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Stellar Parameters,Extinction,and Distances for Stars in SMSS DR2 by the SPar Method
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作者 Mingxu Sun bingqiu chen +8 位作者 Baokun Sun Tao Wang Zheng Yu Baisong Zhang Lin Zhang Yuxi Bao Guangya Zeng Ming Yang Wenyuan Cui 《Research in Astronomy and Astrophysics》 2025年第5期19-33,共15页
The availability of large data sets containing stellar parameters,distances,and extinctions for stars in the Milky Way,particularly within the Galactic disk,is essential for advancing our understanding of the Galaxy’... The availability of large data sets containing stellar parameters,distances,and extinctions for stars in the Milky Way,particularly within the Galactic disk,is essential for advancing our understanding of the Galaxy’s stellar populations,structure,kinematics,and chemical evolution.In this study,we present a catalog of stellar parameters,including effective temperature (T_(eff)),metallicity ([Fe/H]),absolute magnitudes (M_(G)),distances (d),and reddening values (E(G_(BP)-G_(RP))),for a sample of 141 million stars from the SkyMapper Southern Survey.These parameters are derived using the SPar algorithm,which employs a fitting procedure to match multi-band photometric observations and estimate the stellar properties (T_(eff),[Fe/H],M_(G),d,and E(G_(BP)-G_(RP))) on an individual star basis,following the methodology outlined in our previous work.This study successfully determines stellar parameters and extinction values simultaneously for stars located in high and low Galactic latitudes.The resulting stellar parameters and extinction values are in good agreement with results from other studies,demonstrating the robustness of our method.We derive a temperature dispersion of 195 K and a metallicity dispersion of 0.31 dex when comparing our results with spectroscopic data.The catalog produced in this work provides a valuable resource for future research on the Galactic metallicity distribution function,the structure of the Galaxy,threedimensional extinction mapping,and other related astrophysical topics. 展开更多
关键词 (ISM )dust extinction-Stars-stars low-mass-(Galaxy )solar neighborhood
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KMT2D deficiency leads to cellular developmental disorders and enhancer dysregulation in neural-crest-containing brain organoids
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作者 Ziyun Shan Yingying Zhao +22 位作者 Xiuyu chen Guodong Zhan Junju Huang Xuejie Yang Chongshen Xu Ning Guo Zhi Xiong Fang Wu Yujian Liu He Liu Biyuan chen bingqiu chen Jiaoyang Sun Jiangping He Yiping Guo Shangtao Cao Kaixin Wu Rui Mao Guangming Wu Lihui Lin Xiaobing Zou Jie Wang Jiekai chen 《Science Bulletin》 SCIE EI CAS CSCD 2024年第22期3533-3546,共14页
KMT2D,a H3K4me1 methyltransferase primarily regulating enhancers,is a leading cause of KABUKI syndrome.This multisystem disorder leads to craniofacial and cognitive abnormalities,possibly through neural crest and neur... KMT2D,a H3K4me1 methyltransferase primarily regulating enhancers,is a leading cause of KABUKI syndrome.This multisystem disorder leads to craniofacial and cognitive abnormalities,possibly through neural crest and neuronal lineages.However,the impacted cell-of-origin and molecular mechanism of KMT2D during the development of KABUKI disease remains unknown.Here we have optimized a brain organoid model to investigate neural crest and neuronal differentiation.To pinpoint KMT2D's enhancer target,we developed a genome-wide cis-regulatory element explorer(GREE)based on single-cell multiomic integration.Single cell RNA-seq revealed that KMT2D-knockout(KO)and patient-derived organoids exhibited neural crest deformities and GABAergic overproduction.Mechanistically,GREE identified that KMT2D targets a roof-plate-like niche cell and activates the niche cell-specific WNT3A enhancer,providing the microenvironment for neural crest and neuronal development.Interestingly,KMT2D-mutated mice displayed decreased WNT3A expression in the diencephalon roof plate,indicating impaired niche cell function.Deleting the WNT3A enhancer in the organoids presented phenotypic similarities to KMT2D-depletion,emphasizing the WNT3A enhancer as the predominant target of KMT2D.Conversely,reactivating WNT signaling in KMT2D-KO rescued the lineage defects by restoring the microenvironment.Overall,our discovery of KMT2D's primary target provides insights for reconciling complex phenotypes of KABUKI syndrome and establishes a new paradigm for dissecting the mechanisms of genetic disorders from genotype to phenotype. 展开更多
关键词 KMT2D ENHANCER NICHE Cerebral organoids Single-cell multiome
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银河系三维消光图
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作者 陈丙秋 张百松 《科学通报》 EI CAS CSCD 北大核心 2024年第28期4218-4229,共12页
星际尘埃是银河系的重要组成部分,其分布和性质对于理解银河系的结构、形成和演化具有重要意义.尘埃导致的星际消光和红化现象会改变观测到的天体光度和颜色,对其进行消光改正是评估天体内禀性质的关键步骤.银河系的三维尘埃消光图包含... 星际尘埃是银河系的重要组成部分,其分布和性质对于理解银河系的结构、形成和演化具有重要意义.尘埃导致的星际消光和红化现象会改变观测到的天体光度和颜色,对其进行消光改正是评估天体内禀性质的关键步骤.银河系的三维尘埃消光图包含了尘埃分布的空间信息,这对于进行精确的消光改正以及研究尘埃的分布和性质至关重要.然而,描绘银河系中星际消光的三维分布一直是天文学领域中的重要挑战,其困难之处在于需要对大量恒星的消光值和距离值进行精确测量,因此,这一工作的推进依赖于大规模的银河系巡天观测.本文详细总结了当前用于构建银河系三维消光图的各种方法,并根据探测距离从远到近和分辨率从低到高的不同,将现有的消光图分为三类进行深入讨论.同时,简要介绍了在银河系中用于校正天体三维消光的工具.最后对基于银河系三维消光图的尘埃结构研究进行了回顾.尽管当前在消光研究方面已经取得了显著的进步,并且实现了全天范围内的三维消光测量,但我们也认识到,分辨率、精度以及探测距离等方面仍有待进一步地提高.未来的高精度测光巡天项目将提供更高质量、更高精度的数据,这将对深入理解银河系的结构和化学演化起到至关重要的作用. 展开更多
关键词 星际介质 尘埃 消光与红化 银河系结构 银盘
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