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首页> 外文期刊>Classical and Quantum Gravity: An Interantional Journal of Gravity Geometry of Field Theories Supergravity Cosmology >A first test of a sine-Hough method for the detection of pulsars in binary systems using the E4 Virgo engineering run data
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A first test of a sine-Hough method for the detection of pulsars in binary systems using the E4 Virgo engineering run data

机译:使用E4处女座工程运行数据的正弦-霍夫方法在二进制系统中检测脉冲星的首次测试

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摘要

Most of the known pulsars with frequencies lying in the best sensitivity rang e of the Virgo/LIGO/TAMA interferometers belong to binary systems. Accordingly their frequencies are Doppler shifted in an unknown way. We investigate a new method to search for and extract the parameters of such pulsars. A first preliminary test of this method, performed on the Virgo data recorded during the E4 engineering run, is presented. [References: 13]
机译:频率在处女座/ LIGO / TAMA干涉仪的最佳灵敏度范围内的大多数已知脉冲星都属于二元系统。因此,它们的频率以未知的方式被多普勒频移。我们研究了一种搜索和提取此类脉冲星参数的新方法。提出了对该方法的第一个初步测试,该测试是对E4工程运行期间记录的处女座数据进行的。 [参考:13]

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