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
57.7255 27.0168 0.0067 44.1510 178.6306 3.1474948 28.979 TRIG_00180977
Foreground time interval of the image:
-21.115 15.485 (delta_t = 36.600 [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 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)
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 -235.816 sec. to 132.184 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.48280 ( -0.0904218 0.0903864 )
Norm@50keV : 2.19363E-03 ( -0.000111705 0.000111694 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 59.70 using 59 PHA bins.
# Reduced chi-squared = 1.047 for 57 degrees of freedom
# Null hypothesis probability = 3.779412e-01
Photon flux (15-150 keV) in 368 sec: 0.272604 ( -0.0150885 0.0151405 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.68005e-06 ( -4.11744e-07 4.12502e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -235.816 sec. to 132.184 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.18599 ( -0.38423 0.331217 )
Epeak [keV] : 150.080 ( -58.6749 -150.08 )
Norm@50keV : 3.01663E-03 ( -0.000872135 0.00148979 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 57.69 using 59 PHA bins.
# Reduced chi-squared = 1.030 for 56 degrees of freedom
# Null hypothesis probability = 4.126975e-01
Photon flux (15-150 keV) in 368 sec: 0.268027 ( -0.01597 0.016049 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.56656e-06 ( -4.39686e-07 4.37258e-07 ) ergs/cm2
Band function
Time interval is from -235.816 sec. to 132.184 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.788969 ( 0.85747 4.17533 )
beta : -1.61040 ( 1.60867 0.160365 )
Epeak [keV] : 73.5050 ( -73.9129 585.321 )
Norm@50keV : 5.26574E-03 ( -0.00317774 0 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 57.35 using 59 PHA bins.
# Reduced chi-squared = 1.043 for 55 degrees of freedom
# Null hypothesis probability = 3.879357e-01
Photon flux (15-150 keV) in 368 sec: 0.266164 ( ) 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] : 16.7705 ( )
R^2/D10^2 : 2.08290E-02 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 137.27 using 59 PHA bins.
# Reduced chi-squared = 2.4083 for 57 degrees of freedom
# Null hypothesis probability = 1.426660e-08
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.407e-07 4.508e-08
25- 50 1.929e-06 1.417e-07
50-150 3.856e-06 3.338e-07
15-150 6.225e-06 3.882e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 ( )
Norm : 1.12741 (-0.0574183 0.0574146)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 60.98 using 59 PHA bins.
# Reduced chi-squared = 1.070 for 57 degrees of freedom
# Null hypothesis probability = 3.347932e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.033e-06 6.017e-08
25- 50 1.987e-06 1.205e-07
50-150 4.359e-06 3.183e-07
15-150 7.380e-06 4.416e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 8.25404 (-1.43676 1.53226)
R1^2/D10^2 : 0.156030 (-0.0639172 0.135105)
kT2 [keV] : 29.9424 (-5.15728 8.98199)
R2^2/D10^2 : 2.13801E-03 (-0.00126343 0.00216767)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 59.45 using 59 PHA bins.
# Reduced chi-squared = 1.081 for 55 degrees of freedom
# Null hypothesis probability = 3.167817e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.338e-07 1.754e-07
25- 50 2.017e-06 3.091e-07
50-150 4.705e-06 1.292e-06
15-150 7.555e-06 1.419e-06
Peak spectrum fit
Power-law model
Time interval is from -36.316 sec. to -35.316 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.900204 ( -0.457586 0.401352 )
Norm@50keV : 1.04834E-02 ( -0.00276643 0.00259711 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 56.70 using 59 PHA bins.
# Reduced chi-squared = 0.9947 for 57 degrees of freedom
# Null hypothesis probability = 4.863158e-01
Photon flux (15-150 keV) in 1 sec: 1.20321 ( -0.30323 0.309493 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.17644e-07 ( -2.59651e-08 2.59934e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -36.316 sec. to -35.316 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.903490 ( -0.881013 0.396792 )
Epeak [keV] : 9999.16 ( -9999.35 -9999.35 )
Norm@50keV : 1.05754E-02 ( -0.00256284 0.0317052 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 56.70 using 59 PHA bins.
# Reduced chi-squared = 1.013 for 56 degrees of freedom
# Null hypothesis probability = 4.485585e-01
Photon flux (15-150 keV) in 1 sec: 1.20730 ( -0.308407 0.30434 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.17587e-07 ( -2.56983e-08 2.6025e-08 ) ergs/cm2
Band function
Time interval is from -36.316 sec. to -35.316 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.769936 ( 0.769936 0.769936 )
beta : -0.900222 ( -0.401426 0.457296 )
Epeak [keV] : 33.5848 ( -33.5848 -33.5848 )
Norm@50keV : 1.68515E-02 ( -0.00871308 32210.4 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 56.70 using 59 PHA bins.
# Reduced chi-squared = 1.031 for 55 degrees of freedom
# Null hypothesis probability = 4.114399e-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] : 28.2937 (-7.68032 14.2676)
R^2/D10^2 : 2.02698E-02 (-0.0140894 0.0348369)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 60.53 using 59 PHA bins.
# Reduced chi-squared = 1.062 for 57 degrees of freedom
# Null hypothesis probability = 3.498222e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.630e-09 1.364e-09
25- 50 1.582e-08 6.603e-09
50-150 9.133e-08 4.219e-08
15-150 1.098e-07 4.888e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 ( )
Norm : 5.32034 (-1.25665 1.25622)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 64.81 using 59 PHA bins.
# Reduced chi-squared = 1.137 for 57 degrees of freedom
# Null hypothesis probability = 2.229869e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.326e-08 7.955e-09
25- 50 2.551e-08 1.491e-08
50-150 5.595e-08 3.344e-08
15-150 9.473e-08 5.510e-08
Double BB
R1^2/D10^2 : 1.57577E+08 ( )
kT2 [keV] : 29.2856 (-8.32065 15.6388)
R2^2/D10^2 : 1.80890E-02 (-0.0118027 0.0189885)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 56.79 using 59 PHA bins.
#Fit statistic : Chi-Squared = 56.19 using 59 PHA bins.
#Fit statistic : Chi-Squared = 55.88 using 59 PHA bins.
# Reduced chi-squared = 1.032 for 55 degrees of freedom
# Reduced chi-squared = 1.022 for 55 degrees of freedom
# Reduced chi-squared = 1.016 for 55 degrees of freedom
# Null hypothesis probability = 4.082479e-01
# Null hypothesis probability = 4.300562e-01
# Null hypothesis probability = 4.415828e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.364e-09 4.754e-09
25- 50 2.114e-08 1.166e-08
50-150 9.120e-08 5.035e-08
15-150 1.197e-07 6.120e-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: 1.55718 ( -0.0926954 0.0929215 )
Norm@50keV : 6.04973E-03 ( -0.000316263 0.000315816 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 58.75 using 59 PHA bins.
# Reduced chi-squared = 1.031 for 57 degrees of freedom
# Null hypothesis probability = 4.112053e-01
Photon flux (15-150 keV) in 36.6 sec: 0.767459 ( -0.0427601 0.0428773 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.08236e-06 ( -1.15069e-07 1.15341e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.44008 ( -0.362095 0.198434 )
Epeak [keV] : 254.146 ( -254.146 -254.146 )
Norm@50keV : 6.88768E-03 ( -0.00111582 0.00327823 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 58.41 using 59 PHA bins.
# Reduced chi-squared = 1.043 for 56 degrees of freedom
# Null hypothesis probability = 3.870210e-01
Photon flux (15-150 keV) in 36.6 sec: 0.762556 ( -0.044888 0.044822 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.06965e-06 ( -1.2239e-07 1.21549e-07 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 4.94482 ( -4.94482 -4.94482 )
beta : -1.58366 ( -0.099154 0.0975176 )
Epeak [keV] : 21.7717 ( -21.7717 4.12943 )
Norm@50keV : 1420.42 ( -73.5652 2.96171e+06 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 57.39 using 59 PHA bins.
# Reduced chi-squared = 1.044 for 55 degrees of freedom
# Null hypothesis probability = 3.865097e-01
Photon flux (15-150 keV) in 36.6 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) = 1.88e-06
S(50-100 keV) = 2.70e-06
T90 vs. Hardness ratio plot
T90 = 288 sec.
Hardness ratio (energy fluence ratio) = 1.43617
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.57841
Count Ratio (50-100 keV) / (15-25 keV) = 1.28409
Mask shadow pattern
IMX = -9.705164329411058E-01, IMY = -2.319986671718222E-02
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:
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-21.115400 15.484620
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6244 22.0007 1.8 47.9 145.4 1.6389 6.5 1.0 Crab
94.9767 34.5735 2.3 36.5 128.4 0.6465 5.0 ------ UNKNOWN
160.9559 62.5085 2.4 31.9 33.9 0.4132 4.8 ------ UNKNOWN
57.7255 27.0168 0.4 44.2 178.6 3.1475 29.0 ------ UNKNOWN
50.0710 52.2664 2.5 21.4 -156.9 0.2614 4.6 ------ UNKNOWN
33.2657 78.2816 2.4 14.2 -61.3 0.2959 4.7 ------ UNKNOWN
283.9887 58.1034 2.2 50.7 -44.4 1.6611 5.2 ------ UNKNOWN
3.7843 44.6888 3.0 43.1 -112.1 1.0147 3.9 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
81.084590 302.238700
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6363 22.0115 0.3 24.1 107.6 10.1075 44.4 0.2 Crab
75.9270 10.7949 2.1 23.6 141.2 1.0297 5.4 ------ UNKNOWN
57.7543 27.0121 1.3 0.0 131.9 1.5268 9.2 ------ UNKNOWN
54.3375 -11.7511 2.5 38.9 -163.5 1.1749 4.7 ------ UNKNOWN
354.4429 66.1135 3.0 54.7 -15.1 2.0799 3.8 ------ UNKNOWN
49.3789 -19.8446 2.4 47.6 -158.1 1.6976 4.8 ------ UNKNOWN
42.9917 -20.2067 3.1 49.3 -150.5 1.6177 3.7 ------ UNKNOWN
357.5497 42.5218 3.9 50.7 -44.5 3.0284 2.9 ------ UNKNOWN
Plot creation:
Sun May 31 14:16:11 EDT 2015