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
36.1066 -50.9544 0.0266 27.7 -145.3 0.0685 7.2 TRIG_01232755
------------------------------------------
Foreground time interval of the image:
-0.044 0.540 (delta_t = 0.584 [sec])
Background time interval of the image:
-239.216 -146.076 (delta_t = 93.140 [sec])
-145.216 -0.044 (delta_t = 145.172 [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 0.512000
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 0.512000
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 0.512000
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 -0.044 sec. to 0.540 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.83467 ( -0.377593 0.403234 )
Norm@50keV : 6.29087E-03 ( -0.00171859 0.00166982 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 66.52 using 59 PHA bins.
# Reduced chi-squared = 1.167 for 57 degrees of freedom
# Null hypothesis probability = 1.819746e-01
Photon flux (15-150 keV) in 0.584 sec: 0.878789 ( -0.20988 0.210051 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.37887e-08 ( -9.04137e-09 9.30581e-09 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.044 sec. to 0.540 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -1.85653E-02 ( -3.42301 2.05604 )
Epeak [keV] : 43.7514 ( -21.4311 -43.6664 )
Norm@50keV : 7.90856E-02 ( -0.0814802 10.7481 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 64.28 using 59 PHA bins.
# Reduced chi-squared = 1.148 for 56 degrees of freedom
# Null hypothesis probability = 2.093080e-01
Photon flux (15-150 keV) in 0.584 sec: 0.849296 ( -0.211161 0.212844 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.9046e-08 ( -8.51262e-09 1.04796e-08 ) ergs/cm2
Band function
Time interval is from -0.044 sec. to 0.540 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 4.97581 ( -14.7658 -4.97581 )
beta : -2.51089 ( -1.22151 0.658753 )
Epeak [keV] : 30.7397 ( -7.99929 6.31166 )
Norm@50keV : 272.660 ( -62.2184 1480.33 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 62.54 using 59 PHA bins.
# Reduced chi-squared = 1.137 for 55 degrees of freedom
# Null hypothesis probability = 2.260826e-01
Photon flux (15-150 keV) in 0.584 sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 3.16005e-08 ( 0 0 ) ergs/cm2
Single BB
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 10.4821 (-2.24742 2.92223)
R^2/D10^2 : 0.377020 (-0.232425 0.563351)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 65.11 using 59 PHA bins.
# Reduced chi-squared = 1.142 for 57 degrees of freedom
# Null hypothesis probability = 2.153268e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.998e-09 2.233e-09
25- 50 1.326e-08 6.099e-09
50-150 7.920e-09 4.572e-09
15-150 2.618e-08 1.105e-08
Thermal bremsstrahlung (OTTB)
XSPEC12>exit
XSPEC: quit
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 80.8444 (-39.0219 -80.8444)
Norm : 4.22106 (-1.26563 1.75938)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.401e-09 2.318e-09
25- 50 1.056e-08 4.504e-09
50-150 1.502e-08 1.204e-08
15-150 3.198e-08 1.429e-08
Double BB
XSPEC12>exit
XSPEC: quit
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 9.25415 (-9.26968 2.98672)
R1^2/D10^2 : 0.555743 (-0.551013 6.05524)
kT2 [keV] : 75.3744 (-85.4431 -85.4431)
R2^2/D10^2 : 2.71812E-04 (-0.000206283 0.629792)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.557e-09 3.320e-09
25- 50 1.272e-08 7.902e-09
50-150 1.430e-08 6.809e-09
15-150 3.257e-08 1.581e-08
Peak spectrum fit
Power-law model
Time interval is from -0.250 sec. to 0.750 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.92955 ( -0.526575 0.618224 )
Norm@50keV : 3.49653E-03 ( -0.00141969 0.00135068 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 62.05 using 59 PHA bins.
# Reduced chi-squared = 1.089 for 57 degrees of freedom
# Null hypothesis probability = 3.009936e-01
Photon flux (15-150 keV) in 1 sec: 0.508198 ( -0.164788 0.164817 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.21618e-08 ( -1.20823e-08 1.27343e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.250 sec. to 0.750 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.513151 ( -4.86572 1.63832 )
Epeak [keV] : 43.3544 ( )
Norm@50keV : 2.35475E-02 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 61.01 using 59 PHA bins.
# Reduced chi-squared = 1.089 for 56 degrees of freedom
# Null hypothesis probability = 3.007435e-01
Photon flux (15-150 keV) in 1 sec: 0.495439 ( -0.164127 0.165889 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.90225e-08 ( -1.15905e-08 1.36695e-08 ) ergs/cm2
Band function
Time interval is from -0.250 sec. to 0.750 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 4.89220 ( -12.4946 -4.8922 )
beta : -2.59145 ( -2.00105 0.890424 )
Epeak [keV] : 30.0856 ( -30.0856 8.25076 )
Norm@50keV : 158.539 ( -49.8656 5.48391e+06 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 60.45 using 59 PHA bins.
# Reduced chi-squared = 1.099 for 55 degrees of freedom
# Null hypothesis probability = 2.854342e-01
Photon flux (15-150 keV) in 1 sec: 0.504585 ( 6.49542 -0.176506 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.93962e-08 ( 0 0 ) ergs/cm2
Single BB
XSPEC: quit
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 10.1255 (-3.12371 4.59301)
R^2/D10^2 : 0.241427 (-0.241339 0.729311)
(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 5.062e-09 3.163e-09
25- 50 1.281e-08 7.815e-09
50-150 6.930e-09 5.150e-09
15-150 2.480e-08 1.569e-08
Thermal bremsstrahlung (OTTB)
XSPEC12>exit
XSPEC: quit
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 70.7330 (-40.723 -70.733)
Norm : 2.54861 (-0.965786 1.68022)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.546e-09 4.220e-09
25- 50 1.044e-08 6.300e-09
50-150 1.352e-08 1.185e-08
15-150 3.051e-08 2.119e-08
Double BB
XSPEC12>exit
XSPEC: quit
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 18.1634 (-18.4585 -18.4585)
R1^2/D10^2 : 1.49810E-02 (-0.0120761 0.69246)
kT2 [keV] : 6.85114 (-7.02358 90.7984)
R2^2/D10^2 : 0.697935 (-0.659773 -0.659773)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.992e-09 4.038e-09
25- 50 1.095e-08 7.035e-09
50-150 1.048e-08 8.155e-09
15-150 2.742e-08 1.573e-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: 1.83467 ( -0.377593 0.403234 )
Norm@50keV : 6.29087E-03 ( -0.00171859 0.00166982 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 66.52 using 59 PHA bins.
# Reduced chi-squared = 1.167 for 57 degrees of freedom
# Null hypothesis probability = 1.819746e-01
Photon flux (15-150 keV) in 0.584 sec: 0.878789 ( -0.20988 0.210051 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.37887e-08 ( -9.04137e-09 9.30581e-09 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -1.85653E-02 ( -3.42301 2.05604 )
Epeak [keV] : 43.7514 ( -13.2258 -43.6664 )
Norm@50keV : 7.90856E-02 ( -0.0814802 10.7481 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 64.28 using 59 PHA bins.
# Reduced chi-squared = 1.148 for 56 degrees of freedom
# Null hypothesis probability = 2.093080e-01
Photon flux (15-150 keV) in 0.584 sec: 0.849296 ( -0.211161 0.212844 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.9046e-08 ( -8.51262e-09 1.04796e-08 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 4.97581 ( -14.8993 -4.97581 )
beta : -2.51089 ( -1.22151 0.658753 )
Epeak [keV] : 30.7397 ( -7.99929 6.31166 )
Norm@50keV : 272.660 ( -62.2184 1480.33 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 62.54 using 59 PHA bins.
# Reduced chi-squared = 1.137 for 55 degrees of freedom
# Null hypothesis probability = 2.260826e-01
Photon flux (15-150 keV) in 0.584 sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 3.16005e-08 ( 0 0 ) ergs/cm2
S(25-50 keV) vs. S(50-100 keV) plot
S(25-50 keV) = 9.64e-09
S(50-100 keV) = 1.08e-08
T90 vs. Hardness ratio plot
T90 = 0.519999861717224 sec.
Hardness ratio (energy fluence ratio) = 1.12033
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.81959
Count Ratio (50-100 keV) / (15-25 keV) = 1.02978
Mask shadow pattern
IMX = -4.311942510309424E-01, IMY = 2.982210356466494E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.512000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.512000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.512000
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:
-239.216000 -146.076000
-145.216000 -0.044000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.5540 -40.5604 0.7 42.0 -6.9 9.8864 15.5 1.2 Vela X-1
170.4426 -60.6524 8.1 34.9 39.8 1.0509 1.4 4.1 Cen X-3
186.6580 -62.9076 5.9 37.0 52.9 1.8182 1.9 8.2 GX 301-2
127.7692 -55.9706 3.1 25.9 -2.0 1.4792 3.7 ------ UNKNOWN
60.5560 -31.0076 3.6 41.7 -103.6 4.6908 3.2 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-0.044000 0.540000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.4301 -40.5962 4.1 41.9 -7.0 -0.0363 -2.8 5.1 Vela X-1
170.0958 -60.7644 0.0 34.7 39.6 -0.0152 -1.0 10.7 Cen X-3
186.4664 -62.8097 12.6 37.1 52.7 -0.0169 -0.9 5.7 GX 301-2
316.6168 -59.1982 2.3 42.9 138.7 0.1145 5.0 ------ UNKNOWN
36.1066 -50.9543 1.6 27.7 -145.3 0.0685 7.2 ------ UNKNOWN
49.8243 -30.4668 2.4 43.9 -116.8 0.1684 4.8 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
92.784600 197.724000
202.784000 213.314000
214.784000 227.204000
228.784000 306.644000
306.784000 306.904000
307.784000 309.524000
314.784000 315.304000
316.784000 349.764000
350.784000 391.204000
392.784000 406.014000
406.784000 621.134000
622.784000 623.614000
625.784000 626.241700
627.784000 639.934000
640.784000 644.304000
646.784000 651.604000
653.784000 755.984500
756.784000 757.044000
758.784000 792.684000
795.784000 815.974000
818.784000 836.464000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.5693 -40.5447 1.0 37.5 -31.4 21.1213 11.0 2.0 Vela X-1
170.3023 -60.6394 2.4 14.7 15.4 5.4267 4.9 1.1 Cen X-3
186.7164 -62.7562 2.8 14.2 48.0 5.3877 4.1 1.8 GX 301-2
196.8169 -57.5730 2.8 20.8 57.6 5.7796 4.1 ------ UNKNOWN
170.3262 -31.8975 2.3 43.4 13.3 10.5696 4.9 ------ UNKNOWN
345.7857 -49.1337 2.2 55.6 -171.7 22.0868 5.3 ------ UNKNOWN
347.7313 -52.6932 3.2 52.0 -170.2 12.4975 3.6 ------ UNKNOWN
357.1465 -46.4775 3.0 58.0 -162.5 24.6755 3.8 ------ UNKNOWN
134.6165 -20.4282 2.3 57.5 -27.3 31.6229 5.1 ------ UNKNOWN
Plot creation:
Tue Jun 4 03:47:18 EDT 2024