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
86.9305 82.9109 0.0088 18.6644 -22.1108 3.4578330 21.865 TRIG_00557274
Foreground time interval of the image:
-20.812 104.980 (delta_t = 125.792 [sec])
Background time interval of the image:
-590.195 -572.306 (delta_t = 17.890 [sec])
-239.296 -20.812 (delta_t = 218.484 [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 8.192000
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 8.192000
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 8.192000
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 -20.812 sec. to 104.980 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.83538 ( -0.119303 0.122132 )
Norm@50keV : 1.64484E-03 ( -0.000115207 0.000113692 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 40.94 using 59 PHA bins.
# Reduced chi-squared = 0.7182 for 57 degrees of freedom
# Null hypothesis probability = 9.463526e-01
Photon flux (15-150 keV) in 125.8 sec: 0.229839 ( -0.0140227 0.0140501 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.90306e-06 ( -1.33903e-07 1.35541e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -20.812 sec. to 104.980 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.70516 ( -0.46928 0.246063 )
Epeak [keV] : 104.229 ( )
Norm@50keV : 1.93030E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 40.68 using 59 PHA bins.
# Reduced chi-squared = 0.7264 for 56 degrees of freedom
# Null hypothesis probability = 9.384025e-01
Photon flux (15-150 keV) in 125.8 sec: 0.227935 ( -0.015277 0.01511 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.87754e-06 ( -1.58822e-07 1.54759e-07 ) ergs/cm2
Band function
Time interval is from -20.812 sec. to 104.980 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.60901 ( -4.6296 0.384925 )
beta : -8.58710 ( 9.01086 19.0109 )
Epeak [keV] : 81.6978 ( -30.4436 -81.6978 )
Norm@50keV : 2.15805E-03 ( -0.000128875 0.00109755 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 40.80 using 59 PHA bins.
# Reduced chi-squared = 0.7418 for 55 degrees of freedom
# Null hypothesis probability = 9.231620e-01
Photon flux (15-150 keV) in 125.8 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] : 11.6462 (-0.931951 1.02739)
R^2/D10^2 : 5.83116E-02 (-0.0156862 0.0212918)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 108.41 using 59 PHA bins.
# Reduced chi-squared = 1.9020 for 57 degrees of freedom
# Null hypothesis probability = 4.778200e-05
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.098e-07 2.283e-08
25- 50 6.371e-07 4.611e-08
50-150 5.090e-07 7.982e-08
15-150 1.356e-06 9.800e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 98.0235 (-21.2559 32.2584)
Norm : 1.00401 (-0.0878385 0.101796)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 42.85 using 59 PHA bins.
# Reduced chi-squared = 0.7518 for 57 degrees of freedom
# Null hypothesis probability = 9.177863e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.301e-07 3.472e-08
25- 50 5.685e-07 4.296e-08
50-150 9.108e-07 2.907e-07
15-150 1.809e-06 3.013e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.59045 (-1.21094 1.29604)
R1^2/D10^2 : 0.625993 (-0.330746 1.05706)
kT2 [keV] : 20.9126 (-3.70739 5.67039)
R2^2/D10^2 : 5.33129E-03 (-0.00315096 0.00608872)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 43.56 using 59 PHA bins.
# Reduced chi-squared = 0.7920 for 55 degrees of freedom
# Null hypothesis probability = 8.669534e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.488e-07 9.573e-08
25- 50 5.344e-07 1.084e-07
50-150 9.443e-07 2.374e-07
15-150 1.827e-06 3.898e-07
Peak spectrum fit
Power-law model
Time interval is from 11.268 sec. to 12.268 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.46054 ( -0.335075 0.341095 )
Norm@50keV : 6.06180E-03 ( -0.00122674 0.00120385 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 55.40 using 59 PHA bins.
# Reduced chi-squared = 0.9719 for 57 degrees of freedom
# Null hypothesis probability = 5.353561e-01
Photon flux (15-150 keV) in 1 sec: 0.749005 ( -0.14241 0.142482 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.78956e-08 ( -1.28963e-08 1.32718e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 11.268 sec. to 12.268 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.25464 ( -1.43315 1.39582 )
Epeak [keV] : 171.372 ( -172.222 -172.222 )
Norm@50keV : 7.80331E-03 ( -0.00779484 0.0364665 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 55.31 using 59 PHA bins.
# Reduced chi-squared = 0.9876 for 56 degrees of freedom
# Null hypothesis probability = 5.010486e-01
Photon flux (15-150 keV) in 1 sec: 0.742935 ( -0.146538 0.145956 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.67554e-08 ( -1.45043e-08 1.41401e-08 ) ergs/cm2
Band function
Time interval is from 11.268 sec. to 12.268 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 4.77936 ( -4.77936 -4.77936 )
beta : -1.60211 ( -0.464747 0.397069 )
Epeak [keV] : 26.0574 ( -26.0574 105.628 )
Norm@50keV : 345.633 ( -65.0946 3.58619e+06 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 54.68 using 59 PHA bins.
# Reduced chi-squared = 0.9942 for 55 degrees of freedom
# Null hypothesis probability = 4.867322e-01
Photon flux (15-150 keV) in 1 sec: 0.738867 ( ) 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] : 14.1900 (-3.41867 4.8181)
R^2/D10^2 : 0.102428 (-0.0648935 0.166973)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 62.56 using 59 PHA bins.
# Reduced chi-squared = 1.097 for 57 degrees of freedom
# Null hypothesis probability = 2.855357e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.351e-09 1.776e-09
25- 50 1.640e-08 5.743e-09
50-150 2.189e-08 1.075e-08
15-150 4.264e-08 1.498e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.359 (-106.81 -199.363)
Norm : 3.06333 (-0.579704 0.580213)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 55.46 using 59 PHA bins.
# Reduced chi-squared = 0.9731 for 57 degrees of freedom
# Null hypothesis probability = 5.328912e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.628e-09 4.472e-09
25- 50 1.467e-08 8.465e-09
50-150 3.218e-08 1.834e-08
15-150 5.448e-08 3.089e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.38457 (-2.72164 4.59281)
R1^2/D10^2 : 1.09610 (-0.899467 7.84078)
kT2 [keV] : 26.3903 (-10.2052 89.0562)
R2^2/D10^2 : 9.87810E-03 (-0.00956745 0.0525948)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 54.70 using 59 PHA bins.
# Reduced chi-squared = 0.9946 for 55 degrees of freedom
# Null hypothesis probability = 4.860176e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.617e-09 4.427e-09
25- 50 1.411e-08 7.490e-09
50-150 3.545e-08 2.121e-08
15-150 5.717e-08 3.015e-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: 1.83538 ( -0.119303 0.122132 )
Norm@50keV : 1.64484E-03 ( -0.000115207 0.000113692 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 40.94 using 59 PHA bins.
# Reduced chi-squared = 0.7182 for 57 degrees of freedom
# Null hypothesis probability = 9.463526e-01
Photon flux (15-150 keV) in 125.8 sec: 0.229839 ( -0.0140227 0.0140501 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.90306e-06 ( -1.33903e-07 1.35541e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.70516 ( -0.46928 0.246063 )
Epeak [keV] : 104.229 ( )
Norm@50keV : 1.93030E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 40.68 using 59 PHA bins.
# Reduced chi-squared = 0.7264 for 56 degrees of freedom
# Null hypothesis probability = 9.384025e-01
Photon flux (15-150 keV) in 125.8 sec: 0.227935 ( -0.015277 0.01511 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.87754e-06 ( -1.58822e-07 1.54759e-07 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.60901 ( -4.6296 0.384925 )
beta : -8.58710 ( 9.01086 19.0109 )
Epeak [keV] : 81.6978 ( -30.4436 -81.6978 )
Norm@50keV : 2.15805E-03 ( -0.000128875 0.00109755 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 40.80 using 59 PHA bins.
# Reduced chi-squared = 0.7418 for 55 degrees of freedom
# Null hypothesis probability = 9.231620e-01
Photon flux (15-150 keV) in 125.8 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) = 5.43e-07
S(50-100 keV) = 6.08e-07
T90 vs. Hardness ratio plot
T90 = 69.1279999613762 sec.
Hardness ratio (energy fluence ratio) = 1.11971
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.01932
Count Ratio (50-100 keV) / (15-25 keV) = 0.642686
Mask shadow pattern
IMX = 3.129479552960023E-01, IMY = 1.271434766404723E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 8.192000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 8.192000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 8.192000
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:
-590.195400 -572.305500
-239.296000 -20.812000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
196.9250 37.2128 2.4 40.8 113.9 3.7648 4.8 ------ UNKNOWN
169.7399 61.6142 2.1 11.2 119.8 1.0585 5.7 ------ UNKNOWN
168.5712 61.8390 2.6 10.7 121.3 0.8967 4.7 ------ UNKNOWN
346.4959 83.0952 2.3 27.6 -6.5 1.0157 5.1 ------ UNKNOWN
111.7924 23.3483 2.6 51.0 -135.9 4.3694 4.4 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-20.812000 104.980000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
86.9305 82.9109 0.5 18.7 -22.1 3.4582 21.9 ------ UNKNOWN
121.8799 59.1287 2.2 15.4 -118.7 0.7968 5.3 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
344.804590 496.904600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
170.1432 -60.5149 173.0 43.8 -155.5 -0.0201 -0.1 8.2 Cen X-3
186.4523 -62.6909 5.8 40.8 -166.6 0.4822 2.0 7.4 GX 301-2
244.9570 -15.6270 1.2 38.6 86.1 7.6527 9.9 1.5 Sco X-1
235.8238 13.5614 2.0 48.1 43.0 4.8775 5.7 ------ UNKNOWN
227.9613 5.5757 2.4 37.1 41.2 1.5574 4.9 ------ UNKNOWN
223.5443 -62.8885 2.2 41.1 167.8 1.4637 5.2 ------ UNKNOWN
218.8327 -77.4069 3.1 54.1 176.9 2.4893 3.8 ------ UNKNOWN
141.9307 -70.7246 3.6 58.8 -159.3 3.2651 3.2 ------ UNKNOWN
159.5224 -24.0094 3.5 41.2 -99.2 2.8985 3.3 ------ UNKNOWN
Plot creation:
Sat May 30 16:42:41 EDT 2015