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
283.3233 -13.4483 0.0108 27.2186 87.7392 3.2332168 17.883 TRIG_00744773
Foreground time interval of the image:
-69.675 7.972 (delta_t = 77.647 [sec])
Background time interval of the image:
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 4.096000
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 4.096000
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 4.096000
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 -143.864 sec. to 7.972 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.33330 ( -0.0778339 0.0773998 )
Norm@50keV : 3.69883E-03 ( -0.000153455 0.000153414 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 37.36 using 59 PHA bins.
# Reduced chi-squared = 0.6555 for 57 degrees of freedom
# Null hypothesis probability = 9.794295e-01
Photon flux (15-150 keV) in 151.8 sec: 0.444107 ( -0.019985 0.020072 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.50544e-06 ( -2.43062e-07 2.43689e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -143.864 sec. to 7.972 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.32957 ( -0.26826 0.0833196 )
Epeak [keV] : 1.00000E+04 ( -10000 -10000 )
Norm@50keV : 3.71356E-03 ( -0.000153792 0.000153782 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 37.37 using 59 PHA bins.
# Reduced chi-squared = 0.6673 for 56 degrees of freedom
# Null hypothesis probability = 9.738186e-01
Photon flux (15-150 keV) in 151.8 sec: 0.444792 ( -0.022792 0.020778 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.51356e-06 ( -2.72829e-07 2.54795e-07 ) ergs/cm2
Band function
Time interval is from -143.864 sec. to 7.972 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] : 18.7099 ( )
R^2/D10^2 : 2.38139E-02 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 173.30 using 59 PHA bins.
# Reduced chi-squared = 3.0404 for 57 degrees of freedom
# Null hypothesis probability = 1.149807e-13
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.501e-07 2.315e-08
25- 50 1.190e-06 7.590e-08
50-150 3.051e-06 2.110e-07
15-150 4.491e-06 2.285e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-8.23073 -200)
Norm : 1.86826 (-0.0781216 0.0781216)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 67.22 using 59 PHA bins.
# Reduced chi-squared = 1.179 for 57 degrees of freedom
# Null hypothesis probability = 1.667220e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.061e-07 3.567e-08
25- 50 1.358e-06 6.793e-08
50-150 2.979e-06 1.419e-07
15-150 5.044e-06 2.338e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.46661 (-1.13272 1.30249)
R1^2/D10^2 : 0.339245 (-0.138629 0.264268)
kT2 [keV] : 31.4250 (-4.30279 6.78615)
R2^2/D10^2 : 3.58027E-03 (-0.00166986 0.00232563)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 41.92 using 59 PHA bins.
# Reduced chi-squared = 0.7622 for 55 degrees of freedom
# Null hypothesis probability = 9.027516e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.723e-07 9.609e-08
25- 50 1.272e-06 1.480e-07
50-150 3.664e-06 4.949e-07
15-150 5.509e-06 6.702e-07
Peak spectrum fit
Power-law model
Time interval is from -134.708 sec. to -133.708 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.02661 ( -0.104324 0.103061 )
Norm@50keV : 3.96144E-02 ( -0.00241224 0.00240747 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 58.20 using 59 PHA bins.
# Reduced chi-squared = 1.021 for 57 degrees of freedom
# Null hypothesis probability = 4.309675e-01
Photon flux (15-150 keV) in 1 sec: 4.56788 ( -0.28473 0.28519 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.24444e-07 ( -2.73988e-08 2.74952e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -134.708 sec. to -133.708 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.559419 ( -0.453776 0.408432 )
Epeak [keV] : 183.251 ( -61.8113 683.907 )
Norm@50keV : 6.30008E-02 ( -0.0205832 0.0338109 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 54.33 using 59 PHA bins.
# Reduced chi-squared = 0.9702 for 56 degrees of freedom
# Null hypothesis probability = 5.382716e-01
Photon flux (15-150 keV) in 1 sec: 4.48472 ( -0.29358 0.29389 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.18042e-07 ( -2.85308e-08 2.84257e-08 ) ergs/cm2
Band function
Time interval is from -134.708 sec. to -133.708 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] : 22.6454 (-1.73446 1.93544)
R^2/D10^2 : 0.150729 (-0.0342608 0.0432721)
(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 PHA bins.
# Reduced chi-squared = 1.556 for 57 degrees of freedom
# Null hypothesis probability = 4.570808e-03
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.411e-08 1.685e-09
25- 50 7.590e-08 7.040e-09
50-150 2.908e-07 2.795e-08
15-150 3.808e-07 2.865e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.363 ( )
Norm : 18.7848 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 126.45 using 59 PHA bins.
# Reduced chi-squared = 2.2185 for 57 degrees of freedom
# Null hypothesis probability = 3.521405e-07
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.678e-08 3.460e-09
25- 50 8.998e-08 7.225e-09
50-150 1.973e-07 3.700e-08
15-150 3.341e-07 6.000e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.44162 (-1.84566 2.50971)
R1^2/D10^2 : 2.35416 (-1.3893 3.96214)
kT2 [keV] : 30.5425 (-4.19946 7.02489)
R2^2/D10^2 : 5.18749E-02 (-0.0258552 0.0335546)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 52.30 using 59 PHA bins.
# Reduced chi-squared = 0.9509 for 55 degrees of freedom
# Null hypothesis probability = 5.785522e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.971e-08 1.262e-08
25- 50 8.068e-08 2.011e-08
50-150 3.114e-07 6.620e-08
15-150 4.218e-07 7.840e-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: 1.74333 ( -0.149817 0.153249 )
Norm@50keV : 2.49941E-03 ( -0.000231729 0.0002288 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 40.21 using 59 PHA bins.
# Reduced chi-squared = 0.7054 for 57 degrees of freedom
# Null hypothesis probability = 9.550983e-01
Photon flux (15-150 keV) in 77.65 sec: 0.337135 ( -0.028528 0.0285548 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.79154e-06 ( -1.7152e-07 1.73427e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.46905 ( -0.692795 0.634629 )
Epeak [keV] : 88.2606 ( )
Norm@50keV : 3.52531E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 39.63 using 59 PHA bins.
# Reduced chi-squared = 0.7076 for 56 degrees of freedom
# Null hypothesis probability = 9.521274e-01
Photon flux (15-150 keV) in 77.65 sec: 0.333038 ( -0.030006 0.029878 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.74476e-06 ( -2.0189e-07 2.00849e-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) = 1.25e-06
S(50-100 keV) = 1.99e-06
T90 vs. Hardness ratio plot
T90 = 144.46799993515 sec.
Hardness ratio (energy fluence ratio) = 1.592
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.4333
Count Ratio (50-100 keV) / (15-25 keV) = 1.29551
Mask shadow pattern
IMX = 2.028951154618287E-02, IMY = -5.139404562040610E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 4.096000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 4.096000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 4.096000
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:
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-69.675400 7.972000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
270.1403 -25.0756 83.0 41.3 70.3 -0.0659 -0.1 7.8 GX 5-1
270.3229 -25.6262 11.7 41.2 69.4 -0.4928 -1.0 7.1 GRS 1758-258
273.9973 -14.0396 99.0 36.3 87.1 0.0381 0.1 0.5 GX 17+2
276.0219 -30.3883 5.1 38.0 59.9 0.6571 2.3 5.2 H1820-303
284.9799 -24.7798 5.9 28.4 63.2 0.3500 1.9 9.0 HT1900.1-2455
288.7708 10.9204 2.5 31.0 140.0 0.8324 4.7 2.2 GRS 1915+105
299.6083 35.2095 1.1 47.2 173.5 3.1489 10.1 1.0 Cyg X-1
308.2200 40.9409 5.0 51.8 -176.4 0.8906 2.3 5.0 Cyg X-3
326.0744 38.4732 93.0 51.2 -158.6 0.0438 0.1 10.2 Cyg X-2
283.3233 -13.4483 0.6 27.2 87.7 3.2325 17.9 ------ UNKNOWN
339.2962 -62.5173 2.2 55.6 -9.1 2.2992 5.1 ------ UNKNOWN
332.2487 40.7934 3.4 55.1 -154.2 2.3839 3.4 ------ UNKNOWN
356.0803 -24.1431 2.9 44.8 -60.2 2.3391 4.0 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
87.724610 962.978300
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
244.9623 -15.6254 1.1 37.2 86.9 26.3455 10.3 1.3 Sco X-1
255.9985 -37.8232 0.9 34.4 45.0 18.1812 12.6 1.4 4U 1700-377
256.5070 -36.5168 3.9 33.3 46.5 4.0443 3.0 6.6 GX 349+2
262.9985 -24.7277 1.8 22.3 61.6 5.6212 6.3 1.2 GX 1+4
264.7965 -44.6020 6.3 34.9 28.4 2.1768 1.8 9.4 4U 1735-44
268.2182 -1.3190 0.0 19.3 132.8 -1.3014 -1.5 12.0 SW J1753.5-0127
270.4476 -25.0981 16.7 16.8 49.4 0.5717 0.7 9.0 GX 5-1
270.1382 -25.7156 6.6 17.5 48.5 1.4576 1.8 9.0 GRS 1758-258
274.1173 -13.8826 4.7 9.0 91.2 1.7521 2.4 11.3 GX 17+2
275.8526 -30.2742 11.4 18.2 26.3 0.7270 1.0 6.7 H1820-303
285.1810 -24.7566 0.0 11.4 -3.3 0.2940 0.3 12.6 HT1900.1-2455
288.7539 10.9091 1.5 24.9 -162.3 6.1063 7.6 3.4 GRS 1915+105
299.6008 35.1906 1.0 51.0 -157.8 27.1484 11.3 0.8 Cyg X-1
262.8719 -33.9662 10.6 27.7 43.8 1.0557 1.1 9.8 GX 354-0
259.8938 -25.0180 0.7 24.9 64.0 16.4395 16.7 ------ UNKNOWN
268.4515 36.3519 2.6 51.7 169.8 11.2337 4.4 ------ UNKNOWN
285.5894 -65.3992 3.3 52.0 3.9 6.6416 3.5 ------ UNKNOWN
309.2001 -65.7325 3.7 55.1 -7.5 8.2662 3.1 ------ UNKNOWN
323.8371 -54.8663 4.9 52.0 -23.2 5.0189 2.4 ------ UNKNOWN
329.3638 -38.6414 5.3 47.7 -44.3 8.7157 2.2 ------ UNKNOWN
319.6049 10.3433 3.8 43.1 -116.6 12.3461 3.1 ------ UNKNOWN
Plot creation:
Tue Apr 25 19:10:55 EDT 2017