A SYNTHESIS MAP OF THE SKY AT 345-MHZ

被引:42
作者
DWARAKANATH, KS
SHANKAR, NU
机构
[1] Raman Research Institute, Bangalore
关键词
low-frequency; radio continuum; synthesis mapping; wide-field;
D O I
10.1007/BF02709282
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
This paper describes a wide-field survey made at 34.5 MHz using GEETEE,1 the low frequency telescope at Gauribidanur (latitude 13°36′12′′N). This telescope was used in the transit mode and by per forming 1-D synthesis along the north-south direction the entire observable sky was mapped in a single day. This minimized the problems that hinder wide-field low-frequency mapping. This survey covers the declination range of-50° to + 70° (- 33° to +61° without aliasing) and the complete 24 hours of right ascension. The synthesized beam has a resolution of 26′ x 42′ sec (δ- 14°. 1). The sensitivity of the survey is 5 Jy/beam (1σ). Special care has been taken to ensure that the antenna responds to all angular scale structures and is suitable for studies of both point sources and extended objects © 1990 Indian Academy of Sciences.
引用
收藏
页码:323 / 410
页数:88
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