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
255.5751 -35.5898 0.0046 17.1329 26.9289 2.7723581 42.129 TRIG_00421124
Foreground time interval of the image:
-9.696 11.621 (delta_t = 21.317 [sec])
Background time interval of the image:
-239.280 -9.696 (delta_t = 229.584 [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)
The mask-weighted light curves based on cleaned DPHs
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 -9.696 sec. to 102.456 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.76457 ( -0.099807 0.100956 )
Norm@50keV : 2.26516E-03 ( -0.00012369 0.000122726 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 61.45 using 59 PHA bins.
# Reduced chi-squared = 1.078 for 57 degrees of freedom
# Null hypothesis probability = 3.196740e-01
Photon flux (15-150 keV) in 112.2 sec: 0.307951 ( -0.0158636 0.0159208 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.34331e-06 ( -1.32236e-07 1.33446e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -9.696 sec. to 102.456 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.68097 ( -0.402493 0.354856 )
Epeak [keV] : 177.532 ( -117.267 -180.62 )
Norm@50keV : 2.50580E-03 ( -0.000552329 0.00152109 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 61.31 using 59 PHA bins.
# Reduced chi-squared = 1.095 for 56 degrees of freedom
# Null hypothesis probability = 2.912790e-01
Photon flux (15-150 keV) in 112.2 sec: 0.306101 ( -0.017814 0.017141 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.32223e-06 ( -1.65517e-07 1.51335e-07 ) ergs/cm2
Band function
Time interval is from -9.696 sec. to 102.456 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.49143 ( 1.44702 1.44702 )
beta : -1.81656 ( 1.81656 0.147362 )
Epeak [keV] : 68.6085 ( -63.9804 213.2 )
Norm@50keV : 3.30427E-03 ( -0.000938278 0 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 61.20 using 59 PHA bins.
# Reduced chi-squared = 1.113 for 55 degrees of freedom
# Null hypothesis probability = 2.632434e-01
Photon flux (15-150 keV) in 112.2 sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 2.31582e-06 ( 0 0 ) ergs/cm2
Single BB
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 12.4419 ( )
R^2/D10^2 : 6.11789E-02 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 151.50 using 59 PHA bins.
# Reduced chi-squared = 2.6579 for 57 degrees of freedom
# Null hypothesis probability = 1.651317e-10
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.252e-07 2.244e-08
25- 50 7.391e-07 4.813e-08
50-150 7.042e-07 8.123e-08
15-150 1.669e-06 1.010e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 119.283 (-26.4499 32.6912)
Norm : 1.27966 (-0.0845355 0.112099)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 64.02 using 59 PHA bins.
# Reduced chi-squared = 1.123 for 57 degrees of freedom
# Null hypothesis probability = 2.438217e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.741e-07 3.276e-08
25- 50 6.685e-07 4.886e-08
50-150 1.189e-06 3.437e-07
15-150 2.232e-06 3.882e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.91205 (-1.06196 1.25592)
R1^2/D10^2 : 0.655575 (-0.318362 0.75287)
kT2 [keV] : 21.7695 (-3.53441 5.97377)
R2^2/D10^2 : 6.30323E-03 (-0.00367285 0.00611225)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 66.54 using 59 PHA bins.
# Reduced chi-squared = 1.210 for 55 degrees of freedom
# Null hypothesis probability = 1.368554e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.967e-07 8.555e-08
25- 50 6.503e-07 1.043e-07
50-150 1.187e-06 2.380e-07
15-150 2.234e-06 3.871e-07
Peak spectrum fit
Power-law model
Time interval is from 7.592 sec. to 8.592 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.62784 ( -0.189009 0.194116 )
Norm@50keV : 1.29382E-02 ( -0.00146084 0.0014387 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 52.34 using 59 PHA bins.
# Reduced chi-squared = 0.9182 for 57 degrees of freedom
# Null hypothesis probability = 6.502567e-01
Photon flux (15-150 keV) in 1 sec: 1.67727 ( -0.173468 0.173692 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.2061e-07 ( -1.45727e-08 1.48248e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 7.592 sec. to 8.592 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.34748 ( -0.830974 0.73298 )
Epeak [keV] : 110.930 ( -58.7406 -110.93 )
Norm@50keV : 1.81441E-02 ( -0.00652521 0.0302433 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 51.91 using 59 PHA bins.
# Reduced chi-squared = 0.9269 for 56 degrees of freedom
# Null hypothesis probability = 6.304557e-01
Photon flux (15-150 keV) in 1 sec: 1.65313 ( -0.18475 0.09176 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.17497e-07 ( -1.6631e-08 1.6713e-08 ) ergs/cm2
Band function
Time interval is from 7.592 sec. to 8.592 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.32929 ( 1.32931 1.32931 )
beta : -1.92892 ( 1.93272 0.478177 )
Epeak [keV] : 105.373 ( -105.37 -105.37 )
Norm@50keV : 1.85980E-02 ( -0.00698097 0.232918 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 51.91 using 59 PHA bins.
# Reduced chi-squared = 0.9438 for 55 degrees of freedom
# Null hypothesis probability = 5.935430e-01
Photon flux (15-150 keV) in 1 sec: 1.65312 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 1.17442e-07 ( 0 0 ) ergs/cm2
Single BB
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 13.6378 (-1.74615 2.01091)
R^2/D10^2 : 0.255904 (-0.0985519 0.161011)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 72.15 using 59 PHA bins.
# Reduced chi-squared = 1.266 for 57 degrees of freedom
# Null hypothesis probability = 8.519756e-02
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.007e-08 2.040e-09
25- 50 3.649e-08 4.960e-09
50-150 4.408e-08 1.038e-08
15-150 9.065e-08 1.336e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 166.676 (-69.3375 -165.587)
Norm : 6.84491 (-0.73909 0.951461)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 51.99 using 59 PHA bins.
# Reduced chi-squared = 0.9120 for 57 degrees of freedom
# Null hypothesis probability = 6.631984e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.741e-08 9.078e-09
25- 50 3.274e-08 1.742e-08
50-150 6.739e-08 3.769e-08
15-150 1.175e-07 6.384e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.02923 (-1.77652 2.41065)
R1^2/D10^2 : 5.63494 (-4.25748 34.4183)
kT2 [keV] : 19.7155 (-3.9951 7.94903)
R2^2/D10^2 : 5.83466E-02 (-0.0421733 0.0801303)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 51.91 using 59 PHA bins.
# Reduced chi-squared = 0.9438 for 55 degrees of freedom
# Null hypothesis probability = 5.933750e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.842e-08 9.429e-09
25- 50 3.099e-08 1.057e-08
50-150 6.276e-08 3.220e-08
15-150 1.122e-07 4.246e-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: 1.49024 ( -0.0683104 0.068411 )
Norm@50keV : 8.37162E-03 ( -0.000308372 0.000308095 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 68.27 using 59 PHA bins.
# Reduced chi-squared = 1.198 for 57 degrees of freedom
# Null hypothesis probability = 1.458073e-01
Photon flux (15-150 keV) in 21.32 sec: 1.04239 ( -0.0398994 0.0399849 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.69591e-06 ( -6.816e-08 6.84453e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.946417 ( -0.308848 0.288028 )
Epeak [keV] : 98.9368 ( -18.8887 52.8066 )
Norm@50keV : 1.53963E-02 ( -0.00415497 0.0061909 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 57.27 using 59 PHA bins.
# Reduced chi-squared = 1.023 for 56 degrees of freedom
# Null hypothesis probability = 4.278578e-01
Photon flux (15-150 keV) in 21.32 sec: 1.00457 ( -0.044146 0.04421 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.6163e-06 ( -7.9918e-08 7.99713e-08 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.878771 ( -0.337695 2.20264 )
beta : -1.96334 ( 1.9685 0.38777 )
Epeak [keV] : 90.8821 ( -55.4558 55.1886 )
Norm@50keV : 1.68223E-02 ( -0.00533332 0.412622 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 56.99 using 59 PHA bins.
# Reduced chi-squared = 1.036 for 55 degrees of freedom
# Null hypothesis probability = 4.009473e-01
Photon flux (15-150 keV) in 21.32 sec: 1.00284 ( 5.99716 -0.044202 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.61619e-06 ( -1.61604e-06 -8.08604e-08 ) ergs/cm2
S(25-50 keV) vs. S(50-100 keV) plot
S(25-50 keV) = 6.51e-07
S(50-100 keV) = 7.66e-07
T90 vs. Hardness ratio plot
T90 = 97.0039999485016 sec.
Hardness ratio (energy fluence ratio) = 1.17665
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.08235
Count Ratio (50-100 keV) / (15-25 keV) = 0.670346
Mask shadow pattern
IMX = 2.748437865463495E-01, IMY = -1.396105504656576E-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:
-239.280000 -9.696000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
244.9933 -15.6436 0.3 22.8 93.2 11.7165 35.4 0.8 Sco X-1
255.7643 -37.9460 0.0 18.8 21.6 -0.3333 -1.4 12.2 4U 1700-377
256.3834 -36.3820 4.5 17.3 23.5 0.5930 2.5 3.5 GX 349+2
263.0460 -24.5998 4.9 5.1 53.5 0.5690 2.3 9.0 GX 1+4
264.8135 -44.5130 5.6 22.3 -3.7 0.5106 2.1 4.8 4U 1735-44
268.2993 -1.3757 4.6 21.0 170.7 0.6578 2.5 6.2 SW J1753.5-0127
270.2926 -25.0709 2.0 3.4 -46.1 1.5143 5.9 0.7 GX 5-1
270.3500 -25.7121 5.0 3.9 -41.0 0.6140 2.5 3.2 GRS 1758-258
273.9277 -14.0219 2.3 10.0 -155.3 1.2691 5.0 4.6 GX 17+2
275.9713 -30.3656 6.6 10.7 -49.6 0.4474 1.7 2.4 H1820-303
285.1943 -24.8207 99.3 15.8 -87.6 -0.0326 -0.1 10.5 HT1900.1-2455
288.7775 10.9326 1.6 39.0 -156.4 2.9930 7.2 1.5 GRS 1915+105
263.1669 -33.8451 11.1 12.3 9.8 0.2728 1.0 8.9 GX 354-0
247.8931 9.0422 2.7 37.1 135.8 2.4116 4.3 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-9.696000 11.620600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
244.8241 -15.6812 337.0 23.0 93.0 0.0030 0.0 9.3 Sco X-1
256.1814 -37.8226 759.5 18.5 21.0 -0.0010 -0.0 9.3 4U 1700-377
256.4363 -36.4225 8.8 17.3 23.3 -0.0879 -1.3 0.1 GX 349+2
263.0439 -24.9052 5.2 5.3 50.5 -0.1396 -2.2 9.8 GX 1+4
264.9770 -44.3307 0.0 22.1 -3.9 -0.1643 -2.5 12.3 4U 1735-44
268.5053 -1.4825 3.1 20.9 171.3 -0.2499 -3.7 8.4 SW J1753.5-0127
270.0946 -25.2038 0.0 3.4 -42.3 -0.0309 -0.5 12.7 GX 5-1
270.1427 -25.6946 189.3 3.8 -38.8 -0.0044 -0.1 9.1 GRS 1758-258
273.9503 -14.1797 28.6 9.9 -154.7 0.0254 0.4 9.2 GX 17+2
276.1170 -30.2347 0.0 10.6 -50.6 0.1837 2.9 12.7 H1820-303
284.8759 -24.8307 6.2 15.6 -87.4 0.1272 1.9 10.2 HT1900.1-2455
288.9034 10.8299 4.9 39.0 -156.1 0.2157 2.3 9.3 GRS 1915+105
263.1241 -34.0129 0.0 12.4 9.7 0.0569 0.9 12.6 GX 354-0
257.8187 -17.8130 2.5 10.7 103.6 0.3064 4.6 ------ UNKNOWN
255.5751 -35.5836 0.3 17.1 26.9 2.6174 39.4 ------ UNKNOWN
279.1321 -0.2602 2.5 24.6 -162.4 0.2855 4.6 ------ UNKNOWN
275.6320 -45.5400 2.4 24.0 -22.9 0.3156 4.9 ------ UNKNOWN
288.7680 -75.1575 2.3 53.9 -16.3 1.0160 5.0 ------ UNKNOWN
297.0118 -45.7265 2.6 33.1 -48.0 0.3930 4.4 ------ UNKNOWN
311.2707 -18.0784 3.2 40.6 -97.8 0.9273 3.7 ------ UNKNOWN
308.9176 2.6116 2.0 47.0 -126.6 1.7078 5.8 ------ UNKNOWN
UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
51.620600 962.796300
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
186.5759 -62.6769 9.7 49.4 10.5 2.0176 1.2 6.0 GX 301-2
244.9746 -15.6433 0.2 22.1 128.0 48.8597 56.2 0.3 Sco X-1
255.7361 -37.9210 0.0 2.3 -27.2 0.1580 0.2 12.7 4U 1700-377
256.3852 -36.4082 2.5 1.0 -63.1 3.5228 4.6 2.6 GX 349+2
263.2163 -24.6555 0.0 12.8 -170.8 0.9107 1.1 12.5 GX 1+4
264.9883 -44.3961 3.6 11.4 -60.3 2.3033 3.2 11.0 4U 1735-44
268.4398 -1.6094 8.9 36.0 178.3 1.1999 1.3 10.3 SW J1753.5-0127
270.3240 -25.0406 1.4 16.5 -149.6 6.1061 8.2 3.2 GX 5-1
270.4253 -25.6259 4.4 16.2 -147.9 2.1069 2.8 9.7 GRS 1758-258
273.9717 -14.0402 3.4 27.2 -161.8 2.8296 3.4 2.0 GX 17+2
276.0499 -30.2906 3.0 18.0 -125.3 3.3166 3.9 7.9 H1820-303
285.1096 -25.0779 8.9 27.4 -128.3 -1.2856 -1.3 10.3 HT1900.1-2455
288.7733 10.9529 9.5 56.1 -163.6 3.6669 1.2 1.5 GRS 1915+105
262.8514 -33.9522 9.8 6.2 -127.3 0.9118 1.2 9.8 GX 354-0
209.1114 -26.2950 2.5 40.5 66.0 15.1241 4.6 ------ UNKNOWN
155.3460 -82.0129 4.3 56.2 -14.4 8.3983 2.7 ------ UNKNOWN
326.4229 -73.1430 3.7 50.6 -44.7 15.4038 3.2 ------ UNKNOWN
306.7153 -35.3697 4.4 41.2 -98.7 12.7949 2.7 ------ UNKNOWN
Plot creation:
Sun May 31 01:40:47 EDT 2015