Radio frequency interference identification and mitigation in pulsar observations using machine learning techniques

M. McCarty, G. Doran, T. Lazio, D. Thompson, J. Ford, R. Prestage
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Abstract

Summary form only given. Pulsar observations with the Robert C. Byrd Green Bank Telescope (GBT), located in Green Bank, WV, aid researchers in understanding the basic building blocks of our existence - matter, energy, space, and time - and how they behave under extreme physical conditions. Pulsars, rapidly rotating neutron stars with clock-like timing precision, can provide insights into a rich variety of physics and astrophysics.
利用机器学习技术识别和减缓脉冲星观测中的射频干扰
只提供摘要形式。位于WV Green Bank的Robert C. Byrd Green Bank望远镜(GBT)对脉冲星的观测帮助研究人员了解了我们存在的基本组成部分——物质、能量、空间和时间——以及它们在极端物理条件下的行为。脉冲星是一种快速旋转的中子星,具有时钟般的计时精度,可以为丰富多样的物理学和天体物理学提供见解。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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