Click here for the BAT GCN circular template
Image
Pre-slew 15.0-350.0 keV image (Event data)
# RAcent DECcent POSerr Theta Phi Peak Cts SNR Name
232.1136 37.7520 0.0139 40.8985 -179.4794 1.1947861 13.800 TRIG_00582773
Foreground time interval of the image:
-12.520 6.936 (delta_t = 19.456 [sec])
Background time interval of the image:
-239.784 -12.520 (delta_t = 227.264 [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)
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 -12.520 sec. to 6.936 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.59077 ( -0.207026 0.224923 )
Norm@50keV : 3.00049E-03 ( -0.00049058 0.000487272 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 74.95 using 59 PHA bins.
# Reduced chi-squared = 1.315 for 57 degrees of freedom
# Null hypothesis probability = 5.564742e-02
Photon flux (15-150 keV) in 19.46 sec: 0.623802 ( -0.0616014 0.0616122 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.99308e-07 ( -6.96433e-08 7.13828e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -12.520 sec. to 6.936 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.43342 ( -1.27403 0.673343 )
Epeak [keV] : 17.3478 ( )
Norm@50keV : 1.62416E-02 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 70.61 using 59 PHA bins.
# Reduced chi-squared = 1.261 for 56 degrees of freedom
# Null hypothesis probability = 9.053276e-02
Photon flux (15-150 keV) in 19.46 sec: 0.603468 ( -0.063292 0.063532 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.47079e-07 ( -7.1064e-08 7.91205e-08 ) ergs/cm2
Band function
Time interval is from -12.520 sec. to 6.936 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.43315 ( -0.629062 1.56593 )
beta : -10.0000 ( 10 3.55271e-15 )
Epeak [keV] : 17.3477 ( -9.25697 10.2618 )
Norm@50keV : 1.62461E-02 ( -0.0101003 0.0941778 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 70.61 using 59 PHA bins.
# Reduced chi-squared = 1.284 for 55 degrees of freedom
# Null hypothesis probability = 7.649436e-02
Photon flux (15-150 keV) in 19.46 sec: 0.603467 ( 6.39653 -0.063087 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.50683e-07 ( 0 0 ) ergs/cm2
Single BB
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 7.20476 (-0.775678 0.853337)
R^2/D10^2 : 1.02204 (-0.385464 0.640378)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 82.23 using 59 PHA bins.
# Reduced chi-squared = 1.443 for 57 degrees of freedom
# Null hypothesis probability = 1.600216e-02
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.707e-07 2.719e-08
25- 50 2.471e-07 3.376e-08
50-150 4.540e-08 1.721e-08
15-150 4.632e-07 5.780e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 29.5962 (-6.04172 8.03971)
Norm : 5.04384 (-1.0104 1.3421)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 70.63 using 59 PHA bins.
# Reduced chi-squared = 1.239 for 57 degrees of freedom
# Null hypothesis probability = 1.060111e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.984e-07 2.660e-08
25- 50 2.250e-07 2.735e-08
50-150 1.210e-07 4.374e-08
15-150 5.444e-07 6.996e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 3.97776 (-1.60198 1.91896)
R1^2/D10^2 : 7.95257 (-6.05565 94.5959)
kT2 [keV] : 10.6141 (-2.50359 7.02593)
R2^2/D10^2 : 0.141766 (-0.130926 0.380741)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 70.75 using 59 PHA bins.
# Reduced chi-squared = 1.286 for 55 degrees of freedom
# Null hypothesis probability = 7.490353e-02
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.014e-07 1.056e-07
25- 50 2.225e-07 1.143e-07
50-150 1.081e-07 6.314e-08
15-150 5.320e-07 2.697e-07
Peak spectrum fit
Power-law model
Time interval is from 0.388 sec. to 1.388 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.56819 ( -0.271983 0.306123 )
Norm@50keV : 1.01065E-02 ( -0.00226477 0.00223574 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 58.24 using 59 PHA bins.
# Reduced chi-squared = 1.022 for 57 degrees of freedom
# Null hypothesis probability = 4.294959e-01
Photon flux (15-150 keV) in 1 sec: 2.07131 ( -0.28347 0.283481 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.0303e-07 ( -1.66852e-08 1.71951e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.388 sec. to 1.388 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.64695 ( -1.36602 0.347179 )
Epeak [keV] : 14.1385 ( )
Norm@50keV : 3.80409E-02 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 56.01 using 59 PHA bins.
# Reduced chi-squared = 1.000 for 56 degrees of freedom
# Null hypothesis probability = 4.745412e-01
Photon flux (15-150 keV) in 1 sec: 2.03457 ( -0.28449 0.28516 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.69908e-08 ( -1.65488e-08 1.79932e-08 ) ergs/cm2
Band function
Time interval is from 0.388 sec. to 1.388 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.65313 ( -0.440609 1.66065 )
beta : -10.0000 ( 10 1.06581e-14 )
Epeak [keV] : 13.9908 ( -10.2166 15.8073 )
Norm@50keV : 3.76828E-02 ( -0.0197054 0.253216 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 56.01 using 59 PHA bins.
# Reduced chi-squared = 1.018 for 55 degrees of freedom
# Null hypothesis probability = 4.367886e-01
Photon flux (15-150 keV) in 1 sec: 2.03389 ( 4.96611 -0.2791 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.87492e-08 ( -9.87422e-08 -1.87811e-08 ) ergs/cm2
Single BB
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 7.10499 (-1.1892 1.41791)
R^2/D10^2 : 3.62198 (-1.91956 4.27875)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 66.49 using 59 PHA bins.
# Reduced chi-squared = 1.167 for 57 degrees of freedom
# Null hypothesis probability = 1.825818e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.982e-08 7.775e-09
25- 50 4.203e-08 9.230e-09
50-150 7.348e-09 3.659e-09
15-150 7.920e-08 1.601e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 31.3134 (-8.51348 12.3898)
Norm : 16.1175 (-4.10905 6.02008)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 56.19 using 59 PHA bins.
# Reduced chi-squared = 0.9858 for 57 degrees of freedom
# Null hypothesis probability = 5.055121e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.351e-08 5.835e-09
25- 50 3.919e-08 7.925e-09
50-150 2.269e-08 9.925e-09
15-150 9.538e-08 1.756e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 4.23768 (-1.26349 1.4408)
R1^2/D10^2 : 23.7333 (-16.6512 32.2466)
kT2 [keV] : 12.9409 (-3.52255 6.10326)
R2^2/D10^2 : 0.199146 (-0.166234 0.371071)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 54.43 using 59 PHA bins.
# Reduced chi-squared = 0.9896 for 55 degrees of freedom
# Null hypothesis probability = 4.964922e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.543e-08 1.886e-08
25- 50 3.628e-08 1.894e-08
50-150 2.580e-08 1.618e-08
15-150 9.751e-08 5.025e-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: 2.59077 ( -0.207026 0.224923 )
Norm@50keV : 3.00049E-03 ( -0.00049058 0.000487272 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 74.95 using 59 PHA bins.
# Reduced chi-squared = 1.315 for 57 degrees of freedom
# Null hypothesis probability = 5.564742e-02
Photon flux (15-150 keV) in 19.46 sec: 0.623802 ( -0.0616014 0.0616122 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.99308e-07 ( -6.96433e-08 7.13828e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.43342 ( -1.27403 0.673343 )
Epeak [keV] : 17.3478 ( )
Norm@50keV : 1.62416E-02 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 70.61 using 59 PHA bins.
# Reduced chi-squared = 1.261 for 56 degrees of freedom
# Null hypothesis probability = 9.053276e-02
Photon flux (15-150 keV) in 19.46 sec: 0.603468 ( -0.063292 0.063532 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.47079e-07 ( -7.1064e-08 7.91205e-08 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.43315 ( -0.629062 1.56593 )
beta : -10.0000 ( 10 20 )
Epeak [keV] : 17.3477 ( -9.25704 10.2618 )
Norm@50keV : 1.62461E-02 ( -0.0101003 0.0941778 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 70.61 using 59 PHA bins.
# Reduced chi-squared = 1.284 for 55 degrees of freedom
# Null hypothesis probability = 7.649436e-02
Photon flux (15-150 keV) in 19.46 sec: 0.603467 ( 6.39653 -0.063087 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.50683e-07 ( 0 0 ) ergs/cm2
S(25-50 keV) vs. S(50-100 keV) plot
S(25-50 keV) = 2.00e-07
S(50-100 keV) = 1.33e-07
T90 vs. Hardness ratio plot
T90 = 17.3440000414848 sec.
Hardness ratio (energy fluence ratio) = 0.665
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 0.895891
Count Ratio (50-100 keV) / (15-25 keV) = 0.215491
Mask shadow pattern
IMX = -8.661470603614726E-01, IMY = 7.870336004790913E-03
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:
-239.784000 -12.520000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
244.9631 -15.6434 1.0 36.8 -85.4 6.5091 11.7 1.0 Sco X-1
254.5387 35.4169 18.1 52.2 -159.8 -0.3356 -0.6 6.0 Her X-1
177.7019 24.3825 3.7 40.3 103.5 2.6127 3.1 ------ UNKNOWN
221.8412 24.3711 2.2 25.0 177.7 1.0746 5.4 ------ UNKNOWN
244.9435 -24.5088 2.1 41.1 -73.1 4.3263 5.4 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-12.520000 6.936000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
244.7985 -15.7084 3.4 36.7 -85.2 0.4236 3.4 11.2 Sco X-1
254.5175 35.3039 7.4 52.1 -159.7 -0.2213 -1.6 3.7 Her X-1
232.1135 37.7520 0.8 40.9 -179.5 1.1950 13.8 ------ UNKNOWN
248.1213 10.8695 3.2 37.2 -130.5 0.2874 3.7 ------ UNKNOWN
226.2791 -38.4336 2.3 41.9 -41.1 0.4786 5.0 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
152.516590 962.317400
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.4108 35.1336 0.0 18.1 -130.7 0.6294 1.1 12.7 Her X-1
299.5950 35.2671 3.4 53.1 -151.5 6.9262 3.4 3.9 Cyg X-1
308.1234 40.9956 60.2 56.9 -161.2 -0.5900 -0.2 2.6 Cyg X-3
250.6422 56.7981 4.0 22.7 164.7 1.4805 2.9 ------ UNKNOWN
207.8122 -4.5955 2.6 48.0 -8.7 4.2442 4.3 ------ UNKNOWN
Plot creation:
Sat May 30 14:44:48 EDT 2015