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Image
Pre-slew 15.0-350.0 keV image (Event data)
# RAcent DECcent POSerr Theta Phi Peak Cts SNR Name
203.1473 34.0869 0.0094 28.6642 7.3722 1.6696792 20.529 TRIG_00377487
Foreground time interval of the image:
-28.656 18.221 (delta_t = 46.877 [sec])
Background time interval of the image:
-339.379 -28.656 (delta_t = 310.723 [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)
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 -28.656 sec. to 127.388 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.08642 ( -0.140826 0.14655 )
Norm@50keV : 1.01081E-03 ( -9.85773e-05 9.70878e-05 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 59.43 using 59 PHA bins.
# Reduced chi-squared = 1.043 for 57 degrees of freedom
# Null hypothesis probability = 3.870278e-01
Photon flux (15-150 keV) in 156 sec: 0.157969 ( -0.0116328 0.0116358 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.4632e-06 ( -1.28809e-07 1.31045e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -28.656 sec. to 127.388 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.51613 ( -0.633249 0.486506 )
Epeak [keV] : 34.0584 ( -24.2582 13.288 )
Norm@50keV : 2.19454E-03 ( -0.00101243 0.00301222 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 56.15 using 59 PHA bins.
# Reduced chi-squared = 1.003 for 56 degrees of freedom
# Null hypothesis probability = 4.693750e-01
Photon flux (15-150 keV) in 156 sec: 0.154242 ( -0.012089 0.012103 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.37316e-06 ( -1.47384e-07 1.53694e-07 ) ergs/cm2
Band function
Time interval is from -28.656 sec. to 127.388 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.51708 ( -0.596003 0.554981 )
beta : -10.0000 ( 10 1.77636e-15 )
Epeak [keV] : 34.0399 ( -13.1282 13.304 )
Norm@50keV : 2.19141E-03 ( -0.000967456 0.00301699 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 56.15 using 59 PHA bins.
# Reduced chi-squared = 1.021 for 55 degrees of freedom
# Null hypothesis probability = 4.317027e-01
Photon flux (15-150 keV) in 156 sec: 0.155315 ( 6.84469 -0.013428 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.37248e-06 ( -1.37139e-06 -1.48688e-07 ) ergs/cm2
Single BB
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 8.90952 (-0.804866 0.903935)
R^2/D10^2 : 0.111238 (-0.0351447 0.0507316)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 91.34 using 59 PHA bins.
# Reduced chi-squared = 1.603 for 57 degrees of freedom
# Null hypothesis probability = 2.620010e-03
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.668e-07 3.487e-08
25- 50 5.581e-07 4.945e-08
50-150 2.064e-07 4.685e-08
15-150 1.031e-06 8.245e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 56.4117 (-11.3992 15.6179)
Norm : 0.847083 (-0.107433 0.118832)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 56.38 using 59 PHA bins.
# Reduced chi-squared = 0.9891 for 57 degrees of freedom
# Null hypothesis probability = 4.984126e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.286e-07 3.416e-08
25- 50 4.905e-07 3.627e-08
50-150 5.296e-07 1.172e-07
15-150 1.349e-06 1.352e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.75368 (-0.897299 0.954262)
R1^2/D10^2 : 0.465900 (-0.201351 0.418841)
kT2 [keV] : 19.6126 (-4.08818 6.37668)
R2^2/D10^2 : 3.46124E-03 (-0.00229933 0.00585365)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 51.09 using 59 PHA bins.
# Reduced chi-squared = 0.9290 for 55 degrees of freedom
# Null hypothesis probability = 6.246488e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.406e-07 8.572e-08
25- 50 4.713e-07 1.051e-07
50-150 5.849e-07 3.028e-07
15-150 1.397e-06 4.338e-07
Peak spectrum fit
Power-law model
Time interval is from 0.064 sec. to 1.064 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.19794 ( -0.277639 0.265118 )
Norm@50keV : 9.17367E-03 ( -0.00130445 0.00130125 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 67.54 using 59 PHA bins.
# Reduced chi-squared = 1.185 for 57 degrees of freedom
# Null hypothesis probability = 1.602513e-01
Photon flux (15-150 keV) in 1 sec: 1.07649 ( -0.159903 0.160577 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.31251e-08 ( -1.45356e-08 1.46434e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.064 sec. to 1.064 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.19445 ( -0.297782 0.250212 )
Epeak [keV] : 1.00000E+04 ( )
Norm@50keV : 9.21741E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 67.56 using 59 PHA bins.
# Reduced chi-squared = 1.207 for 56 degrees of freedom
# Null hypothesis probability = 1.384178e-01
Photon flux (15-150 keV) in 1 sec: 1.08194 ( -0.163334 0.1557 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.29691e-08 ( -1.43911e-08 1.40029e-08 ) ergs/cm2
Band function
Time interval is from 0.064 sec. to 1.064 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 4.92749 ( -4.92749 -4.92749 )
beta : -1.23006 ( -0.290589 0.289511 )
Epeak [keV] : 22.3073 ( -22.3073 9.13832 )
Norm@50keV : 1300.20 ( -183.872 3.10999e+06 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 67.15 using 59 PHA bins.
# Reduced chi-squared = 1.221 for 55 degrees of freedom
# Null hypothesis probability = 1.261156e-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] : 19.8134 (-5.40143 8.22158)
R^2/D10^2 : 4.79654E-02 (-0.0471258 0.0896929)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 90.95 using 59 PHA bins.
# Reduced chi-squared = 1.596 for 57 degrees of freedom
# Null hypothesis probability = 2.847859e-03
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.643e-09 1.353e-09
25- 50 1.803e-08 4.870e-09
50-150 5.242e-08 1.487e-08
15-150 7.409e-08 1.795e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 ( )
Norm : 4.47693 (-0.650315 0.650226)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 74.06 using 59 PHA bins.
# Reduced chi-squared = 1.299 for 57 degrees of freedom
# Null hypothesis probability = 6.397295e-02
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.115e-08 6.260e-09
25- 50 2.145e-08 1.196e-08
50-150 4.706e-08 2.643e-08
15-150 7.966e-08 4.423e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 8.73900 (-2.03817 2.44295)
R1^2/D10^2 : 0.611380 (-0.318304 0.629656)
kT2 [keV] : 99.9567 (-58.6938 -99.9972)
R2^2/D10^2 : 6.49206E-04 (-0.00047518 0.00375007)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 61.42 using 59 PHA bins.
# Reduced chi-squared = 1.117 for 55 degrees of freedom
# Null hypothesis probability = 2.568010e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.341e-09 4.821e-09
25- 50 2.134e-08 1.124e-08
50-150 6.880e-08 6.930e-08
15-150 9.948e-08 8.124e-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: 1.76915 ( -0.144649 0.148238 )
Norm@50keV : 2.17030E-03 ( -0.000192742 0.000189903 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 54.89 using 59 PHA bins.
# Reduced chi-squared = 0.9630 for 57 degrees of freedom
# Null hypothesis probability = 5.546281e-01
Photon flux (15-150 keV) in 46.88 sec: 0.295561 ( -0.023286 0.0233108 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.37877e-07 ( -8.54327e-08 8.64636e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.68018 ( -0.54097 0.528932 )
Epeak [keV] : 165.922 ( -155.459 -165.922 )
Norm@50keV : 2.42417E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 54.80 using 59 PHA bins.
# Reduced chi-squared = 0.9785 for 56 degrees of freedom
# Null hypothesis probability = 5.204451e-01
Photon flux (15-150 keV) in 46.88 sec: 0.294280 ( -0.024251 0.024101 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.30273e-07 ( -9.6315e-08 9.22927e-08 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.68015 ( 1.68015 0.540353 )
beta : -9.36949 ( 9.37144 19.3714 )
Epeak [keV] : 165.868 ( -104.948 -165.868 )
Norm@50keV : 2.42372E-03 ( -0.000441164 0.000827256 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 54.80 using 59 PHA bins.
# Reduced chi-squared = 0.9963 for 55 degrees of freedom
# Null hypothesis probability = 4.823191e-01
Photon flux (15-150 keV) in 46.88 sec: 0.294001 ( ) 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) = 4.51e-07
S(50-100 keV) = 4.25e-07
T90 vs. Hardness ratio plot
T90 = 101.759999930859 sec.
Hardness ratio (energy fluence ratio) = 0.94235
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.02606
Count Ratio (50-100 keV) / (15-25 keV) = 0.532743
Mask shadow pattern
IMX = 5.421540797947368E-01, IMY = -7.014620699431262E-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:
-339.379360 -28.656000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.3775 35.3279 4.0 13.1 178.2 0.6683 2.9 4.0 Her X-1
268.3635 -1.4614 23.4 46.7 -133.0 0.3896 0.5 0.6 SW J1753.5-0127
288.7960 10.9504 3.0 51.9 -163.9 2.5593 3.9 0.3 GRS 1915+105
299.5890 35.1979 0.8 49.1 162.2 11.1291 14.6 0.2 Cyg X-1
275.9653 6.6619 4.4 45.2 -148.4 1.3589 2.6 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-28.656000 18.220590
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.3034 35.5102 0.0 13.0 177.4 -0.0986 -1.4 12.6 Her X-1
268.2707 -1.4707 9.9 46.7 -132.9 -0.2851 -1.2 5.9 SW J1753.5-0127
288.7640 11.0535 104.6 51.8 -164.0 0.0224 0.1 6.8 GRS 1915+105
299.6261 35.0224 5.7 49.1 162.4 -0.4305 -2.0 10.9 Cyg X-1
242.3945 74.8604 2.9 39.0 92.2 1.1489 3.9 ------ UNKNOWN
300.7114 27.8998 2.3 52.7 170.4 1.3538 5.1 ------ UNKNOWN
203.1473 34.0869 0.6 28.7 7.4 1.6697 20.5 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
74.020580 231.820600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.6151 35.4778 51.1 41.9 -153.7 -0.0539 -0.2 11.2 Her X-1
152.2945 33.7493 2.2 41.7 58.0 2.8145 5.2 ------ UNKNOWN
150.3884 16.8890 2.9 50.0 37.2 2.7370 4.0 ------ UNKNOWN
201.2718 76.3757 2.5 42.3 132.9 1.8695 4.6 ------ UNKNOWN
167.5259 13.8491 2.3 38.0 20.1 1.0255 5.0 ------ UNKNOWN
163.2046 -8.2054 2.7 56.7 2.9 3.3845 4.3 ------ UNKNOWN
268.4179 42.9631 2.6 50.6 -167.1 1.4573 4.5 ------ UNKNOWN
266.6114 24.8992 4.6 55.2 -145.1 2.1058 2.5 ------ UNKNOWN
256.5054 19.2980 3.6 49.4 -133.4 1.9762 3.2 ------ UNKNOWN
Plot creation:
Sun May 31 02:32:38 EDT 2015