A 1–bit Raw Voltage-recording System for Dedicated Observations of Transients at Low Radio Frequencies

Kshitij S. Bane, I. V. Barve, G. Gireesh, C. Kathiravan, R. Ramesh
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Abstract

Recently we had reported commissioning of a prototype for pulsar observations at low radio frequencies (<100 MHz) using log-periodic dipole antennas in the Gauribidanur Radio Observatory (≈77°E, 14°N) near Bangalore in India (https://www.iiap.res.in/?q=centers/radio). The aforementioned system (the Gauribidanur Pulsar System) is currently being augmented to directly digitize the radio-frequency signals from the individual antennas in the array. Our initial results using a 1–bit raw voltage-recording system indicate that such a back-end receiver offers distinct advantages like (i) simultaneous observations of any set of desired directions in the sky with multiple offline beams and smaller data rate/volume, and (ii) archival of the observed data with minimal resources for reanalysis in the future, either in the same or a different set of directions in the sky.
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用于专门观测低无线电频率瞬变的 1 位原始电压记录系统
最近,我们报告了在印度班加罗尔附近的高里比达努尔射电天文台(≈77°E,14°N)使用对数周期偶极子天线进行低射电频率(<100 MHz)脉冲星观测的原型(https://www.iiap.res.in/?q=centers/radio)。上述系统(高里比达努尔脉冲星系统)目前正在进行扩充,以直接数字化来自阵列中各个天线的射频信号。我们使用 1 位原始电压记录系统的初步结果表明,这种后端接收器具有以下明显优势:(i) 以多个离线波束和较小的数据速率/容量对天空中任何一组所需的方向同时进行观测;(ii) 以最少的资源将观测数据存档,以便将来在天空中相同或不同的方向上进行重新分析。
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