Growth of Black Holes and Their Host Spheroids in （Sub）mm-loud High-Redshift QSOs

We study the growth of black holes and stellar population in spheroids at high redshift using several （sub）mm-loud QSO samples. Applying the same criteria established in an earlier work, we find that, similar to IR QSOs at low redshift, the far-infrared emission of these （sub）mm-loud QSOs mainly originates from dust heated by starbursts. By combining low-z IR QSOs and high-z （sub）mm-loud QSOs, we find a trend that the star formation rate （M＊） increases with the accretion rate （Mace）. We compare the values of M＊/Macc for submm emitting galaxies （SMGs）, far-infrared ultraluminous/hypeduminous QSOs and typical QSOs, and construct a likely evolution scenario for these objects. The （sub）mm-loud QSO transition phase has both high Macc and M＊ and hence is important for establishing the correlation between the masses of black holes and spheroids.     

A GRB Follow-up System at the Xinglong Observatory and Detection of the High-Redshift GRB 060927

A gamma-ray burst (GRB) optical photometric follow-up system at the Xinglong Observatory of National Astronomical Observatories of China (NAOC) has been constructed. It uses the 0.8-m Tsinghua-NAOC Telescope (TNT) and the 1-m EST telescope, and can au-tomatically respond to GRB Coordinates Network (GCN) alerts. Both telescopes slew rela-tively fast, being able to point to a new target field within ～ 1 min upon a request. Whenever available, the 2.16-m NAOC telescope is also used. In 2006 the system responded to 15 GRBs and detected seven early afterglows. In 2007 six GRBs have been detected among 18 follow-up observations. TNT observations of the second most distant GRB 060927 (z = 5.5) are shown, which started as early as 91 s after the GRB trigger. The afterglow was detected in the combined image of the first 19 × 20 s unfiltered exposures. This GRB follow-up system has joined the East-Asia GRB Follow-up Observation Network (EAFON).     

星系的红移

红移（redshift）对于天文爱好者来说是一个非常熟悉的概念了。根据多普勒效应,波源朝向观察者运动时,光谱会向短波端移动,叫做紫移（blueshift）;反之,当波源背向观察者运动时,光谱就会移向长波端,产生红移（redshift）。     

新疆阿尔泰山南缘红墩SEDEX型铅锌矿的成矿模式

克兰裂谷盆地位于新疆阿尔泰山南缘的中部,其沉积构造演化经历了三个阶段：早期酸性火山-沉积阶段;中期基性火山-沉积阶段;晚期碎屑沉积阶段。红墩铅锌矿床形成于盆地中期基性火山-沉积阶段的被动陆缘裂谷构造环境,具有SEDEX型铅锌矿床的地质特征,找矿潜力大。     

腹腔注射恩诺沙星和氟苯尼考对红笛鲷血清IgM含量的影响

以20mg·kg-1恩诺沙星和氟苯尼考分别腹腔注射红笛鲷,通过间接酶联免疫吸附实验法(ELISA)测定红笛鲷血清IgM的含量,研究恩诺沙星与氟苯尼考对红笛鲷血清IgM含量的影响。结果显示:健康红笛鲷血清中IgM抗体的含量为3.591±0.314mg·mL-1,注射后,恩诺沙星组增加至4.234±0.013mg·mL-1,第3周后恢复至初始水平,而氟苯尼考组则降低至2.538±0.214mg·mL-1,第5周仍未恢复至初始水平。可见,恩诺沙星可提高红笛鲷血清中抗体IgM的含量,而氟苯尼考则降低鱼体血清中抗体IgM的含量,且影响时间也较长。     

对相对论束模型的一种分类及相应的统计检验方法

本根据视横向速度是否红移依赖对相对论束模型进行分类并提出对相应模型进行统计检验的方法，作为应用的例子，本利用前人献所给视超光速样本进行统计分析，并对有关结果进行了讨论。     

4株海洋红球菌产类胡萝卜素分析及其全基因组测序

以源于东太平洋海水的4株红球菌分离菌Rhodococcussp. EPR-134、Rhodococcus sp. EPR-147、Rhodococcus sp. EPR-157和Rhodococcus sp. EPR-279为研究对象,开展了菌株的色素提取和色素全波长扫描,并基于全基因组测序分析了4株细菌类胡萝卜素代谢通路中的相关基因。色素全波长扫描结果显示,菌株EPR-134不具备类胡萝卜素产生能力,而其它3株红球菌能够产生类胡萝卜素,且所产类胡萝卜素组分不同。基因组分析表明,4个细菌基因组中存在较为完整的促使类胡萝卜素形成的基因簇。对菌株参与番茄红素形成的3个关键基因crt E、crt B和crt I的氨基酸序列同源性两两比对分析表明,菌株EPR-134 3个基因氨基酸序列与其它3个菌株相应基因氨基酸序列同源性最低,这可能是导致该菌株不产类胡萝卜素的关键原因。该研究结果为产类胡萝卜素红球菌的遗传改造,以及为产类胡萝卜素工程菌的构建奠定了前期基础。     

东营凹陷南斜坡沙四段高频沉积旋回对滩坝砂体的沉积控制作用

在东营凹陷南斜坡的沙四段地层中,常发育典型的湖相滩坝砂体沉积.详细观察表明,这些滩坝砂体在垂向上常发育较为对称的高频基准面上升半旋回和下降半旋回,且对滩坝砂体的沉积过程有明显的控制作用.通过测井曲线的频谱分析,高频基准面的变化与米兰柯维奇轨道气候周期有着密切的关系,而单砂体规模的滩坝砂体在平面展布上又有着明显的对称性.这些都表明滩坝砂体主要沉积在湖平面升降转换的相对稳定期,同生断层活动产生的陡坎或隆起会有助于滩坝砂体的富集.可根据滩坝砂体的垂向沉积序列和组合方式来判断滩坝主体的分布位置.