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
285.9741 -0.1348 0.0111 38.8815 99.0328 5.6639932 17.450 TRIG_00981957
Foreground time interval of the image:
-4.720 12.541 (delta_t = 17.261 [sec])
Background time interval of the image:
-239.760 -4.720 (delta_t = 235.040 [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 -4.720 sec. to 29.728 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.41368 ( -0.10433 0.104275 )
Norm@50keV : 1.58911E-02 ( -0.000950656 0.000950244 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 55.78 using 59 bins.
Reduced chi-squared = 0.978596
# Null hypothesis probability of 5.21e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 34.45 sec: 1.94137 ( -0.12232 0.12259 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.27595e-06 ( -3.39675e-07 3.40726e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -4.720 sec. to 29.728 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.09360 ( -0.439506 0.362882 )
Epeak [keV] : 152.810 ( -59.3132 -152.81 )
Norm@50keV : 2.25422E-02 ( -0.00712475 0.0133557 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 53.94 using 59 bins.
Reduced chi-squared = 0.963214
# Null hypothesis probability of 5.53e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 34.45 sec: 1.91208 ( -0.12759 0.12774 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.50639e-06 ( -4.60187e-07 4.49476e-06 ) ergs/cm2
Band function
Time interval is from -4.720 sec. to 29.728 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] : 17.0477 (-1.28255 1.41597)
R^2/D10^2 : 0.144209 (-0.0349438 0.0452998)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 110.96 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.48e-05 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.938e-07 3.665e-08
25- 50 1.303e-06 1.156e-07
50-150 2.706e-06 3.037e-07
15-150 4.303e-06 3.135e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-20.5511 -200)
Norm : 8.07922 (-0.483642 0.483642)
------------------------------------------------------------
#Fit statistic : Chi-Squared 60.21 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.60e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.931e-07 4.823e-08
25- 50 1.333e-06 1.061e-07
50-150 2.924e-06 5.362e-07
15-150 4.950e-06 6.597e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.59876 (-1.65329 1.87526)
R1^2/D10^2 : 1.38154 (-0.684831 1.79883)
kT2 [keV] : 28.1961 (-4.9217 8.82616)
R2^2/D10^2 : 2.05076E-02 (-0.0125422 0.0211729)
------------------------------------------------------------
#Fit statistic : Chi-Squared 54.77 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.84e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.682e-07 1.605e-07
25- 50 1.310e-06 2.933e-07
50-150 3.313e-06 9.343e-07
15-150 5.191e-06 1.392e-06
Peak spectrum fit
Power-law model
Time interval is from 0.196 sec. to 1.196 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.12337 ( -0.208574 0.205951 )
Norm@50keV : 6.62785E-02 ( -0.00847921 0.00847891 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 62.81 using 59 bins.
Reduced chi-squared = 1.10193
# Null hypothesis probability of 2.78e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.260764 ( 0.046159 0.209152 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.87939e-07 ( -9.72621e-08 9.80745e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.196 sec. to 1.196 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.120707 ( -1.11745 0.875767 )
Epeak [keV] : 99.8760 ( -27.8643 267.911 )
Norm@50keV : 0.200694 ( -0.122786 0.477005 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 58.89 using 59 bins.
Reduced chi-squared = 1.05161
# Null hypothesis probability of 3.70e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 7.47820 ( -1.02255 1.02361 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.49935e-07 ( -1.07659e-07 1.0648e-07 ) ergs/cm2
Band function
Time interval is from 0.196 sec. to 1.196 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] : 18.3088 (-2.66851 3.31704)
R^2/D10^2 : 0.501516 (-0.211417 0.340393)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 64.02 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.44e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.347e-08 8.495e-09
25- 50 1.568e-07 3.220e-08
50-150 3.831e-07 9.005e-08
15-150 5.733e-07 1.044e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-35.3282 -200)
Norm : 31.3471 (-4.12744 4.12744)
------------------------------------------------------------
#Fit statistic : Chi-Squared 72.05 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.65e-02 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.807e-08 4.391e-08
25- 50 1.502e-07 8.340e-08
50-150 3.294e-07 1.830e-07
15-150 5.576e-07 3.121e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 10.3887 (-4.29332 4.41045)
R1^2/D10^2 : 1.71496 (-0.952064 3.55021)
kT2 [keV] : 30.8514 (-13.8643 -35.4422)
R2^2/D10^2 : 6.10553E-02 (-0.039026 0.207325)
------------------------------------------------------------
#Fit statistic : Chi-Squared 57.40 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.86e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.708e-08 2.825e-08
25- 50 1.557e-07 8.455e-08
50-150 4.287e-07 2.449e-07
15-150 6.316e-07 3.318e-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: 1.32334 ( -0.119037 0.118309 )
Norm@50keV : 2.14896E-02 ( -0.00145648 0.00145647 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 61.45 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.20e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 17.26 sec: 2.57511 ( -0.183634 0.184027 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.64485e-06 ( -2.67306e-07 2.68186e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.16681 ( -0.473717 0.216981 )
Epeak [keV] : 289.301 ( -289.302 -289.302 )
Norm@50keV : 2.54922E-02 ( -0.0052496 0.0165645 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 61.08 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.99e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 17.26 sec: 2.55784 ( -0.18947 0.18969 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.61718e-06 ( -2.8246e-07 2.76988e-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) = 1.25e-06
S(50-100 keV) = 1.87e-06
T90 vs. Hardness ratio plot
T90 = 29.3600000143051 sec.
Hardness ratio (energy fluence ratio) = 1.496
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.46198
Count Ratio (50-100 keV) / (15-25 keV) = 1.23909
Mask shadow pattern
IMX = -1.265991246325264E-01, IMY = -7.963656060771516E-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:
-239.760000 -4.720000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
255.9618 -37.8590 1.5 44.2 25.9 4.4540 7.8 1.5 4U 1700-377
256.4958 -36.4453 4.3 44.1 28.0 1.6082 2.7 3.2 GX 349+2
262.8716 -24.6692 16.1 41.8 46.9 0.5026 0.7 8.8 GX 1+4
264.7212 -44.4878 3.4 37.4 16.2 -1.4650 -3.4 2.4 4U 1735-44
270.3692 -25.0877 4.4 35.3 50.0 -1.4456 -2.6 4.7 GX 5-1
270.2699 -25.6981 3.8 35.2 49.0 1.6620 3.1 3.2 GRS 1758-258
273.8809 -14.0736 10.5 37.4 69.2 -0.7643 -1.1 7.6 GX 17+2
276.1363 -30.4093 0.0 29.0 43.0 -0.6930 -1.9 11.2 H1820-303
284.9970 -24.7991 5.6 23.0 60.5 0.6781 2.1 7.6 HT1900.1-2455
263.0172 -33.6867 6.6 39.3 33.6 -0.9356 -1.8 9.0 GX 354-0
356.2436 4.8672 3.4 57.2 -161.6 5.9551 3.4 368.7 UNKNOWN
283.0635 -74.2808 4.0 44.7 -30.4 1.4429 2.9 ------ UNKNOWN
354.7084 -7.0685 2.8 48.3 -151.3 2.9547 4.1 529.3 UNKNOWN
229.2516 -73.6596 2.6 57.2 -21.2 5.3905 4.4 ------ UNKNOWN
353.7833 -26.2063 2.7 38.4 -127.2 2.3398 4.3 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-4.720000 12.540600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
255.9839 -37.8433 352.4 44.2 26.0 -0.0058 -0.0 0.1 4U 1700-377
256.5291 -36.5178 8.8 44.0 28.0 0.2448 1.3 7.3 GX 349+2
262.9366 -24.9522 13.6 41.7 46.5 -0.2056 -0.8 13.0 GX 1+4
264.7011 -44.5463 6.0 37.4 16.1 0.2149 1.9 6.0 4U 1735-44
270.3323 -25.0583 4.3 35.4 50.1 0.3795 2.7 2.9 GX 5-1
270.1944 -25.8568 23.5 35.2 48.7 0.0661 0.5 9.0 GRS 1758-258
273.9918 -14.1788 167.1 37.3 69.1 0.0156 0.1 8.6 GX 17+2
276.0599 -30.4562 6.5 29.0 42.9 0.1682 1.8 8.8 H1820-303
285.0098 -25.1307 0.0 22.9 59.8 0.0919 1.1 12.7 HT1900.1-2455
263.0941 -33.6368 0.0 39.2 33.7 -0.1304 -0.9 13.0 GX 354-0
285.9742 -0.1349 0.7 38.9 99.0 5.6935 17.3 ------ UNKNOWN
266.3600 -52.7351 3.4 37.8 2.6 0.3053 3.4 ------ UNKNOWN
266.5791 -53.3665 3.2 37.8 1.5 0.3193 3.5 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
147.740600 837.836500
900.240000 962.304300
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
244.9728 -15.6245 0.7 43.4 170.1 29.2401 16.7 1.0 Sco X-1
255.9877 -37.8633 2.9 46.8 135.9 13.7272 4.0 1.2 4U 1700-377
256.5677 -36.5288 10.0 45.5 136.7 -3.4182 -1.1 9.0 GX 349+2
263.0084 -24.7457 10.4 33.2 143.5 1.4592 1.1 0.0 GX 1+4
268.2659 -1.4306 5.3 17.9 -171.2 -1.7655 -2.2 6.3 SW J1753.5-0127
270.2182 -25.2269 13.4 29.4 133.2 1.1342 0.9 9.6 GX 5-1
270.2437 -25.7416 5.5 29.8 132.6 2.9659 2.2 3.2 GRS 1758-258
274.1884 -14.1513 43.3 18.3 142.5 -0.2346 -0.3 12.7 GX 17+2
275.9245 -30.3656 8.2 31.7 119.8 2.0453 1.4 0.1 H1820-303
285.2249 -25.0380 0.0 24.9 104.8 -0.7213 -0.6 12.5 HT1900.1-2455
288.7699 11.0361 24.0 11.5 -63.6 0.4221 0.5 5.7 GRS 1915+105
299.5684 35.2047 3.2 37.5 -58.8 6.3482 3.6 1.1 Cyg X-1
308.1294 40.8152 19.9 45.6 -53.6 2.1930 0.6 8.3 Cyg X-3
262.8325 -33.8611 16.8 40.1 133.5 1.6711 0.7 8.0 GX 354-0
323.8194 4.6316 3.1 38.0 5.3 4.6211 3.7 ------ UNKNOWN
251.0082 29.8059 3.4 44.9 -122.0 11.8314 3.4 ------ UNKNOWN
244.8921 27.0491 3.4 48.0 -129.1 15.4721 3.4 ------ UNKNOWN
Plot creation:
Mon Nov 16 12:42:50 EST 2020