SnowCluster 2015: The Art of Galaxy Cluster Mass Measurement

SnowCluster 2015：星系团质量测量的艺术

• 批准号: 1463660
• 负责人: David Kieda
• 金额: $ 2.05万
• 依托单位: University of Utah
• 依托单位国家: 美国
• 项目类别: Standard Grant
• 财政年份: 2015
• 资助国家: 美国
• 起止时间: 2015-01-15 至 2015-12-31
• 项目状态: 已结题
• 来源: https://www.nsf.gov/awardsearch/showAward?AWD_ID=1463660&HistoricalAwards=false
• 关键词: SnowCluster; 2015; Art; Galaxy; Cluster

Clusters of galaxies are sensitive cosmological probes which can be used to study large-scale structure formation, the physics of diffuse astrophysical plasmas, and dark matter on megaparsec scales. A better understanding is needed of cluster masses, which rely critically on knowledge of cluster astrophysics, as well as biases and limitations of various measurement methods. This conference provides the opportunity for the astrophysical community to critically examine how all mass estimators can be combined for maximum accuracy in galaxy cluster mass estimation.This workshop will be an excellent opportunity for young astrophysicists to gain information and for them to interact with more experienced researchers in an informal setting. The Scientific Organizing Committee has taken care to include key representatives from underrepresented groups in the invitation list.

星系团是敏感的宇宙学探测器，可用于研究大尺度结构的形成、弥散天体物理等离子体的物理学以及兆秒差距尺度上的暗物质。 需要更好地了解星团质量，这主要依赖于星团天体物理学知识，以及各种测量方法的偏差和局限性。这次会议为天体物理学界提供了机会，批判性地研究如何组合所有质量估计器，以实现星系团质量估计的最大精度。本次研讨会将为年轻的天体物理学家提供获取信息并与更有经验的研究人员互动的绝佳机会在非正式场合。科学组委会已注意将代表性不足群体的主要代表纳入邀请名单中。