The obscuration by dust of most of the growth of supermassive black holes

Supermassive black holes underwent periods of exponential growth during which we see them as quasars in the distant Universe. The summed emission from these quasars generates the cosmic X-ray background, the spectrum of which has been used to argue that most black-hole growth is obscured. There are clear examples of obscured black-hole growth in the form of 'type-2' quasars, but their numbers are fewer than expected from modelling of the X-ray background. Here we report the direct detection of a population of distant type-2 quasars, which is at least comparable in size to the well-known unobscured type-1 population. We selected objects that have mid-infrared and radio emissions characteristic of quasars, but which are faint at near-infrared and optical wavelengths. We conclude that this population is responsible for most of the black-hole growth in the young Universe and that, throughout cosmic history, black-hole growth occurs in the dusty, gas-rich centres of active galaxies.     

Evolutionary information for specifying a protein fold

Classical studies show that for many proteins, the information required for specifying the tertiary structure is contained in the amino acid sequence. Here, we attempt to define the sequence rules for specifying a protein fold by computationally creating artificial protein sequences using only statistical information encoded in a multiple sequence alignment and no tertiary structure information. Experimental testing of libraries of artificial WW domain sequences shows that a simple statistical energy function capturing coevolution between amino acid residues is necessary and sufficient to specify sequences that fold into native structures. The artificial proteins show thermodynamic stabilities similar to natural WW domains, and structure determination of one artificial protein shows excellent agreement with the WW fold at atomic resolution. The relative simplicity of the information used for creating sequences suggests a marked reduction to the potential complexity of the protein-folding problem.     

立体投影光学引擎的研究

立体投影显示是三维(3D)显示中较成熟的一种技术,应用前景广阔。文中介绍了立体投影显示技术的光学引擎成像原理,阐述了DLP(digital light processing),LCD(liquid crystal display)和LCoS(liquid crystal on silicon)3大类立体投影光学引擎结构的特点,分析了影响立体效果的原因并提出了改善方法,最后对各种立体投影显示技术做了性能评价和应用展望。     

单个大气超细颗粒物源特征的同步辐射光源X射线探针初步研究

研究了单个大气超细颗粒分析靶样的制备方法, 在美国阿贡国家实验室APS同步光源的13-ID-C试验站, 用束斑为2 μm的X射线探针分析了不同污染源超细颗粒物, 得到了单个超细颗粒物的特征X射线谱. 实验结果表明, 来自不同污染源的超细单颗粒具有不同的特征X射线能谱. 这为单颗粒分析方法识别大气超细颗粒物来源提供了依据. 超细含铅颗粒物的分析暗示, 大气颗粒物中的铅污染是多源的, 除燃烧加铅汽油外, 燃煤和钢铁工业也是大气铅污染的排放源. 来自燃煤排放的超细颗粒分析提示, 燃煤超细颗粒物对人体健康具有更大的潜在危害.     

An analysis of patient register data in the Longitudinal Study - what does it tell us about the quality of the data?

This article uses data for members of the ONS Longitudinal Study (LS) from both Census 2001 enumeration and patient registrations "frozen" on census day 2001 from the National Health Service Central Register (NHSCR) to examine potential sources of difference in area of usual residence.Overall 95.7 per cent of ONS LS members enumerated at census resided in the same area as recorded on the NHSCR data. Where areas differed, or the ONS LS member was not on the NHSCR on census day, subsequent NHSCR records were examined. Records flagged on the NHSCR as ONS LS members in England and Wales on census day but with no census record were also investigated.     

混合式可重构数字多核并行处理器平台

一种高性能、RISC-VLIW融合的多核、可重构数字媒体处理器已经从专利发明顺利形成了一个先进的数据处理器设计平台(Digital Multi-processor Platform)。研发的结果体现若干先进处理器技术的融合。(1)应用:低功耗并行运算处理覆盖数字信号处理(DSP)、数字媒体处理(DMP)和超级并行处理器(SPP)的应用扩展领域;(2)体系结构:精简指令(RISC)和超常指令字(VLIW)处理器融合于同一个可配置的平台;(3)运算能力:处理器群调用异构的通用处理器核,使用两类处理器核实例:通用处理器核(包括ALU等的通用运算)和专用处理器核(包括DDCU的用户自定义运算核);(4)可配置和可重构:硅编译器、SoC集成工具、用户自定义运算单元、多核间的和槽内的流水线、包括运算单元的现场编程;(5)设计自动化平台:专用工具用于设计、分析与验证;与商业电子自动化设计(EDA)流程接口;(6)产品模式:硅知识产权(Silicon IP)、通用处理器芯片系列(IC Series)、定制单片系统(SoC)。命名为Fusion的融合式数字多核处理器平台把数个先进处理器技术集成到一个统一的体系结构和设计环境之中...     

Jovian-like aurorae on Saturn

Planetary aurorae are formed by energetic charged particles streaming along the planet's magnetic field lines into the upper atmosphere from the surrounding space environment. Earth's main auroral oval is formed through interactions with the solar wind, whereas that at Jupiter is formed through interactions with plasma from the moon Io inside its magnetic field (although other processes form aurorae at both planets). At Saturn, only the main auroral oval has previously been observed and there remains much debate over its origin. Here we report the discovery of a secondary oval at Saturn that is approximately 25 per cent as bright as the main oval, and we show this to be caused by interaction with the middle magnetosphere around the planet. This is a weak equivalent of Jupiter's main oval, its relative dimness being due to the lack of as large a source of ions as Jupiter's volcanic moon Io. This result suggests that differences seen in the auroral emissions from Saturn and Jupiter are due to scaling differences in the conditions at each of these two planets, whereas the underlying formation processes are the same.