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
238.1466 -50.8480 0.0232 26.1096 -67.7966 2.3545221 8.236 TRIG_01152509
Foreground time interval of the image:
-23.912 72.301 (delta_t = 96.213 [sec])
Background time interval of the image:
-239.000 -23.912 (delta_t = 215.088 [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
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)
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 -23.912 sec. to 195.592 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.69844 ( -0.134436 0.136454 )
Norm@50keV : 1.86314E-03 ( -0.000151776 0.000150462 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 40.16 using 59 bins.
Reduced chi-squared = 0.704561
# Null hypothesis probability of 9.56e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 219.5 sec: 0.247322 ( -0.019022 0.019048 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.78752e-06 ( -3.22507e-07 3.25918e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -23.912 sec. to 195.592 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.21963 ( -0.597772 0.520033 )
Epeak [keV] : 75.9345 ( -20.927 -75.9345 )
Norm@50keV : 3.35086E-03 ( -0.00153343 0.00352515 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 37.72 using 59 bins.
Reduced chi-squared = 0.673571
# Null hypothesis probability of 9.71e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 219.5 sec: 0.241619 ( -0.020038 0.020021 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.62146e-06 ( -3.67114e-07 3.71032e-07 ) ergs/cm2
Band function
Time interval is from -23.912 sec. to 195.592 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] : 12.7279 (-1.18395 1.32704)
R^2/D10^2 : 4.78128E-02 (-0.0146039 0.020737)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 72.66 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.90e-02 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.606e-07 5.125e-08
25- 50 1.214e-06 1.164e-07
50-150 1.227e-06 2.085e-07
15-150 2.801e-06 2.656e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 133.424 (-38.8245 60.2114)
Norm : 1.02502 (-0.0927204 0.12021)
------------------------------------------------------------
#Fit statistic : Chi-Squared 37.81 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.77e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.829e-07 6.058e-08
25- 50 1.061e-06 1.519e-07
50-150 1.991e-06 7.836e-07
15-150 3.635e-06 9.307e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.47449 (-1.54817 1.8275)
R1^2/D10^2 : 0.359839 (-0.199084 0.592656)
kT2 [keV] : 22.1216 (-4.6508 9.33568)
R2^2/D10^2 : 4.83854E-03 (-0.00354973 0.00754952)
------------------------------------------------------------
#Fit statistic : Chi-Squared 37.50 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.66e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.828e-07 2.145e-07
25- 50 1.079e-06 3.178e-07
50-150 1.932e-06 8.575e-07
15-150 3.594e-06 1.207e-06
Peak spectrum fit
Power-law model
Time interval is from 148.108 sec. to 149.108 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.990223 ( -0.535143 0.464219 )
Norm@50keV : 7.70987E-03 ( -0.00198826 0.00188446 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 49.31 using 59 bins.
Reduced chi-squared = 0.865088
# Null hypothesis probability of 7.56e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.887176 ( -0.22611 0.228324 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.367e-08 ( -2.08005e-08 2.0932e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 148.108 sec. to 149.108 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.00920 ( -0.563065 0.445249 )
Epeak [keV] : 9999.36 ( -9999.36 -9999.36 )
Norm@50keV : 7.78540E-03 ( -0.00201453 0.0105792 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 49.33 using 59 bins.
Reduced chi-squared = 0.880893
# Null hypothesis probability of 7.24e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.907019 ( -0.246117 0.208321 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.37009e-08 ( -2.08748e-08 2.0877e-08 ) ergs/cm2
Band function
Time interval is from 148.108 sec. to 149.108 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] : 27.3145 (-10.3829 25.132)
R^2/D10^2 : 1.53746E-02 (-0.0151175 0.0520388)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 56.41 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.97e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.898e-09 1.151e-09
25- 50 1.124e-08 6.745e-09
50-150 6.106e-08 3.767e-08
15-150 7.420e-08 4.235e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-77.3957 -200)
Norm : 3.76244 (-0.923743 0.923743)
------------------------------------------------------------
#Fit statistic : Chi-Squared 54.06 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.86e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.376e-09 5.470e-09
25- 50 1.804e-08 1.069e-08
50-150 3.955e-08 2.324e-08
15-150 6.697e-08 3.966e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 8.84779 (-3.85554 5.78304)
R1^2/D10^2 : 0.437120 (-0.360057 2.94285)
kT2 [keV] : 99.9865 (-74.1968 -100.003)
R2^2/D10^2 : 6.26900E-04 (-0.000542255 0.00827355)
------------------------------------------------------------
#Fit statistic : Chi-Squared 47.31 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.60e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.984e-09 4.342e-09
25- 50 1.674e-08 1.039e-08
50-150 6.531e-08 6.115e-08
15-150 8.903e-08 5.755e-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: 1.69332 ( -0.263151 0.271054 )
Norm@50keV : 1.64087E-03 ( -0.000264805 0.000259363 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 70.32 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.11e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 96.21 sec: 0.217420 ( -0.0323086 0.0323755 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.46246e-06 ( -2.44884e-07 2.49525e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.55523 ( -1.05308 0.891506 )
Epeak [keV] : 150.176 ( -150.176 -150.176 )
Norm@50keV : 1.94679E-03 ( -0.000565921 0.00504185 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 70.25 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.53e-02 with 56 degrees of freedom
Photon flux (15-150 keV) in 96.21 sec: 0.216116 ( -0.03221 0.033179 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.44447e-06 ( -2.73458e-07 2.63134e-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) = 1.03e-06
S(50-100 keV) = 1.26e-06
T90 vs. Hardness ratio plot
T90 = 186.192000031471 sec.
Hardness ratio (energy fluence ratio) = 1.2233
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.27704
Count Ratio (50-100 keV) / (15-25 keV) = 0.849996
Mask shadow pattern
IMX = 1.852074809784956E-01, IMY = 4.537608147384308E-01
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:
-239.000000 -23.912000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
170.1768 -60.7970 7.6 37.0 5.6 -0.8319 -1.5 11.2 Cen X-3
187.0876 -62.7515 273.1 32.1 -6.0 0.0197 0.0 11.9 GX 301-2
244.9990 -15.6635 0.9 36.1 -138.1 7.4510 13.0 1.8 Sco X-1
256.0270 -37.7962 4.4 36.7 -96.8 2.7646 2.6 3.5 4U 1700-377
256.5214 -36.3542 6.6 37.3 -99.0 1.9990 1.7 5.9 GX 349+2
180.1912 -4.3033 3.3 41.0 104.0 4.3804 3.5 ------ UNKNOWN
176.5046 -17.0824 3.4 34.8 84.8 3.1394 3.4 ------ UNKNOWN
227.2085 -85.9290 1.9 52.0 -27.5 9.2104 6.1 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-23.912000 72.300580
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
170.2537 -60.6242 2.8 36.9 5.8 1.0707 4.2 1.8 Cen X-3
186.4569 -62.6820 4.1 32.2 -5.5 0.6043 2.8 7.6 GX 301-2
244.9289 -15.6266 4.2 36.1 -138.2 0.9219 2.8 3.0 Sco X-1
256.0616 -37.7233 15.9 36.7 -96.9 -0.4751 -0.7 8.1 4U 1700-377
256.2415 -36.3093 4.9 37.1 -99.1 1.6083 2.4 11.6 GX 349+2
193.5567 -24.5071 2.2 17.6 92.9 1.1061 5.2 ------ UNKNOWN
219.8678 -71.6818 2.6 37.9 -30.8 1.2617 4.5 ------ UNKNOWN
238.1466 -50.8480 1.4 26.1 -67.8 2.3533 8.2 ------ UNKNOWN
258.5702 -40.0039 2.3 38.4 -92.7 3.8390 5.0 ------ UNKNOWN
256.0111 -5.4309 2.2 51.0 -139.7 4.5134 5.2 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
134.700610 963.182900
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
170.4414 -60.4834 6.8 37.6 46.3 4.5266 1.7 9.2 Cen X-3
186.3894 -62.8434 2.7 29.7 44.1 8.1333 4.2 8.5 GX 301-2
244.9862 -15.6405 1.0 35.6 -170.9 22.5541 11.5 0.4 Sco X-1
255.9997 -37.8662 6.0 18.1 -131.2 3.0249 1.9 1.5 4U 1700-377
256.5754 -36.3251 3.1 19.6 -132.9 5.5814 3.7 9.0 GX 349+2
262.8909 -24.8614 6.3 32.2 -136.8 3.4533 1.8 9.5 GX 1+4
264.9988 -44.5249 16.8 19.0 -101.2 1.1195 0.7 11.8 4U 1735-44
270.3500 -25.1306 6.0 35.6 -126.3 4.7078 1.9 4.7 GX 5-1
270.3315 -25.6009 4.2 35.2 -125.8 6.4883 2.7 8.7 GRS 1758-258
274.1705 -14.1138 4.0 46.8 -130.8 15.0537 2.9 10.7 GX 17+2
275.7545 -30.4001 11.3 34.5 -114.0 -2.5781 -1.0 9.0 H1820-303
262.7984 -33.8152 6.1 24.7 -126.3 2.7872 1.9 9.6 GX 354-0
189.0730 -41.0398 3.7 34.8 84.7 11.0183 3.1 ------ UNKNOWN
38.2195 -72.7541 2.7 55.6 -9.2 12.7141 4.3 ------ UNKNOWN
Plot creation:
Fri Jun 16 09:15:20 EDT 2023