RUI: Parameter Estimation, Data Analysis, and Detector Characterization for LIGO

激光干涉引力波天文台（LIGO）现在达到了目标灵敏度。包括卡尔顿学院在内的许多机构的研究人员正在积极分析数据，以寻找引力辐射事件。任何时候都可能出现初步检测。LIGO观测到的所有事件都将产生丰富的天体物理信息。卡尔顿大学的教师和学生将运行他们的信号搜索程序。此外，卡尔顿大学的研究小组将在研究环境噪声（如地震活动）如何破坏搜索方面发挥重要作用。卡尔顿学院是培养未来科学家的领导者。该项目为对物理和统计感兴趣的学生提供了研究机会，并有助于培养他们成为下一代科学家。LIGO预期的令人兴奋和戏剧性的结果刺激了学生，并吸引他们进入科学世界。卡尔顿的学生渴望参与令人兴奋的研究，他们对重力波天文学的兴趣很大。卡尔顿小组和合作者开发的统计方法也将在物理学的其他领域产生重大影响。

The Laser Interferometric Gravitational-Wave Observatory (LIGO) is now at its target sensitivity. Researchers at a number of institutions, including Carleton College, are vigorously analyzing the data in search of gravitational radiation events. An initial detection could come at any time. All events seen by LIGO will produce a wealth of astrophysical information. Faculty and students at Carleton will be running their signal search programs. In addition, the Carleton team will play asignificant role in finding how noise from the environment (such as seismic activity) can corrupt the search.Carleton College is a leader in producing future scientists. This project provides research opportunities to motivated students with interests in physics and statistics, and helps to train them to become the next generation of scientists. The exciting and dramatic results expected by LIGO stimulate students, and attract them to the world of science. Carleton students are eager to participate in exciting research, and their interest in gravity wave astronomy is large. The statistical methods developed by the Carleton group and collaborators will also have a significant influence in other areas of physics.