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
185.6864 29.9859 0.0181 35.0314 -141.9895 0.9653575 10.565 TRIG_01275005
Foreground time interval of the image:
-1.824 26.160 (delta_t = 27.984 [sec])
Background time interval of the image:
-118.387 -1.824 (delta_t = 116.563 [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 12.160000
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 12.160000
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 12.160000
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 -1.824 sec. to 26.160 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.31928 ( -0.267203 0.26188 )
Norm@50keV : 2.01003E-03 ( -0.000325349 0.00032534 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 56.11 using 59 bins.
Reduced chi-squared = 0.984386
# Null hypothesis probability of 5.09e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 27.98 sec: 0.240678 ( -0.040581 0.040772 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.53257e-07 ( -9.57078e-08 9.64205e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -1.824 sec. to 26.160 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.419933 ( -1.27725 0.983686 )
Epeak [keV] : 95.4890 ( -31.6993 -95.4821 )
Norm@50keV : 5.32138E-03 ( -0.00532217 0.0136259 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 53.72 using 59 bins.
Reduced chi-squared = 0.959286
# Null hypothesis probability of 5.62e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 27.98 sec: 0.232558 ( -0.041834 0.041882 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.31237e-07 ( -9.86354e-08 9.98626e-08 ) ergs/cm2
Band function
Time interval is from -1.824 sec. to 26.160 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] : 18.8003 (-3.31992 4.14107)
R^2/D10^2 : 1.35247E-02 (-0.00668372 0.0128104)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 58.54 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 2.639e-08 8.986e-09
25- 50 1.260e-07 4.191e-08
50-150 3.266e-07 1.012e-07
15-150 4.789e-07 1.238e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-65.0275 -200)
Norm : 1.01293 (-0.164813 0.164813)
------------------------------------------------------------
#Fit statistic : Chi-Squared 57.12 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.71e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.060e-08 4.078e-08
25- 50 1.358e-07 7.685e-08
50-150 2.979e-07 1.661e-07
15-150 5.043e-07 2.825e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.37573 (-2.38481 3.78809)
R1^2/D10^2 : 0.261390 (-0.212476 0.934405)
kT2 [keV] : 24.2729 (-5.54378 10.3822)
R2^2/D10^2 : 4.91564E-03 (-0.00352202 0.00721972)
------------------------------------------------------------
#Fit statistic : Chi-Squared 51.45 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.11e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.718e-08 3.356e-08
25- 50 1.285e-07 6.925e-08
50-150 3.559e-07 2.009e-07
15-150 5.416e-07 2.900e-07
Peak spectrum fit
Power-law model
Time interval is from 8.888 sec. to 9.888 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.24983 ( -0.522468 0.483173 )
Norm@50keV : 5.10991E-03 ( -0.00173475 0.00172901 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 64.12 using 59 bins.
Reduced chi-squared = 1.12491
# Null hypothesis probability of 2.41e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.604118 ( -0.212708 0.216064 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.11635e-08 ( -1.77232e-08 1.79034e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 8.888 sec. to 9.888 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -1.82019 ( -7.58462 2.78642 )
Epeak [keV] : 63.8289 ( -16.3918 77.5755 )
Norm@50keV : 0.161638 ( -0.200615 864.772 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 59.97 using 59 bins.
Reduced chi-squared = 1.07089
# Null hypothesis probability of 3.34e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.570559 ( -0.204505 0.215094 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.52262e-08 ( -1.70955e-08 1.86354e-08 ) ergs/cm2
Band function
Time interval is from 8.888 sec. to 9.888 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] : 16.7054 (-4.22647 6.42577)
R^2/D10^2 : 5.79071E-02 (-0.0579071 0.102078)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 60.10 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.64e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.307e-09 2.108e-09
25- 50 1.443e-08 8.660e-09
50-150 2.858e-08 1.983e-08
15-150 4.631e-08 2.974e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.363 (-112.321 -199.363)
Norm : 2.60872 (-0.883421 0.883449)
------------------------------------------------------------
#Fit statistic : Chi-Squared 64.36 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.35e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.496e-09 4.217e-09
25- 50 1.250e-08 8.115e-09
50-150 2.741e-08 1.734e-08
15-150 4.640e-08 2.906e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 199.924 (-199.924 -199.924)
R1^2/D10^2 : 1.22929E-05 (-1.22929e-05 -1.22929e-05)
kT2 [keV] : 16.0742 (-16.0742 6.96662)
R2^2/D10^2 : 6.39354E-02 (-0.0639354 0.0951793)
------------------------------------------------------------
#Fit statistic : Chi-Squared 60.07 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.97e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.349e-09 8.310e-06
25- 50 1.443e-08 7.710e-05
50-150 2.875e-08 1.788e-03
15-150 4.652e-08 1.664e-03
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: 1.31928 ( -0.267203 0.26188 )
Norm@50keV : 2.01003E-03 ( -0.000325349 0.00032534 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 56.11 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.09e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 27.98 sec: 0.240675 ( -0.0405792 0.0407703 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.53187e-07 ( -9.56874e-08 9.64823e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.420405 ( -1.27714 0.983801 )
Epeak [keV] : 95.5162 ( -31.5911 -95.4839 )
Norm@50keV : 5.31841E-03 ( -0.00532222 0.0136256 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 53.72 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.62e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 27.98 sec: 0.232549 ( -0.041828 0.041861 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.31455e-07 ( -9.86295e-08 1.00034e-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) = 1.25e-07
S(50-100 keV) = 1.99e-07
T90 vs. Hardness ratio plot
T90 = 23.3519998788834 sec.
Hardness ratio (energy fluence ratio) = 1.592
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.37192
Count Ratio (50-100 keV) / (15-25 keV) = 1.54536
Mask shadow pattern
IMX = -5.523357671686940E-01, IMY = 4.316954955359277E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 12.160000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 12.160000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 12.160000
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:
-118.387400 -1.824000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.4365 -40.5504 3.5 53.7 5.1 1.5862 3.3 4.2 Vela X-1
116.3987 33.7638 3.1 42.3 117.0 3.3018 3.7 ------ UNKNOWN
141.0115 50.4746 2.6 41.9 154.0 1.7115 4.4 ------ UNKNOWN
179.4252 -38.7922 2.5 54.1 -36.7 4.8443 4.7 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-1.824000 26.160000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.6364 -40.5941 9.1 53.7 4.9 0.3002 1.3 5.5 Vela X-1
134.7620 -41.0358 2.1 54.4 5.5 1.4292 5.3 ------ UNKNOWN
185.6864 29.9859 1.1 35.0 -142.0 0.9653 10.6 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
129.812590 962.223900
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
186.5769 31.8750 2.9 2.0 177.1 4.0289 4.0 ------ UNKNOWN
189.7973 -2.8319 2.5 33.1 -32.2 6.3226 4.7 ------ UNKNOWN
Plot creation:
Fri Jun 20 01:59:32 EDT 2025