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
129.8729 79.2186 0.0083 7.6661 -153.7391 1.6569498 23.060 TRIG_01072990
Foreground time interval of the image:
-19.360 7.104 (delta_t = 26.464 [sec])
Background time interval of the image:
-239.264 -19.360 (delta_t = 219.904 [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 0.512000
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 0.512000
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 0.512000
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 -19.360 sec. to 7.104 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.47705 ( -0.11344 0.114325 )
Norm@50keV : 3.99458E-03 ( -0.000269937 0.000268798 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 63.73 using 59 bins.
Reduced chi-squared = 1.11807
# Null hypothesis probability of 2.52e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 26.46 sec: 0.495678 ( -0.03255 0.032573 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.0067e-06 ( -7.53351e-08 7.60791e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -19.360 sec. to 7.104 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.736520 ( -0.552903 0.487048 )
Epeak [keV] : 82.5220 ( -17.4804 64.4651 )
Norm@50keV : 9.62503E-03 ( -0.00415399 0.00872724 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 56.59 using 59 bins.
Reduced chi-squared = 1.01054
# Null hypothesis probability of 4.53e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 26.46 sec: 0.478293 ( -0.034464 0.03443 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.41045e-07 ( -8.5742e-08 8.68057e-08 ) ergs/cm2
Band function
Time interval is from -19.360 sec. to 7.104 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] : 14.3679 (-1.11905 1.23954)
R^2/D10^2 : 6.59562E-02 (-0.016653 0.0218295)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 86.71 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.80e-03 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.589e-08 8.652e-09
25- 50 2.895e-07 2.118e-08
50-150 3.987e-07 5.755e-08
15-150 7.641e-07 6.390e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-43.9169 -200)
Norm : 2.02809 (-0.131285 0.131285)
------------------------------------------------------------
#Fit statistic : Chi-Squared 60.12 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.64e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.339e-07 1.012e-08
25- 50 2.576e-07 2.588e-08
50-150 5.649e-07 1.484e-07
15-150 9.564e-07 1.899e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 8.39780 (-2.23139 2.12233)
R1^2/D10^2 : 0.264091 (-0.120599 0.451385)
kT2 [keV] : 26.2611 (-6.55944 15.5595)
R2^2/D10^2 : 5.61111E-03 (-0.00402389 0.0120487)
------------------------------------------------------------
#Fit statistic : Chi-Squared 56.77 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.09e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.095e-07 3.023e-08
25- 50 2.759e-07 7.897e-08
50-150 5.642e-07 2.517e-07
15-150 9.496e-07 3.547e-07
Peak spectrum fit
Power-law model
Time interval is from 0.220 sec. to 1.220 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.40289 ( -0.168271 0.169199 )
Norm@50keV : 1.36618E-02 ( -0.00153781 0.00153151 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 74.59 using 59 bins.
Reduced chi-squared = 1.3086
# Null hypothesis probability of 5.89e-02 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 1.66490 ( -0.18193 0.182 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.31941e-07 ( -1.63936e-08 1.66149e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.220 sec. to 1.220 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -0.755416 ( -1.34676 1.01545 )
Epeak [keV] : 56.6132 ( -8.42759 15.0279 )
Norm@50keV : 0.210544 ( -0.210856 0.992786 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 57.70 using 59 bins.
Reduced chi-squared = 1.03036
# Null hypothesis probability of 4.12e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 1.56315 ( -0.18484 0.1862 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.08883e-07 ( -1.68741e-08 1.8479e-08 ) ergs/cm2
Band function
Time interval is from 0.220 sec. to 1.220 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] : 13.5580 (-1.44081 1.68155)
R^2/D10^2 : 0.293986 (-0.100175 0.143826)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 59.27 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.93e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.144e-08 2.286e-09
25- 50 4.120e-08 5.430e-09
50-150 4.903e-08 1.086e-08
15-150 1.017e-07 1.401e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-63.4852 -200)
Norm : 6.89015 (-0.744261 0.744261)
------------------------------------------------------------
#Fit statistic : Chi-Squared 71.23 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.73e-02 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.716e-08 9.185e-09
25- 50 3.301e-08 1.819e-08
50-150 7.239e-08 3.954e-08
15-150 1.226e-07 6.730e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 12.1993 (-4.39814 2.22545)
R1^2/D10^2 : 0.393953 (-0.169669 0.499012)
kT2 [keV] : 200.000 (-200 -200)
R2^2/D10^2 : 1.07815E-04 (-8.56743e-05 0.000375105)
------------------------------------------------------------
#Fit statistic : Chi-Squared 55.07 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.72e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.277e-08 3.798e-09
25- 50 4.072e-08 1.450e-08
50-150 6.529e-08 3.110e-08
15-150 1.188e-07 4.413e-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: 1.47705 ( -0.11344 0.114325 )
Norm@50keV : 3.99458E-03 ( -0.000269937 0.000268798 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 63.73 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.52e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 26.46 sec: 0.495666 ( -0.0325483 0.0325713 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.00657e-06 ( -7.53967e-08 7.60865e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.736521 ( -0.552903 0.487048 )
Epeak [keV] : 82.5220 ( -17.4804 64.4651 )
Norm@50keV : 9.62503E-03 ( -0.00415399 0.00872724 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 56.59 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.53e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 26.46 sec: 0.478246 ( -0.034456 0.034421 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.41394e-07 ( -8.58812e-08 8.69581e-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) = 2.46e-07
S(50-100 keV) = 3.55e-07
T90 vs. Hardness ratio plot
T90 = 20.6959999799728 sec.
Hardness ratio (energy fluence ratio) = 1.44309
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.559
Count Ratio (50-100 keV) / (15-25 keV) = 1.02388
Mask shadow pattern
IMX = -1.207106120989392E-01, IMY = 5.955634539474253E-02
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.512000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.512000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.512000
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:
-239.264000 -19.360000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6291 22.0059 1.6 53.4 9.5 7.1992 7.2 0.6 Crab
332.5040 57.8261 2.9 43.7 131.1 3.9779 4.0 ------ UNKNOWN
323.7671 57.4766 2.4 45.4 137.4 4.7195 4.7 ------ UNKNOWN
248.7316 45.8066 2.9 57.6 -165.4 5.2315 4.0 ------ UNKNOWN
175.9986 55.9388 3.2 32.6 -110.0 1.7869 3.6 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-19.360000 7.104000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.7423 21.9611 8.9 53.5 9.3 0.3549 1.3 6.9 Crab
268.2583 55.2001 2.8 50.0 177.9 0.7665 4.1 ------ UNKNOWN
129.8730 79.2186 0.5 7.7 -153.7 1.6570 23.1 ------ UNKNOWN
237.7426 42.4577 2.3 59.3 -155.5 2.2358 5.1 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
41.036600 622.236600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
355.9641 57.4708 2.5 40.7 95.7 7.6330 4.7 ------ UNKNOWN
277.6848 57.9601 3.2 41.6 157.3 3.8934 3.6 ------ UNKNOWN
265.5633 62.1002 3.1 36.4 165.6 2.7764 3.7 ------ UNKNOWN
240.5129 36.8428 2.9 57.6 -165.4 10.6867 4.0 ------ UNKNOWN
104.3884 25.8576 4.9 54.5 -19.6 4.0815 2.4 ------ UNKNOWN
Plot creation:
Mon Oct 24 05:19:33 EDT 2022