Estimated redshift from machine learning (Ukwatta et al. 2016) - may take a few minute to calcaulte
Image
Pre-slew 15.0-350.0 keV image (Event data)
# RAcent DECcent POSerr Theta Phi Peak Cts SNR Name
140.9424 39.8311 0.0060 32.6096 -28.8195 3.3524248 31.875 TRIG_01257556
Foreground time interval of the image:
-21.336 17.349 (delta_t = 38.685 [sec])
Background time interval of the image:
-239.152 -21.336 (delta_t = 217.816 [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 -21.336 sec. to 34.916 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.96459 ( -0.0925114 0.0943323 )
Norm@50keV : 4.01006E-03 ( -0.000224116 0.000222135 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 58.29 using 59 bins.
Reduced chi-squared = 1.02263
# Null hypothesis probability of 4.28e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 56.25 sec: 0.591965 ( -0.030262 0.030325 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.07717e-06 ( -1.119e-07 1.12619e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -21.336 sec. to 34.916 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.50727 ( -0.416161 0.379351 )
Epeak [keV] : 49.4150 ( -11.894 26.057 )
Norm@50keV : 7.04395E-03 ( -0.00257999 0.00464289 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 53.99 using 59 bins.
Reduced chi-squared = 0.964107
# Null hypothesis probability of 5.51e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 56.25 sec: 0.576679 ( -0.032622 0.032708 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.99569e-06 ( -1.29212e-07 1.30112e-07 ) ergs/cm2
Band function
Time interval is from -21.336 sec. to 34.916 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : ( )
beta : ( )
Epeak [keV] : ( )
Norm@50keV : ( )
------------------------------------------------------------
Photon flux (15-150 keV) in 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] : 11.3243 ( )
R^2/D10^2 : 0.166419 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 136.75 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.67e-08 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.521e-07 2.191e-08
25- 50 7.397e-07 4.162e-08
50-150 5.477e-07 6.421e-08
15-150 1.539e-06 8.803e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 76.8541 (-11.4468 14.7859)
Norm : 2.77304 (-0.222902 0.246979)
------------------------------------------------------------
#Fit statistic : Chi-Squared 54.62 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.65e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.036e-07 3.097e-08
25- 50 6.579e-07 3.291e-08
50-150 9.037e-07 1.012e-07
15-150 1.965e-06 1.207e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.68665 (-0.998993 1.14905)
R1^2/D10^2 : 1.50956 (-0.719352 1.69588)
kT2 [keV] : 18.6419 (-2.65197 4.15747)
R2^2/D10^2 : 1.85546E-02 (-0.0105134 0.0170747)
------------------------------------------------------------
#Fit statistic : Chi-Squared 57.25 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.91e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.082e-07 7.290e-08
25- 50 6.384e-07 8.691e-08
50-150 8.882e-07 2.067e-07
15-150 1.935e-06 3.023e-07
Peak spectrum fit
Power-law model
Time interval is from -0.276 sec. to 0.724 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.45841 ( -0.198566 0.199964 )
Norm@50keV : 1.32513E-02 ( -0.00167036 0.00166725 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 50.71 using 59 bins.
Reduced chi-squared = 0.889649
# Null hypothesis probability of 7.08e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 1.63651 ( -0.21127 0.21175 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.26628e-07 ( -1.7071e-08 1.71591e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.276 sec. to 0.724 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.519422 ( -0.9931 0.817386 )
Epeak [keV] : 84.6473 ( -20.7457 172.16 )
Norm@50keV : 3.73522E-02 ( -0.0218508 0.0672775 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 46.78 using 59 bins.
Reduced chi-squared = 0.835357
# Null hypothesis probability of 8.05e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 1.58837 ( -0.21742 0.21685 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.22659e-07 ( -1.75016e-08 1.76224e-08 ) ergs/cm2
Band function
Time interval is from -0.276 sec. to 0.724 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : ( )
beta : ( )
Epeak [keV] : ( )
Norm@50keV : ( )
------------------------------------------------------------
Photon flux (15-150 keV) in 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] : 17.1860 (-2.29218 2.6306)
R^2/D10^2 : 0.123149 (-0.0486471 0.0799659)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 55.21 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.43e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.385e-09 1.780e-09
25- 50 3.296e-08 5.770e-09
50-150 6.974e-08 1.549e-08
15-150 1.101e-07 1.804e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-65.2834 -200)
Norm : 6.81942 (-0.848367 0.848367)
------------------------------------------------------------
#Fit statistic : Chi-Squared 49.40 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.53e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.698e-08 9.620e-09
25- 50 3.267e-08 1.817e-08
50-150 7.165e-08 3.983e-08
15-150 1.213e-07 6.800e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.56269 (-2.64543 3.50512)
R1^2/D10^2 : 2.80820 (-2.29778 47.185)
kT2 [keV] : 21.2303 (-3.75866 6.46075)
R2^2/D10^2 : 5.16394E-02 (-0.0338742 0.0571344)
------------------------------------------------------------
#Fit statistic : Chi-Squared 44.98 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.30e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.465e-08 7.726e-09
25- 50 3.130e-08 1.441e-08
50-150 7.672e-08 3.758e-08
15-150 1.227e-07 4.095e-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: 1.89294 ( -0.0871865 0.0885729 )
Norm@50keV : 5.29937E-03 ( -0.000273465 0.000271576 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 54.02 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.87e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 38.68 sec: 0.758248 ( -0.0372926 0.0373744 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.88443e-06 ( -9.62919e-08 9.67236e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.47522 ( -0.380844 0.35024 )
Epeak [keV] : 59.3996 ( -11.4119 58.6771 )
Norm@50keV : 8.76746E-03 ( -0.00295669 0.0050041 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 49.82 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.07e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 38.68 sec: 0.739911 ( -0.040086 0.040173 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.82141e-06 ( -1.09658e-07 1.09917e-07 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : ( )
beta : ( )
Epeak [keV] : ( )
Norm@50keV : ( )
------------------------------------------------------------
Photon flux (15-150 keV) in 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) = 6.19e-07
S(50-100 keV) = 6.36e-07
T90 vs. Hardness ratio plot
T90 = 43.3039999008179 sec.
Hardness ratio (energy fluence ratio) = 1.02746
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.13269
Count Ratio (50-100 keV) / (15-25 keV) = 0.619574
Mask shadow pattern
IMX = 5.605232606910161E-01, IMY = 3.083993593445276E-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:
-239.152000 -21.336000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.3938 35.2633 4.6 54.4 -176.4 -2.1376 -2.5 5.7 Her X-1
251.1791 30.6222 2.3 57.3 -170.9 6.0928 5.0 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-21.336000 17.348630
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.4681 35.4864 5.4 54.3 -176.6 -0.5081 -2.1 8.6 Her X-1
238.1610 38.8153 2.6 45.0 -163.8 0.6217 4.4 ------ UNKNOWN
140.9424 39.8311 0.4 32.6 -28.8 3.3523 31.9 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
94.148580 326.348610
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
96.5130 33.3376 2.3 35.9 61.0 3.6413 5.0 ------ UNKNOWN
182.6625 74.4120 2.3 39.5 163.4 2.6198 4.9 ------ UNKNOWN
130.7740 36.9354 1.9 8.5 40.3 1.6836 6.0 ------ UNKNOWN
Plot creation:
Sat Oct 19 18:14:19 EDT 2024