Pushchino multibeams pulsar search: First results

S. Tyul’bashev, G. E. Tyul’basheva, M. Kitaeva
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Abstract

Since the discovery of pulsars, dozens of surveys have already been conducted with their searches. In the course of surveys in the sky, areas from thousands to tens of thousands of square degrees are explored. Despite repeated observations of the same areas, new pulsars are constantly being discovered. We present Pushchino Multibeam Pulsar Search (PUMPS), having a sensitivity that is an order of magnitude higher than the sensitivity of all previously made surveys on pulsar search. In PUMPS daily round-the-clock observations are carried out of the area located on declinations $-9^o<\delta<+42^o$. The survey is carried out on 96 beams of a Large Phased Array (LPA) at a frequency of 111 MHz. During the observation period of August 2014 - August 2022, the survey was repeated approximately 3,000 times. The expected sensitivity in the survey reaches up to 0.1 mJy. The paper considers some tasks that can be solved when processing the received data.
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普什奇诺多波束脉冲星搜索:初步结果
自从发现脉冲星以来,已经进行了数十次调查。在对天空的调查过程中,探测的面积从几千平方度到几万平方度不等。尽管对同一区域进行了多次观测,但新的脉冲星不断被发现。我们提出了普什奇诺多波束脉冲星搜索(泵),其灵敏度比以前所有脉冲星搜索的灵敏度高一个数量级。在泵每天24小时的观测是在位于赤纬$-9^o<\delta<+42^o$的区域进行的。该测量是在频率为111 MHz的大型相控阵(LPA)的96束上进行的。在2014年8月至2022年8月的观察期间,该调查重复了约3000次。该调查的预期灵敏度可达0.1 mJy。本文考虑了在处理接收数据时可以解决的一些问题。
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