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
270.6416 24.4948 0.0033 34.9447 -37.6417 4.4226708 59.071 TRIG_01208389
Foreground time interval of the image:
-0.376 7.216 (delta_t = 7.592 [sec])
Background time interval of the image:
-239.696 -0.376 (delta_t = 239.320 [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 0.512000
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 0.512000
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 0.512000
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 -0.376 sec. to 7.216 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.93891 ( -0.0526961 0.0530798 )
Norm@50keV : 3.51744E-02 ( -0.00102182 0.00101983 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 67.00 using 59 bins.
Reduced chi-squared = 1.17544
# Null hypothesis probability of 1.71e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 7.592 sec: 5.13370 ( -0.16296 0.16364 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.45717e-06 ( -7.04276e-08 7.04721e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.376 sec. to 7.216 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.48411 ( -0.236798 0.224357 )
Epeak [keV] : 57.1622 ( -6.61885 10.8724 )
Norm@50keV : 5.89337E-02 ( -0.0129751 0.0178308 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 54.44 using 59 bins.
Reduced chi-squared = 0.972143
# Null hypothesis probability of 5.34e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 7.592 sec: 4.95570 ( -0.18157 0.1826 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.37655e-06 ( -8.06825e-08 8.04593e-08 ) ergs/cm2
Band function
Time interval is from -0.376 sec. to 7.216 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] : 12.6974 ( )
R^2/D10^2 : 0.923936 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 296.79 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.95e-34 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.398e-07 1.272e-08
25- 50 8.051e-07 2.733e-08
50-150 8.092e-07 4.950e-08
15-150 1.854e-06 5.808e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 87.9150 (-7.94851 9.25433)
Norm : 22.7573 (-1.07428 1.13771)
------------------------------------------------------------
#Fit statistic : Chi-Squared 55.75 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.22e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.505e-07 2.004e-08
25- 50 7.579e-07 2.213e-08
50-150 1.138e-06 6.036e-08
15-150 2.346e-06 7.288e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.21772 (-0.786727 0.814841)
R1^2/D10^2 : 5.44236 (-1.61468 2.68707)
kT2 [keV] : 23.3061 (-2.75885 3.85292)
R2^2/D10^2 : 6.35740E-02 (-0.0289497 0.0441483)
------------------------------------------------------------
#Fit statistic : Chi-Squared 67.33 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.23e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.038e-07 4.153e-08
25- 50 7.758e-07 4.840e-08
50-150 1.142e-06 1.139e-07
15-150 2.322e-06 1.852e-07
Peak spectrum fit
Power-law model
Time interval is from 0.128 sec. to 1.128 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.96183 ( -0.0713177 0.0723254 )
Norm@50keV : 8.45518E-02 ( -0.00359542 0.00357808 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 55.23 using 59 bins.
Reduced chi-squared = 0.968947
# Null hypothesis probability of 5.42e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 12.4662 ( -0.5278 0.5292 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.78538e-07 ( -3.22611e-08 3.23484e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.128 sec. to 1.128 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.45639 ( -0.310478 0.289208 )
Epeak [keV] : 52.2749 ( -7.97027 11.8639 )
Norm@50keV : 0.153601 ( -0.0435334 0.0668204 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 45.85 using 59 bins.
Reduced chi-squared = 0.81875
# Null hypothesis probability of 8.31e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 12.0957 ( -0.5633 0.5651 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.52575e-07 ( -3.56231e-08 3.55589e-08 ) ergs/cm2
Band function
Time interval is from 0.128 sec. to 1.128 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] : 11.9072 ( )
R^2/D10^2 : 2.90398 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 182.04 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.52e-15 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.702e-08 6.550e-09
25- 50 2.714e-07 1.265e-08
50-150 2.302e-07 2.045e-08
15-150 5.885e-07 2.625e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 81.6290 (-9.65863 11.7551)
Norm : 57.1355 (-3.65954 3.95079)
------------------------------------------------------------
#Fit statistic : Chi-Squared 46.42 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.40e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.484e-07 9.200e-09
25- 50 2.455e-07 1.050e-08
50-150 3.513e-07 2.815e-08
15-150 7.453e-07 3.245e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.62132 (-0.849909 0.884608)
R1^2/D10^2 : 18.6290 (-6.56381 12.0995)
kT2 [keV] : 21.7131 (-2.74624 3.75282)
R2^2/D10^2 : 0.206534 (-0.0992299 0.159867)
------------------------------------------------------------
#Fit statistic : Chi-Squared 49.04 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.00e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.415e-07 1.700e-08
25- 50 2.464e-07 2.530e-08
50-150 3.553e-07 5.815e-08
15-150 7.433e-07 9.160e-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: 1.93891 ( -0.0526961 0.0530798 )
Norm@50keV : 3.51744E-02 ( -0.00102182 0.00101983 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 67.00 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.71e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 7.592 sec: 5.13336 ( -0.162936 0.16361 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.45675e-06 ( -7.04253e-08 7.0486e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.48410 ( -0.236797 0.224357 )
Epeak [keV] : 57.1620 ( -6.61885 10.8724 )
Norm@50keV : 5.89341E-02 ( -0.0129751 0.0178308 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 54.44 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.34e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 7.592 sec: 4.95470 ( -0.18146 0.18249 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.37719e-06 ( -8.08244e-08 8.03537e-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) = 7.26e-07
S(50-100 keV) = 7.58e-07
T90 vs. Hardness ratio plot
T90 = 4.92399990558624 sec.
Hardness ratio (energy fluence ratio) = 1.04408
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.21043
Count Ratio (50-100 keV) / (15-25 keV) = 0.695337
Mask shadow pattern
IMX = 5.533171433505845E-01, IMY = 4.267536605397633E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.512000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.512000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.512000
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:
-239.696000 -0.376000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.5052 35.3786 3.0 41.2 -10.6 1.9548 3.9 3.2 Her X-1
288.9103 10.8357 14.1 35.0 -76.7 0.4461 0.8 9.3 GRS 1915+105
299.5719 35.1831 1.9 9.0 -64.4 1.9822 5.9 1.4 Cyg X-1
308.1563 41.0236 4.8 1.0 -144.9 0.8171 2.4 4.7 Cyg X-3
326.2367 38.1179 0.0 14.9 168.6 -0.3048 -0.9 12.6 Cyg X-2
320.7866 73.4280 2.7 32.2 77.5 3.2262 4.2 ------ UNKNOWN
244.2249 34.8683 2.3 48.9 -5.9 3.0213 5.1 ------ UNKNOWN
318.9294 -3.7499 3.0 46.8 -125.5 5.5869 3.9 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-0.376000 7.216000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.5048 35.2668 6.0 41.2 -10.7 -0.1580 -1.9 5.1 Her X-1
288.6827 11.0322 4.9 34.9 -76.2 0.2561 2.3 8.6 GRS 1915+105
299.7196 35.0181 0.0 9.1 -65.6 0.1091 2.0 12.7 Cyg X-1
307.9917 41.1449 0.0 0.8 -142.6 -0.0792 -1.4 12.7 Cyg X-3
326.3016 38.4004 4.9 14.8 167.5 -0.1341 -2.4 7.7 Cyg X-2
8.8234 42.9839 2.6 44.3 137.2 0.7792 4.4 ------ UNKNOWN
270.6416 24.4948 0.2 34.9 -37.6 4.4226 59.1 ------ UNKNOWN
351.0469 -2.8282 2.5 59.6 -162.7 1.6350 4.6 563.1 UNKNOWN
289.0376 4.2170 2.5 41.0 -81.0 1.0836 4.5 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
96.804600 236.004590
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
244.9747 -15.6330 3.1 47.3 -27.3 1.4526 3.8 0.5 Sco X-1
254.6804 35.2928 17.3 17.5 70.0 -0.1680 -0.7 11.3 Her X-1
268.3684 -1.4488 41.5 26.0 -56.8 0.0691 0.3 0.2 SW J1753.5-0127
273.9189 -14.0756 22.3 38.7 -67.0 0.2311 0.5 5.6 GX 17+2
288.7202 10.7489 0.0 22.0 -116.5 0.4624 2.0 12.7 GRS 1915+105
299.5536 35.2493 3.7 27.2 178.0 0.7268 3.1 3.4 Cyg X-1
308.1087 40.8287 11.3 35.2 171.1 0.2917 1.0 7.4 Cyg X-3
326.1219 38.3191 4.8 48.6 177.6 -1.4233 -2.4 2.3 Cyg X-2
240.7361 45.7608 3.5 32.1 77.2 1.5656 3.3 ------ UNKNOWN
264.6045 41.5587 2.9 17.8 103.3 0.9969 3.9 ------ UNKNOWN
302.0962 39.0631 2.7 30.3 171.7 1.0633 4.3 ------ UNKNOWN
254.8820 -4.8748 2.0 33.1 -32.2 1.4360 5.6 ------ UNKNOWN
255.7890 -16.0847 3.2 43.0 -40.8 1.4041 3.6 ------ UNKNOWN
Plot creation:
Sat Mar 9 15:16:43 EST 2024