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
84.2961 +22.1650 0.0102 0.2 83.3 2.5002 18.8 TRIG_01212789
------------------------------------------
Foreground time interval of the image:
0.000 64.000 (delta_t = 64.000 [sec])
Background time interval of the image:
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 64.000000
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 64.000000
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 64.000000
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 0.000 sec. to 64.000 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.16809 ( -0.134999 0.140335 )
Norm@50keV : 2.04729E-03 ( -0.000184791 0.000181946 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 59.08 using 59 PHA bins.
# Reduced chi-squared = 1.037 for 57 degrees of freedom
# Null hypothesis probability = 3.992997e-01
Photon flux (15-150 keV) in 64 sec: 0.333351 ( -0.021999 0.0220136 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.22668e-06 ( -9.5689e-08 9.72787e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.000 sec. to 64.000 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.93434 ( -0.666363 0.0667147 )
Epeak [keV] : 11.1612 ( -11.0099 -11.1612 )
Norm@50keV : 2.81490E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 58.56 using 59 PHA bins.
# Reduced chi-squared = 1.046 for 56 degrees of freedom
# Null hypothesis probability = 3.818344e-01
Photon flux (15-150 keV) in 64 sec: 0.329020 ( -0.024105 0.011844 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.18927e-06 ( -1.25459e-07 1.24813e-07 ) ergs/cm2
Band function
Time interval is from 0.000 sec. to 64.000 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.34385 ( 1.376 1.376 )
beta : -2.34437 ( 2.38343 0.275821 )
Epeak [keV] : 26.2142 ( -26.0505 9.00486 )
Norm@50keV : 7.00561E-03 ( -0.00702613 1468.94 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 57.08 using 59 PHA bins.
# Reduced chi-squared = 1.038 for 55 degrees of freedom
# Null hypothesis probability = 3.977148e-01
Photon flux (15-150 keV) in 64 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] : 8.76040 (-0.657453 0.715493)
R^2/D10^2 : 0.245077 (-0.0660452 0.0901372)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 98.41 using 59 PHA bins.
# Reduced chi-squared = 1.726 for 57 degrees of freedom
# Null hypothesis probability = 5.457950e-04
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.310e-07 2.525e-08
25- 50 4.704e-07 3.542e-08
50-150 1.651e-07 3.542e-08
15-150 8.664e-07 6.784e-08
Thermal bremsstrahlung (OTTB)
XSPEC12>exit
XSPEC: quit
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 50.1543 (-8.96236 12.4488)
Norm : 1.85378 (-0.218517 0.269256)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.903e-07 2.723e-08
25- 50 4.174e-07 3.034e-08
50-150 4.064e-07 8.045e-08
15-150 1.114e-06 9.824e-08
Double BB
XSPEC12>exit
XSPEC: quit
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.47835 (-1.22296 1.07873)
R1^2/D10^2 : 0.668915 (-0.277794 0.62696)
kT2 [keV] : 24.8199 (-8.66977 25.2672)
R2^2/D10^2 : 2.60462E-03 (-0.00225715 0.0114976)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.823e-07 4.797e-08
25- 50 4.114e-07 8.720e-08
50-150 5.013e-07 2.507e-07
15-150 1.195e-06 3.264e-07
Peak spectrum fit
Power-law model
Time interval is from 0.000 sec. to 64.000 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.16809 ( -0.134999 0.140335 )
Norm@50keV : 2.04729E-03 ( -0.000184791 0.000181946 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 59.08 using 59 PHA bins.
# Reduced chi-squared = 1.037 for 57 degrees of freedom
# Null hypothesis probability = 3.992997e-01
Photon flux (15-150 keV) in 64 sec: 0.333351 ( -0.021999 0.0220136 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.22668e-06 ( -9.5689e-08 9.72787e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.000 sec. to 64.000 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.93434 ( -0.666363 0.0667147 )
Epeak [keV] : 11.1612 ( -11.0099 -11.1612 )
Norm@50keV : 2.81490E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 58.56 using 59 PHA bins.
# Reduced chi-squared = 1.046 for 56 degrees of freedom
# Null hypothesis probability = 3.818344e-01
Photon flux (15-150 keV) in 64 sec: 0.329020 ( -0.024105 0.011844 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.18927e-06 ( -1.25459e-07 1.24813e-07 ) ergs/cm2
Band function
Time interval is from 0.000 sec. to 64.000 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.34385 ( 1.376 1.376 )
beta : -2.34437 ( 2.38343 0.275821 )
Epeak [keV] : 26.2142 ( -26.0505 9.00486 )
Norm@50keV : 7.00561E-03 ( -0.00702613 1468.94 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 57.08 using 59 PHA bins.
# Reduced chi-squared = 1.038 for 55 degrees of freedom
# Null hypothesis probability = 3.977148e-01
Photon flux (15-150 keV) in 64 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] : 8.76040 (-0.657453 0.715493)
R^2/D10^2 : 0.245077 (-0.0660452 0.0901372)
(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 2.310e-07 2.570e-08
25- 50 4.704e-07 3.568e-08
50-150 1.651e-07 3.418e-08
15-150 8.664e-07 7.040e-08
Thermal bremsstrahlung (OTTB)
XSPEC12>exit
XSPEC: quit
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 50.1543 (-8.96236 12.4488)
Norm : 1.85378 (-0.218517 0.269256)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.903e-07 2.678e-08
25- 50 4.174e-07 3.030e-08
50-150 4.064e-07 8.038e-08
15-150 1.114e-06 9.664e-08
Double BB
XSPEC12>exit
XSPEC: quit
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.47835 (-1.22296 1.07873)
R1^2/D10^2 : 0.668915 (-0.277794 0.62696)
kT2 [keV] : 24.8199 (-8.66977 25.2672)
R2^2/D10^2 : 2.60462E-03 (-0.00225715 0.0114976)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.823e-07 5.254e-08
25- 50 4.114e-07 7.827e-08
50-150 5.013e-07 2.569e-07
15-150 1.195e-06 3.261e-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: 2.16809 ( -0.134999 0.140335 )
Norm@50keV : 2.04729E-03 ( -0.000184791 0.000181946 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 59.08 using 59 PHA bins.
# Reduced chi-squared = 1.037 for 57 degrees of freedom
# Null hypothesis probability = 3.992997e-01
Photon flux (15-150 keV) in 64 sec: 0.333351 ( -0.021999 0.0220136 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.22668e-06 ( -9.5689e-08 9.72787e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.93434 ( -0.666363 0.0667147 )
Epeak [keV] : 11.1612 ( -11.0099 -11.1612 )
Norm@50keV : 2.81490E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 58.56 using 59 PHA bins.
# Reduced chi-squared = 1.046 for 56 degrees of freedom
# Null hypothesis probability = 3.818344e-01
Photon flux (15-150 keV) in 64 sec: 0.329020 ( -0.024105 0.011844 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.18927e-06 ( -1.25459e-07 1.24813e-07 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.34385 ( 1.376 1.376 )
beta : -2.34437 ( 2.38343 0.275821 )
Epeak [keV] : 26.2142 ( -26.0505 9.00486 )
Norm@50keV : 7.00561E-03 ( -0.00702613 1468.94 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 57.08 using 59 PHA bins.
# Reduced chi-squared = 1.038 for 55 degrees of freedom
# Null hypothesis probability = 3.977148e-01
Photon flux (15-150 keV) in 64 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) = 3.86e-07
S(50-100 keV) = 3.43e-07
T90 vs. Hardness ratio plot
T90 = 64 sec.
Hardness ratio (energy fluence ratio) = 0.888601
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 0.957527
Count Ratio (50-100 keV) / (15-25 keV) = 0.377389
Mask shadow pattern
IMX = 4.181955131176806E-04, IMY = -3.549027128157085E-03
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 64.000000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 64.000000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 64.000000
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:
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
0.000000 64.000000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.4611 22.1543 0.0 0.6 -83.8 0.2461 1.8 12.7 Crab
110.7666 73.4179 2.7 53.3 12.8 2.7287 4.2 ------ UNKNOWN
92.7039 -21.0933 2.0 44.0 171.9 1.5163 5.8 ------ UNKNOWN
84.3055 22.1650 0.6 0.2 83.7 2.4903 18.7 ------ UNKNOWN
68.2175 -35.3115 2.3 59.4 -161.4 4.6885 5.0 ------ UNKNOWN
49.5024 -10.7179 3.2 47.2 -127.0 2.3436 3.6 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
77.700600 210.060000
211.000000 243.139600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.8048 21.8767 9.3 0.5 -119.2 0.3608 1.3 12.6 Crab
84.3609 22.1375 0.6 0.1 124.6 6.2466 21.5 ------ UNKNOWN
56.7024 -20.2752 3.1 50.3 -142.1 3.3677 3.8 ------ UNKNOWN
Plot creation:
Sun Feb 4 20:39:28 EST 2024