NuSTAR catches the unveiling nucleus of NGC 1068
NuSTAR catches the unveiling nucleus of NGC 1068
 
  We present a NuSTAR and XMM–Newton monitoring campaign in 2014/2015 of the Compton-thick Seyfert 2 galaxy, NGC 1068. During the 2014 August observation, we detect with NuSTAR a flux excess above 20 keV (32 ± 6?per?cent) with respect to the 2012 December observation and to a later observation performed in 2015 February. We do not detect any spectral variation below 10 keV in the XMM–Newton data. The transient excess can be explained by a temporary decrease of the column density of the obscuring material along the line of sight (from NH ? 1025 cm?2 to NH = 6.7 ± 1.0 × 1024 cm?2), which allows us for the first time to unveil the direct nuclear radiation of the buried active galactic nucleus in NGC 1068 and to infer an intrinsic 2–10 keV luminosity LX=7+7?4×1043 erg s?1
  
  
  L94-L98
  
    
      Gandhi, Poshak
      
        5bc3b5af-42b0-4dd8-8f1f-f74048d4d4a9
      
     
  
  
   
  
  
    
    
  
    
      17 December 2015
    
    
  
  
    
      Gandhi, Poshak
      
        5bc3b5af-42b0-4dd8-8f1f-f74048d4d4a9
      
     
  
       
    
 
  
    
      
  
  
  
  
  
  
    Gandhi, Poshak
  
  
  
  
   
    (2015)
  
  
    
    NuSTAR catches the unveiling nucleus of NGC 1068.
  
  
  
  
    Monthly Notices of the Royal Astronomical Society, 456 (1), .
  
   (doi:10.1093/mnrasl/slv178). 
  
  
   
  
  
  
  
  
   
  
    
    
      
        
          Abstract
          We present a NuSTAR and XMM–Newton monitoring campaign in 2014/2015 of the Compton-thick Seyfert 2 galaxy, NGC 1068. During the 2014 August observation, we detect with NuSTAR a flux excess above 20 keV (32 ± 6?per?cent) with respect to the 2012 December observation and to a later observation performed in 2015 February. We do not detect any spectral variation below 10 keV in the XMM–Newton data. The transient excess can be explained by a temporary decrease of the column density of the obscuring material along the line of sight (from NH ? 1025 cm?2 to NH = 6.7 ± 1.0 × 1024 cm?2), which allows us for the first time to unveil the direct nuclear radiation of the buried active galactic nucleus in NGC 1068 and to infer an intrinsic 2–10 keV luminosity LX=7+7?4×1043 erg s?1
         
      
      
        
          
            
  
    Text
 __soton.ac.uk_UDE_PersonalFiles_Users_skr1c15_mydocuments_eprints_Gandhi_NuStar catches the unveiling nucleaus of NCG 1068.pdf
     - Accepted Manuscript
   
  
  
    
  
 
          
            
          
            
           
            
           
        
        
       
    
   
  
  
  More information
  
    
      Accepted/In Press date: 10 November 2015
 
    
      Published date: 17 December 2015
 
    
  
  
    
  
    
  
    
  
    
  
    
  
    
  
    
     
        Organisations:
        Astronomy Group
      
    
  
    
  
  
  
    
  
  
        Identifiers
        Local EPrints ID: 396270
        URI: http://eprints.soton.ac.uk/id/eprint/396270
        
          
        
        
        
          ISSN: 1365-2966
        
        
          PURE UUID: 5da29e44-0c0d-437b-aeab-8262f51e2caa
        
  
    
        
          
            
              
            
          
        
    
  
  Catalogue record
  Date deposited: 02 Jun 2016 13:46
  Last modified: 22 Aug 2025 02:12
  Export record
  
  
   Altmetrics
   
   
  
 
 
  
  
    Download statistics
    
      Downloads from ePrints over the past year. Other digital versions may also be available to download e.g. from the publisher's website.
      
      View more statistics