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
170.8828 8.9315 0.0022 15.6865 -108.9418 23.9560912 85.771 TRIG_00525068
Foreground time interval of the image:
-15.124 139.885 (delta_t = 155.009 [sec])
Background time interval of the image:
-239.016 -15.124 (delta_t = 223.892 [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
8 ms binning
From T100_start-3 s to T100_start+3 s
2 ms binning
From T100_start-1 s to T100_start+1 s
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 -15.124 sec. to 192.772 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.11617 ( -0.0270059 0.0268945 )
Norm@50keV : 1.36740E-02 ( -0.00020404 0.000203042 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 38.77 using 59 PHA bins.
# Reduced chi-squared = 0.6801 for 57 degrees of freedom
# Null hypothesis probability = 9.692294e-01
Photon flux (15-150 keV) in 207.9 sec: 1.58866 ( -0.0257845 0.0259414 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.95707e-05 ( -4.02436e-07 4.02538e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -15.124 sec. to 192.772 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.11159 ( -0.0283388 0.0260507 )
Epeak [keV] : 9999.36 ( -9999.36 -9999.36 )
Norm@50keV : 1.37481E-02 ( -0.000190892 0.000639305 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 39.12 using 59 PHA bins.
# Reduced chi-squared = 0.6986 for 56 degrees of freedom
# Null hypothesis probability = 9.578205e-01
Photon flux (15-150 keV) in 207.9 sec: 1.58771 ( -0.02582 0.02587 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.95754e-05 ( -3.99168e-07 4.0395e-07 ) ergs/cm2
Band function
Time interval is from -15.124 sec. to 192.772 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.766749 ( 0.847056 5.8378 )
beta : -1.11792 ( -0.0269344 0.0270108 )
Epeak [keV] : 92.0202 ( -62.6305 -62.6305 )
Norm@50keV : 2.43950E-02 ( -0.0101751 475407 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 38.56 using 59 PHA bins.
# Reduced chi-squared = 0.7011 for 55 degrees of freedom
# Null hypothesis probability = 9.547407e-01
Photon flux (15-150 keV) in 207.9 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] : 24.3543 ( )
R^2/D10^2 : 3.86714E-02 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 1031.42 using 59 PHA bins.
# Reduced chi-squared = 18.0951 for 57 degrees of freedom
# Null hypothesis probability = 7.691724e-179
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.398e-07 2.568e-08
25- 50 4.700e-06 1.112e-07
50-150 2.074e-05 3.555e-07
15-150 2.628e-05 4.054e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.363 ( )
Norm : 7.14613 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 1001.54 using 59 PHA bins.
# Reduced chi-squared = 17.5710 for 57 degrees of freedom
# Null hypothesis probability = 1.055181e-172
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.699e-06 6.341e-08
25- 50 7.116e-06 1.175e-07
50-150 1.561e-05 2.422e-07
15-150 2.642e-05 3.950e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 8.95085 (-0.546227 0.576808)
R1^2/D10^2 : 0.588008 (-0.108046 0.138031)
kT2 [keV] : 39.8354 (-2.33109 2.81305)
R2^2/D10^2 : 7.19935E-03 (-0.00134534 0.0014841)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 50.27 using 59 PHA bins.
# Reduced chi-squared = 0.9140 for 55 degrees of freedom
# Null hypothesis probability = 6.555978e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.209e-06 1.324e-07
25- 50 6.101e-06 1.684e-07
50-150 2.142e-05 5.353e-07
15-150 2.973e-05 6.133e-07
Peak spectrum fit
Power-law model
Time interval is from 138.056 sec. to 139.056 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.966001 ( -0.0778721 0.0773949 )
Norm@50keV : 4.77714E-02 ( -0.00211306 0.00211202 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 51.34 using 59 PHA bins.
# Reduced chi-squared = 0.9007 for 57 degrees of freedom
# Null hypothesis probability = 6.864192e-01
Photon flux (15-150 keV) in 1 sec: 5.49144 ( -0.244908 0.245039 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.22955e-07 ( -2.61174e-08 2.61839e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 138.056 sec. to 139.056 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.500760 ( -0.342004 0.316328 )
Epeak [keV] : 185.881 ( -54.9171 249.223 )
Norm@50keV : 7.67773E-02 ( -0.0207001 0.0307 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 44.82 using 59 PHA bins.
# Reduced chi-squared = 0.8004 for 56 degrees of freedom
# Null hypothesis probability = 8.581297e-01
Photon flux (15-150 keV) in 1 sec: 5.38882 ( -0.25467 0.25443 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.1149e-07 ( -2.7867e-08 2.775e-08 ) ergs/cm2
Band function
Time interval is from 138.056 sec. to 139.056 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 4.99997 ( -4.99997 -4.99997 )
beta : -0.983674 ( -0.0811842 0.080822 )
Epeak [keV] : 23.8285 ( -23.8285 5.04406 )
Norm@50keV : 4113.90 ( -180.882 6.86352e+06 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 50.37 using 59 PHA bins.
# Reduced chi-squared = 0.9158 for 55 degrees of freedom
# Null hypothesis probability = 6.518486e-01
Photon flux (15-150 keV) in 1 sec: 5.38965 ( ) 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] : 22.1755 (-1.29187 1.40531)
R^2/D10^2 : 0.195533 (-0.0336574 0.0398744)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 100.79 using 59 PHA bins.
# Reduced chi-squared = 1.7683 for 57 degrees of freedom
# Null hypothesis probability = 3.120523e-04
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.773e-08 1.615e-09
25- 50 9.419e-08 5.935e-09
50-150 3.461e-07 2.650e-08
15-150 4.581e-07 2.630e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.363 ( )
Norm : 21.6140 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 193.34 using 59 PHA bins.
# Reduced chi-squared = 3.3919 for 57 degrees of freedom
# Null hypothesis probability = 9.927930e-17
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.382e-08 2.640e-09
25- 50 1.035e-07 5.595e-09
50-150 2.271e-07 4.325e-08
15-150 3.844e-07 3.110e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.80515 (-1.61473 2.11073)
R1^2/D10^2 : 3.37749 (-1.92429 5.60015)
kT2 [keV] : 29.2271 (-3.18042 4.77886)
R2^2/D10^2 : 7.48298E-02 (-0.0296241 0.0347833)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 43.03 using 59 PHA bins.
# Reduced chi-squared = 0.7824 for 55 degrees of freedom
# Null hypothesis probability = 8.793041e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.454e-08 9.805e-09
25- 50 9.359e-08 1.256e-08
50-150 3.825e-07 4.105e-08
15-150 5.106e-07 5.945e-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: 1.19787 ( -0.0315644 0.031458 )
Norm@50keV : 9.49021E-03 ( -0.000158039 0.000157603 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 27.75 using 59 PHA bins.
# Reduced chi-squared = 0.4869 for 57 degrees of freedom
# Null hypothesis probability = 9.996191e-01
Photon flux (15-150 keV) in 155 sec: 1.11362 ( -0.0206123 0.020712 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.49327e-05 ( -2.40033e-07 2.40163e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.19282 ( -0.0317986 0.0317073 )
Epeak [keV] : 9996.82 ( -9997.51 -9997.51 )
Norm@50keV : 9.53621E-03 ( -0.000156085 0.000688134 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 27.86 using 59 PHA bins.
# Reduced chi-squared = 0.4975 for 56 degrees of freedom
# Null hypothesis probability = 9.994100e-01
Photon flux (15-150 keV) in 155 sec: 1.11294 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 1.48925e-05 ( -2.69375e-07 3.57693e-07 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.639261 ( 0.819895 5.72257 )
beta : -1.19998 ( -0.0341193 0.0325721 )
Epeak [keV] : 59.4277 ( -60.2053 267.599 )
Norm@50keV : 2.48318E-02 ( -0.0156428 0 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 27.50 using 59 PHA bins.
# Reduced chi-squared = 0.5000 for 55 degrees of freedom
# Null hypothesis probability = 9.992946e-01
Photon flux (15-150 keV) in 155 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) = 5.90e-06
S(50-100 keV) = 1.09e-05
T90 vs. Hardness ratio plot
T90 = 179.663999915123 sec.
Hardness ratio (energy fluence ratio) = 1.84746
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.6202
Count Ratio (50-100 keV) / (15-25 keV) = 1.59205
Mask shadow pattern
IMX = -9.116022833228478E-02, IMY = 2.656252137694277E-01
TIME vs. PHA plot around the trigger time
TIME vs. DetID plot around the trigger time
100 us light curve (15-350 keV)
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:
-239.016000 -15.124000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
227.7513 7.2905 3.0 40.6 71.4 2.9745 3.8 ------ UNKNOWN
231.5882 48.6514 2.2 54.2 16.7 5.4234 5.3 ------ UNKNOWN
212.4656 44.7032 2.4 41.7 9.3 1.4665 4.9 ------ UNKNOWN
148.8587 -22.8481 2.4 49.2 -149.9 2.1765 4.8 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-15.124000 139.884590
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
232.6529 42.9948 3.2 52.1 23.4 5.3529 3.6 ------ UNKNOWN
189.0461 -42.5255 2.7 52.0 159.5 5.5157 4.3 ------ UNKNOWN
215.3490 58.1905 3.1 53.4 -0.1 3.4395 3.7 ------ UNKNOWN
170.8828 8.9315 0.1 15.7 -108.9 23.9556 85.8 ------ UNKNOWN
192.3601 59.5283 2.6 50.3 -14.7 2.7196 4.4 ------ UNKNOWN
162.3136 15.4163 2.4 24.6 -91.9 1.6955 4.9 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
264.084590 439.784600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
186.5878 -62.7182 2.7 40.8 -78.9 3.5913 4.2 3.7 GX 301-2
244.9791 -15.6383 0.6 31.7 41.4 5.2342 19.1 0.1 Sco X-1
255.9887 -37.8348 0.6 8.3 64.8 3.1737 18.8 0.6 4U 1700-377
256.6624 -36.3518 5.5 9.9 67.4 0.3761 2.1 11.8 GX 349+2
262.9888 -24.9014 5.5 22.2 79.4 0.4908 2.1 9.4 GX 1+4
264.8556 -44.6463 0.0 7.0 141.3 0.1301 0.7 12.7 4U 1735-44
270.3348 -25.1231 4.4 24.3 95.5 0.6435 2.7 3.8 GX 5-1
270.1825 -25.6387 5.5 23.8 95.8 0.5185 2.2 9.0 GRS 1758-258
273.9379 -14.1192 7.1 35.7 92.7 0.7865 1.6 6.3 GX 17+2
275.9968 -30.4327 4.3 22.5 113.4 0.6266 2.7 5.4 H1820-303
284.9686 -24.9414 42.8 31.9 118.9 -0.0870 -0.3 3.9 HT1900.1-2455
263.1042 -33.8160 3.9 13.7 89.2 0.5502 2.9 5.8 GX 354-0
6.4305 -70.8028 3.2 53.2 -142.1 3.9363 3.6 ------ UNKNOWN
6.6320 -67.5154 4.4 55.3 -145.3 3.9733 2.6 ------ UNKNOWN
186.7600 -36.5756 3.8 50.6 -44.6 2.8618 3.1 ------ UNKNOWN
13.4432 -82.0456 2.6 48.0 -129.1 3.5699 4.6 ------ UNKNOWN
Plot creation:
Sat May 30 19:23:06 EDT 2015