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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]

我们提出针对两颗仍处于最新爆发后恢复阶段的射电强磁星（magnetar）XTE J1810-197与Swift J1818.0-1607的XMM-牛顿（XMM-Newton）望远镜观测计划。其中XTE J1810-197因持续存在热斑结构，其软X射线通量为标称值的2倍；该源当前展现出此前在爆发或宁静阶段均未观测到的独特时域特性。另一方面，Swift J1818.0-1607迄今已衰减两个数量级，其辐射衰减仅由作用区域收缩驱动，未观测到任何冷却迹象——这一特性与多数磁星理论模型的预期相符。因此，厘清这两颗源向宁静态演化的X射线演化规律，对于深入理解磁星爆发的物理驱动机制具有关键意义。[文本已截断，完整内容请参阅实际数据集]