竹内氏によるセミナー

日時
2017年3月28日(火) 15:00-16:00

登録不要・参加無料

場所
統計数理研究所 セミナー室2 (3F)
講演者
竹内 努 (名古屋大学)
演題
銀河の形成進化の統計的側面: 主にガスの物理から
Abstract
Studies on galaxy formation and evolution have just entered a new phase: some new generation observational facilities like James Webb Space Telescope (JWST), Thirty Meter Telescope (TMT), Atacama Large Millimeter / Submillimeter Array (ALMA), Square Kilometre Array (SKA), etc., and we expect a flood of data with unprecedented precision and amount.
We, then, should deeply consider how to deal with such datasets and to tackle physical problems without getting lost on the way of analysis.
I introduce the framework of currently accepted scenario for the galaxy formation and evolution, with a great emphasis on the gaseous side. On the way, I plan to discuss some statistical aspects of this issue, and point out some differences in the point of view of statisticians and physicists.