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
相关论文
共 79 条
[1]   The rise times of high- and low-redshift Type Ia supernovae are consistent [J].
Aldering, G ;
Knop, R ;
Nugent, P .
ASTRONOMICAL JOURNAL, 2000, 119 (05) :2110-2117
[2]   Type Ia supernova SN 2003du: Optical observations [J].
Anupama, GC ;
Sahu, DK ;
Jose, J .
ASTRONOMY & ASTROPHYSICS, 2005, 429 (02) :667-676
[3]  
ASTIER P, 1999, 7258 IAU, P1
[4]  
BALLAND C, 2005, 8516 IAU, P1
[5]   Twenty-three high-redshift supernovae from the Institute for Astronomy Deep Survey:: Doubling the supernova sample at z > 0.7 [J].
Barris, BJ ;
Tonry, JL ;
Blondin, S ;
Challis, P ;
Chornock, R ;
Clocchiatti, A ;
Filippenko, AV ;
Garnavich, P ;
Holland, ST ;
Jha, S ;
Kirshner, RP ;
Krisciunas, K ;
Leibundgut, B ;
Li, WD ;
Matheson, T ;
Miknaitis, G ;
Riess, AG ;
Schmidt, BP ;
Smith, RC ;
Sollerman, J ;
Spyromilio, J ;
Stubbs, CW ;
Suntzeff, NB ;
Aussel, H ;
Chambers, KC ;
Connelley, MS ;
Donovan, D ;
Henry, JP ;
Kaiser, N ;
Liu, MC ;
Martín, EL ;
Wainscoat, RJ .
ASTROPHYSICAL JOURNAL, 2004, 602 (02) :571-594
[6]  
BASA, 2005, UNPUB
[7]   Supernova 2002bo: inadequacy of the single parameter description [J].
Benetti, S ;
Meikle, P ;
Stehle, M ;
Altavilla, G ;
Desidera, S ;
Folatelli, G ;
Goobar, A ;
Mattila, S ;
Mendez, J ;
Navasardyan, H ;
Pastorello, A ;
Patat, F ;
Riello, M ;
Ruiz-Lapuente, P ;
Tsvetkov, D ;
Turatto, M ;
Mazzali, P ;
Hillebrandt, W .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2004, 348 (01) :261-278
[8]  
BENETTI S, 2005, ARXIVASTROPH0411059
[9]   THE TYPE-I SUPER-NOVA 1981B IN NGC-4536 - THE 1ST 100 DAYS [J].
BRANCH, D ;
LACY, CH ;
MCCALL, ML ;
SUTHERLAND, PG ;
UOMOTO, A ;
WHEELER, JC ;
WILLS, BJ .
ASTROPHYSICAL JOURNAL, 1983, 270 (01) :123-&