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
94.5506 -44.9724 0.0329 11.7149 65.6685 0.8689872 5.842 TRIG_01222955
Foreground time interval of the image:
-74.036 46.368 (delta_t = 120.404 [sec])
Background time interval of the image:
-239.432 -74.036 (delta_t = 165.396 [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 4.096000
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 4.096000
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 4.096000
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 -74.036 sec. to 46.368 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.64309 ( -0.312282 0.329535 )
Norm@50keV : 5.60273E-04 ( -0.000106256 0.000101947 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 82.29 using 59 bins.
Reduced chi-squared = 1.44368
# Null hypothesis probability of 1.58e-02 with 57 degrees of freedom
Photon flux (15-150 keV) in 120.4 sec: 7.29948E-02 ( -0.0118604 0.0118661 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.27894e-07 ( -1.25359e-07 1.28828e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -74.036 sec. to 46.368 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.64708 ( -0.319284 0.326613 )
Epeak [keV] : 9999.36 ( -9999.35 -9999.36 )
Norm@50keV : 5.60435E-04 ( -0.000106027 0.000754743 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 82.29 using 59 bins.
Reduced chi-squared = 1.46946
# Null hypothesis probability of 1.26e-02 with 56 degrees of freedom
Photon flux (15-150 keV) in 120.4 sec: 7.31360E-02 ( -0.0120862 0.0118175 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.2762e-07 ( -1.24969e-07 1.28876e-07 ) ergs/cm2
Band function
Time interval is from -74.036 sec. to 46.368 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] : 13.2445 (-3.02385 4.01526)
R^2/D10^2 : 1.20181E-02 (-0.00717431 0.0181648)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 98.27 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.63e-04 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.381e-08 1.866e-08
25- 50 1.891e-07 5.621e-08
50-150 2.119e-07 8.648e-08
15-150 4.548e-07 1.134e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 181.995 (-102.294 -178.882)
Norm : 0.294794 (-0.0492605 0.0672064)
------------------------------------------------------------
#Fit statistic : Chi-Squared 83.51 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.26e-02 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.939e-08 4.970e-08
25- 50 1.701e-07 9.271e-08
50-150 3.615e-07 2.029e-07
15-150 6.210e-07 3.512e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 4.57821 (-1.71421 2.53109)
R1^2/D10^2 : 0.457904 (-0.376016 4.00487)
kT2 [keV] : 23.5541 (-7.36476 20.4354)
R2^2/D10^2 : 1.38462E-03 (-0.00118203 0.00493276)
------------------------------------------------------------
#Fit statistic : Chi-Squared 81.89 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.08e-02 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.095e-07 6.218e-08
25- 50 1.396e-07 7.471e-08
50-150 3.783e-07 2.289e-07
15-150 6.274e-07 3.392e-07
Peak spectrum fit
Power-law model
Time interval is from 0.352 sec. to 1.352 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.34787 ( -0.337288 0.338771 )
Norm@50keV : 5.83821E-03 ( -0.00114738 0.00113923 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 53.76 using 59 bins.
Reduced chi-squared = 0.943158
# Null hypothesis probability of 5.97e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.703038 ( -0.137045 0.137272 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.70545e-08 ( -1.25207e-08 1.27286e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.352 sec. to 1.352 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.07922 ( -1.52381 1.62878 )
Epeak [keV] : 178.730 ( -178.736 -178.736 )
Norm@50keV : 7.91940E-03 ( -0.00318135 0.0332519 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 53.62 using 59 bins.
Reduced chi-squared = 0.9575
# Null hypothesis probability of 5.66e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.696168 ( -0.141238 0.140436 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.6119e-08 ( -1.32691e-08 1.32427e-08 ) ergs/cm2
Band function
Time interval is from 0.352 sec. to 1.352 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] : 17.3230 (-3.87094 5.32097)
R^2/D10^2 : 5.07662E-02 (-0.0301149 0.0688559)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 59.33 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.91e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.086e-09 1.113e-09
25- 50 1.386e-08 5.137e-09
50-150 2.987e-08 1.199e-08
15-150 4.681e-08 1.794e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.362 (-86.0241 -199.363)
Norm : 2.89139 (-0.55928 0.560591)
------------------------------------------------------------
#Fit statistic : Chi-Squared 54.70 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.62e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.200e-09 4.279e-09
25- 50 1.385e-08 7.985e-09
50-150 3.037e-08 1.754e-08
15-150 5.142e-08 2.955e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 4.65487 (-3.13669 6.14429)
R1^2/D10^2 : 2.74317 (-2.57472 15.8932)
kT2 [keV] : 22.8081 (-6.40331 21.4538)
R2^2/D10^2 : 1.80371E-02 (-0.0161985 0.0116148)
------------------------------------------------------------
#Fit statistic : Chi-Squared 53.00 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.51e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.674e-09 3.829e-09
25- 50 1.193e-08 6.445e-09
50-150 3.591e-08 2.128e-08
15-150 5.451e-08 2.946e-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: 1.64309 ( -0.312282 0.329535 )
Norm@50keV : 5.60273E-04 ( -0.000106256 0.000101947 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 82.29 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.58e-02 with 57 degrees of freedom
Photon flux (15-150 keV) in 120.4 sec: 7.29921E-02 ( -0.0118598 0.0118654 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.27814e-07 ( -1.25297e-07 1.28812e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.18811 ( -1.19592 0.0717652 )
Epeak [keV] : 71.2484 ( )
Norm@50keV : 2.98076E-04 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared 81.94 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.35e-02 with 56 degrees of freedom
Photon flux (15-150 keV) in 120.4 sec: 7.30414E-02 ( -0.0119291 0.0118255 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.28151e-07 ( -1.25562e-07 1.25203e-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) = 1.66e-07
S(50-100 keV) = 2.12e-07
T90 vs. Hardness ratio plot
T90 = 114.256000041962 sec.
Hardness ratio (energy fluence ratio) = 1.27711
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 0.908631
Count Ratio (50-100 keV) / (15-25 keV) = 0.881827
Mask shadow pattern
IMX = 8.543604536943343E-02, IMY = -1.889426024036979E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 4.096000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 4.096000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 4.096000
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:
-239.432000 -74.036000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
117.2377 -8.7938 2.8 49.6 25.5 3.4472 4.1 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-74.036000 46.368000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
356.1776 -78.6088 2.3 44.5 166.4 1.2992 5.0 ------ UNKNOWN
94.5506 -44.9724 2.0 11.7 65.7 0.8691 5.8 ------ UNKNOWN
330.4099 -69.0378 1.7 54.2 175.1 3.7146 7.0 ------ UNKNOWN
83.5548 -24.5412 2.4 21.0 -15.5 0.7280 4.9 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
92.668600 962.697600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.4105 -40.5133 6.8 30.0 71.9 3.6318 1.7 5.9 Vela X-1
134.3064 -39.3663 2.7 29.7 69.1 8.4790 4.3 ------ UNKNOWN
90.0900 -12.1545 2.2 33.1 -32.2 6.3907 5.1 ------ UNKNOWN
Plot creation:
Sat Oct 19 18:29:21 EDT 2024