The Deep Space Network (DSN) is a worldwide array of radio telescopes which supports NASA’s interplanetary spacecraft missions. When the DSN antennas are not communicating with spacecraft, they provide a valuable resource for performing observations of radio magnetars, searches for new pulsars at the Galactic Center, and additional pulsar-related studies. We describe the DSN’s capabilities for carrying out these types of observations. We also present results from observations of three radio magnetars, PSR J1745–2900, PSR J1622–4950, and XTE J1810–197, and the transitional magnetar candidate, PSR J1119–6127, using the DSN radio telescopes near Canberra, Australia.

中文翻译：

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利用深空网观测无线电电磁

深空网络（DSN）是全球范围内的射电望远镜阵列，可支持NASA的行星际航天器飞行任务。当DSN天线不与航天器通信时，它们提供了宝贵的资源，可用于执行无线电磁星的观测，在银河中心搜索新的脉冲星，以及其他与脉冲星相关的研究。我们描述了DSN进行此类观察的能力。我们还提供了在澳大利亚堪培拉附近使用DSN射电望远镜观测到的三个射电磁铁PSR J1745-2900，PSR J1622-4950和XTE J1810197以及过渡磁星候选PSR J1119-6127的结果。