Spectral distributions in compact radio sources - I. Imaging with VLBI data

被引:36
作者
Lobanov, AP [1 ]
机构
[1] Max Planck Inst Radioastron, D-53121 Bonn, Germany
来源
ASTRONOMY & ASTROPHYSICS SUPPLEMENT SERIES | 1998年 / 132卷 / 02期
关键词
methods : data analysis; methods : observational; quasars : individual : 3C 345; techniques : interferometric;
D O I
10.1051/aas:1998446
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We discuss a technique for mapping the synchrotron turnover frequency distribution using nearly simultaneous, multi-frequency VLBI observations. The limitations of the technique arising from limited spatial sampling and frequency coverage are investigated. The errors caused ha uneven spatial sampling of typical multifrequency VLBA datasets are estimated through numerical simulations, and are shown to be of the order of 10%, for pixels with the deconvolution SNR similar to 7. The fitted spectral parameters are corrected for the errors due to limited frequency coverage of VLBI data. First results from mapping the turnover frequency distribution in 3C 345 are presented.
引用
收藏
页码:261 / 273
页数:13
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