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
244.9590 -15.8461 0.1012 32.1 -115.5 3.6015 1.9 TRIG_01016010
------------------------------------------
Foreground time interval of the image:
-173.180 130.132 (delta_t = 303.312 [sec])
131.000 452.501 (delta_t = 321.501 [sec])
Background time interval of the image:
-219.899 -209.930 (delta_t = 9.969 [sec])
-209.000 -173.180 (delta_t = 35.820 [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 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
-173.180000 130.132300
131.000000 545.668000
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 5.93907 ( -0.303872 0.305174 )
Norm@50keV : 1.12296E-04 ( -2.65699e-05 3.29356e-05 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 52.39 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.48e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 718 sec: 0.434743 ( -0.0356997 0.0361057 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.40401e-06 ( -6.95238e-07 7.01856e-07 ) ergs/cm2
Cutoff power-law model
Multiple GTIs in the spectrum
tstart tstop
-173.180000 130.132300
131.000000 545.668000
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.55448 ( )
Epeak [keV] : 2.21558 ( )
Norm@50keV : 0.374695 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared 46.07 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.26e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 718 sec: 0.417193 ( -0.040829 0.039977 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.95626e-06 ( -8.02868e-07 7.85851e-07 ) ergs/cm2
Band function
Multiple GTIs in the spectrum
tstart tstop
-173.180000 130.132300
131.000000 545.668000
XSPEC12>exit
XSPEC: quit
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -7.61528 ( 4.42896 7.61528 )
beta : -5.96832 ( -0.284435 0.326809 )
Epeak [keV] : 315.990 ( -315.99 -315.99 )
Norm@50keV : 1.48654E-02 ( -0.00339608 0.00470667 )
------------------------------------------------------------
Photon flux (15-150 keV) in 718 sec: 0.380885 ( ) 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] : 2.73486 (-0.155397 0.172746)
R^2/D10^2 : 105.271 (-40.7093 64.9208)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 48.90 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.69e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.768e-06 1.087e-06
25- 50 8.100e-07 1.305e-07
50-150 5.931e-10 3.107e-10
15-150 8.579e-06 1.218e-06
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 4.83069 (-0.397992 0.464213)
Norm : 109.042 (-35.8639 52.8355)
------------------------------------------------------------
#Fit statistic : Chi-Squared 46.08 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.49e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.993e-06 9.912e-07
25- 50 9.335e-07 1.422e-07
50-150 4.055e-09 2.187e-09
15-150 8.930e-06 1.116e-06
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 2.55886 (-2.345 0.304743)
R1^2/D10^2 : 165.715 (-84.3319 -167.759)
kT2 [keV] : 6.78619 (-6.24652 -6.61929)
R2^2/D10^2 : 5.41748E-02 (-0.0654655 99.1137)
------------------------------------------------------------
#Fit statistic : Chi-Squared 45.90 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.04e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.797e-06 1.009e-06
25- 50 8.366e-07 1.234e-07
50-150 4.743e-07 3.416e-07
15-150 9.107e-06 1.135e-06
Peak spectrum fit
Power-law model
Time interval is from 201.804 sec. to 202.804 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.63028 ( -0.806434 1.19962 )
Norm@50keV : 3.92378E-03 ( -0.00392187 0.0025484 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 65.19 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.13e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.836659 ( -0.266483 0.266019 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.07668e-08 ( -1.71445e-08 1.92422e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 201.804 sec. to 202.804 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 3.89149 ( -1.98688 -1.98688 )
Epeak [keV] : 472.666 ( -86.1533 -471.583 )
Norm@50keV : 9.78537E-04 ( -0.000989837 0.00374909 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 62.74 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.50e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.833995 ( -0.264659 0.264595 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.13153e-08 ( -1.77231e-08 1.48355e-08 ) ergs/cm2
Band function
Time interval is from 201.804 sec. to 202.804 sec.
XSPEC12>exit
XSPEC: quit
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.87408 ( 1.87412 1.87412 )
beta : -2.62999 ( -1.19978 0.806544 )
Epeak [keV] : 0.674660 ( -0.674909 -0.674909 )
Norm@50keV : 5.58661E-02 ( 0.822496 -0.0558933 )
------------------------------------------------------------
Photon flux (15-150 keV) in 1 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] : 5.50349 (-1.65775 1.98705)
R^2/D10^2 : 4.34227 (-4.34228 18.7488)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 66.97 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.72e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.527e-08 9.140e-09
25- 50 1.254e-08 7.980e-09
50-150 7.951e-10 7.280e-10
15-150 2.861e-08 1.772e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 18.3312 (-9.86826 63.214)
Norm : 10.7472 (-7.44019 24.3851)
------------------------------------------------------------
#Fit statistic : Chi-Squared 66.72 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.78e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.542e-08 9.170e-09
25- 50 1.260e-08 8.585e-09
50-150 3.246e-09 3.080e-09
15-150 3.126e-08 2.004e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.10273 (-1.83132 1.48569)
R1^2/D10^2 : 5.80786 (-3.7188 35.0783)
kT2 [keV] : 89.7064 (-71.4519 -95.0957)
R2^2/D10^2 : 3.20444E-04 (-0.00025054 0.00819273)
------------------------------------------------------------
#Fit statistic : Chi-Squared 60.91 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.72e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.529e-08 9.485e-09
25- 50 1.232e-08 7.490e-09
50-150 2.623e-08 8.450e-09
15-150 5.384e-08 2.009e-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: 5.87482 ( -0.310554 0.312792 )
Norm@50keV : 1.21736E-04 ( -2.9593e-05 3.68439e-05 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 58.88 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.07e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 624.8 sec: 0.441951 ( -0.0365816 0.0369869 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.34689e-06 ( -6.22645e-07 6.28043e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.53526 ( )
Epeak [keV] : 2.33305 ( )
Norm@50keV : 0.375715 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared 52.67 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.02e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 624.8 sec: 0.424272 ( -0.041705 0.040857 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.94427e-06 ( -7.15896e-07 7.01338e-07 ) ergs/cm2
Band function
XSPEC12>exit
XSPEC: quit
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -7.59802 ( 4.47755 7.59802 )
beta : -5.90397 ( -0.292041 0.333432 )
Epeak [keV] : 319.089 ( -319.089 -319.089 )
Norm@50keV : 1.61141E-02 ( -0.00378751 0.00525804 )
------------------------------------------------------------
Photon flux (15-150 keV) in 624.8 sec: 0.380885 ( ) 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) = 1.18e-06
S(50-100 keV) = 7.66e-08
T90 vs. Hardness ratio plot
T90 = 601.131999969482 sec.
Hardness ratio (energy fluence ratio) = 0.0649153
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 0.105663
Count Ratio (50-100 keV) / (15-25 keV) = 0.00800137
Mask shadow pattern
IMX = -2.699272863648293E-01, IMY = 5.662455991203250E-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:
-219.899410 -209.930000
-209.000000 -173.180000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
170.3915 -60.6184 7.8 43.8 17.0 -0.2620 -1.5 2.2 Cen X-3
186.7913 -62.9002 6.2 39.4 6.8 -0.2534 -1.9 8.6 GX 301-2
245.0012 -15.7732 1.3 32.2 -115.6 1.3149 8.9 8.1 Sco X-1
255.8446 -37.9577 5.9 37.6 -73.7 0.4476 1.9 9.6 4U 1700-377
256.5540 -36.2704 3.7 38.1 -76.5 -0.8145 -3.1 10.8 GX 349+2
182.8905 -29.7370 4.0 26.1 66.1 0.3606 2.9 ------ UNKNOWN
191.7485 -21.7449 2.2 19.7 90.3 0.5532 5.1 ------ UNKNOWN
219.2464 18.7039 2.5 46.4 177.3 0.9321 4.6 ------ UNKNOWN
223.2047 24.6254 2.6 52.9 -179.3 1.4316 4.5 ------ UNKNOWN
237.8370 26.7033 3.0 59.2 -165.0 2.5555 3.9 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-173.180000 130.132300
131.000000 452.500600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
170.1584 -60.5536 4.2 43.8 17.2 6.2592 2.7 6.2 Cen X-3
186.8003 -62.8926 6.2 39.4 6.8 3.3119 1.9 8.3 GX 301-2
244.9360 -15.7698 7.7 32.1 -115.6 2.8293 1.5 8.2 Sco X-1
255.8680 -37.9506 3.5 37.7 -73.7 -9.6574 -3.3 8.5 4U 1700-377
256.5525 -36.2708 4.3 38.1 -76.5 8.8539 2.7 10.7 GX 349+2
272.8346 -65.7321 2.3 53.2 -37.9 31.2123 4.9 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
616.500600 667.260000
668.000000 723.130000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.6179 35.4092 7.2 42.6 -12.0 -6.5628 -1.6 8.8 Her X-1
288.8075 10.8956 4.5 35.7 -75.9 -18.0556 -2.5 3.0 GRS 1915+105
299.8116 35.2951 6.2 9.8 -59.3 -5.4854 -1.9 12.2 Cyg X-1
307.9977 41.1470 0.0 1.2 -45.8 -3.5881 -1.3 12.7 Cyg X-3
326.1046 38.1813 10.7 13.2 167.3 -2.8714 -1.1 9.0 Cyg X-2
355.5220 28.7767 3.0 39.3 161.7 15.7294 3.8 ------ UNKNOWN
Plot creation:
Wed Jan 6 16:45:03 EST 2021