The warm-hot intergalactic medium in inter-cluster filaments - A forecast for HUBS observations based on eRASS1 superclusters

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Table 7.

Properties of additional candidate filaments connected to massive clusters.

Filament Name	Cluster Name	z	M₅₀₀	D_phys	λ_fil	θ	O VIIIS/N
		(–)	(10¹⁴ M_⊙)	(Mpc)	(arcmin)	(deg)	(–)
J0859+0306	1eRASS J085751.0+031014	0.2025 ± 0.0012	$6 . 20_{- 0.67}^{+ 0.60}$ $6.20_{-0.67}^{+0.60}$	40.3	4.21	7.4	8.71
	1eRASS J085932.4+030832	0.1955 ± 0.0010	$1 . 84_{- 0.50}^{+ 0.41}$ $1.84_{-0.50}^{+0.41}$

J1242+2731	1eRASS J124325.7+271700	0.1924 ± 0.0022	$5 . 83_{- 0.65}^{+ 0.46}$ $5.83_{-0.65}^{+0.46}$	20.5	3.88	14.7	6.39
	1eRASS J124356.3+274155	0.1958 ± 0.0013	$2 . 19_{- 0.34}^{+ 0.27}$ $2.19_{-0.34}^{+0.27}$

Notes. Member clusters properties, geometrical properties, and O VIIIS/N of the two additional candidate filaments connected to massive clusters.

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