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
129.1904 73.1549 0.0071 27.1114 -111.1573 3.2113232 27.090 TRIG_01221874
Foreground time interval of the image:
-0.696 37.512 (delta_t = 38.208 [sec])
Background time interval of the image:
-121.699 -0.696 (delta_t = 121.003 [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 -0.696 sec. to 37.512 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.28650 ( -0.133511 0.138616 )
Norm@50keV : 4.12121E-03 ( -0.000354428 0.000348378 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 44.47 using 59 bins.
Reduced chi-squared = 0.780175
# Null hypothesis probability of 8.87e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 38.21 sec: 0.714927 ( -0.044672 0.044794 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.50147e-06 ( -1.04918e-07 1.06349e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.696 sec. to 37.512 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.35632 ( -0.414652 0.378688 )
Epeak [keV] : 207.603 ( )
Norm@50keV : 3.75480E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared 44.30 using 59 bins.
Reduced chi-squared = 0.791071
# Null hypothesis probability of 8.71e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 38.21 sec: 0.715589 ( -0.089255 0.046996 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.45388e-06 ( -9.92566e-08 1.30825e-07 ) ergs/cm2
Band function
Time interval is from -0.696 sec. to 37.512 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] : 8.20554 ( )
R^2/D10^2 : 0.649795 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 126.94 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.06e-07 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.079e-07 3.506e-08
25- 50 5.628e-07 4.318e-08
50-150 1.605e-07 3.116e-08
15-150 1.031e-06 7.527e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 46.5485 (-8.03398 10.9046)
Norm : 4.05892 (-0.503972 0.62258)
------------------------------------------------------------
#Fit statistic : Chi-Squared 57.17 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.69e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.726e-07 3.082e-08
25- 50 5.213e-07 3.458e-08
50-150 4.723e-07 8.809e-08
15-150 1.366e-06 1.185e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.05813 (-0.627977 0.673631)
R1^2/D10^2 : 3.99480 (-1.65809 3.21228)
kT2 [keV] : 20.7810 (-3.55102 4.83604)
R2^2/D10^2 : 1.21413E-02 (-0.00655412 0.0129853)
------------------------------------------------------------
#Fit statistic : Chi-Squared 40.07 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.35e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.267e-07 7.277e-08
25- 50 4.553e-07 7.533e-08
50-150 6.355e-07 1.915e-07
15-150 1.518e-06 3.099e-07
Peak spectrum fit
Power-law model
Time interval is from 5.100 sec. to 6.100 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.35019 ( -0.16069 0.168649 )
Norm@50keV : 2.48534E-02 ( -0.00282076 0.00276736 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 49.64 using 59 bins.
Reduced chi-squared = 0.870877
# Null hypothesis probability of 7.45e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 4.46851 ( -0.36571 0.36602 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.39889e-07 ( -2.19123e-08 2.22007e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 5.100 sec. to 6.100 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.99197 ( -0.485845 -1.99197 )
Epeak [keV] : 0.918644 ( -0.334479 0.849885 )
Norm@50keV : 4.01782E-02 ( -0.00657057 0.00785137 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 50.03 using 59 bins.
Reduced chi-squared = 0.893393
# Null hypothesis probability of 6.99e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 4.39842 ( -0.35017 0.36104 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.32129e-07 ( -2.1969e-08 2.36059e-08 ) ergs/cm2
Band function
Time interval is from 5.100 sec. to 6.100 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] : 7.87259 (-0.752272 0.834425)
R^2/D10^2 : 5.04443 (-1.7292 2.6425)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 87.51 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.79e-03 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.585e-08 7.380e-09
25- 50 9.505e-08 9.835e-09
50-150 2.367e-08 6.205e-09
15-150 1.746e-07 1.880e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 40.3452 (-7.73447 10.361)
Norm : 28.3271 (-4.58286 5.63356)
------------------------------------------------------------
#Fit statistic : Chi-Squared 54.08 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.85e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.524e-08 7.570e-09
25- 50 8.614e-08 7.725e-09
50-150 6.727e-08 1.721e-08
15-150 2.186e-07 2.170e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.54483 (-0.972514 0.959679)
R1^2/D10^2 : 17.9464 (-8.39352 20.7879)
kT2 [keV] : 21.6655 (-6.3442 12.0883)
R2^2/D10^2 : 5.35165E-02 (-0.0425275 0.168452)
------------------------------------------------------------
#Fit statistic : Chi-Squared 48.77 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.10e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.874e-08 3.627e-08
25- 50 7.299e-08 3.731e-08
50-150 6.880e-08 3.957e-08
15-150 2.105e-07 1.021e-07
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: 2.28650 ( -0.133511 0.138616 )
Norm@50keV : 4.12121E-03 ( -0.000354428 0.000348378 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 44.47 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.87e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 38.21 sec: 0.714848 ( -0.0446635 0.0447859 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.50114e-06 ( -1.04956e-07 1.06333e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.99345 ( -0.22168 -1.99345 )
Epeak [keV] : 1.03471 ( -0.382261 1.09881 )
Norm@50keV : 5.89101E-03 ( -0.000764937 0.000895015 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 46.48 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.14e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 38.21 sec: 0.714510 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 1.49751e-06 ( -1.0865e-07 1.08394e-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) = 4.85e-07
S(50-100 keV) = 3.97e-07
T90 vs. Hardness ratio plot
T90 = 30.8000000715256 sec.
Hardness ratio (energy fluence ratio) = 0.818557
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 0.768917
Count Ratio (50-100 keV) / (15-25 keV) = 0.374855
Mask shadow pattern
IMX = -1.847879492131420E-01, IMY = 4.774667470488252E-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:
-121.699400 -0.696000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.5213 35.3615 12.3 50.3 4.4 0.4645 0.9 3.3 Her X-1
143.2516 33.9365 2.4 36.2 169.3 1.3085 4.8 ------ UNKNOWN
270.9871 37.8652 3.1 57.2 -9.9 4.2279 3.7 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-0.696000 37.512000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.4304 35.3786 7.2 50.2 4.5 -0.4676 -1.6 2.5 Her X-1
127.2250 19.4410 2.5 56.2 173.7 2.4191 4.5 ------ UNKNOWN
124.9071 26.9535 2.4 51.4 -178.8 1.1301 4.9 ------ UNKNOWN
252.7152 43.8262 2.4 43.3 -2.4 0.8201 4.8 ------ UNKNOWN
153.6306 68.1824 2.3 18.1 -117.8 0.4931 5.0 ------ UNKNOWN
129.1905 73.1549 0.4 27.1 -111.2 3.2112 27.1 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
Plot creation:
Sat Oct 19 18:30:36 EDT 2024