Estimated redshift from machine learning (Ukwatta et al. 2016) - may take a few minute to calcaulte
Image
Pre-slew 15.0-350.0 keV image (Event data)
# RAcent DECcent POSerr Theta Phi Peak Cts SNR Name
322.0525 -29.6103 0.0029 12.3527 -172.9403 4.4081526 65.870 TRIG_00722604
Foreground time interval of the image:
-5.996 11.645 (delta_t = 17.641 [sec])
Background time interval of the image:
-72.955 -5.996 (delta_t = 66.959 [sec])
Lightcurves
Notes:
- 1) The mask-weighted light curves are using the flight position.
- 2) Multiple plots of different time binning/intervals are shown to cover all scenarios of short/long GRBs, rate/image triggers, and real/false positives.
- 3) For all the mask-weighted lightcurves, the y-axis units are counts/sec/det where a det is 0.4 x 0.4 = 0.16 sq cm.
- 4) The verticle lines correspond to following: green dotted lines are T50 interval, black dotted lines are T90 interval, blue solid line(s) is a spacecraft slew start time, and orange solid line(s) is a spacecraft slew end time.
- 5) Time of each bin is in the middle of the bin.
1 s binning
From T0-310 s to T0+310 s
From T100_start - 20 s to T100_end + 30 s
Full time interval
64 ms binning
Full time interval
From T100_start to T100_end
From T0-5 sec to T0+5 sec
16 ms binning
From T100_start-5 s to T100_start+5 s
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.024000
8 ms binning
From T100_start-3 s to T100_start+3 s
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.024000
2 ms binning
From T100_start-1 s to T100_start+1 s
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.024000
SN=5 or 10 sec. binning (whichever binning is satisfied first)
SN=5 or 10 sec. binning (T < 200 sec)
Quad-rate summed light curves (from T0-300s to T0+1000s)
Spectral Evolution
Spectra
Notes:
- 1) The fitting includes the systematic errors.
- 2) When the burst includes telescope slew time periods, the fitting uses an average response file made from multiple 5-s response files through out the slew time plus single time preiod for the non-slew times, and weighted by the total counts in the corresponding time period using addrmf. An average response file is needed becuase a spectral fit using the pre-slew DRM will introduce some errors in both a spectral shape and a normalization if the PHA file contains a lot of the slew/post-slew time interval.
- 3) For fits to more complicated models (e.g. a power-law over a cutoff power-law), the BAT team has decided to require a chi-square improvement of more than 6 for each extra dof.
Time averaged spectrum fit using the average DRM
Power-law model
Time interval is from -5.996 sec. to 154.436 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.82769 ( )
Norm@50keV : 1.42267E-02 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 122.03 using 59 PHA bins.
# Reduced chi-squared = 2.1408 for 57 degrees of freedom
# Null hypothesis probability = 1.240448e-06
Photon flux (15-150 keV) in 160.4 sec: 1.98196 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 2.0994e-05 ( 0 0 ) ergs/cm2
Cutoff power-law model
Time interval is from -5.996 sec. to 154.436 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.20030 ( -0.122674 0.119758 )
Epeak [keV] : 73.0521 ( -3.70999 4.7972 )
Norm@50keV : 2.66722E-02 ( -0.00294443 0.00338964 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 34.64 using 59 PHA bins.
# Reduced chi-squared = 0.6185 for 56 degrees of freedom
# Null hypothesis probability = 9.889438e-01
Photon flux (15-150 keV) in 160.4 sec: 1.85653 ( -0.04161 0.04198 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.02173e-05 ( -3.25484e-07 3.25726e-07 ) ergs/cm2
Band function
Time interval is from -5.996 sec. to 154.436 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : ( )
beta : ( )
Epeak [keV] : ( )
Norm@50keV : ( )
------------------------------------------------------------
Photon flux (15-150 keV) in sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 0 ( 0 0 ) ergs/cm2
Single BB
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 15.8530 ( )
R^2/D10^2 : 0.158933 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 865.46 using 59 PHA bins.
# Reduced chi-squared = 15.184 for 57 degrees of freedom
# Null hypothesis probability = 6.800410e-145
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.327e-06 4.202e-08
25- 50 5.541e-06 1.163e-07
50-150 9.700e-06 2.037e-07
15-150 1.657e-05 2.486e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 118.280 (-5.60602 7.2543)
Norm : 8.18596 (-0.20427 0.184008)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 35.84 using 59 PHA bins.
# Reduced chi-squared = 0.6288 for 57 degrees of freedom
# Null hypothesis probability = 9.872856e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.331e-06 1.500e-07
25- 50 5.989e-06 2.013e-07
50-150 1.084e-05 2.031e-06
15-150 2.016e-05 2.109e-06
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.91038 (-0.461118 0.474197)
R1^2/D10^2 : 1.32405 (-0.236188 0.307292)
kT2 [keV] : 24.4951 (-1.22927 1.44171)
R2^2/D10^2 : 2.29199E-02 (-0.00491216 0.00564072)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 48.47 using 59 PHA bins.
# Reduced chi-squared = 0.8812 for 55 degrees of freedom
# Null hypothesis probability = 7.207893e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.770e-06 1.347e-07
25- 50 6.264e-06 1.548e-07
50-150 1.073e-05 2.823e-07
15-150 1.977e-05 4.571e-07
Peak spectrum fit
Power-law model
Time interval is from 110.996 sec. to 111.996 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.77441 ( -0.0678074 0.0685205 )
Norm@50keV : 4.99134E-02 ( -0.00200951 0.00200295 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 52.16 using 59 PHA bins.
# Reduced chi-squared = 0.9151 for 57 degrees of freedom
# Null hypothesis probability = 6.568476e-01
Photon flux (15-150 keV) in 1 sec: 6.81125 ( -0.27545 0.27596 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.60055e-07 ( -1.8952e-08 1.90161e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 110.996 sec. to 111.996 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.30001 ( -0.292841 0.275209 )
Epeak [keV] : 73.4409 ( -11.8397 33.5995 )
Norm@50keV : 8.66748E-02 ( -0.0232434 0.0343686 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 43.12 using 59 PHA bins.
# Reduced chi-squared = 0.7700 for 56 degrees of freedom
# Null hypothesis probability = 8.962879e-01
Photon flux (15-150 keV) in 1 sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 0 ( 0 0 ) ergs/cm2
Band function
Time interval is from 110.996 sec. to 111.996 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : ( )
beta : ( )
Epeak [keV] : ( )
Norm@50keV : ( )
------------------------------------------------------------
Photon flux (15-150 keV) in sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 0 ( 0 0 ) ergs/cm2
Single BB
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 13.2174 ( )
R^2/D10^2 : 1.13563 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 188.84 using 59 PHA bins.
# Reduced chi-squared = 3.3130 for 57 degrees of freedom
# Null hypothesis probability = 4.972467e-16
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.206e-08 3.195e-09
25- 50 1.475e-07 7.050e-09
50-150 1.644e-07 1.325e-08
15-150 3.540e-07 1.550e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 120.656 (-19.7382 19.5406)
Norm : 28.4231 (-1.39858 1.68477)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 43.44 using 59 PHA bins.
# Reduced chi-squared = 0.7621 for 57 degrees of freedom
# Null hypothesis probability = 9.071652e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.402e-08 5.000e-09
25- 50 1.325e-07 7.100e-09
50-150 2.372e-07 5.870e-08
15-150 4.437e-07 6.355e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.83529 (-0.842831 0.896379)
R1^2/D10^2 : 8.34805 (-2.83285 4.93949)
kT2 [keV] : 23.1110 (-2.69744 3.69351)
R2^2/D10^2 : 0.106268 (-0.0469965 0.0696966)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 43.61 using 59 PHA bins.
# Reduced chi-squared = 0.7930 for 55 degrees of freedom
# Null hypothesis probability = 8.656851e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.135e-08 9.380e-09
25- 50 1.357e-07 1.265e-08
50-150 2.348e-07 3.490e-08
15-150 4.419e-07 5.405e-08
Pre-slew spectrum (Pre-slew PHA with pre-slew DRM)
Power-law model
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.894482 ( )
Norm@50keV : 1.66309E-02 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 120.82 using 59 PHA bins.
# Reduced chi-squared = 2.1196 for 57 degrees of freedom
# Null hypothesis probability = 1.738886e-06
Photon flux (15-150 keV) in 17.64 sec: 1.90879 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 3.29947e-06 ( 0 0 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.42824E-02 ( -0.190845 0.18282 )
Epeak [keV] : 138.306 ( -14.1389 20.429 )
Norm@50keV : 3.82407E-02 ( -0.00593081 0.00729198 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 44.06 using 59 PHA bins.
# Reduced chi-squared = 0.7868 for 56 degrees of freedom
# Null hypothesis probability = 8.760701e-01
Photon flux (15-150 keV) in 17.64 sec: 1.84499 ( -0.04653 0.04659 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.20983e-06 ( -8.28022e-08 8.26081e-08 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : ( )
beta : ( )
Epeak [keV] : ( )
Norm@50keV : ( )
------------------------------------------------------------
Photon flux (15-150 keV) in sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 0 ( 0 0 ) ergs/cm2
S(25-50 keV) vs. S(50-100 keV) plot
S(25-50 keV) = 5.97e-06
S(50-100 keV) = 6.74e-06
T90 vs. Hardness ratio plot
T90 = 125.699999928474 sec.
Hardness ratio (energy fluence ratio) = 1.12898
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.32722
Count Ratio (50-100 keV) / (15-25 keV) = 0.831938
Mask shadow pattern
IMX = -2.173391656766071E-01, IMY = 2.691597681904080E-02
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.024000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.024000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.024000
Spacecraft aspect plot
Bright source in the pre-burst/pre-slew/post-slew images
Pre-burst image of 15-350 keV band
Time interval of the image:
-72.955380 -5.996000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
274.1620 -14.0791 6.7 41.5 -64.2 -0.5223 -1.7 9.4 GX 17+2
275.9782 -30.2419 29.6 39.4 -89.2 0.1681 0.4 8.0 H1820-303
284.9509 -24.8724 8.1 30.8 -81.7 0.2214 1.4 5.5 HT1900.1-2455
288.8902 11.0464 4.9 40.4 -19.2 0.3147 2.3 8.1 GRS 1915+105
299.5392 35.1909 5.7 55.8 9.3 1.0301 2.0 2.6 Cyg X-1
287.3058 -5.2671 2.3 31.9 -43.3 0.6037 4.9 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-5.996000 11.644600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
273.9667 -13.9223 5.6 41.8 -64.0 -0.5154 -2.1 7.2 GX 17+2
276.0876 -30.2941 28.0 39.3 -89.3 0.1214 0.4 9.5 H1820-303
285.2258 -24.9953 9.1 30.5 -82.0 -0.1471 -1.3 11.3 HT1900.1-2455
288.7427 10.8917 10.5 40.4 -19.6 0.1152 1.1 4.6 GRS 1915+105
299.6619 35.1768 6.3 55.8 9.4 0.7714 1.8 3.8 Cyg X-1
13.9687 -42.0948 2.7 53.5 156.3 1.7484 4.2 ------ UNKNOWN
322.0624 15.4632 2.4 33.8 35.1 0.5377 4.7 ------ UNKNOWN
322.0525 -29.6103 0.2 12.4 -172.9 4.4076 65.9 ------ UNKNOWN
295.3913 -16.4626 2.4 21.0 -62.2 0.3745 4.8 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
49.644600 962.239400
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
275.9536 -30.3614 202.7 39.7 -86.4 0.1832 0.1 1.5 H1820-303
284.8802 -24.7979 0.0 33.3 -74.2 -1.4916 -1.2 11.2 HT1900.1-2455
288.7416 10.8797 3.7 51.7 -26.9 5.3663 3.1 5.2 GRS 1915+105
32.2401 -60.1284 2.4 54.9 161.6 22.1191 4.9 ------ UNKNOWN
322.0588 -29.6136 0.3 0.0 -77.5 25.0906 43.3 ------ UNKNOWN
309.9942 3.4825 2.9 35.1 -4.7 3.0256 4.0 ------ UNKNOWN
286.9688 -79.2873 2.9 51.9 -155.6 7.4099 4.0 ------ UNKNOWN
Plot creation:
Sun Dec 4 17:17:38 EST 2016