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First Detailed Analysis of a Relatively Deep, Low Mass-ratio Contact Binary:ATO J108.6991+27.8306
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作者 Shuo Ma jinzhong liu +3 位作者 Yu Zhang Guoliang LYU Ting Wu Chenyang He 《Research in Astronomy and Astrophysics》 SCIE CAS CSCD 2023年第3期104-110,共7页
We present the first detailed photometric analysis of ATO J108.6991+27.8306(hereinafter as J108).The shortperiod close binary J108 was observed by the Nanshan 1 m Wide Field Telescope of the Xinjiang Astronomical Obse... We present the first detailed photometric analysis of ATO J108.6991+27.8306(hereinafter as J108).The shortperiod close binary J108 was observed by the Nanshan 1 m Wide Field Telescope of the Xinjiang Astronomical Observatory.The obtained BVRI-band light curves were used to determine the photometric solution by using the 2003 version of the Wilson-Devinney code.J108 is a typical deep(f>50%),low mass ratio(q<0.25)overcontact binary system with a mass ratio of q=0.1501 and a fill-out factor of f=50.1%,suggesting that it is in the late evolutionary stage of contact binary systems.We found the target to be a W-type W UMa binary and provided evidence for the presence of starspots on both components.From the temperature-luminosity diagram,the main component is the evolved main sequence star with an evolutionary age of about 7.94 Gyr. 展开更多
关键词 BINARY RATIO DEEP
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SAGES南山1米大视场望远镜g、r、i波段测光数据流量定标
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作者 肖凯 苑海波 +16 位作者 黄博闻 徐帅 郑捷 李春 范舟 王炜 赵刚 冯国杰 张轩 刘进忠 张若羿 杨琳 张余 白春海 牛虎彪 艾力·伊沙木丁 马路 《科学通报》 EI CAS CSCD 北大核心 2023年第21期2790-2804,共15页
均匀且精确的流量定标是大视场测光巡天数据处理的难点和核心所在.本文借助LAMOST(Large Sky Area Multi-Object Fiber Spectroscopic Telescope)DR7光谱数据、修正后的Gaia EDR3测光数据和Gaia测光丰度数据,使用基于光谱的SCR(Stellar ... 均匀且精确的流量定标是大视场测光巡天数据处理的难点和核心所在.本文借助LAMOST(Large Sky Area Multi-Object Fiber Spectroscopic Telescope)DR7光谱数据、修正后的Gaia EDR3测光数据和Gaia测光丰度数据,使用基于光谱的SCR(Stellar Color Regression)方法和基于测光的SCR方法(SCR′方法)构建了南山1米大视场望远镜g、r、i波段精度约为10~20毫星等的260多万颗标准星,进而对SAGES(Stellar Abundance and Galactic Evolution Survey)南山1米望远镜拍摄的约4254平方度天区的测光数据进行了相对流量定标.在此过程中,我们仔细考虑了定标零点随不同图像(时间)、探测器不同通道及星像在探测器不同位置的变化.基于修正后的Pan-STARRS(PS1)DR1测光数据,进行了绝对流量定标,并给出了南山g、r、i波段定标后的星等与PS1星等之间的相互转换关系.基于相邻图之间的共同源对定标精度进行了内部一致性检验,发现3个波段的定标精度均约为2.0毫星等.同时,我们还对定标精度做了外部检验,使用Gaia DR3无缝光谱合成的PS1星等,发现定标均匀性在1.3°分辨本领下分别为2.4、2.3和0.9毫星等.此外,本文还讨论了恒星平场和探测器通道间相对增益随时间的变化. 展开更多
关键词 大视场测光巡天 流量定标 恒星参数 星际消光
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Evidence for transforming mineralization of Baiguoyuan silver-vanadium deposit hosted in black shale in Hubei,China 被引量:1
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作者 Hanping Zhuang Jialan Lu +3 位作者 Jiamo Fu jinzhong liu Chigang Ren Degang Zou 《Chinese Science Bulletin》 SCIE EI CAS 1999年第3期263-267,共5页
Baiguoyuan silver-vanadium deposit is generally thought to be of sedimentary-diagenetic origin. Based on the characteristics of barites, it is suggested that hydrothermal transformation has been involved in mineraliza... Baiguoyuan silver-vanadium deposit is generally thought to be of sedimentary-diagenetic origin. Based on the characteristics of barites, it is suggested that hydrothermal transformation has been involved in mineralization. The barites in black shale can be grouped into irregular ones which were formed during early diagenesis and tabular ones which were formed during late diagenesis. The tabular barites are replaced by pyrite and have formed a regular girdle around them. PIXE analysis states that Ag is greatly concentrated in pyrite replacement girdle. The girdle is the product of hydrothermal transformation. The transformation is one of the main mineralization stages of Baiguoyuan deposit. 展开更多
关键词 Baiguoyuan silver-vanadium deposit BARITE transformation.
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