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Image
Pre-slew 15.0-350.0 keV image (Event data)
# RAcent DECcent POSerr Theta Phi Peak Cts SNR Name
10.0692 -63.1812 0.0045 34.9501 -46.4975 21.9194497 42.408 TRIG_00630019
Foreground time interval of the image:
-13.699 389.664 (delta_t = 403.363 [sec])
Background time interval of the image:
Lightcurves
Notes:
- 1) All plots contain as much data as has been downloaded to date.
- 2) The mask-weighted light curves are using the flight position.
- 3) Multiple plots of different time binning/intervals are shown to cover all scenarios of short/long GRBs, rate/image triggers, and real/false positives.
- 4) 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.
- 5) 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.
- 6) 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 64.000000
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 64.000000
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 64.000000
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) For long bursts, a spectral fit of 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.
- 4) For short bursts (T90<1sec), the specrtum is also fit with Blackbody, OTTB, and Double Blackbody.
Time averaged spectrum fit using the pre-slew DRM
Power-law model
Time interval is from -22.252 sec. to 389.664 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.33698 ( -0.0479666 0.0477609 )
Norm@50keV : 3.67437E-03 ( -9.41332e-05 9.40437e-05 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 52.22 using 59 PHA bins.
# Reduced chi-squared = 0.9161 for 57 degrees of freedom
# Null hypothesis probability = 6.547072e-01
Photon flux (15-150 keV) in 411.9 sec: 0.441488 ( -0.0126228 0.0126629 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.48255e-05 ( -3.89895e-07 3.90209e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -22.252 sec. to 389.664 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.16078 ( -0.192315 0.0953506 )
Epeak [keV] : 275.321 ( -112.838 -275.321 )
Norm@50keV : 4.38647E-03 ( -0.000619909 0.00090437 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 49.56 using 59 PHA bins.
# Reduced chi-squared = 0.8849 for 56 degrees of freedom
# Null hypothesis probability = 7.157514e-01
Photon flux (15-150 keV) in 411.9 sec: 0.435865 ( -0.013797 0.013844 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.46893e-05 ( -4.19561e-07 4.18078e-07 ) ergs/cm2
Band function
Time interval is from -22.252 sec. to 389.664 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 1.74234 ( -3.41365 -0.983128 )
beta : -1.36765 ( -0.059065 0.0562262 )
Epeak [keV] : 30.6897 ( -11.0137 118.867 )
Norm@50keV : 0.675582 ( -0.675865 108.177 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 47.97 using 59 PHA bins.
# Reduced chi-squared = 0.8722 for 55 degrees of freedom
# Null hypothesis probability = 7.377990e-01
Photon flux (15-150 keV) in 411.9 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] : 19.4084 ( )
R^2/D10^2 : 2.09122E-02 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 338.81 using 59 PHA bins.
# Reduced chi-squared = 5.9440 for 57 degrees of freedom
# Null hypothesis probability = 1.101807e-41
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.328e-07 3.357e-08
25- 50 3.089e-06 1.265e-07
50-150 8.585e-06 3.460e-07
15-150 1.231e-05 3.645e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.363 ( )
Norm : 1.87869 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 125.96 using 59 PHA bins.
# Reduced chi-squared = 2.2098 for 57 degrees of freedom
# Null hypothesis probability = 4.060396e-07
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.927e-06 5.602e-08
25- 50 3.707e-06 1.083e-07
50-150 8.129e-06 2.430e-07
15-150 1.376e-05 3.892e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.47209 (-0.742258 0.824261)
R1^2/D10^2 : 0.318249 (-0.0947396 0.143366)
kT2 [keV] : 29.7070 (-2.347 3.01434)
R2^2/D10^2 : 4.24911E-03 (-0.00119778 0.00142158)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 49.35 using 59 PHA bins.
# Reduced chi-squared = 0.8973 for 55 degrees of freedom
# Null hypothesis probability = 6.893437e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.495e-06 1.664e-07
25- 50 3.433e-06 2.136e-07
50-150 9.750e-06 5.396e-07
15-150 1.468e-05 7.455e-07
Peak spectrum fit
Power-law model
Time interval is from 0.000 sec. to 0.000 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.12129 ( -0.0677749 0.0675631 )
Norm@50keV : 8.65484E-02 ( -0.00333714 0.00333618 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 56.60 using 59 PHA bins.
# Reduced chi-squared = 0.9931 for 57 degrees of freedom
# Null hypothesis probability = 4.898917e-01
Photon flux (15-150 keV) in 1 sec: 10.0608 ( -0.4008 0.40119 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.98824e-07 ( -3.78769e-08 3.79587e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.000 sec. to 0.000 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.834430 ( -0.28013 0.259973 )
Epeak [keV] : 234.260 ( -87.5664 1414.53 )
Norm@50keV : 0.116145 ( -0.0260213 0.0372644 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 53.13 using 59 PHA bins.
# Reduced chi-squared = 0.9488 for 56 degrees of freedom
# Null hypothesis probability = 5.840350e-01
Photon flux (15-150 keV) in 1 sec: 9.93598 ( -0.41569 0.41612 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.88567e-07 ( -3.975e-08 3.9566e-08 ) ergs/cm2
Band function
Time interval is from 0.000 sec. to 0.000 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.825846 ( -0.262688 0.573738 )
beta : -1.42980 ( 1.44817 0.334604 )
Epeak [keV] : 226.208 ( -110.769 1332.17 )
Norm@50keV : 0.117486 ( -0.0222199 0.351044 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 53.10 using 59 PHA bins.
# Reduced chi-squared = 0.9655 for 55 degrees of freedom
# Null hypothesis probability = 5.474014e-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] : 20.7111 ( )
R^2/D10^2 : 0.424842 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 164.07 using 59 PHA bins.
# Reduced chi-squared = 2.8785 for 57 degrees of freedom
# Null hypothesis probability = 2.643684e-12
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.463e-08 2.605e-09
25- 50 1.765e-07 9.750e-09
50-150 5.635e-07 3.850e-08
15-150 7.746e-07 3.600e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.363 ( )
Norm : 41.5929 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 166.86 using 59 PHA bins.
# Reduced chi-squared = 2.9273 for 57 degrees of freedom
# Null hypothesis probability = 1.035135e-12
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.036e-07 4.340e-09
25- 50 1.992e-07 7.750e-09
50-150 4.370e-07 1.920e-08
15-150 7.397e-07 3.265e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 8.15835 (-1.38157 1.60313)
R1^2/D10^2 : 4.49992 (-1.83543 3.65189)
kT2 [keV] : 32.1172 (-3.93855 6.12543)
R2^2/D10^2 : 8.81877E-02 (-0.0386351 0.0495685)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 54.81 using 59 PHA bins.
# Reduced chi-squared = 0.9966 for 55 degrees of freedom
# Null hypothesis probability = 4.817691e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.857e-08 1.086e-08
25- 50 1.858e-07 2.130e-08
50-150 6.389e-07 8.215e-08
15-150 8.933e-07 1.049e-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: 1.33079 ( -0.0477297 0.0475185 )
Norm@50keV : 3.72762E-03 ( -9.51796e-05 9.5119e-05 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 55.81 using 59 PHA bins.
# Reduced chi-squared = 0.9791 for 57 degrees of freedom
# Null hypothesis probability = 5.198996e-01
Photon flux (15-150 keV) in 403.4 sec: 0.447336 ( -0.0127408 0.0127802 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.4751e-05 ( -3.86356e-07 3.86651e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.14895 ( -0.192139 0.0950824 )
Epeak [keV] : 270.723 ( -108.791 9422.8 )
Norm@50keV : 4.47492E-03 ( -0.00064887 0.000921247 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 52.96 using 59 PHA bins.
# Reduced chi-squared = 0.9458 for 56 degrees of freedom
# Null hypothesis probability = 5.905209e-01
Photon flux (15-150 keV) in 403.4 sec: 0.441499 ( -0.013915 0.013962 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.46119e-05 ( -4.1643e-07 4.14211e-07 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 1.79619 ( -1.73011 -0.849096 )
beta : -1.36221 ( -0.0595122 0.0562545 )
Epeak [keV] : 30.7222 ( -16.86 124.67 )
Norm@50keV : 0.738253 ( -0.738863 106.05 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 51.33 using 59 PHA bins.
# Reduced chi-squared = 0.9332 for 55 degrees of freedom
# Null hypothesis probability = 6.158066e-01
Photon flux (15-150 keV) in 403.4 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) = 3.37e-06
S(50-100 keV) = 5.33e-06
T90 vs. Hardness ratio plot
T90 = 74.9999999403954 sec.
Hardness ratio (energy fluence ratio) = 1.5816
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.57192
Count Ratio (50-100 keV) / (15-25 keV) = 1.44728
Mask shadow pattern
IMX = 4.811215238076407E-01, IMY = 5.069512404961517E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 64.000000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 64.000000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 64.000000
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:
-13.699410 389.664000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
170.2853 -60.6169 2.2 22.2 104.6 1.9740 5.2 1.0 Cen X-3
186.5497 -62.8086 3.8 19.2 125.7 1.1065 3.1 3.7 GX 301-2
256.0009 -37.8447 1.1 48.6 -155.5 8.5864 10.2 0.7 4U 1700-377
256.4793 -36.4374 4.1 50.1 -155.3 2.5207 2.8 2.3 GX 349+2
264.7341 -44.4617 14.5 43.3 -144.8 0.4872 0.8 0.8 4U 1735-44
262.7774 -33.7753 4.3 53.5 -149.4 -3.4112 -2.7 11.1 GX 354-0
152.4546 -58.2719 1.7 26.2 83.9 3.3575 6.6 ------ UNKNOWN
106.2200 -68.9351 2.8 22.3 28.3 1.2390 4.1 ------ UNKNOWN
73.3987 -58.0484 3.1 36.8 6.2 1.9628 4.9 ------ UNKNOWN
73.5688 -58.3047 3.5 36.5 6.2 2.0162 5.0 ------ UNKNOWN
238.7790 -26.0091 4.1 58.3 -175.6 5.0058 2.8 ------ UNKNOWN
301.8411 -67.3693 2.8 26.1 -99.4 1.7310 4.1 ------ UNKNOWN
292.4410 -64.8603 2.7 27.4 -109.1 1.9843 4.4 ------ UNKNOWN
10.0692 -63.1812 0.3 35.0 -46.5 21.9193 42.4 ------ UNKNOWN
349.5917 -53.4857 3.0 44.0 -64.2 5.2677 3.9 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
462.900610 723.130000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
264.6526 -44.4997 6.8 57.3 -155.2 -10.4894 -1.7 4.9 4U 1735-44
69.0436 -35.7619 2.9 44.7 51.1 15.0558 3.9 ------ UNKNOWN
99.5654 -66.2553 3.8 35.1 105.5 7.5586 3.0 ------ UNKNOWN
59.5884 -44.6462 3.3 33.3 50.1 5.9997 3.5 ------ UNKNOWN
223.6405 -69.0244 3.5 45.7 166.1 7.5030 3.3 ------ UNKNOWN
32.7840 -55.7211 2.7 13.6 37.4 4.1513 4.2 ------ UNKNOWN
330.0365 -74.7166 2.5 17.9 -176.4 4.3078 4.6 ------ UNKNOWN
31.8256 -16.0679 2.7 49.5 -2.0 9.3965 4.2 ------ UNKNOWN
337.0099 -57.2749 3.1 17.2 -115.2 3.9535 3.7 ------ UNKNOWN
18.0017 -7.0134 2.2 56.4 -20.5 21.6216 5.2 ------ UNKNOWN
295.1384 -40.5270 3.1 48.0 -129.0 18.1512 3.8 ------ UNKNOWN
Plot creation:
Tue Apr 28 14:53:18 EDT 2015