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
351.4653 -55.1233 0.0022 9.6945 -97.1075 54.6124363 86.816 TRIG_01213095
Foreground time interval of the image:
-0.836 79.064 (delta_t = 79.900 [sec])
Background time interval of the image:
-131.747 -0.836 (delta_t = 130.911 [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 -0.836 sec. to 79.064 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.22695 ( -0.0269177 0.0268896 )
Norm@50keV : 3.54811E-02 ( -0.000481618 0.000481515 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 49.73 using 59 bins.
Reduced chi-squared = 0.872456
# Null hypothesis probability of 7.42e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 79.9 sec: 5.95913 ( -0.12458 0.12556 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.67656e-05 ( -3.92788e-07 3.92942e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.836 sec. to 79.064 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.99122 ( -0.0843122 -1.99122 )
Epeak [keV] : 2.14407 ( -0.227616 0.285339 )
Norm@50keV : 4.47885E-02 ( -0.00127477 0.00138564 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 40.90 using 59 bins.
Reduced chi-squared = 0.730357
# Null hypothesis probability of 9.35e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 79.9 sec: 5.74747 ( -0.09918 0.09412 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.52567e-05 ( 5.97829e-07 1.31667e-06 ) ergs/cm2
Band function
Time interval is from -0.836 sec. to 79.064 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] : 14.0872 ( )
R^2/D10^2 : 0.585009 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 1424.10 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.90e-260 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.958e-06 6.432e-08
25- 50 7.328e-06 1.562e-07
50-150 9.606e-06 1.958e-07
15-150 1.889e-05 2.437e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 69.7817 ( )
Norm : 25.9205 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared 129.27 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.55e-07 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.312e-06 1.406e-07
25- 50 8.444e-06 1.558e-07
50-150 1.082e-05 2.117e-07
15-150 2.458e-05 3.316e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.23597 (-0.322074 0.33287)
R1^2/D10^2 : 6.58303 (-1.06962 1.32995)
kT2 [keV] : 23.9169 (-1.15536 1.32535)
R2^2/D10^2 : 4.98640E-02 (-0.0102067 0.0119108)
------------------------------------------------------------
#Fit statistic : Chi-Squared 96.45 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.67e-04 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.978e-06 2.621e-07
25- 50 8.918e-06 1.958e-07
50-150 1.082e-05 2.237e-07
15-150 2.471e-05 4.834e-07
Peak spectrum fit
Power-law model
Time interval is from 39.068 sec. to 40.068 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.57013 ( -0.0333602 0.0333844 )
Norm@50keV : 0.378868 ( -0.00692479 0.00692421 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 66.67 using 59 bins.
Reduced chi-squared = 1.16965
# Null hypothesis probability of 1.79e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 48.2481 ( -1.0301 1.0337 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.5573e-06 ( -6.58968e-08 6.58807e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 39.068 sec. to 40.068 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.16083 ( -0.145793 0.141556 )
Epeak [keV] : 118.838 ( -16.6929 31.8713 )
Norm@50keV : 0.571228 ( -0.0739117 0.0875055 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 41.14 using 59 bins.
Reduced chi-squared = 0.734643
# Null hypothesis probability of 9.32e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 40.1725 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 3.48803e-06 ( -7.0361e-08 7.0249e-08 ) ergs/cm2
Band function
Time interval is from 39.068 sec. to 40.068 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] : 17.2225 ( )
R^2/D10^2 : 3.23707 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 584.10 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.77e-88 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.948e-07 7.400e-09
25- 50 8.710e-07 2.310e-08
50-150 1.852e-06 5.600e-08
15-150 2.918e-06 5.900e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-8.62598 -200)
Norm : 195.747 (-3.56458 3.56458)
------------------------------------------------------------
#Fit statistic : Chi-Squared 44.97 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.76e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.876e-07 1.005e-08
25- 50 9.379e-07 2.005e-08
50-150 2.057e-06 4.450e-08
15-150 3.482e-06 7.600e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 8.18824 (-0.643169 0.68024)
R1^2/D10^2 : 27.2955 (-6.1186 8.53129)
kT2 [keV] : 28.0065 (-1.92546 2.42067)
R2^2/D10^2 : 0.443568 (-0.120653 0.142425)
------------------------------------------------------------
#Fit statistic : Chi-Squared 57.07 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.98e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.932e-07 2.530e-08
25- 50 9.528e-07 3.515e-08
50-150 2.101e-06 1.015e-07
15-150 3.447e-06 1.100e-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: 2.22695 ( -0.0269177 0.0268896 )
Norm@50keV : 3.54811E-02 ( -0.000481618 0.000481515 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 49.73 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.42e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 79.9 sec: 5.95852 ( -0.124558 0.125523 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.67599e-05 ( -3.92274e-07 3.92931e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.99131 ( -0.0843727 -1.99131 )
Epeak [keV] : 2.12394 ( -0.225547 0.282763 )
Norm@50keV : 4.47850E-02 ( -0.00127437 0.00138557 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 40.90 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.35e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 79.9 sec: 5.78576 ( -0.15326 0.15512 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.63187e-05 ( -4.60304e-07 4.6318e-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) = 8.55e-06
S(50-100 keV) = 7.29e-06
T90 vs. Hardness ratio plot
T90 = 47.3040000200272 sec.
Hardness ratio (energy fluence ratio) = 0.852632
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 0.960627
Count Ratio (50-100 keV) / (15-25 keV) = 0.437913
Mask shadow pattern
IMX = -2.113739400886126E-02, IMY = 1.695209670042056E-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:
-131.747400 -0.836000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
264.6540 -44.4770 8.0 58.1 -155.0 1.8865 1.4 4.1 4U 1735-44
43.5550 -53.7432 2.8 20.5 58.5 1.1511 4.2 ------ UNKNOWN
35.5785 -16.9667 2.3 47.6 7.9 2.2247 5.0 ------ UNKNOWN
11.6989 -72.0923 2.6 12.3 143.3 0.9937 4.5 ------ UNKNOWN
272.8816 -45.5253 2.8 53.7 -150.1 3.3416 4.1 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-0.836000 79.064000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
264.8493 -44.3875 5.5 58.1 -154.8 -7.4494 -2.1 5.9 4U 1735-44
48.2331 -47.3669 3.1 26.8 50.4 3.1996 3.8 ------ UNKNOWN
41.1628 -15.9783 2.4 50.4 14.1 11.1986 4.9 ------ UNKNOWN
231.9383 -68.1005 2.6 47.9 170.6 6.3859 4.5 ------ UNKNOWN
35.8964 -21.1992 3.1 43.7 10.2 4.8451 3.8 ------ UNKNOWN
351.4653 -55.1233 0.1 9.7 -97.1 54.6128 86.8 ------ UNKNOWN
258.1025 -56.6219 2.7 50.7 -167.9 5.9669 4.3 ------ UNKNOWN
6.5327 -33.3440 2.3 26.6 -31.4 3.4573 5.1 ------ UNKNOWN
350.6475 -25.1884 2.7 36.6 -55.7 4.4428 4.3 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
Plot creation:
Sat Mar 9 15:14:43 EST 2024