The eROSITA Final Equatorial-Depth Survey (eFEDS) - A complete census of X-ray properties of Subaru Hyper Suprime-Cam weak lensing shear-selected clusters in the eFEDS footprint

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Volume 661 (May 2022)

A&A, 661 (2022) A14

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

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Table 1

Properties of the shear-selected clusters within the eFEDS footprint.

eFEDS ID	^zMCMF		ID	z	M₅₀₀
(eFEDSJ+)		[10⁴³ erg s⁻¹]			[10¹⁴ M_⊙]
091403.3+013846	0.168		114	0.161
085931.9+030839	0.196		62	0.179
092241.9+020719	0.198		117	0.200
085751.6+031039	0.201		16	0.188
093403.5–001422	0.240		133	0.238
085230.6+002457	0.270		49	0.281
091351.1–004507	0.294		53	0.265
092844.0+005318	0.318		158	0.300
091610.1–002348	0.322		29	0.332
092121.2+031726	0.333		24	0.353
084528.6+032739	0.334		6	0.349
093431.3–002309	0.342		20	0.331
092846.5+000056	0.344		162	0.336
093302.7-010145	0.356		12	0.338
093513.0+004757	0.356		8	0.357
090805.9+011952	0.659		159	0.644

083654.6+025954	0.191		94	0.193
091849.0+021204	0.283		18	0.274
092209.3+034628	0.270		35	0.252
093546.3–000115	0.339		58	0.339
084129.0+002645	0.402		104	0.398

			141	0.160
			169	0.255
			146	0.356
			144	0.439

Notes. The horizontal lines divide the unique, primary and nonmatches categories (from top to bottom). Weak-lensing peaks not matched to an eFEDS cluster have no corresponding eFEDS ID and redshift.

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