Investigating variable stars in the open cluster NGC 1912 and its surrounding field     

李春燕  艾力·伊沙木丁  张余  宋芳芳  曾祥云  陈力  牛虎彪  白建银  刘军辉 《天文和天体物理学研究(英文版)》2021,(3):167-183

In this work,we studied the variable stars in the open cluster NGC 1912 based on the photometric observations and Gaia DR2 data.More than 3600 CCD frames in B,V,R filters were reduced,and we obtained the light curves that span about 63 hours.By analyzing these light curves,we detected 24 variable stars,including 16 periodic variable stars,seven eclipsing binaries and one star whose type is unclear.Among these 24 variable stars,11 are newly discovered,which are classified as sixγDoradus stars,oneδScuti star,three detached binaries and one contact binary.We also confirmed 13 previously known variable stars.Based on cluster members identified by Cantat-Gaudin et al.(2018),we inferred cluster memberships for these detected variable stars.Using Gaia DR2 data,we plotted a new color-magnitude diagram for NGC1912,and showed the nature of variable cluster members in kinematical properties and heliocentric distance.Among the 24 variable stars,seven variables are probable cluster members,which show homogeneity in kinematic characters and space position with the established cluster members.Four of the seven variable cluster members are the previously discovered stars,consisting of twoγDor stars and twoδSct stars.The remaining three variable cluster members,which are allγDor stars,are firstly detected in this work.The main physical parameters of these variable cluster members estimated from the color-magnitude diagram are log(age/yr)=8.75,[Fe/H]=-0.1,m-M=10.03 mag,and E(B-V)=0.307.  相似文献   

基于NPSVM模型的超新星识别方法          下载免费PDF全文

王精东  陈星星  梁吴颖  黄泽锋  全少武  沈锦泫  石雄辉 《天文学报》2021,62(2):15-53

巡天观测与高能物理、黑洞天文等领域均有密切的联系.基于星系-超新星二分类问题,研究光谱数据预处理,结合余弦相似度改善PCA(Principal Component Analysis)光谱分解特征提取方法,用SDSS(the Sloan Digital Sky Survey)、WISeREP(the Weizmann Interactive Supernova data REPository)组成的5620条光谱数据集训练支持向量机,可以得到0.498%泛化误差的识别模型和新样本分类概率.使用Neyman-Pearson决策方法建立NPSVM(Neyman-Pearson Support Vector Machine)模型可进一步降低超新星的漏判率.  相似文献   

基于双谱滤波的综合脉冲星时算法研究          下载免费PDF全文

周庆勇  魏子卿  张华  刘思伟  孙鹏飞  张奋  姜坤  刘晓刚  李奎 《天文学报》2021,62(2):19-95

毫秒脉冲星的自转频率非常稳定,提供了一种独立的基于遥远自然天体并能持续数百万乃至数十亿年的时间基准,具有稳定性强、运行时间长、服务范围广等特点.为了减弱毫秒脉冲星计时观测中各种高斯噪声对脉冲星时的影响,研究了一种基于双谱滤波的综合脉冲星时构建算法,处理分析了国际脉冲星计时阵(International Pul-sar Timing Array,IPTA)最新发布的4颗毫秒脉冲星(PSR J0437-4715、J0613-0200、J1713+0747和J1909-3744)的观测数据,分析了不同时间尺度综合脉冲星时的稳定性,并与构成国际原子时(International Atomic Time,TAI)的4家授时单位原子钟稳定性进行了比较.结果表明:双谱滤波算法能够较好地抑制观测噪声,提高综合脉冲星时的稳定性.相比于经典加权算法,综合脉冲星时1 yr、10 yr稳定度从7.77×10^-14、8.56×10^-16分别提高到1.50×10^-14、3.50×10^-16,单脉冲星时稳定性的提升也类似.同时发现,综合脉冲星时稳定性在5 yr及以上时间尺度上优于原子钟稳定性,可用于改善当前原子时的长期稳定性.  相似文献   

薄分子云湍流结构函数的倾角改正及其应用          下载免费PDF全文

钱磊 《天文学报》2021,62(1):7-87

通过结构函数可以测量湍流的能量级联速率.在实际观测中,无法测量分子云中气体的3维速度,这使得其湍流结构函数难以测量.对垂直于视线方向的薄分子云的情形,结构函数Stt2可以通过云核速度弥散(core velocity dispersion,CVD)进行测量,CVD2=1/2Stt2.对此进行推广,对于不垂直于视线方向的薄分子云,CVD2=1/2Stt2(1-1/8cos2θ)R2/3,其中,θ是视线方向与投影方向的夹角,平均投影距离与3维距离之比R可以用第2类椭圆积分E(k,φ)表示为R=2/πE(cosθ,π/2).  相似文献   

A star-based method for precise wavelength calibration of the Chinese Space Station Telescope(CSST) slitless spectroscopic survey     

Hai-Bo Yuan  Ding-Shan Deng  Yang Sun 《天文和天体物理学研究(英文版)》2021,(3):235-242

The Chinese Space Station Telescope(CSST)spectroscopic survey aims to deliver high-quality low-resolution(R>200)slitless spectra for hundreds of millions of targets down to a limiting magnitude of about 21 mag,distributed within a large survey area(17500 deg2)and covering a wide wavelength range(255-1000 nm by three bands GU,GV,and GI).As slitless spectroscopy precludes the usage of wavelength calibration lamps,wavelength calibration is one of the most challenging issues in the reduction of slitless spectra,yet it plays a key role in measuring precise radial velocities of stars and redshifts of galaxies.In this work,we propose a star-based method that can monitor and correct for possible errors in the CSST wavelength calibration using normal scientific observations,taking advantage of the facts that(ⅰ)there are about ten million stars with reliable radial velocities now available thanks to spectroscopic surveys like LAMOST,(ⅱ)the large field of view of CSST enables efficient observations of such stars in a short period of time,and(ⅲ)radial velocities of such stars can be reliably measured using only a narrow segment of CSST spectra.We demonstrate that it is possible to achieve a wavelength calibration precision of a few km s^-1 for the GU band,and about 10 to 20 kms^-1 for the GV and GI bands,with only a few hundred velocity standard stars.Implementations of the method to other surveys are also discussed.  相似文献   

Detection of a high-confidence quasi-periodic oscillation in radio light curve of the high redshift FSRQ PKS J0805–0111     

Guo-Wei Ren  Hao-Jing Zhang  Xiong Zhang  Nan Ding  Xing Yang  Fu-Ting Li  Pei-Lin Yan  Xiao-Lin Xu 《天文和天体物理学研究(英文版)》2021,(3):243-250

In this work,we have searched for quasi-periodic oscillations(QPOs)in the 15 GHz light curve of the FSRQ PKS J0805-0111 monitored by the Owens Valley Radio Observatory(OVRO)40 m telescope during the period from 2008 January 9 to 2019 May 9,using the weighted wavelet Z-transform(WWZ)and the Lomb-Scargle Periodogram(LSP)techniques.This is the first time to search for a periodic radio signal in the FSRQ PKS J0805-0111 by these two methods.Both methods consistently reveal a repeating signal with a periodicity of 3.38±0.8 yr(>99.7%confidence level).In order to determine the significance of the periods,the false alarm probability method was applied,and a large number of Monte Carlo simulations were performed.As possible explanations,we discuss a number of scenarios including the thermal instability of thin disks scenario,the spiral jet scenario and the binary supermassive black hole scenario.We expect that the binary black hole scenario,where the QPO is caused by the precession of binary black holes,is the most likely explanation.FSRQ PKS J0805-0111 thus could be a good binary black hole candidate.In the binary black hole scenario,the distance between the primary black hole and the secondary black hole is about 1.71×10¹⁶ cm.  相似文献   

裂缝智能检测技术研究及其在埕岛潜山的应用          下载免费PDF全文

于世娜  李帅  高喜龙  周红科  武群虎  黄捍东 《CT理论与应用研究》2020,29(1):23-30

断裂（裂缝）对油气藏既有破坏又有保存作用。胜利埕岛奥陶系潜山油藏受裂缝控制，非均质性强，勘探目标预测难度大。本文以地震边缘检测为先验信息和启发因子，在自适应地震相干数据体上进行蚂蚁体追踪，精细检测裂缝，弥补了单一相干体检测分辨低的缺陷，获得了与钻井和实际地下情况吻合度更高的裂缝检测结果。对该区的油气勘探起到了指导作用。   相似文献   

湘西金矿复杂地层大口径充填孔定向钻进技术          下载免费PDF全文

伍新民  易振兴  吴俊贤  宋会娟 《探矿工程》2020,47(6):26-29

根据湘西金矿深厚陡倾角地层的特点，采用传统防斜方法（如满眼组合防斜技术、钟摆组合防斜技术）不能保证钻孔垂直度，首次使用随钻测斜仪配合螺杆定向钻进先施工引导孔，再用气动潜孔锤冲击回转钻进快速完成大口径充填孔扩孔，取得了较好的效果。采用螺杆能较好地实现定向钻进，钻孔轨迹偏斜位移能被控制在8.67 m范围内。  相似文献   

噬菌弧菌N1对淡水和海水养殖水体细菌群落影响PCR-DGGE分析     

陈慧黠  韩民泳  于佳豪  刘琳 《广东海洋大学学报》2019,(5)

【目的】研究噬菌弧菌Bacteriovorax sp. N1在一个投放周期内对淡水和海水养殖环境中细菌、弧菌总数及细菌群落结构的影响。【方法】自市售微生态制剂分离蛭弧菌N1并进行分子鉴定,测定其裂解效果,制备高浓度N1菌液分别投放至淡水红鲤鱼(red carp)和海水仿刺参(Apostichopus japonicus)养殖水体,采用细菌平板计数法及PCR-变性梯度凝胶电泳(PCR-DGGE)技术分析48 h内水体环境中细菌、弧菌总数及细菌群落结构变化。【结果】经鉴定蛭弧菌N1为噬菌弧菌,其对大肠杆菌(Escherichia coli)、溶藻弧菌(Vibrio alginolyticus)、黄海希瓦氏菌(Shewanella smarisflavi)、灿烂弧菌(Vibrio splendidus)、哈氏弧菌(Vibrio harveyi)和金黄色葡萄球菌(Staphylococcus aureus)均有裂解效果。将噬菌弧菌N1投放进淡水和海水养殖环境的12～24 h,其能显著降低两种环境中弧菌含量(P 0.05)。DGGE分析显示添加噬菌弧菌N1后淡水组优势菌群弧菌属(Vibrio,a1)和不可培养杆菌属(Uncultured bacterium, a5)在12 h以后含量有明显的减少,假单胞菌属(Pseudomonas, a3)和红杆菌科Shimia属(Shimia, a6)菌含量增加。海水组优势菌群不可培养杆菌属(c2)菌在12 h时变成非优势菌群,而白杆菌属(Albirhodobacter,c1)增加成为优势菌群。噬菌弧菌N1在水中含量在24 h时降至最低。【结论】噬菌弧菌N1对海水和淡水环境中的弧菌属和不可培养杆菌属菌群有明显的裂解作用导致其含量下降,但也使假单胞菌属(Pseudomonas),红杆菌科Shimia属和白杆菌属(Albirhodobacter)菌群含量增加,但生物效应不明。为维持噬菌弧菌N1对弧菌的控制,需要24 h左右重新补充投放。  相似文献   

基于图幅调查的城市规划建设场地适宜性评价 ——以广西南宁市西津幅为例     

李春玲  江思义  黄栋声  潘兴鱼  李海良  杨春莲  彭河明 《南方国土资源》2019,(3)

文章介绍以图幅的形式进行野外地质调查,得到图幅的地貌图、工程地质图、水文地质图和地质灾害分布图,之后参照规范要求及研究区地质环境现状调查与分析,确定影响研究区建设场地适宜性的主要因子,进而开展图幅调查并对城市规划建设场地适宜性研究,为城市地质及城市规划建设提供参考。  相似文献