Special notes of this burst
Image
Pre-slew 15.0-350.0 keV image (Event data)
# RAcent DECcent POSerr Theta Phi Peak Cts SNR Name
59.4757 -15.1358 0.0156 40.2471 -59.5840 0.6253832 12.360 TRIG_01290305
Foreground time interval of the image:
-0.220 1.844 (delta_t = 2.064 [sec])
Background time interval of the image:
-194.491 -0.220 (delta_t = 194.271 [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 -0.220 sec. to 1.844 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.41801 ( -0.229011 0.22981 )
Norm@50keV : 2.00056E-02 ( -0.00266355 0.00265496 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 45.64 using 59 bins.
Reduced chi-squared = 0.800702
# Null hypothesis probability of 8.60e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 2.064 sec: 2.44650 ( -0.33155 0.33247 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.97595e-07 ( -5.79303e-08 5.8379e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.220 sec. to 1.844 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.27291 ( -0.998392 1.36152 )
Epeak [keV] : 260.707 ( -266.328 -266.328 )
Norm@50keV : 2.35518E-02 ( -0.0194291 0.0458727 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 45.57 using 59 bins.
Reduced chi-squared = 0.81375
# Null hypothesis probability of 8.39e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 2.064 sec: 2.43319 ( -0.3423 0.33308 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.94511e-07 ( -6.14989e-08 5.96395e-08 ) ergs/cm2
Band function
Time interval is from -0.220 sec. to 1.844 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] : 17.0339 (-2.6673 3.25392)
R^2/D10^2 : 0.182816 (-0.0828602 0.146547)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 59.05 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.01e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.229e-08 6.290e-09
25- 50 9.876e-08 2.055e-08
50-150 2.047e-07 4.926e-08
15-150 3.258e-07 6.398e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-63.5338 -200)
Norm : 10.1155 (-1.33445 1.33445)
------------------------------------------------------------
#Fit statistic : Chi-Squared 46.79 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.31e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.199e-08 2.938e-08
25- 50 1.000e-07 5.538e-08
50-150 2.194e-07 1.233e-07
15-150 3.714e-07 2.040e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 4.93354 (-2.00262 3.451)
R1^2/D10^2 : 8.16973 (-6.98152 89.0001)
kT2 [keV] : 22.7709 (-4.84845 10.6036)
R2^2/D10^2 : 5.97389E-02 (-0.0444793 0.0817335)
------------------------------------------------------------
#Fit statistic : Chi-Squared 45.26 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.23e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.050e-08 2.680e-08
25- 50 8.736e-08 3.625e-08
50-150 2.443e-07 1.299e-07
15-150 3.821e-07 1.489e-07
Peak spectrum fit
Power-law model
Time interval is from 0.424 sec. to 1.424 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.33719 ( -0.257948 0.260136 )
Norm@50keV : 2.41030E-02 ( -0.0039001 0.00389427 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 50.68 using 59 bins.
Reduced chi-squared = 0.889123
# Null hypothesis probability of 7.10e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 2.89622 ( -0.48126 0.48291 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.36118e-07 ( -4.12009e-08 4.15015e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.424 sec. to 1.424 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -5.13541E-02 ( -1.66889 1.18114 )
Epeak [keV] : 84.7899 ( -19.6206 135.047 )
Norm@50keV : 9.98790E-02 ( -0.0998791 0.351531 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 46.50 using 59 bins.
Reduced chi-squared = 0.830357
# Null hypothesis probability of 8.13e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 2.74153 ( -0.51078 0.50578 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.49415e-08 ( -4.40135e-08 1.71666e-08 ) ergs/cm2
Band function
Time interval is from 0.424 sec. to 1.424 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] : 19.0576 (-2.93604 3.54623)
R^2/D10^2 : 0.161623 (-0.0715145 0.122873)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 48.04 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.95e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.153e-08 3.816e-09
25- 50 5.555e-08 1.593e-08
50-150 1.484e-07 4.723e-08
15-150 2.154e-07 5.260e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-64.5192 -200)
Norm : 12.1239 (-1.96233 1.96233)
------------------------------------------------------------
#Fit statistic : Chi-Squared 51.31 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.87e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.019e-08 1.731e-08
25- 50 5.808e-08 3.310e-08
50-150 1.274e-07 7.100e-08
15-150 2.156e-07 1.212e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 4.01849 (-2.28189 3.98854)
R1^2/D10^2 : 16.4562 (-15.5616 2377.55)
kT2 [keV] : 21.1669 (-3.64331 5.12137)
R2^2/D10^2 : 0.106307 (-0.0576333 0.0624676)
------------------------------------------------------------
#Fit statistic : Chi-Squared 43.04 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.79e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.427e-08 1.258e-08
25- 50 5.192e-08 2.011e-08
50-150 1.548e-07 7.405e-08
15-150 2.310e-07 8.769e-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: 1.41801 ( -0.229011 0.22981 )
Norm@50keV : 2.00056E-02 ( -0.00266355 0.00265496 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 45.64 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.60e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 2.064 sec: 2.44646 ( -0.331538 0.332444 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.97547e-07 ( -5.79262e-08 5.83965e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.26594 ( -1.00665 0.371925 )
Epeak [keV] : 235.055 ( -265.861 -265.861 )
Norm@50keV : 2.36779E-02 ( -0.00605764 0.0458433 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 45.61 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.38e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 2.064 sec: 2.43291 ( -0.3422 0.33525 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.94666e-07 ( -6.15278e-08 6.05309e-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) = 9.43e-08
S(50-100 keV) = 1.41e-07
T90 vs. Hardness ratio plot
T90 = 1.79999995231628 sec.
Hardness ratio (energy fluence ratio) = 1.49523
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.40748
Count Ratio (50-100 keV) / (15-25 keV) = 1.3685
Mask shadow pattern
IMX = 4.285496407615806E-01, IMY = 7.299776838040873E-01
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:
-194.491400 -0.220000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6311 22.0258 0.8 43.8 8.4 6.8711 13.9 0.7 Crab
135.5592 -40.6044 2.5 36.8 167.3 1.8880 4.5 3.3 Vela X-1
154.1997 -62.0998 2.3 57.0 -173.8 5.7641 5.0 ------ UNKNOWN
61.7114 -42.5922 2.3 41.5 -102.2 6.9574 5.0 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-0.220000 1.844000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6753 21.9164 3.7 43.7 8.3 0.0982 3.1 6.3 Crab
135.2866 -40.5495 0.0 36.6 167.4 -0.0341 -1.4 11.0 Vela X-1
133.9363 -66.4516 2.6 52.7 -163.1 0.2456 4.5 ------ UNKNOWN
59.4758 -15.1358 0.9 40.2 -59.6 0.6254 12.4 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
105.908580 903.048000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6382 22.0310 0.9 44.1 42.1 19.3005 13.3 1.0 Crab
88.1215 -65.6299 2.5 54.0 174.9 9.8678 4.6 ------ UNKNOWN
16.4254 -25.2517 3.1 41.5 -102.1 12.3747 3.7 ------ UNKNOWN
Plot creation:
Fri Jun 20 17:35:25 EDT 2025