Table 2: Spectral-type content of the volume-limited samples as a function of neighbour density.
neigh = 0 1 $\leq$ neigh $\leq$ 2 3 $\leq$ neigh $\leq$ 8 neigh > 8

M_B T₁ T₂ T₃₊₄ $\Sigma$ T₁ T₂ T₃₊₄ $\Sigma$ T₁ T₂ T₃₊₄ $\Sigma$ T₁ T₂ T₃₊₄ $\Sigma$

-22.0
153 94 17 264 297 102 14 413 281 52 10 343 51 1 0 52

-21.5 348 213 39 600 649 288 65 1002 684 175 40 899 184 23 0 207

-21.0 466 344 92 902 823 549 165 1537 1022 425 142 1589 392 77 22 491

-20.5 398 436 166 1000 830 701 325 1856 1057 641 279 1977 447 130 58 635

-20.0 254 427 206 887 652 656 445 1753 817 606 361 1784 411 171 88 670

-19.5 139 250 181 570 346 424 353 1123 441 377 303 1121 268 132 81 481

-19.0 81 147 153 381 157 255 280 692 177 217 264 658 128 73 76 277

-18.5 40 80 114 234 73 156 265 494 81 161 218 460 83 70 66 219

-18.0 15 42 71 128 33 107 159 299 44 114 163 321 66 64 58 188

-17.5 4 23 48 75 7 55 84 146 26 77 107 210 40 34 37 111

**Table 2:** Spectral-type content of the volume-limited samples as a function of neighbour density.
	neigh = 0	1 $\leq$ neigh $\leq$ 2	3 $\leq$ neigh $\leq$ 8	neigh > 8
M_B	T₁	T₂	T₃₊₄	$\Sigma$	T₁	T₂	T₃₊₄	$\Sigma$	T₁	T₂	T₃₊₄	$\Sigma$	T₁	T₂	T₃₊₄	$\Sigma$
-22.0	153	94	17	264	297	102	14	413	281	52	10	343	51	1	0	52
-21.5	348	213	39	600	649	288	65	1002	684	175	40	899	184	23	0	207
-21.0	466	344	92	902	823	549	165	1537	1022	425	142	1589	392	77	22	491
-20.5	398	436	166	1000	830	701	325	1856	1057	641	279	1977	447	130	58	635
-20.0	254	427	206	887	652	656	445	1753	817	606	361	1784	411	171	88	670
-19.5	139	250	181	570	346	424	353	1123	441	377	303	1121	268	132	81	481
-19.0	81	147	153	381	157	255	280	692	177	217	264	658	128	73	76	277
-18.5	40	80	114	234	73	156	265	494	81	161	218	460	83	70	66	219
-18.0	15	42	71	128	33	107	159	299	44	114	163	321	66	64	58	188
-17.5	4	23	48	75	7	55	84	146	26	77	107	210	40	34	37	111

Source LaTeX | All tables | In the text

	1 Introduction
	2 The sample
	3 The dependence on luminosity of the satellite-density distribution
	4 The dependence on satellite-density of the spectral-type/luminosity relation
	5 The role of satelite density for passive and SF galaxies
	6 The dependence on luminosity of the spectral-type/neighbour density relation
	7 Summary and conclusions
	References