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
291.0805 24.1397 0.0072 30.9195 -160.9503 6.3875123 26.556 TRIG_00518507
Foreground time interval of the image:
-150.512 12.941 (delta_t = 163.453 [sec])
Background time interval of the image:
-239.360 -150.512 (delta_t = 88.848 [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 -150.512 sec. to 142.456 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.31194 ( -0.0448914 0.0447148 )
Norm@50keV : 3.47520E-03 ( -8.06226e-05 8.04914e-05 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 43.02 using 59 PHA bins.
# Reduced chi-squared = 0.7548 for 57 degrees of freedom
# Null hypothesis probability = 9.147888e-01
Photon flux (15-150 keV) in 293 sec: 0.415526 ( -0.0108781 0.0109392 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.0033e-05 ( -2.35626e-07 2.35864e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -150.512 sec. to 142.456 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.30848 ( -0.0860052 0.0444885 )
Epeak [keV] : 9998.62 ( -9998.86 -9998.86 )
Norm@50keV : 3.48717E-03 ( -7.98385e-05 0.000411803 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 43.08 using 59 PHA bins.
# Reduced chi-squared = 0.7692 for 56 degrees of freedom
# Null hypothesis probability = 8.971925e-01
Photon flux (15-150 keV) in 293 sec: 0.415291 ( -0.010875 0.01091 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.00297e-05 ( -2.31324e-07 2.38912e-07 ) ergs/cm2
Band function
Time interval is from -150.512 sec. to 142.456 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.14927 ( 0.951689 0.951689 )
beta : -1.31509 ( 1.31379 0.0467267 )
Epeak [keV] : 153.198 ( -61.726 -61.726 )
Norm@50keV : 4.47348E-03 ( -0.00107619 0 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 42.99 using 59 PHA bins.
# Reduced chi-squared = 0.7817 for 55 degrees of freedom
# Null hypothesis probability = 8.802162e-01
Photon flux (15-150 keV) in 293 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] : 20.0062 ( )
R^2/D10^2 : 1.77040E-02 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 453.73 using 59 PHA bins.
# Reduced chi-squared = 7.9602 for 57 degrees of freedom
# Null hypothesis probability = 3.584838e-63
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.002e-07 1.934e-08
25- 50 1.994e-06 7.691e-08
50-150 5.916e-06 2.080e-07
15-150 8.310e-06 2.110e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.363 ( )
Norm : 1.77887 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 163.26 using 59 PHA bins.
# Reduced chi-squared = 2.8642 for 57 degrees of freedom
# Null hypothesis probability = 3.469171e-12
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.298e-06 3.560e-08
25- 50 2.497e-06 6.475e-08
50-150 5.476e-06 1.450e-07
15-150 9.270e-06 2.476e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 8.41299 (-0.740828 0.786967)
R1^2/D10^2 : 0.211458 (-0.0535889 0.077546)
kT2 [keV] : 35.4971 (-3.34836 4.46504)
R2^2/D10^2 : 2.26285E-03 (-0.000701767 0.000868501)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 51.25 using 59 PHA bins.
# Reduced chi-squared = 0.9319 for 55 degrees of freedom
# Null hypothesis probability = 6.185389e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.383e-07 7.179e-08
25- 50 2.335e-06 1.065e-07
50-150 6.778e-06 4.410e-07
15-150 1.005e-05 5.230e-07
Peak spectrum fit
Power-law model
Time interval is from 33.676 sec. to 34.676 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.12602 ( -0.0674519 0.0672086 )
Norm@50keV : 4.94254E-02 ( -0.00185366 0.00185263 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 56.78 using 59 PHA bins.
# Reduced chi-squared = 0.9961 for 57 degrees of freedom
# Null hypothesis probability = 4.834575e-01
Photon flux (15-150 keV) in 1 sec: 5.74830 ( -0.223086 0.223381 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.12545e-07 ( -2.1091e-08 2.11346e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 33.676 sec. to 34.676 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.999772 ( -0.262716 0.156489 )
Epeak [keV] : 457.641 ( -457.641 -457.641 )
Norm@50keV : 5.62436E-02 ( -0.0081246 0.0167264 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 56.04 using 59 PHA bins.
# Reduced chi-squared = 1.001 for 56 degrees of freedom
# Null hypothesis probability = 4.733915e-01
Photon flux (15-150 keV) in 1 sec: 5.71442 ( -0.23222 0.23238 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.0998e-07 ( -2.1993e-08 2.1911e-08 ) ergs/cm2
Band function
Time interval is from 33.676 sec. to 34.676 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 0.448062 ( 0.609645 0.609645 )
beta : -1.16216 ( 1.15467 0.0820154 )
Epeak [keV] : 43.5295 ( -43.5181 87.1244 )
Norm@50keV : 0.615063 ( -0.618161 1159.11 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 55.15 using 59 PHA bins.
# Reduced chi-squared = 1.003 for 55 degrees of freedom
# Null hypothesis probability = 4.688705e-01
Photon flux (15-150 keV) in 1 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] : 21.0829 ( )
R^2/D10^2 : 0.227188 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 193.90 using 59 PHA bins.
# Reduced chi-squared = 3.4017 for 57 degrees of freedom
# Null hypothesis probability = 8.117760e-17
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.905e-08 1.505e-09
25- 50 9.814e-08 5.250e-09
50-150 3.252e-07 2.050e-08
15-150 4.424e-07 2.155e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.363 ( )
Norm : 23.7944 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 169.75 using 59 PHA bins.
# Reduced chi-squared = 2.9781 for 57 degrees of freedom
# Null hypothesis probability = 3.879834e-13
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.925e-08 2.450e-09
25- 50 1.140e-07 4.600e-09
50-150 2.500e-07 9.750e-09
15-150 4.232e-07 1.875e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.44933 (-1.01184 1.18998)
R1^2/D10^2 : 3.67541 (-1.39887 2.40083)
kT2 [keV] : 32.3764 (-3.44431 4.84203)
R2^2/D10^2 : 5.01753E-02 (-0.018034 0.0224299)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 53.43 using 59 PHA bins.
# Reduced chi-squared = 0.9715 for 55 degrees of freedom
# Null hypothesis probability = 5.347525e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.263e-08 6.905e-09
25- 50 1.034e-07 1.095e-08
50-150 3.679e-07 3.930e-08
15-150 5.140e-07 4.990e-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: 1.21156 ( -0.0702956 0.0695993 )
Norm@50keV : 2.72419E-03 ( -0.000101795 0.000101505 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 55.93 using 59 PHA bins.
# Reduced chi-squared = 0.9812 for 57 degrees of freedom
# Null hypothesis probability = 5.153578e-01
Photon flux (15-150 keV) in 163.5 sec: 0.320294 ( -0.0129851 0.0130506 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.5042e-06 ( -1.7271e-07 1.73071e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.21003 ( -0.129239 0.0678813 )
Epeak [keV] : 9999.35 ( -9999.36 -9999.36 )
Norm@50keV : 2.73601E-03 ( -0.000101186 0.000499091 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 55.98 using 59 PHA bins.
# Reduced chi-squared = 0.9996 for 56 degrees of freedom
# Null hypothesis probability = 4.757083e-01
Photon flux (15-150 keV) in 163.5 sec: 0.320490 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 4.50292e-06 ( -1.71528e-07 1.73016e-07 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.771790 ( 0.76565 0.76565 )
beta : -1.23059 ( 1.23051 0.0845798 )
Epeak [keV] : 89.9909 ( -86.9871 412.948 )
Norm@50keV : 5.20925E-03 ( -0.0027774 217.727 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 55.59 using 59 PHA bins.
# Reduced chi-squared = 1.011 for 55 degrees of freedom
# Null hypothesis probability = 4.525038e-01
Photon flux (15-150 keV) in 163.5 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) = 2.25e-06
S(50-100 keV) = 3.62e-06
T90 vs. Hardness ratio plot
T90 = 118.423999965191 sec.
Hardness ratio (energy fluence ratio) = 1.60889
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.44023
Count Ratio (50-100 keV) / (15-25 keV) = 1.27397
Mask shadow pattern
IMX = -5.661482109179601E-01, IMY = 1.954902831321166E-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:
-239.360000 -150.512000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
244.9733 -15.6184 0.9 36.3 70.0 3.4218 12.4 1.4 Sco X-1
254.3234 35.4573 0.0 47.2 150.6 0.5794 1.6 9.5 Her X-1
256.1182 -38.0210 23.8 39.7 30.1 0.0945 0.5 12.3 4U 1700-377
256.2779 -36.4100 5.7 38.4 31.6 0.3799 2.0 7.6 GX 349+2
263.1635 -24.7624 8.8 25.8 37.8 0.1597 1.3 8.5 GX 1+4
264.9033 -44.4757 5.9 41.8 16.3 0.3617 2.0 7.0 4U 1735-44
268.4627 -1.4531 4.5 12.4 105.8 0.2727 2.6 5.7 SW J1753.5-0127
270.2334 -25.0068 3.8 22.3 24.5 0.3346 3.0 5.1 GX 5-1
270.1618 -25.6756 3.4 22.9 23.9 0.3928 3.4 8.6 GRS 1758-258
274.0426 -14.0174 3.5 11.0 33.7 0.3182 3.4 2.4 GX 17+2
275.9253 -30.3702 90.0 25.8 8.5 0.0145 0.1 0.2 H1820-303
284.8809 -25.0743 0.0 20.6 -12.0 -0.1887 -1.7 12.5 HT1900.1-2455
288.7706 10.9576 1.0 18.0 -152.5 1.1705 11.6 1.8 GRS 1915+105
299.5331 35.2441 2.6 44.1 -157.6 0.8478 4.5 3.8 Cyg X-1
308.1080 40.8990 7.9 52.4 -153.9 0.4761 1.5 3.2 Cyg X-3
263.1397 -34.0047 0.0 33.1 26.4 0.0029 0.0 12.7 GX 354-0
240.8236 2.2938 2.3 40.1 99.2 2.1314 4.9 ------ UNKNOWN
248.2148 23.6080 2.5 42.4 133.4 1.5431 4.7 ------ UNKNOWN
295.9528 -57.8077 3.0 54.2 -10.4 1.1886 3.9 ------ UNKNOWN
321.7934 -17.9108 3.1 42.5 -69.0 1.7788 3.7 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-150.512000 12.940600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
245.0206 -15.6965 14.9 36.3 69.8 -0.4624 -0.8 4.1 Sco X-1
254.4777 35.3453 40.1 47.1 150.6 0.2060 0.3 1.0 Her X-1
256.1394 -37.9401 29.4 39.7 30.2 -0.1664 -0.4 9.2 4U 1700-377
256.2826 -36.3302 28.7 38.4 31.7 -0.1664 -0.4 9.2 GX 349+2
262.9707 -24.7986 15.5 25.9 38.0 -0.1925 -0.7 3.8 GX 1+4
264.8994 -44.5510 5.2 41.8 16.3 -0.9090 -2.2 9.0 4U 1735-44
268.2725 -1.5874 7.0 12.5 104.9 -0.4070 -1.7 9.9 SW J1753.5-0127
270.2103 -25.2069 5.0 22.5 24.3 0.5450 2.3 8.7 GX 5-1
270.4553 -25.8328 11.6 22.9 23.1 0.2393 1.0 9.9 GRS 1758-258
274.0738 -14.0665 5.0 11.0 33.4 -0.4660 -2.3 4.4 GX 17+2
275.8618 -30.3752 6.3 25.8 8.6 0.4313 1.8 3.3 H1820-303
284.8807 -25.0088 13.1 20.5 -12.1 0.1908 0.9 10.0 HT1900.1-2455
288.9454 10.9301 4.6 18.0 -152.0 0.5219 2.5 8.7 GRS 1915+105
299.4676 35.3569 21.0 44.1 -157.7 -0.2046 -0.5 11.1 Cyg X-1
308.2552 40.8744 10.9 52.5 -153.8 0.6997 1.1 8.1 Cyg X-3
262.9261 -33.8948 6.2 33.2 26.7 0.5879 1.9 4.8 GX 354-0
268.6866 10.5636 2.7 19.4 143.0 0.9835 4.3 ------ UNKNOWN
291.0805 24.1397 0.4 30.9 -161.0 6.3873 26.6 ------ UNKNOWN
294.7805 22.0183 2.9 30.5 -153.1 1.0227 4.1 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
64.140600 962.708300
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.2574 35.4271 0.0 33.7 112.6 2.7306 2.5 11.0 Her X-1
268.4002 -1.5016 2.3 33.8 38.3 3.7103 5.0 3.5 SW J1753.5-0127
270.3718 -25.0095 11.9 53.1 18.0 -2.2767 -1.0 6.3 GX 5-1
270.3762 -25.8753 7.8 53.9 17.6 -3.7970 -1.5 8.9 GRS 1758-258
274.1268 -14.0453 9.2 41.6 19.6 1.0660 1.3 7.1 GX 17+2
284.9972 -24.9469 6.3 49.4 1.7 2.0887 1.8 2.6 HT1900.1-2455
288.7989 10.9507 0.4 13.4 4.1 13.1608 27.6 0.3 GRS 1915+105
299.5883 35.1856 0.8 13.3 -153.8 7.6623 15.0 1.0 Cyg X-1
308.0594 40.9752 0.9 22.0 -149.5 6.8604 12.6 2.7 Cyg X-3
326.2855 38.2882 4.4 33.0 -129.4 2.1225 2.6 5.7 Cyg X-2
294.0893 67.2733 3.9 43.2 176.1 2.4329 3.0 ------ UNKNOWN
339.6305 35.5755 3.2 43.2 -122.6 6.8748 3.7 ------ UNKNOWN
350.2008 47.9459 4.3 51.9 -138.6 8.7541 2.7 ------ UNKNOWN
321.5707 -16.9112 3.8 50.7 -44.5 9.1874 3.1 ------ UNKNOWN
345.4847 40.2226 2.6 48.0 -128.9 10.8574 4.4 ------ UNKNOWN
Plot creation:
Sat May 30 19:58:03 EDT 2015