王嵐

2008年獲得北京大學天體物理博士學位。2008年至2010年分別在中國科學院上海天文台和德國馬普天體物理研究所從事博士後研究。2010年入職中科院國家天文台工作至今。主要從事星系的形成和演化方面的研究，包括宇宙學數值模擬，以數值模擬為基礎建立星系形成和演化的統計模型等，同時對星系的形態從理論到觀測的多方面進行研究。發表文章20餘篇。 ^[1] 

1. Wang, Lan; Zheng, Zheng; Hao, Cai-Na et al., HI content of massive red spiral galaxies observed by FAST, 2022, MNRAS, 516, 2337

2. Zeng, Guangquan; Wang, Lan; Gao, Liang, Formation of massive disc galaxies in the IllustrisTNG simulation, 2021, MNRAS, 507, 3301

3. Wang, Lan; Xu, Dandan; Gao, Liang et al., Comparing galaxy morphology in hydrodynamical simulation and in semi-analytic model, 2019, MNRAS, 485, 2083

4. Wang, Lan; Wang, Lixin; Li, Cheng et al., The clustering of galaxies with pseudo-bulge and classical bulge in the local Universe, 2019, MNRAS, 484, 3865

5. Wang, Lan; Gonzalez-Perez, Violeta; Xie, Lizhi et al., The galaxy population in cold and warm dark matter cosmologies, 2017, MNRAS, 468, 4579

6. Wang, Lan; Weinmann, Simone M.; De Lucia, Gabriella, Yang, Xiaohu, Detection of galaxy assembly bias, 2013, MNRAS, 433, 515

7. Wang, Lan; Weinmann, Simone M.; Neistein, Eyal, A modified star formation law as a solution to open problems in galaxy evolution, MNRAS, 421, 3450

8. Wang, Lan; Jing, Y. P., Modelling galaxy stellar mass evolution from z ~ 0.8 to today, 2010, MNRAS, 402, 1796

9. Wang, Lan; Li, Cheng; Kauffmann, Guinevere; De Lucia, Gabriella, Modelling and interpreting the dependence of clustering on the spectral energy distributions of galaxies, 2007, MNRAS, 377, 1419

10. Wang, Lan; Li, Cheng; Kauffmann, Guinevere; De Lucia, Gabriella,Modelling galaxy clustering in a high-resolution simulation of structure formation, 2006, MNRAS, 371, 537 ^[1]