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
83.7205 +22.2071 0.0078 36.4 -16.1 5.9921 24.8 TRIG_01064361
------------------------------------------
Foreground time interval of the image:
-81.799 70.701 (delta_t = 152.500 [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
Multiple GTIs in the spectrum
tstart tstop
-163.600000 98.720000
104.000000 104.996000
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.08027 ( -0.0862395 0.0879234 )
Norm@50keV : 2.20624E-03 ( -0.000109344 0.000108307 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 55.70 using 59 PHA bins.
# Reduced chi-squared = 0.9771 for 57 degrees of freedom
# Null hypothesis probability = 5.241268e-01
Photon flux (15-150 keV) in 263.3 sec: 0.343757 ( -0.0155153 0.0155993 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.38738e-06 ( -2.46018e-07 2.47221e-07 ) ergs/cm2
Cutoff power-law model
Multiple GTIs in the spectrum
tstart tstop
-163.600000 98.720000
104.000000 104.996000
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.97246 ( -0.361668 0.179979 )
Epeak [keV] : 11.5958 ( -10.7023 -11.5958 )
Norm@50keV : 2.52035E-03 ( -0.000287229 0.00138255 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 55.37 using 59 PHA bins.
# Reduced chi-squared = 0.9887 for 56 degrees of freedom
# Null hypothesis probability = 4.988495e-01
Photon flux (15-150 keV) in 263.3 sec: 0.340964 ( -0.017361 0.017255 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.32922e-06 ( -3.02505e-07 2.90446e-07 ) ergs/cm2
Band function
Multiple GTIs in the spectrum
tstart tstop
-163.600000 98.720000
104.000000 104.996000
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.46285 ( 1.47626 1.47626 )
beta : -2.18618 ( 2.18813 0.155225 )
Epeak [keV] : 31.0114 ( -31.3668 9.69819 )
Norm@50keV : 5.26151E-03 ( -0.00197548 22.0335 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 53.80 using 59 PHA bins.
# Reduced chi-squared = 0.9782 for 55 degrees of freedom
# Null hypothesis probability = 5.204529e-01
Photon flux (15-150 keV) in 263.3 sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 5.26771e-06 ( 0 0 ) ergs/cm2
Single BB
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 10.3444 ( )
R^2/D10^2 : 0.129656 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 180.38 using 59 PHA bins.
# Reduced chi-squared = 3.1646 for 57 degrees of freedom
# Null hypothesis probability = 9.863772e-15
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.519e-07 5.911e-08
25- 50 1.960e-06 8.965e-08
50-150 1.127e-06 1.307e-07
15-150 3.839e-06 2.027e-07
Thermal bremsstrahlung (OTTB)
XSPEC12>exit
XSPEC: quit
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 65.4030 (-8.39596 10.3629)
Norm : 1.67732 (-0.132008 0.146259)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.124e-06 6.740e-08
25- 50 1.755e-06 7.649e-08
50-150 2.140e-06 2.109e-07
15-150 5.019e-06 2.462e-07
Double BB
XSPEC12>exit
XSPEC: quit
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.75924 (-0.766699 0.757908)
R1^2/D10^2 : 0.539994 (-0.171957 0.300871)
kT2 [keV] : 25.2712 (-4.60088 7.16578)
R2^2/D10^2 : 2.81654E-03 (-0.00165138 0.0033316)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.087e-06 1.132e-07
25- 50 1.751e-06 2.116e-07
50-150 2.393e-06 7.116e-07
15-150 5.231e-06 8.518e-07
Peak spectrum fit
Power-law model
Time interval is from -141.136 sec. to -140.136 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.58573 ( -0.479585 0.502332 )
Norm@50keV : 5.47485E-03 ( -0.00152821 0.00147441 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 51.66 using 59 PHA bins.
# Reduced chi-squared = 0.9062 for 57 degrees of freedom
# Null hypothesis probability = 6.751287e-01
Photon flux (15-150 keV) in 1 sec: 0.700470 ( -0.187578 0.188027 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.12925e-08 ( -1.50066e-08 1.51623e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -141.136 sec. to -140.136 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.10787 ( -1.78392 0.0365436 )
Epeak [keV] : 42.6260 ( )
Norm@50keV : 2.91556E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 51.56 using 59 PHA bins.
# Reduced chi-squared = 0.9207 for 56 degrees of freedom
# Null hypothesis probability = 6.433954e-01
Photon flux (15-150 keV) in 1 sec: 0.703855 ( -0.191802 0.184985 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.12848e-08 ( -1.50003e-08 1.49549e-08 ) ergs/cm2
Band function
Time interval is from -141.136 sec. to -140.136 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.27433 ( 1.27557 1.27557 )
beta : -1.58542 ( 1.5857 0.479492 )
Epeak [keV] : 29.4037 ( -28.7682 -28.7682 )
Norm@50keV : 1.14698E-02 ( -0.0114968 221.005 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 51.66 using 59 PHA bins.
# Reduced chi-squared = 0.9392 for 55 degrees of freedom
# Null hypothesis probability = 6.031986e-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] : 16.3100 (-5.27695 8.10445)
R^2/D10^2 : 5.69001E-02 (-0.0428062 0.164086)
(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 3.116e-09 1.909e-09
25- 50 1.333e-08 7.974e-09
50-150 2.496e-08 1.457e-08
15-150 4.140e-08 2.262e-08
Thermal bremsstrahlung (OTTB)
XSPEC12>exit
XSPEC: quit
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.359 (-199.362 -199.362)
Norm : 2.83360 (-0.742535 0.967492)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.056e-09 4.336e-09
25- 50 1.357e-08 8.295e-09
50-150 2.977e-08 1.822e-08
15-150 5.040e-08 3.005e-08
Double BB
XSPEC12>exit
XSPEC: quit
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 4.38073 (-1.92634 3.54014)
R1^2/D10^2 : 5.67904 (-5.24699 105.406)
kT2 [keV] : 25.3063 (-9.60691 46.9682)
R2^2/D10^2 : 1.07185E-02 (-0.0101352 0.0467722)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.074e-09 5.715e-09
25- 50 1.043e-08 5.485e-09
50-150 3.213e-08 1.908e-08
15-150 5.163e-08 2.920e-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: 2.06738 ( -0.108701 0.111614 )
Norm@50keV : 2.23602E-03 ( -0.000145579 0.000143597 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 49.26 using 59 PHA bins.
# Reduced chi-squared = 0.8643 for 57 degrees of freedom
# Null hypothesis probability = 7.570907e-01
Photon flux (15-150 keV) in 152.5 sec: 0.346226 ( -0.0193303 0.0194031 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.15895e-06 ( -1.88771e-07 1.90209e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.08636 ( -0.362706 0.0266797 )
Epeak [keV] : 206.228 ( )
Norm@50keV : 2.18397E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 49.28 using 59 PHA bins.
# Reduced chi-squared = 0.8799 for 56 degrees of freedom
# Null hypothesis probability = 7.253979e-01
Photon flux (15-150 keV) in 152.5 sec: 0.345934 ( -0.019555 0.019406 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.15869e-06 ( -2.26707e-07 1.89069e-07 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.79795 ( 1.809 1.809 )
beta : -2.11995 ( 2.12045 0.15734 )
Epeak [keV] : 26.7510 ( -26.2149 -26.2149 )
Norm@50keV : 3.27300E-03 ( -0.000846331 916270 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 49.06 using 59 PHA bins.
# Reduced chi-squared = 0.8920 for 55 degrees of freedom
# Null hypothesis probability = 6.998553e-01
Photon flux (15-150 keV) in 152.5 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) = 1.66e-06
S(50-100 keV) = 1.57e-06
T90 vs. Hardness ratio plot
T90 = 227.427999854088 sec.
Hardness ratio (energy fluence ratio) = 0.945783
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.04172
Count Ratio (50-100 keV) / (15-25 keV) = 0.515169
Mask shadow pattern
IMX = 7.079069140020381E-01, IMY = 2.046783067693740E-01
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:
-81.799400 70.700600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.7042 22.1556 0.5 36.4 -16.1 5.3340 22.2 9.3 Crab
52.2399 11.5855 3.0 50.2 26.7 2.5721 3.9 ------ UNKNOWN
251.4310 74.3708 2.9 47.3 176.8 1.6633 4.0 ------ UNKNOWN
214.3380 79.1578 3.0 40.4 -173.8 0.9647 3.8 ------ UNKNOWN
222.8867 67.9827 2.1 51.4 -169.6 2.5670 5.5 ------ UNKNOWN
81.9438 6.5442 2.9 51.9 -11.8 1.5823 3.9 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-81.799400 70.700600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.7040 22.1556 0.5 36.4 -16.1 5.3378 22.1 9.3 Crab
52.2403 11.5849 2.9 50.2 26.7 2.6207 3.9 ------ UNKNOWN
251.4304 74.3679 2.9 47.3 176.8 1.6844 4.0 ------ UNKNOWN
214.3119 79.1473 3.0 40.4 -173.8 0.9895 3.9 ------ UNKNOWN
222.8864 67.9821 2.1 51.4 -169.6 2.6168 5.6 ------ UNKNOWN
81.9450 6.5452 2.9 51.9 -11.8 1.5936 4.0 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
129.900590 189.210000
190.000000 243.170000
244.000000 246.570000
248.000000 248.024600
250.000000 322.370000
323.000000 661.330000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.7009 22.1686 0.2 0.0 21.0 21.2549 46.6 10.0 Crab
63.0642 -5.0657 2.4 33.9 42.6 3.5018 4.8 ------ UNKNOWN
72.0913 -21.8441 2.9 45.5 18.8 3.8219 3.9 ------ UNKNOWN
68.9253 -3.9666 2.9 29.9 34.3 2.3508 3.9 ------ UNKNOWN
64.7776 55.6266 3.0 36.3 165.5 2.6518 3.9 ------ UNKNOWN
63.8419 61.3507 2.7 41.5 169.3 3.5178 4.3 ------ UNKNOWN
106.0338 19.7011 4.4 21.0 -83.7 1.5660 2.6 ------ UNKNOWN
130.3028 60.1801 2.6 49.9 -148.2 5.3637 4.4 ------ UNKNOWN
128.6475 24.4624 3.7 41.1 -98.7 7.5601 3.1 ------ UNKNOWN
Plot creation:
Sun Aug 8 21:13:13 EDT 2021