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GRB 110201A
  
  The Swift Burst Analyser — GRB 110201A 
Last updated using ObsID 00444230000, version 12; 
Data were analysed using HEASOFT version 6.35.2
Related pages: 
    Position 
 |     Light curve 
 |     Spectrum 
 |     Image 
 |     XRT Catalogue entry 
 |     Download obs data 
 |     BAT analysis 
 |     GCN Notices 
 |     GCN Circulars 
  
From 2016 January, the light curve plots support interactive zooming and exploring. See the jsPlot documentation  for details.
Also, from the same date, the first plot on this page is the observed  flux
         in the native band of each instrument (including UVOT where available).
  Index of bursts .
  About these products .
  
  
  
    Caveats 
    If the answer to any of the following is "yes," you should investigate further before
    accepting the light curves. See the documentation  for details.
    
      Is Γ discontinuous between BAT and XRT? 
      Is the BAT spectral fit a cut-off power law? 
      Are the Γ values extreme?  
      Are the errors on Γ/CF large? 
      Do all the BAT or XRT bins have identically Γ/CF bins? 
     
    Close .
  
   
  
  Jump to: 
  Observed flux  | BAT+XRT  | BAT  | XRT  | BAT no evolution .
  
  
  Downloads: 
  BAT spectral evolution data  | XRT spectral evolution data  | All files for this object: [tar ][tar.gz ][zip ].
 
All data uses absorption NH =2.163 × 1022  cm-2  at z=0.XRT spectrum repository ).
  
  Observed BAT+XRT+UVOT flux 
Reliability checks .
Show  Observed Flux hardness ratio
BAT binning: 
SNR 4 SNR 5 SNR 6 SNR 7 64 ms bins 1 s bins 10 s bins  
Subplot: 
no photon index counts to flux conversion factor  
Show UVOT upper limits? 
Renormalise UVOT data? 
UVOT data are normalised to the v  band.
Show 'bad' BAT points? Explain 
 
■ BAT
■ XRT (all modes)
■ white
■ v
■ b
■ u
■ uvw1
■ uvw2
■ uvm2
 
 
BAT-XRT unabsorbed flux light curves 
Reliability checks .
Show  BAT-XRT hardness ratio
BAT binning: 
SNR 4 SNR 5 SNR 6 SNR 7 64 ms bins 1 s bins 10 s bins  
Subplot: 
no photon index counts to flux conversion factor  
Display which bands? 
Flux density at 10 keV 
0.3—10 keV flux 
15—50 keV flux 
Show 'bad' BAT points? Explain 
 
BAT unabsorbed flux light curves 
Reliability checks .
Show  BAT hardness ratio
BAT binning: 
SNR 4 SNR 5 SNR 6 SNR 7 64 ms bins 1 s bins 10 s bins  
Subplot: 
no photon index counts to flux conversion factor  
Display which bands? 
Flux density at 10 keV 
0.3—10 keV flux 
15—50 keV flux 
Show 'bad' BAT points? Explain 
 
XRT unabsorbed flux light curves 
Reliability checks .
Show  XRT hardness ratio
Subplot: 
no photon index counts to flux conversion factor  
Display which bands? 
Flux density at 10 keV 
0.3—10 keV flux 
15—50 keV flux 
 
The fit to the T90  spectrum was used to create the plots in this section.90  was 11.0, from 1.6 to 12.6
Count-rate light curves are available from GCN .
BAT unabsorbed flux light curves, no spectral evolution 
BAT binning: 
SNR 4 SNR 5 SNR 6 SNR 7 64 ms bins 1 s bins 10 s bins  
Display which bands? 
Flux density at 10 keV 
0.3—10 keV flux 
15—50 keV flux 
Show 'bad' BAT points? Explain