A Glimpse of Satellite Galaxies in the Milky Way with the 2.5-meter Wide Field Survey Telescope (WFST): Bootes III and Draco

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Main Authors: Yang, Chao, Pan, Zhizheng, Fang, Min, Zheng, Xian Zhong, Liu, Binyang, Li, Guoliang, Sun, Tian-Rui, Jiang, Ji-An, Zhang, Miaomiao, Wan, Zhen, Liu, Shuang, Qu, Han, Yang, Ji, Kong, Xu, Liu, Wenhao, Shu, Yiping, Chang, Jiang, Wang, Tinggui, Fan, Lulu, Xue, Yongquan, Luo, Wentao, Zhang, Hongxin, Lou, Zheng, Zhao, Haibin, Li, Bin, Wang, Hairen, Yao, Dazhi, Wang, Jian, Zhang, Hongfei, Li, Feng, Liu, Hao, Liang, Ming, Tang, Jinlong, Zhang, Yuheng, Qiao, Man, Wen, Run, Lyu, Zongfei
Format: Preprint
Published: 2025
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author Yang, Chao
Pan, Zhizheng
Fang, Min
Zheng, Xian Zhong
Liu, Binyang
Li, Guoliang
Sun, Tian-Rui
Jiang, Ji-An
Zhang, Miaomiao
Wan, Zhen
Liu, Shuang
Qu, Han
Yang, Ji
Kong, Xu
Liu, Wenhao
Shu, Yiping
Chang, Jiang
Wang, Tinggui
Fan, Lulu
Xue, Yongquan
Luo, Wentao
Zhang, Hongxin
Lou, Zheng
Zhao, Haibin
Li, Bin
Wang, Hairen
Yao, Dazhi
Wang, Jian
Zhang, Hongfei
Li, Feng
Liu, Hao
Liang, Ming
Tang, Jinlong
Zhang, Yuheng
Qiao, Man
Wen, Run
Lyu, Zongfei
author_facet Yang, Chao
Pan, Zhizheng
Fang, Min
Zheng, Xian Zhong
Liu, Binyang
Li, Guoliang
Sun, Tian-Rui
Jiang, Ji-An
Zhang, Miaomiao
Wan, Zhen
Liu, Shuang
Qu, Han
Yang, Ji
Kong, Xu
Liu, Wenhao
Shu, Yiping
Chang, Jiang
Wang, Tinggui
Fan, Lulu
Xue, Yongquan
Luo, Wentao
Zhang, Hongxin
Lou, Zheng
Zhao, Haibin
Li, Bin
Wang, Hairen
Yao, Dazhi
Wang, Jian
Zhang, Hongfei
Li, Feng
Liu, Hao
Liang, Ming
Tang, Jinlong
Zhang, Yuheng
Qiao, Man
Wen, Run
Lyu, Zongfei
contents We carry out deep imaging of the Milky Way satellite galaxies, Bootes III and Draco, with WFST as one pilot observing program to demonstrate the capability of WFST. Combining catalogs with PS1 DR2 and Gaia DR3, we derive proper motions for candidate member stars in these two satellite galaxies over a 12-year time baseline, yielding uncertainties of ~1.8 mas/yr at 21 mag and ~3.0 mas/yr at 22 mag in the r band. The proper motions derived from bright and faint stars are consistent, indicating no significant variation in proper motion across stellar luminosity as these galaxies undergo tidal interactions with the MW. Meanwhile, we suggest that Bootes III represents the bound remnant of the progenitor galaxy that gave rise to the Styx stream, as evidenced by its elongated density profile and overdensity in both spatial and kinematic space. This is the first paper to use WFST to measure the proper motions of faint stars in Milky Way satellite galaxies. More detailed analyses will be presented in forthcoming papers from the wide field survey (WFS) program.
format Preprint
id arxiv_https___arxiv_org_abs_2506_20997
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle A Glimpse of Satellite Galaxies in the Milky Way with the 2.5-meter Wide Field Survey Telescope (WFST): Bootes III and Draco
Yang, Chao
Pan, Zhizheng
Fang, Min
Zheng, Xian Zhong
Liu, Binyang
Li, Guoliang
Sun, Tian-Rui
Jiang, Ji-An
Zhang, Miaomiao
Wan, Zhen
Liu, Shuang
Qu, Han
Yang, Ji
Kong, Xu
Liu, Wenhao
Shu, Yiping
Chang, Jiang
Wang, Tinggui
Fan, Lulu
Xue, Yongquan
Luo, Wentao
Zhang, Hongxin
Lou, Zheng
Zhao, Haibin
Li, Bin
Wang, Hairen
Yao, Dazhi
Wang, Jian
Zhang, Hongfei
Li, Feng
Liu, Hao
Liang, Ming
Tang, Jinlong
Zhang, Yuheng
Qiao, Man
Wen, Run
Lyu, Zongfei
Astrophysics of Galaxies
We carry out deep imaging of the Milky Way satellite galaxies, Bootes III and Draco, with WFST as one pilot observing program to demonstrate the capability of WFST. Combining catalogs with PS1 DR2 and Gaia DR3, we derive proper motions for candidate member stars in these two satellite galaxies over a 12-year time baseline, yielding uncertainties of ~1.8 mas/yr at 21 mag and ~3.0 mas/yr at 22 mag in the r band. The proper motions derived from bright and faint stars are consistent, indicating no significant variation in proper motion across stellar luminosity as these galaxies undergo tidal interactions with the MW. Meanwhile, we suggest that Bootes III represents the bound remnant of the progenitor galaxy that gave rise to the Styx stream, as evidenced by its elongated density profile and overdensity in both spatial and kinematic space. This is the first paper to use WFST to measure the proper motions of faint stars in Milky Way satellite galaxies. More detailed analyses will be presented in forthcoming papers from the wide field survey (WFS) program.
title A Glimpse of Satellite Galaxies in the Milky Way with the 2.5-meter Wide Field Survey Telescope (WFST): Bootes III and Draco
topic Astrophysics of Galaxies
url https://arxiv.org/abs/2506.20997