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
341.1816 -29.7446 0.0132 29.6778 55.4667 4.8690528 14.637 TRIG_00920783
Foreground time interval of the image:
-12.499 83.701 (delta_t = 96.200 [sec])
Background time interval of the image:
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 80.000000
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 80.000000
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 80.000000
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 -206.480 sec. to 341.552 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.61867 ( -0.105697 0.10657 )
Norm@50keV : 1.90910E-03 ( -0.000112469 0.000111916 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 44.33 using 59 PHA bins.
# Reduced chi-squared = 0.7778 for 57 degrees of freedom
# Null hypothesis probability = 8.895547e-01
Photon flux (15-150 keV) in 548 sec: 0.246776 ( -0.014475 0.014512 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.76383e-06 ( -6.15311e-07 6.19596e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -206.480 sec. to 341.552 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.61978 ( -0.108336 0.10545 )
Epeak [keV] : 9999.36 ( -9999.36 -9999.36 )
Norm@50keV : 1.90717E-03 ( -0.000345459 0.000885329 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 44.34 using 59 PHA bins.
# Reduced chi-squared = 0.7919 for 56 degrees of freedom
# Null hypothesis probability = 8.695895e-01
Photon flux (15-150 keV) in 548 sec: 0.247419 ( -0.017141 0.01528 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.79402e-06 ( -7.10159e-07 5.00605e-07 ) ergs/cm2
Band function
Time interval is from -206.480 sec. to 341.552 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] : 14.6248 ( )
R^2/D10^2 : 2.86187E-02 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 143.35 using 59 PHA bins.
# Reduced chi-squared = 2.5149 for 57 degrees of freedom
# Null hypothesis probability = 2.189413e-09
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.050e-07 8.028e-08
25- 50 2.736e-06 2.137e-07
50-150 3.936e-06 4.724e-07
15-150 7.377e-06 5.124e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 185.683 (-51.4997 -184.791)
Norm : 0.993794 (-0.059583 0.0696148)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 47.28 using 59 PHA bins.
# Reduced chi-squared = 0.8294 for 57 degrees of freedom
# Null hypothesis probability = 8.172047e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.368e-06 1.167e-07
25- 50 2.610e-06 4.776e-07
50-150 5.587e-06 2.419e-06
15-150 9.565e-06 2.939e-06
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.93061 (-0.912408 1.04722)
R1^2/D10^2 : 0.522425 (-0.239189 0.496574)
kT2 [keV] : 25.5590 (-3.59548 5.12926)
R2^2/D10^2 : 3.33537E-03 (-0.00156291 0.00241163)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 42.13 using 59 PHA bins.
# Reduced chi-squared = 0.7659 for 55 degrees of freedom
# Null hypothesis probability = 8.986681e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.520e-06 3.017e-07
25- 50 2.455e-06 3.567e-07
50-150 5.788e-06 1.163e-06
15-150 9.763e-06 1.422e-06
Peak spectrum fit
Power-law model
Time interval is from 151.572 sec. to 152.572 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.91730 ( -0.386008 0.446182 )
Norm@50keV : 8.86763E-03 ( -0.00275317 0.002649 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 73.17 using 59 PHA bins.
# Reduced chi-squared = 1.284 for 57 degrees of freedom
# Null hypothesis probability = 7.320159e-02
Photon flux (15-150 keV) in 1 sec: 1.28213 ( -0.324947 0.32498 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.15511e-08 ( -2.39846e-08 2.47824e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 151.572 sec. to 152.572 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.428527 ( -2.42453 1.56307 )
Epeak [keV] : 47.8596 ( )
Norm@50keV : 5.91427E-02 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 70.53 using 59 PHA bins.
# Reduced chi-squared = 1.259 for 56 degrees of freedom
# Null hypothesis probability = 9.157560e-02
Photon flux (15-150 keV) in 1 sec: 1.26699 ( -0.323326 0.32398 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.7707e-08 ( -2.30948e-08 2.48724e-08 ) ergs/cm2
Band function
Time interval is from 151.572 sec. to 152.572 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] : 11.4618 (-2.87412 3.79582)
R^2/D10^2 : 0.395365 (-0.260272 0.742498)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 72.56 using 59 PHA bins.
# Reduced chi-squared = 1.273 for 57 degrees of freedom
# Null hypothesis probability = 8.021661e-02
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.093e-08 5.406e-09
25- 50 3.255e-08 1.499e-08
50-150 2.490e-08 1.567e-08
15-150 6.838e-08 3.222e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 76.5134 (-36.807 113.062)
Norm : 6.31820 (-1.92802 2.64251)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 71.30 using 59 PHA bins.
# Reduced chi-squared = 1.251 for 57 degrees of freedom
# Null hypothesis probability = 9.639545e-02
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.634e-08 6.009e-09
25- 50 2.661e-08 1.326e-08
50-150 3.644e-08 3.006e-08
15-150 7.939e-08 4.862e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.09100 (-5.10156 -5.10156)
R1^2/D10^2 : 3.95476 (-3.93953 -3.93953)
kT2 [keV] : 15.7904 (-15.8055 -15.8055)
R2^2/D10^2 : 9.48760E-02 (-0.0945085 0.462146)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 70.09 using 59 PHA bins.
# Reduced chi-squared = 1.274 for 55 degrees of freedom
# Null hypothesis probability = 8.269122e-02
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.524e-08 8.290e-09
25- 50 2.746e-08 1.463e-08
50-150 3.570e-08 2.250e-08
15-150 7.839e-08 4.165e-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: 1.60223 ( -0.145627 0.147557 )
Norm@50keV : 3.10386E-03 ( -0.000276415 0.000274174 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 44.07 using 59 PHA bins.
# Reduced chi-squared = 0.7731 for 57 degrees of freedom
# Null hypothesis probability = 8.950154e-01
Photon flux (15-150 keV) in 96.2 sec: 0.399136 ( -0.0339467 0.0339762 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.7917e-06 ( -2.66552e-07 2.6909e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.24484 ( -0.646631 0.43159 )
Epeak [keV] : 99.9916 ( -38.2849 -99.9964 )
Norm@50keV : 4.80496E-03 ( -0.00190536 0.00561318 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 42.93 using 59 PHA bins.
# Reduced chi-squared = 0.7666 for 56 degrees of freedom
# Null hypothesis probability = 9.001611e-01
Photon flux (15-150 keV) in 96.2 sec: 0.393404 ( -0.035265 0.03515 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.7067e-06 ( -3.01068e-07 2.95344e-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) = 2.55e-06
S(50-100 keV) = 3.33e-06
T90 vs. Hardness ratio plot
T90 = 375.759999990463 sec.
Hardness ratio (energy fluence ratio) = 1.30588
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.14371
Count Ratio (50-100 keV) / (15-25 keV) = 0.893643
Mask shadow pattern
IMX = 3.230544599709423E-01, IMY = -4.694627845241600E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 80.000000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 80.000000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 80.000000
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:
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-12.499380 83.700610
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
326.2914 -28.0396 3.4 42.8 57.5 2.3256 3.4 ------ UNKNOWN
354.7226 15.3589 2.7 44.1 135.7 4.4944 4.3 ------ UNKNOWN
316.8564 -45.0342 2.6 50.1 33.8 3.1599 4.5 ------ UNKNOWN
341.1816 -29.7446 0.8 29.7 55.5 4.8692 14.6 ------ UNKNOWN
29.6782 -16.4251 2.3 16.6 -132.7 0.9628 5.1 ------ UNKNOWN
40.1332 23.3534 1.8 54.1 -167.0 4.2461 6.4 ------ UNKNOWN
45.6648 2.9771 2.5 41.1 -144.2 1.4731 4.6 ------ UNKNOWN
48.8767 -25.4627 2.7 31.5 -97.5 1.2209 4.3 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
97.900600 196.700610
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
343.9737 6.4639 2.8 40.8 115.5 2.9633 4.1 ------ UNKNOWN
341.1671 -29.7336 0.7 29.6 52.7 6.5193 17.5 ------ UNKNOWN
358.2333 -1.3642 2.3 25.7 127.0 1.5574 5.1 133.9 UNKNOWN
18.3420 -63.6454 2.0 41.2 -19.9 1.8194 5.8 ------ UNKNOWN
56.3678 4.7862 2.9 50.3 -134.0 4.3543 4.0 ------ UNKNOWN
Plot creation:
Wed Oct 9 18:11:01 EDT 2019