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
231.5627 -2.1733 0.0400 40.1461 0.0783 0.5030698 4.800 TRIG_01221183
Foreground time interval of the image:
-0.368 27.397 (delta_t = 27.765 [sec])
Background time interval of the image:
-114.603 -0.368 (delta_t = 114.235 [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 2.048000
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 2.048000
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 2.048000
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 -0.368 sec. to 33.920 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.67542 ( -0.417198 0.427243 )
Norm@50keV : 1.53227E-03 ( -0.000376666 0.000363158 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 41.50 using 59 bins.
Reduced chi-squared = 0.72807
# Null hypothesis probability of 9.39e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 34.29 sec: 0.201794 ( -0.04627 0.046391 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.87549e-07 ( -1.23158e-07 1.25193e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.368 sec. to 33.920 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.69492 ( -0.516787 0.414632 )
Epeak [keV] : 9999.36 ( -9999.35 -9999.36 )
Norm@50keV : 1.51642E-03 ( -0.000373949 0.00326873 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 41.52 using 59 bins.
Reduced chi-squared = 0.741429
# Null hypothesis probability of 9.26e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 34.29 sec: 0.202286 ( -0.047357 0.046409 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.50331e-07 ( -1.78972e-07 9.50152e-08 ) ergs/cm2
Band function
Time interval is from -0.368 sec. to 33.920 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] : 9.66924 (-2.33035 3.87619)
R^2/D10^2 : 0.106322 (-0.0767568 0.20003)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 49.61 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.46e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.857e-08 3.159e-08
25- 50 1.624e-07 6.623e-08
50-150 7.685e-08 4.682e-08
15-150 3.078e-07 1.520e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 161.228 (-103.507 -161.228)
Norm : 0.818034 (-0.196091 0.327136)
------------------------------------------------------------
#Fit statistic : Chi-Squared 42.54 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.23e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.157e-08 4.058e-08
25- 50 1.340e-07 7.472e-08
50-150 2.723e-07 1.621e-07
15-150 4.779e-07 2.796e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.52940 (-2.06249 2.22902)
R1^2/D10^2 : 0.241226 (-0.103855 0.4714)
kT2 [keV] : 86.7183 (-163.714 -195.05)
R2^2/D10^2 : 1.09269E-04 (-1.37601e-05 0.00119332)
------------------------------------------------------------
#Fit statistic : Chi-Squared 36.79 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.72e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.270e-08 5.126e-08
25- 50 1.423e-07 8.314e-08
50-150 3.096e-07 1.706e-07
15-150 5.346e-07 2.789e-07
Peak spectrum fit
Power-law model
Time interval is from 32.868 sec. to 33.868 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.60287 ( -0.493998 0.498937 )
Norm@50keV : 7.40114E-03 ( -0.00226659 0.00224491 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 57.76 using 59 bins.
Reduced chi-squared = 1.01333
# Null hypothesis probability of 4.47e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.951976 ( -0.295299 0.297704 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.92006e-08 ( -2.19464e-08 2.22886e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 32.868 sec. to 33.868 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.687966 ( -3.16176 1.54355 )
Epeak [keV] : 68.1151 ( -68.1137 -68.1137 )
Norm@50keV : 2.26059E-02 ( -0.0226071 1.12428 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 57.17 using 59 bins.
Reduced chi-squared = 1.02089
# Null hypothesis probability of 4.31e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.927039 ( -0.300572 0.303051 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.50609e-08 ( -2.36228e-08 2.41936e-08 ) ergs/cm2
Band function
Time interval is from 32.868 sec. to 33.868 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] : 13.5230 (-4.20155 6.19854)
R^2/D10^2 : 0.157973 (-0.15735 0.454724)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 58.84 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.08e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.119e-09 3.832e-09
25- 50 2.197e-08 1.370e-08
50-150 2.597e-08 1.669e-08
15-150 5.406e-08 3.265e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 155.108 (-100.66 -155.462)
Norm : 3.99258 (-1.25162 1.88858)
------------------------------------------------------------
#Fit statistic : Chi-Squared 57.36 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.62e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.022e-08 6.010e-09
25- 50 1.904e-08 1.112e-08
50-150 3.811e-08 2.409e-08
15-150 6.737e-08 4.041e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 8.21171 (-8.21863 -8.21863)
R1^2/D10^2 : 0.668753 (-0.666602 -0.666602)
kT2 [keV] : 27.5741 (-27.6744 -27.6744)
R2^2/D10^2 : 7.84132E-03 (-0.00772489 0.286381)
------------------------------------------------------------
#Fit statistic : Chi-Squared 56.73 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.10e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.290e-09 5.965e-09
25- 50 2.104e-08 1.268e-08
50-150 3.657e-08 2.269e-08
15-150 6.691e-08 3.314e-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: 1.66875 ( -0.698833 0.71212 )
Norm@50keV : 1.13214E-03 ( -0.000434326 0.000400394 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 42.30 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.27e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 27.76 sec: 0.148760 ( -0.0512186 0.0511857 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.91744e-07 ( -1.10999e-07 1.13939e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.28246 ( -1.50679 0.519183 )
Epeak [keV] : 104.414 ( )
Norm@50keV : 4.98858E-04 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared 41.50 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.26e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 27.76 sec: 0.149006 ( -0.025624 0.050884 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.88349e-07 ( -1.07821e-07 1.1315e-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) = 1.31e-07
S(50-100 keV) = 1.64e-07
T90 vs. Hardness ratio plot
T90 = 33.2640000581741 sec.
Hardness ratio (energy fluence ratio) = 1.25191
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.43237
Count Ratio (50-100 keV) / (15-25 keV) = 0.815484
Mask shadow pattern
IMX = 8.434542707590268E-01, IMY = -1.152957767770145E-03
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 2.048000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 2.048000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 2.048000
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:
-114.603400 -0.368000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
195.5788 -29.5613 3.0 32.1 77.5 1.7356 3.9 ------ UNKNOWN
200.7481 -16.2291 3.1 20.6 58.4 0.9483 3.8 ------ UNKNOWN
239.2581 -13.3309 2.1 49.7 13.6 2.9552 5.4 ------ UNKNOWN
242.4405 10.0951 2.5 51.0 -17.2 2.4280 4.6 ------ UNKNOWN
220.7686 17.4338 2.5 32.3 -35.8 1.2241 4.6 ------ UNKNOWN
166.6011 40.3002 2.1 44.2 -123.6 4.3618 5.4 ------ UNKNOWN
158.9416 40.4358 2.3 48.2 -129.5 5.5212 5.0 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-0.368000 27.396590
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
Post-slew image of 15-350 keV band
Time interval of the image:
158.596600 562.196600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
244.9744 -15.6256 0.8 18.9 -30.4 11.4755 14.9 0.9 Sco X-1
254.3602 35.3113 36.6 43.1 -139.1 -0.4879 -0.3 5.1 Her X-1
256.0642 -37.8928 6.6 42.2 -15.8 2.0598 1.7 4.7 4U 1700-377
256.2600 -36.3588 8.5 41.1 -17.5 1.5766 1.4 9.3 GX 349+2
263.0097 -24.7863 5.2 37.8 -37.2 2.5368 2.2 2.4 GX 1+4
264.8672 -44.4022 5.8 51.5 -16.8 -3.8006 -2.0 6.0 4U 1735-44
268.3308 -1.4877 7.1 36.7 -77.1 2.6160 1.6 3.1 SW J1753.5-0127
270.2034 -24.9679 7.2 43.7 -41.8 2.4013 1.6 8.0 GX 5-1
270.1981 -25.8951 19.1 44.1 -40.6 0.9406 0.6 10.7 GRS 1758-258
273.9887 -14.0585 34.7 43.6 -58.4 -1.0415 -0.3 1.7 GX 17+2
275.9124 -30.2678 5.8 50.5 -38.2 5.4560 2.0 6.0 H1820-303
262.9609 -33.9971 7.9 43.3 -25.8 -1.8815 -1.5 9.8 GX 354-0
201.8198 -15.2651 2.6 32.1 77.5 7.1460 4.4 ------ UNKNOWN
200.3989 23.0677 2.9 39.5 144.8 7.8024 3.9 ------ UNKNOWN
253.0844 -47.4406 2.4 49.0 -5.9 6.4088 4.7 ------ UNKNOWN
Plot creation:
Sat Oct 19 18:31:53 EDT 2024