First author:
[1]."The THREE HUNDRED Project: the evolution of physical baryon profiles"
Qingyang Li, Weiguang Cui, Xiaohu Yang, Romeel Dave, Elena Rasia, Stefano Borgani, Meneghetti
Massimo, Alexander Knebe, Klaus Dolag, and Jack Sayers, 2023, MNRAS, 523, 1228
[2]."Groups and Protocluster Candidates in the CLAUDS and HSC-SSP Joint Deep Surveys"
Qingyang Li, Xiaohu Yang, Chengze Liu, Yipeng Jing, Min He, Jia-Sheng Huang, Y. Sophia Dai, Marcin
Sawicki, Stephane Arnouts, Stephen Gwyn, Thibaud Moutard, H. J. Mo, Kai Wang, Antonios Katsianis,
Weiguang Cui, Jiaxin Han, I. Non Chiu, Yizhou Gu, and Haojie Xu, 2022, ApJ, 933, 9
[3]."What to expect from dynamical modelling of cluster haloes II. Investigating dynamical state indicators with Random Forest"
Qingyang Li, Jiaxin Han, Wenting Wang, Weiguang Cui, Federico De Luca, Xiaohu Yang, Yanrui Zhou,
and Rui Shi, 2022, MNRAS, 514, 5890
[4]."What to expect from dynamical modelling of cluster haloes I. The information content of different dynamical tracers"
Qingyang Li, Jiaxin Han, Wenting Wang, Weiguang Cui, Zhaozhou Li, and Xiaohu Yang, 2021, MNRAS, 505, 3907
[5]."The Three Hundred project: the stellar and gas profiles"
Qingyang Li, Weiguang Cui, Xiaohu Yang, Elena Rasia, Romeel Dave, Marco De Petris, Alexander
Knebe, John A. Peacock, Frazer Pearce, and Gustavo Yepes, 2020, MNRAS, 495, 2930
[1]."Measuring the X-ray luminosities of DESI groups from eROSITA Final Equatorial-Depth Survey - I. X-ray luminosity-halo mass scaling relation"
Zheng Y., Yang X., He M., Shen S., Li Q., Li X., 2023, MNRAS, 523, 4909
[2]."Late-formed haloes prefer to host quiescent central galaxies - I. Observational results"
Wang K., Chen Y., Li Q., Yang X., 2023, MNRAS, 522, 3188
[3]."DarkAI: I. Mapping the large-scale density field of dark matter using AI"
Wang Z., Shi, F., Yang X., Li Q., Liu Y., Li X., arXiv:2305.11431
[4]."The impact of halo concentration on the Sunyaev Zel'dovich effect signal from massive galaxy clusters"
Baxter E., Pandey S., Adhikari S., Cui W., Shin T., Li Q., Rasia E., arXiv:2304.08731
[5]."Halo Properties and Mass Functions of Groups/Clusters from the DESI Legacy Imaging Surveys DR9"
Wang J., Yang X., Zhang J., Li H., Fong M., Xu H., He M., Gu Y., Luo W., Dong F., Wang Y., Li, Q., Katsianis A., Wang H., Shen Z., Alonso V., Liu C., Huang Y., Liu Z., 2022, ApJ, 936, 161
[6]."A machine learning approach to infer the accreted stellar mass fractions of central galaxies in the TNG100 simulation"
Shi R., Wang W., Li Z., Han J., Shi J., Rodriguez-Gomez V., Peng Y., Li Q., 2022, MNRAS, 515, 3938
[7]."THE THREE HUNDRED project: The GIZMO-SIMBA run"
Cui W., Dave R., Knebe A., Rasia E., Gray M., Pearce F., Power C., Yepes G., Anbajagane D., Ceverino D., Contreras-Santos A., de Andres D., De Petris M., Ettori S., Haggar R., Li Q., Wang Y., Yang X., Borgani S., Dolag K., Zu Y., Kuchner U., Canas R., Ferragamo. A., Gianfagna G., 2022, MNRAS, 514, 977
[8]."An Extended Halo-based Group/Cluster Finder: Application to the DESI Legacy Imaging Surveys DR8"
Yang X., Xu H., He M., Gu Y., Katsianis A., Meng J., Shi F., Zou H., Zhang Y., Liu C., Wang Z., Dong F., Lu Y., Li Q., Chen Y., Wang H., Mo H., Fu J., Guo H., Leauthaud A., Luo Y., Zhang J., Zu Y., 2021, ApJ, 909, 143