Estimated redshift from machine learning (Ukwatta et al. 2016) - may take a few minutes to calcaulte
Image
Pre-slew 15-350 keV image (Event data; bkg subtracted)
# RAcent DECcent POSerr Theta Phi Peak Cts SNR Name
299.7104 +35.1411 0.0083 9.1 -5.4 3.0392 23.0 TRIG_00889443
------------------------------------------
Foreground time interval of the image:
-16.599 71.001 (delta_t = 87.600 [sec])
Background time interval of the image:
Lightcurves
Notes:
- 1) All plots contain as much data as has been downloaded to date.
- 2) The mask-weighted light curves are using the flight position.
- 3) Multiple plots of different time binning/intervals are shown to cover all scenarios of short/long GRBs, rate/image triggers, and real/false positives.
- 4) 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.
- 5) 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.
- 6) 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 64.000000
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 64.000000
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 64.000000
SN=5 or 10 sec. binning (whichever binning is satisfied first)
SN=5 or 10 sec. binning (T < 200 sec)
Spectra
Notes:
- 1) The fitting includes the systematic errors.
- 2) For long bursts, a spectral fit of 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.
- 4) For short bursts (T90<1sec), the specrtum is also fit with Blackbody, OTTB, and Double Blackbody.
Time averaged spectrum fit using the pre-slew DRM
Power-law model
Time interval is from -92.016 sec. to 145.620 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.74554 ( -0.111529 0.11361 )
Norm@50keV : 1.50595E-03 ( -0.000103424 0.000102497 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 63.03 using 59 PHA bins.
# Reduced chi-squared = 1.106 for 57 degrees of freedom
# Null hypothesis probability = 2.715407e-01
Photon flux (15-150 keV) in 237.6 sec: 0.203296 ( -0.01257 0.0125799 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.30254e-06 ( -2.35081e-07 2.37705e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -92.016 sec. to 145.620 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.950105 ( -0.548975 0.485429 )
Epeak [keV] : 59.7271 ( -9.6297 25.5469 )
Norm@50keV : 4.04762E-03 ( -0.00180473 0.00390535 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 54.64 using 59 PHA bins.
# Reduced chi-squared = 0.9757 for 56 degrees of freedom
# Null hypothesis probability = 5.265469e-01
Photon flux (15-150 keV) in 237.6 sec: 0.195006 ( -0.013442 0.013451 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.05076e-06 ( -2.67989e-07 2.75925e-07 ) ergs/cm2
Band function
Time interval is from -92.016 sec. to 145.620 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.950039 ( -0.364113 0.696644 )
beta : -10.0000 ( 10 1.77636e-15 )
Epeak [keV] : 59.7152 ( -9.63303 25.5439 )
Norm@50keV : 4.04771E-03 ( -0.00180473 0.00390757 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 54.64 using 59 PHA bins.
# Reduced chi-squared = 0.9934 for 55 degrees of freedom
# Null hypothesis probability = 4.884075e-01
Photon flux (15-150 keV) in 237.6 sec: 0.196310 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 3.06007e-06 ( 0 0 ) ergs/cm2
Single BB
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 12.1524 (-0.86702 0.944882)
R^2/D10^2 : 4.65646E-02 (-0.011239 0.0146639)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 90.89 using 59 PHA bins.
# Reduced chi-squared = 1.595 for 57 degrees of freedom
# Null hypothesis probability = 2.886921e-03
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.459e-07 3.635e-08
25- 50 1.105e-06 8.078e-08
50-150 9.892e-07 1.428e-07
15-150 2.440e-06 1.797e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 99.8785 (-15.9084 47.4527)
Norm : 0.900055 (-0.0934297 0.0673139)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 56.21 using 59 PHA bins.
# Reduced chi-squared = 0.9862 for 57 degrees of freedom
# Null hypothesis probability = 5.046452e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.590e-07 5.548e-08
25- 50 9.663e-07 7.271e-08
50-150 1.565e-06 4.682e-07
15-150 3.090e-06 5.346e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.11403 (-1.78713 1.96318)
R1^2/D10^2 : 0.323466 (-0.183613 0.801924)
kT2 [keV] : 18.6818 (-3.47492 6.61117)
R2^2/D10^2 : 7.31457E-03 (-0.00521133 0.0101528)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 55.93 using 59 PHA bins.
# Reduced chi-squared = 1.017 for 55 degrees of freedom
# Null hypothesis probability = 4.398235e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.120e-07 1.950e-07
25- 50 9.772e-07 2.591e-07
50-150 1.497e-06 5.332e-07
15-150 2.986e-06 9.113e-07
Peak spectrum fit
Power-law model
Time interval is from -91.364 sec. to -90.364 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 3.01853 ( -1.30401 2.22039 )
Norm@50keV : 2.11107E-03 ( -0.00211107 0.00315461 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 55.19 using 59 PHA bins.
# Reduced chi-squared = 0.9683 for 57 degrees of freedom
# Null hypothesis probability = 5.432265e-01
Photon flux (15-150 keV) in 1 sec: 0.588440 ( -0.29948 0.304912 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.55825e-08 ( -1.57187e-08 2.30959e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -91.364 sec. to -90.364 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -9.86866 ( 9.89981 11.9609 )
Epeak [keV] : 18.8867 ( -4.24808 4.49848 )
Norm@50keV : 1.18682E+08 ( -1.40715e+08 3.70583e+09 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 54.37 using 59 PHA bins.
# Reduced chi-squared = 0.9709 for 56 degrees of freedom
# Null hypothesis probability = 5.367105e-01
Photon flux (15-150 keV) in 1 sec: 0.582788 ( -0.294497 0.307398 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.3843e-16 ( 0 0 ) ergs/cm2
Band function
Time interval is from -91.364 sec. to -90.364 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 4.32852 ( 1.76306 1.76306 )
beta : -4.79218 ( 3.17773 1.44089 )
Epeak [keV] : 17.7636 ( -5.71306 -5.71306 )
Norm@50keV : 2817.08 ( -2816.57 7.19929e+06 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 54.66 using 59 PHA bins.
# Reduced chi-squared = 0.9938 for 55 degrees of freedom
# Null hypothesis probability = 4.875245e-01
Photon flux (15-150 keV) in 1 sec: 0.226692 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 1.43875e-08 ( 0 0 ) ergs/cm2
Single BB
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 3.94539 (-1.47722 2.76678)
R^2/D10^2 : 15.4293 (-15.4351 195.48)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 55.15 using 59 PHA bins.
# Reduced chi-squared = 0.9676 for 57 degrees of freedom
# Null hypothesis probability = 5.447364e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.312e-08 8.075e-09
25- 50 4.555e-09 3.328e-09
50-150 5.093e-11 7.535e-11
15-150 1.773e-08 1.110e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 12.2329 (-7.75995 91.1818)
Norm : 13.1688 (-13.1644 118.481)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 55.45 using 59 PHA bins.
# Reduced chi-squared = 0.9729 for 57 degrees of freedom
# Null hypothesis probability = 5.332446e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.219e-08 7.450e-09
25- 50 6.740e-09 4.906e-09
50-150 7.687e-10 8.750e-10
15-150 1.970e-08 1.278e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 3.68878 (-3.64498 2.45014)
R1^2/D10^2 : 20.0863 (-20.6038 551.638)
kT2 [keV] : 25.6547 (-25.3625 -25.3625)
R2^2/D10^2 : 4.48504E-03 (-0.00462541 -0.00462541)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 53.92 using 59 PHA bins.
# Reduced chi-squared = 0.9803 for 55 degrees of freedom
# Null hypothesis probability = 5.160721e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.267e-08 8.305e-09
25- 50 6.371e-09 3.450e-09
50-150 1.415e-08 1.114e-08
15-150 3.320e-08 1.982e-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: 1.85512 ( -0.144116 0.149062 )
Norm@50keV : 1.70344E-03 ( -0.000161684 0.000159234 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 57.81 using 59 PHA bins.
# Reduced chi-squared = 1.014 for 57 degrees of freedom
# Null hypothesis probability = 4.450773e-01
Photon flux (15-150 keV) in 87.6 sec: 0.239936 ( -0.0187847 0.0187893 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.37197e-06 ( -1.29254e-07 1.31541e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.10741 ( -0.711706 0.606862 )
Epeak [keV] : 51.2353 ( -10.2528 38.774 )
Norm@50keV : 4.49291E-03 ( -0.00241065 0.00678187 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 53.24 using 59 PHA bins.
# Reduced chi-squared = 0.9507 for 56 degrees of freedom
# Null hypothesis probability = 5.800397e-01
Photon flux (15-150 keV) in 87.6 sec: 0.231879 ( -0.019762 0.019786 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.26771e-06 ( -1.45171e-07 1.52722e-07 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.10737 ( -0.467106 0.905404 )
beta : -10.0000 ( 10 20 )
Epeak [keV] : 51.2252 ( -10.2315 38.755 )
Norm@50keV : 4.49276E-03 ( -0.00251919 0.00679236 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 53.24 using 59 PHA bins.
# Reduced chi-squared = 0.9680 for 55 degrees of freedom
# Null hypothesis probability = 5.421837e-01
Photon flux (15-150 keV) in 87.6 sec: 0.233645 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 1.26973e-06 ( 0 0 ) ergs/cm2
S(25-50 keV) vs. S(50-100 keV) plot
S(25-50 keV) = 9.11e-07
S(50-100 keV) = 1.09e-06
T90 vs. Hardness ratio plot
T90 = 197.503999948502 sec.
Hardness ratio (energy fluence ratio) = 1.19649
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.3045
Count Ratio (50-100 keV) / (15-25 keV) = 0.761589
Mask shadow pattern
IMX = 1.595078730756845E-01, IMY = 1.494283711746114E-02
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 64.000000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 64.000000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 64.000000
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:
-16.599400 71.000590
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.3327 35.4784 309.8 41.8 45.9 -0.0150 -0.0 10.2 Her X-1
268.2414 -1.4678 9.2 56.1 -3.6 -0.6508 -1.3 7.6 SW J1753.5-0127
288.9337 10.9960 5.8 34.8 -19.7 0.3776 2.0 8.5 GRS 1915+105
299.7104 35.1411 0.5 9.1 -5.4 3.0390 23.0 6.9 Cyg X-1
308.0305 40.7803 8.9 0.7 -51.5 -0.1833 -1.3 11.0 Cyg X-3
325.9451 38.3596 7.1 14.0 -137.2 0.2392 1.6 10.9 Cyg X-2
30.0719 75.2330 2.9 48.2 145.7 2.2616 4.0 ------ UNKNOWN
34.3156 64.0989 2.4 51.9 159.6 2.6007 4.7 ------ UNKNOWN
0.0587 27.1689 2.6 44.5 -142.4 1.4640 4.4 ------ UNKNOWN
2.6854 20.0003 2.2 50.6 -136.4 3.7982 5.2 ------ UNKNOWN
318.5993 0.2291 2.2 42.3 -69.8 3.2205 5.1 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
101.200600 368.563400
370.000000 963.081500
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.2544 35.2874 0.0 36.8 52.2 -4.0478 -2.2 10.5 Her X-1
268.2954 -1.4729 3.7 46.9 -6.2 -4.5464 -3.1 4.5 SW J1753.5-0127
273.9964 -14.0173 4.7 54.9 -20.7 5.6044 2.5 1.3 GX 17+2
288.8164 10.9822 1.9 26.1 -26.8 5.3063 6.2 2.4 GRS 1915+105
299.5898 35.2070 0.3 0.1 79.9 30.1212 40.0 0.3 Cyg X-1
308.1536 40.9459 7.0 8.8 174.8 1.3564 1.6 2.0 Cyg X-3
325.9333 38.3935 0.0 21.2 -158.2 0.5351 0.6 12.0 Cyg X-2
313.5920 61.5864 2.4 27.9 142.5 5.2129 4.8 ------ UNKNOWN
308.4472 46.0832 3.3 12.8 156.9 2.3712 3.5 ------ UNKNOWN
283.0839 17.5717 3.0 22.9 -7.3 3.0790 3.9 ------ UNKNOWN
265.0134 -11.8416 3.0 57.3 -10.2 13.0518 3.9 ------ UNKNOWN
285.8505 3.2277 2.2 34.4 -26.6 5.3872 5.2 ------ UNKNOWN
269.4080 -16.9780 2.6 59.5 -17.6 20.6122 4.4 ------ UNKNOWN
Plot creation:
Mon Feb 18 20:37:36 EST 2019