Physical Properties of Strongly Lensed Quasars

强透镜类星体的物理特性

• 批准号: 2274471
• 金额: --
• 依托单位: University of Cambridge
• 依托单位国家: 英国
• 项目类别: Studentship
• 财政年份: 2019
• 资助国家: 英国
• 起止时间: 2019 至 无数据
• 项目状态: 已结题
• 来源: https://gtr.ukri.org/projects?ref=studentship-2274471
• 关键词: Physical; Properties; Strongly; Lensed; Quasars

It is challenging to study the host galaxies of quasars as they outshine their hosts.However, using the spectra from gravitationally lensed quasars givesus an insight into the properties of the host galaxy.Analysing high signal to noise spectra, from the NTT and ESI, of newlyconfirmed gravitationally lensed quasars and their host galaxies will allow usto gain a better understanding of the host galaxy-super massive black holerelationship.

研究类星体的宿主星系远远超过宿主是一项挑战。但是，使用重力镜头的类星体中的光谱使宿主星系的性质深入了解宿主的特性。Analysing高信号到噪声光谱，来自NTT和ESI的噪声光谱，OF NTT和ESI，OF的ESI，OF of of of ntt and Esi，新确认的重力镜头类星体及其宿主星系将使USTO可以更好地了解宿主星系，巨大的黑色全神贯位置。