Spectroscopy of twelve type Ia supernovae at intermediate redshift

被引:12
|
作者
Balland, C [1 ]
Mouchet, M
Pain, R
Walton, NA
Amanullah, R
Astier, P
Ellis, RS
Fabbro, S
Goobar, A
Hardin, D
Hook, IM
Irwin, MJ
McMahon, RG
Mendez, JM
Ruiz-Lapuente, P
Sainton, G
Schahmaneche, K
Stanishev, V
机构
[1] CNRS, LPHNE, IN2P3, F-75252 Paris, France
[2] Univ Paris 06, F-75252 Paris, France
[3] Univ Paris 07, F-75252 Paris, France
[4] APC, F-75231 Paris, France
[5] CNRS, UMR 8617, IAS, F-91405 Orsay, France
[6] Univ Paris Sud 11, F-91405 Orsay, France
[7] Observ Paris, CNRS, Sect Meudon, LUTH,UMR 8102, F-92195 Meudon, France
[8] Univ Cambridge, Inst Astron, Cambridge CB3 0HA, England
[9] Univ Stockholm, Dept Phys, S-10691 Stockholm, Sweden
[10] CALTECH, Pasadena, CA 91125 USA
[11] IST, Ctr M Astrofis, Lisbon, Portugal
[12] IST, Dept Phys, Lisbon, Portugal
[13] Univ Barcelona, Dept Astron, E-08028 Barcelona, Spain
[14] Isaac Newton Grp Telescopes, Santa Cruz De La Palma 38700, Spain
关键词
cosmology : observations; supernovae : general;
D O I
10.1051/0004-6361:20053552
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present spectra of twelve type Ia supernovae obtained in 1999 at the William Herschel Telescope and the Nordic Optical Telescope during a search for type Ia supernovae ( SN Ia) at intermediate redshift. The spectra range from z = 0.178 to z = 0.493, including five high signal-to-noise ratio SN Ia spectra in the still largely unexplored range 0.15 = z = 0.3. Most of the spectra were obtained before or around restframe B-band maximum light. None of them shows the peculiar spectral features found in low-redshift over-or under-luminous SN Ia. Expansion velocities of characteristic spectral absorption features such as Si II at 6355 angstrom, S II at 5640 angstrom and Ca II at 3945 angstrom are found to be consistent with those of their low-z SN Ia counterparts.
引用
收藏
页码:387 / U36
页数:36
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