A Programme of Astrophysics, Cosmology and Technology in Cardiff 2016-19

卡迪夫天体物理学、宇宙学和技术项目 2016-19

• 批准号: ST/N000706/1
• 负责人: Walter Kieran Gear
• 金额: $ 407.6万
• 依托单位: CARDIFF UNIVERSITY
• 依托单位国家: 英国
• 项目类别: Research Grant
• 财政年份: 2016
• 资助国家: 英国
• 起止时间: 2016 至 无数据
• 项目状态: 已结题
• 来源: https://gtr.ukri.org/projects?ref=ST%2FN000706%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, and how galaxies form and evolve. This programme will combine observational data from world-class ground and space-based observatories, as well as theoretical modelling and simulations of the processes that result in the Universe we observe around us. We will also 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 potentially have 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的技术发展计划，以研究我们自己和其他星系中恒星和行星的形成，以及星系的形成和演化。该方案将结合来自世界级地面和天基观测站的观测数据，以及对导致我们观察到的周围宇宙的过程的理论建模和模拟。我们还将继续开发世界上最灵敏的用于超长红外波长的探测器，以及相关的光学部件，这些部件利用由人类设计和制造的材料类别，具有最适合他们的任务的性能，而不是依赖于自然产生的矿物和塑料。这两个技术开发领域在天文学之外都有潜在的广泛应用，例如在安全扫描仪和生物医学成像等领域。用于成像的技术还可以扩展到进行光谱分析，我们提出了一项计划，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中的条件是至关重要的。

项目成果

The NIKA2 large-field-of-view millimetre continuum camera for the 30 m IRAM telescope

• DOI: 10.1051/0004-6361/201731503
• 发表时间: 2017-07
• 期刊: Astronomy and Astrophysics
• 影响因子: 6.5
• 作者: R. Adam;A. Adane;P. Ade;P. Andr'e;A. Andrianasolo;H. Aussel;A. Beelen;A. Benoȋt;A. Bideaud;N. Billot;O. Bourrion;A. Bracco;M. Calvo;A. Catalano;G. Coiffard;B. Comis;M. Petris;F. D'esert;S. Doyle;E. Driessen;R. Evans;J. Goupy;C. Kramer;G. Lagache;S. Leclercq;J. Leggeri;J. Lestrade;J. Macías-Pérez;P. Mauskopf;F. Mayet;A. Maury;A. Monfardini;S. Navarro;E. Pascale;L. Perotto;G. Pisano;N. Ponthieu;V. Révéret;A. Rigby;A. Ritacco;C. Romero;H. Roussel;F. Ruppin;K. Schuster;A. Sievers;S. Triqueneaux;C. Tucker;R. Zylka

Mapping the hot gas temperature in galaxy clusters using X-ray and Sunyaev-Zel'dovich imaging

使用 X 射线和 Sunyaev-Zeldovich 成像绘制星系团中的热气体温度

• DOI: 10.1051/0004-6361/201629810
• 发表时间: 2017
• 期刊: Astronomy & Astrophysics
• 影响因子: 6.5
• 作者: Adam R

Substructure and merger detection in resolved NIKA Sunyaev-Zel'dovich images of distant clusters

遥远星团解析 NIKA Sunyaev-Zeldovich 图像中的子结构和合并检测

• DOI: 10.1051/0004-6361/201731950
• 发表时间: 2018
• 期刊: Astronomy & Astrophysics
• 影响因子: 6.5
• 作者: Adam R

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

BICEP2 / Keck Array IX: New bounds on anisotropies of CMB polarization rotation and implications for axionlike particles and primordial magnetic fields

• DOI: 10.1103/physrevd.96.102003
• 发表时间: 2017-05
• 期刊: Physical Review D
• 影响因子: 5
• 作者: Keck Array;BICEP2 Collaborations P. A. R. Ade;Z. Ahmed;R. Aikin;K. Alexander;D. Barkats;S. Benton;C. Bischoff;J. Bock;R. Bowens-Rubin;J. Brevik;I. Buder;E. Bullock;V. Buza;J. Connors;B. Crill;L. Duband;C. Dvorkin;J. Filippini;S. Fliescher;T. S. Germaine;T. Ghosh;J. Grayson;S. Harrison;S. Hildebrandt;G. Hilton;H. Hui;K. Irwin;J. Kang;K. Karkare;E. Karpel;J. Kaufman;B. Keating;S. Kefeli;S. Kernasovskiy;J. Kovac;C. Kuo;N. Larsen;E. Leitch;K. Megerian;L. Moncelsi;T. Namikawa;C. Netterfield;H. Nguyen;R. O’Brient;IV R.W.Ogburn;C. Pryke;S. Richter;A. Schillaci;R. Schwarz;C. Sheehy;Z. Staniszewski;B. Steinbach;R. Sudiwala;G. Teply;K. Thompson;J. Tolan;C. Tucker;A. Turner;A. Vieregg;A. Weber;D. Wiebe;J. Willmert;C. L. Wong;W. L. K. Wu;K. Yoon