中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
MEASURING STRUCTURAL PARAMETERS THROUGH STACKING GALAXY IMAGES

文献类型:期刊论文

作者Li, Yubin1,2; Zheng, Xian Zhong1; Gu, Qiu-Sheng3,4; Wang, Yi-Peng3,4; Wen, Zhang Zheng1,2; Guo, Kexin1; An, Fang Xia1,2
刊名ASTRONOMICAL JOURNAL
出版日期2016-12-01
卷号152期号:6页码:15
ISSN号0004-6256
关键词galaxies: photometry Galaxy: evolution Galaxy: structure
DOI10.3847/0004-6256/152/6/201
通讯作者Zheng, Xian Zhong(xzzheng@pmo.ac.cn)
英文摘要It remains challenging to detect the low surface brightness structures of faint high-z galaxies, which are key to understanding the structural evolution of galaxies. The technique of image stacking allows us to measure the averaged light profile beneath the detection limit and probe the extended structure of a group of galaxies. We carry out simulations to examine the recovery of the averaged surface brightness profile through stacking model Hubble Space Telescope/Advanced Camera for Surveys images of a set of galaxies as functions of the Sersic index (n), effective radius (R-e) and axis ratio (AR). The Sersic profile best fitting the radial profile of the stacked image is taken as the recovered profile, in comparison with the intrinsic mean profile of the model galaxies. Our results show that, in general, the structural parameters of the mean profile can be properly determined through stacking, though systematic biases need to be corrected when spreads of R-e and AR are counted. We find that the Sersic index is slightly overestimated and R-e is underestimated at AR < 0.5 because the stacked image appears to be more compact due to the presence of inclined galaxies; the spread of Re biases the stacked profile to have a higher Sersic index. We stress that the measurements of structural parameters through stacking should take these biases into account. We estimate the biases in the recovered structural parameters from stacks of galaxies when the samples have distributions of R-e, AR and n seen in local galaxies.
WOS关键词DIGITAL SKY SURVEY ; STAR-FORMING GALAXIES ; HUBBLE-SPACE-TELESCOPE ; EXTRAGALACTIC LEGACY SURVEY ; MASS-METALLICITY RELATION ; INSIDE-OUT GROWTH ; SIMILAR-TO 2 ; QUIESCENT GALAXIES ; ELLIPTIC GALAXIES ; SIZE EVOLUTION
WOS研究方向Astronomy & Astrophysics
语种英语
出版者IOP PUBLISHING LTD
WOS记录号WOS:000390360900004
源URL[http://libir.pmo.ac.cn/handle/332002/23374]  
专题中国科学院紫金山天文台
通讯作者Zheng, Xian Zhong
作者单位1.Chinese Acad Sci, Purple Mt Observ, 2 West Beijing Rd, Nanjing 210008, Jiangsu, Peoples R China
2.Univ Chinese Acad Sci, 19A Yuquan Rd, Beijing 100049, Peoples R China
3.Nanjing Univ, Sch Astron & Space Sci, Nanjing 210093, Jiangsu, Peoples R China
4.Nanjing Univ, Minist Educ, Key Lab Modern Astron & Astrophys, Nanjing 210093, Jiangsu, Peoples R China
推荐引用方式
GB/T 7714
Li, Yubin,Zheng, Xian Zhong,Gu, Qiu-Sheng,et al. MEASURING STRUCTURAL PARAMETERS THROUGH STACKING GALAXY IMAGES[J]. ASTRONOMICAL JOURNAL,2016,152(6):15.
APA Li, Yubin.,Zheng, Xian Zhong.,Gu, Qiu-Sheng.,Wang, Yi-Peng.,Wen, Zhang Zheng.,...&An, Fang Xia.(2016).MEASURING STRUCTURAL PARAMETERS THROUGH STACKING GALAXY IMAGES.ASTRONOMICAL JOURNAL,152(6),15.
MLA Li, Yubin,et al."MEASURING STRUCTURAL PARAMETERS THROUGH STACKING GALAXY IMAGES".ASTRONOMICAL JOURNAL 152.6(2016):15.

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来源:紫金山天文台

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