The integral high-energy cut-off distribution of type 1 active galactic nuclei
The integral high-energy cut-off distribution of type 1 active galactic nuclei
 
  In this Letter we present the primary continuum parameters, the photon index ?, and the high-energy cut-off E c of 41 type-1 Seyfert galaxies extracted from the International Gamma-Ray Astrophysics Laboratory (INTEGRAL) complete sample of active galactic nuclei (AGNs). We performed broadband (0.3-100 keV) spectral analysis by simultaneously fitting the soft and hard X-ray spectra obtained by XMM and INTEGRAL/IBIS-Swift/BAT, respectively, in order to investigate the general properties of these parameters, in particular their distribution and mean values. We find a mean photon index of 1.73 with a standard deviation of 0.17 and a mean high-energy cut-off of 128 keV with a standard deviation of 46 keV for the whole sample. This is the first time that the cut-off energy is constrained in such a large number of AGNs. We have 26 measurements of the cut-off, which corresponds to 63% of the entire sample, distributed between 50 and 200 keV. There are a further 11 lower limits mostly below 300 keV. Using the main parameters of the primary continuum, we have been able to obtain the actual physical parameters of the Comptonizing region, i.e., the plasma temperature kT e from 20 to 100 keV and the optical depth ? < 4. Finally, with the high signal-to-noise ratio spectra starting to come from NuSTAR it will soon be possible to better constrain the cut-off values in many AGNs, allowing the determination of more physical models and thus better understand the continuum emission and geometry of the region surrounding black holes.
  
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      Malizia, A.
      
        efa63850-cf26-482c-ae3b-54b0c8fb8a87
      
     
  
    
      Molina, M.
      
        28a3f3b6-aedf-4fa5-9a4f-dbcba001435d
      
     
  
    
      Bassani, L.
      
        07e5602c-f97e-4334-a0fa-c2212431a61a
      
     
  
    
      Stephen, J.B.
      
        c0b1afce-f3d9-4568-b2c1-51482f80cd9a
      
     
  
    
      Bazzano, A.
      
        8eef0c6e-1a5f-4bcd-a034-9a5c3b29104d
      
     
  
    
      Ubertini, P.
      
        7035748e-152c-473e-8766-a2fa3ac49fcb
      
     
  
    
      Bird, A.J.
      
        045ee141-4720-46fd-a412-5aa848a91b32
      
     
  
  
   
  
  
    
    
  
    
    
  
    
      20 February 2014
    
    
  
  
    
      Malizia, A.
      
        efa63850-cf26-482c-ae3b-54b0c8fb8a87
      
     
  
    
      Molina, M.
      
        28a3f3b6-aedf-4fa5-9a4f-dbcba001435d
      
     
  
    
      Bassani, L.
      
        07e5602c-f97e-4334-a0fa-c2212431a61a
      
     
  
    
      Stephen, J.B.
      
        c0b1afce-f3d9-4568-b2c1-51482f80cd9a
      
     
  
    
      Bazzano, A.
      
        8eef0c6e-1a5f-4bcd-a034-9a5c3b29104d
      
     
  
    
      Ubertini, P.
      
        7035748e-152c-473e-8766-a2fa3ac49fcb
      
     
  
    
      Bird, A.J.
      
        045ee141-4720-46fd-a412-5aa848a91b32
      
     
  
       
    
 
  
    
      
  
  
  
  
  
  
    Malizia, A., Molina, M., Bassani, L., Stephen, J.B., Bazzano, A., Ubertini, P. and Bird, A.J.
  
  
  
  
   
    (2014)
  
  
    
    The integral high-energy cut-off distribution of type 1 active galactic nuclei.
  
  
  
  
    The Astrophysical Journal Letters, 782 (2), , [L25].
  
   (doi:10.1088/2041-8205/782/2/L25). 
  
  
   
  
  
  
  
  
   
  
    
    
      
        
          Abstract
          In this Letter we present the primary continuum parameters, the photon index ?, and the high-energy cut-off E c of 41 type-1 Seyfert galaxies extracted from the International Gamma-Ray Astrophysics Laboratory (INTEGRAL) complete sample of active galactic nuclei (AGNs). We performed broadband (0.3-100 keV) spectral analysis by simultaneously fitting the soft and hard X-ray spectra obtained by XMM and INTEGRAL/IBIS-Swift/BAT, respectively, in order to investigate the general properties of these parameters, in particular their distribution and mean values. We find a mean photon index of 1.73 with a standard deviation of 0.17 and a mean high-energy cut-off of 128 keV with a standard deviation of 46 keV for the whole sample. This is the first time that the cut-off energy is constrained in such a large number of AGNs. We have 26 measurements of the cut-off, which corresponds to 63% of the entire sample, distributed between 50 and 200 keV. There are a further 11 lower limits mostly below 300 keV. Using the main parameters of the primary continuum, we have been able to obtain the actual physical parameters of the Comptonizing region, i.e., the plasma temperature kT e from 20 to 100 keV and the optical depth ? < 4. Finally, with the high signal-to-noise ratio spectra starting to come from NuSTAR it will soon be possible to better constrain the cut-off values in many AGNs, allowing the determination of more physical models and thus better understand the continuum emission and geometry of the region surrounding black holes.
         
      
      
        
          
            
  
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      Accepted/In Press date: 14 January 2014
 
    
      e-pub ahead of print date: 3 February 2014
 
    
      Published date: 20 February 2014
 
    
  
  
    
  
    
  
    
  
    
  
    
  
    
  
    
     
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        Local EPrints ID: 401051
        URI: http://eprints.soton.ac.uk/id/eprint/401051
        
          
        
        
        
        
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  Date deposited: 04 Oct 2016 08:54
  Last modified: 22 Aug 2025 01:36
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      Contributors
      
          
          Author:
          
            
            
              A. Malizia
            
          
        
      
          
          Author:
          
            
            
              M. Molina
            
          
        
      
          
          Author:
          
            
            
              L. Bassani
            
          
        
      
          
          Author:
          
            
            
              J.B. Stephen
            
          
        
      
          
          Author:
          
            
            
              A. Bazzano
            
          
        
      
          
          Author:
          
            
            
              P. Ubertini
            
          
        
      
        
      
      
      
    
  
   
  
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