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
132.7362 71.1764 0.0097 25.1047 91.8245 2.1162630 19.787 TRIG_01014316
Foreground time interval of the image:
-25.184 7.816 (delta_t = 33.000 [sec])
Background time interval of the image:
-239.184 -25.184 (delta_t = 214.000 [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 -25.184 sec. to 7.816 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.34553 ( -0.130796 0.130563 )
Norm@50keV : 4.17213E-03 ( -0.000320951 0.000320751 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 66.25 using 59 bins.
Reduced chi-squared = 1.16228
# Null hypothesis probability of 1.88e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 33 sec: 0.502169 ( -0.039629 0.039695 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.34621e-06 ( -1.13749e-07 1.14531e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -25.184 sec. to 7.816 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.603277 ( -0.651061 0.564872 )
Epeak [keV] : 99.3725 ( -24.2941 135.121 )
Norm@50keV : 9.47915E-03 ( -0.00432397 0.00946029 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 61.05 using 59 bins.
Reduced chi-squared = 1.09018
# Null hypothesis probability of 2.99e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 33 sec: 0.485532 ( -0.041875 0.041682 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.28536e-06 ( -1.23576e-07 1.24107e-07 ) ergs/cm2
Band function
Time interval is from -25.184 sec. to 7.816 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] : 17.2007 (-1.50299 1.68466)
R^2/D10^2 : 3.74575E-02 (-0.0102874 0.0138308)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 80.30 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.27e-02 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.424e-08 1.079e-08
25- 50 3.316e-07 3.544e-08
50-150 7.029e-07 9.785e-08
15-150 1.109e-06 1.069e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-25.8104 -200)
Norm : 2.08755 (-0.160558 0.160558)
------------------------------------------------------------
#Fit statistic : Chi-Squared 70.28 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.11e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.715e-07 1.605e-08
25- 50 3.300e-07 5.732e-08
50-150 7.237e-07 2.496e-07
15-150 1.225e-06 3.313e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.06203 (-1.90138 2.95409)
R1^2/D10^2 : 1.09588 (-0.871248 5.71541)
kT2 [keV] : 20.9104 (-2.7321 4.72406)
R2^2/D10^2 : 1.74292E-02 (-0.00954751 0.0117552)
------------------------------------------------------------
#Fit statistic : Chi-Squared 60.30 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.90e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.400e-07 6.056e-08
25- 50 3.062e-07 7.357e-08
50-150 7.976e-07 1.620e-07
15-150 1.244e-06 2.302e-07
Peak spectrum fit
Power-law model
Time interval is from -0.184 sec. to 0.816 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.876445 ( -0.254459 0.241586 )
Norm@50keV : 1.32046E-02 ( -0.00213397 0.00211518 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 57.18 using 59 bins.
Reduced chi-squared = 1.00316
# Null hypothesis probability of 4.69e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 1.51543 ( -0.24279 0.24387 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.49586e-07 ( -2.43382e-08 2.44464e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.184 sec. to 0.816 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -0.480294 ( -1.40553 1.06303 )
Epeak [keV] : 108.900 ( -28.8308 158.641 )
Norm@50keV : 5.01998E-02 ( -0.0319982 0.126383 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 52.11 using 59 bins.
Reduced chi-squared = 0.930536
# Null hypothesis probability of 6.23e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 1.46245 ( -0.24436 0.24654 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.4392e-07 ( -2.5703e-08 2.55918e-08 ) ergs/cm2
Band function
Time interval is from -0.184 sec. to 0.816 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] : 23.5866 (-3.9858 5.16473)
R^2/D10^2 : 4.74468E-02 (-0.0217666 0.0372715)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 53.36 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.12e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.725e-09 1.583e-09
25- 50 2.599e-08 7.405e-09
50-150 1.079e-07 2.985e-08
15-150 1.386e-07 3.723e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-33.3042 -200)
Norm : 6.01532 (-1.01505 1.01505)
------------------------------------------------------------
#Fit statistic : Chi-Squared 75.52 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.09e-02 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.497e-08 8.655e-09
25- 50 2.880e-08 1.632e-08
50-150 6.316e-08 3.623e-08
15-150 1.069e-07 6.040e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 10.1277 (-10.1294 189.433)
R1^2/D10^2 : 0.197796 (-0.198389 -0.198389)
kT2 [keV] : 29.1626 (-29.196 -29.196)
R2^2/D10^2 : 2.10135E-02 (-0.0209334 0.0455347)
------------------------------------------------------------
#Fit statistic : Chi-Squared 51.55 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.07e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.994e-09 4.276e-09
25- 50 2.784e-08 1.489e-08
50-150 1.110e-07 6.150e-08
15-150 1.458e-07 7.745e-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: 1.34553 ( -0.130796 0.130563 )
Norm@50keV : 4.17213E-03 ( -0.000320951 0.000320751 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 66.25 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.88e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 33 sec: 0.502163 ( -0.0396281 0.0396914 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.34605e-06 ( -1.13879e-07 1.14552e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.603277 ( -0.651061 0.564872 )
Epeak [keV] : 99.3725 ( -24.2941 135.121 )
Norm@50keV : 9.47915E-03 ( -0.00432397 0.00946029 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 61.05 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.99e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 33 sec: 0.485498 ( -0.041867 0.041671 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.28588e-06 ( -1.23839e-07 1.24209e-07 ) 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) = 3.07e-07
S(50-100 keV) = 4.85e-07
T90 vs. Hardness ratio plot
T90 = 29 sec.
Hardness ratio (energy fluence ratio) = 1.5798
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.50578
Count Ratio (50-100 keV) / (15-25 keV) = 1.47335
Mask shadow pattern
IMX = -1.491751994915043E-02, IMY = -4.682970903408430E-01
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:
-239.184000 -25.184000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.4506 35.3374 16.4 40.9 -81.0 -0.7715 -0.7 0.5 Her X-1
308.1824 40.8131 0.0 50.3 -139.8 -1.3401 -1.4 9.0 Cyg X-3
63.2547 62.2192 2.4 44.3 127.2 4.9162 4.9 ------ UNKNOWN
56.9112 64.4917 2.3 42.4 131.7 3.9561 5.0 ------ UNKNOWN
157.4598 87.1012 3.3 16.2 131.9 0.7802 3.5 ------ UNKNOWN
184.5740 49.7495 2.2 28.2 17.2 1.2526 5.3 ------ UNKNOWN
209.5173 14.8498 2.2 58.3 -24.7 7.2277 5.3 ------ UNKNOWN
312.0297 38.9405 3.0 53.2 -142.4 4.9183 3.9 ------ UNKNOWN
301.6619 39.9363 3.9 49.2 -133.4 3.2504 3.0 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-25.184000 7.816000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.3925 35.4820 4.3 40.7 -81.0 0.9088 2.7 9.0 Her X-1
307.8652 40.8745 11.5 50.2 -139.6 -0.3114 -1.0 12.1 Cyg X-3
132.7363 71.1764 0.6 25.1 91.8 2.1164 19.8 ------ UNKNOWN
327.7780 66.3459 2.1 32.7 -173.1 0.4896 5.5 ------ UNKNOWN
289.2076 40.2157 2.2 45.3 -121.5 1.7399 5.2 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
58.116600 717.265200
720.816000 839.544800
840.816000 934.336000
935.816000 941.923200
942.816000 962.826000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
134.3745 24.2705 3.5 46.9 40.4 7.0649 3.3 ------ UNKNOWN
37.3310 44.4831 3.7 50.1 154.5 10.0156 3.1 ------ UNKNOWN
159.6113 17.7423 4.4 55.7 11.0 9.5906 2.6 ------ UNKNOWN
8.6221 46.7244 2.5 55.6 178.8 17.5127 4.7 ------ UNKNOWN
333.2223 59.7397 3.2 48.3 -151.4 7.3060 3.6 ------ UNKNOWN
305.9746 59.4929 3.1 49.2 -133.2 13.5392 3.7 ------ UNKNOWN
299.5835 60.5407 2.4 47.9 -129.0 15.0090 4.7 ------ UNKNOWN
Plot creation:
Sat Jul 30 07:22:08 EDT 2022