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
301.3236 16.5400 0.0255 22.6196 -103.7447 0.0505713 7.507 TRIG_01207446
Foreground time interval of the image:
0.000 0.096 (delta_t = 0.096 [sec])
Background time interval of the image:
-25.723 0.000 (delta_t = 25.723 [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 0.064000
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 0.064000
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 0.064000
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 0.000 sec. to 0.096 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.91241 ( -0.330065 0.346571 )
Norm@50keV : 1.92038E-02 ( -0.00522058 0.00516118 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 72.18 using 59 bins.
Reduced chi-squared = 1.26632
# Null hypothesis probability of 8.48e-02 with 57 degrees of freedom
Photon flux (15-150 keV) in 0.096 sec: 2.77136 ( -0.73575 0.73785 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.69497e-08 ( -4.53996e-09 4.56136e-09 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.000 sec. to 0.096 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -1.59907 ( -2.58104 1.85911 )
Epeak [keV] : 49.4730 ( -8.34399 8.42182 )
Norm@50keV : 1.43128 ( -1.43636 20.3228 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 61.07 using 59 bins.
Reduced chi-squared = 1.09054
# Null hypothesis probability of 2.99e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 0.096 sec: 2.99910 ( -0.74717 0.75077 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.86574e-08 ( -4.48704e-09 4.5038e-09 ) ergs/cm2
Band function
Time interval is from 0.000 sec. to 0.096 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] : 12.8125 (-2.10594 2.14673)
R^2/D10^2 : 0.710387 (-0.341127 0.665766)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 60.99 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.35e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.375e-09 9.091e-10
25- 50 8.050e-09 3.110e-09
50-150 8.283e-09 3.588e-09
15-150 1.871e-08 5.453e-09
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 74.4227 (-28.4905 66.2777)
Norm : 14.7011 (-4.53277 5.38869)
------------------------------------------------------------
#Fit statistic : Chi-Squared 68.22 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.47e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.642e-09 1.152e-09
25- 50 5.889e-09 1.899e-09
50-150 7.908e-09 4.785e-09
15-150 1.744e-08 6.029e-09
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.44911 (-6.27075 -6.27075)
R1^2/D10^2 : 0.284550 (-0.331277 -0.331277)
kT2 [keV] : 12.9610 (-12.9593 7.39892)
R2^2/D10^2 : 0.664248 (-0.666631 0.707506)
------------------------------------------------------------
#Fit statistic : Chi-Squared 60.97 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.70e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 0.000e+00 0.000e+00
25- 50 0.000e+00 0.000e+00
50-150 0.000e+00 0.000e+00
15-150 0.000e+00 0.000e+00
Peak spectrum fit
Power-law model
Time interval is from -0.444 sec. to 0.556 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.29062 ( -0.456198 0.442439 )
Norm@50keV : 5.89946E-03 ( -0.00156841 0.00156627 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 89.66 using 59 bins.
Reduced chi-squared = 1.57298
# Null hypothesis probability of 3.73e-03 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.702630 ( -0.190526 0.191394 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.84386e-08 ( -1.69212e-08 1.72708e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.444 sec. to 0.556 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.612139 ( -2.2849 1.07192 )
Epeak [keV] : 104.815 ( -104.817 -104.817 )
Norm@50keV : 1.28390E-02 ( -0.0128386 0.155475 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 89.13 using 59 bins.
Reduced chi-squared = 1.59161
# Null hypothesis probability of 3.20e-03 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.686311 ( -0.194672 0.195196 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.58097e-08 ( -1.83297e-08 1.83879e-08 ) ergs/cm2
Band function
Time interval is from -0.444 sec. to 0.556 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] : 17.0084 (-5.35408 8.21881)
R^2/D10^2 : 5.46377E-02 (-0.0398896 0.144032)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 91.53 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.52e-03 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.219e-09 1.836e-09
25- 50 1.425e-08 8.490e-09
50-150 2.943e-08 1.813e-08
15-150 4.690e-08 2.588e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.361 (-106.734 -199.362)
Norm : 2.92248 (-0.779936 0.781728)
------------------------------------------------------------
#Fit statistic : Chi-Squared 90.25 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.30e-03 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.277e-09 4.506e-09
25- 50 1.400e-08 8.235e-09
50-150 3.070e-08 1.831e-08
15-150 5.198e-08 3.117e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 8.13563 (-5.28582 -8.11426)
R1^2/D10^2 : 0.400333 (-0.379006 8.80903)
kT2 [keV] : 29.4354 (-16.8936 -29.3809)
R2^2/D10^2 : 6.72300E-03 (-0.00674715 0.0661937)
------------------------------------------------------------
#Fit statistic : Chi-Squared 88.55 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.77e-03 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.772e-09 3.803e-09
25- 50 1.438e-08 7.765e-09
50-150 3.721e-08 2.161e-08
15-150 5.736e-08 2.967e-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: 1.91241 ( -0.330065 0.346571 )
Norm@50keV : 1.92038E-02 ( -0.00522058 0.00516118 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 72.18 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.48e-02 with 57 degrees of freedom
Photon flux (15-150 keV) in 0.096 sec: 2.77117 ( -0.735668 0.737785 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.69465e-08 ( -4.53821e-09 4.56096e-09 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -1.59883 ( -2.58105 1.85909 )
Epeak [keV] : 49.4730 ( -8.34399 8.42183 )
Norm@50keV : 1.43090 ( -1.43636 20.3228 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 61.07 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.99e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 0.096 sec: 2.99890 ( -0.747 0.75064 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.86623e-08 ( -4.48829e-09 4.51286e-09 ) 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) = 4.96e-09
S(50-100 keV) = 5.27e-09
T90 vs. Hardness ratio plot
T90 = 0.0800000429153442 sec.
Hardness ratio (energy fluence ratio) = 1.0625
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.93662
Count Ratio (50-100 keV) / (15-25 keV) = 2.38704
Mask shadow pattern
IMX = -9.899695004969376E-02, IMY = 4.047305283342757E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.064000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.064000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.064000
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:
-25.723400 0.000000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.5578 35.2334 10.9 39.7 -11.6 0.1072 1.1 8.2 Her X-1
288.9176 10.8839 135.5 31.4 -81.4 0.0090 0.1 7.9 GRS 1915+105
299.6583 35.1290 3.3 5.6 -63.9 0.2231 3.5 5.5 Cyg X-1
308.1037 40.7900 2.8 3.1 120.8 0.2624 4.2 9.8 Cyg X-3
326.1189 38.1716 29.2 16.7 153.6 0.0257 0.4 9.3 Cyg X-2
330.0797 25.7430 2.4 25.0 -178.0 0.3487 4.9 ------ UNKNOWN
267.6620 8.7374 2.4 44.9 -54.7 1.0996 4.9 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
0.000000 0.096000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.4015 35.3184 26.7 39.8 -11.4 0.0032 0.4 3.1 Her X-1
288.8947 10.9283 4.8 31.4 -81.3 -0.0209 -2.4 5.8 GRS 1915+105
299.7657 35.1589 4.8 5.5 -64.3 0.0126 2.4 9.0 Cyg X-1
308.1504 41.1036 4.5 3.4 116.8 -0.0130 -2.5 9.2 Cyg X-3
325.9142 38.2915 0.0 16.5 153.2 0.0029 0.6 12.3 Cyg X-2
357.0132 16.5884 2.2 50.5 168.6 0.0864 5.3 ------ UNKNOWN
350.4110 11.4653 2.1 48.9 179.1 0.0634 5.5 ------ UNKNOWN
242.5143 25.7332 2.1 53.2 -17.1 0.0895 5.5 ------ UNKNOWN
301.3236 16.5400 1.5 22.6 -103.7 0.0506 7.5 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
782.076600 962.308500
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
86.1839 3.6326 2.4 39.3 93.9 4.2396 4.8 ------ UNKNOWN
122.6322 -36.9029 2.9 53.9 167.1 4.6167 4.0 ------ UNKNOWN
45.8161 6.8371 3.6 35.5 25.0 1.3165 3.2 ------ UNKNOWN
67.5276 -59.4389 2.5 33.8 -138.3 1.6109 4.6 ------ UNKNOWN
Plot creation:
Sat Mar 9 15:17:19 EST 2024