Estimated redshift from machine learning (Ukwatta et al. 2016) - may take a few minutes to calcaulte
Image
Pre-slew 15-350 keV image (Event data; bkg subtracted)
# RAcent DECcent POSerr Theta Phi Peak Cts SNR Name
201.3118 +25.6221 0.0150 25.3 -151.9 1.8331 12.9 TRIG_01280056
------------------------------------------
Foreground time interval of the image:
-63.136 32.545 (delta_t = 95.681 [sec])
Background time interval of the image:
-239.056 -63.136 (delta_t = 175.920 [sec])
Lightcurves
Notes:
- 1) All plots contain as much data as has been downloaded to date.
- 2) The mask-weighted light curves are using the flight position.
- 3) Multiple plots of different time binning/intervals are shown to cover all scenarios of short/long GRBs, rate/image triggers, and real/false positives.
- 4) 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.
- 5) 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.
- 6) 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)
Spectra
Notes:
- 1) The fitting includes the systematic errors.
- 2) For long bursts, a spectral fit of 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.
- 4) For short bursts (T90<1sec), the specrtum is also fit with Blackbody, OTTB, and Double Blackbody.
Time averaged spectrum fit using the pre-slew DRM
Power-law model
Time interval is from -63.136 sec. to 218.208 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.63479 ( -0.189272 0.193375 )
Norm@50keV : 6.49435E-04 ( -7.18875e-05 7.07341e-05 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 59.65 using 59 PHA bins.
# Reduced chi-squared = 1.047 for 57 degrees of freedom
# Null hypothesis probability = 3.793752e-01
Photon flux (15-150 keV) in 281.3 sec: 8.43799E-02 ( -0.0087019 0.00871735 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.70172e-06 ( -2.01064e-07 2.03463e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -63.136 sec. to 218.208 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.63512 ( -0.29493 0.192641 )
Epeak [keV] : 9999.29 ( -9999.34 -9999.35 )
Norm@50keV : 6.50494E-04 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 59.66 using 59 PHA bins.
# Reduced chi-squared = 1.065 for 56 degrees of freedom
# Null hypothesis probability = 3.440001e-01
Photon flux (15-150 keV) in 281.3 sec: 8.44964E-02 ( -0.0088557 0.0085985 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.69008e-06 ( -1.90302e-07 2.13372e-07 ) ergs/cm2
Band function
Time interval is from -63.136 sec. to 218.208 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.29862 ( 1.29829 1.29829 )
beta : -1.63482 ( 1.63482 0.189324 )
Epeak [keV] : 27.9869 ( -28.2016 -28.2016 )
Norm@50keV : 1.41461E-03 ( -0.00082996 0.096468 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 59.65 using 59 PHA bins.
# Reduced chi-squared = 1.085 for 55 degrees of freedom
# Null hypothesis probability = 3.102834e-01
Photon flux (15-150 keV) in 281.3 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] : 13.5646 (-2.14532 2.63696)
R^2/D10^2 : 1.27165E-02 (-0.005854 0.0108694)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 99.76 using 59 PHA bins.
# Reduced chi-squared = 1.750 for 57 degrees of freedom
# Null hypothesis probability = 3.978687e-04
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.394e-07 3.263e-08
25- 50 5.020e-07 7.778e-08
50-150 5.982e-07 1.439e-07
15-150 1.240e-06 1.747e-07
Thermal bremsstrahlung (OTTB)
XSPEC12>exit
XSPEC: quit
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 175.057 (-71.9734 -175.845)
Norm : 0.342179 (-0.0369853 0.0444307)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.405e-07 1.342e-07
25- 50 4.583e-07 2.395e-07
50-150 9.790e-07 5.332e-07
15-150 1.678e-06 8.907e-07
Double BB
XSPEC12>exit
XSPEC: quit
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.77470 (-1.32484 1.58626)
R1^2/D10^2 : 0.212672 (-0.127092 0.402014)
kT2 [keV] : 27.5641 (-6.54431 12.9268)
R2^2/D10^2 : 8.92056E-04 (-0.000623584 0.000804567)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.818e-07 1.399e-07
25- 50 4.160e-07 1.321e-07
50-150 1.048e-06 5.448e-07
15-150 1.746e-06 6.182e-07
Peak spectrum fit
Power-law model
Time interval is from 1.556 sec. to 2.556 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.924614 ( -0.517607 0.447679 )
Norm@50keV : 5.16509E-03 ( -0.00135235 0.00127945 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 58.43 using 59 PHA bins.
# Reduced chi-squared = 1.025 for 57 degrees of freedom
# Null hypothesis probability = 4.227531e-01
Photon flux (15-150 keV) in 1 sec: 0.593029 ( -0.150436 0.151334 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.7422e-08 ( -1.43211e-08 1.43917e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 1.556 sec. to 2.556 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.929792 ( -0.729632 0.440582 )
Epeak [keV] : 9999.36 ( -9999.36 -9999.36 )
Norm@50keV : 5.20860E-03 ( -0.00122248 0.00832744 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 58.44 using 59 PHA bins.
# Reduced chi-squared = 1.044 for 56 degrees of freedom
# Null hypothesis probability = 3.858127e-01
Photon flux (15-150 keV) in 1 sec: 0.596914 ( -0.154797 0.147571 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.73505e-08 ( -1.42475e-08 1.41359e-08 ) ergs/cm2
Band function
Time interval is from 1.556 sec. to 2.556 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 5.00000 ( -5 -5 )
beta : -0.935767 ( -0.463197 0.522502 )
Epeak [keV] : 20.9344 ( -20.9398 -20.9398 )
Norm@50keV : 917.242 ( -298.063 0 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 58.36 using 59 PHA bins.
# Reduced chi-squared = 1.061 for 55 degrees of freedom
# Null hypothesis probability = 3.529284e-01
Photon flux (15-150 keV) in 1 sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 0 ( 0 0 ) ergs/cm2
Single BB
XSPEC: quit
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 28.4280 (-9.88795 23.0157)
R^2/D10^2 : 9.50728E-03 (-0.00942765 0.0257864)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.242e-09 7.765e-10
25- 50 7.487e-09 4.486e-09
50-150 4.356e-08 2.639e-08
15-150 5.229e-08 2.917e-08
Thermal bremsstrahlung (OTTB)
XSPEC12>exit
XSPEC: quit
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-72.4373 -200)
Norm : 2.47194 (-0.619327 0.619327)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.155e-09 3.668e-09
25- 50 1.184e-08 7.045e-09
50-150 2.597e-08 1.545e-08
15-150 4.396e-08 2.660e-08
Double BB
XSPEC12>exit
XSPEC: quit
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 8.12027 (-3.96784 7.09246)
R1^2/D10^2 : 0.349553 (-0.292367 1.16022)
kT2 [keV] : 64.4590 (-43.5746 -68.3711)
R2^2/D10^2 : 1.01611E-03 (-0.000718164 0.0101583)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.589e-09 2.995e-09
25- 50 1.042e-08 5.695e-09
50-150 4.542e-08 2.460e-08
15-150 6.043e-08 3.114e-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: 1.54686 ( -0.163316 0.165275 )
Norm@50keV : 1.30648E-03 ( -0.000125976 0.000125033 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 51.00 using 59 PHA bins.
# Reduced chi-squared = 0.8947 for 57 degrees of freedom
# Null hypothesis probability = 6.986127e-01
Photon flux (15-150 keV) in 95.68 sec: 0.165243 ( -0.0155293 0.0155548 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.17734e-06 ( -1.23253e-07 1.24402e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.35670 ( -0.643811 0.278659 )
Epeak [keV] : 168.677 ( -168.677 -168.677 )
Norm@50keV : 1.63311E-03 ( -0.000582846 0.0017563 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 50.69 using 59 PHA bins.
# Reduced chi-squared = 0.9051 for 56 degrees of freedom
# Null hypothesis probability = 6.755934e-01
Photon flux (15-150 keV) in 95.68 sec: 0.163854 ( -0.015929 0.008052 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.16132e-06 ( -1.33541e-07 1.33655e-07 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.86709 ( 1.86709 6.86707 )
beta : -1.54701 ( -0.165113 0.16347 )
Epeak [keV] : 9992.64 ( -9992.56 -9992.56 )
Norm@50keV : 1.30653E-03 ( -0.000120179 0.102322 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 51.00 using 59 PHA bins.
# Reduced chi-squared = 0.9272 for 55 degrees of freedom
# Null hypothesis probability = 6.283638e-01
Photon flux (15-150 keV) in 95.68 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) = 4.48e-07
S(50-100 keV) = 5.77e-07
T90 vs. Hardness ratio plot
T90 = 229.664000034332 sec.
Hardness ratio (energy fluence ratio) = 1.28795
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.04425
Count Ratio (50-100 keV) / (15-25 keV) = 0.790139
Mask shadow pattern
IMX = -4.175244349364401E-01, IMY = 2.225254047237350E-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:
-239.056000 -63.136000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
185.7394 20.9800 2.7 14.2 176.7 0.9838 4.2 ------ UNKNOWN
177.9014 -31.2777 3.0 38.6 -5.1 1.3232 3.9 ------ UNKNOWN
180.8350 -37.7992 2.7 44.9 -9.8 1.6154 4.3 ------ UNKNOWN
212.8915 38.3689 2.1 41.2 -156.6 2.0711 5.4 ------ UNKNOWN
217.2750 34.1481 2.4 41.4 -148.3 1.8580 4.8 ------ UNKNOWN
203.8612 -45.7563 2.6 55.9 -29.8 5.6206 4.5 ------ UNKNOWN
230.2503 24.3534 2.9 48.1 -129.2 3.9558 3.9 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-63.136000 32.544600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
154.1179 -17.8517 2.7 38.1 36.3 1.0663 4.3 ------ UNKNOWN
181.2297 -35.3510 2.7 42.4 -10.0 0.8582 4.4 ------ UNKNOWN
201.3118 25.6221 0.9 25.3 -151.9 1.8326 12.9 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
95.944580 325.174000
325.944000 352.924000
353.944000 792.484000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.4214 35.4368 5.3 46.2 -136.1 -4.6036 -2.2 5.9 Her X-1
219.3878 28.6435 2.9 16.4 -125.3 3.5113 4.0 ------ UNKNOWN
255.9592 30.2157 2.7 48.1 -129.2 16.6420 4.2 ------ UNKNOWN
Plot creation:
Thu Jan 9 01:22:40 EST 2025