Densely Sampling the High Redshift Universe

对高红移宇宙进行密集采样

• 批准号: 0908805
• 负责人: Charles Steidel
• 金额: $ 55.71万
• 依托单位: California Institute of Technology
• 依托单位国家: 美国
• 项目类别: Standard Grant
• 财政年份: 2009
• 资助国家: 美国
• 起止时间: 2009-09-01 至 2013-08-31
• 项目状态: 已结题
• 来源: https://www.nsf.gov/awardsearch/showAward?AWD_ID=0908805&HistoricalAwards=false
• 关键词: Densely; Sampling; Redshift; Universe

This award is funded under the American Recovery and Reinvestment Act of 2009 (Public Law 111-5).Dr Steidel will make a detailed study of the galaxies and gas within a few million light years of bright quasars that we observe as they were 10 billion years ago. Using the Keck telescopes, he will take high-resolution optical and near-infrared spectra to measure the absorption lines of gas lying between us and the quasar. These spectra will target lines of highly ionized oxygen to trace warm and hot gas, Lyman-beta to measure neutral hydrogen, and additional lines that probe the chemical abundance and physical conditions in the gas. These observations will be compared with theoretical models for the effect that active galactic nuclei such as quasars should have on their surroundings. Deep optical and near-infrared images will be taken to pick out galaxies likely to lie close to the quasar. Optical and infrared spectra of these objects should yield accurate redshifts (and hence distances), dynamical masses and chemical abundances for about 150 galaxies around each quasar. The infrared spectroscopy should be particularly effective when the galaxies are partially obscured by dust. Two or three graduate students will be trained as they participate in the research. Both the published results and primary data will be made available as soon as possible to the astronomical community. Dr Steidel is Project Scientist for the MOSFIRE imaging spectrograph (Multi-Object Spectrometer for InfraRed Exploration); this new instrument will serve the Keck Observatory's large user community.

该奖项是根据2009年美国复苏和再投资法案（公法111-5）资助的。Steidel博士将对我们观察到的100亿年前明亮类星体数百万光年内的星系和气体进行详细研究。 利用凯克望远镜，他将获得高分辨率的光学和近红外光谱，以测量位于我们和类星体之间的气体的吸收线。 这些光谱将以高度电离的氧线为目标，以跟踪温暖和炎热的气体，莱曼-β测量中性氢，以及探测气体中化学丰度和物理条件的其他线。 这些观测结果将与理论模型进行比较，以确定活动星系核（如类星体）对其周围环境的影响。 将拍摄深层光学和近红外图像，以挑选出可能靠近类星体的星系。 这些物体的光学和红外光谱应该可以提供精确的红移（以及距离），动力学质量和化学丰度，每个类星体周围大约有150个星系。 当星系部分被尘埃遮蔽时，红外光谱应该特别有效。 两三名研究生将在参与研究时接受培训。 公布的结果和原始数据将尽快提供给天文学界。 Steidel博士是MOSFIRE成像光谱仪（用于红外探测的多目标光谱仪）的项目科学家;这种新仪器将为凯克天文台的大型用户社区服务。