THE STANDARDIZED CANDLE METHOD FOR TYPE II PLATEAU SUPERNOVAE

被引：125

作者：

Olivares E, Felipe ^{[1
,2
]}

Hamuy, Mario ^{[1
]}

Pignata, Giuliano ^{[1
,3
]}

Maza, Jose ^{[1
]}

Bersten, Melina ^{[1
]}

Phillips, Mark M. ^{[4
]}

Suntzeff, Nicholas B. ^{[5
]}

Filippenko, Alexei V. ^{[6
]}

Morrel, Nidia I. ^{[4
]}

Kirshner, Robert P. ^{[7
]}

Matheson, Thomas ^{[8
]}

机构：

[1] Univ Chile, Dept Astron, Santiago, Chile

[2] Max Planck Inst Extraterr Phys, D-85740 Garching, Germany

[3] Univ Andres Bello, Dept Ciencias Fis, Santiago, Chile

[4] Carnegie Observ, Las Campanas Observ, La Serena, Chile

[5] Texas A&M Univ, Dept Phys, College Stn, TX 77843 USA

[6] Univ Calif Berkeley, Dept Astron, Berkeley, CA 94720 USA

[7] Harvard Smithsonian Ctr Astrophys, Cambridge, MA 02138 USA

[8] Natl Opt Astron Observ, Tucson, AZ 85719 USA

来源：

ASTROPHYSICAL JOURNAL | 2010年 / 715卷 / 02期

基金：

美国国家科学基金会;

关键词：

distance scale; galaxies: distances and redshifts; supernovae: general; QUANTITATIVE SPECTROSCOPIC ANALYSIS; PROBE WMAP OBSERVATIONS; DARK ENERGY; IA SUPERNOVAE; HUBBLE DIAGRAM; P SUPERNOVAE; LIGHT CURVES; SN; 2005CS; GALAXY DISTANCES; DECLINE RATE;

D O I：

10.1088/0004-637X/715/2/833

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

In this paper, we study the "standardized candle method" using a sample of 37 nearby (redshift z < 0.06) Type II plateau supernovae having BVRI photometry and optical spectroscopy. An analytic procedure is implemented to fit light curves, color curves, and velocity curves. We find that the V-I color toward the end of the plateau can be used to estimate the host-galaxy reddening with a precision of sigma(A(V)) = 0.2 mag. The correlation between plateau luminosity and expansion velocity previously reported in the literature is recovered. Using this relation and assuming a standard reddening law (R-V = 3.1), we obtain Hubble diagrams (HDs) in the BVI bands with dispersions of similar to 0.4 mag. Allowing R-V to vary and minimizing the spread in the HDs, we obtain a dispersion range of 0.25-0.30 mag, which implies that these objects can deliver relative distances with precisions of 12%-14%. The resulting best-fit value of R-V is 1.4 +/- 0.1.

引用

页码：833 / 853

页数：21

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