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
319.1705 48.9776 0.0079 10.4621 142.0517 1.0414320 24.224 TRIG_00597841
Foreground time interval of the image:
-1.664 16.453 (delta_t = 18.117 [sec])
Background time interval of the image:
-378.947 -363.368 (delta_t = 15.579 [sec])
-239.448 -1.664 (delta_t = 237.784 [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 -1.664 sec. to 17.392 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.22493 ( -0.132111 0.131083 )
Norm@50keV : 3.51691E-03 ( -0.000240042 0.000240037 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 51.17 using 59 PHA bins.
# Reduced chi-squared = 0.8978 for 57 degrees of freedom
# Null hypothesis probability = 6.923041e-01
Photon flux (15-150 keV) in 19.06 sec: 0.414319 ( -0.0294944 0.0296204 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.7538e-07 ( -5.16181e-08 5.18983e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -1.664 sec. to 17.392 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.22674 ( -0.13875 0.126487 )
Epeak [keV] : 9999.36 ( -9999.36 -9999.36 )
Norm@50keV : 3.52535E-03 ( -0.000240928 0.000625273 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 51.22 using 59 PHA bins.
# Reduced chi-squared = 0.9147 for 56 degrees of freedom
# Null hypothesis probability = 6.559980e-01
Photon flux (15-150 keV) in 19.06 sec: 0.414904 ( -0.030385 0.028884 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.74793e-07 ( -5.08235e-08 5.26037e-08 ) ergs/cm2
Band function
Time interval is from -1.664 sec. to 17.392 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.972463 ( 0.973224 0.973224 )
beta : -1.22491 ( -0.131085 0.132093 )
Epeak [keV] : 49.6299 ( -48.8949 -48.8949 )
Norm@50keV : 6.46414E-03 ( -0.00248829 0.504153 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 51.17 using 59 PHA bins.
# Reduced chi-squared = 0.9304 for 55 degrees of freedom
# Null hypothesis probability = 6.215711e-01
Photon flux (15-150 keV) in 19.06 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] : 20.1608 (-1.98841 2.28561)
R^2/D10^2 : 1.78987E-02 (-0.00524511 0.0072492)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 109.89 using 59 PHA bins.
# Reduced chi-squared = 1.9279 for 57 degrees of freedom
# Null hypothesis probability = 3.270727e-05
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.665e-08 3.955e-09
25- 50 1.334e-07 1.539e-08
50-150 4.025e-07 5.203e-08
15-150 5.625e-07 5.375e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 ( )
Norm : 1.71987 (-0.119664 0.119646)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 72.78 using 59 PHA bins.
# Reduced chi-squared = 1.277 for 57 degrees of freedom
# Null hypothesis probability = 7.758479e-02
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.165e-08 6.804e-09
25- 50 1.571e-07 2.348e-08
50-150 3.445e-07 9.139e-08
15-150 5.832e-07 1.228e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.46761 (-1.40939 1.97428)
R1^2/D10^2 : 0.952466 (-0.645895 2.49618)
kT2 [keV] : 29.3580 (-4.74628 8.31992)
R2^2/D10^2 : 4.86738E-03 (-0.00262005 0.00374909)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 52.25 using 59 PHA bins.
# Reduced chi-squared = 0.9501 for 55 degrees of freedom
# Null hypothesis probability = 5.802102e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.499e-08 2.917e-08
25- 50 1.279e-07 2.883e-08
50-150 4.787e-07 8.911e-08
15-150 6.816e-07 1.158e-07
Peak spectrum fit
Power-law model
Time interval is from 1.444 sec. to 2.444 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.49709 ( -0.261691 0.26691 )
Norm@50keV : 6.99272E-03 ( -0.00110209 0.00108362 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 67.27 using 59 PHA bins.
# Reduced chi-squared = 1.180 for 57 degrees of freedom
# Null hypothesis probability = 1.658211e-01
Photon flux (15-150 keV) in 1 sec: 0.872285 ( -0.128452 0.128532 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.63678e-08 ( -1.15117e-08 1.17649e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 1.444 sec. to 2.444 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.47072 ( -1.04865 0.422413 )
Epeak [keV] : 939.816 ( )
Norm@50keV : 7.22566E-03 ( -0.00131974 0.0229955 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 67.26 using 59 PHA bins.
# Reduced chi-squared = 1.201 for 56 degrees of freedom
# Null hypothesis probability = 1.440212e-01
Photon flux (15-150 keV) in 1 sec: 0.870651 ( -0.131888 0.129759 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.58222e-08 ( -1.31953e-08 1.22481e-08 ) ergs/cm2
Band function
Time interval is from 1.444 sec. to 2.444 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.686367 ( 0.958921 0.958921 )
beta : -1.60964 ( 1.59764 0.348844 )
Epeak [keV] : 54.3926 ( -54.2632 -54.2632 )
Norm@50keV : 2.31370E-02 ( -0.0239524 1014.66 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 66.97 using 59 PHA bins.
# Reduced chi-squared = 1.218 for 55 degrees of freedom
# Null hypothesis probability = 1.292196e-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] : 13.0533 (-2.29784 3.00118)
R^2/D10^2 : 0.159417 (-0.0825841 0.157882)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 77.96 using 59 PHA bins.
# Reduced chi-squared = 1.368 for 57 degrees of freedom
# Null hypothesis probability = 3.403565e-02
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.761e-09 1.636e-09
25- 50 1.993e-08 4.290e-09
50-150 2.152e-08 7.305e-09
15-150 4.721e-08 1.135e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.363 (-95.6557 -199.363)
Norm : 3.56031 (-0.521747 0.521765)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 67.48 using 59 PHA bins.
# Reduced chi-squared = 1.184 for 57 degrees of freedom
# Null hypothesis probability = 1.614113e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.865e-09 5.035e-09
25- 50 1.705e-08 9.475e-09
50-150 3.740e-08 2.083e-08
15-150 6.332e-08 3.588e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 9.24342 (-3.1093 2.69685)
R1^2/D10^2 : 0.440999 (-0.25914 0.371113)
kT2 [keV] : 61.4841 (-55.3582 -61.4883)
R2^2/D10^2 : 8.96288E-04 (-0.000745019 0.0174424)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 66.43 using 59 PHA bins.
# Reduced chi-squared = 1.208 for 55 degrees of freedom
# Null hypothesis probability = 1.389734e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.747e-09 3.339e-09
25- 50 1.883e-08 8.065e-09
50-150 4.141e-08 2.062e-08
15-150 6.798e-08 3.391e-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: 1.21819 ( -0.134624 0.13346 )
Norm@50keV : 3.55790E-03 ( -0.000246444 0.000246432 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 53.77 using 59 PHA bins.
# Reduced chi-squared = 0.9433 for 57 degrees of freedom
# Null hypothesis probability = 5.971767e-01
Photon flux (15-150 keV) in 18.12 sec: 0.418724 ( -0.0302574 0.0303863 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.50758e-07 ( -5.04897e-08 5.07625e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.22108 ( -0.145621 0.127995 )
Epeak [keV] : 9999.36 ( -9999.36 -9999.36 )
Norm@50keV : 3.57416E-03 ( -0.000247521 0.000631398 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 53.82 using 59 PHA bins.
# Reduced chi-squared = 0.9610 for 56 degrees of freedom
# Null hypothesis probability = 5.579311e-01
Photon flux (15-150 keV) in 18.12 sec: 0.419476 ( -0.03105 0.029543 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.46942e-07 ( -4.67786e-08 5.33815e-08 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.982954 ( 0.982954 0.982954 )
beta : -1.21817 ( 1.21818 0.13461 )
Epeak [keV] : 46.6995 ( -46.6984 -46.6984 )
Norm@50keV : 6.45495E-03 ( -0.00314295 0.510641 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 53.77 using 59 PHA bins.
# Reduced chi-squared = 0.9776 for 55 degrees of freedom
# Null hypothesis probability = 5.218628e-01
Photon flux (15-150 keV) in 18.12 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) = 1.44e-07
S(50-100 keV) = 2.46e-07
T90 vs. Hardness ratio plot
T90 = 15.1199999451637 sec.
Hardness ratio (energy fluence ratio) = 1.70833
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.25851
Count Ratio (50-100 keV) / (15-25 keV) = 1.23625
Mask shadow pattern
IMX = -1.456122689975370E-01, IMY = -1.135532740789120E-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:
-378.947400 -363.368000
-239.448000 -1.664000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
299.6101 35.2055 0.4 25.1 92.4 7.5200 25.6 1.0 Cyg X-1
308.0788 40.9288 1.6 16.9 101.5 1.6202 7.4 2.0 Cyg X-3
325.9846 38.2923 3.9 5.4 52.1 0.5762 2.9 9.0 Cyg X-2
317.2819 29.1254 3.7 17.1 52.2 0.6376 3.2 ------ UNKNOWN
21.4544 65.0066 2.5 36.1 -137.9 1.5757 4.6 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-1.664000 16.452590
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
299.5279 35.0195 10.4 25.3 92.1 -0.0744 -1.1 11.3 Cyg X-1
308.1179 41.1127 6.5 16.9 102.0 -0.0906 -1.8 9.6 Cyg X-3
326.0660 38.2588 3.9 5.4 51.3 -0.1303 -3.0 6.2 Cyg X-2
319.1704 48.9775 0.5 10.5 142.1 1.0417 24.2 ------ UNKNOWN
340.3747 29.6298 2.4 14.9 -26.2 0.2096 4.9 ------ UNKNOWN
352.6700 3.7953 2.3 43.2 -24.6 0.3778 5.1 495.0 UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
53.852580 962.619600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
288.7746 10.9177 2.5 45.7 47.2 9.7284 4.5 2.2 GRS 1915+105
299.5808 35.1984 0.2 19.9 56.7 27.9296 46.0 0.5 Cyg X-1
308.0643 40.9793 1.3 11.2 51.7 4.7860 8.9 2.6 Cyg X-3
326.3154 38.1699 6.0 12.0 -24.8 1.1833 1.9 11.3 Cyg X-2
323.7408 27.8798 3.1 21.4 -7.9 2.1343 3.7 ------ UNKNOWN
125.1162 72.1822 3.1 58.4 -171.7 12.2244 3.8 ------ UNKNOWN
338.5381 -3.9118 3.1 55.5 -20.4 8.0747 3.7 ------ UNKNOWN
12.3958 35.3688 4.7 40.8 -87.7 9.8102 2.5 ------ UNKNOWN
Plot creation:
Sat May 30 13:39:21 EDT 2015