1.Hou, J. Xu, Z., Yuan, S., et al., 2020, 'Spectro-polarimetric observations at the NVST: I. instrumental polarization calibration and primary measurements', RAA, 20, 45
2.Xu, Z., Yang,K., Guo, Y. et al., 2017, 'Homologous Circular-ribbon Flares Driven by Twisted Flux Emergence', ApJ, 851, 30
3.Shen, J., Xu, Z. et al., 2022, 'Granular-scale Magnetic Flux Emergence and its Associated Features in an Emerging Active Region', ApJ, 925, 46
4.Xu,Z.,Lagg, A., Solanki, S., 2010,'Magnetic structure of an emerging flux region in the solar photosphere and chromosphere.',A&A, 520, 77.
5.Xu, Z. Lagg, A, Solanki ,S., 2012, 'Magnetic Fields of an Active Region Filament from Full Stokes Analysis of Si I 1082.7 and He I 1083.0 nm.', ApJ, 749 138.
6.Wang, R., Xu, Z., Jin, Z., Li, Z., Fu, Y., Liu,Z.., 2013, The first observation and data reduction of the Multi-wavelength Spectrometer on the New Vacuum Solar Telescope.,, RAA, 13, 1240.
7.Xu, Z., H noux, J. C., Chambe, G., Petrashen, A. G., Fang, C., 2006, 'First Results of Mg I (3p 1P1-4d 1D2) Line Linear Impact Polarization during the Solar Flare on 2001 June 15', ApJ, 650, 1193
8.Fang, C., Tang, Y., Xu, Z., et al., 2006, 'Spectral Analysis of Ellerman Bombs', ApJ, 643, 1325