Jaeckel F T, Ambarish C V, Christensen N, Gruenke R, Hu L, McCammon D, McPheron M, Meyer M, Nelms K L, Roy A, Wulf D, Zhang S, Zhou Y, Adams J S, Bandler S R, Chervenak J A, Datesman A M, Eckart M E, Ewin A J, Finkbeiner F M, Kelley R, Kilbourne C A, Miniussi A R, Porter F S, Sadleir J E, Sakai K, Smith S J, Wakeham N, Wassell E, Yoon W, Morgan K M, Schmidt D R, Swetz D S, Ullom J N
Department of Physics, University of Wisconsin-Madison, 1150 University Avenue, Madison, WI 53706.
NASA Goddard Space Flight Center, 8800 Greenbelt Rd, Greenbelt, MD 20771.
IEEE Trans Appl Supercond. 2019 Aug;29(5). doi: 10.1109/TASC.2019.2899856. Epub 2019 Feb 18.
With the improving energy resolution of transitionedge sensor (TES) based microcalorimeters, performance verification and calibration of these detectors has become increasingly challenging, especially in the energy range below 1 keV where fluorescent atomic X-ray lines have linewidths that are wider than the detector energy resolution and require impractically high statistics to determine the gain and deconvolve the instrumental profile. Better behaved calibration sources such as grating monochromators are too cumbersome for space missions and are difficult to use in the lab. As an alternative, we are exploring the use of pulses of 3 eV optical photons delivered by an optical fiber to generate combs of known energies with known arrival times. Here, we discuss initial results of this technique obtained with 2 eV and 0.7 eV resolution X-ray microcalorimeters. With the 2 eV detector, we have achieved photon number resolution for pulses with mean photon number up to 133 (corresponding to 0.4 keV).
随着基于过渡边传感器(TES)的微热量计能量分辨率的提高,这些探测器的性能验证和校准变得越来越具有挑战性,特别是在低于1 keV的能量范围内,其中荧光原子X射线线的线宽比探测器能量分辨率宽,并且需要不切实际的高统计量来确定增益并解卷积仪器轮廓。对于太空任务来说,像光栅单色仪这样性能更好的校准源过于繁琐,并且在实验室中也难以使用。作为替代方案,我们正在探索使用由光纤传输的3 eV光学光子脉冲来生成具有已知到达时间的已知能量梳。在这里,我们讨论了使用2 eV和0.7 eV分辨率的X射线微热量计获得的该技术的初步结果。使用2 eV探测器,我们已经实现了对平均光子数高达133(对应于0.4 keV)的脉冲的光子数分辨率。