0320010

We ask for 3 observations of 300 ks each to observe in target-of-opportunity (TOO) up to 3 blazars conditional to stringent and well defined triggering criteria based on optical X-ray or gamma-ray brightening. Serendipitous detections of bright blazars by INTEGRAL itself and by Swift/BAT will also be instrumental to TOO activation. By coordinating these INTEGRAL observations with XMM-Newton campaigns and by complementing these with monitoring at TeV optical and radio frequencies we will guarantee the coverage of a broad energy range. This will allow us to follow the evolution of the overall spectral distribution of blazars during a flare episode and thus constrain the time-dependent parameters of the emission model.=======Please note that the exposures indicated in the Observation Details Panel are purely indicative only to fill the form. The required time is 3 observation of 300 ks each in ToO. [truncated! Please see actual data for full text]

我们申请开展3次观测，每次时长300千秒（ks），用于机遇目标（target-of-opportunity，TOO）观测最多3个耀变体（blazar），观测需满足基于光学、X射线或伽马射线增亮的严格且明确的触发标准。INTEGRAL自身及Swift/BAT对明亮耀变体的偶然探测，也将对TOO触发起到关键作用。通过将这些INTEGRAL观测与XMM-Newton项目协调，并辅以太电子伏特（TeV）、光学及射电频段的监测，我们将确保覆盖广泛的能谱范围。这将使我们能够追踪耀变体在爆发期间整体能谱分布的演化，从而约束辐射模型的时间依赖参数。=======请注意，观测详情面板中所示的曝光时间仅为填写表单的指示性数据。所需时间为3次TOO观测，每次300千秒（ks）。[内容截断！请查阅实际数据获取完整文本]