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eROSITA in-orbit calibration strategy and plan: from the ground to the science

机译:eROSITA在轨校准策略和计划:从地面到科学

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eROSITA is a German X-ray astronomical observatory on-board Spectrum-Roentgen-Gamma (SRG) with anexpected launch in 2014 and operation at libration point L2. It consists of 7 identical mirror modules with 7identical CCD cameras as focal plane instrumentation. It will observe the X-ray sky in the 0.25 − 10 keV range(4 yr all-sky survey, then pointed observations). Another instrument aboard SRG, ART-XC, will extend thespectral range to higher energies. We describe how the on-ground calibration is planned for the PANTER andPUMA X-ray test facilities, with respect to maximum scientific exploitation, in combination with an in-orbitcalibration. This will be performed within one module and between the 7 eROSITA modules. If XMM-Newtonwill still be operational, a dedicated cross-calibration campaign is envisaged. The selection of the celestial targetsand the procedure of the measurements with the internal Fe-55 calibration source are outlined.© (2012) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
机译:eROSITA是德国X射线天文观测台上的Spectrum-Rentgen-Gamma(SRG)卫星,预计于2014年发射,并在解放点L2运作。它由7个相同的反射镜模块和7个相同的CCD相机作为焦平面仪器组成。它将观测0.25 − 10 keV范围内的X射线天空(4年全天候观测,然后进行尖锐观测)。 SRG上的另一台仪器ART-XC将把光谱范围扩大到更高的能量。我们描述了如何针对PANTER和PUMA X射线测试设备进行地面校准,并结合在轨校准,以最大程度地利用科学知识。这将在一个模块内以及7个eROSITA模块之间执行。如果XMM-Newton仍可运行,则可以设想进行专门的交叉校准。概述了天体目标的选择以及使用内部Fe-55校准源进行的测量过程。©(2012)COPYRIGHT光电仪器工程师协会(SPIE)。摘要的下载仅允许个人使用。

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