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Lancaster University Observational Astrophysics 2018-2021

兰卡斯特大学观测天体物理学 2018-2021

基本信息

批准号：
ST/R000514/1
负责人：
Isobel Mary Hook
金额：
$ 29.48万
依托单位：
Lancaster University
依托单位国家：
英国
项目类别：
Research Grant
财政年份：
2018
资助国家：
英国
起止时间：
2018 至无数据
项目状态：
已结题

来源：
https://gtr.ukri.org/projects?ref=ST%2FR000514%2F1
关键词：
Lancaster University Observational Astrophysics 2018

项目摘要

The work proposed here tackles some of the most important open questions in astrophysics, broadly centred on understanding the formation and evolution of galaxies and the properties of the Universe itself. It is closely linked with the STFC Science Roadmap challenges pertaining to the roles and nature of dark matter and dark energy, the formation of the first stars and galaxies in the Universe and the still unsolved key question of how galaxies evolve. In order to address such fundamental questions, we use complementary approaches involving observation and modeling of the most distant and relatively nearby systems. We will shed light on the properties of nearby, faint dwarf galaxies by searching for traces of gas absorption in background quasar spectra. Looking further back in cosmic time, we will uncover the properties of thousands of "cosmic noon" galaxies, also along the lines-of-sight to distant QSOs, in order to explain the link between their star formation and the gas that fuels it. We will obtain a new sample of very distant galaxies using unique wide-area surveys, which provide the bright targets needed for detailed study of their physical properties. Finally, we will use Type Ia supernovae to study the evolution of the universe itself, making fundamental tests of the constancy of dark energy in time, and preparing for tests of spatial variation.Our research involves making state-of-the-art observations using the world's most powerful and advanced telescopes such as the Hubble Space Telescope and facilities run by the European Southern Observatory including ALMA (the Atacama Large Millimeter Array) and the VLT (Very Large Telescope). At the same time the group is involved in the scientific planning for several new telescopes and instruments that will come online in the next 10 years and that will revolutionise research in astrophysics. These include the 4-m Multi-Object Spectroscopic Telescope (4MOST), the Large Synoptic Survey Telescope (LSST), the European Extremely Large Telescope (E-ELT) and in space the James Webb Space Telescope (JWST) and the European Space Agency's Euclid mission.

这里提出的工作解决了天体物理学中一些最重要的开放问题，主要集中在理解星系的形成和演化以及宇宙本身的特性。它与STFC科学路线图的挑战密切相关，这些挑战涉及暗物质和暗能量的作用和性质，宇宙中第一批恒星和星系的形成以及星系如何演化这一尚未解决的关键问题。为了解决这些基本问题，我们使用互补的方法，包括对最远和相对较近的系统进行观察和建模。我们将通过在背景类星体光谱中寻找气体吸收的痕迹来揭示附近微弱的矮星系的特性。回顾宇宙时间，我们将发现数千个“宇宙正午”星系的特性，也沿着遥远qso的视线，以解释它们的恒星形成和燃料气体之间的联系。我们将通过独特的广域巡天获得非常遥远星系的新样本，这为详细研究它们的物理特性提供了所需的明亮目标。最后，我们将利用Ia型超新星来研究宇宙本身的演化，对暗能量在时间上的恒常性进行基础测试，并为空间变异测试做准备。我们的研究包括使用世界上最强大和最先进的望远镜进行最先进的观测，如哈勃太空望远镜和欧洲南方天文台运行的设施，包括ALMA（阿塔卡马大型毫米波阵列）和VLT（甚大望远镜）。与此同时，该小组还参与了几架新望远镜和仪器的科学规划，这些望远镜和仪器将在未来10年内上线，这将彻底改变天体物理学的研究。其中包括4米多目标光谱望远镜（4MOST）、大型综合巡天望远镜（LSST）、欧洲超大望远镜（E-ELT）和詹姆斯·韦伯太空望远镜（JWST）以及欧洲航天局的欧几里得任务。

项目成果

期刊论文数量（10）

专著数量（0）

科研奖励数量（0）

会议论文数量（0）

专利数量（0）

Quasar Sightline and Galaxy Evolution (QSAGE) survey – I. The galaxy environment of O vi absorbers up to z = 1.4 around PKS 0232−04

类星体视线和星系演化 (QSAGE) 调查 – I. PKS 0232−04 周围 z = 1.4 范围内 O vi 吸收体的星系环境

DOI：
发表时间：
2018
期刊：
Monthly notices of the Royal Astronomical Society
影响因子：
4.8
作者：
R. Bielby;J. Stott;F. Cullen;T. Tripp;J. Burchett;M. Fumagalli;S. Morris;N. Tejos;R. Crain;R. Bower;J. Prochaska
通讯作者：
J. Prochaska

The ESO’s VLT type Ia supernova spectral set of the final two years of SNLS

DOI：
10.1051/0004-6361/201731924
发表时间：
2017-12
期刊：
Astronomy & Astrophysics
影响因子：
6.5
作者：
C. Balland;F. Cellier-Holzem;C. Lidman;P. Astier;M. Betoule;R. Carlberg;A. Conley;R. Ellis;R. Ellis;J. Guy;D. Hardin;I. Hook;I. Hook;D. Howell;D. Howell;R. Pain;C. Pritchet;N. Regnault;M. Sullivan;V. Arsenijević;S. Baumont;P. El-Hage;S. Fabbro;D. Fouchez;A. Mitra;A. Moller;A. Mourão;J. Neveu;M. Roman;V. Ruhlmann-Kleider
通讯作者：
C. Balland;F. Cellier-Holzem;C. Lidman;P. Astier;M. Betoule;R. Carlberg;A. Conley;R. Ellis;R. Ellis;J. Guy;D. Hardin;I. Hook;I. Hook;D. Howell;D. Howell;R. Pain;C. Pritchet;N. Regnault;M. Sullivan;V. Arsenijević;S. Baumont;P. El-Hage;S. Fabbro;D. Fouchez;A. Mitra;A. Moller;A. Mourão;J. Neveu;M. Roman;V. Ruhlmann-Kleider

Optimizing a magnitude-limited spectroscopic training sample for photometric classification of supernovae