KiDS-Legacy: Cosmological constraints from cosmic shear with the complete Kilo-Degree Survey

Open Access

Table B.1.

Early-type galaxy sample properties for the mass-dependent intrinsic alignment model per tomographic bin.

Bin	⟨z⟩	${log}_{10} (\frac{⟨ L_{r} ⟩}{L_{0}})$ $\log_{10} \left( \frac{\langle L_r\rangle }{ L_0 } \right)$	log₁₀M_eff[h⁻¹ M_⊙]	f_r
1	0.34	−1.32	11.69	0.15
2	0.48	−0.72	12.46	0.20
3	0.59	−0.47	12.76	0.17
4	0.79	−0.28	12.93	0.24
5	0.94	−0.14	13.08	0.19
6	1.23	0.01	13.21	0.03

Notes. Columns, from left to right: tomographic bin number, mean redshift, logarithmic normalised galaxy luminosity in the r-band, logarithm of the effective halo mass, and the red galaxy fraction.

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.