Zobrazeno 1 - 10
of 199
pro vyhledávání: '"Tan Qinghua"'
Autor:
Li Jialiang, Li Jiaxi, Yang Yubing, He Xijing, Wei Xinyu, Tan Qinghua, Wang Yiqun, Xu Siyue, Chang Sue, Liu Weiwei
Publikováno v:
Open Life Sciences, Vol 18, Iss 1, Pp 1703608-71 (2023)
Externí odkaz:
https://doaj.org/article/94f848ec455a448caddc16b90ad6870c
Autor:
Sillassen, Nikolaj B., Jin, Shuowen, Magdis, Georgios E., Daddi, Emanuele, Wang, Tao, Lu, Shiying, Sun, Hanwen, Arumugam, Vinod, Liu, Daizhong, Brinch, Malte, D'Eugenio, Chiara, Gobat, Raphael, Gómez-Guijarro, Carlos, Rich, Michael, Schinnerer, Eva, Strazzullo, Veronica, Tan, Qinghua, Valentino, Francesco, Wang, Yijun, Xiao, Mengyuan, Zhou, Luwenjia, Blánquez-Sesé, David, Cai, Zheng, Chen, Yanmei, Ciesla, Laure, Dai, Yu, Delvecchio, Ivan, Elbaz, David, Finoguenov, Alexis, Gao, Fangyou, Gu, Qiusheng, Hale, Catherine, Hao, Qiaoyang, Huang, Jiasheng, Jarvis, Matt, Kalita, Boris, Ke, Xu, Bail, Aurelien Le, Magnelli, Benjamin, Shi, Yong, Vaccari, Mattia, Whittam, Imogen, Yang, Tiancheng, Zhang, Zhiyu
Publikováno v:
A&A 690, A55 (2024)
The NOEMA formIng Cluster survEy (NICE) is a large program targeting 69 massive galaxy group candidates at $z>2$ in six deep fields. We report spectroscopic confirmation of eight groups at $1.65\leq z\leq3.61$ in COSMOS. Homogeneously selected as sig
Externí odkaz:
http://arxiv.org/abs/2407.02973
Autor:
Tan Qinghua, Liu Yujie
Publikováno v:
Open Geosciences, Vol 12, Iss 1, Pp 1200-1211 (2020)
Lakes are important indicators of climate change. The change in lake water level objectively reflects the availability of regional water resources. Analyzing the changes in water level and climate response of major lakes in countries along the “Bel
Externí odkaz:
https://doaj.org/article/2cd17614c4584b87ad7a727a82417768
Autor:
Zhou, Luwenjia, Wang, Tao, Daddi, Emanuele, Coogan, Rosemary, Sun, Hanwen, Xu, Ke, Arumugam, Vinodiran, Jin, Shuowen, Liu, Daizhong, Lu, Shiying, Sillassen, Nikolaj, Wang, Yijun, Shi, Yong, Zhang, Zhi-Yu, Tan, Qinghua, Gu, Qiusheng, Elbaz, David, Bail, Aurelien Le, Magnelli, Benjamin, Gómez-Guijarro, Carlos, d'Eugenio, Chiara, Magdis, Georgios E., Valentino, Francesco, Ji, Zhiyuan, Gobat, Raphael, Delvecchio, Ivan, Xiao, Mengyuan, Strazzullo, Veronica, Finoguenov, Alexis, Schinnerer, Eva, Rich, R. Michael, Huang, Jiasheng, Dai, Yu, Chen, Yanmei, Gao, Fangyou, Yang, Tiancheng, Hao, Qiaoyang
Publikováno v:
A&A, 684, A196 (2024)
The study of distant galaxy groups and clusters at the peak epoch of star formation is limited by the lack of a statistically and homogeneously selected and spectroscopically confirmed sample. Recent discoveries of concentrated starburst activities i
Externí odkaz:
http://arxiv.org/abs/2310.15925
Autor:
Jiang, Yan, Li, Jiang-Tao, Gao, Yu, Bregman, Joel N., Ji, Li, Jiang, Xuejian, Tan, Qinghua, Wang, Jianfa, Wang, Q. Daniel, Yang, Yang
Molecular gas plays a critical role in explaining the quiescence of star formation (SF) in massive isolated spiral galaxies, which could be a result of either the low molecular gas content and/or the low SF efficiency. We present IRAM 30m observation
Externí odkaz:
http://arxiv.org/abs/2308.06750
Autor:
Zhou, Jing, Zhang, Zhi-Yu, Gao, Yu, Wang, Junzhi, Shi, Yong, Gu, Qiusheng, Yang, Chentao, Wang, Tao, Tan, Qinghua
Both Galactic and extragalactic studies on star formation suggest that stars form directly from dense molecular gas. To trace such high volume density gas, HCN and HCO+ J=1-0 have been widely used for their high dipole moments, relatively high abunda
Externí odkaz:
http://arxiv.org/abs/2207.13724
Autor:
Jin, Shuowen, Daddi, Emanuele, Magdis, Georgios E., Liu, Daizhong, Weaver, John R., Tan, Qinghua, Valentino, Francesco, Gao, Yu, Schinnerer, Eva, Calabro, Antonello, Gu, Qiusheng, Sese, David Blanquez
Publikováno v:
A&A 665, A3 (2022)
Using NOEMA and ALMA 3mm line scans, we measure spectroscopic redshifts of six new dusty galaxies at 3.5
Externí odkaz:
http://arxiv.org/abs/2206.10401
Autor:
Kalita, Boris S., Daddi, Emanuele, Bournaud, Frederic, Rich, R. Michael, Valentino, Francesco, Gómez-Guijarro, Carlos, Codis, Sandrine, Delvecchio, Ivan, Elbaz, David, Strazzullo, Veronica, Magalhaes, Victor de Sousa, Pety, Jérôme, Tan, Qinghua
Publikováno v:
A&A 666, A44 (2022)
We present well-resolved near-IR and sub-mm analysis of the three highly star-forming massive ($>10^{11}\,\rm M_{\odot}$) galaxies within the core of the RO-1001 galaxy group at $\rm z=2.91$. Each of them displays kpc-scale compact star-bursting core
Externí odkaz:
http://arxiv.org/abs/2206.05217
Autor:
Zhang, Yuheng, Zheng, Xian Zhong, Shi, Dong Dong, Gao, Yu, Dannerbauer, Helmut, An, Fang Xia, Shu, Xinwen, Gao, Zhen-Kai, Wang, Wei-Hao, Wang, Xin, Cai, Zheng, Fan, Xiaohui, Fang, Min, Pan, Zhizheng, Liu, Wenhao, Tan, Qinghua, Qin, Jianbo, Ren, Jian, Qiao, Man, Wen, Run, Liu, Shuang
Submillimetre galaxies represent a rapid growth phase of both star formation and massive galaxies. Mapping SMGs in galaxy protoclusters provides key insights into where and how these extreme starbursts take place in connections with the assembly of t
Externí odkaz:
http://arxiv.org/abs/2203.09260
Autor:
Qin, Jianbo, Zheng, Xian Zhong, Fang, Min, Pan, Zhizheng, Wuyts, Stijn, Shi, Yong, Peng, Yingjie, Gonzalez, Valentino, Bian, Fuyan, Huang, Jia-Sheng, Gu, Qiu-Sheng, Liu, Wenhao, Tan, Qinghua, Shi, Dong Dong, Ren, Jian, Zhang, Yuheng, Qiao, Man, Wen, Run, Liu, Shuang
While the slope of the dust attenuation curve ($\delta$) is found to correlate with effective dust attenuation ($A_V$) as obtained through spectral energy distribution (SED) fitting, it remains unknown how the fitting degeneracies shape this relation
Externí odkaz:
http://arxiv.org/abs/2201.05467