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
243.9285 14.3985 0.0047 38.3319 43.0422 19.8607083 40.786 TRIG_01054681
Foreground time interval of the image:
-12.040 13.613 (delta_t = 25.653 [sec])
Background time interval of the image:
-239.688 -12.040 (delta_t = 227.648 [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 -12.040 sec. to 142.472 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.13132 ( -0.0270876 0.0269844 )
Norm@50keV : 2.26312E-02 ( -0.000350687 0.000349993 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 32.22 using 59 bins.
Reduced chi-squared = 0.565263
# Null hypothesis probability of 9.97e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 154.5 sec: 2.63362 ( -0.04432 0.04442 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.62041e-05 ( -5.25484e-07 5.24809e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -12.040 sec. to 142.472 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.977445 ( -0.11223 0.105688 )
Epeak [keV] : 428.312 ( -151.283 901.742 )
Norm@50keV : 2.59879E-02 ( -0.00127949 0.00268712 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 26.49 using 59 bins.
Reduced chi-squared = 0.473036
# Null hypothesis probability of 1.00e+00 with 56 degrees of freedom
Photon flux (15-150 keV) in 154.5 sec: 2.60512 ( -0.04813 0.04836 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.60594e-05 ( -5.36467e-07 5.37037e-07 ) ergs/cm2
Band function
Time interval is from -12.040 sec. to 142.472 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] : 23.5674 ( )
R^2/D10^2 : 7.21141E-02 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 799.84 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.39e-131 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.108e-06 3.569e-08
25- 50 6.094e-06 1.514e-07
50-150 2.525e-05 4.558e-07
15-150 3.245e-05 5.098e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.363 ( )
Norm : 11.7195 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared 871.78 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.54e-146 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.509e-06 7.493e-08
25- 50 8.673e-06 1.483e-07
50-150 1.902e-05 3.090e-07
15-150 3.220e-05 5.176e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 9.31645 (-0.609146 0.64135)
R1^2/D10^2 : 0.808238 (-0.149011 0.192933)
kT2 [keV] : 37.3827 (-2.16517 2.62324)
R2^2/D10^2 : 1.40045E-02 (-0.00274514 0.00303282)
------------------------------------------------------------
#Fit statistic : Chi-Squared 27.11 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.99e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.555e-06 1.475e-07
25- 50 7.545e-06 2.325e-07
50-150 2.602e-05 7.262e-07
15-150 3.612e-05 8.575e-07
Peak spectrum fit
Power-law model
Time interval is from 7.948 sec. to 8.948 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.665326 ( -0.0955809 0.0936348 )
Norm@50keV : 0.116409 ( -0.00654709 0.00649662 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 70.06 using 59 bins.
Reduced chi-squared = 1.22912
# Null hypothesis probability of 1.15e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.692270 ( -0.019182 0.43008 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.44371e-06 ( -8.19518e-08 8.21335e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 7.948 sec. to 8.948 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.658243 ( -0.097362 0.0933276 )
Epeak [keV] : 9999.36 ( -9999.36 -9999.36 )
Norm@50keV : 0.117346 ( -0.00621124 0.0409666 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 70.07 using 59 bins.
Reduced chi-squared = 1.25125
# Null hypothesis probability of 9.78e-02 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 13.5069 ( -0.8248 0.7958 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.44451e-06 ( -9.54539e-08 6.21318e-08 ) ergs/cm2
Band function
Time interval is from 7.948 sec. to 8.948 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] : 28.6411 ( )
R^2/D10^2 : 0.240195 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 123.84 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.43e-07 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.170e-08 3.380e-09
25- 50 1.918e-07 1.645e-08
50-150 1.130e-06 8.850e-08
15-150 1.353e-06 9.200e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.363 ( )
Norm : 49.1917 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared 294.42 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.04e-33 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.225e-07 7.850e-09
25- 50 2.356e-07 2.590e-08
50-150 5.168e-07 1.354e-07
15-150 8.749e-07 1.970e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 12.6520 (-3.28031 3.06093)
R1^2/D10^2 : 1.44730 (-0.614554 1.44019)
kT2 [keV] : 68.5691 (-26.8493 -71.9493)
R2^2/D10^2 : 2.04360E-02 (-0.0101615 0.0411632)
------------------------------------------------------------
#Fit statistic : Chi-Squared 70.83 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.40e-02 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.725e-08 1.518e-08
25- 50 2.266e-07 5.930e-08
50-150 1.152e-06 4.899e-07
15-150 1.436e-06 5.503e-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: 0.806162 ( -0.0370019 0.0367172 )
Norm@50keV : 5.17088E-02 ( -0.00112893 0.00112478 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 46.04 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.50e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 25.65 sec: 5.94174 ( -0.126391 0.126578 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.54594e-05 ( -3.15362e-07 3.15474e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.722541 ( -0.148336 0.11839 )
Epeak [keV] : 998.500 ( -999.834 -999.834 )
Norm@50keV : 5.57153E-02 ( -0.00468544 0.00767837 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 45.10 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.51e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 25.65 sec: 5.92065 ( -0.13101 0.12892 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.54502e-05 ( -3.18291e-07 3.17547e-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) = 7.29e-06
S(50-100 keV) = 1.33e-05
T90 vs. Hardness ratio plot
T90 = 69.3839999437332 sec.
Hardness ratio (energy fluence ratio) = 1.82442
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.80071
Count Ratio (50-100 keV) / (15-25 keV) = 1.86276
Mask shadow pattern
IMX = 5.778535244441950E-01, IMY = -5.396527728179455E-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:
-239.688000 -12.040000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.5696 35.5188 0.0 49.5 13.4 0.3378 0.6 11.9 Her X-1
230.5493 19.3091 2.3 25.6 33.5 1.3517 5.0 ------ UNKNOWN
251.7571 43.1883 2.8 49.6 2.9 2.0056 4.2 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-12.040000 13.612600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.5696 35.5188 0.0 49.5 13.4 -0.0423 -0.1 11.9 Her X-1
243.9285 14.3985 0.3 38.3 43.0 19.8619 40.8 ------ UNKNOWN
203.2302 -12.0390 3.0 26.5 140.4 0.8588 3.9 ------ UNKNOWN
178.7643 53.0800 3.5 43.5 -64.0 1.7285 3.4 ------ UNKNOWN
158.1695 20.0544 2.5 44.3 -117.9 2.2277 4.6 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
73.012600 720.022000
720.312000 962.370100
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
244.9959 -15.6382 0.6 30.1 110.2 25.0915 20.1 1.0 Sco X-1
254.3252 35.2185 8.4 22.8 -45.4 -1.1856 -1.4 9.9 Her X-1
268.5353 -1.5375 0.0 29.1 53.4 -1.8837 -1.5 11.3 SW J1753.5-0127
274.1072 -13.9388 3.9 41.2 64.4 7.5718 3.0 8.3 GX 17+2
288.7695 10.8892 12.6 43.8 21.4 1.2665 0.9 3.8 GRS 1915+105
299.6203 35.2066 1.6 53.9 -11.1 15.0327 7.1 1.5 Cyg X-1
281.8400 44.5264 3.0 44.0 -28.7 5.4389 3.8 ------ UNKNOWN
217.5038 37.0600 5.4 32.6 -108.9 3.0868 2.1 ------ UNKNOWN
194.6708 30.7475 3.1 47.9 -129.1 13.7120 3.8 ------ UNKNOWN
Plot creation:
Sat Jul 30 06:58:54 EDT 2022