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
190.1030 -2.8870 0.0052 26.8836 37.4443 4.1253786 37.300 TRIG_01273106
Foreground time interval of the image:
-15.120 15.181 (delta_t = 30.301 [sec])
Background time interval of the image:
-239.120 -15.120 (delta_t = 224.000 [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 -15.120 sec. to 64.880 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.45122 ( -0.0471175 0.0471154 )
Norm@50keV : 8.64605E-03 ( -0.000224301 0.000224296 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 85.62 using 59 bins.
Reduced chi-squared = 1.50211
# Null hypothesis probability of 8.42e-03 with 57 degrees of freedom
Photon flux (15-150 keV) in 80 sec: 1.06585 ( -0.02997 0.03004 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.6182e-06 ( -1.8229e-07 1.82756e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -15.120 sec. to 64.880 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.874078 ( -0.213192 0.203585 )
Epeak [keV] : 106.093 ( -14.9112 28.2902 )
Norm@50keV : 1.59799E-02 ( -0.00304008 0.00395268 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 60.31 using 59 bins.
Reduced chi-squared = 1.07696
# Null hypothesis probability of 3.23e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 80 sec: 1.02640 ( -0.032496 0.03259 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.3772e-06 ( -2.02157e-07 2.0165e-07 ) ergs/cm2
Band function
Time interval is from -15.120 sec. to 64.880 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] : 16.8708 ( )
R^2/D10^2 : 8.03613E-02 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 270.18 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.83e-29 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.734e-07 1.744e-08
25- 50 1.642e-06 6.040e-08
50-150 3.329e-06 1.500e-07
15-150 5.345e-06 1.696e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-6.69312 -200)
Norm : 4.42103 (-0.114637 0.114637)
------------------------------------------------------------
#Fit statistic : Chi-Squared 85.12 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.28e-03 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.809e-07 2.680e-08
25- 50 1.694e-06 4.600e-08
50-150 3.716e-06 1.084e-07
15-150 6.292e-06 1.880e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.75544 (-0.876558 0.963232)
R1^2/D10^2 : 0.655796 (-0.197287 0.313257)
kT2 [keV] : 25.9031 (-2.27317 3.08305)
R2^2/D10^2 : 1.43608E-02 (-0.00500008 0.00613851)
------------------------------------------------------------
#Fit statistic : Chi-Squared 60.58 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.82e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.884e-07 6.660e-08
25- 50 1.682e-06 1.028e-07
50-150 3.971e-06 3.068e-07
15-150 6.341e-06 3.756e-07
Peak spectrum fit
Power-law model
Time interval is from 8.380 sec. to 9.380 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.47461 ( -0.235545 0.241994 )
Norm@50keV : 1.18151E-02 ( -0.00189051 0.00187467 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 57.98 using 59 bins.
Reduced chi-squared = 1.01719
# Null hypothesis probability of 4.39e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 1.46518 ( -0.22561 0.22574 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.12582e-07 ( -1.95441e-08 1.98064e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 8.380 sec. to 9.380 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -9.18361E-03 ( -1.46189 1.10763 )
Epeak [keV] : 65.6412 ( -14.3523 53.5449 )
Norm@50keV : 7.00599E-02 ( -0.0700599 0.329264 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 52.38 using 59 bins.
Reduced chi-squared = 0.935357
# Null hypothesis probability of 6.13e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 1.41956 ( -0.22771 0.22827 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.03727e-07 ( -2.0003e-08 2.08621e-08 ) ergs/cm2
Band function
Time interval is from 8.380 sec. to 9.380 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] : 14.5380 (-2.19751 2.62817)
R^2/D10^2 : 0.203064 (-0.0907071 0.156476)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 55.29 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.40e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.027e-09 2.563e-09
25- 50 3.483e-08 7.345e-09
50-150 4.939e-08 1.421e-08
15-150 9.324e-08 1.929e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.363 (-91.212 -199.363)
Norm : 6.07543 (-0.922317 0.922462)
------------------------------------------------------------
#Fit statistic : Chi-Squared 56.05 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.11e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.513e-08 8.640e-09
25- 50 2.910e-08 1.618e-08
50-150 6.383e-08 3.612e-08
15-150 1.081e-07 6.115e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 8.36951 (-8.33821 -8.39865)
R1^2/D10^2 : 0.665933 (-0.575337 -0.663076)
kT2 [keV] : 21.0716 (-21.1123 -21.1124)
R2^2/D10^2 : 3.83776E-02 (-0.0376217 0.170387)
------------------------------------------------------------
#Fit statistic : Chi-Squared 52.01 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.90e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.192e-08 6.930e-09
25- 50 3.301e-08 1.876e-08
50-150 5.981e-08 3.485e-08
15-150 1.047e-07 5.370e-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: 1.07745 ( -0.0655463 0.0649345 )
Norm@50keV : 9.35416E-03 ( -0.000357033 0.000356656 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 69.79 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.19e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 30.3 sec: 1.08277 ( -0.0427481 0.042814 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.98501e-06 ( -1.20423e-07 1.2063e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.450344 ( -0.299788 0.28024 )
Epeak [keV] : 141.714 ( -28.0072 66.0161 )
Norm@50keV : 1.77633E-02 ( -0.00431033 0.00609579 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 54.03 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.50e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 30.3 sec: 1.05331 ( -0.04456 0.0446 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.89953e-06 ( -1.29269e-07 1.28539e-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) = 1.60e-06
S(50-100 keV) = 2.34e-06
T90 vs. Hardness ratio plot
T90 = 64 sec.
Hardness ratio (energy fluence ratio) = 1.4625
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.59557
Count Ratio (50-100 keV) / (15-25 keV) = 1.28203
Mask shadow pattern
IMX = 4.025049784344334E-01, IMY = -3.082318771517079E-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:
-239.120000 -15.120000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
244.9603 -15.6409 0.8 35.5 -90.0 13.8545 14.2 1.1 Sco X-1
254.3856 35.4301 9.6 46.8 -171.9 -0.9789 -1.2 6.3 Her X-1
185.4740 -23.3217 2.9 41.0 9.0 2.5151 3.9 ------ UNKNOWN
229.0037 -5.9994 3.3 17.1 -86.4 1.5023 3.5 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-15.120000 15.180590
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
245.0403 -15.8244 0.0 35.6 -89.8 0.3556 1.7 11.6 Sco X-1
254.4078 35.1717 5.7 46.6 -171.6 0.3313 2.0 10.5 Her X-1
178.0105 23.3963 2.4 40.8 84.5 1.9219 4.9 ------ UNKNOWN
208.3882 53.3640 1.9 48.8 138.0 2.5433 6.0 ------ UNKNOWN
190.1030 -2.8870 0.3 26.9 37.4 4.1248 37.3 ------ UNKNOWN
255.3973 49.9603 2.2 55.9 173.6 2.3493 5.2 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
80.980600 284.180600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
173.6514 30.6745 2.6 37.1 132.8 3.4762 4.4 ------ UNKNOWN
165.4177 -31.8699 2.8 37.1 12.6 2.1311 4.1 ------ UNKNOWN
162.1694 -49.2235 2.6 52.1 -0.6 3.2239 4.5 ------ UNKNOWN
Plot creation:
Fri Jun 20 02:01:53 EDT 2025