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| 1 | Kinematics and activity of M dwarfs in LAMOST DR1显示文摘We report on the first investigation into kinematics and chromospheric activity of M dwarfs from the Guo Shou Jing Telescope(also called the Large Sky Area Multi-Object Fiber Spectroscopic Telescope – LAMOST) data release one(DR1).The sample comprises 71 304 M dwarfs. Their fundamental parameters such as spectral types, radial velocities, important molecular band indices and magnetic activities are measured. Their distances are determined by a spectroscopic parallax relation.Space motion(U, V, W) and Galactocentric cylindrical coordinates(R, θ, Z) for the M dwarfs are also computed. We examine velocity dispersion as a function of height from the Galactic plane and find that all three components of velocity dispersion increase with height as measured with respect to the Galactic plane. The investigation into chromospheric activities along the height from the Galactic plane confirms that M dwarfs closer to the Galactic plane are more likely to be active. We take a pure kinematical approach to select thin disk stars and thick disk stars from our sample, then to investigate the differences in properties between these two populations. Our analysis is in excellent agreement with previous studies and leads to a better understanding of the structure of the Galactic disk. | Zhen-Ping Yi A-Li Luo Jing-Kun Zhao Yi-Han Song Jing-Chang Pan Yong-Heng Zhao Yong Zhang | 2015 | Research in Astronomy and Astrophysics2015，15，6： | 3 |
| 2 | Preface: The LAMOST Galactic surveys and early results显示文摘By the time of this writing, the ongoing LAMOST Galactic surveys have collected approximately 4.5 million stellar spectra with signal-to-noise ratios better than 10 per pixel. This special issue is devoted to early results from the surveys,mostly based on the LAMOST Data Release 1(DR1; Luo et al., this volume) that contains data secured by May 2013, the end of the first year of regular surveys, although a few studies have made use of data collected in the second year of regular surveys. LAMOST DR1 was released to the Chinese astronomical community and international partners in August 2013 and made public to the whole world in March2015. Here we briefly review the scope and motivation, data reduction and release, as well as early results of the surveys. As the project advances, one can expect that these surveys will yield an exquisite description of the distribution, kinematics and chemistry of Galactic stellar populations, especially those within a few kpc of the Sun, a robust measurement of the local dark matter density, and, consequently, shed light on how our Galaxy, and other galaxies in general, form and evolve. | Xiao-Wei Liu Gang Zhao Jin-Liang Hou | 2015 | Research in Astronomy and Astrophysics2015，15，8： | 3 |
| 3 | The first data release(DR1) of the LAMOST regular survey显示文摘The Large sky Area Multi-Object Fiber Spectroscopic Telescope(LAMOST) general survey is a spectroscopic survey that will eventually cover approximately half of the celestial sphere and collect 10 million spectra of stars, galaxies and QSOs. Objects in both the pilot survey and the first year regular survey are included in the LAMOST DR1. The pilot survey started in October 2011 and ended in June 2012, and the data have been released to the public as the LAMOST Pilot Data Release in August 2012. The regular survey started in September 2012, and completed its first year of operation in June 2013. The LAMOST DR1 includes a total of 1202 plates containing 2 955 336 spectra, of which 1 790 879 spectra have observed signalto-noise ratio(SNR) ≥ 10. All data with SNR ≥ 2 are formally released as LAMOST DR1 under the LAMOST data policy. This data release contains a total of 2 204 696 spectra, of which 1 944 329 are stellar spectra, 12 082 are galaxy spectra and 5017 are quasars. The DR1 not only includes spectra, but also three stellar catalogs with measured parameters: late A,FGK-type stars with high quality spectra(1 061 918 entries), A-type stars(100 073 entries), and M-type stars(121 522 entries). This paper introduces the survey design, the observational and instrumental limitations, data reduction and analysis, and some caveats. A description of the FITS structure of spectral files and parameter catalogs is also provided. | A-Li Luo Yong-Heng Zhao Gang Zhao Li-Cai Deng Xiao-Wei Liu Yi-Peng Jing Gang Wang Hao-Tong Zhang Jian-Rong Shi Xiang-Qun Cui Yao-Quan Chu Guo-Ping Li Zhong-Rui Bai Yue Wu Yan Cai Shu-Yun Cao Zi-Huang Cao Jeffrey L.Carlin Hai-Yuan Chen Jian-Jun Chen Kun-Xin Chen Li Chen Xue-Lei Chen Xiao-Yan Chen Ying Chen Norbert Christlieb Jia-Ru Chu Chen-Zhou Cui Yi-Qiao Dong Bing Du Dong-Wei Fan Lei Feng Jian-Ning Fu Peng Gao Xue-Fei Gong Bo-Zhong Gu Yan-Xin Guo Zhan-Wen Han Bo-Liang He Jin-Liang Hou Yong-Hui Hou Wen Hou Hong-Zhuan Hu Ning-Sheng Hu Zhong-Wen Hu Zhi-Ying Huo Lei Jia Fang-Hua Jiang Xiang Jiang Zhi-Bo Jiang Ge Jin Xiao Kong Xu Kong Ya-Juan Lei Ai-Hua Li Chang-Hua Li Guang-Wei Li Hai-Ning Li Jian Li Qi Li Shuang Li Sha-Sha Li Xin-Nan Li Yan Li Yin-Bi Li Ye-Ping Li Yuan Liang Chien-Cheng Lin Chao Liu Gen-Rong Liu Guan-Qun Liu Zhi-Gang Liu Wen-Zhi Lu Yu Luo Yin-Dun Mao Heidi Newberg Ji-Jun Ni Zhao-Xiang Qi Yong-Jun Qi Shi-Yin Shen Huo-Ming Shi Jing Song Yi-Han Song Ding-Qiang Su Hong-Jun Su Zheng-Hong Tang Qing-Sheng Tao Yuan Tian Dan Wang Da-Qi Wang Feng-Fei Wang Guo-Min Wang Hai Wang Hong-Chi Wang Jian Wang Jia-Ning Wang Jian-Ling Wang Jian-Ping Wang Jun-Xian Wang Lei Wang Meng-Xin Wang Shou-Guan Wang Shu-Qing Wang Xia Wang Ya-Nan Wang You Wang Yue-Fei Wang You-Fen Wang Peng Wei Ming-Zhi Wei Hong Wu Ke-Fei Wu Xue-Bing Wu Yu-Zhong Wu Xiao-Zheng Xing Ling-Zhe Xu Xin-Qi Xu Yan Xu Tai-Sheng Yan De-Hua Yang Hai-Feng Yang Hui-Qin Yang Ming Yang Zheng-Qiu Yao Yong Yu Hui Yuan Hai-Bo Yuan Hai-Long Yuan Wei-Min Yuan Chao Zhai En-Peng Zhang Hua-Wei Zhang Jian-Nan Zhang Li-Pin Zhang Wei Zhang Yong Zhang Yan-Xia Zhang Zheng-Chao Zhang Ming Zhao Fang Zhou Xu Zhou Jie Zhu Yong-Tian Zhu Si-Cheng Zou Fang Zuo | 2015 | Research in Astronomy and Astrophysics2015，15，8： | 2 |
| 4 | 中间锦鸡儿CiDR1的克隆及干旱胁迫下的表达分析显示文摘[目的]研究并了解中间锦鸡儿CiDR1基因功能及其对干旱胁迫的响应,为抗性育种提供候选基因。[方法]通过RACE技术从中间锦鸡儿中克隆CiDR1基因的c DNA全长,利用生物信息学分析软件对其基因结构及功能进行分析和预测。再通过qRT-PCR技术对干旱胁迫后的幼苗中的CiDR1表达模式进行研究。[结果]从中间锦鸡儿中克隆到CiDR1基因的c DNA全长共计4 297 bp,Gen Bank登录号为KP277100。生物信息学分析表明,预测的CiDR1蛋白序列中含有1 243个氨基酸残基,具有抗病基因特征结构域TIR、NB-ARC、LRR等,其等电点为6.35,不稳定指数为42.91,不具备信号肽,为非分泌蛋白,定位于细胞质中。定量PCR检测发现,CiDR1基因在幼年期的茎中表达量较低,在成年期的叶片中表达量较高;在干旱胁迫处理后的幼苗中,CiDR1表达水平有明显下降,表明该基因的表达受干旱抑制,可能与中间锦鸡儿适应干旱相关。[结论]中间锦鸡儿在干旱胁迫后其根、茎和叶中CiDR1的表达均明显下降,表明CiDR1的表达受干旱抑制,可能与中间锦鸡儿适应干旱相关,进一步研究发现CiDR1在根、茎、叶中的表达水平可能受发育阶段调控。 | 武苾菲 李万峰 徐海燕 张立峰 齐力旺 韩素英 | 2017 | 林业科学研究2017，30，2： | 2 |
| 5 | 有机聚合物PMMA/DR1热光开关显示文摘利用光漂白方法在 PMMA/DR1有机聚合物光波导上制备出 Mach- Zehnder干涉型耦合器 ,形成低开关功率的 2× 2热光开关 ,在 1 .0 64μm波长处实现了光开关效应 . | 贾振红 地里木拉提.吐尔逊 李芮 | 2001 | 新疆大学学报(理工版)2001，18，4： | 1 |
| 6 | Validation of LAMOST stellar parameters with the PASTEL catalog显示文摘The Large Sky Area Multi-Object Fiber Spectroscopic Telescope(LAMOST) published its first data release(DRl)in 2013,which is currently the largest dataset of stellar spectra in the world.We combine the PASTEL catalog and SIMBAD radial velocities as a testing standard to validate stellar parameters(effective temperature T_(eff),surface gravity log g,metallicity[Fe/H]and radial velocity V_r)derived from DR1.Through cross-identification of the DR1 catalogs and the PASTEL catalog,we obtain a preliminary sample of 422 stars.After removal of stellar parameter measurements from problematic spectra and applying effective temperature constraints to the sample,we compare the stellar parameters from DR1 with those from PASTEL and SIMBAD to demonstrate that the DR1 results are reliable in restricted ranges of T_(eff).We derive standard deviations of 110 K,0.19 dex and 0.11 dex for T_(eff),log g and[Fe/H]respectively when T_(eff)<8000 K,and 4.91 km S^(-1) for V_r when T_(eff)<10 000 K.Systematic errors are negligible except for those of V_r.In addition,metallicities in DR1 are systematically higher than those in PASTEL,in the range of PASTEL[Fe/H]<-1.5. | Hua Gao Hua-Wei Zhang Mao-Sheng Xiang Yang Huang Xiao-Wei Liu A-Li Luo Hao-Tong Zhang Yue Wu Yong Zhang Guang-Wei Li Bing Du | 2015 | Research in Astronomy and Astrophysics2015，15，12： | 1 |
| 7 | 聚合物PMMA/DR1薄膜棱镜的制备显示文摘本文研究了用光漂白方法制备PMMA/DR1聚合物光薄膜棱镜的方法测量了这种波导棱镜对1064μm光的TE模和TM模在波导内传播光束的方向改变。 | 贾振红 李劬 | 2000 | 新疆大学学报(自然科学版)2000，17，1： | 0 |
| 8 | Electro-optic Properties of DR1 Doped SiO_2 Organic/inorganic Guest-host Films显示文摘We made a comprehensive investigation on the electro-optic(EO) properties of hybrid sol-gel silica film doped with Dispersed Red 1 dye(DR1/SiO2). An important finding is that the dipoles which don't orient along the direction of corona poling field in the films can be instantaneously poled by alternate modulation electrical field. This instant poling effect results in the EO coefficients dependent on the frequency and intensity of alternate modulation electric field, and some experiments have proved it. We also investigated the electro-optic coefficients and thickness of films at different stir temperatures(Ts) of start solution and at different number densities of DR1. Experimentally the DR1 number density was optimized to an order of 1021/cm3 and a large EO coefficient of γ33=37 pm/V for DR1/SiO2 film was measured by simple reflection technique at 1 kHz frequencies of modulation electric field. These findings may benefit the practical application of DR1/SiO2 films in the field of EO modulator and EO probing. | LIU Shao-lin YANG Han JIN Ru-long YAN Zhao-xu YI Mao-bin | 2009 | Chemical Research in Chinese Universities2009，25，5： | 0 |
| 9 | 应用Gaia DR1的木卫六天体测量试验观测显示文摘木卫六是木星最大的一颗不规则天然卫星,为了获得它的高精度观测位置,天体测量归算过程中各方面都需要考虑,其中特别重要的是参考星表的选择。应用最新公布的星表Gaia Data Release 1(Gaia DR1),同时采用UCAC4星表进行比较,对2015年云南天文台获得的185个木卫六的观测资料进行处理和归算,结果显示,采用Gaia DR1星表的木卫六的位置测量精度在赤经和赤纬两个方向都约为0.02″,比采用UCAC4的结果有显著提升。 | 彭焕文 彭青玉 王娜 | 2017 | 天文研究与技术2017，14，3： | 0 |
| 10 | 比索尼还要好——Sound Design FoB SD05数字功率放大器显示文摘索尼的全数字功率放大器TA-DR1在业界获得很多好评,它是由原索尼公司的石田正臣先生(Masaomi Ishida)设计的。由于非常喜欢音响,他在加入索尼公司后曾设计过开放式录音卡座TC-R7、盒式录音卡座TC~K777、CD唱机CDPR1和CDP-MS1等。他在设计完TA—DR1后离开索尼公司,并于2004年9月设立了自己的Sound Design有限公司。同年11月,其听音室(Sound Design Fan Club)开张, | 王烨 | 2008 | 无线电与电视2008，，10： | 0 |
| 11 | CaII H&K emission distribution of ~120000 F,G and K stars in LAMOST DR1显示文摘We present chromospheric activity index SHK measurements for 119 995 F, G and K stars with high signal-to-noise ratio(S/N > 80) spectra, extracted from LAMOST DR1 in SDSS g band. The index δS for each of these stars is calculated by the difference between its SHK value and the baseline determined from very inactive stars. The effect of metallicity on measurement of δS varies with stellar Teff. No evident Vaughan-Preston gap appears in our sample. The relation between δS and vertical distance from the Galactic plane is determined for stars with Teff < 5500 K. Stars with higher δS tend to be closer to the Galactic plane. Two open clusters in the DR1 sample, M45 and M67, exhibit the expected general trend that δS decays with age.For stars with Teff > 5500 K, similar δS levels appear in both young and old cluster stars, which supports Pace's suggestion that caution should be exercised when deriving the age of a single star by using its chromospheric activity. Finally, we investigate the relation between δS and the kinematics of our sample. | Jing-Kun Zhao Terry D.Oswalt Yu-Qin Chen Jian-Rong Shi Ke-Feng Tan Xiang-Song Fang Gang Zhao Ming Yang Yong Zhang Yong-Hui Hou Yue-Fei Wang | 2015 | Research in Astronomy and Astrophysics2015，15，8： | 0 |
| 12 | Searching for classical Be stars in LAMOST DR1显示文摘We report on searching for Classical B-type emission-line(CBe) stars in the first data release of the Large Sky Area Multi-Object fiber Spectroscopic Telescope(LAMOST; also called the Guo Shou Jing Telescope). A total of 192 objects(including 12 previously known CBes) were identified as CBe candidates with prominent He I λ4387, He I λ4471 and Mg II λ4481 absorption lines, as well as Hβλ4861and Hαλ6563 emission lines. These candidates significantly increase the currently known sample of CBes by about 8%. Most of the CBe candidates are distributed near the Galactic Anti-Center due to the observing strategy used for LAMOST. Only two CBes are in star clusters. These two CBes have ages of 15.8 and 398 Myr, respectively. | Chien-Cheng Lin Jin-Liang Hou Li Chen Zheng-Yi Shao Jing Zhong Po-Chieh Yu | 2015 | Research in Astronomy and Astrophysics2015，15，8： | 0 |
| 13 | 郭守敬望远镜发布首批巡天光谱数据DR1包含220万光谱,超过世界上所有已知恒星巡天项目的光谱总数显示文摘3月19日,中国科学院国家天文台向世界发布了自2011年9月以来先导巡天和第一年正式巡天的首批光谱数据集(Data Release1,DR1)。有关人士表示,这充分显示了我国重大科技基础设施的自主创新能力。 | 马伟 | 2015 | 科技中国2015，0，4： | 0 |
| 14 | A search for double-peaked narrow emission line galaxies and AGNs in the LAMOST DR1显示文摘The Large Sky Area Multi-Object Fiber Spectroscopic Telescope(LAMOST) has released more than two million spectra,which provide the opportunity to search for double-peaked narrow emission line(NEL) galaxies and active galactic nuclei(AGNs).The double-peaked narrow-line profiles can be well modeled by two velocity components,respectively blueshifted and redshifted with respect to the systemic recession velocity.This paper presents 20 double-peaked NEL galaxies and AGNs found from LAMOST DR1 using a search method based on a multi-Gaussian fit of the narrow emission lines.Among them,ten have already been published by other authors,either listed as genuine double-peaked NEL objects or as asymmetric NEL objects,and the remaining ten are original discoveries.We discuss some possible origins for the double-peaked narrow-line features,such as interaction between jet and narrow line regions,interaction with companion galaxies,and black hole binaries.Spatially resolved optical imaging and/or follow-up observations in other spectral bands are needed to further discuss the physical mechanisms at work. | Zhi-Xin Shi A-Li Luo Georges Comte Xiao-Yan Chen Peng Wei Yong-Heng Zhao Fu-Chao Wu Yan-Xia Zhang Shi-Yin Shen Ming Yang Hong Wu Xue-Bing Wu Hao-Tong Zhang Ya-Juan Lei Jian-Nan Zhang Ting-Gui Wang Ge Jin Yong Zhang | 2014 | Research in Astronomy and Astrophysics2014，14，10： | 0 |
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