Based on a large group/cluster catalog recently constructed from the DESI Legacy Imaging Surveys DR9 using an extended halo-based group finder, we measure and model the group-galaxy weak lensing signals for groups/clusters in a few redshift bins within redshift range $0.1 \leqslant z<0.6$. Here, the background shear signals are obtained based on the DECaLS survey shape catalog derived with the \textsc{Fourier\_Quad} method. We divide the lens samples into 5 equispaced redshift bins and 7 mass bins, which allow us to probe the redshift and mass dependence of the lensing signals and hence the resulting halo properties. In addition to these sample selections, we have also checked the signals around different group centers, e.g., brightest cent...
The Kilo-Degree Survey is an optical wide-field survey designed to map the matter distribution in th...
We infer the connection between the stellar mass of galaxies from the Subaru Hyper Suprime-Cam (HSC)...
The Kilo-Degree Survey is an optical wide-field survey designed to map the matter distribution in th...
Galaxy-galaxy lensing is rapidly becoming one of the most promising means to accurately measure the ...
Galaxy-galaxy lensing is rapidly becoming one of the most promising means to accurately measure the ...
Galaxy-galaxy lensing is rapidly becoming one of the most promising means to accurately measure the ...
We present a maximum-likelihood weak lensing analysis of the mass distribution in optically selected...
We present a maximum-likelihood weak lensing analysis of the mass distribution in optically selected...
The Kilo-Degree Survey is an optical wide-field survey designed to map the matter distribution in th...
The Kilo-Degree Survey is an optical wide-field survey designed to map the matter distribution in th...
The Kilo-Degree Survey is an optical wide-field survey designed to map the matter distribution in th...
We present a maximum-likelihood weak-lensing analysis of the mass distribution in optically selected...
This is the first in a series of papers on the weak lensing effect caused by clusters of galaxies in...
We infer the connection between the stellar mass of galaxies from the Subaru Hyper Suprime-Cam (HSC)...
The Kilo-Degree Survey (KiDS) is an optical wide-field survey designed to map the matter distributio...
The Kilo-Degree Survey is an optical wide-field survey designed to map the matter distribution in th...
We infer the connection between the stellar mass of galaxies from the Subaru Hyper Suprime-Cam (HSC)...
The Kilo-Degree Survey is an optical wide-field survey designed to map the matter distribution in th...
Galaxy-galaxy lensing is rapidly becoming one of the most promising means to accurately measure the ...
Galaxy-galaxy lensing is rapidly becoming one of the most promising means to accurately measure the ...
Galaxy-galaxy lensing is rapidly becoming one of the most promising means to accurately measure the ...
We present a maximum-likelihood weak lensing analysis of the mass distribution in optically selected...
We present a maximum-likelihood weak lensing analysis of the mass distribution in optically selected...
The Kilo-Degree Survey is an optical wide-field survey designed to map the matter distribution in th...
The Kilo-Degree Survey is an optical wide-field survey designed to map the matter distribution in th...
The Kilo-Degree Survey is an optical wide-field survey designed to map the matter distribution in th...
We present a maximum-likelihood weak-lensing analysis of the mass distribution in optically selected...
This is the first in a series of papers on the weak lensing effect caused by clusters of galaxies in...
We infer the connection between the stellar mass of galaxies from the Subaru Hyper Suprime-Cam (HSC)...
The Kilo-Degree Survey (KiDS) is an optical wide-field survey designed to map the matter distributio...
The Kilo-Degree Survey is an optical wide-field survey designed to map the matter distribution in th...
We infer the connection between the stellar mass of galaxies from the Subaru Hyper Suprime-Cam (HSC)...
The Kilo-Degree Survey is an optical wide-field survey designed to map the matter distribution in th...