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
1.0977 -14.9686 0.0164 7.1527 -168.8929 0.9031220 11.697 TRIG_01048618
Foreground time interval of the image:
-2.528 28.917 (delta_t = 31.445 [sec])
Background time interval of the image:
-239.984 -2.528 (delta_t = 237.456 [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 -2.528 sec. to 56.896 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.25792 ( -0.284195 0.281329 )
Norm@50keV : 1.00175E-03 ( -0.000162152 0.000161689 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 53.90 using 59 bins.
Reduced chi-squared = 0.945614
# Null hypothesis probability of 5.92e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 59.42 sec: 0.118636 ( -0.0192284 0.019252 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.94557e-07 ( -1.09165e-07 1.11196e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -2.528 sec. to 56.896 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.832177 ( -1.33164 0.668011 )
Epeak [keV] : 139.995 ( -139.995 -139.995 )
Norm@50keV : 1.63103E-03 ( -0.0007734 0.00546883 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 53.45 using 59 bins.
Reduced chi-squared = 0.954464
# Null hypothesis probability of 5.72e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 59.42 sec: 0.116412 ( -0.0201468 0.02004 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.7371e-07 ( -1.21924e-07 1.22199e-07 ) ergs/cm2
Band function
Time interval is from -2.528 sec. to 56.896 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] : 17.2236 (-3.38937 4.4364)
R^2/D10^2 : 8.78874E-03 (-0.00467028 0.00954406)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 59.88 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.72e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.144e-08 1.112e-08
25- 50 1.405e-07 4.323e-08
50-150 2.989e-07 1.022e-07
15-150 4.709e-07 1.157e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-65.2008 -200)
Norm : 0.485445 (-0.0786997 0.0786997)
------------------------------------------------------------
#Fit statistic : Chi-Squared 56.32 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.00e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.183e-08 4.115e-08
25- 50 1.382e-07 7.888e-08
50-150 3.030e-07 1.713e-07
15-150 5.130e-07 2.862e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.64574 (-4.45389 6.07661)
R1^2/D10^2 : 7.32128E-02 (-0.0583975 1.85277)
kT2 [keV] : 27.7872 (-9.76474 -27.7872)
R2^2/D10^2 : 1.45824E-03 (-0.00143499 0.00551409)
------------------------------------------------------------
#Fit statistic : Chi-Squared 53.28 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.41e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.533e-08 3.120e-08
25- 50 1.371e-07 7.428e-08
50-150 3.823e-07 2.227e-07
15-150 5.747e-07 2.980e-07
Peak spectrum fit
Power-law model
Time interval is from 0.836 sec. to 1.836 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.759879 ( -0.470359 0.414803 )
Norm@50keV : 5.54097E-03 ( -0.00140393 0.00134422 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 50.96 using 59 bins.
Reduced chi-squared = 0.894035
# Null hypothesis probability of 7.00e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.637956 ( -0.151126 0.152248 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.58749e-08 ( -1.59669e-08 1.61055e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.836 sec. to 1.836 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.23164 ( -0.2467 0.320099 )
Epeak [keV] : 69.8079 ( )
Norm@50keV : 9.85655E-05 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared 49.80 using 59 bins.
Reduced chi-squared = 0.889286
# Null hypothesis probability of 7.07e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.637655 ( -0.154678 0.151927 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.58537e-08 ( -1.66067e-08 1.53676e-08 ) ergs/cm2
Band function
Time interval is from 0.836 sec. to 1.836 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] : 29.0543 (-9.13072 17.3168)
R^2/D10^2 : 1.03481E-02 (-0.00736861 0.0212625)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 54.41 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.73e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.393e-09 7.538e-10
25- 50 8.481e-09 4.687e-09
50-150 5.117e-08 2.821e-08
15-150 6.105e-08 2.936e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-63.4581 -200)
Norm : 2.52149 (-0.631347 0.631347)
------------------------------------------------------------
#Fit statistic : Chi-Squared 60.50 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.51e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.282e-09 3.855e-09
25- 50 1.208e-08 7.215e-09
50-150 2.650e-08 1.566e-08
15-150 4.487e-08 2.730e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 9.14501 (-4.06742 8.94565)
R1^2/D10^2 : 0.200647 (-0.178476 1.23346)
kT2 [keV] : 51.5469 (-45.8631 -50.7497)
R2^2/D10^2 : 1.87513E-03 (-0.001888 0.00673053)
------------------------------------------------------------
#Fit statistic : Chi-Squared 49.67 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.78e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.824e-09 2.393e-09
25- 50 1.104e-08 6.270e-09
50-150 5.151e-08 2.965e-08
15-150 6.637e-08 3.513e-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: 1.14672 ( -0.24001 0.234594 )
Norm@50keV : 1.71195E-03 ( -0.000224275 0.000224274 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 43.53 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.06e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 31.44 sec: 0.199571 ( -0.0266779 0.0267429 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.5463e-07 ( -8.2182e-08 8.32698e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.06400 ( -1.01133 0.313214 )
Epeak [keV] : 599.082 ( -599.192 -599.192 )
Norm@50keV : 1.87717E-03 ( -0.00187714 0.00370337 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 43.50 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.88e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 31.44 sec: 0.198821 ( -0.027511 0.027195 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.51351e-07 ( -9.21664e-08 8.59915e-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) = 1.29e-07
S(50-100 keV) = 2.16e-07
T90 vs. Hardness ratio plot
T90 = 55.7120000123978 sec.
Hardness ratio (energy fluence ratio) = 1.67442
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 2.30225
Count Ratio (50-100 keV) / (15-25 keV) = 1.44964
Mask shadow pattern
IMX = -1.231402794661389E-01, IMY = 2.417502438582406E-02
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:
-239.984000 -2.528000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
335.8294 -60.2352 4.0 42.8 44.9 1.9584 2.9 ------ UNKNOWN
341.4129 -10.6640 2.5 23.5 140.6 1.4750 4.6 ------ UNKNOWN
351.8042 34.7537 3.5 57.6 -165.4 4.1506 3.3 ------ UNKNOWN
355.3478 37.2635 3.5 59.6 -161.5 7.9010 3.3 ------ UNKNOWN
12.2336 32.7357 3.4 55.4 -145.0 4.8512 3.4 ------ UNKNOWN
39.7682 -2.1027 4.1 40.9 -88.3 3.9743 2.8 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-2.528000 28.916600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
21.9468 -57.1449 2.4 37.9 8.7 0.5906 4.9 ------ UNKNOWN
17.6535 -51.8860 2.0 32.1 8.3 0.5638 5.8 ------ UNKNOWN
357.2802 -17.8307 2.1 6.7 152.0 0.3933 5.5 ------ UNKNOWN
1.0977 -14.9686 1.0 7.2 -168.9 0.9031 11.7 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
58.316600 949.616600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
319.2355 -28.1924 2.8 40.8 96.4 9.5594 4.1 ------ UNKNOWN
17.4309 -35.7383 3.9 25.4 0.1 2.4472 2.9 ------ UNKNOWN
21.4603 25.6350 3.2 45.3 -121.4 10.3558 3.6 ------ UNKNOWN
Plot creation:
Sat Jul 30 07:01:06 EDT 2022