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
171.0546 42.1523 0.0094 35.6533 70.3758 0.6915236 20.636 TRIG_01014037
Foreground time interval of the image:
-0.056 0.168 (delta_t = 0.224 [sec])
Background time interval of the image:
-42.379 -0.056 (delta_t = 42.323 [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 0.128000
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 0.128000
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 0.128000
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 -0.056 sec. to 0.168 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.57587 ( -0.135901 0.139297 )
Norm@50keV : 0.180785 ( -0.0159344 0.0158349 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 63.16 using 59 bins.
Reduced chi-squared = 1.10807
# Null hypothesis probability of 2.68e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 0.224 sec: 23.0623 ( -1.975 1.9762 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.79933e-07 ( -3.57829e-08 3.60044e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.056 sec. to 0.168 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.968236 ( -0.599512 0.532398 )
Epeak [keV] : 88.3117 ( -22.2242 203.851 )
Norm@50keV : 0.362763 ( -0.162408 0.341338 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 59.29 using 59 bins.
Reduced chi-squared = 1.05875
# Null hypothesis probability of 3.57e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 0.224 sec: 22.6968 ( -2.0041 2.004 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.72176e-07 ( -3.70346e-08 3.70545e-08 ) ergs/cm2
Band function
Time interval is from -0.056 sec. to 0.168 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] : 15.3639 (-1.56261 1.71207)
R^2/D10^2 : 2.47951 (-0.767366 1.12251)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 89.22 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.09e-03 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.733e-08 4.580e-09
25- 50 1.110e-07 1.248e-08
50-150 1.802e-07 2.946e-08
15-150 3.185e-07 3.461e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 188.374 (-62.9467 -190.615)
Norm : 94.8618 (-8.1796 8.83952)
------------------------------------------------------------
#Fit statistic : Chi-Squared 60.15 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.62e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.298e-08 1.114e-08
25- 50 1.018e-07 3.284e-08
50-150 2.225e-07 1.039e-07
15-150 3.773e-07 1.584e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.33434 (-1.39397 1.98348)
R1^2/D10^2 : 58.2808 (-39.9418 149.723)
kT2 [keV] : 21.2464 (-3.07672 4.53366)
R2^2/D10^2 : 0.663546 (-0.355807 0.549029)
------------------------------------------------------------
#Fit statistic : Chi-Squared 57.24 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.92e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.346e-08 2.434e-08
25- 50 9.649e-08 2.412e-08
50-150 2.216e-07 5.587e-08
15-150 3.716e-07 8.243e-08
Peak spectrum fit
Power-law model
Time interval is from -0.442 sec. to 0.558 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.54237 ( -0.157346 0.160795 )
Norm@50keV : 4.39432E-02 ( -0.00441488 0.00438549 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 68.67 using 59 bins.
Reduced chi-squared = 1.20474
# Null hypothesis probability of 1.38e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 5.55091 ( -0.54294 0.54332 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.142e-07 ( -4.48739e-08 4.51461e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.442 sec. to 0.558 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.997324 ( -0.704117 0.599984 )
Epeak [keV] : 93.9886 ( -28.6382 -93.9886 )
Norm@50keV : 8.27339E-02 ( -0.0403913 0.0996245 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 66.36 using 59 bins.
Reduced chi-squared = 1.185
# Null hypothesis probability of 1.62e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 5.46770 ( -0.55261 0.55205 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.04101e-07 ( -4.68611e-08 4.68922e-08 ) ergs/cm2
Band function
Time interval is from -0.442 sec. to 0.558 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] : 15.1229 (-1.74218 1.96808)
R^2/D10^2 : 0.629669 (-0.220184 0.336403)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 88.68 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.57e-03 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.011e-08 5.545e-09
25- 50 1.205e-07 1.658e-08
50-150 1.883e-07 3.715e-08
15-150 3.389e-07 4.145e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.363 (-70.5873 -199.363)
Norm : 22.8012 (-2.18676 2.18938)
------------------------------------------------------------
#Fit statistic : Chi-Squared 66.87 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.74e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.678e-08 2.025e-08
25- 50 1.092e-07 2.944e-08
50-150 2.395e-07 1.266e-07
15-150 4.055e-07 1.479e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.61340 (-1.97162 3.18154)
R1^2/D10^2 : 11.2510 (-8.64728 55.9318)
kT2 [keV] : 21.5458 (-4.07582 8.76421)
R2^2/D10^2 : 0.150693 (-0.111495 0.188387)
------------------------------------------------------------
#Fit statistic : Chi-Squared 66.67 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.35e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.560e-08 2.623e-08
25- 50 1.048e-07 3.416e-08
50-150 2.391e-07 8.585e-08
15-150 3.995e-07 1.283e-07
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: 1.57587 ( -0.135901 0.139297 )
Norm@50keV : 0.180785 ( -0.0159344 0.0158349 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 63.16 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.68e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 0.224 sec: 23.0615 ( -1.97482 1.97617 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.79882e-07 ( -3.58382e-08 3.60125e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.968231 ( -0.59951 0.5324 )
Epeak [keV] : 88.3110 ( -22.224 203.853 )
Norm@50keV : 0.362766 ( -0.16241 0.341337 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 59.29 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.57e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 0.224 sec: 22.6942 ( -2.0037 2.0035 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.72313e-07 ( 0 0 ) 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) = 9.74e-08
S(50-100 keV) = 1.31e-07
T90 vs. Hardness ratio plot
T90 = 0.164000034332275 sec.
Hardness ratio (energy fluence ratio) = 1.34497
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.3214
Count Ratio (50-100 keV) / (15-25 keV) = 1.08818
Mask shadow pattern
IMX = 2.409176770347630E-01, IMY = -6.756719300417512E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.128000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.128000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.128000
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:
-42.379340 -0.056000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.4054 35.1346 0.0 27.6 -121.4 -0.3911 -3.6 12.7 Her X-1
193.9145 8.4015 2.3 41.3 5.5 0.6287 4.9 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-0.056000 0.168000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.2312 35.3907 0.0 27.3 -121.8 -0.0181 -1.6 11.4 Her X-1
171.0546 42.1523 0.6 35.7 70.4 0.6915 20.6 ------ UNKNOWN
214.0492 17.6409 3.0 25.6 -22.5 0.0434 3.9 ------ UNKNOWN
238.0174 5.6191 2.7 40.4 -64.1 0.0923 4.3 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
71.620600 753.220600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
239.2963 47.1694 3.9 47.2 -132.5 6.3294 3.0 ------ UNKNOWN
242.2564 46.8609 3.0 49.2 -133.1 10.3888 3.9 ------ UNKNOWN
Plot creation:
Sat Jul 30 07:22:40 EDT 2022