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Table 3.

Redshift, distances, sizes, stellar masses, sSFRs, metallicities, EWs, and He II λ4684 fluxes of the proposed BBs.

ID redshift. Dist. size log M log sSFR metallicity EW[O II] EWHβ EWO III EWHα log fHe II Compact
MPA HEC/S HEC SED SED MPA MPA MPA MPA MPA FADO
(Mpc) (kpc) (M) (yr−1) (12+log(O/H)) (Å) (Å) (Å) (Å) (erg s−2 cm−2)
1 157 6.9 −7.4 N
2 0.0399 182 1.9 7.0 −7.0 8.6 89 191 1194 1000 −15.8 N
3 75 3.9 6.4 −6.8 N
4 0.0388 176 2.0 7.3 −7.6 7.7 54 183 1186 841 −16.2 Y
5 0.0292 131 4.1 5.9 −6.3 7.9 31 125 711 577 N
6 151 8.4 7.0 −7.2 N
7 0.0421 192 5.1 7.6 −6.4 7.8 49 202 1143 1028 −15.3 Y
8 0.0281 127 2.5 7.2 −7.7 32 230 1119 1038 −16.2 Y
9 0.0325 147 4.9 7.8 −7.1 7.9 64 236 1583 1348 −15.4 Y
10 0.038 172 3.2 6.8 −6.5 7.8 49 195 1202 1283 −15.9 Y
11 0.0377 171 1.8 8.2 −7.5 7.8 76 193 1103 1086 −15.0 Y
12 0.0225 101 1.4 6.4 −6.9 7.9 251 1896 1460 −15.6 Y
13 143 7.6 −8.4 N
14 0.0327 148 1.9 7.3 −7.4 7.9 36 289 2062 1296 −15.8 Y
15 187 2.4 7.9 −7.7 N
16 128 4.8 7.1 −6.4 N
17 185 7.8 −7.6 Y
18 0.0331 150 2.0 7.0 −7.1 7.7 60 168 856 853 −15.7 Y
19 150 2.4 7.6 −7.5 Y
20 0.0203 91 4.3 7.0 −7.4 8.1 296 1893 1284 −16.0 N
21 116 2.1 7.1 −6.9 Y
22 0.0227 102 5.4 8.3 −6.6 237 −14.7 Y
23 130 3.3 7.8 −8.1 Y
24 126 6.4 6.4 −7.0 N
25 0.0224 101 1.6 6.2 −6.9 7.9 255 1301 1279 Y
26 177 2.1 6.7 −8.0 Y
27 0.0404 184 2.7 7.7 −7.1 7.9 54 104 583 548 −15.7 Y
28 93 3.4 8.1 −8.7 Y
29 108 7.7 −7.8 Y
30 0.0328 148 2.2 7.4 −7.5 7.8 50 129 638 743 −15.2 Y
31 0.0433 197 3.4 7.9 −7.1 8.1 79 76 362 379 −15.7 N
32 0.0274 123 5.0 8.8 −8.0 8.0 73 148 1005 792 −15.1 Y
33 0.0277 125 3.5 7.8 −8.0 8.6 75 132 839 703 −15.6 N
34 0.0263 118 7.0 7.0 −7.0 8.3 134 649 685 −16.1 N
35 95 7.4 −8.0 Y
36 0.0225 101 1.1 6.6 −7.1 7.8 168 883 795 −15.9 Y
37 122 6.5 −7.1 N
38 140 2.9 7.7 −6.3 Y
39 155 6.9 −6.4 N
40 161 4.6 6.6 −7.0 N
41 162 5.4 7.2 −7.2 Y
42 18 1.3 7.1 −8.7 N
43 181 5.2 7.7 −8.0 N
44 85 2.7 6.8 −7.0 Y
45 162 4.5 6.7 −6.5 N
46 130 2.1 7.4 −7.6 N
47 124 1.3 7.3 −7.0 Y
48 107 4.0 6.9 −7.1 N

Notes. “MPA” refers to results provided by MPA-JHU, “HEC” to HECATE, “S” to spectral fitting, and “SED” to SED fitting. Distances are as reported in HECATE except for objects with spectroscopic observations, where distances are based on their redshift. Y = Yes and N = No if the BB is compact based on visual inspection. Uncertainties are provided in the table available at the CDS.

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