Understanding radio polarimetry .2. Instrumental calibration of an interferometer array

被引:108
作者
Sault, RJ
Hamaker, JP
Bregman, JD
机构
[1] NETHERLANDS FDN RES ASTRON,7990 AA DWINGELOO,NETHERLANDS
[2] CSIRO,AUSTRALIA TELESCOPE NATL FACIL,EPPING,NSW 2121,AUSTRALIA
来源
ASTRONOMY & ASTROPHYSICS SUPPLEMENT SERIES | 1996年 / 117卷 / 01期
关键词
methods; analytical; data analysis; techniques; interferometers; polarimeters;
D O I
10.1051/aas:1996100
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
In a companion paper, a mathematical formalism to describe the polarimetric response of a radio interferometer was presented. Some of the instrumental parameters, however, are either unknown or poorly known. Here we consider the determination of these parameters both by a traditional radio-interferometry instrumental approach as well as by using optical polarimetry principles. In doing so, we establish links between the two fields. We show that some degrees of freedom cannot be solved for with various calibration or self-calibration schemes. These degrees of freedom are identified with instrumental parameters and physical source properties. The number of unsolvable degrees of freedom is reduced for a long synthesis with alt-az antennas. We also consider the effect of errors in the assumed instrumental parameters on the resultant calibrated data. The polarimetric calibration procedure for some telescopes is reviewed in the context of this analysis.
引用
收藏
页码:149 / 159
页数:11
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