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
204.2840 14.4757 0.0136 35.7802 49.3752 1.5435991 14.182 TRIG_01054627
Foreground time interval of the image:
-5.976 11.352 (delta_t = 17.328 [sec])
Background time interval of the image:
-239.560 -5.976 (delta_t = 233.584 [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 1.024000
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 1.024000
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 1.024000
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 -5.976 sec. to 11.352 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.41325 ( -0.186704 0.185768 )
Norm@50keV : 6.23186E-03 ( -0.000645462 0.00064323 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 66.11 using 59 bins.
Reduced chi-squared = 1.15982
# Null hypothesis probability of 1.91e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 17.33 sec: 0.761253 ( -0.081518 0.081815 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.0409e-06 ( -1.17799e-07 1.18435e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -5.976 sec. to 11.352 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.40773 ( -0.185664 0.189003 )
Epeak [keV] : 9999.09 ( -9999.36 -9999.36 )
Norm@50keV : 6.25468E-03 ( -0.00625435 0.00330818 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 66.13 using 59 bins.
Reduced chi-squared = 1.18089
# Null hypothesis probability of 1.67e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 17.33 sec: 0.766006 ( -0.116122 0.106623 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.04623e-06 ( -1.62688e-07 1.52655e-07 ) ergs/cm2
Band function
Time interval is from -5.976 sec. to 11.352 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] : 17.4215 (-2.63433 3.23265)
R^2/D10^2 : 5.07031E-02 (-0.0222303 0.038717)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 102.81 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.92e-04 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.394e-08 1.122e-08
25- 50 2.433e-07 4.514e-08
50-150 5.312e-07 1.109e-07
15-150 8.284e-07 1.084e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-44.6833 -200)
Norm : 3.14551 (-0.325248 0.325248)
------------------------------------------------------------
#Fit statistic : Chi-Squared 69.86 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.18e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.358e-07 2.762e-08
25- 50 2.611e-07 1.418e-07
50-150 5.727e-07 3.148e-07
15-150 9.696e-07 4.023e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.27992 (-1.57066 2.15847)
R1^2/D10^2 : 1.26934 (-0.828316 2.66044)
kT2 [keV] : 32.0244 (-7.89153 18.2099)
R2^2/D10^2 : 5.76762E-03 (-0.0042081 0.00887956)
------------------------------------------------------------
#Fit statistic : Chi-Squared 65.14 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.64e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.381e-07 6.915e-08
25- 50 2.324e-07 9.071e-08
50-150 7.009e-07 3.626e-07
15-150 1.071e-06 4.005e-07
Peak spectrum fit
Power-law model
Time interval is from -0.292 sec. to 0.708 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.50681 ( -0.25477 0.258534 )
Norm@50keV : 2.01453E-02 ( -0.00317887 0.00315567 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 47.96 using 59 bins.
Reduced chi-squared = 0.841404
# Null hypothesis probability of 7.98e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 2.51962 ( -0.39594 0.3965 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.90924e-07 ( -3.24128e-08 3.26596e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.292 sec. to 0.708 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.19560 ( -1.11673 0.552802 )
Epeak [keV] : 131.899 ( -131.899 -131.899 )
Norm@50keV : 2.89601E-02 ( -0.0289601 0.0730205 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 47.65 using 59 bins.
Reduced chi-squared = 0.850893
# Null hypothesis probability of 7.79e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 2.49858 ( -0.40289 0.4018 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.88005e-07 ( -3.39733e-08 3.38402e-08 ) ergs/cm2
Band function
Time interval is from -0.292 sec. to 0.708 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] : 15.5850 (-2.8709 3.59056)
R^2/D10^2 : 0.254324 (-0.132052 0.267093)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 58.53 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.19e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.284e-08 3.867e-09
25- 50 5.282e-08 1.336e-08
50-150 8.876e-08 2.840e-08
15-150 1.544e-07 3.650e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.363 (-88.9586 -199.363)
Norm : 10.3793 (-1.59053 1.59095)
------------------------------------------------------------
#Fit statistic : Chi-Squared 47.79 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.03e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.585e-08 1.499e-08
25- 50 4.972e-08 2.801e-08
50-150 1.090e-07 5.980e-08
15-150 1.846e-07 1.044e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.97588 (-2.48198 4.05416)
R1^2/D10^2 : 4.38663 (-3.57379 34.4928)
kT2 [keV] : 23.7535 (-6.49847 20.8446)
R2^2/D10^2 : 4.79171E-02 (-0.0425631 0.11076)
------------------------------------------------------------
#Fit statistic : Chi-Squared 47.39 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.57e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.552e-08 1.415e-08
25- 50 4.709e-08 2.557e-08
50-150 1.139e-07 6.700e-08
15-150 1.865e-07 8.782e-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: 1.41325 ( -0.186704 0.185768 )
Norm@50keV : 6.23186E-03 ( -0.000645462 0.00064323 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 66.11 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.91e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 17.33 sec: 0.761239 ( -0.0815137 0.0818102 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.04076e-06 ( -1.1778e-07 1.1844e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.41208 ( -0.406301 1.2946 )
Epeak [keV] : 9999.32 ( -9999.36 -9999.36 )
Norm@50keV : 6.25262E-03 ( -0.00625275 0.0033095 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 66.13 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.67e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 17.33 sec: 0.763069 ( -0.08399 0.079929 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.03452e-06 ( -1.12265e-07 1.25724e-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) = 2.46e-07
S(50-100 keV) = 3.71e-07
T90 vs. Hardness ratio plot
T90 = 13.6160000562668 sec.
Hardness ratio (energy fluence ratio) = 1.50813
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.1352
Count Ratio (50-100 keV) / (15-25 keV) = 1.10171
Mask shadow pattern
IMX = 4.692482888128566E-01, IMY = -5.470022311397643E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.024000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.024000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.024000
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:
-239.560000 -5.976000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.4859 -40.5616 4.8 52.3 -162.7 1.5077 2.4 2.0 Vela X-1
165.2079 37.3644 4.7 37.0 -23.9 0.7658 2.5 ------ UNKNOWN
162.5793 32.1826 2.8 32.4 -29.6 1.1541 4.2 ------ UNKNOWN
140.6376 43.5508 2.9 50.6 -44.6 4.0582 4.0 ------ UNKNOWN
123.1315 -25.1463 2.5 52.9 -139.3 5.4244 4.6 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-5.976000 11.352000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.5831 -40.5569 34.9 52.3 -162.7 -0.0420 -0.3 2.5 Vela X-1
204.2840 14.4757 0.8 35.8 49.4 1.5432 14.2 ------ UNKNOWN
166.9932 -46.2050 2.3 47.1 167.2 0.6484 5.0 ------ UNKNOWN
182.6464 35.0359 2.4 36.0 0.1 0.3179 4.8 ------ UNKNOWN
161.3248 -29.0210 2.3 31.1 179.8 0.2847 4.9 ------ UNKNOWN
133.2568 21.2531 2.2 42.0 -74.6 0.9500 5.4 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
73.740590 890.840600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.4399 35.3219 51.1 49.4 21.6 -0.4750 -0.2 1.5 Her X-1
254.8792 30.0931 2.9 48.9 28.5 9.3534 4.0 ------ UNKNOWN
179.3968 -26.1972 3.2 47.3 176.8 5.6758 3.6 ------ UNKNOWN
197.2968 31.8101 2.9 18.4 -53.1 2.6305 4.0 ------ UNKNOWN
156.2117 5.9855 2.3 48.0 -129.1 13.9383 5.0 ------ UNKNOWN
157.6578 12.1746 2.7 45.3 -121.1 10.9511 4.3 ------ UNKNOWN
Plot creation:
Sat Jul 30 06:59:26 EDT 2022