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
297.2547 +36.0684 0.0184 51.8 -159.3 7.7458 10.4 TRIG_01186304
------------------------------------------
Foreground time interval of the image:
0.000 243.044 (delta_t = 243.044 [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 320.000000
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 320.000000
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 320.000000
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 243.044 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.81019 ( -0.150782 0.154052 )
Norm@50keV : 2.18731E-03 ( -0.000213309 0.000211831 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 48.98 using 59 PHA bins.
# Reduced chi-squared = 0.8593 for 57 degrees of freedom
# Null hypothesis probability = 7.662480e-01
Photon flux (15-150 keV) in 243 sec: 0.302605 ( -0.0291259 0.0292108 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.89157e-06 ( -4.81638e-07 4.84078e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.000 sec. to 243.044 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.778591 ( -0.810863 0.67961 )
Epeak [keV] : 55.9940 ( -9.48845 22.3949 )
Norm@50keV : 7.66684E-03 ( -0.00425485 0.0127527 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 41.75 using 59 PHA bins.
# Reduced chi-squared = 0.7455 for 56 degrees of freedom
# Null hypothesis probability = 9.218076e-01
Photon flux (15-150 keV) in 243 sec: 0.291321 ( -0.029987 0.030077 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.60004e-06 ( -5.17809e-07 5.2279e-07 ) ergs/cm2
Band function
Time interval is from 0.000 sec. to 243.044 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 4.93549 ( -6.01049 -4.93549 )
beta : -2.07057 ( -0.275617 0.205232 )
Epeak [keV] : 28.5002 ( -4.63566 3.81514 )
Norm@50keV : 121.826 ( -11.0567 296.43 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 39.52 using 59 PHA bins.
# Reduced chi-squared = 0.7185 for 55 degrees of freedom
# Null hypothesis probability = 9.426775e-01
Photon flux (15-150 keV) in 243 sec: 0.290141 ( 6.70986 -0.029775 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.7229e-06 ( -4.7212e-06 -4.93849e-07 ) ergs/cm2
Single BB
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 12.4250 (-1.24305 1.38514)
R^2/D10^2 : 6.56254E-02 (-0.02176 0.0322143)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 58.09 using 59 PHA bins.
# Reduced chi-squared = 1.019 for 57 degrees of freedom
# Null hypothesis probability = 4.350573e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.218e-07 8.845e-08
25- 50 1.710e-06 1.978e-07
50-150 1.623e-06 2.907e-07
15-150 3.854e-06 4.228e-07
Thermal bremsstrahlung (OTTB)
XSPEC12>exit
XSPEC: quit
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 98.8618 (-25.2912 42.2857)
Norm : 1.35529 (-0.171277 0.198758)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.608e-07 1.243e-07
25- 50 1.485e-06 1.471e-07
50-150 2.391e-06 8.198e-07
15-150 4.736e-06 9.149e-07
Double BB
XSPEC12>exit
XSPEC: quit
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.72804 (-2.13786 2.26404)
R1^2/D10^2 : 0.257966 (-0.139172 0.452178)
kT2 [keV] : 22.9271 (-6.46287 19.5566)
R2^2/D10^2 : 4.14746E-03 (-0.00373213 0.00701175)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.552e-07 2.985e-07
25- 50 1.606e-06 5.961e-07
50-150 2.299e-06 1.136e-06
15-150 4.660e-06 1.964e-06
Peak spectrum fit
Power-law model
Time interval is from 0.000 sec. to 243.044 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.81019 ( -0.150782 0.154052 )
Norm@50keV : 2.18731E-03 ( -0.000213309 0.000211831 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 48.98 using 59 PHA bins.
# Reduced chi-squared = 0.8593 for 57 degrees of freedom
# Null hypothesis probability = 7.662480e-01
Photon flux (15-150 keV) in 243 sec: 0.302605 ( -0.0291259 0.0292108 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.89157e-06 ( -4.81638e-07 4.84078e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.000 sec. to 243.044 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.778591 ( -0.810863 0.67961 )
Epeak [keV] : 55.9940 ( -9.48845 22.3949 )
Norm@50keV : 7.66684E-03 ( -0.00425485 0.0127527 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 41.75 using 59 PHA bins.
# Reduced chi-squared = 0.7455 for 56 degrees of freedom
# Null hypothesis probability = 9.218076e-01
Photon flux (15-150 keV) in 243 sec: 0.291321 ( -0.029987 0.030077 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.60004e-06 ( -5.17809e-07 5.2279e-07 ) ergs/cm2
Band function
Time interval is from 0.000 sec. to 243.044 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 4.93549 ( -6.01049 -4.93549 )
beta : -2.07057 ( -0.275617 0.205232 )
Epeak [keV] : 28.5002 ( -4.63566 3.81514 )
Norm@50keV : 121.826 ( -11.0567 296.43 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 39.52 using 59 PHA bins.
# Reduced chi-squared = 0.7185 for 55 degrees of freedom
# Null hypothesis probability = 9.426775e-01
Photon flux (15-150 keV) in 243 sec: 0.290141 ( 6.70986 -0.029775 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.7229e-06 ( -4.7212e-06 -4.93849e-07 ) ergs/cm2
Single BB
XSPEC: quit
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 12.4250 (-1.24305 1.38514)
R^2/D10^2 : 6.56254E-02 (-0.02176 0.0322143)
(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 5.218e-07 8.991e-08
25- 50 1.710e-06 1.875e-07
50-150 1.623e-06 3.153e-07
15-150 3.854e-06 4.350e-07
Thermal bremsstrahlung (OTTB)
XSPEC12>exit
XSPEC: quit
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 98.8618 (-25.2912 42.2857)
Norm : 1.35529 (-0.171277 0.198758)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.608e-07 1.270e-07
25- 50 1.485e-06 1.448e-07
50-150 2.391e-06 8.207e-07
15-150 4.736e-06 9.611e-07
Double BB
XSPEC12>exit
XSPEC: quit
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.72804 (-2.13786 2.26404)
R1^2/D10^2 : 0.257966 (-0.139172 0.452178)
kT2 [keV] : 22.9271 (-6.46287 19.5566)
R2^2/D10^2 : 4.14746E-03 (-0.00373213 0.00701175)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.552e-07 3.129e-07
25- 50 1.606e-06 6.443e-07
50-150 2.299e-06 1.195e-06
15-150 4.660e-06 1.863e-06
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: 1.81019 ( -0.150782 0.154052 )
Norm@50keV : 2.18731E-03 ( -0.000213309 0.000211831 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 48.98 using 59 PHA bins.
# Reduced chi-squared = 0.8593 for 57 degrees of freedom
# Null hypothesis probability = 7.662480e-01
Photon flux (15-150 keV) in 243 sec: 0.302605 ( -0.0291259 0.0292108 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.89157e-06 ( -4.81638e-07 4.84078e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.778591 ( -0.810863 0.67961 )
Epeak [keV] : 55.9940 ( -9.48845 22.3949 )
Norm@50keV : 7.66684E-03 ( -0.00425485 0.0127527 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 41.75 using 59 PHA bins.
# Reduced chi-squared = 0.7455 for 56 degrees of freedom
# Null hypothesis probability = 9.218076e-01
Photon flux (15-150 keV) in 243 sec: 0.291321 ( -0.029987 0.030077 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.60004e-06 ( -5.17809e-07 5.2279e-07 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 4.93549 ( -6.01049 -4.93549 )
beta : -2.07057 ( -0.275617 0.205232 )
Epeak [keV] : 28.5002 ( -4.63566 3.81514 )
Norm@50keV : 121.826 ( -11.0567 296.43 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 39.52 using 59 PHA bins.
# Reduced chi-squared = 0.7185 for 55 degrees of freedom
# Null hypothesis probability = 9.426775e-01
Photon flux (15-150 keV) in 243 sec: 0.290141 ( 6.70986 -0.029775 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.7229e-06 ( -4.7212e-06 -4.93849e-07 ) ergs/cm2
S(25-50 keV) vs. S(50-100 keV) plot
S(25-50 keV) = 1.38e-06
S(50-100 keV) = 1.58e-06
T90 vs. Hardness ratio plot
T90 = 320 sec.
Hardness ratio (energy fluence ratio) = 1.14493
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.71519
Count Ratio (50-100 keV) / (15-25 keV) = 1.02698
Mask shadow pattern
IMX = -1.187182865783212E+00, IMY = 4.487872352313782E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 320.000000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 320.000000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 320.000000
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 243.044300
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
299.5941 35.2003 77.0 49.7 -159.5 0.1013 0.1 0.2 Cyg X-1
308.0898 40.9213 3.9 46.3 -148.6 -1.8370 -3.0 2.1 Cyg X-3
326.3960 38.4327 9.7 34.4 -136.3 0.5103 1.2 12.5 Cyg X-2
297.2547 36.0684 1.1 51.8 -159.3 7.7429 10.4 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
-60.000000 -38.780000
-10.000000 63.100000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
299.4246 35.2853 0.0 49.8 -159.5 -0.5260 -1.6 9.5 Cyg X-1
308.1137 40.8336 5.2 46.2 -148.7 -0.6442 -2.2 7.1 Cyg X-3
326.3457 38.3422 46.1 34.3 -136.4 0.0495 0.3 8.3 Cyg X-2
313.3139 -9.2436 2.5 37.1 132.8 1.3263 4.6 ------ UNKNOWN
299.6133 7.4044 3.1 45.7 163.0 1.3194 3.7 ------ UNKNOWN
23.5487 -12.6554 3.1 43.2 10.5 0.9657 3.7 ------ UNKNOWN
297.2726 36.0711 1.7 51.8 -159.3 2.3829 6.7 ------ UNKNOWN
Plot creation:
Mon Aug 21 20:47:04 EDT 2023