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
23.0970 -1.7629 0.0075 50.8417 169.3183 18.3744612 25.569 TRIG_01011980
Foreground time interval of the image:
-31.656 11.445 (delta_t = 43.101 [sec])
Background time interval of the image:
-199.155 -31.656 (delta_t = 167.499 [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 -31.656 sec. to 32.344 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.56221 ( -0.0620561 0.0619481 )
Norm@50keV : 2.30320E-02 ( -0.000816966 0.000816966 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 85.21 using 59 bins.
Reduced chi-squared = 1.49491
# Null hypothesis probability of 9.13e-03 with 57 degrees of freedom
Photon flux (15-150 keV) in 64 sec: 2.92621 ( -0.11674 0.11713 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.38551e-05 ( -5.04529e-07 5.05079e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -31.656 sec. to 32.344 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.25300 ( -0.25931 0.245156 )
Epeak [keV] : 131.950 ( -36.7121 257.376 )
Norm@50keV : 3.21431E-02 ( -0.00729489 0.0100702 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 80.51 using 59 bins.
Reduced chi-squared = 1.43768
# Null hypothesis probability of 1.76e-02 with 56 degrees of freedom
Photon flux (15-150 keV) in 64 sec: 2.87527 ( -0.12274 0.12322 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.3654e-05 ( -5.33226e-07 5.31658e-07 ) ergs/cm2
Band function
Time interval is from -31.656 sec. to 32.344 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] : 16.1645 ( )
R^2/D10^2 : 0.248090 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 257.27 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.06e-27 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.558e-07 6.176e-08
25- 50 3.633e-06 1.776e-07
50-150 6.660e-06 4.125e-07
15-150 1.115e-05 4.512e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-24.4161 -200)
Norm : 11.9275 (-0.422684 0.422684)
------------------------------------------------------------
#Fit statistic : Chi-Squared 80.61 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.15e-02 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.902e-06 8.064e-08
25- 50 3.658e-06 1.510e-07
50-150 8.022e-06 3.232e-07
15-150 1.358e-05 5.920e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 8.66990 (-0.894246 0.954345)
R1^2/D10^2 : 1.58409 (-0.44544 0.67116)
kT2 [keV] : 32.7564 (-4.65914 7.26341)
R2^2/D10^2 : 1.51980E-02 (-0.00739713 0.0111951)
------------------------------------------------------------
#Fit statistic : Chi-Squared 72.76 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.46e-02 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.608e-06 1.683e-07
25- 50 3.897e-06 2.931e-07
50-150 8.173e-06 1.255e-06
15-150 1.368e-05 1.386e-06
Peak spectrum fit
Power-law model
Time interval is from 7.844 sec. to 8.844 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.49792 ( -0.146628 0.148038 )
Norm@50keV : 9.81969E-02 ( -0.0088976 0.00887446 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 53.27 using 59 bins.
Reduced chi-squared = 0.934561
# Null hypothesis probability of 6.16e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 12.2523 ( -1.1524 1.1543 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.31987e-07 ( -8.9545e-08 8.98697e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 7.844 sec. to 8.844 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.21322 ( -0.686711 0.365227 )
Epeak [keV] : 148.071 ( -70.6743 -148.084 )
Norm@50keV : 0.135207 ( -0.0444706 0.151563 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 52.66 using 59 bins.
Reduced chi-squared = 0.940357
# Null hypothesis probability of 6.02e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 5.89702 ( -1.45523 2.06523 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.24358e-07 ( -4.97771e-08 9.18673e-08 ) ergs/cm2
Band function
Time interval is from 7.844 sec. to 8.844 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] : 15.9123 (-1.61856 1.82245)
R^2/D10^2 : 1.18068 (-0.380928 0.546343)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 79.87 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.45e-02 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.189e-08 1.066e-08
25- 50 2.592e-07 3.360e-08
50-150 4.577e-07 6.805e-08
15-150 7.788e-07 9.305e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-47.9006 -200)
Norm : 50.5398 (-4.55589 4.55589)
------------------------------------------------------------
#Fit statistic : Chi-Squared 53.42 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.10e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.264e-07 1.410e-08
25- 50 2.431e-07 3.745e-08
50-150 5.331e-07 1.727e-07
15-150 9.026e-07 2.447e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 9.88458 (-3.42659 2.92164)
R1^2/D10^2 : 4.52797 (-2.40745 11.0291)
kT2 [keV] : 40.9187 (-18.3791 -41.2455)
R2^2/D10^2 : 3.13491E-02 (-0.0294563 0.228615)
------------------------------------------------------------
#Fit statistic : Chi-Squared 54.35 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.00e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.640e-08 2.749e-08
25- 50 2.652e-07 8.160e-08
50-150 5.603e-07 2.636e-07
15-150 9.219e-07 3.541e-07
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: 1.51487 ( -0.0624699 0.0622967 )
Norm@50keV : 2.99297E-02 ( -0.00107174 0.00107168 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 76.87 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.08e-02 with 57 degrees of freedom
Photon flux (15-150 keV) in 43.1 sec: 3.75154 ( -0.150883 0.151369 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.22081e-05 ( -4.48675e-07 4.48934e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.23425 ( -0.260296 0.246189 )
Epeak [keV] : 150.988 ( -47.2739 538.017 )
Norm@50keV : 4.03785E-02 ( -0.00911356 0.0125283 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 73.06 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.25e-02 with 56 degrees of freedom
Photon flux (15-150 keV) in 43.1 sec: 3.69364 ( -0.15811 0.15874 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.20658e-05 ( -4.71342e-07 4.69531e-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) = 3.53e-06
S(50-100 keV) = 4.78e-06
T90 vs. Hardness ratio plot
T90 = 48 sec.
Hardness ratio (energy fluence ratio) = 1.35411
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.70359
Count Ratio (50-100 keV) / (15-25 keV) = 1.31125
Mask shadow pattern
IMX = -1.206666607996190E+00, IMY = -2.276023443369052E-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:
-199.155400 -31.656000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6156 22.0255 1.1 34.2 69.1 6.8335 10.4 1.2 Crab
74.7803 7.7557 2.8 40.8 94.4 5.7616 4.2 ------ UNKNOWN
84.7340 26.3127 0.3 32.1 62.0 20.3222 33.9 ------ UNKNOWN
27.8804 -5.7572 2.8 52.6 161.7 6.3573 4.2 ------ UNKNOWN
125.4569 42.4944 2.7 53.2 15.4 4.8951 4.3 ------ UNKNOWN
17.3725 7.3799 2.5 45.8 -177.9 3.1126 4.7 ------ UNKNOWN
9.2292 30.9497 3.0 34.8 -143.0 1.6952 3.9 ------ UNKNOWN
351.3429 25.3563 2.3 51.0 -137.1 7.6807 5.1 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-31.656000 11.444600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.5220 21.9264 4.5 34.2 69.3 0.7458 2.6 8.1 Crab
55.1593 15.1343 2.7 27.7 123.3 0.8188 4.3 ------ UNKNOWN
23.0970 -1.7629 0.5 50.8 169.3 18.3751 25.6 ------ UNKNOWN
36.6936 33.8978 2.5 14.0 -171.1 0.5397 4.7 ------ UNKNOWN
128.6595 71.4031 2.5 46.4 -21.8 0.9217 4.6 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
99.444590 962.427100
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
352.9920 20.7673 3.8 37.1 -22.1 2.9607 3.1 ------ UNKNOWN
348.3534 1.5462 3.5 34.9 -55.9 4.2735 3.3 ------ UNKNOWN
2.6558 -47.7142 3.3 49.3 -133.0 12.7459 3.5 ------ UNKNOWN
359.8755 -45.1308 2.5 48.0 -129.1 15.9859 4.7 ------ UNKNOWN
Plot creation:
Sat Jul 30 07:24:18 EDT 2022