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[1] What to expect from dynamical modelling of galactic haloes - II. The spherical Jeans equation MNRAS, 2018,
[2]wangwenting. Do satellite galaxies trace matter in galaxy clusters? MNRAS, 2018,
[3] What to expect from dynamical modelling of galactic haloes MNRAS, 2017,
[4]wangwenting. Galaxy formation in the Planck cosmology - IV. Mass and environmental quenching, conformity and clustering MNRAS, 2017,
[5]wangwenting. Predictions for the detection of tidal streams with Gaia using great-circle methods MNRAS, 2017,
[6]wangwenting. Strong bimodality in the host halo mass of central galaxies from galaxy-galaxy lensing MNRAS, 2016,
[7]wangwenting. A sample of galaxy pairs identified from the LAMOST spectral survey and the Sloan Digital Sky Survey RAA, 2016,
[8] A weak gravitational lensing recalibration of the scaling relations linking the gas properties of dark haloes to their mass MNRAS, 2016,
[9]wangwenting. The orbital PDF: general inference of the gravitational potential from steady-state tracers MNRAS, 2016,
[10]wangwenting. The orbital PDF: the dynamical state of Milky Way sized haloes and the intrinsic uncertainty in the determination of their masses MNRAS, 2016,
[11]wangwenting. Planck intermediate results. XXXVII. Evidence of unbound gas from the kinetic Sunyaev-Zeldovich effect A&A, 2016,
[12]wangwenting. Evidence of the Missing Baryons from the Kinematic Sunyaev-Zeldovich Effect in Planck Data PhRvL, 2015,
[13] Estimating the dark matter halo mass of our Milky Way using dynamical tracers MNRAS, 2015,
[14]wangwenting. Planes of satellite galaxies: when exceptions are the rule MNRAS, 2015,
[15]wangwenting. Unifying X-ray scaling relations from galaxies to clusters MNRAS, 2015,
total56 3/4
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