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
220.0414 -0.1646 0.0103 27.7807 158.1826 2.2877529 18.593 TRIG_00305288
Foreground time interval of the image:
-52.979 18.421 (delta_t = 71.400 [sec])
Background time interval of the image:
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 -71.764 sec. to 318.396 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.21769 ( -0.143073 0.148643 )
Norm@50keV : 6.27201E-04 ( -6.1967e-05 6.12051e-05 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 54.52 using 59 PHA bins.
# Reduced chi-squared = 0.9565 for 57 degrees of freedom
# Null hypothesis probability = 5.686496e-01
Photon flux (15-150 keV) in 390.2 sec: 0.104811 ( -0.00744758 0.00745144 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.3069e-06 ( -1.93304e-07 1.96934e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -71.764 sec. to 318.396 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.64949 ( -0.753899 0.355382 )
Epeak [keV] : 23.3019 ( -21.5723 11.3558 )
Norm@50keV : 1.39310E-03 ( -0.000606137 0.00269357 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 51.93 using 59 PHA bins.
# Reduced chi-squared = 0.9273 for 56 degrees of freedom
# Null hypothesis probability = 6.297710e-01
Photon flux (15-150 keV) in 390.2 sec: 0.102044 ( -0.0079718 0.007972 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.14558e-06 ( -2.42018e-07 2.56408e-07 ) ergs/cm2
Band function
Time interval is from -71.764 sec. to 318.396 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.65351 ( 1.70188 0.268192 )
beta : -10.0000 ( 10 3.55271e-15 )
Epeak [keV] : 23.2450 ( -10.9978 11.4153 )
Norm@50keV : 1.38350E-03 ( -0.000606405 0.00270555 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 51.93 using 59 PHA bins.
# Reduced chi-squared = 0.9441 for 55 degrees of freedom
# Null hypothesis probability = 5.928107e-01
Photon flux (15-150 keV) in 390.2 sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 2.21306e-06 ( -2.21033e-06 -2.07032e-07 ) ergs/cm2
Single BB
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 8.19710 (-0.643809 0.70828)
R^2/D10^2 : 0.101087 (-0.0291169 0.040529)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 78.85 using 59 PHA bins.
# Reduced chi-squared = 1.383 for 57 degrees of freedom
# Null hypothesis probability = 2.924935e-02
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.877e-07 5.424e-08
25- 50 8.900e-07 7.745e-08
50-150 2.530e-07 5.781e-08
15-150 1.631e-06 1.426e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 44.8161 (-8.15695 11.3333)
Norm : 0.624090 (-0.0853242 0.102215)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 52.38 using 59 PHA bins.
# Reduced chi-squared = 0.9190 for 57 degrees of freedom
# Null hypothesis probability = 6.487165e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.791e-07 5.521e-08
25- 50 7.984e-07 5.736e-08
50-150 6.964e-07 1.551e-07
15-150 2.074e-06 1.846e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.25886 (-0.953828 0.896356)
R1^2/D10^2 : 0.250886 (-0.0981616 0.179129)
kT2 [keV] : 23.6024 (-7.34327 14.7065)
R2^2/D10^2 : 9.15596E-04 (-0.000735566 0.00310936)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 47.63 using 59 PHA bins.
# Reduced chi-squared = 0.8659 for 55 degrees of freedom
# Null hypothesis probability = 7.495029e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.757e-07 1.073e-07
25- 50 7.857e-07 1.576e-07
50-150 8.785e-07 4.625e-07
15-150 2.240e-06 6.278e-07
Peak spectrum fit
Power-law model
Time interval is from 1.272 sec. to 2.272 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.91347 ( -0.225619 0.239108 )
Norm@50keV : 9.16071E-03 ( -0.00146898 0.00143629 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 58.39 using 59 PHA bins.
# Reduced chi-squared = 1.024 for 57 degrees of freedom
# Null hypothesis probability = 4.240407e-01
Photon flux (15-150 keV) in 1 sec: 1.32223 ( -0.174685 0.174736 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.42345e-08 ( -1.30272e-08 1.33243e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 1.272 sec. to 2.272 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.718411 ( -1.57435 1.10878 )
Epeak [keV] : 43.8149 ( -11.6548 43.8068 )
Norm@50keV : 4.58292E-02 ( -0.0458618 0.356413 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 54.96 using 59 PHA bins.
# Reduced chi-squared = 0.9813 for 56 degrees of freedom
# Null hypothesis probability = 5.144269e-01
Photon flux (15-150 keV) in 1 sec: 1.27429 ( -0.17872 0.18041 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.52084e-08 ( -1.40005e-08 1.54991e-08 ) ergs/cm2
Band function
Time interval is from 1.272 sec. to 2.272 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.272514 ( -1.40835 0.252156 )
beta : -2.60450 ( 2.60945 0.697876 )
Epeak [keV] : 39.5757 ( -16.6717 18.0519 )
Norm@50keV : 9.14630E-02 ( -0.109074 435.058 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 54.13 using 59 PHA bins.
# Reduced chi-squared = 0.9841 for 55 degrees of freedom
# Null hypothesis probability = 5.079905e-01
Photon flux (15-150 keV) in 1 sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 7.74631e-08 ( -7.74561e-08 -1.40834e-08 ) ergs/cm2
Single BB
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 10.1864 (-1.34981 1.57968)
R^2/D10^2 : 0.597838 (-0.254439 0.430692)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 59.99 using 59 PHA bins.
# Reduced chi-squared = 1.052 for 57 degrees of freedom
# Null hypothesis probability = 3.679016e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.271e-08 2.859e-09
25- 50 3.243e-08 5.525e-09
50-150 1.785e-08 6.574e-09
15-150 6.299e-08 1.140e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 72.7104 (-23.9794 46.1942)
Norm : 6.48855 (-1.21354 1.48574)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 55.58 using 59 PHA bins.
# Reduced chi-squared = 0.9751 for 57 degrees of freedom
# Null hypothesis probability = 5.285459e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.671e-08 3.165e-09
25- 50 2.686e-08 4.130e-09
50-150 3.547e-08 1.595e-08
15-150 7.904e-08 1.503e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 8.10322 (-5.04219 2.33672)
R1^2/D10^2 : 1.16427 (-0.565302 22.9107)
kT2 [keV] : 27.4887 (-13.438 -28.6503)
R2^2/D10^2 : 6.57590E-03 (-0.00565697 0.407591)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 54.54 using 59 PHA bins.
# Reduced chi-squared = 0.9917 for 55 degrees of freedom
# Null hypothesis probability = 4.921198e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.477e-08 7.929e-09
25- 50 2.983e-08 1.490e-08
50-150 3.356e-08 1.918e-08
15-150 7.817e-08 3.780e-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: 1.91413 ( -0.143621 0.148152 )
Norm@50keV : 1.77398E-03 ( -0.00016398 0.000161585 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 61.28 using 59 PHA bins.
# Reduced chi-squared = 1.075 for 57 degrees of freedom
# Null hypothesis probability = 3.252721e-01
Photon flux (15-150 keV) in 71.4 sec: 0.256126 ( -0.0200259 0.0200444 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.16467e-06 ( -1.04697e-07 1.06223e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.23226 ( -0.693647 0.589504 )
Epeak [keV] : 48.6086 ( -11.2904 38.808 )
Norm@50keV : 4.27189E-03 ( -0.00223582 0.00614066 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 57.28 using 59 PHA bins.
# Reduced chi-squared = 1.023 for 56 degrees of freedom
# Null hypothesis probability = 4.275346e-01
Photon flux (15-150 keV) in 71.4 sec: 0.247718 ( -0.021224 0.021231 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.08585e-06 ( -1.19709e-07 1.24036e-07 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.23223 ( -0.498323 0.792744 )
beta : -10.0000 ( 10 1.77636e-15 )
Epeak [keV] : 48.5989 ( -11.2865 26.4298 )
Norm@50keV : 4.27161E-03 ( -0.00198177 0.00615209 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 57.28 using 59 PHA bins.
# Reduced chi-squared = 1.041 for 55 degrees of freedom
# Null hypothesis probability = 3.906768e-01
Photon flux (15-150 keV) in 71.4 sec: 0.248958 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 1.08715e-06 ( 0 0 ) ergs/cm2
S(25-50 keV) vs. S(50-100 keV) plot
S(25-50 keV) = 7.33e-07
S(50-100 keV) = 6.31e-07
T90 vs. Hardness ratio plot
T90 = 363.212000012398 sec.
Hardness ratio (energy fluence ratio) = 0.860846
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 0.947645
Count Ratio (50-100 keV) / (15-25 keV) = 0.376563
Mask shadow pattern
IMX = -4.890763693368319E-01, IMY = -1.957889539151486E-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:
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-52.979410 18.420600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
170.2158 -60.7081 7.0 44.2 -8.3 0.2835 1.7 5.9 Cen X-3
187.0917 -62.7880 5.3 39.5 -18.4 0.3002 2.2 12.0 GX 301-2
244.9760 -15.6467 0.3 31.7 -141.5 4.0246 34.3 0.4 Sco X-1
256.0170 -37.9750 6.0 37.4 -98.9 0.4711 1.9 8.0 4U 1700-377
256.2837 -36.2926 5.7 37.5 -101.7 0.5144 2.0 10.7 GX 349+2
263.0094 -24.7461 78.5 44.6 -118.2 -0.0566 -0.1 0.0 GX 1+4
220.0414 -0.1646 0.6 27.8 158.2 2.2880 18.6 ------ UNKNOWN
226.0544 2.7072 2.2 32.3 167.9 0.6764 5.3 ------ UNKNOWN
248.8935 -69.3576 2.7 47.1 -53.2 1.7976 4.3 ------ UNKNOWN
263.4887 -18.9675 2.4 46.8 -125.7 1.9235 4.7 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
77.820590 962.786400
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
244.9716 -15.6393 0.2 29.0 -61.7 51.3216 70.9 0.5 Sco X-1
254.4613 35.2392 5.0 47.8 -146.6 3.1228 2.3 6.2 Her X-1
256.0191 -37.8089 3.5 50.1 -42.3 7.4219 3.3 2.6 4U 1700-377
256.4638 -36.4250 9.8 49.5 -44.0 2.5532 1.2 1.4 GX 349+2
189.4888 25.4800 4.4 39.1 128.2 4.3322 2.6 ------ UNKNOWN
220.1032 -0.1698 1.9 0.0 -131.1 3.1295 6.1 ------ UNKNOWN
229.4442 -58.2514 2.3 58.5 -10.8 15.2502 5.0 ------ UNKNOWN
261.0784 -1.7162 3.0 41.0 -92.7 10.2816 3.9 ------ UNKNOWN
Plot creation:
Sun May 31 08:10:05 EDT 2015