Terrestrial Planets in the era of PLATO

重新评估开普勒深场中的类地行星和评估PLATO对它们重新观测的能力。这包括使用开普勒输入目录中有关主星的数据，并与盖亚的结果进行更新，然后重新评估主星的特性及其对行星特性的影响。需要使用PLATO仿真工具对结果进行仿真。此外，我们想给学生的项目一个观测元素，所以我们设计了一个额外的组件，使用望远镜专门用于高速观测，以便通过微透镜特征在球状星团的光晕中搜索小行星（正如HST观测所暗示的那样）。这一特性对博士生的经历很有帮助。

Reassessment of the terrestrial planets in the Kepler deep field and assessment of the capabilities of PLATO for their re-observation. This involves using data from the Kepler Input Catalogue for the relevant host stars and updating with Gaia results and then reassessing the host properties and their implication on the planetary properties. Simulation of the results using the PLATO simulation tool is needed.In addition we want to give the student an observational element to their project so have devised an extra component using a telescope dedicated to high speed observations in order to search for small planets in the halo's of globular clusters through their microlensing signature (as has been hinted at by HST observations). This properties plays into the hands of the experience of the PhD Student.