高里比都努尔脉冲星系统

Kshitij S. Bane, I. V. Barve, G. Gireesh, Chinnadurai Kathiravan, R. Ramesh
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引用次数: 0

摘要

最近在印度班加罗尔附近的高里比达努尔射电天文台投入使用了一个专门用于观测脉冲星和其他天体物理瞬变频率在50-80兆赫兹范围内的系统。该系统的一个显著特征是数字延迟波束形成,与通用电缆相位/延迟移位器相比,它可以同时将天线响应方向(“波束”)相位到天空的不同方向,后者有助于在给定的时间点只观察天空的特定方向。对于使用在低频率的大型天线阵列来说,机械转向是困难的。所报告的工作预期将为SKA-Low的类似工作提供有用的投入。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Gauribidanur Pulsar System
A dedicated system for observations of Pulsars and other astrophysical transients in the frequency range of 50–80 MHz has been recently commissioned at the Gauribidanur Radio Observatory near Bangalore, India. One of the salient features of the system is digital delay beamforming to simultaneously phase the antenna response pattern (“beam”) to different directions in the sky as compared to the generic cable phase/delay shifters which help to observe only a particular direction of the sky at a given epoch. Mechanical steering is difficult for the large antenna arrays used at low frequencies. The work reported is expected to provide useful inputs for similar work with SKA-Low.
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