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
295.2250 -76.9432 0.0156 47.2375 -44.6527 4.1406216 12.351 TRIG_01071488
Foreground time interval of the image:
29.736 73.301 (delta_t = 43.565 [sec])
Background time interval of the image:
-144.499 29.736 (delta_t = 174.235 [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 29.736 sec. to 84.632 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.06608 ( -0.168731 0.176853 )
Norm@50keV : 6.05428E-03 ( -0.00069844 0.000684822 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 49.85 using 59 bins.
Reduced chi-squared = 0.874561
# Null hypothesis probability of 7.38e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 54.9 sec: 0.936936 ( -0.087581 0.087664 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.07937e-06 ( -3.2494e-07 3.29825e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from 29.736 sec. to 84.632 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.49451 ( -0.876315 0.691901 )
Epeak [keV] : 36.8144 ( -31.723 -36.8151 )
Norm@50keV : 1.29630E-02 ( -0.00751068 0.0295694 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 47.91 using 59 bins.
Reduced chi-squared = 0.855536
# Null hypothesis probability of 7.71e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 54.9 sec: 0.917088 ( -0.091054 0.090942 ) ph/cm2/s
Energy fluence (15-150 keV) : 0 ( 0 0 ) ergs/cm2
Band function
Time interval is from 29.736 sec. to 84.632 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] : 9.25752 (-0.951974 1.08328)
R^2/D10^2 : 0.580082 (-0.205579 0.31244)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 66.44 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.84e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.388e-07 8.534e-08
25- 50 1.196e-06 1.414e-07
50-150 4.971e-07 1.360e-07
15-150 2.232e-06 2.492e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 59.9096 (-14.3613 21.3402)
Norm : 4.90101 (-0.752027 0.868059)
------------------------------------------------------------
#Fit statistic : Chi-Squared 47.96 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.98e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.761e-07 8.729e-08
25- 50 1.028e-06 1.054e-07
50-150 1.169e-06 2.959e-07
15-150 2.873e-06 3.475e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.01466 (-1.22027 1.17932)
R1^2/D10^2 : 1.42193 (-0.61967 1.32742)
kT2 [keV] : 27.2549 (-9.3398 25.3191)
R2^2/D10^2 : 5.35074E-03 (-0.00465101 0.0193356)
------------------------------------------------------------
#Fit statistic : Chi-Squared 43.84 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.60e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.546e-07 1.746e-07
25- 50 1.064e-06 3.058e-07
50-150 1.299e-06 6.642e-07
15-150 3.018e-06 1.003e-06
Peak spectrum fit
Power-law model
Time interval is from 60.636 sec. to 61.636 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.10593 ( -0.357699 0.387491 )
Norm@50keV : 1.40055E-02 ( -0.0043504 0.00428514 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 70.90 using 59 bins.
Reduced chi-squared = 1.24386
# Null hypothesis probability of 1.02e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 2.21130 ( -0.63192 0.63472 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.30122e-07 ( -3.8183e-08 3.85877e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 60.636 sec. to 61.636 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -4.07470 ( 2.85343 3.04592 )
Epeak [keV] : 35.4349 ( -6.98901 9.39692 )
Norm@50keV : 107.687 ( -114.624 1.34203e+06 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 59.12 using 59 bins.
Reduced chi-squared = 1.05571
# Null hypothesis probability of 3.62e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 2.36947 ( -0.62646 0.62805 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.20492e-07 ( -3.56599e-08 3.91621e-08 ) ergs/cm2
Band function
Time interval is from 60.636 sec. to 61.636 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] : 9.72307 (-1.78714 2.27899)
R^2/D10^2 : 1.49136 (-0.87575 1.82323)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 59.93 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.70e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.842e-08 1.179e-08
25- 50 6.788e-08 2.612e-08
50-150 3.264e-08 1.792e-08
15-150 1.289e-07 5.004e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 52.9720 (-19.7679 40.3572)
Norm : 13.5894 (-4.64073 6.14534)
------------------------------------------------------------
#Fit statistic : Chi-Squared 65.83 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.98e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.365e-08 1.172e-08
25- 50 4.930e-08 1.655e-08
50-150 5.050e-08 3.010e-08
15-150 1.334e-07 4.937e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 8.81575 (-8.56888 -8.56888)
R1^2/D10^2 : 1.83113 (-0.755389 -0.755389)
kT2 [keV] : 16.5362 (-10.3916 -10.3916)
R2^2/D10^2 : 3.97110E-02 (-0.0391108 3.16271)
------------------------------------------------------------
#Fit statistic : Chi-Squared 59.69 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.09e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.862e-08 4.866e-05
25- 50 6.754e-08 4.795e-04
50-150 3.344e-08 1.034e-02
15-150 1.296e-07 1.144e-02
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: 2.01982 ( -0.16724 0.174753 )
Norm@50keV : 6.97490E-03 ( -0.000789555 0.000774785 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 54.67 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.63e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 43.56 sec: 1.05589 ( -0.0993705 0.0994683 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.80502e-06 ( -2.96833e-07 3.00609e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.48115 ( -0.807804 0.647737 )
Epeak [keV] : 40.9121 ( -40.7455 -40.9121 )
Norm@50keV : 1.41724E-02 ( -0.0079779 0.0275813 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 52.70 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.00e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 43.56 sec: 1.03493 ( -0.102519 0.10252 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.67079e-06 ( -3.39663e-07 3.41929e-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) = 9.44e-07
S(50-100 keV) = 9.00e-07
T90 vs. Hardness ratio plot
T90 = 46.7840000391006 sec.
Hardness ratio (energy fluence ratio) = 0.95339
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.22729
Count Ratio (50-100 keV) / (15-25 keV) = 0.609051
Mask shadow pattern
IMX = 7.692286945106462E-01, IMY = 7.599590648781670E-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:
-144.499400 29.736000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
9.8549 -0.3670 3.3 39.2 128.2 1.8558 3.5 591.7 UNKNOWN
296.8341 -41.9883 2.4 49.7 2.6 2.1873 4.8 ------ UNKNOWN
16.5283 -36.7909 2.5 10.3 -160.7 0.8687 4.6 ------ UNKNOWN
60.2280 -10.2986 3.0 57.6 -165.4 3.7158 3.9 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
29.736000 73.300600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
317.6714 -66.0190 1.9 37.3 -32.4 0.8808 6.0 ------ UNKNOWN
295.2251 -76.9432 0.9 47.2 -44.7 4.1405 12.4 ------ UNKNOWN
10.0043 -83.6700 2.9 44.6 -62.3 1.7438 3.9 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
137.900600 710.673600
721.000000 840.300000
841.000000 963.070000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
170.2558 -60.6215 10.9 38.3 -97.2 2.3820 1.1 1.8 Cen X-3
186.6179 -62.7371 3.2 33.7 -86.0 4.8989 3.6 2.3 GX 301-2
255.9180 -37.9713 13.6 42.5 -5.4 -0.9300 -0.9 8.3 4U 1700-377
256.3659 -36.4342 5.1 43.9 -4.4 2.8556 2.3 3.4 GX 349+2
262.9194 -24.7800 12.1 54.4 5.7 -2.9541 -1.0 5.3 GX 1+4
264.7729 -44.4540 12.0 34.8 2.9 1.0011 1.0 1.3 4U 1735-44
270.3286 -25.2208 25.3 53.1 13.9 1.3102 0.5 8.8 GX 5-1
270.2098 -25.7894 7.1 52.5 13.6 4.4006 1.6 5.7 GRS 1758-258
276.1432 -30.4548 0.0 47.3 19.8 -1.5264 -0.9 12.5 H1820-303
284.9071 -24.9615 14.6 52.2 30.5 3.8831 0.8 7.4 HT1900.1-2455
262.8771 -33.8945 9.1 45.4 3.7 -1.6810 -1.3 6.6 GX 354-0
318.2809 -38.0192 6.0 40.1 70.9 6.4377 1.9 ------ UNKNOWN
294.1636 -39.3492 2.9 37.6 41.0 5.4675 4.0 ------ UNKNOWN
280.1840 -33.3432 3.4 44.1 24.2 4.7246 3.4 ------ UNKNOWN
288.9613 -51.4828 3.4 25.5 33.2 2.7543 3.4 ------ UNKNOWN
257.2214 -31.0889 2.5 49.0 -2.0 6.0577 4.7 ------ UNKNOWN
256.4327 -52.3724 2.7 28.5 -11.1 3.1895 4.4 ------ UNKNOWN
255.6378 -78.2979 3.7 8.5 -75.9 2.0038 3.1 ------ UNKNOWN
243.9805 -31.5515 3.0 50.9 -16.6 6.2399 3.9 ------ UNKNOWN
240.4027 -28.6784 3.8 54.4 -19.5 6.8424 3.1 ------ UNKNOWN
240.0567 -28.6165 4.1 54.6 -19.9 6.7151 3.1 ------ UNKNOWN
Plot creation:
Mon Oct 24 05:20:47 EDT 2022