The eROSITA Final Equatorial-Depth Survey (eFEDS) - X-ray observable-to-mass-and-redshift relations of galaxy clusters and groups with weak-lensing mass calibration from the Hyper Suprime-Cam Subaru Strategic Program survey

The Early Data Release of eROSITA and Mikhail Pavlinsky ART-XC on the SRG mission

Free Access

Table 1

Summary of the priors used in the modeling (see Sect. 5.4 for more details).

Parameter	Prior
	The M_WL−M₅₀₀−z relation Eq. (42)

A_WL	or
B_WL	or
γwL	or
σ_wL	or

	The η−M₅₀₀−z relation Eq. (48) with

A_η
B_η
δ_η
γ_η
σ_η	and
A_f
B_f
δ_f
γ_f

	The χ−M₅₀₀−z relation Eq. (46)

B_χ
δ_χ
γ_χ
σ_χ

	χ = L_X with

	χ = L_b with

	χ = T_X with

	χ = Mg with

	χ = Y_X with

	Correlated scatter



	Mislefting

f_mis
σ_mis

	Cosmological parameters

Ω_M
σ₈
H₀

Notes. The first and second columns represent the name of and the prior on the parameters, respectively. The former and latter priors on the parameters of the M_WL−M₅₀₀−z relation describe the cases of modeling the lensing profile with R > 0.2h⁻¹Mpc and R > 0.5h⁻¹Mpc, respectively.

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.