ABSTRACT

We present observations of 35 high spin-down energy radio pulsars using the MeerKAT telescope. Polarization profiles and associated parameters are also presented. We derive the geometry for a selection of pulsars which show interpulse emission. We point out that, in several cases, these radio pulsars should also be seen in γ-rays but that improved radio timing is required to aid the high-energy detection. We discuss the relationship between the width of the radio profile and its high-energy detectability. Finally, we reflect on the correlation between the spin-down energy and the radio polarization fraction and the implications this may have for γ-ray emission.

中文翻译：

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MeerKAT IV 上的千脉冲星阵列计划：年轻、高能脉冲星的极化特性

摘要

我们使用 MeerKAT 望远镜对 35 颗高自旋能量射电脉冲星进行了观测。还介绍了偏振分布和相关参数。我们推导出了一些显示脉冲间发射的脉冲星的几何形状。我们指出，在一些情况下，这些射电脉冲星也应该在 γ 射线中看到，但需要改进无线电定时来帮助高能探测。我们讨论了无线电剖面的宽度与其高能量可探测性之间的关系。最后，我们反思了自旋向下能量与无线电极化率之间的相关性，以及这可能对 γ 射线发射产生的影响。