A programme of Astrophysics, Cosmology and Technology in Cardiff 2013-2016

卡迪夫天体物理学、宇宙学和技术项目 2013-2016

• 批准号: ST/K000926/1
• 负责人: Walter Kieran Gear
• 金额: $ 265.26万
• 依托单位: CARDIFF UNIVERSITY
• 依托单位国家: 英国
• 项目类别: Research Grant
• 财政年份: 2013
• 资助国家: 英国
• 起止时间: 2013 至 无数据
• 项目状态: 已结题
• 来源: https://gtr.ukri.org/projects?ref=ST%2FK000926%2F1
• 关键词: programme; Astrophysics; Cosmology; Technology; Cardiff

We propose a programme of Astrophysics, Cosmology and Technology development for Astrophysics and Cosmology, to investigate star and planet formation in our own and other galaxies, how galaxies form and evolve, and how the Universe we see around us today originated in the big bang. We will use our world-leading position in exploitation of the Herschel satellite galactic and extragalactic surveys, along with complemeantary observations with other facilities and theoretical modelling. We will also develop new sophisticated yet robust statistical methods for exploiting the large datasets emerging from the Planck satellite and other large cosmological surveys. We will continue to develop the world's most sensitive detectors for very long infrared wavelengths, along with associated optical components utilising 'metamaterials' the class of materials designed and manufactured by human beings to have the properties best suited to their task, rather than relying on naturally occurring minerals and plastics. Both of these areas of technology development have potential wide applications outside of Astronomy, in areas such as security scanners and bio-medical imaging for example. The technologies used for imaging can also be extended to undertake spectroscopy, and we propose a programme to develop the capability to obtain a spectrum of every point in a large area image of the sky, which is essential for understanding how far away the objects found in deep surveys are, but also what the conditions in the gas that make up these objects are.

我们提出了一个天体物理学，宇宙学和天体物理学和宇宙学技术发展的方案，以研究我们自己和其他星系中的星星和行星的形成，星系如何形成和演变，以及我们今天看到的宇宙如何起源于大爆炸。我们将利用我们的世界领先地位，利用赫歇尔卫星星系和河外星系调查，沿着与其他设施和理论建模的补充观测。我们还将开发新的复杂而强大的统计方法，用于利用普朗克卫星和其他大型宇宙学调查中出现的大型数据集。我们将继续开发世界上最灵敏的甚长红外波长探测器，并沿着利用“超材料”的相关光学元件，超材料是人类设计和制造的一类材料，具有最适合其任务的特性，而不是依赖于自然产生的矿物和塑料。这两个技术发展领域在天文学之外都有潜在的广泛应用，例如安全扫描仪和生物医学成像。用于成像的技术也可以扩展到光谱学，我们提出了一个方案，以发展获得大面积天空图像中每个点的光谱的能力，这对于了解在深度调查中发现的物体有多远以及组成这些物体的气体的条件是什么是必不可少的。

项目成果

Evidence for gravitational lensing of the cosmic microwave background polarization from cross-correlation with the cosmic infrared background.

• DOI: 10.1103/physrevlett.112.131302
• 发表时间: 2013-12
• 期刊: Physical review letters
• 影响因子: 8.6
• 作者: P. Ade;Y. Akiba;A. Anthony;K. Arnold;M. Atlas;D. Barron;D. Boettger;J. Borrill;C. Borys;S. Chapman;Y. Chinone;M. Dobbs;T. Elleflot;J. Errard;G. Fabbian;C. Feng;D. Flanigan;A. Gilbert;W. Grainger;N. Halverson;M. Hasegawa;K. Hattori;M. Hazumi;W. Holzapfel;Y. Hori;J. Howard;P. Hyland;Y. Inoue;G. Jaehnig;A. Jaffe;B. Keating;Z. Kermish;R. Keskitalo;T. Kisner;M. Le Jeune;A. Lee;E. Leitch;E. Linder;M. Lungu;F. Matsuda;T. Matsumura;X. Meng;N. Miller;H. Morii;S. Moyerman;M. Myers;M. Navaroli;H. Nishino;H. Paar;J. Peloton;D. Poletti;E. Quealy;G. Rebeiz;C. Reichardt;P. Richards;C. Ross;K. Rotermund;I. Schanning;D. Schenck;B. Sherwin;A. Shimizu;C. Shimmin;M. Shimon;Praweeen Siritanasak;G. Smecher;H. Spieler;N. Stebor;B. Steinbach;R. Stompor;A. Suzuki;S. Takakura;A. Tikhomirov;T. Tomaru;B. Wilson;A. Yadav;O. Zahn

BICEP2/KECK ARRAY. VII. MATRIX BASED E/B SEPARATION APPLIED TO BICEP2 AND THE KECK ARRAY

BICEP2/KECK 阵列。

• DOI: 10.3847/0004-637x/825/1/66
• 发表时间: 2016
• 期刊: The Astrophysical Journal
• 作者: Ade P

High resolution SZ observations at the IRAM 30-m telescope with NIKA

NIKA 使用 IRAM 30 米望远镜进行高分辨率 SZ 观测

• DOI: 10.48550/arxiv.1409.1137
• 发表时间: 2014
• 期刊: arXiv e-prints
• 作者: Adam R.

VizieR Online Data Catalog: NIKA maps of ClG J1226.9+3332 at 150 and 250GHz (Adam+, 2015)

VizieR 在线数据目录：ClG J1226.9 3332 在 150 和 250GHz 的 NIKA 地图（Adam，2015）

• DOI: 10.26093/cds/vizier.35760012
• 发表时间: 2015
• 期刊: VizieR Online Data Catalog
• 作者: Adam R. A.

First observation of the thermal Sunyaev-Zel'dovich effect with kinetic inductance detectors

首次用动感电感探测器观察热 Sunyaev-Zeldovich 效应

• DOI: 10.1051/0004-6361/201322902
• 发表时间: 2014
• 期刊: Astronomy & Astrophysics
• 影响因子: 6.5
• 作者: Adam R