Type Ia supernova spectral line ratios as luminosity indicators

被引:33
作者
Bongard, Sebastien
Baron, E.
Smadja, G.
Branch, David
Hauschildt, Peter H.
机构
[1] Lawrence Berkeley Natl Lab, Div Phys, Berkeley, CA 94720 USA
[2] Univ Oklahoma, Dept Phys & Astron, Norman, OK 73019 USA
[3] Univ Lyon 1, Inst Phys Nucl, F-69622 Villeurbanne, France
[4] Lawrence Berkeley Natl Lab, Computat Res Div, Berkeley, CA 94720 USA
[5] Hamburger Sternwarte, D-21029 Hamburg, Germany
基金
美国国家科学基金会;
关键词
dark matter; stars : atmospheres; supernovae : general;
D O I
10.1086/505322
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Type Ia supernovae have played a crucial role in the discovery of the dark energy, via the measurement of their light curves and the determination of the peak brightness via fitting templates to the observed light-curve shape. Two spectroscopic indicators are also known to be well correlated with peak luminosity. Since the spectroscopic luminosity indicators are obtained directly from observed spectra, they will have different systematic errors than do measurements using photometry. In addition, these spectroscopic indicators may be useful for studies of effects of evolution or age of the SNe Ia progenitor population. We present several new variants of such spectroscopic indicators that are easy to automate and that minimize the effects of noise. We show that these spectroscopic indicators can be measured by proposed JDEM missions such as SNAP and JEDI.
引用
收藏
页码:513 / 524
页数:12
相关论文
共 32 条
[1]  
ALDERING G, 2004, UNPUB PASP
[2]   Spectral modeling of SNe Ia near maximum light: Probing the characteristics of hydrodynamical models [J].
Baron, E. ;
Bongard, Sebastien ;
Branch, David ;
Hauschildt, Peter H. .
ASTROPHYSICAL JOURNAL, 2006, 645 (01) :480-487
[3]   Non-local thermodynamic equilibrium effects in modelling of supernovae near maximum light [J].
Baron, E ;
Hauschildt, PH ;
Nugent, P ;
Branch, D .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1996, 283 (01) :297-315
[4]   Statistical connections between the properties of type Ia supernovae and the B-V colors of their parent galaxies, and the value of H-0 [J].
Branch, D ;
Romanishin, W ;
Baron, E .
ASTROPHYSICAL JOURNAL, 1996, 465 (01) :73-78
[5]   ON THE RELATIVE FREQUENCIES OF SPECTROSCOPICALLY NORMAL AND PECULIAR TYPE-IA SUPERNOVAE [J].
BRANCH, D ;
FISHER, A ;
NUGENT, P .
ASTRONOMICAL JOURNAL, 1993, 106 (06) :2383-2391
[6]  
CROTTS A, 2005, JOINT EFFICIENT DARK
[7]   An integral field spectrograph for SNAP supernova studies [J].
Ealet, A ;
Prieto, E ;
Bonissent, A ;
Malina, R ;
Bernstein, G ;
Basa, S ;
LeFevre, O ;
Mazure, A ;
Bonneville, C ;
Akerlof, C ;
Aldering, G ;
Amanullah, R ;
Astier, P ;
Barrelet, E ;
Bebek, C ;
Bergström, L ;
Bercovitz, J ;
Bester, M ;
Bonissent, A ;
Bower, C ;
Carithers, W ;
Commins, E ;
Day, C ;
Deustua, S ;
DiGennaro, R ;
Ealet, A ;
Ellis, R ;
Eriksson, M ;
Fruchter, A ;
Genat, JF ;
Goldhaber, G ;
Goobar, A ;
Groom, D ;
Harris, S ;
Harvey, P ;
Heetderks, H ;
Holland, S ;
Huterer, D ;
Karcher, A ;
Kim, A ;
Kolbe, W ;
Krieger, B ;
Lafever, R ;
Lamoureux, J ;
Lampton, M ;
Levi, M ;
Levin, D ;
Linder, E ;
Loken, S ;
Malina, R .
IR SPACE TELESCOPES AND INSTRUMENTS, PTS 1 AND 2, 2003, 4850 :1169-1178
[8]   The luminosity of SN 1999by in NGC 2841 and the nature of "peculiar" Type Ia supernovae [J].
Garnavich, PM ;
Bonanos, AZ ;
Krisciunas, K ;
Jha, S ;
Kirshner, RP ;
Schlegel, EM ;
Challis, P ;
Macri, LM ;
Hatano, K ;
Branch, D ;
Bothun, GD ;
Freedman, WL .
ASTROPHYSICAL JOURNAL, 2004, 613 (02) :1120-1132
[9]   Constraints on cosmological models from Hubble Space Telescope observations of high-z supernovae [J].
Garnavich, PM ;
Kirshner, RP ;
Challis, P ;
Tonry, J ;
Gilliland, RL ;
Smith, RC ;
Clocchiatti, A ;
Diercks, A ;
Filippenko, AV ;
Hamuy, M ;
Hogan, CJ ;
Leibundgut, B ;
Phillips, MM ;
Reiss, D ;
Riess, AG ;
Schmidt, BP ;
Schommer, RA ;
Spyromilio, J ;
Stubbs, C ;
Suntzeff, NB ;
Wells, L .
ASTROPHYSICAL JOURNAL, 1998, 493 (02) :L53-+
[10]   Timescale stretch parameterization of Type Ia supernova B-band light curves [J].
Goldhaber, G ;
Groom, DE ;
Kim, A ;
Aldering, G ;
Astier, P ;
Conley, A ;
Deustua, SE ;
Ellis, R ;
Fabbro, S ;
Fruchter, AS ;
Goobar, A ;
Hook, I ;
Irwin, M ;
Kim, M ;
Knop, RA ;
Lidman, C ;
McMahon, R ;
Nugent, PE ;
Pain, R ;
Panagia, N ;
Pennypacker, CR ;
Perlmutter, S ;
Ruiz-Lapuente, P ;
Schaefer, B ;
Walton, NA ;
York, T .
ASTROPHYSICAL JOURNAL, 2001, 558 (01) :359-368