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Home All issues Volume 507 / No 3 (December I 2009) A&A, 507 3 (2009) 1345-1358 Full HTML
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Table 2:

Main results obtained from the analysis of the optical spectra of the 17 AGNs of the present sample of Swift sources.
Object $F_{\rm H_\alpha}$ $F_{\rm H_\beta}$ $F_{\rm [OIII]}$ Class z DL E(B-V) $L_{\rm Radio}$
            (Mpc) Gal. AGN (erg s-1)
Swift J0059.4+3150 * 87 $\pm$ 5 37 $\pm$ 2 Sy1.2 0.015 84.2 0.061 - -
  * [105 $\pm$ 6] [45 $\pm$ 3]            
Swift J0134.1-3625 9.4 $\pm$ 0.3 in abs. 5.3 $\pm$ 2.2 Sy2 0.029 136.7 0.020 - -
  [9.9 $\pm$ 0.4] [in abs.] [5.6 $\pm$ 2.3]            
Swift J0342.0-2115 * 2000 $\pm$ 400 400 $\pm$ 80 Sy1 0.0139 67.6 0.032 - -
  * [2700 $\pm$ 600] [460 $\pm$ 90]            
Swift J0350.1-5019 38 $\pm$ 3 6.9 $\pm$ 0.9 11 $\pm$ 1 Sy2 0.035 165.8 0.015 0.216 -
  [39 $\pm$ 3] [7.2 $\pm$ 0.9] [11 $\pm$ 1]            
Swift J0505.7-2348 38 $\pm$ 1 9 $\pm$ 1 48 $\pm$ 1 Sy2 0.036 172.1 0.040 0.144 $3.1 \times 10^{38}$ (1.4 GHz)
  [41 $\pm$ 1] [10 $\pm$ 1] [55 $\pm$ 1]            
Swift J0501.9-3239 180 $\pm$ 20 52 $\pm$ 11 320 $\pm$ 30 Sy2 0.0126 58.9 0.017 0.036 7.0 $\times$ 1037 (843 MHz)
  [190$\pm$20] [59 $\pm$ 13] [350 $\pm$ 30]            
Swift J0640.1-4328 3.1 $\pm$ 0.5 0.7 $\pm$ 0.3 2.3 $\pm$ 0.4 Sy2 0.061 293.9 0.084 - 8.1 $\times$ 1039 (843 MHz)
  [4.1 $\pm$ 0.7] [3.6 $\pm$ 1.7] [3.0 $\pm$ 0.6]            
Swift J0727.5-2406 * 2.1 $\pm$ 0.7 21 $\pm$ 1 Sy1.9 0.123 619.0 1.047 - $1.9 \times 10^{40}$ (1.4 GHz)
  * [47 $\pm$ 7] [385 $\pm$ 17]            
Swift J0739.6-3144 36 $\pm$ 2 2.3 $\pm$ 0.5 32 $\pm$ 1 Sy2 0.026 122.3 0.613 0.360 2.5 $\times$ 1038 (1.4 GHz)
  142 $\pm$ 7 [18 $\pm$ 4] [216 $\pm$ 5]           $6.4 \times 10^{38}$ (843 MHz)
Swift J0743.0-2543 * 11 $\pm$ 2 4.5 $\pm$ 0.7 Sy1.2 0.023 108.0 0.678 - $1.2 \times 10^{37}$ (1.4 GHz)
  * [146 $\pm$ 20] [38 $\pm$ 6]            
Swift J0811.5+0937 - in abs. - XBONG 0.286 1582.6 0.026 - $ 1.8 \times 10 ^{40}$ (1.4 GHz)
    [in abs.]              
Swift J0902.0+6007 * $52 \pm 5$ $98 \pm 5$ Sy2 0.012 56.2 0.043 0.198 $1.6 \times 10^{38}$ (1.4 GHz)
  * [58 $\pm$ 6] [114 $\pm$ 6]            
Swift J0904.3+5538 * 30.9 $\pm$ 7.9 23.1 $\pm$ 0.8 Sy1.5 0.0374 177.4 0.021 - -
  * [36.1 $\pm$ 9.9] [24.5 $\pm$ 0.9]            
Swift J0911.2+4533 4.2 $\pm$ 0.2 <0.3 4.4 $\pm$ 0.2 Sy2 0.0269 127.1 0.019 >0.360 $8.4 \times 10^{37}$ (1.4 GHz)
  [4.4 $\pm$ 0.2] [< 0.2] [4.4 $\pm$ 0.3]            
Swift J0917.2-6221 * 1450 $\pm$ 40 270 $\pm$ 3 Sy1.2 0.057 274.3 0.182 - $4.7 \times 10^{39}$ (843 MHz)
  * [2380 $\pm$ 60] [518 $\pm$ 6]            
Swift J0923.7+2255 * 127 $\pm$ 13 92 $\pm$ 4 NLSy1 0.034 160.9 0.043 - $4.5 \times 10^{38}$ (1.4 GHz)
  * [140 $\pm$ 14] [105 $\pm$ 5]            
Swift J1049.4+2258 26 $\pm$ 1 4.4 $\pm$ 0.4 87 $\pm$ 1 Sy2 0.033 156.0 0.029 0.261 -
  [29 $\pm$ 1] [4.7 $\pm$ 0.5] [$93 \pm 1$]            

Note: emission line fluxes are reported both as observed and (between square brackets) corrected for the intervening Galactic absorption $E(B-V)_{\rm Gal}$ 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 $\pm$0.001 but for the SDSS and 6dFGS spectra, for which an uncertainty of $\pm$0.0003 can be assumed; *: heavily blended with [N II] lines.


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