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
46.3058 -50.4948 0.0054 36.0550 109.7556 8.4119131 35.273 TRIG_00232683
Foreground time interval of the image:
-4.056 14.797 (delta_t = 18.853 [sec])
Background time interval of the image:
-35.403 -4.056 (delta_t = 31.347 [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 -4.056 sec. to 248.288 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.02025 ( -0.0233575 0.0232508 )
Norm@50keV : 1.66048E-02 ( -0.000228442 0.000227482 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 27.93 using 59 PHA bins.
# Reduced chi-squared = 0.4899 for 57 degrees of freedom
# Null hypothesis probability = 9.995803e-01
Photon flux (15-150 keV) in 252.3 sec: 1.91392 ( -0.0277783 0.0277863 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.49813e-05 ( -5.31571e-07 5.31157e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -4.056 sec. to 248.288 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.01498 ( -0.0249264 0.0222851 )
Epeak [keV] : 1.00000E+04 ( -10000 -10000 )
Norm@50keV : 1.66929E-02 ( -0.00023379 0.00019709 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 28.29 using 59 PHA bins.
# Reduced chi-squared = 0.5052 for 56 degrees of freedom
# Null hypothesis probability = 9.992609e-01
Photon flux (15-150 keV) in 252.3 sec: 1.91279 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 4.49967e-05 ( -5.36642e-07 5.29325e-07 ) ergs/cm2
Band function
Time interval is from -4.056 sec. to 248.288 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.835612 ( 0.835612 0.835612 )
beta : -1.02025 ( -0.0232519 0.0233567 )
Epeak [keV] : 42.1546 ( -42.1546 -42.1546 )
Norm@50keV : 2.89584E-02 ( -0.00962638 654500 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 27.93 using 59 PHA bins.
# Reduced chi-squared = 0.5077 for 55 degrees of freedom
# Null hypothesis probability = 9.991188e-01
Photon flux (15-150 keV) in 252.3 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] : 26.7714 ( )
R^2/D10^2 : 3.63337E-02 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 1185.37 using 59 PHA bins.
# Reduced chi-squared = 20.7959 for 57 degrees of freedom
# Null hypothesis probability = 1.303888e-210
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.099e-06 2.965e-08
25- 50 6.450e-06 1.362e-07
50-150 3.384e-05 4.920e-07
15-150 4.138e-05 5.298e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.363 ( )
Norm : 8.80047 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 1885.49 using 59 PHA bins.
# Reduced chi-squared = 33.0788 for 57 degrees of freedom
# Null hypothesis probability = 0.000000e+00
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.529e-06 7.695e-08
25- 50 1.064e-05 1.615e-07
50-150 2.333e-05 3.141e-07
15-150 3.949e-05 5.803e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 9.11178 (-0.513891 0.542978)
R1^2/D10^2 : 0.618447 (-0.105739 0.132117)
kT2 [keV] : 41.0167 (-1.94879 2.29006)
R2^2/D10^2 : 8.62511E-03 (-0.00130687 0.00139914)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 33.84 using 59 PHA bins.
# Reduced chi-squared = 0.6153 for 55 degrees of freedom
# Null hypothesis probability = 9.890058e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.002e-06 1.615e-07
25- 50 8.686e-06 2.296e-07
50-150 3.359e-05 6.686e-07
15-150 4.528e-05 7.947e-07
Peak spectrum fit
Power-law model
Time interval is from 45.144 sec. to 46.144 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.684462 ( -0.0463159 0.0460264 )
Norm@50keV : 0.127101 ( -0.00322189 0.00320638 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 43.40 using 59 PHA bins.
# Reduced chi-squared = 0.7614 for 57 degrees of freedom
# Null hypothesis probability = 9.079452e-01
Photon flux (15-150 keV) in 1 sec: 14.7105 ( -0.355812 0.356007 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.56241e-06 ( -4.17135e-08 4.18336e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 45.144 sec. to 46.144 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.12632 ( )
Epeak [keV] : 38.5294 ( )
Norm@50keV : 1.70597E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 52.48 using 59 PHA bins.
# Reduced chi-squared = 0.9372 for 56 degrees of freedom
# Null hypothesis probability = 6.088534e-01
Photon flux (15-150 keV) in 1 sec: 14.7061 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 1.5622e-06 ( 0 0 ) ergs/cm2
Band function
Time interval is from 45.144 sec. to 46.144 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.879708 ( 0.879708 0.879708 )
beta : -0.684462 ( -0.0460254 0.0463182 )
Epeak [keV] : 16.0846 ( -16.0846 -16.0846 )
Norm@50keV : 0.178950 ( -0.0498703 2.22309e+06 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 43.40 using 59 PHA bins.
# Reduced chi-squared = 0.7891 for 55 degrees of freedom
# Null hypothesis probability = 8.708069e-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] : 28.8162 ( )
R^2/D10^2 : 0.253467 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 271.51 using 59 PHA bins.
# Reduced chi-squared = 4.7633 for 57 degrees of freedom
# Null hypothesis probability = 1.076434e-29
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.374e-08 1.695e-09
25- 50 2.046e-07 7.400e-09
50-150 1.218e-06 4.650e-08
15-150 1.456e-06 4.300e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.363 ( )
Norm : 55.4421 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 943.90 using 59 PHA bins.
# Reduced chi-squared = 16.560 for 57 degrees of freedom
# Null hypothesis probability = 6.839577e-161
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.381e-07 3.550e-09
25- 50 2.656e-07 7.300e-09
50-150 5.824e-07 1.595e-08
15-150 9.861e-07 2.510e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 8.50069 (-1.01604 1.16488)
R1^2/D10^2 : 4.28434 (-1.36613 2.1472)
kT2 [keV] : 43.5590 (-3.92646 5.35577)
R2^2/D10^2 : 7.34993E-02 (-0.0196538 0.0219366)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 38.45 using 59 PHA bins.
# Reduced chi-squared = 0.6990 for 55 degrees of freedom
# Null hypothesis probability = 9.560490e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.526e-08 8.740e-09
25- 50 2.313e-07 1.810e-08
50-150 1.285e-06 7.450e-08
15-150 1.591e-06 1.010e-07
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: 1.05504 ( -0.0505186 0.0501838 )
Norm@50keV : 3.08479E-02 ( -0.00086861 0.000866234 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 39.99 using 59 PHA bins.
# Reduced chi-squared = 0.7015 for 57 degrees of freedom
# Null hypothesis probability = 9.575257e-01
Photon flux (15-150 keV) in 18.85 sec: 3.56420 ( -0.104326 0.104461 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.16961e-06 ( -1.79035e-07 1.79261e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.926811 ( -0.199075 0.157984 )
Epeak [keV] : 502.682 ( -502.682 -502.682 )
Norm@50keV : 3.49679E-02 ( -0.004513 0.00726565 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 38.69 using 59 PHA bins.
# Reduced chi-squared = 0.6908 for 56 degrees of freedom
# Null hypothesis probability = 9.623626e-01
Photon flux (15-150 keV) in 18.85 sec: 3.54041 ( -0.10959 0.1098 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.14259e-06 ( -1.86181e-07 1.85296e-07 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 4.99996 ( -4.99996 -4.99996 )
beta : -1.07934 ( -0.053257 0.0532332 )
Epeak [keV] : 26.2875 ( -26.2875 3.7776 )
Norm@50keV : 1597.69 ( -43.531 4.36481e+06 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 37.98 using 59 PHA bins.
# Reduced chi-squared = 0.6905 for 55 degrees of freedom
# Null hypothesis probability = 9.611136e-01
Photon flux (15-150 keV) in 18.85 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) = 8.44e-06
S(50-100 keV) = 1.66e-05
T90 vs. Hardness ratio plot
T90 = 75.7360000014305 sec.
Hardness ratio (energy fluence ratio) = 1.96682
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.7028
Count Ratio (50-100 keV) / (15-25 keV) = 1.81018
Mask shadow pattern
IMX = -2.460731369944117E-01, IMY = -6.851610378352506E-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:
-35.403400 -4.056000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.8050 -40.6144 0.0 39.8 -142.5 -0.1772 -2.1 13.1 Vela X-1
170.4489 -60.8005 3.2 25.3 -93.1 0.2376 3.6 11.3 Cen X-3
186.9068 -62.9431 0.0 26.4 -74.8 0.0144 0.2 12.4 GX 301-2
264.7078 -44.5086 5.4 55.3 -14.9 0.3970 2.1 3.8 4U 1735-44
92.0664 -37.4541 2.0 42.5 165.2 0.5243 5.8 ------ UNKNOWN
291.2513 -53.4222 2.3 47.4 7.9 0.5786 5.1 ------ UNKNOWN
145.2024 -56.2181 1.7 25.5 -125.8 0.4179 6.9 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-4.056000 14.796600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.4501 -40.6888 25.6 39.7 -142.9 0.0381 0.4 8.8 Vela X-1
170.4342 -60.8155 0.0 25.3 -93.1 -0.1454 -2.0 12.1 Cen X-3
186.9121 -62.6405 14.6 26.7 -75.1 -0.0580 -0.8 10.5 GX 301-2
264.6212 -44.4497 11.4 55.4 -14.9 0.2156 1.0 5.2 4U 1735-44
46.3058 -50.4948 0.3 36.1 109.8 8.4113 35.3 ------ UNKNOWN
289.7856 -44.3441 2.4 56.4 6.7 2.1607 4.9 ------ UNKNOWN
179.4233 -69.0770 3.1 19.6 -74.4 0.2299 3.7 ------ UNKNOWN
135.2909 -25.1401 3.4 55.1 -145.3 1.0194 3.4 ------ UNKNOWN
153.8824 -36.8515 1.8 45.6 -122.7 1.4963 6.3 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
69.796600 962.772000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
46.3208 -50.4866 0.6 0.0 113.3 6.9142 18.0 ------ UNKNOWN
54.0792 -70.8733 3.5 20.7 -59.2 1.3857 3.2 ------ UNKNOWN
Plot creation:
Sun May 31 11:43:44 EDT 2015