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Table 1:

Best fit models for the HLIRG's SED.

Source 		z Type CTa Best Fit modelb $\log L_{\rm BOL}$c AGN / SBd
        all datae no X-raysf composite temp.g (erg s-1)  
        Model $\alpha$ Model $\alpha$      

Class A HLIRG 		   

PG 1206+459 		1.158 QSO N AGN1-L ... 1 AGN1 ... 1 AGN1-L 48.4 1 / 0
PG 1206+459 2.038 QSO N AGN1-L ... 1 AGN1 ... 1 AGN1-L 49.2 1 / 0
PG 1206+459 0.780 QSO N AGN1-L SB1 0.3 AGN1 SB4 0.5 AGN1-L+SB1 47.7 0.3 / 0.7
PG 1206+459 0.323 QSO N ... SB2 0 AGN1 SB2 0.3 SB2 46.7 0.3 / 0.7
PG 1206+459 1.21 QSO N AGN1 SB1 0.4 AGN1 SB1 0.3 AGN1+SB1 47.2 0.4 / 0.6
PG 1206+459 1.334 QSO N AGN1-L ... 1 AGN1 ... 1 AGN1-L 48.9 1 / 0
PG 1206+459 0.297 QSO N AGN1 SB3 0.8 AGN1 SB3 0.8 AGN1+SB3 47.4 0.8 / 0.2

Class B HLIRG 		   

PG 1206+459 		0.575 NL-SB  Y ... SB3 0 ... SB3 0 CP1 46.7 $\sim$0.5 / $\sim$0.5
PG 1206+459 0.292 SB  N AGN4 SB1 0.06 AGN3 SB1 0.3 CP1 47.0 $\sim$0.5 / $\sim$0.5
PG 1206+459 0.327 QSO 2 Y AGN3 SB4 0.06 AGN3 SB3 0.3 CP1 46.6 $\sim$0.5 / $\sim$0.5
PG 1206+459 0.442 QSO 2 Y AGN4 SB4 0.09 AGN3 SB1 0.8 CP2 47.3 $\sim$0.7 / $\sim$0.3
PG 1206+459 0.32 Sy2 Y AGN5 SB4 0.06 AGN3 SB2 0.9 CP2 46.7 $\sim$0.7 / $\sim$0.3
PG 1206+459 0.926 QSO 2 Y AGN1 SB3 0.03 AGN3 SB1 0.8 CP1 47.9 $\sim$0.5 / $\sim$0.5

Notes. (a) Compton-thick candidates.
(b) The best fit adopted to estimate the bolometric luminosity and the AGN and SB fraction is marked in bold fonts.
(c) Bolometric luminosity in CGS units.
(d) Fraction of the bolometric luminosity originated in AGN and SB. Calculated through the parameter $\alpha$ of the best-fit model.
(e) Best fit using our original set of templates.
(f) Best fit not using X-ray data.
(g) Best fit including the templates of composite sources.


Source LaTeX | All tables | In the text

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