Follow‐up spectroscopic observations of HD 107148 B: A new white dwarf companion of an exoplanet host star

We report on our follow‐up spectroscopy of HD 1071478 B, a recently detected faint co‐moving companion of the exoplanet host star HD 107148 A. The companion is separated from its primary star by about 35″ (or 1790 AU of projected separation) and its optical and near infrared photometry is consistent with a white dwarf, located at the distance of HD 107148 A. In order to confirm the white dwarf nature of the co‐moving companion, we obtained follow‐up spectroscopic observations of HD 107148 B with CAFOS at the CAHA 2.2 m telescope. According to our CAFOS spectroscopy HD 107148 B is a DA white dwarf with an effective temperature in the range between 5900 and 6400K. The properties of HD 107148 B can further be constrained with the derived effective temperature and the known visual and infrared photometry of the companion, using evolutionary models of DA white dwarfs. We obtain for HD 107148 B a mass of 0.56 ± 0.05 M_⊙, a luminosity of (2.0 ± 0.2) × 10^–4 L_⊙, log g [cm s^–2]) = 7.95 ± 0.09, and a cooling age of 2100 ± 270 Myr. With its white dwarf companion the exoplanet host star HD 107148 A forms an evolved stellar system, which hosts at least one exoplanet. So far, only few of these evolved systems are known, which represent only about 5 % of all known exoplanet host multiple stellar systems. HD 107148 B is the second confirmed white dwarf companion of an exoplanet host star with a projected separation to its primary star of more than 1000 AU. (© 2016 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)     

基于抗差LM的视觉惯性里程计与伪卫星混合高精度室内定位

视觉惯性里程计（VIO）和伪卫星已经广泛应用于室内环境定位中,但在实际应用中,二者各自都有明显的缺陷。视觉里程计依赖于实际场景,在景深变化明显和光照不均匀的环境下会产生粗差,而且误差会不可避免地随着时间累积,但是在相邻帧间能保证相对高精度的位姿测量。由于受到室内多径的影响,伪卫星室内定位的精度和可靠性很难保证。为增加室内定位的可靠性和稳定性,基于抗差LM非线性优化理论,本文主要研究利用视觉惯性里程计的相邻帧间高精度位姿测量和伪卫星融合的室内高精度定位技术。该算法不仅可以抵抗粗差,而且可以减弱不同传感器间权重设置不合理带来的影响。最后使用在室内环境下搭建的高精度动态捕捉设备对组合定位方法进行实验验证。试验结果表明,该方法不依赖回环即可消除视觉惯性里程计的累积误差,有效提高室内定位精度及可靠性。利用改进的LM算法融合后场景1和场景2,相对于VIO单独定位精度分别提高了59.0%和77.5%。     

试论词汇学与心理学应用于大学英语词汇记忆的五种方法

从词汇学和心理学角度出发，分析了英语词汇的构成特征和英语学习者的记忆特点，探讨了将其综合应用于大学英语词汇记忆的5种方法。     

A coupled model for solid deformation and gas leak flow

From the viewpoint of interaction mechanics of solid and gas, a coupled mathematical model is presented for solid coal/rock‐mass deformation and gas leak flow in parallel deformable coal seams. Numerical solutions using the strong implicit procedure (SIP) method to the coupled mathematical model for double parallel coal seams are also developed in detail. Numerical simulations for the prediction of safety range using protection layer mining are performed with experimental data from a mine with potential danger of coal/gas outbursts. Analyses show that the numerical simulation results are consistent with the measured data on the spot. The coupled model shows a positive future for applications in a wide range of gas‐leak‐flow‐related problems in mining engineering, gas drainage engineering and mining safety engineering. Copyright © 2004 John Wiley & Sons, Ltd.     

Optical Observations of Meteors

Optical observations remain the most widely used method for studying meteors, even though they are limited by daylight and weather conditions. Visual observations have been used throughout history. They lack the precision of other methods, since they rely on the judgment of observers for trajectory information. However, since no special equipment is required, visual observations are widespread, and can give valuable information on the activity profile of showers. Photographic observations are much more precise. Rotating shutters allow velocities to be determined, and networks of cameras permit the height and trajectory of a meteor to be calculated. Except for the Super-Schmidt observations at Harvard, most photographic observations record only meteors brighter than 0 magnitude. Video observations, using image intensifiers, can record much fainter meteors down to +7 magnitude. Processing is becoming very automated, so that large quantities of data can be reduced relatively easily. Most video cameras have much lower precision than photographic cameras, but new technologies are changing this. Spectral observations of meteors, using video or photographic techniques, can be used to investigate the chemistry of meteoroids, while telescopic observations allow measurements to be extended to much fainter meteors (+10 or fainter).     

Triple and Multiple Systems

The triple systems display several interesting effects; and are also important for understanding the origin and evolution of binaries. Namely mutual inclination of two orbits, changes of observed inclination, and problems with the third light will be discussed in this contribution.     

多源矢量空间数据可用性评估的可视分析

本文将可视分析引入到多源矢量空间数据可用性评估中,为用户提供探索发现数据可用性的环境。在论证可行性的基础上,制定了多源矢量空间数据可用性评估可视分析应遵循的基本原则。在反映多源空间数据的同时,根据用户需求确定评估内容,触发相应模型计算并可视化表达,将用户需求、人脑认知通过交互界面和计算机算法模型相结合,允许用户按照自身需求了解不同数据的各种信息,帮助用户发现隐藏在数据中的知识,进而制定科学合理的数据使用方案。     

A direct imaging search for close stellar and sub‐stellar companions to young nearby stars

A total of 28 young nearby stars (ages ≤60 Myr) have been observed in the K_s‐band with the adaptive optics imager Naos‐Conica of the Very Large Telescope at the Paranal Observatory in Chile. Among the targets are ten visual binaries and one triple system at distances between 10 and 130 pc, all previously known. During a first observing epoch a total of 20 faint stellar or sub‐stellar companion‐candidates were detected around seven of the targets. These fields, as well as most of the stellar binaries, were re‐observed with the same instrument during a second epoch, about one year later. We present the astrometric observations of all binaries. Their analysis revealed that all stellar binaries are co‐moving. In two cases (HD 119022 AB and FG Aqr B/C) indications for significant orbital motions were found. However, all sub‐stellar companion candidates turned out to be non‐moving background objects except PZ Tel which is part of this project but whose results were published elsewhere. Detection limits were determined for all targets, and limiting masses were derived adopting three different age values; they turn out to be less than 10 Jupiter masses in most cases, well below the brown dwarf mass range. The fraction of stellar multiplicity and of the sub‐stellar companion occurrence in the star forming regions in Chamaeleon are compared to the statistics of our search, and possible reasons for the observed differences are discussed. (© 2015 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)     

鱼类视蛋白的研究进展

鱼类作为脊椎动物最重要的类群之一, 在其生长发育和进化中, 视蛋白在视觉图像形成和 生物钟昼夜节律等非图像形成功能调节方面起着至关重要的作用, 根据其是否直接参与视觉成像分 视觉视蛋白和非视觉视蛋白两大类。本文对国内外鱼类视蛋白生物学的最新研究进展进行了综述, 重点介绍鱼类视觉系统视蛋白和非视觉系统视蛋白的研究进展, 包括各自的组成、分类、分布、生 理功能及视蛋白基因等, 为进一步深入研究鱼类视觉感知的分子机制及鱼类资源的保护及应用奠定 理论基础。     

一种基于视觉特征的多分辨率快速图像融合方法

以红外与可见光图像融合为例,提出了一种基于图像视觉特征相关量值的多分辨率快速图像融合方法.该方法先利用CDF9/7小波将输入图像进行提升分解,然后在对分解后的小波系数矩阵采用视觉特征进行融合处理,最后通过提升逆变换得到重构图像.实验表明该方法即使在图像信噪比较低的情况下,仍能得到较好的熵、边缘及较高分辨率的效果,且执行效率高.