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
335.4042 +7.0484 0.0088 21.1 -0.8 1.3200 21.8 TRIG_01404904
------------------------------------------
Foreground time interval of the image:
-5.480 15.949 (delta_t = 21.429 [sec])
Background time interval of the image:
-60.152 -5.480 (delta_t = 54.672 [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 1.024000
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 1.024000
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 1.024000
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 -5.480 sec. to 125.080 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.39628 ( -0.198098 0.196119 )
Norm@50keV : 9.53236E-04 ( -9.92594e-05 9.892e-05 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 58.86 using 59 PHA bins.
# Reduced chi-squared = 1.033 for 57 degrees of freedom
# Null hypothesis probability = 4.072219e-01
Photon flux (15-150 keV) in 130.6 sec: 0.115989 ( -0.0123332 0.0123618 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.20384e-06 ( -1.40322e-07 1.41489e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -5.480 sec. to 125.080 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.39203 ( -0.562586 0.122641 )
Epeak [keV] : 133.559 ( )
Norm@50keV : 2.81580E-04 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 54.55 using 59 PHA bins.
# Reduced chi-squared = 0.9742 for 56 degrees of freedom
# Null hypothesis probability = 5.297754e-01
Photon flux (15-150 keV) in 130.6 sec: 0.115951 ( -0.012349 0.012343 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.20132e-06 ( -1.37757e-07 1.31168e-07 ) ergs/cm2
Band function
Time interval is from -5.480 sec. to 125.080 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.17743 ( 1.17742 1.17742 )
beta : -1.39620 ( -0.196122 0.198276 )
Epeak [keV] : 20.8335 ( -20.8274 -20.8274 )
Norm@50keV : 1.91966E-03 ( -0.001065 0.00708597 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 58.86 using 59 PHA bins.
# Reduced chi-squared = 1.070 for 55 degrees of freedom
# Null hypothesis probability = 3.361303e-01
Photon flux (15-150 keV) in 130.6 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] : 16.1108 (-3.24355 4.65416)
R^2/D10^2 : 9.74714E-03 (-0.00545182 0.011483)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 107.68 using 59 PHA bins.
# Reduced chi-squared = 1.8891 for 57 degrees of freedom
# Null hypothesis probability = 5.757973e-05
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.821e-08 1.574e-08
25- 50 2.887e-07 4.754e-08
50-150 5.252e-07 1.075e-07
15-150 8.821e-07 1.394e-07
Thermal bremsstrahlung (OTTB)
XSPEC12>exit
XSPEC: quit
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-44.4577 -200)
Norm : 0.476199 (-0.0494326 0.0494326)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.549e-07 4.361e-08
25- 50 2.979e-07 1.601e-07
50-150 6.534e-07 3.465e-07
15-150 1.106e-06 5.825e-07
Double BB
XSPEC12>exit
XSPEC: quit
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.30115 (-1.34805 1.56313)
R1^2/D10^2 : 0.127228 (-0.0642974 0.144229)
kT2 [keV] : 54.6217 (-19.5321 97.4755)
R2^2/D10^2 : 2.14996E-04 (-0.000156318 0.000465453)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.569e-07 6.036e-08
25- 50 2.830e-07 8.580e-08
50-150 8.763e-07 4.422e-07
15-150 1.316e-06 5.113e-07
Peak spectrum fit
Power-law model
Time interval is from 6.412 sec. to 7.412 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.21720 ( -0.199575 0.196047 )
Norm@50keV : 1.09564E-02 ( -0.00132821 0.00132796 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 61.69 using 59 PHA bins.
# Reduced chi-squared = 1.082 for 57 degrees of freedom
# Null hypothesis probability = 3.120339e-01
Photon flux (15-150 keV) in 1 sec: 1.28926 ( -0.159625 0.159839 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.10623e-07 ( -1.47638e-08 1.48814e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 6.412 sec. to 7.412 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.668391 ( -0.896205 0.709206 )
Epeak [keV] : 125.848 ( )
Norm@50keV : 2.05189E-02 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 60.13 using 59 PHA bins.
# Reduced chi-squared = 1.074 for 56 degrees of freedom
# Null hypothesis probability = 3.285563e-01
Photon flux (15-150 keV) in 1 sec: 1.26986 ( -0.16235 0.16224 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.06993e-07 ( -1.61105e-08 1.5892e-08 ) ergs/cm2
Band function
Time interval is from 6.412 sec. to 7.412 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 2.87641 ( -4.34043 -3.72098 )
beta : -1.44487 ( -0.392804 0.312752 )
Epeak [keV] : 36.3555 ( -20.5031 61.6652 )
Norm@50keV : 5.95242 ( -5.94793 102.58 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 58.47 using 59 PHA bins.
# Reduced chi-squared = 1.063 for 55 degrees of freedom
# Null hypothesis probability = 3.492536e-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] : 17.3516 (-2.67173 3.32304)
R^2/D10^2 : 9.58920E-02 (-0.0425477 0.0728798)
(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 5.846e-09 1.421e-09
25- 50 2.629e-08 5.465e-09
50-150 5.687e-08 1.358e-08
15-150 8.900e-08 1.752e-08
Thermal bremsstrahlung (OTTB)
XSPEC12>exit
XSPEC: quit
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-37.4362 -200)
Norm : 5.32481 (-0.656548 0.656548)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.326e-08 7.515e-09
25- 50 2.550e-08 1.407e-08
50-150 5.593e-08 3.109e-08
15-150 9.469e-08 5.235e-08
Double BB
XSPEC12>exit
XSPEC: quit
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 9.69680 (-3.00298 3.61869)
R1^2/D10^2 : 0.439874 (-0.256756 0.469984)
kT2 [keV] : 37.4133 (-12.0517 -37.4211)
R2^2/D10^2 : 5.71639E-03 (-0.00514935 0.0228781)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.412e-09 5.104e-09
25- 50 2.705e-08 1.438e-08
50-150 7.296e-08 3.957e-08
15-150 1.094e-07 5.365e-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: 1.28730 ( -0.115334 0.114206 )
Norm@50keV : 4.12251E-03 ( -0.000267677 0.000267661 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 60.83 using 59 PHA bins.
# Reduced chi-squared = 1.067 for 57 degrees of freedom
# Null hypothesis probability = 3.396781e-01
Photon flux (15-150 keV) in 21.43 sec: 0.490695 ( -0.0331618 0.0332129 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.75752e-07 ( -6.24669e-08 6.2734e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.19693 ( -0.442057 0.146712 )
Epeak [keV] : 441.545 ( -481.497 -481.497 )
Norm@50keV : 4.55836E-03 ( -0.00125049 0.00275295 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 60.74 using 59 PHA bins.
# Reduced chi-squared = 1.085 for 56 degrees of freedom
# Null hypothesis probability = 3.091613e-01
Photon flux (15-150 keV) in 21.43 sec: 0.488796 ( -0.034241 0.034182 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.7117e-07 ( -6.63151e-08 6.55629e-08 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 3.99521 ( -3.99578 -3.99578 )
beta : -1.32797 ( -0.135668 0.129377 )
Epeak [keV] : 24.8687 ( -24.8631 109.623 )
Norm@50keV : 66.3126 ( -66.4169 102.266 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 59.85 using 59 PHA bins.
# Reduced chi-squared = 1.088 for 55 degrees of freedom
# Null hypothesis probability = 3.040254e-01
Photon flux (15-150 keV) in 21.43 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) = 2.82e-07
S(50-100 keV) = 4.29e-07
T90 vs. Hardness ratio plot
T90 = 116.896000027657 sec.
Hardness ratio (energy fluence ratio) = 1.52128
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.50211
Count Ratio (50-100 keV) / (15-25 keV) = 1.09957
Mask shadow pattern
IMX = 3.855045564478867E-01, IMY = 5.642856939992835E-03
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.024000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.024000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.024000
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:
-60.152000 -5.480000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
326.0972 38.2398 8.6 51.6 18.6 0.4764 1.3 6.0 Cyg X-2
359.9341 15.9828 4.0 26.4 64.7 0.3985 2.9 ------ UNKNOWN
355.3473 -47.0767 2.6 38.9 -143.8 0.6702 4.4 ------ UNKNOWN
330.7163 -41.1016 2.3 36.8 -113.5 0.9489 5.0 ------ UNKNOWN
297.4862 10.1096 2.2 55.2 -29.1 2.4481 5.3 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-5.480000 15.948600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
326.2443 38.3454 17.9 51.7 18.8 -0.1701 -0.6 3.7 Cyg X-2
335.4042 7.0484 0.5 21.1 -0.8 1.3201 21.8 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
95.748600 242.895700
498.848000 548.231400
549.848000 561.735800
563.848000 574.730800
584.848000 589.658400
591.848000 615.963800
617.848000 962.903700
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
299.5733 35.2102 0.7 43.2 -37.8 24.5147 17.4 1.0 Cyg X-1
308.0316 40.9377 3.4 41.7 -25.0 4.5972 3.4 3.7 Cyg X-3
326.0248 38.2361 5.5 32.3 -7.3 1.7390 2.1 8.6 Cyg X-2
355.6681 -37.7734 2.3 48.7 165.1 10.6969 5.1 ------ UNKNOWN
332.3940 16.7419 2.7 10.1 -10.0 3.5061 4.3 ------ UNKNOWN
299.3967 -20.3408 2.4 44.7 -122.0 15.9794 4.9 ------ UNKNOWN
299.5159 -24.9996 3.1 47.4 -127.3 15.3074 3.7 ------ UNKNOWN
Plot creation:
Sat Oct 18 20:18:20 EDT 2025