Doppler tomography by total variation minimization

被引:9
|
作者
Uemura, Makoto [1 ]
Kato, Taichi [2 ]
Nogami, Daisaku [3 ,4 ]
Mennickent, Ronald [5 ]
机构
[1] Hiroshima Univ, Hiroshima Astrophys Sci Ctr, Hiroshima 7398526, Japan
[2] Kyoto Univ, Dept Astron, Sakyo Ku, Kyoto 6068502, Japan
[3] Kyoto Univ, Kwasan Observ, Yamashina Ku, Kyoto 6078471, Japan
[4] Kyoto Univ, Hida Observ, Yamashina Ku, Kyoto 6078471, Japan
[5] Univ Concepcion, Dept Astron, Concepcion, Chile
关键词
accretion; accretion disks; methods: data analysis; novae; cataclysmic variables; ACCRETION; STAR;
D O I
10.1093/pasj/psu154
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We have developed a new model of Doppler tomography using total variation minimization (DTTVM). This method can reconstruct localized and nonaxisymmetric profiles with sharp edges in the Doppler map. This characteristic is emphasized in the case where input data are small in number. We apply this model to natural data for the dwarf nova WZ Sge in superoutburst and TU Men in quiescence. We confirm that DTTVM can reproduce the observed spectra with high precision. Compared with the models based on the maximum entropy method, our new model can provide Doppler maps that little depend on the hyperparameter and on the presence of the absorption core. We also introduce a cross-validation method of estimating reasonable values of a hyperparameter in the model from the data themselves.
引用
收藏
页数:12
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