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
219.1205 -67.4058 0.0043 24.5428 88.2863 6.1487488 44.910 TRIG_00155284
Foreground time interval of the image:
-4.499 56.916 (delta_t = 61.415 [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 64.000000
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 64.000000
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 64.000000
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 -9.124 sec. to 56.916 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.88667 ( -0.0615787 0.0620983 )
Norm@50keV : 5.86294E-03 ( -0.000198396 0.000197766 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 73.62 using 59 PHA bins.
# Reduced chi-squared = 1.292 for 57 degrees of freedom
# Null hypothesis probability = 6.841046e-02
Photon flux (15-150 keV) in 66.04 sec: 0.836672 ( -0.0292371 0.0293432 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.55943e-06 ( -1.19909e-07 1.20184e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -9.124 sec. to 56.916 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.37401 ( -0.281655 0.26462 )
Epeak [keV] : 59.4409 ( -7.26838 14.634 )
Norm@50keV : 1.06394E-02 ( -0.00275936 0.00404717 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 62.11 using 59 PHA bins.
# Reduced chi-squared = 1.109 for 56 degrees of freedom
# Null hypothesis probability = 2.676335e-01
Photon flux (15-150 keV) in 66.04 sec: 0.804889 ( -0.032877 0.033031 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.40492e-06 ( -1.42422e-07 1.42739e-07 ) ergs/cm2
Band function
Time interval is from -9.124 sec. to 56.916 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.28389 ( -0.322706 1.05454 )
beta : -2.31445 ( 2.31445 0.330983 )
Epeak [keV] : 55.7993 ( -18.5001 15.3747 )
Norm@50keV : 1.19901E-02 ( -0.00382089 0.0459198 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 61.48 using 59 PHA bins.
# Reduced chi-squared = 1.118 for 55 degrees of freedom
# Null hypothesis probability = 2.552933e-01
Photon flux (15-150 keV) in 66.04 sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 3.40438e-06 ( 0 0 ) ergs/cm2
Single BB
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 12.4948 ( )
R^2/D10^2 : 0.161615 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 229.53 using 59 PHA bins.
# Reduced chi-squared = 4.0268 for 57 degrees of freedom
# Null hypothesis probability = 1.451501e-22
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.533e-07 2.196e-08
25- 50 1.165e-06 4.326e-08
50-150 1.122e-06 7.859e-08
15-150 2.640e-06 9.279e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 92.0521 (-10.127 12.2742)
Norm : 3.68697 (-0.191763 0.205453)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 62.23 using 59 PHA bins.
# Reduced chi-squared = 1.092 for 57 degrees of freedom
# Null hypothesis probability = 2.955607e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.357e-07 3.801e-08
25- 50 1.080e-06 3.995e-08
50-150 1.668e-06 3.992e-07
15-150 3.384e-06 3.906e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.74202 (-0.869278 0.912748)
R1^2/D10^2 : 1.07296 (-0.366797 0.67373)
kT2 [keV] : 21.2977 (-2.51981 3.59898)
R2^2/D10^2 : 1.57622E-02 (-0.00741607 0.0110409)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 69.82 using 59 PHA bins.
# Reduced chi-squared = 1.269 for 55 degrees of freedom
# Null hypothesis probability = 8.609582e-02
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.855e-07 6.994e-08
25- 50 1.092e-06 7.826e-08
50-150 1.647e-06 2.027e-07
15-150 3.324e-06 2.724e-07
Peak spectrum fit
Power-law model
Time interval is from -3.076 sec. to -2.076 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.59700 ( -0.15216 0.154924 )
Norm@50keV : 1.78329E-02 ( -0.00162712 0.00161383 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 44.92 using 59 PHA bins.
# Reduced chi-squared = 0.7881 for 57 degrees of freedom
# Null hypothesis probability = 8.767827e-01
Photon flux (15-150 keV) in 1 sec: 2.28945 ( -0.201653 0.201969 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.66837e-07 ( -1.63371e-08 1.64788e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -3.076 sec. to -2.076 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.35250 ( -0.647505 0.376383 )
Epeak [keV] : 130.512 ( -63.8667 -130.513 )
Norm@50keV : 2.38185E-02 ( -0.0146976 0.0267323 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 44.40 using 59 PHA bins.
# Reduced chi-squared = 0.7929 for 56 degrees of freedom
# Null hypothesis probability = 8.682127e-01
Photon flux (15-150 keV) in 1 sec: 2.26491 ( -0.21008 0.20918 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.63875e-07 ( -1.8076e-08 1.7717e-08 ) ergs/cm2
Band function
Time interval is from -3.076 sec. to -2.076 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.08651 ( 1.09245 1.09245 )
beta : -1.74678 ( 1.75655 0.290527 )
Epeak [keV] : 74.0264 ( -76.8436 -76.8436 )
Norm@50keV : 3.47070E-02 ( -0.0168064 0 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 44.22 using 59 PHA bins.
# Reduced chi-squared = 0.8039 for 55 degrees of freedom
# Null hypothesis probability = 8.507343e-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] : 13.5869 (-1.46728 1.70398)
R^2/D10^2 : 0.358229 (-0.123707 0.182512)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 74.96 using 59 PHA bins.
# Reduced chi-squared = 1.315 for 57 degrees of freedom
# Null hypothesis probability = 5.557140e-02
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.400e-08 2.345e-09
25- 50 5.052e-08 5.525e-09
50-150 6.045e-08 1.132e-08
15-150 1.250e-07 1.405e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 179.088 (-63.1556 -179.143)
Norm : 9.34259 (-0.853595 0.971623)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 44.46 using 59 PHA bins.
# Reduced chi-squared = 0.7799 for 57 degrees of freedom
# Null hypothesis probability = 8.869255e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.357e-08 7.395e-09
25- 50 4.476e-08 1.754e-08
50-150 9.460e-08 5.082e-08
15-150 1.629e-07 6.437e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.95324 (-2.48997 2.2091)
R1^2/D10^2 : 1.67104 (-0.877305 2.46828)
kT2 [keV] : 29.3785 (-9.27018 26.8353)
R2^2/D10^2 : 1.69672E-02 (-0.0145828 0.0549183)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 46.69 using 59 PHA bins.
# Reduced chi-squared = 0.8490 for 55 degrees of freedom
# Null hypothesis probability = 7.797143e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.135e-08 7.209e-09
25- 50 4.716e-08 1.464e-08
50-150 9.569e-08 4.626e-08
15-150 1.642e-07 6.523e-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: 1.88495 ( -0.0620958 0.0626191 )
Norm@50keV : 6.02273E-03 ( -0.00020583 0.00020516 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 75.10 using 59 PHA bins.
# Reduced chi-squared = 1.318 for 57 degrees of freedom
# Null hypothesis probability = 5.430678e-02
Photon flux (15-150 keV) in 61.42 sec: 0.858855 ( -0.0302372 0.0303509 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.40062e-06 ( -1.15739e-07 1.16022e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.39738 ( -0.282534 0.265255 )
Epeak [keV] : 59.9827 ( -7.70075 16.7217 )
Norm@50keV : 1.06345E-02 ( -0.00277086 0.00407612 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 64.80 using 59 PHA bins.
# Reduced chi-squared = 1.157 for 56 degrees of freedom
# Null hypothesis probability = 1.965977e-01
Photon flux (15-150 keV) in 61.42 sec: 0.828124 ( -0.033927 0.034155 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.25903e-06 ( -1.37734e-07 1.37925e-07 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.13244 ( -0.469628 1.15781 )
beta : -2.16070 ( 2.16053 0.200391 )
Epeak [keV] : 50.0493 ( -14.684 20.6277 )
Norm@50keV : 1.53697E-02 ( -0.0069503 0.0748259 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 63.67 using 59 PHA bins.
# Reduced chi-squared = 1.158 for 55 degrees of freedom
# Null hypothesis probability = 1.978496e-01
Photon flux (15-150 keV) in 61.42 sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 3.26647e-06 ( -3.26604e-06 -1.38201e-07 ) ergs/cm2
S(25-50 keV) vs. S(50-100 keV) plot
S(25-50 keV) = 1.03e-06
S(50-100 keV) = 1.12e-06
T90 vs. Hardness ratio plot
T90 = 43.0960000157356 sec.
Hardness ratio (energy fluence ratio) = 1.08738
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.16755
Count Ratio (50-100 keV) / (15-25 keV) = 0.67041
Mask shadow pattern
IMX = 1.365583999024523E-02, IMY = -4.564246376089915E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 64.000000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 64.000000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 64.000000
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:
-4.499400 56.916000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.3739 -40.4191 0.0 36.9 -158.9 -0.0409 -0.3 10.8 Vela X-1
170.2887 -60.6877 49.7 15.1 150.4 0.0217 0.2 4.0 Cen X-3
186.6179 -62.7758 0.8 13.9 118.5 1.2732 14.5 1.1 GX 301-2
219.1197 -67.4057 0.3 24.5 88.3 6.1477 44.9 ------ UNKNOWN
229.2329 -46.5561 2.7 28.1 39.2 0.4929 4.3 ------ UNKNOWN
234.0319 -10.7076 2.6 54.5 -0.3 1.5517 4.5 ------ UNKNOWN
138.0279 -18.6523 2.4 49.5 -132.4 2.1433 4.9 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
120.100600 303.110400
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.3124 -40.5473 25.9 50.8 -146.0 0.2071 0.4 9.9 Vela X-1
170.1575 -60.4847 6.9 21.9 -138.6 0.2508 1.7 9.5 Cen X-3
186.6683 -62.7635 0.5 14.2 -129.6 3.3581 24.2 0.5 GX 301-2
244.9972 -15.6400 1.3 54.4 -11.9 4.2413 9.2 1.0 Sco X-1
255.8251 -37.8619 6.3 35.9 10.5 -0.3428 -1.8 7.7 4U 1700-377
256.5857 -36.4286 7.5 37.5 10.5 0.3080 1.5 7.3 GX 349+2
262.9038 -24.6680 15.0 50.4 11.7 0.3212 0.8 7.4 GX 1+4
264.7262 -44.4876 4.4 33.0 26.4 0.4890 2.6 2.4 4U 1735-44
270.3951 -25.0750 16.7 52.5 20.0 0.4419 0.7 6.0 GX 5-1
270.2468 -25.7033 9.0 51.9 20.1 0.7645 1.3 3.8 GRS 1758-258
275.9226 -30.2384 10.7 49.7 28.4 0.6425 1.1 7.7 H1820-303
263.0707 -33.7577 2.8 42.0 16.5 1.0088 4.2 6.2 GX 354-0
253.4647 -39.8573 1.9 33.4 8.9 1.1048 6.0 ------ UNKNOWN
96.5255 -50.9032 2.8 54.1 177.9 2.1008 4.1 ------ UNKNOWN
98.4139 -47.3433 3.5 56.9 -179.0 2.6827 3.3 ------ UNKNOWN
163.7184 -36.0127 3.0 44.0 -116.5 2.3837 3.9 ------ UNKNOWN
Plot creation:
Sun May 31 15:38:25 EDT 2015