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
231.4229 -0.5465 0.0175 18.2395 -15.6573 0.1071848 11.043 TRIG_01285677
Foreground time interval of the image:
-0.020 0.564 (delta_t = 0.584 [sec])
Background time interval of the image:
-239.696 -0.020 (delta_t = 239.676 [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 -0.020 sec. to 0.564 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.30271 ( -0.272629 0.274668 )
Norm@50keV : 1.13863E-02 ( -0.0017251 0.00172233 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 54.13 using 59 bins.
Reduced chi-squared = 0.949649
# Null hypothesis probability of 5.83e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 0.584 sec: 1.35912 ( -0.21049 0.21108 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.56737e-08 ( -1.11265e-08 1.12275e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.020 sec. to 0.564 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.30143 ( -0.429267 0.274201 )
Epeak [keV] : 9999.28 ( -9999.36 -9999.36 )
Norm@50keV : 1.14248E-02 ( -0.00173417 0.0212233 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 54.13 using 59 bins.
Reduced chi-squared = 0.966607
# Null hypothesis probability of 5.46e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 0.584 sec: 1.35890 ( -0.21048 0.21092 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.57584e-08 ( -1.15454e-08 9.59845e-09 ) ergs/cm2
Band function
Time interval is from -0.020 sec. to 0.564 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] : 18.7110 (-3.64528 4.78153)
R^2/D10^2 : 7.55299E-02 (-0.0397788 0.0799717)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 65.83 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.98e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.052e-09 9.969e-10
25- 50 1.452e-08 3.895e-09
50-150 3.724e-08 1.121e-08
15-150 5.482e-08 1.430e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-59.697 -200)
Norm : 5.60833 (-0.85637 0.85637)
------------------------------------------------------------
#Fit statistic : Chi-Squared 57.11 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.71e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.158e-09 4.637e-09
25- 50 1.569e-08 8.938e-09
50-150 3.442e-08 1.946e-08
15-150 5.827e-08 3.238e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 3.96313 (-2.4132 3.97314)
R1^2/D10^2 : 11.9346 (-11.1354 5425.94)
kT2 [keV] : 24.2205 (-6.11927 22.1678)
R2^2/D10^2 : 2.97721E-02 (-0.0258743 0.0509678)
------------------------------------------------------------
#Fit statistic : Chi-Squared 54.42 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.97e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.861e-09 4.150e-09
25- 50 1.218e-08 5.587e-09
50-150 4.392e-08 2.109e-08
15-150 6.397e-08 2.752e-08
Peak spectrum fit
Power-law model
Time interval is from -0.226 sec. to 0.774 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.24759 ( -0.381345 0.375283 )
Norm@50keV : 5.87643E-03 ( -0.00122446 0.00122444 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 65.64 using 59 bins.
Reduced chi-squared = 1.15158
# Null hypothesis probability of 2.02e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.694757 ( -0.150371 0.151285 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.88545e-08 ( -1.34342e-08 1.35607e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.226 sec. to 0.774 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.48973 ( -3.22277 0.111546 )
Epeak [keV] : 159.304 ( )
Norm@50keV : 1.27274E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared 65.58 using 59 bins.
Reduced chi-squared = 1.17107
# Null hypothesis probability of 1.79e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.690232 ( -0.158075 0.154661 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.85113e-08 ( -1.4041e-08 1.37956e-08 ) ergs/cm2
Band function
Time interval is from -0.226 sec. to 0.774 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] : 19.5689 (-4.68437 6.89944)
R^2/D10^2 : 3.40688E-02 (-0.0214033 0.0508804)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 69.86 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.18e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.536e-09 1.107e-09
25- 50 1.245e-08 4.426e-09
50-150 3.523e-08 1.711e-08
15-150 5.022e-08 2.158e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-79.7122 -200)
Norm : 2.89058 (-0.612979 0.612979)
------------------------------------------------------------
#Fit statistic : Chi-Squared 67.74 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.56e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.198e-09 4.229e-09
25- 50 1.385e-08 8.045e-09
50-150 3.037e-08 1.733e-08
15-150 5.141e-08 3.005e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 1.69839 (-1.1613 4.16815)
R1^2/D10^2 : 1635.33 (-1633 -1633.92)
kT2 [keV] : 21.5291 (-5.29984 8.42275)
R2^2/D10^2 : 2.40918E-02 (-0.0157841 0.0354536)
------------------------------------------------------------
#Fit statistic : Chi-Squared 63.31 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.07e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.296e-09 2.383e-09
25- 50 1.093e-08 6.388e-09
50-150 3.769e-08 1.947e-08
15-150 5.392e-08 2.341e-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: 1.30271 ( -0.272629 0.274668 )
Norm@50keV : 1.13863E-02 ( -0.0017251 0.00172233 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 54.13 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.83e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 0.584 sec: 1.35910 ( -0.210484 0.211072 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.56679e-08 ( -1.11266e-08 1.123e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.30029 ( -0.426514 0.274673 )
Epeak [keV] : 9999.28 ( -9999.36 -9999.36 )
Norm@50keV : 1.14269E-02 ( -0.00173394 0.0212228 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 54.13 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.46e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 0.584 sec: 1.35984 ( -0.21257 0.20941 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.55844e-08 ( -1.1238e-08 1.12753e-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) = 1.47e-08
S(50-100 keV) = 2.37e-08
T90 vs. Hardness ratio plot
T90 = 0.483999967575073 sec.
Hardness ratio (energy fluence ratio) = 1.61224
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.50775
Count Ratio (50-100 keV) / (15-25 keV) = 1.29388
Mask shadow pattern
IMX = 3.173179519661429E-01, IMY = 8.893923559529868E-02
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:
-239.696000 -0.020000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
244.9653 -15.6139 0.7 35.9 -38.3 7.4206 16.1 1.8 Sco X-1
254.4526 35.3770 2.0 27.0 -151.1 2.1396 5.9 2.1 Her X-1
190.4125 41.7204 2.8 42.4 117.7 8.1128 4.1 ------ UNKNOWN
208.6265 13.2670 2.6 22.4 66.1 1.6731 4.5 ------ UNKNOWN
211.2108 10.6144 2.8 20.8 57.1 1.4870 4.1 ------ UNKNOWN
211.1897 -18.6552 2.7 41.4 14.0 2.4152 4.3 ------ UNKNOWN
266.0223 0.7583 2.6 38.0 -83.0 4.1684 4.5 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-0.020000 0.564000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
244.9728 -15.5537 5.0 35.8 -38.4 -0.0308 -2.3 5.2 Sco X-1
254.5484 35.1666 4.1 27.0 -150.7 -0.0286 -2.8 11.5 Her X-1
231.4230 -0.5465 1.0 18.2 -15.7 0.1072 11.0 ------ UNKNOWN
224.3981 -39.6229 2.3 57.7 -9.3 0.2446 5.1 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
61.804600 962.343900
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
244.9698 -15.6420 0.6 20.2 -58.9 28.3538 20.2 0.6 Sco X-1
254.4155 35.3876 5.7 41.8 -169.5 3.8080 2.0 3.4 Her X-1
255.7991 -37.9715 7.3 43.6 -46.1 4.8879 1.6 11.7 4U 1700-377
256.3950 -36.5521 9.9 42.8 -47.9 3.2943 1.2 8.0 GX 349+2
263.1782 -24.7344 87.8 39.1 -67.3 -0.3900 -0.1 9.2 GX 1+4
268.4963 -1.5489 15.0 37.1 -106.1 2.4761 0.8 9.6 SW J1753.5-0127
262.9341 -33.8593 64.9 44.5 -56.3 -0.8567 -0.2 3.1 GX 354-0
199.0337 28.3517 2.6 42.4 117.6 32.8256 4.5 ------ UNKNOWN
201.6871 -1.8943 3.0 29.7 69.1 8.4220 3.8 ------ UNKNOWN
223.3815 -51.9339 2.5 51.8 -11.7 11.5457 4.6 ------ UNKNOWN
227.8000 -56.1899 2.1 55.7 -15.6 16.6849 5.5 ------ UNKNOWN
Plot creation:
Fri Jun 20 01:53:55 EDT 2025