmutter, S, Quimby, R, Raux, J, Regnault, N, Ruiz-Lapuente, P, Schaefer, B, Schahmaneche, K, Spadafora, AL, Walton, N, Wang, L, Wood-Vasey, WM & Collaboration, SCP 2001, 'Interpretation of High-z SN Spectra', pp. 84.01. <https://ui.adsabs.harvard.edu/abs/2001AAS...199.8401N>

TY - CONF

T1 - Interpretation of High-z SN Spectra

AU - Nugent, P.

AU - Aldering, G.

AU - Amanullah, R.

AU - Antilogus, P.

AU - Astier, P.

AU - Balland, C.

AU - Blanc, G.

AU - Burns, M. S.

AU - Conley, A.

AU - Deustua, S.

AU - Ellis, R.

AU - Fabbro, S.

AU - Folatelli, G.

AU - Fruchter, A.

AU - Garavini, G.

AU - Gibbons, R.

AU - Goldhaber, G.

AU - Goobar, A.

AU - Groom, D. E.

AU - Hardin, D.

AU - Hook, I. M.

AU - Howell, D. A.

AU - Irwin, M.

AU - Kasen, D.

AU - Kim, A.

AU - Knop, R. A.

AU - Levy, J. -M.

AU - Lidman, C.

AU - McMahon, R.

AU - Mouchet, M.

AU - Nobili, S.

AU - Pain, R.

AU - Panagia, N.

AU - Pécontal, E.

AU - Pennypacker, C. R.

AU - Perlmutter, S.

AU - Quimby, R.

AU - Raux, J.

AU - Regnault, N.

AU - Ruiz-Lapuente, P.

AU - Schaefer, B.

AU - Schahmaneche, K.

AU - Spadafora, A. L.

AU - Walton, N.

AU - Wang, L.

AU - Wood-Vasey, W. M.

AU - Collaboration, Supernova Cosmology Project

PY - 2001/12/1

Y1 - 2001/12/1

N2 - We present several quality spectra of high-redshift Type Ia Supernovae (SNe Ia) observed over the past 7 years by the Supernova Cosmology Project. These spectra are first and foremost used to classify the supernova type since non-Ia contamination can contribute a significant systematic error in the measurement of the cosmological parameters. A secondary effort is under way to use SNe Ia spectra at both high and low redshift as an independent tool to measure the intrinsic brightness of a supernova and to quantify/constrain possible evolutionary effects. PEN acknowledges ongoing support from the DOE and NASA.

AB - We present several quality spectra of high-redshift Type Ia Supernovae (SNe Ia) observed over the past 7 years by the Supernova Cosmology Project. These spectra are first and foremost used to classify the supernova type since non-Ia contamination can contribute a significant systematic error in the measurement of the cosmological parameters. A secondary effort is under way to use SNe Ia spectra at both high and low redshift as an independent tool to measure the intrinsic brightness of a supernova and to quantify/constrain possible evolutionary effects. PEN acknowledges ongoing support from the DOE and NASA.

M3 - Paper

SP - 84.01

ER -

Interpretation of High-z SN Spectra

Abstract

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