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Table 2.

Halo mass estimate methods in this work.

Method Input SHMR SMF Overdensity NFW fit Assumption
(Stellar mass scaling with SHMR)

Mh(1) M*, BCG Behroozi et al. (2013)
Mh(2a) M*, tot Shuntov et al. (2022) Muzzin et al. (2013) Virialization
Mh(2b) M*, tot van der Burg et al. (2014) Muzzin et al. (2013) Virialization

(Galaxy overdensity-based)
Mh(3) This work Virialization

(M* surface density profile fitting)
Mh(4) ΣM*(R) This work NFW profile
Mh(5) ΣM*(R) This work NFW profile and fixed c( * )

Notes. The details are described in Sect. 4.4, and the results are presented on Table 4. ( * )c is the concentration parameter of the dark matter halo.

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