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
240.2072 13.0081 0.0090 12.2229 -34.0132 1.6588231 21.328 TRIG_00915381
Foreground time interval of the image:
-0.280 17.037 (delta_t = 17.317 [sec])
Background time interval of the image:
-102.363 -0.280 (delta_t = 102.083 [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 -0.280 sec. to 202.124 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.66537 ( -0.0881746 0.0890782 )
Norm@50keV : 2.70810E-03 ( -0.000131142 0.000130313 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 62.50 using 59 PHA bins.
# Reduced chi-squared = 1.097 for 57 degrees of freedom
# Null hypothesis probability = 2.871130e-01
Photon flux (15-150 keV) in 202.4 sec: 0.355438 ( -0.016128 0.01615 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.09085e-06 ( -2.64033e-07 2.66757e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.280 sec. to 202.124 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.45876 ( -0.35865 0.271551 )
Epeak [keV] : 123.346 ( -51.0243 -123.346 )
Norm@50keV : 3.46925E-03 ( -0.000857486 0.00181768 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 61.39 using 59 PHA bins.
# Reduced chi-squared = 1.096 for 56 degrees of freedom
# Null hypothesis probability = 2.889028e-01
Photon flux (15-150 keV) in 202.4 sec: 0.350236 ( -0.018091 0.01808 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.96764e-06 ( -3.2719e-07 3.28631e-07 ) ergs/cm2
Band function
Time interval is from -0.280 sec. to 202.124 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] : 12.8901 ( )
R^2/D10^2 : 6.35221E-02 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 163.61 using 59 PHA bins.
# Reduced chi-squared = 2.8703 for 57 degrees of freedom
# Null hypothesis probability = 3.088453e-12
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.531e-07 4.149e-08
25- 50 1.546e-06 8.167e-08
50-150 1.616e-06 1.747e-07
15-150 3.615e-06 2.206e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 149.478 (-33.8065 43.1662)
Norm : 1.44260 (-0.0743091 0.0939758)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 62.25 using 59 PHA bins.
# Reduced chi-squared = 1.092 for 57 degrees of freedom
# Null hypothesis probability = 2.948905e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.501e-07 5.212e-08
25- 50 1.390e-06 1.275e-07
50-150 2.739e-06 8.210e-07
15-150 4.879e-06 1.068e-06
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.69904 (-1.01899 1.07162)
R1^2/D10^2 : 0.457901 (-0.178528 0.361535)
kT2 [keV] : 24.4851 (-3.92437 6.01891)
R2^2/D10^2 : 4.98194E-03 (-0.00268006 0.00458619)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 63.47 using 59 PHA bins.
# Reduced chi-squared = 1.154 for 55 degrees of freedom
# Null hypothesis probability = 2.025158e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.431e-07 1.327e-07
25- 50 1.396e-06 1.762e-07
50-150 2.769e-06 5.442e-07
15-150 4.908e-06 7.853e-07
Peak spectrum fit
Power-law model
Time interval is from 0.268 sec. to 1.268 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.38902 ( -0.0971697 0.0976764 )
Norm@50keV : 4.52520E-02 ( -0.00254767 0.00254035 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 46.38 using 59 PHA bins.
# Reduced chi-squared = 0.8136 for 57 degrees of freedom
# Null hypothesis probability = 8.415539e-01
Photon flux (15-150 keV) in 1 sec: 5.49736 ( -0.30398 0.30412 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.38299e-07 ( -2.79532e-08 2.81777e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.268 sec. to 1.268 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.06335 ( -0.405416 0.359254 )
Epeak [keV] : 142.814 ( -53.9698 -142.816 )
Norm@50keV : 6.62738E-02 ( -0.0218284 0.039179 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 44.12 using 59 PHA bins.
# Reduced chi-squared = 0.7879 for 56 degrees of freedom
# Null hypothesis probability = 8.747406e-01
Photon flux (15-150 keV) in 1 sec: 5.41428 ( -0.31834 0.31796 ) ph/cm2/s
Energy fluence (15-150 keV) : 0 ( 0 0 ) ergs/cm2
Band function
Time interval is from 0.268 sec. to 1.268 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] : 15.0520 (-1.10854 1.22763)
R^2/D10^2 : 0.622943 (-0.146127 0.187487)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 108.53 using 59 PHA bins.
# Reduced chi-squared = 1.9040 for 57 degrees of freedom
# Null hypothesis probability = 4.637225e-05
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.953e-08 3.320e-09
25- 50 1.177e-07 8.600e-09
50-150 1.818e-07 2.115e-08
15-150 3.290e-07 2.150e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-19.9411 -200)
Norm : 22.5382 (-1.235 1.235)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 51.09 using 59 PHA bins.
# Reduced chi-squared = 0.8963 for 57 degrees of freedom
# Null hypothesis probability = 6.953818e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.613e-08 3.400e-09
25- 50 1.080e-07 6.500e-09
50-150 2.368e-07 5.035e-08
15-150 4.009e-07 5.530e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 8.38888 (-1.30264 1.39942)
R1^2/D10^2 : 3.11980 (-1.1496 2.10816)
kT2 [keV] : 32.9978 (-7.06628 13.8883)
R2^2/D10^2 : 3.32157E-02 (-0.021725 0.0425199)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 39.34 using 59 PHA bins.
# Reduced chi-squared = 0.7153 for 55 degrees of freedom
# Null hypothesis probability = 9.450605e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.636e-08 9.400e-09
25- 50 1.120e-07 1.700e-08
50-150 2.750e-07 1.177e-07
15-150 4.333e-07 1.287e-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: 1.67377 ( -0.135077 0.138109 )
Norm@50keV : 5.59611E-03 ( -0.000458304 0.00045277 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 66.01 using 59 PHA bins.
# Reduced chi-squared = 1.158 for 57 degrees of freedom
# Null hypothesis probability = 1.935275e-01
Photon flux (15-150 keV) in 17.32 sec: 0.736545 ( -0.0528783 0.0528976 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.994e-07 ( -7.83269e-08 7.97408e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.03347 ( -0.630628 0.549234 )
Epeak [keV] : 68.1980 ( -15.5783 118.641 )
Norm@50keV : 1.24059E-02 ( -0.00602442 0.0144806 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 61.96 using 59 PHA bins.
# Reduced chi-squared = 1.106 for 56 degrees of freedom
# Null hypothesis probability = 2.719768e-01
Photon flux (15-150 keV) in 17.32 sec: 0.710068 ( -0.057121 0.057178 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.36272e-07 ( -9.06927e-08 9.46607e-08 ) 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) = 1.36e-06
S(50-100 keV) = 1.71e-06
T90 vs. Hardness ratio plot
T90 = 185.827999949455 sec.
Hardness ratio (energy fluence ratio) = 1.25735
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.16097
Count Ratio (50-100 keV) / (15-25 keV) = 0.790549
Mask shadow pattern
IMX = 1.795632528918745E-01, IMY = 1.211770814712049E-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:
-102.363410 -0.280000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
244.9662 -15.6911 2.0 16.9 144.8 2.3842 5.9 3.2 Sco X-1
254.4938 35.1576 0.0 36.1 -8.1 0.2004 0.4 11.2 Her X-1
256.1951 -37.7462 43.3 40.8 137.3 -0.4732 -0.3 11.5 4U 1700-377
256.3632 -36.5098 100.5 39.7 136.4 -0.1867 -0.1 6.3 GX 349+2
262.9637 -24.8117 4.6 32.7 117.8 2.0664 2.5 4.7 GX 1+4
268.4502 -1.6363 40.5 26.5 70.1 0.1697 0.3 12.1 SW J1753.5-0127
270.3529 -24.9685 7.5 37.7 109.9 2.1471 1.5 7.6 GX 5-1
270.4686 -25.7654 11.0 38.3 110.8 1.6594 1.0 9.1 GRS 1758-258
273.8147 -14.0957 0.0 34.9 91.2 2.3792 2.3 11.7 GX 17+2
263.1578 -33.7322 2.6 39.9 126.7 8.0963 4.4 10.4 GX 354-0
227.4820 -47.6256 2.4 50.2 167.3 8.6383 4.8 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-0.280000 17.036600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
244.8056 -15.6502 10.9 16.8 145.3 -0.0948 -1.1 10.1 Sco X-1
254.4278 35.4497 4.0 36.4 -8.4 0.3091 2.9 6.6 Her X-1
256.1785 -37.8408 6.4 40.9 137.4 0.5706 1.8 9.1 4U 1700-377
256.2465 -36.5147 3.8 39.7 136.6 0.8814 3.1 10.6 GX 349+2
263.0700 -24.7479 13.1 32.8 117.5 -0.1525 -0.9 3.3 GX 1+4
268.3067 -1.5743 12.0 26.4 70.0 -0.1331 -1.0 8.2 SW J1753.5-0127
270.3427 -24.9661 12.8 37.7 109.9 -0.2486 -0.9 7.5 GX 5-1
270.1275 -25.7392 9.8 38.0 111.1 0.3498 1.2 9.5 GRS 1758-258
274.0471 -13.9201 5.1 35.0 90.8 -0.5331 -2.3 7.4 GX 17+2
263.2280 -33.7442 0.0 40.0 126.7 -0.4359 -1.3 13.1 GX 354-0
285.8752 31.0084 2.6 51.2 24.1 1.5806 4.4 ------ UNKNOWN
231.8768 -46.9741 2.3 48.7 163.8 1.5114 5.0 ------ UNKNOWN
243.6319 9.1884 2.2 8.4 -14.8 0.4002 5.2 ------ UNKNOWN
240.2072 13.0081 0.5 12.2 -34.0 1.6588 21.3 ------ UNKNOWN
193.0182 -15.1886 2.4 51.1 -135.9 1.8048 4.8 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
49.836600 856.336600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
244.9743 -15.6571 1.7 29.0 140.9 25.9920 6.5 1.1 Sco X-1
254.4577 35.3426 2700.0 25.8 -2.1 0.0078 0.0 0.0 Her X-1
268.3360 -1.4888 5.1 31.4 85.8 -12.1491 -2.3 2.9 SW J1753.5-0127
273.1820 -5.7975 3.5 37.7 88.2 26.3682 3.3 ------ UNKNOWN
213.6771 20.1050 2.6 26.4 -100.4 12.6919 4.5 ------ UNKNOWN
196.7136 17.8213 2.3 42.1 -107.3 52.2074 5.1 ------ UNKNOWN
Plot creation:
Thu Aug 15 14:48:02 EDT 2019