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王文婷

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A machine learning approach to infer the accreted stellar mass fractions of central galaxies in the TNG100 simulation

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Journal:MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY

ISSN No.:0035-8711

Translation or Not:no

Date of Publication:2022-08-01

Indexed by:期刊论文

Date of Publication:2022-08-01

Pre One:What to expect from dynamical modelling of cluster haloes - II. Investigating dynamical state indicators with Random Forest

Next One:The stellar mass in and around isolated central galaxies: Connections to the total mass distribution through galaxy-galaxy lensing in the Hyper Suprime-Cam survey

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