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We propose XMM-Newton observations of two radio-loud magnetars XTE J1810-197and Swift J1818.0-1607 which are still recovering from their most-recentoutbursts. XTE J1810-197 is still exhibiting a soft X-ray flux a factor 2 largerthan the nominal value due to the continued existence of a thermal hot spot.The source is currently displaying unique temporal properties not observedbefore neither in outburst nor quiescence. On the other hand SwiftJ1818.0-1607 has decayed by 2 order of magnitude so far solely driven by an areashrinkage with no sign of any cooling an expected property of most magnetartheoretical scenarios. Hence establishing the X-ray evolution of these twosources towards quiescence is crucial for a better understanding of the physical driver of magnetar outbursts. [truncated! Please see actual data for full text]

我们提议对两颗仍处于最新爆发恢复期的射电活跃磁星——XTE J1810-197与Swift J1818.0-1607——开展XMM-牛顿（XMM-Newton）观测。由于热斑持续存在，XTE J1810-197的软X射线流量仍较标准值高出一倍。该源目前展现出独特的时域特性，这在爆发态与宁静态中均未曾被观测到。另一方面，Swift J1818.0-1607迄今已衰减两个数量级，其衰减仅由表面积收缩驱动，未观测到任何冷却迹象——这符合多数磁星理论模型的预期特性。因此，厘清这两颗源向宁静态演化的X射线辐射过程，对于深入理解磁星爆发的物理驱动机制至关重要。【文本已截断！完整内容请查阅实际数据集】