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
331.8091 10.1520 0.0158 37.8036 -72.6200 2.5436999 12.243 TRIG_01036024
Foreground time interval of the image:
-2.424 23.512 (delta_t = 25.936 [sec])
Background time interval of the image:
-93.995 -2.424 (delta_t = 91.571 [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 -2.424 sec. to 23.512 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.37520 ( -0.206614 0.206266 )
Norm@50keV : 6.52671E-03 ( -0.000751343 0.000747782 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 67.45 using 59 bins.
Reduced chi-squared = 1.18333
# Null hypothesis probability of 1.62e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 25.94 sec: 0.790486 ( -0.090611 0.090775 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.64464e-06 ( -2.13307e-07 2.16249e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -2.424 sec. to 23.512 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.37828 ( -0.212003 0.203535 )
Epeak [keV] : 9999.33 ( -9999.36 -9999.36 )
Norm@50keV : 6.53075E-03 ( -0.00654362 0.00920373 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 67.46 using 59 bins.
Reduced chi-squared = 1.20464
# Null hypothesis probability of 1.40e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 25.94 sec: 0.792019 ( -0.09522 0.09127 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.64919e-06 ( -2.41131e-07 2.16161e-07 ) ergs/cm2
Band function
Time interval is from -2.424 sec. to 23.512 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] : 14.6787 (-2.01027 2.49479)
R^2/D10^2 : 9.68525E-02 (-0.0407677 0.0654016)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 84.75 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.97e-03 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.137e-07 2.565e-08
25- 50 4.428e-07 7.484e-08
50-150 6.429e-07 1.655e-07
15-150 1.199e-06 2.053e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-54.1798 -200)
Norm : 3.24506 (-0.367419 0.367419)
------------------------------------------------------------
#Fit statistic : Chi-Squared 69.79 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.19e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.096e-07 1.155e-07
25- 50 4.032e-07 2.233e-07
50-150 8.844e-07 4.837e-07
15-150 1.497e-06 8.302e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 10.6502 (-1.86134 2.01974)
R1^2/D10^2 : 0.247328 (-0.134443 0.135705)
kT2 [keV] : 200.000 (-161.274 -200)
R2^2/D10^2 : 1.18454E-04 (-3.367e-05 0.000442015)
------------------------------------------------------------
#Fit statistic : Chi-Squared 64.18 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.86e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.585e-07 5.550e-08
25- 50 4.392e-07 1.519e-07
50-150 1.089e-06 8.174e-07
15-150 1.687e-06 9.418e-07
Peak spectrum fit
Power-law model
Time interval is from 1.036 sec. to 2.036 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.712104 ( -0.389043 0.327468 )
Norm@50keV : 2.11166E-02 ( -0.00454493 0.00427915 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 54.01 using 59 bins.
Reduced chi-squared = 0.947544
# Null hypothesis probability of 5.88e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 2.43860 ( -0.47264 0.47692 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.56383e-07 ( -4.68946e-08 4.7069e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 1.036 sec. to 2.036 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.705325 ( -0.885451 0.399709 )
Epeak [keV] : 1.00000E+04 ( -10000 -10000 )
Norm@50keV : 2.12846E-02 ( -0.0045472 -0.0212846 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 54.02 using 59 bins.
Reduced chi-squared = 0.964643
# Null hypothesis probability of 5.50e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 2.42547 ( -0.45742 0.48606 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.56289e-07 ( -4.71909e-08 4.7177e-08 ) ergs/cm2
Band function
Time interval is from 1.036 sec. to 2.036 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] : 23.0970 (-6.45548 15.2147)
R^2/D10^2 : 7.73569E-02 (-0.0780875 0.14784)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 61.96 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.04e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.463e-09 3.116e-09
25- 50 4.059e-08 1.557e-08
50-150 1.617e-07 6.611e-08
15-150 2.098e-07 6.590e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-40.3471 -200)
Norm : 10.0506 (-1.99923 1.99923)
------------------------------------------------------------
#Fit statistic : Chi-Squared 72.07 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.62e-02 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.502e-08 1.450e-08
25- 50 4.814e-08 2.810e-08
50-150 1.056e-07 5.985e-08
15-150 1.787e-07 1.028e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 12.0519 (-2.94541 2.16334)
R1^2/D10^2 : 0.441749 (-0.22347 0.623075)
kT2 [keV] : 200.000 (-200 -200)
R2^2/D10^2 : 6.12987E-04 (-0.000207895 0.00281621)
------------------------------------------------------------
#Fit statistic : Chi-Squared 45.17 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.25e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.434e-08 8.530e-09
25- 50 4.876e-08 2.750e-08
50-150 2.045e-07 1.399e-07
15-150 2.676e-07 1.676e-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: 1.37520 ( -0.206614 0.206266 )
Norm@50keV : 6.52671E-03 ( -0.000751343 0.000747782 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 67.45 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.62e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 25.94 sec: 0.790474 ( -0.0906077 0.0907708 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.64442e-06 ( -2.13262e-07 2.16287e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.09205 ( -0.246888 0.0269139 )
Epeak [keV] : 34.7447 ( )
Norm@50keV : 2.27419E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared 66.96 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.50e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 25.94 sec: 0.790900 ( -0.09158 0.0901 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.64352e-06 ( -2.31364e-07 2.1463e-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) = 3.81e-07
S(50-100 keV) = 5.89e-07
T90 vs. Hardness ratio plot
T90 = 23.8400000333786 sec.
Hardness ratio (energy fluence ratio) = 1.54593
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.60911
Count Ratio (50-100 keV) / (15-25 keV) = 1.08678
Mask shadow pattern
IMX = 2.317318179404066E-01, IMY = 7.403615920151344E-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:
-93.995400 -2.424000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
288.7051 11.0172 12.2 39.7 -2.2 -0.2690 -0.9 7.0 GRS 1915+105
299.5186 35.1497 3.2 14.3 11.3 0.6416 3.6 4.7 Cyg X-1
307.9353 40.9022 2.6 5.5 8.3 0.7571 4.4 8.5 Cyg X-3
326.2535 38.2627 5.0 11.4 -103.4 0.4129 2.3 5.2 Cyg X-2
33.9671 74.5266 2.2 45.0 159.4 2.2129 5.2 ------ UNKNOWN
309.9228 60.6545 2.6 16.3 131.1 0.8470 4.4 ------ UNKNOWN
44.6112 49.0047 2.2 58.6 -172.3 5.5904 5.2 ------ UNKNOWN
312.0703 -7.0267 2.6 51.6 -40.6 3.9379 4.5 ------ UNKNOWN
326.2881 1.4523 2.5 44.5 -60.7 3.4356 4.6 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-2.424000 23.512000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
288.7688 11.1216 4.2 39.6 -2.3 0.3927 2.7 10.7 GRS 1915+105
299.6380 34.9952 0.0 14.3 10.5 0.0987 1.1 12.6 Cyg X-1
308.1467 41.0852 35.5 5.3 8.6 0.0283 0.3 8.1 Cyg X-3
326.3080 38.2788 6.8 11.4 -103.6 -0.1458 -1.7 6.9 Cyg X-2
266.4648 25.3960 2.5 42.4 36.8 0.8997 4.7 ------ UNKNOWN
331.8091 10.1521 0.9 37.8 -72.6 2.5441 12.2 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
158.604630 962.194000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
299.3852 35.2139 17.4 58.4 -27.1 -3.4868 -0.7 10.1 Cyg X-1
307.9646 41.0604 6.4 49.4 -27.5 4.0343 1.8 9.2 Cyg X-3
326.1717 38.3217 26.8 40.4 -43.2 -0.6562 -0.4 0.0 Cyg X-2
267.2518 59.6457 4.8 55.8 11.3 12.9141 2.4 ------ UNKNOWN
298.2403 48.0360 3.4 50.3 -14.7 7.7999 3.4 ------ UNKNOWN
44.3594 -3.4970 3.5 59.6 -161.2 33.5211 3.3 ------ UNKNOWN
329.3465 27.8660 3.4 45.8 -56.9 11.5465 3.4 ------ UNKNOWN
Plot creation:
Sat Jul 30 07:11:39 EDT 2022