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Table 6

Main results obtained from the analysis of the optical spectra of the 7 type 1 AGNs.

Object F Hα * F Hβ F [OIII] Class z D L E(BV) NED name

(Mpc) Gal. AGN

PBC J0503.0+2300 699  ±  55 113  ±  23 93  ±  7 Sy1.5 0.058 259.3 0.515 0.424 2MASX J05025822+2259520
[2670  ±  153] [600  ±  64] [436  ±  45]
PBC J0543.6−2738 83.9  ±  18.4 107  ±  17 22.6  ±  3.1 Sy1.2 0.009 38.8 0.029 0 ESO 424-G012
[88  ±  14.9] [120  ±  9] [25.4  ±  3.2]
PBC J0814.4+0421 394  ±  35 43.9  ±  7.7 31.9  ±  2.3 NLS1 0.034 149.4 0.027 1.073 CGCG 031-072
[433  ±  37] [49.5  ±  7.8] [36.3  ±  5.6]
PBC J1345.4+4141 27.3  ±  1.5 0.7  ±  0.2 3.7  ±  1.8 Sy1.9 0.009 37.1 0.007 2.716 NGC 5290
[33.9  ±  1.9] [0.7  ±  0.2] [3.7  ±  1.8]
PBC J1439.0+1413 16.5  ±  3.1 Sy1.9 0.072 325.1 0.019 2MASX J14391186+1415215
[17.7  ±  3.2]
PBC J1453.0+2553 470  ±  68 111  ±  22 19.7  ±  3.3 Sy1 0.049 217.7 0.039 0.406 2MASX J14530794+2554327
[502  ±  72] [115  ±  22] [20.6  ±  3.3]
PBC J1546.5+6931 181  ±  20 26  ±  5 97.8  ±  8.6 Sy1.9 0.037 162.9 0.041 1.036 2MASX J15462424+6929102
[244  ±  23] [29  ±  5] [113  ±  16]

Notes. Emission line fluxes are reported both as observed and (between square brackets) corrected for the intervening Galactic absorption E(BV)Gal along the object line of sight (from Schlegel et al. 1998). Line fluxes are in units of 10-15 erg cm-2 s-1, the typical error on the redshift measurement is ± 0.001 except for the SDSS and 6dFGS spectra, for which an uncertainty of ± 0.0003 can be assumed.

(*)

Blended with [N ii] lines.

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