Supernova Type Ia Evolution and Grey Dust: Ground and Spaced Based Follow up of a Type Ia Supernova at z=0.54

S. Nobili; C. Lidman; 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; R. McMahon; M. Mouchet; P. Nugent; 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 Type Ia Evolution and Grey Dust: Ground and Spaced Based Follow up of a Type Ia Supernova at z=0.54

S. Nobili, C. Lidman, 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. GroomD. Hardin, I. M. Hook, D. A. Howell, M. Irwin, D. Kasen, A. Kim, R. A. Knop, J. -M. Levy, R. McMahon, M. Mouchet, P. Nugent, 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

Research School of Astronomy & Astrophysics

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Abstract

As part of the Spring 2000 campaign to discover and follow up high redshift type Ia supernovae, the SCP spectroscopically confirmed a type Ia supernova at z=0.54 two weeks before maximum light. The early discovery, at the CFHT, allowed us to obtain an extensive data set, which includes ground-based, multi-epoch infrared data from ISAAC on the ESO VLT, ground-based spectroscopic data from the VLT and Keck telescope, and high signal-to-noise optical lightcurves from HST. The exquisite S/N of this data allows us to examine this supernova in great detail. The data show that this supernova is quite normal and will allow us to place constraints on the amount of dust, be it normal or grey.

Original language	English
Pages	16.11
Publication status	Published - 1 Dec 2001

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https://ui.adsabs.harvard.edu/abs/2001AAS...199.1611N

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Nobili, S., Lidman, C., 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., ... Wood-Vasey, W. M. (2001). Supernova Type Ia Evolution and Grey Dust: Ground and Spaced Based Follow up of a Type Ia Supernova at z=0.54. 16.11. https://ui.adsabs.harvard.edu/abs/2001AAS...199.1611N

@conference{46506923ba7d42d3bc526f1c3df63a21,

title = "Supernova Type Ia Evolution and Grey Dust: Ground and Spaced Based Follow up of a Type Ia Supernova at z=0.54",

abstract = "As part of the Spring 2000 campaign to discover and follow up high redshift type Ia supernovae, the SCP spectroscopically confirmed a type Ia supernova at z=0.54 two weeks before maximum light. The early discovery, at the CFHT, allowed us to obtain an extensive data set, which includes ground-based, multi-epoch infrared data from ISAAC on the ESO VLT, ground-based spectroscopic data from the VLT and Keck telescope, and high signal-to-noise optical lightcurves from HST. The exquisite S/N of this data allows us to examine this supernova in great detail. The data show that this supernova is quite normal and will allow us to place constraints on the amount of dust, be it normal or grey.",

author = "S. Nobili and C. Lidman 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 R. McMahon and M. Mouchet and P. Nugent 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.}",

year = "2001",

month = dec,

day = "1",

language = "English",

pages = "16.11",

}

Nobili, S, Lidman, C, 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, McMahon, R, Mouchet, M, Nugent, P, 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 2001, 'Supernova Type Ia Evolution and Grey Dust: Ground and Spaced Based Follow up of a Type Ia Supernova at z=0.54', pp. 16.11. <https://ui.adsabs.harvard.edu/abs/2001AAS...199.1611N>

TY - CONF

T1 - Supernova Type Ia Evolution and Grey Dust: Ground and Spaced Based Follow up of a Type Ia Supernova at z=0.54

AU - Nobili, S.

AU - Lidman, C.

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 - McMahon, R.

AU - Mouchet, M.

AU - Nugent, P.

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.

PY - 2001/12/1

Y1 - 2001/12/1

N2 - As part of the Spring 2000 campaign to discover and follow up high redshift type Ia supernovae, the SCP spectroscopically confirmed a type Ia supernova at z=0.54 two weeks before maximum light. The early discovery, at the CFHT, allowed us to obtain an extensive data set, which includes ground-based, multi-epoch infrared data from ISAAC on the ESO VLT, ground-based spectroscopic data from the VLT and Keck telescope, and high signal-to-noise optical lightcurves from HST. The exquisite S/N of this data allows us to examine this supernova in great detail. The data show that this supernova is quite normal and will allow us to place constraints on the amount of dust, be it normal or grey.

AB - As part of the Spring 2000 campaign to discover and follow up high redshift type Ia supernovae, the SCP spectroscopically confirmed a type Ia supernova at z=0.54 two weeks before maximum light. The early discovery, at the CFHT, allowed us to obtain an extensive data set, which includes ground-based, multi-epoch infrared data from ISAAC on the ESO VLT, ground-based spectroscopic data from the VLT and Keck telescope, and high signal-to-noise optical lightcurves from HST. The exquisite S/N of this data allows us to examine this supernova in great detail. The data show that this supernova is quite normal and will allow us to place constraints on the amount of dust, be it normal or grey.

M3 - Paper

SP - 16.11

ER -

Supernova Type Ia Evolution and Grey Dust: Ground and Spaced Based Follow up of a Type Ia Supernova at z=0.54

Abstract

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