WEAK LENSING CALIBRATED<i>M</i>-<i>T</i>SCALING RELATION OF GALAXY GROUPS IN THE COSMOS FIELD
WEAK LENSING CALIBRATED<i>M</i>-<i>T</i>SCALING RELATION OF GALAXY GROUPS IN THE COSMOS FIELD
The scaling between X-ray observables and mass for galaxy clusters and groups is instrumental for cluster-based cosmology and an important probe for the thermodynamics of the intracluster gas. We calibrate a scaling relation between the weak lensing mass and X-ray spectroscopic temperature for 10 galaxy groups in the COSMOS field, …