1. Zhang, W., Papadakis, I. E., Dov？iak, M., Bursa, M., Karas, V., A theoretical study of the time-lags due to Comptonization and the constraints on the X-ray corona in AGN, accepted for publication in Monthly Notices of the Royal Astronomical Society, 2022
2. Zhang, Wenda, Dov？iak, Michal, Bursa, Michal, Karas, Vladimír, Matt, Giorgio, Ursini, Francesco, Investigating the X-ray polarization of lamp-post coronae in BHXRBs, Monthly Notices of the Royal Astronomical Society, 2022, 515, 2882-2889
3. Zhang W., XMM-Newton detection of soft time lags in the TDE candidate AT 2018fyk, Monthly Notices of the Royal Astronomical Society Letters, 2022, 511, 19-23
4. Zhang W., Yu W., Karas V., Dovciak M., Probing the Bardeen-Petterson Effect in Tidal Disruption Events with Spectral line Reverberation Mapping, The Astrophysical Journal, 2019, 884, 72-79
5. Zhang W., Dovciak M., Bursa M.. Constraining the Size of the Corona with Fully Relativistic Calculations of Spectra of Extended Coronae. I. The Monte Carlo Radiative Transfer Code, The Astrophysical Journal, 2019, 875, 148-160
6. Zhang W., Yu W., Karas V., Dovciak M., Predictions for the Reverberating Spectral Line from a Newly Formed Black Hole Accretion Disk: Case of Tidal Disruption Flares, The Astrophysical Journal, 2015, 807, 89-100
7. Zhang W., Yu W., Low-frequency QPOs and Possible Change in the Accretion Geometry during the Outbursts of Aquila X-1, The Astrophysical Journal, 2015, 805, 139-146
8. Taverna R., Zhang W. et al., Towards a complete description of spectra and polarization of black hole accretion discs: albedo profiles and returning radiation, Monthly Notices of the Royal Astronomical Society, 2020, 493, 4960-4977
9. Yan Z., Zhang W., Soria R., Altamirano D., Yu W.. X-Ray Outbursts of ESO 243-49 HLX-1: Comparison with Galactic Low-mass X-Ray Binary Transients, The Astrophysical Journal, 2015, 811, 23-33
10.Yu W. & Zhang W., Energy-dependent Power Spectral States and Origin of Aperiodic Variability in Black Hole Binaries. The Astrophysical Journal, 2013, 770, 135-140
