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
332.8825 32.7207 0.0154 54.6549 0.5964 4.1594981 12.446 TRIG_01325580
Foreground time interval of the image:
-29.320 14.296 (delta_t = 43.616 [sec])
Background time interval of the image:
-272.920 -29.320 (delta_t = 243.600 [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
8 ms binning
From T100_start-3 s to T100_start+3 s
2 ms binning
From T100_start-1 s to T100_start+1 s
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 -29.320 sec. to 14.296 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.13353 ( -0.210812 0.226659 )
Norm@50keV : 5.65169E-03 ( -0.000819416 0.000799922 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 71.72 using 59 bins.
Reduced chi-squared = 1.25825
# Null hypothesis probability of 9.07e-02 with 57 degrees of freedom
Photon flux (15-150 keV) in 43.62 sec: 0.904241 ( -0.114957 0.115409 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.29893e-06 ( -3.02494e-07 3.04737e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -29.320 sec. to 14.296 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.02958 ( -1.18636 0.934254 )
Epeak [keV] : 41.8898 ( -17.9547 13.0283 )
Norm@50keV : 2.14446E-02 ( -0.0214449 0.0684626 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 67.51 using 59 bins.
Reduced chi-squared = 1.20554
# Null hypothesis probability of 1.39e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 43.62 sec: 0.861113 ( -0.120434 0.120828 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.19415e-06 ( -3.11861e-07 3.16731e-07 ) ergs/cm2
Band function
Time interval is from -29.320 sec. to 14.296 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] : 11.2722 (-1.39731 1.57678)
R^2/D10^2 : 0.265034 (-0.106794 0.178674)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 76.95 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.03e-02 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.083e-07 6.698e-08
25- 50 8.992e-07 1.433e-07
50-150 6.574e-07 1.861e-07
15-150 1.865e-06 2.903e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 62.2532 (-16.4692 25.3914)
Norm : 4.63983 (-0.867085 1.02579)
------------------------------------------------------------
#Fit statistic : Chi-Squared 67.80 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.55e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.116e-07 8.299e-08
25- 50 7.873e-07 1.119e-07
50-150 9.233e-07 2.600e-07
15-150 2.222e-06 3.160e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 2.27025 (-1.13629 2.59169)
R1^2/D10^2 : 248.580 (-245.688 178668)
kT2 [keV] : 12.7480 (-1.87277 2.8786)
R2^2/D10^2 : 0.152501 (-0.0915362 0.135129)
------------------------------------------------------------
#Fit statistic : Chi-Squared 65.60 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.55e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.159e-07 2.029e-07
25- 50 7.870e-07 1.786e-07
50-150 7.850e-07 2.441e-07
15-150 2.088e-06 4.851e-07
Peak spectrum fit
Power-law model
Time interval is from 0.188 sec. to 1.188 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 3.21147 ( -0.401442 0.61146 )
Norm@50keV : 9.10595E-03 ( -0.00421461 0.00394741 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 74.32 using 59 bins.
Reduced chi-squared = 1.30386
# Null hypothesis probability of 6.14e-02 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 2.93403 ( -0.82633 0.8264 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.21392e-07 ( -3.62351e-08 3.63982e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.188 sec. to 1.188 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -7.51464E-02 ( -2.94786 1.99698 )
Epeak [keV] : 34.8515 ( -35.0089 13.0765 )
Norm@50keV : 0.464456 ( -0.477931 10.5849 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 66.40 using 59 bins.
Reduced chi-squared = 1.18571
# Null hypothesis probability of 1.61e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 3.05884 ( -0.86667 0.84817 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.58453e-07 ( -4.02278e-08 4.3235e-08 ) ergs/cm2
Band function
Time interval is from 0.188 sec. to 1.188 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] : 10.7713 (-2.37574 2.08199)
R^2/D10^2 : 1.19102 (-0.631244 1.87622)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 67.04 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.71e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.874e-08 1.454e-08
25- 50 7.909e-08 4.050e-08
50-150 5.099e-08 2.721e-08
15-150 1.588e-07 6.734e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 29.3004 (-10.2769 10.2642)
Norm : 26.9292 (-9.22437 14.4722)
------------------------------------------------------------
#Fit statistic : Chi-Squared 67.85 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.54e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.414e-08 1.732e-08
25- 50 6.105e-08 2.383e-08
50-150 3.241e-08 2.116e-08
15-150 1.476e-07 5.012e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 2.72103 (-1.62255 2.20003)
R1^2/D10^2 : 309.513 (-299.494 816832)
kT2 [keV] : 11.8861 (-2.3783 2.28133)
R2^2/D10^2 : 0.689610 (-0.416767 1.02343)
------------------------------------------------------------
#Fit statistic : Chi-Squared 62.12 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.38e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.133e-08 2.971e-08
25- 50 6.722e-08 4.081e-08
50-150 5.408e-08 3.616e-08
15-150 1.726e-07 9.370e-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: 2.13353 ( -0.210812 0.226659 )
Norm@50keV : 5.65169E-03 ( -0.000819416 0.000799922 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 71.72 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.07e-02 with 57 degrees of freedom
Photon flux (15-150 keV) in 43.62 sec: 0.904160 ( -0.114941 0.115388 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.29851e-06 ( -3.0244e-07 3.04749e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.02949 ( -1.18634 0.93428 )
Epeak [keV] : 41.8899 ( -17.9217 13.0148 )
Norm@50keV : 2.14471E-02 ( -0.0214454 0.0684621 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 67.51 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.39e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 43.62 sec: 0.860957 ( -0.120387 0.120766 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.19467e-06 ( -3.11818e-07 3.17035e-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) = 7.15e-07
S(50-100 keV) = 6.54e-07
T90 vs. Hardness ratio plot
T90 = 36.527999997139 sec.
Hardness ratio (energy fluence ratio) = 0.914685
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.29312
Count Ratio (50-100 keV) / (15-25 keV) = 0.66738
Mask shadow pattern
IMX = 1.409917349138206E+00, IMY = -1.467674873633135E-02
TIME vs. PHA plot around the trigger time
TIME vs. DetID plot around the trigger time
100 us light curve (15-350 keV)
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:
-272.920000 -29.320000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.3523 35.3150 5.4 23.0 105.9 0.9940 2.1 5.4 Her X-1
299.5772 35.1910 0.8 35.4 29.3 8.3804 14.7 0.9 Cyg X-1
308.3765 40.9825 0.0 35.5 13.7 1.1172 2.2 12.2 Cyg X-3
326.1455 38.3222 55.7 46.8 1.3 -0.1267 -0.2 1.2 Cyg X-2
161.0329 54.6445 2.9 49.3 -132.1 6.8585 4.0 ------ UNKNOWN
21.7768 71.0634 3.8 44.9 -60.2 5.5550 3.0 ------ UNKNOWN
26.7267 73.5656 2.9 43.8 -64.1 7.3082 4.0 ------ UNKNOWN
159.7148 56.9585 3.0 48.1 -129.2 7.3479 3.8 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-29.320000 14.296000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.4548 35.3101 4.3 22.9 105.6 0.2733 2.7 1.9 Her X-1
299.6133 35.0588 13.2 35.6 29.4 0.1161 0.9 8.6 Cyg X-1
308.2829 40.8802 13.2 35.6 13.9 -0.0993 -0.9 9.0 Cyg X-3
326.0824 38.4086 5.4 46.7 1.3 0.3650 2.1 6.7 Cyg X-2
332.8825 32.7207 0.9 54.7 0.6 4.1602 12.4 ------ UNKNOWN
190.4906 53.7678 2.0 36.7 -149.3 0.6226 5.7 ------ UNKNOWN
358.2886 45.0421 2.1 57.5 -27.2 2.5203 5.5 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
775.980590 962.099300
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
299.5682 35.2025 0.7 27.6 137.1 5.8572 15.4 1.1 Cyg X-1
308.1960 40.9738 7.2 21.3 152.4 0.4931 1.6 4.1 Cyg X-3
326.2797 38.4573 37.0 7.9 171.3 0.0804 0.3 9.6 Cyg X-2
291.9659 48.6959 2.5 34.4 162.6 1.9596 4.6 ------ UNKNOWN
256.0716 62.5104 2.5 55.4 179.5 4.8291 4.6 ------ UNKNOWN
10.9736 -3.8645 2.1 51.4 -19.4 3.9021 5.6 ------ UNKNOWN
23.5206 27.2386 3.2 43.8 -64.1 5.1058 3.6 ------ UNKNOWN
25.1766 72.8963 2.7 48.1 -129.2 6.7627 4.3 ------ UNKNOWN
Plot creation:
Sun Mar 1 23:38:55 EST 2026