Discovery of two new fast X-ray transients with INTEGRAL: IGR J03346+4414 and IGR J20344+3913
Discovery of two new fast X-ray transients with INTEGRAL: IGR J03346+4414 and IGR J20344+3913
 
  We report on the discovery of two fast X-ray transients (FXTs) from analysis of archival INTEGRAL data. Both are characterized by a remarkable hard X-ray activity above 20?keV, in terms of duration (?15 and 30 min, respectively), peak flux (?10?9?erg?cm?2 s?1) and dynamic range (?2400 and 1360, respectively). Swift/X-ray telescope follow-up observations failed to detect any quiescent or low-level soft X-ray emission from either of the two FXTs, providing an upper limit of the order of a few times 10?12?erg?cm?2 s?1. The main spectral and temporal Imager on Board INTEGRAL Satellite (IBIS)/INTEGRAL Soft Gamma-Ray Imager (ISGRI) characteristics are presented and discussed with the aim of inferring possible hints on their nature.
  
  
  2885-2892
  
    
      Sguera, V.
      
        371bb568-7e56-496e-a624-dba6de79d9e1
      
     
  
    
      Sidoli, L.
      
        2207422d-1a4d-448c-8c0b-8f0c2bf78a18
      
     
  
    
      Paizis, A.
      
        1f5ac404-8b17-43be-8e4a-6ada9bbf480c
      
     
  
    
      Bird, A.J.
      
        045ee141-4720-46fd-a412-5aa848a91b32
      
     
  
  
   
  
  
    
    
  
    
    
  
    
      11 December 2016
    
    
  
  
    
      Sguera, V.
      
        371bb568-7e56-496e-a624-dba6de79d9e1
      
     
  
    
      Sidoli, L.
      
        2207422d-1a4d-448c-8c0b-8f0c2bf78a18
      
     
  
    
      Paizis, A.
      
        1f5ac404-8b17-43be-8e4a-6ada9bbf480c
      
     
  
    
      Bird, A.J.
      
        045ee141-4720-46fd-a412-5aa848a91b32
      
     
  
       
    
 
  
    
      
  
  
  
  
  
  
    Sguera, V., Sidoli, L., Paizis, A. and Bird, A.J.
  
  
  
  
   
    (2016)
  
  
    
    Discovery of two new fast X-ray transients with INTEGRAL: IGR J03346+4414 and IGR J20344+3913.
  
  
  
  
    Monthly Notices of the Royal Astronomical Society, 463 (3), .
  
   (doi:10.1093/mnras/stw2183). 
  
  
   
  
  
  
  
  
   
  
    
    
      
        
          Abstract
          We report on the discovery of two fast X-ray transients (FXTs) from analysis of archival INTEGRAL data. Both are characterized by a remarkable hard X-ray activity above 20?keV, in terms of duration (?15 and 30 min, respectively), peak flux (?10?9?erg?cm?2 s?1) and dynamic range (?2400 and 1360, respectively). Swift/X-ray telescope follow-up observations failed to detect any quiescent or low-level soft X-ray emission from either of the two FXTs, providing an upper limit of the order of a few times 10?12?erg?cm?2 s?1. The main spectral and temporal Imager on Board INTEGRAL Satellite (IBIS)/INTEGRAL Soft Gamma-Ray Imager (ISGRI) characteristics are presented and discussed with the aim of inferring possible hints on their nature.
         
      
      
        
          
            
  
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      Accepted/In Press date: 26 August 2016
 
    
      e-pub ahead of print date: 1 September 2016
 
    
      Published date: 11 December 2016
 
    
  
  
    
  
    
  
    
  
    
  
    
  
    
  
    
     
        Organisations:
        Astronomy Group
      
    
  
    
  
  
  
    
  
  
        Identifiers
        Local EPrints ID: 403367
        URI: http://eprints.soton.ac.uk/id/eprint/403367
        
          
        
        
        
          ISSN: 1365-2966
        
        
          PURE UUID: ab20b6dc-e277-4ded-bde6-b88bb738ede0
        
  
    
        
          
        
    
        
          
        
    
        
          
        
    
        
          
            
              
            
          
        
    
  
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  Date deposited: 30 Nov 2016 11:55
  Last modified: 21 Aug 2025 01:37
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      Contributors
      
          
          Author:
          
            
            
              V. Sguera
            
          
        
      
          
          Author:
          
            
            
              L. Sidoli
            
          
        
      
          
          Author:
          
            
            
              A. Paizis
            
          
        
      
        
      
      
      
    
  
   
  
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