LOFAR Deep Fields: Probing the sub-mJy regime of polarized extragalactic sources in ELAIS-N1 - II. Analysis

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Volume 693 (January 2025)

A&A, 693 (2025) A100

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Table 6

Nearby superclusters in the field and their cluster members.

Source	RRM	ɀ_source	Supercluster	ɀ_supercluster	Cluster	RA, Dec, ɀ_cluster
	(rad m⁻²)					(deg, deg)
(1)	(2)	(3)	(4)	(5)	(6)	(7)
08	+5.73 ± 2.26	1.1215	MSCC 476 ^(a),SCL 162	0.065	A2168	243.27, +54.16, 0.064
12	−0.76 ± 2.23	0.9928			A2149A	240.35, +53.87, 0.0657

			MSCC 473^(b)	0.141	A2149E	240.35, +53.87, 0.139
					A2149F	240.35, +53.87, 0.142

Notes. (4) MSCC is the Main SuperCluster Catalog of Chow-Martínez et al. (2014). SCL: supercluster in the Einasto et al. 2001 catalog. (6) A2149 consists of several components along the same line of sight, so that the coordinates of the components are the same as those of A2149. (7) The redshifts of the clusters are from Chow-Martínez et al. (2014). ^(a)Supercluster with J2000 coordinates RA = 241.84°, Dec = 54.01°. This position corresponds to the geometrical center between the two members of the supercluster, A2168 and A2149A. The three-dimensional separation between the two clusters in the supercluster is 10.8 $h_{70}^{- 1}$ $h_{70}^{ - 1}$ Mpc (Chow-Martínez et al. 2014).^(b)Supercluster with J2000 coordinates RA = 240.35°, Dec = 53.87°. The two clusters in this supercluster are in the same position on the sky, and their line-of-sight separation is $12 h_{70}^{−1}$ $12 h_{70}^1$ Mpc (Chow-Martínez et al. 2014).

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