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
317.5410 41.5303 0.0060 42.3540 -20.5187 4.5324260 32.224 TRIG_01199764
Foreground time interval of the image:
-1.748 17.149 (delta_t = 18.897 [sec])
Background time interval of the image:
-32.251 -1.748 (delta_t = 30.503 [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)
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 -1.748 sec. to 122.072 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.68358 ( -0.0393366 0.0394022 )
Norm@50keV : 1.07732E-02 ( -0.000219114 0.000219107 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 58.18 using 59 bins.
Reduced chi-squared = 1.0207
# Null hypothesis probability of 4.32e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 123.8 sec: 1.42275 ( -0.03406 0.0342 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.23672e-05 ( -2.56436e-07 2.56641e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -1.748 sec. to 122.072 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.38770 ( -0.170709 0.164591 )
Epeak [keV] : 114.047 ( -22.5842 70.8221 )
Norm@50keV : 1.46684E-02 ( -0.0022633 0.00278643 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 48.57 using 59 bins.
Reduced chi-squared = 0.867321
# Null hypothesis probability of 7.49e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 123.8 sec: 1.38528 ( -0.03908 0.03936 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.21172e-05 ( -2.91629e-07 2.90521e-07 ) ergs/cm2
Band function
Time interval is from -1.748 sec. to 122.072 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] : 15.6336 ( )
R^2/D10^2 : 0.126705 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 496.06 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.65e-71 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.966e-07 3.541e-08
25- 50 3.285e-06 9.656e-08
50-150 5.562e-06 2.024e-07
15-150 9.644e-06 2.241e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 158.352 (-15.0377 18.785)
Norm : 5.72551 (-0.15822 0.16143)
------------------------------------------------------------
#Fit statistic : Chi-Squared 49.55 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.48e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.798e-06 8.790e-08
25- 50 3.363e-06 1.609e-07
50-150 6.815e-06 1.413e-06
15-150 1.198e-05 1.552e-06
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.33634 (-0.665099 0.730633)
R1^2/D10^2 : 1.24351 (-0.33789 0.501799)
kT2 [keV] : 25.3340 (-1.97444 2.58179)
R2^2/D10^2 : 1.71835E-02 (-0.00535035 0.00648096)
------------------------------------------------------------
#Fit statistic : Chi-Squared 72.21 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.97e-02 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.629e-06 1.188e-07
25- 50 3.432e-06 1.529e-07
50-150 6.797e-06 3.367e-07
15-150 1.186e-05 4.283e-07
Peak spectrum fit
Power-law model
Time interval is from 88.712 sec. to 89.712 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.90241 ( -0.0993167 0.101738 )
Norm@50keV : 2.74505E-02 ( -0.00189056 0.00187497 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 80.32 using 59 bins.
Reduced chi-squared = 1.40912
# Null hypothesis probability of 2.26e-02 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 3.94373 ( -0.24399 0.24413 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.52418e-07 ( -1.71353e-08 1.72379e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 88.712 sec. to 89.712 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.619354 ( -0.589107 0.516689 )
Epeak [keV] : 47.1456 ( -4.76258 6.4657 )
Norm@50keV : 0.143501 ( -0.069219 0.163836 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 59.24 using 59 bins.
Reduced chi-squared = 1.05786
# Null hypothesis probability of 3.58e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 3.81466 ( -0.24913 0.24939 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.32049e-07 ( -1.82676e-08 1.86427e-08 ) ergs/cm2
Band function
Time interval is from 88.712 sec. to 89.712 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] : 11.0093 (-0.687927 0.736676)
R^2/D10^2 : 1.35798 (-0.298877 0.378733)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 86.01 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.80e-03 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.440e-08 3.475e-09
25- 50 9.737e-08 6.805e-09
50-150 6.671e-08 1.007e-08
15-150 1.985e-07 1.400e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 78.5682 (-12.8802 17.0995)
Norm : 18.9551 (-1.68286 1.84827)
------------------------------------------------------------
#Fit statistic : Chi-Squared 64.03 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.44e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.913e-08 3.945e-09
25- 50 8.052e-08 5.195e-09
50-150 1.123e-07 1.481e-08
15-150 2.419e-07 1.940e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 8.22857 (-1.85585 1.51848)
R1^2/D10^2 : 3.08038 (-1.16257 2.83081)
kT2 [keV] : 23.9896 (-7.80947 34.3207)
R2^2/D10^2 : 3.47421E-02 (-0.0321053 0.119781)
------------------------------------------------------------
#Fit statistic : Chi-Squared 56.97 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.01e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.203e-08 6.840e-09
25- 50 9.039e-08 1.976e-08
50-150 1.048e-07 4.242e-08
15-150 2.373e-07 6.755e-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: 0.900238 ( -0.0650585 0.0640249 )
Norm@50keV : 1.65367E-02 ( -0.000661967 0.000658411 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 61.89 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.06e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 18.9 sec: 1.89804 ( -0.0761004 0.0762984 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.50727e-06 ( -1.31353e-07 1.31401e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.205900 ( -0.319918 0.297124 )
Epeak [keV] : 165.154 ( -32.1335 72.9069 )
Norm@50keV : 3.11065E-02 ( -0.0071751 0.00994425 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 44.56 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.64e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 18.9 sec: 1.84420 ( -0.07877 0.07904 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.46643e-06 ( -1.35626e-07 1.34984e-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) = 3.33e-06
S(50-100 keV) = 4.13e-06
T90 vs. Hardness ratio plot
T90 = 106.324000000954 sec.
Hardness ratio (energy fluence ratio) = 1.24024
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.30027
Count Ratio (50-100 keV) / (15-25 keV) = 0.908279
Mask shadow pattern
IMX = 8.538162070997549E-01, IMY = 3.195459684732280E-01
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:
-32.251400 -1.748000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
299.6535 35.2002 3.8 52.3 -36.5 1.0101 3.0 3.1 Cyg X-1
308.0221 40.8356 12.9 48.1 -26.7 -0.1504 -0.9 8.1 Cyg X-3
326.2725 38.4367 269.7 35.3 -17.2 0.0043 0.0 8.4 Cyg X-2
315.3641 50.2504 2.2 49.0 -12.4 0.9285 5.1 ------ UNKNOWN
313.5159 34.8716 2.2 41.5 -31.5 0.6418 5.2 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-1.748000 17.148600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
299.6107 35.1513 11.1 52.3 -36.6 -0.3942 -1.0 3.2 Cyg X-1
308.1274 41.1351 5.0 48.1 -26.3 0.4455 2.3 11.0 Cyg X-3
326.1656 38.3173 25.4 35.3 -17.4 0.0495 0.5 0.4 Cyg X-2
28.9539 26.1490 2.4 39.2 78.4 1.3527 4.9 ------ UNKNOWN
319.2085 59.4478 2.5 54.1 -2.2 1.4598 4.6 ------ UNKNOWN
319.7056 38.5871 2.6 39.3 -22.6 0.5356 4.4 ------ UNKNOWN
317.5410 41.5303 0.4 42.4 -20.5 4.5325 32.2 ------ UNKNOWN
321.9086 -22.7670 2.6 43.8 -123.1 1.3289 4.4 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
99.948610 476.748600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.5268 35.3941 5.6 48.6 -48.1 -6.2903 -2.1 4.6 Her X-1
288.8882 10.8638 45.9 39.6 -105.1 0.5386 0.3 7.2 GRS 1915+105
299.5858 35.1851 0.4 15.4 -81.1 18.7038 27.8 1.0 Cyg X-1
308.0862 41.0012 2.4 7.1 -63.8 3.0695 4.8 3.1 Cyg X-3
326.1165 38.2453 4.2 7.4 141.1 1.7415 2.7 5.3 Cyg X-2
1.8586 51.0318 3.6 31.6 84.6 4.2980 3.2 ------ UNKNOWN
336.6650 62.3640 3.2 23.7 49.7 2.9769 3.5 ------ UNKNOWN
341.7662 14.3445 2.5 34.4 162.6 4.2576 4.7 ------ UNKNOWN
334.9901 15.2964 2.7 30.3 172.3 3.5149 4.3 ------ UNKNOWN
263.8728 46.3134 2.1 38.2 -36.7 5.2737 5.7 ------ UNKNOWN
261.1624 36.9663 3.4 43.1 -49.3 5.2503 3.5 ------ UNKNOWN
Plot creation:
Tue Dec 26 16:59:55 EST 2023