Multifrequency polarimetry of 300 radio pulsars
Multifrequency polarimetry of 300 radio pulsars
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DOI：
10.1046/j.1365-8711.1998.02018.x
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发表时间：
1998-11
影响因子：
4.8
通讯作者：
D. M. Gould;A. Lyne
中科院分区：
文献类型：
--
作者：
D. M. Gould;A. Lyne
使用 Jodrell Bank 的 76 米洛弗尔望远镜，以 230、400、600、920、1400 和 1600 MHz 左右的无线电频率对 300 颗脉冲星进行了偏振观测。超过一半的脉冲星没有先前发布的偏振剖面，该汇编大约是先前发布的所有脉冲星偏振数据总和的三倍。提供了一系列集成偏振分布。给出了所有脉冲星的脉冲宽度以及线性和圆偏振度的表，这些数据充当所有数据的索引，这些数据可以通过匿名 ftp 以数字和图形形式获得。
Polarimetric observations of 300 pulsars have been conducted with the 76-m Lovell telescope at Jodrell Bank at radio frequencies centred around 230, 400, 600, 920, 1400 and 1600 MHz. More than half of the pulsars have no previously published polarization profiles and this compilation represents about three times the sum of all previously published pulsar polarization data. A selection of integrated polarization profiles is provided. Tables of pulse widths and the degree of both linear and circular polarization are given for all pulsars, and these act as an index for all the data, which are available by anonymous ftp in numerical and graphical form.