The Sloan great wall. Rich clusters | Astronomy & Astrophysics (A&A)

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Table 3

Galaxy populations in rich clusters.

(1)	(2)	(3)	(4)	(5)	(6)	(7)	(8)	(9)	(10)	(11)

Scl ID	No	ID	(g − r)_mean	F _red	F_ell	F_rs	slope_red	SD_red	SD_Ered	SD_Sred

SCl 91	1	1066	0.73	0.73	0.36	0.58	–0.024	0.043	0.024	0.053
	2	1205	0.68	0.62	0.38	0.45	–0.012	0.030	0.027	0.033
SCl 111	3	1424	0.73	0.71	0.44	0.49	–0.007	0.046	0.033	0.057
	4	1516	0.76	0.85	0.56	0.34	–0.018	0.032	0.032	0.033
SCl 126	5	1650 ×	0.78	0.94	0.56	0.40	–0.010	0.039	0.036	0.042
	6	1658 ×	0.74	0.83	0.58	0.29	–0.026	0.029	0.031	0.024
	7	1663 ×	0.75	0.83	0.49	0.43	–0.007	0.037	0.032	0.042
	8	1750 ×	0.78	0.91	0.62	0.33	–0.013	0.042	0.041	0.046
	9	1773 ×	0.73	0.77	0.53	0.41	–0.011	0.040	0.032	0.048
	10	1809	0.75	0.84	0.51	0.43	–0.015	0.029	0.027	0.032

Notes. Columns in the table are as follows: Cols. 1–3: supercluster ID, cluster No and Abell ID, Col. 4: (g − r)_mean – the mean g − r colour of galaxies, Cols. 5–11: fraction of red galaxies, fraction of elliptical galaxies, fraction of spirals among red galaxies, and the slope and the rms scatter of the red sequence in the colour–magnitude diagram (the scatter of all red galaxies, and that of red ellipticals and red spirals).

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