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Table 2.

Measurements of the host galaxy, AGN continuum, and emission lines parameters with ULySS.

SDSS ID fλ(5100) AGN f Sp. index SSP f SSP age SSP cz SSP σ HβNCz OIII z FeII z FeII σ HβNCσ HβNC flux [OIII] σ [OIII] flux
[10−17erg s−1 cm−2 Å−1] [%] [%] [Myr] [km s−1 ] [km s−1 ] [km s−1] [km s−1] [km s−1] [km s−1] [km s−1] [⋆⋆] [km s−1] [⋆⋆]
(1) (2) (3) (4) (5) (6) (7) (8) (9) (10) (11) *(12) (13) (14) (15) (16)
J003657.17−100810.6 29.74 46.8 ± 0.3 −0.66 ± 0.23 44.0 ± 0.2 5398 ± 469 60 ± 9 196 ± 10 −8 ± 20 38 ± 6 288 ± 173 1635 ± 143 189 ± 26 2.80 ± 0.01 155 ± 10 6.21 ± 0.15
J010933.91+152559.0 10.87 50.9 ± 0.7 −0.04 ± 0.15 38.6 ± 0.7 4445 ± 905 119 ± 15 138 ± 17 4 ± 26 95 ± 29 30 ± 174 1492 ± 227 138 ± 31 1.86 ± 0.36 129 ± 40 1.45 ± 0.58
J011807.98+150512.9 10.02 55.8 ± 0.6 −0.25 ± 0.05 34.5 ± 0.6 6649 ± 245 −40 ± 20 170 ± 22 −60 ± 17 −43 ± 7 252 ± 62 1375 ± 252 119 ± 19 1.87 ± 0.04 139 ± 11 5.01 ± 0.66
J031715.10−073822.3 12.87 64.3 ± 0.6 −0.81 ± 0.04 27.3 ± 0.6 1595 ± 329 170 ± 16 104 ± 20 132 ± 11 145 ± 11 88 ± 97 1953 ± 799 145 ± 12 3.84 ± 0.28 102 ± 15 2.55 ± 0.17
J075059.82+352005.2 6.91 59.1 ± 0.4 −1.25 ± 0.06 33.5 ± 0.5 1431 ± 89 66 ± 10 95 ± 14 107 ± 18 104 ± 5 232 ± 138 1302 ± 155 129 ± 21 1.75 ± 0.23 153 ± 6 7.86 ± 0.22
082205.19+584058.3 8.00 69.2 ± 0.6 −0.25 ± 0.20 22.5 ± 0.6 6252 ± 477 −7 ± 26 127 ± 31 −45 ± 24 68 ± 13 568 ± 65 2256 ± 497 47 ± 24 0.82 ± 0.06 134 ± 19 3.74 ± 0.50
082205.24+455349.1 17.47 77.4 ± 0.4 −0.79 ± 0.01 13.7 ± 0.3 3493 ± 194 60 ± 21 100 ± 27 −5 ± 24 −3 ± 14 252 ± 106 1273 ± 89 76 ± 29 0.52 ± 0.52 186 ± 16 0.00 ± 0.44
091017.07+060238.6 12.22 50.3 ± 0.3 −2.00 ± 0.00 42.5 ± 0.3 3037 ± 74 154 ± 11 116 ± 13 99 ± 56 66 ± 12 176 ± 208 1408 ± 248 170 ± 70 0.86 ± 0.11 161 ± 20 4.59 ± 0.13
091020.11+312417.8 13.89 60.0 ± 0.5 −0.48 ± 0.11 34.2 ± 0.5 3434 ± 52 71 ± 14 151 ± 17 73 ± 15 45 ± 14 387 ± 145 1676 ± 623 147 ± 19 2.55 ± 0.10 124 ± 17 1.91 ± 0.21
092620.62+101734.8 9.46 47.7 ± 0.6 −0.12 ± 0.17 45.5 ± 0.6 5623 ± 206 66 ± 12 142 ± 15 61 ± 31 22 ± 23 872 ± 105 1310 ± 251 148 ± 36 1.70 ± 0.21 95 ± 37 1.16 ± 1.01
094249.40+593206.4 14.30 57.6 ± 0.5 −0.21 ± 0.03 35.6 ± 0.5 5724 ± 417 84 ± 12 137 ± 14 95 ± 29 39 ± 33 318 ± 158 1454 ± 206 173 ± 35 1.76 ± 0.06 135 ± 35 0.84 ± 1.96
094305.88+535048.4 9.69 51.4 ± 0.3 −1.85 ± 0.04 40.8 ± 0.3 4428 ± 352 14 ± 15 149 ± 17 35 ± 32 41 ± 12 -128 ± 80 1288 ± 284 176 ± 37 1.58 ± 0.37 154 ± 24 4.87 ± 0.64
103021.24+170825.4 16.30 64.1 ± 0.3 −0.90 ± 0.09 21.3 ± 0.3 9363 ± 290 134 ± 13 86 ± 16 173 ± 38 76 ± 25 -88 ± 278 1881 ± 118 47 ± 41 0.29 ± 0.04 212 ± 68 2.31 ± 0.17
105530.40+132117.7 38.72 70.4 ± 0.3 −1.20 ± 0.03 23.9 ± 0.2 3072 ± 246 41 ± 11 106 ± 14 −81 ± 32 93 ± 17 -215 ± 213 1701 ± 200 131 ± 37 0.72 ± 0.00 132 ± 0 2.26 ± 0.57
105705.40+580437.4 40.27 36.8 ± 0.5 −0.63 ± 0.09 55.9 ± 0.5 1601 ± 177 51 ± 9 144 ± 10 30 ± 15 −6 ± 27 253 ± 143 829 ± 77 81 ± 18 1.24 ± 2.31 130 ± 40 1.59 ± 0.98
112930.76+431017.3 20.58 35.2 ± 0.4 −1.10 ± 0.16 58.6 ± 0.3 3333 ± 159 100 ± 6 110 ± 8 87 ± 26 94 ± 23 364 ± 232 1378 ± 214 139 ± 31 1.47 ± 0.24 103 ± 35 1.19 ± 0.63
113630.11+621902.4 19.49 55.6 ± 0.5 −0.89 ± 0.10 36.4 ± 0.4 1933 ± 74 130 ± 14 143 ± 16 51 ± 26 −35 ± 10 327 ± 139 2206 ± 456 171 ± 33 3.00 ± 0.01 179 ± 14 7.16 ± 0.38
113651.66+445016.4 42.49 36.6 ± 0.3 −1.13 ± 0.22 57.1 ± 0.3 2535 ± 191 −8 ± 8 147 ± 9 −79 ± 12 67 ± 14 70 ± 294 1633 ± 340 165 ± 14 3.28 ± 0.21 84 ± 22 1.85 ± 0.38
123431.08+515629.2 11.37 40.4 ± 0.8 −0.17 ± 0.29 52.1 ± 0.8 2838 ± 408 40 ± 11 117 ± 13 44 ± 12 0 ± 14 368 ± 113 1391 ± 384 31 ± 0 1.97 ± 0.37 164 ± 19 4.48 ± 0.20
124533.87+534838.3 10.65 53.4 ± 0.6 −0.71 ± 0.13 38.3 ± 0.7 1355 ± 66 −8 ± 14 112 ± 18 34 ± 22 102 ± 34 385 ± 241 1464 ± 314 107 ± 28 1.27 ± 0.09 56 ± 64 0.28 ± 0.75
125219.55+182036.0 18.69 61.1 ± 0.5 −0.14 ± 0.07 30.9 ± 0.5 3182 ± 250 106 ± 14 142 ± 16 76 ± 32 77 ± 7 204 ± 156 1457 ± 208 166 ± 51 1.77 ± 0.20 73 ± 13 2.51 ± 0.13
133612.29+094746.8 12.96 48.4 ± 0.6 −0.19 ± 0.09 43.5 ± 0.5 6914 ± 709 79 ± 15 178 ± 16 −46 ± 42 54 ± 23 337 ± 106 1324 ± 179 153 ± 56 1.16 ± 0.58 84 ± 36 1.27 ± 0.13
134748.06+404632.6 13.72 44.5 ± 0.4 −0.84 ± 0.08 49.3 ± 0.4 4761 ± 427 122 ± 15 201 ± 16 −36 ± 122 14 ± 23 926 ± 88 1430 ± 386 289 ± 183 1.14 ± 0.14 88 ± 33 0.87 ± 0.11
134938.08+033543.8 18.60 50.0 ± 0.3 −1.81 ± 0.07 44.0 ± 0.2 5606 ± 738 90 ± 13 169 ± 14 35 ± 28 73 ± 10 -71 ± 250 1656 ± 339 159 ± 35 1.91 ± 0.43 190 ± 17 6.39 ± 0.06
135008.55+233146.0 20.82 66.1 ± 0.3 −0.73 ± 0.18 22.9 ± 0.3 3766 ± 229 80 ± 15 150 ± 18 85 ± 30 13 ± 15 193 ± 106 2500 ± 176 71 ± 34 0.34 ± 0.24 214 ± 16 0.00 ± 0.03
141131.86+442001.0 15.64 38.1 ± 0.4 −1.15 ± 0.15 55.3 ± 0.4 4704 ± 719 58 ± 15 221 ± 16 21 ± 44 −14 ± 5 1321 ± 148 995 ± 324 170 ± 56 1.18 ± 0.45 139 ± 6 5.52 ± 0.08
143651.50+343602.4 8.43 44.4 ± 0.4 −2.00 ± 0.00 47.3 ± 0.3 9489 ± 1150 4 ± 21 198 ± 22 −88 ± 54 −51 ± 12 192 ± 134 1755 ± 498 203 ± 62 2.26 ± 0.68 229 ± 13 0.00 ± 1.34
151600.39+572415.7 24.42 35.8 ± 0.6 −0.22 ± 0.05 57.6 ± 0.6 1595 ± 785 96 ± 9 172 ± 11 48 ± 17 −21 ± 13 313 ± 162 1286 ± 331 170 ± 22 3.06 ± 0.21 156 ± 18 3.13 ± 0.45
155950.79+512504.1 11.79 63.3 ± 0.6 −0.19 ± 0.11 27.8 ± 0.6 4366 ± 506 126 ± 21 152 ± 24 171 ± 24 48 ± 12 224 ± 179 1488 ± 235 144 ± 32 2.00 ± 0.32 120 ± 18 4.27 ± 0.07
161002.70+202108.5 18.09 40.7 ± 0.6 −0.07 ± 0.16 50.9 ± 0.6 3439 ± 397 79 ± 9 141 ± 11 24 ± 16 −34 ± 6 291 ± 126 1316 ± 178 155 ± 18 3.24 ± 0.20 153 ± 13 9.03 ± 0.16
162612.16+143029.0 8.57 40.7 ± 0.6 −0.29 ± 0.16 48.1 ± 0.5 11 220 ± 645 112 ± 16 198 ± 17 40 ± 27 435 ± 21 98 ± 152 2252 ± 302 253 ± 31 3.74 ± 0.30 138 ± 30 3.26 ± 0.17
170250.46+334409.6 20.89 50.8 ± 0.4 −0.30 ± 0.30 39.5 ± 0.3 9704 ± 392 50 ± 11 156 ± 12 108 ± 36 92 ± 12 279 ± 102 1324 ± 161 161 ± 48 1.54 ± 0.05 185 ± 18 5.65 ± 0.17

Notes. (1) SDSS ID of the object; (2) flux measured at 5100 Å in 10−17 erg s−1 cm2 Å−1 (hereafter in the table [⋆⋆]) (Richards et al. 2006); (3) fraction of power law continuum; (4) power law spectral index (errors present 1σ dispersion obtained from Monte Carlo simulations); (5) contribution of the host galaxy; (6) SSP age (errors present a dispersion obtained from Monte Carlo simulations); (7) mean stellar velocity; (8) stellar velocity dispersion (9) shift of the Hβ narrow component; (10) shift of narrow [OIII]λ5007 line; (11) shift of FeII lines; (12) width of FeII lines; (13) width of Hβ narrow component; (14) flux of Hβ narrow component; (15) width of narrow [OIII]λ5007 component; (16) flux of narrow [OIII]λ5007 component.

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