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搜索结果: 1-15 共查到SDSS相关记录46条 . 查询时间(0.046 秒)
近日,国家天文台白宇副研究员、刘继峰研究员基于LAMOST和SDSS数据库,利用机器学习的方法,开发天体分类器和恒星温度回归器,并把天体分类器应用到最新发布的Gaia DR2星表,揭示了Gaia DR2中天体类型组成。这是国际上使用最大样本开发的天体分类器和恒星温度回归器,该项研究成果已经被《天文学杂志》(AJ)接收,应用于Gaia DR2的最新结果已经发表在《天文和天体物理学研究》(2018,R...
近日,国家天文台天体丰度与星系演化研究团组博士后依明阿吉与赵刚研究员合作,首次利用我国LAMOST释放的第四次巡天数据与美国SDSS释放的第八次巡天数据中天琴座RR变星,测量出银河系旋转速度与银河系质量,该项研究结果已在国际核心期刊《天体物理学报》(The Astrophysical Journal)上发表。 近年来,随着大规模巡天项目(测光和光谱)的开展,进而可以测量银河系的质量分布,更加细...
近日,山东大学威海校区石维彬副教授等人通过分析LAMOST K巨星数据与SDSS RGB数据确认了一个已知分支,并在人马矮星系Leading星流上证认了一个新分支。这个新分支有助于限制人马矮星系星流的子结构和银河系势能。此成果已发表在国际知名天文期刊“Astronomy & Astrophysics”(A&A,2017, 597, A54)上。
Lack of reliable, up to date, available and qualified geospatial data is one of the problems we are faced to have a proper response to natural disasters. On the other hand, complexity of earthquake ph...
Geographic Information Technology has developed at a remarkable pace over the past two decades and will play a key role in development of nations in the 21st Century; thereupon many countries have a...
We investigate the incidence of major mergers creating massive (Mstar > 1011 M⊙) galaxies in present-day (z≤ 0.12) groups and clusters. Using a volume-limited sample of 845 groups with dark matter hal...
经过三年多的准备工作,中国科学院上海天文台作为正式成员单位参与的国际大规模巡天“斯隆数字化巡天第四阶段项目”(以下简称SDSS-IV)于7月1日正式启动,开始为期六年的巡天观测和科学研究任务。
利用云南天文台丽江2.4m望远镜对一个新发现的射电噪窄线赛弗特1(RL-NLS1)活动星系核SDSSJ125438.25+114105.8进行了光学波段的短时标监测,观测结果表明,SDSSJ125438.25+114105.8存在光学微光变,典型的光变幅度为0.05~0.1 mag,光变时标仅为h的量级。这个天体是到目前为止极少数几个探测到光学微光变的RL-NLSl之一,推断出它的光学光度至少有一...
Most massive galaxies contain supermassive black holes (SMBHs) in their cores. When galaxies merge, gas is driven to nuclear regions and can accrete onto the central black hole. Thus one expects to se...
Theoretical predictions for the ensemble quasar structure function are tested using multi-epoch observations of Stripe 82 collected by the Sloan Digital Sky Survey. We reanalyze the entire available v...
We show that the distribution of luminosities of Brightest Cluster Galaxies, in two SDSS-based group catalogs, suggests that BCG luminosities are just the statistical extremes of the group galaxy lumi...
We investigate in detail the probability distribution function (pdf) of the proper-motion measurement errors in the SDSS+USNO-B proper-motion catalog of \citet{mun04} using clean quasar samples. The p...
We analyze the three-year SDSS-II Superernova (SN) Survey data and identify a sample of 1070 photometric SN Ia candidates based on their multi-band light curve data. This sample consists of SN candida...
We obtain cosmological constraints from a measurement of the spherically averaged power spectrum (PS) of the distribution of about 90000 luminous red galaxies (LRGs) across 7646 deg2 in the Northern G...
Taking into account a range of parameters determined from the evolutionary models and available observational data, the detailed non-LTE spectra for the primary star and the irradiated donor star in t...

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