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
199.3003 60.6126 0.0179 31.9520 116.7761 2.0342732 10.723 TRIG_01210276
Foreground time interval of the image:
-1.872 59.053 (delta_t = 60.925 [sec])
Background time interval of the image:
-239.648 -1.872 (delta_t = 237.776 [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 -1.872 sec. to 136.064 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.64213 ( -0.219667 0.225703 )
Norm@50keV : 1.30195E-03 ( -0.00017574 0.000172912 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 55.38 using 59 bins.
Reduced chi-squared = 0.971579
# Null hypothesis probability of 5.36e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 137.9 sec: 0.169570 ( -0.021272 0.021295 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.67133e-06 ( -2.38637e-07 2.42235e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -1.872 sec. to 136.064 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.31019 ( -1.32404 0.543643 )
Epeak [keV] : 96.8698 ( -53.7038 -97.1122 )
Norm@50keV : 1.96178E-03 ( -0.00195756 0.00801941 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 55.10 using 59 bins.
Reduced chi-squared = 0.983929
# Null hypothesis probability of 5.09e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 137.9 sec: 0.167228 ( -0.022905 0.022501 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.62045e-06 ( -2.91146e-07 2.54176e-07 ) ergs/cm2
Band function
Time interval is from -1.872 sec. to 136.064 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] : 12.7640 (-1.6383 1.95339)
R^2/D10^2 : 3.37084E-02 (-0.013742 0.0219853)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 63.78 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.50e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.606e-07 3.705e-08
25- 50 5.423e-07 8.832e-08
50-150 5.525e-07 1.666e-07
15-150 1.255e-06 2.156e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 157.998 (-70.7257 -156.223)
Norm : 0.694507 (-0.0926531 0.126539)
------------------------------------------------------------
#Fit statistic : Chi-Squared 55.12 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.46e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.448e-07 1.315e-07
25- 50 4.572e-07 2.435e-07
50-150 9.216e-07 5.324e-07
15-150 1.624e-06 9.081e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 2.11425 (-0.985707 2.2588)
R1^2/D10^2 : 52.1528 (-44.2231 142146)
kT2 [keV] : 14.2066 (-2.10521 2.91757)
R2^2/D10^2 : 2.16081E-02 (-0.010713 0.0146585)
------------------------------------------------------------
#Fit statistic : Chi-Squared 54.59 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.90e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.274e-07 7.547e-08
25- 50 4.879e-07 1.174e-07
50-150 6.314e-07 1.896e-07
15-150 1.347e-06 2.899e-07
Peak spectrum fit
Power-law model
Time interval is from 2.164 sec. to 3.164 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.36573 ( -0.579828 0.567077 )
Norm@50keV : 7.72720E-03 ( -0.00246918 0.00244152 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 61.74 using 59 bins.
Reduced chi-squared = 1.08316
# Null hypothesis probability of 3.11e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.933985 ( -0.298638 0.299815 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.5216e-08 ( -2.62201e-08 2.69038e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 2.164 sec. to 3.164 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.36267 ( -2.4719 -1.31628 )
Epeak [keV] : 9999.19 ( -9999.21 -9999.21 )
Norm@50keV : 7.75668E-03 ( -0.00775668 0.174417 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 61.74 using 59 bins.
Reduced chi-squared = 1.1025
# Null hypothesis probability of 2.78e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.935580 ( -0.302468 0.29965 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.54362e-08 ( -2.94444e-08 2.26369e-08 ) ergs/cm2
Band function
Time interval is from 2.164 sec. to 3.164 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] : 13.6019 (-4.99959 11.556)
R^2/D10^2 : 0.148748 (-0.146302 0.5964)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 64.99 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.18e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.827e-09 3.775e-09
25- 50 2.105e-08 1.332e-08
50-150 2.525e-08 1.810e-08
15-150 5.213e-08 3.329e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.363 (-199.363 -199.363)
Norm : 3.85394 (-1.21568 1.21567)
------------------------------------------------------------
#Fit statistic : Chi-Squared 62.13 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.99e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.597e-09 5.945e-09
25- 50 1.846e-08 1.177e-08
50-150 4.049e-08 2.534e-08
15-150 6.854e-08 4.297e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 9.48351 (-2.30813 5.38112)
R1^2/D10^2 : 0.449305 (-0.386711 2.92345)
kT2 [keV] : 124.312 (-47.1438 -125.179)
R2^2/D10^2 : 2.95260E-04 (-0.000241758 0.0416298)
------------------------------------------------------------
#Fit statistic : Chi-Squared 60.36 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.88e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.292e-09 5.150e-09
25- 50 2.044e-08 1.273e-08
50-150 4.849e-08 1.676e-08
15-150 7.722e-08 3.252e-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: 1.46528 ( -0.208549 0.20898 )
Norm@50keV : 2.48509E-03 ( -0.00030606 0.000304482 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 57.10 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.72e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 60.92 sec: 0.307430 ( -0.0377841 0.0378478 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.44471e-06 ( -1.94413e-07 1.96595e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.12486 ( -1.12331 0.52211 )
Epeak [keV] : 124.225 ( -124.591 -124.591 )
Norm@50keV : 3.74543E-03 ( -0.00179385 0.0105925 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 56.71 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.48e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 60.92 sec: 0.303346 ( -0.039701 0.039375 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.40277e-06 ( -2.32495e-07 2.23857e-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) = 4.41e-07
S(50-100 keV) = 5.65e-07
T90 vs. Hardness ratio plot
T90 = 89.8400000333786 sec.
Hardness ratio (energy fluence ratio) = 1.28118
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.51487
Count Ratio (50-100 keV) / (15-25 keV) = 0.764906
Mask shadow pattern
IMX = -2.809824120636634E-01, IMY = -5.568273803114844E-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:
-239.648000 -1.872000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
244.9524 -15.6178 2.9 58.0 -25.3 7.1532 4.0 2.1 Sco X-1
254.6495 35.3127 5.2 11.4 -78.7 0.8290 2.2 9.6 Her X-1
299.4965 35.0579 5.2 43.7 -123.1 2.8685 2.2 9.8 Cyg X-1
308.2468 41.1062 5.7 47.3 -134.9 -2.2026 -2.0 11.1 Cyg X-3
199.6759 17.7853 3.1 44.3 46.7 4.9685 3.7 ------ UNKNOWN
265.9263 70.3831 2.4 30.3 171.7 2.2272 4.7 ------ UNKNOWN
266.8387 45.6627 2.4 17.3 -132.3 1.8131 4.7 ------ UNKNOWN
298.5993 32.1435 2.2 44.5 -118.9 8.6170 5.3 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-1.872000 59.052590
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
245.0142 -15.7239 4.4 58.1 -25.3 1.6103 2.6 5.4 Sco X-1
254.2070 35.2906 0.0 11.1 -77.4 -0.1166 -1.2 12.7 Her X-1
299.4033 35.2594 0.0 43.6 -123.3 0.5805 1.8 9.8 Cyg X-1
308.1091 40.9519 39.5 47.3 -134.7 0.0890 0.3 0.1 Cyg X-3
202.7752 9.2277 2.8 48.4 35.5 2.1184 4.1 ------ UNKNOWN
199.3005 60.6126 1.1 32.0 116.8 2.0397 10.7 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
129.652600 926.352590
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
213.7884 16.9914 2.5 44.9 -15.7 8.2951 4.6 ------ UNKNOWN
Plot creation:
Sat Mar 9 15:16:04 EST 2024