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
39.1671 18.1628 0.0155 22.2107 76.8604 0.1456588 12.463 TRIG_00621229
Foreground time interval of the image:
0.000 0.336 (delta_t = 0.336 [sec])
Background time interval of the image:
-239.984 0.000 (delta_t = 239.984 [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 0.064000
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 0.064000
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 0.064000
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 0.000 sec. to 0.336 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.60425 ( -0.219852 0.231131 )
Norm@50keV : 2.30658E-02 ( -0.00348168 0.00343023 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 59.02 using 59 PHA bins.
# Reduced chi-squared = 1.035 for 57 degrees of freedom
# Null hypothesis probability = 4.015232e-01
Photon flux (15-150 keV) in 0.336 sec: 2.96796 ( -0.42006 0.420192 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.24443e-08 ( -1.15968e-08 1.16837e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.000 sec. to 0.336 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.14621 ( -0.939046 0.432799 )
Epeak [keV] : 94.8647 ( )
Norm@50keV : 3.96550E-02 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 58.03 using 59 PHA bins.
# Reduced chi-squared = 1.036 for 56 degrees of freedom
# Null hypothesis probability = 4.003087e-01
Photon flux (15-150 keV) in 0.336 sec: 2.95180 ( -0.42172 0.4215 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.15848e-08 ( -1.20416e-08 1.19754e-08 ) ergs/cm2
Band function
Time interval is from 0.000 sec. to 0.336 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.10730 ( 1.10746 0.728872 )
beta : -9.35007 ( 9.37159 19.3716 )
Epeak [keV] : 91.6462 ( -33.6548 -91.6966 )
Norm@50keV : 4.14352E-02 ( -0.0210771 0.0208544 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 58.04 using 59 PHA bins.
# Reduced chi-squared = 1.055 for 55 degrees of freedom
# Null hypothesis probability = 3.640047e-01
Photon flux (15-150 keV) in 0.336 sec: 2.94783 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 7.15431e-08 ( 0 0 ) ergs/cm2
Single BB
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 14.1824 (-2.41677 2.94466)
R^2/D10^2 : 0.420012 (-0.204023 0.386239)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 71.59 using 59 PHA bins.
# Reduced chi-squared = 1.256 for 57 degrees of freedom
# Null hypothesis probability = 9.239397e-02
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.988e-09 1.623e-09
25- 50 2.256e-08 5.250e-09
50-150 3.007e-08 9.079e-09
15-150 5.862e-08 1.242e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 174.924 (-78.6526 -174.759)
Norm : 12.2897 (-1.78997 2.04305)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 58.10 using 59 PHA bins.
# Reduced chi-squared = 1.019 for 57 degrees of freedom
# Null hypothesis probability = 4.346978e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.045e-08 5.959e-09
25- 50 1.978e-08 1.073e-08
50-150 4.144e-08 2.318e-08
15-150 7.167e-08 3.921e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.67827 (-1.89926 2.95231)
R1^2/D10^2 : 6.72188 (-5.16084 27.4409)
kT2 [keV] : 22.8878 (-5.91872 10.7008)
R2^2/D10^2 : 6.22143E-02 (-0.0476473 0.128591)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 57.20 using 59 PHA bins.
# Reduced chi-squared = 1.040 for 55 degrees of freedom
# Null hypothesis probability = 3.935278e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.089e-08 5.713e-09
25- 50 1.862e-08 9.059e-09
50-150 4.269e-08 2.412e-08
15-150 7.220e-08 3.284e-08
Peak spectrum fit
Power-law model
Time interval is from -0.324 sec. to 0.676 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.51297 ( -0.269401 0.278506 )
Norm@50keV : 9.78945E-03 ( -0.00170895 0.00168871 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 57.33 using 59 PHA bins.
# Reduced chi-squared = 1.006 for 57 degrees of freedom
# Null hypothesis probability = 4.626793e-01
Photon flux (15-150 keV) in 1 sec: 1.22642 ( -0.204453 0.204628 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.26754e-08 ( -1.74787e-08 1.77884e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.324 sec. to 0.676 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.481038 ( -1.50935 1.1154 )
Epeak [keV] : 72.7566 ( -20.8006 -72.757 )
Norm@50keV : 3.30408E-02 ( -0.0330403 0.153311 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 54.91 using 59 PHA bins.
# Reduced chi-squared = 0.9805 for 56 degrees of freedom
# Null hypothesis probability = 5.163141e-01
Photon flux (15-150 keV) in 1 sec: 1.18709 ( -0.209777 0.20951 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.71497e-08 ( -1.81251e-08 1.88213e-08 ) ergs/cm2
Band function
Time interval is from -0.324 sec. to 0.676 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.482249 ( -0.647191 0.883286 )
beta : -10.0000 ( 10 3.55271e-15 )
Epeak [keV] : 72.7752 ( -20.8377 362.381 )
Norm@50keV : 3.29945E-02 ( -0.0329944 0.153369 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 54.91 using 59 PHA bins.
# Reduced chi-squared = 0.9983 for 55 degrees of freedom
# Null hypothesis probability = 4.782012e-01
Photon flux (15-150 keV) in 1 sec: 1.20387 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 9.01973e-08 ( 0 0 ) ergs/cm2
Single BB
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 14.8405 (-2.54846 3.1424)
R^2/D10^2 : 0.151768 (-0.0749313 0.141034)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 59.02 using 59 PHA bins.
# Reduced chi-squared = 1.035 for 57 degrees of freedom
# Null hypothesis probability = 4.017131e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.010e-09 2.457e-09
25- 50 2.758e-08 7.190e-09
50-150 4.114e-08 1.301e-08
15-150 7.573e-08 1.709e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 198.973 (-102.601 -199.058)
Norm : 5.04958 (-0.828119 0.916314)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 56.14 using 59 PHA bins.
# Reduced chi-squared = 0.9848 for 57 degrees of freedom
# Null hypothesis probability = 5.075105e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.258e-08 7.370e-09
25- 50 2.419e-08 1.346e-08
50-150 5.302e-08 2.999e-08
15-150 8.978e-08 5.055e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 4.95610 (-3.10942 7.76419)
R1^2/D10^2 : 3.10599 (-2.92336 561.735)
kT2 [keV] : 18.5144 (-4.5104 28.0475)
R2^2/D10^2 : 6.10402E-02 (-0.0544194 0.100153)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 54.60 using 59 PHA bins.
# Reduced chi-squared = 0.9928 for 55 degrees of freedom
# Null hypothesis probability = 4.897489e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.144e-08 6.130e-09
25- 50 2.426e-08 1.264e-08
50-150 4.928e-08 2.859e-08
15-150 8.497e-08 4.676e-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: 1.60425 ( -0.219852 0.231131 )
Norm@50keV : 2.30658E-02 ( -0.00348168 0.00343023 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 59.02 using 59 PHA bins.
# Reduced chi-squared = 1.035 for 57 degrees of freedom
# Null hypothesis probability = 4.015232e-01
Photon flux (15-150 keV) in 0.336 sec: 2.96796 ( -0.42006 0.420192 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.24443e-08 ( -1.15968e-08 1.16837e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.14621 ( -0.939046 0.432799 )
Epeak [keV] : 94.8647 ( )
Norm@50keV : 3.96550E-02 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 58.03 using 59 PHA bins.
# Reduced chi-squared = 1.036 for 56 degrees of freedom
# Null hypothesis probability = 4.003087e-01
Photon flux (15-150 keV) in 0.336 sec: 2.95180 ( -0.42172 0.4215 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.15848e-08 ( -1.20416e-08 1.19754e-08 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.10730 ( 1.10746 0.728872 )
beta : -9.35007 ( 9.37159 19.3716 )
Epeak [keV] : 91.6462 ( -33.6548 -91.6966 )
Norm@50keV : 4.14352E-02 ( -0.0210771 0.0208544 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 58.04 using 59 PHA bins.
# Reduced chi-squared = 1.055 for 55 degrees of freedom
# Null hypothesis probability = 3.640047e-01
Photon flux (15-150 keV) in 0.336 sec: 2.94783 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 7.15431e-08 ( 0 0 ) ergs/cm2
S(25-50 keV) vs. S(50-100 keV) plot
S(25-50 keV) = 1.88e-08
S(50-100 keV) = 2.48e-08
T90 vs. Hardness ratio plot
T90 = 0.287999987602234 sec.
Hardness ratio (energy fluence ratio) = 1.31915
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.08161
Count Ratio (50-100 keV) / (15-25 keV) = 1.07014
Mask shadow pattern
IMX = 9.281901866037730E-02, IMY = -3.976206769161882E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.064000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.064000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.064000
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:
-239.984000 0.000000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
352.4782 60.9590 3.0 55.3 -1.6 3.2225 3.8 ------ UNKNOWN
333.1022 18.0061 3.0 44.7 -60.3 3.8254 3.9 ------ UNKNOWN
339.4205 -3.4957 3.5 40.7 -93.0 3.4846 3.3 ------ UNKNOWN
347.2300 -28.4347 2.8 48.0 -129.1 4.6265 4.2 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
0.000000 0.336000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
39.1671 18.1628 0.9 22.2 76.9 0.1457 12.5 ------ UNKNOWN
43.9570 -14.1574 2.2 34.5 145.3 0.0815 5.3 ------ UNKNOWN
30.8112 20.7328 2.2 16.8 57.8 0.0455 5.1 ------ UNKNOWN
26.8784 0.4764 2.3 12.1 147.9 0.0363 5.0 ------ UNKNOWN
11.4770 3.2586 2.3 8.9 -116.9 0.0378 4.9 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
53.316590 962.111400
1683.016000 1683.416580
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
62.3312 16.3554 2.6 22.2 105.8 2.8774 4.4 ------ UNKNOWN
35.9681 70.6334 3.2 52.5 13.4 8.2328 3.7 ------ UNKNOWN
23.2712 53.1744 2.9 37.1 -1.0 2.8660 4.0 ------ UNKNOWN
4.6260 53.4248 2.2 44.2 -14.2 4.6413 5.2 ------ UNKNOWN
31.9246 -5.9267 3.7 25.1 -148.2 1.7270 3.1 ------ UNKNOWN
353.5005 55.8056 2.7 50.9 -16.5 4.8263 4.4 ------ UNKNOWN
344.9304 59.4511 3.4 56.6 -14.9 8.1852 3.4 ------ UNKNOWN
29.8134 -39.1277 5.5 57.9 -156.8 9.7260 2.1 ------ UNKNOWN
345.4162 45.0769 2.4 51.9 -31.6 9.4045 4.9 ------ UNKNOWN
347.8443 30.1421 3.1 47.9 -50.7 11.2316 3.7 ------ UNKNOWN
11.0433 -21.1551 3.1 48.0 -129.0 11.3478 3.7 ------ UNKNOWN
Plot creation:
Thu May 28 13:55:46 EDT 2015