The Art of Measuring Physical Parameters in Galaxies

NSF支持将于2018年4月10日至13日在加州大学滨江棕榈沙漠会议中心举行的“Galerkin中测量物理参数的艺术”研讨会。这次研讨会建立在成功的宇宙大会近红外深河外遗留物调查（CANDELS）项目的基础上，并将其扩展。该奖项将帮助支持20名年轻天文学家和少数群体成员的出席。 现在有一个广泛的光度和光谱数据集可用于CANDELS星系，驱动需要测量其相关的物理参数。研讨会的目的是汇集该领域的领导人，讨论和确定使用从X射线到无线电波长的组合数据测量这些参数的最佳方法，讨论最先进的科学，该奖项反映了NSF的法定使命，并被认为是值得通过使用评估来支持的。基金会的学术价值和更广泛的影响审查标准。

NSF support is provided for a workshop on "The Art of Measuring Physical Parameters in Galaxies" to be held during April 10-13th 2018 at the Palm Desert conference center of the University of California, Riverside. This workshop builds upon and extends the successful Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey (CANDELS) project. The award will help support attendance of 20 younger astronomers and members of the minority groups. There is now an extensive photometric and spectroscopic dataset available for CANDELS galaxies, driving a need to measure their associated physical parameters. The aim of the workshop is to bring together leaders in the field to discuss and identify the optimum ways to measure these parameters using the combined data from X-ray to radio wavelengths, to discuss the state-of-the-art science, and to identify the outstanding and fundamental projects that are only possible by exploiting such data.This award reflects NSF's statutory mission and has been deemed worthy of support through evaluation using the Foundation's intellectual merit and broader impacts review criteria.