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
278.1292 +34.4226 0.0371 22.9 -30.7 0.4359 5.2 TRIG_01014012
------------------------------------------
Foreground time interval of the image:
25.704 65.064 (delta_t = 39.360 [sec])
Background time interval of the image:
-239.000 25.704 (delta_t = 264.704 [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
8 ms binning
From T100_start-3 s to T100_start+3 s
2 ms binning
From T100_start-1 s to T100_start+1 s
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 25.704 sec. to 65.064 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.59176 ( -0.452071 0.463763 )
Norm@50keV : 6.95629E-04 ( -0.000217484 0.00021468 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 76.35 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.45e-02 with 57 degrees of freedom
Photon flux (15-150 keV) in 39.36 sec: 8.91551E-02 ( -0.0261479 0.0262119 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.56437e-07 ( -8.32153e-08 8.69502e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 25.704 sec. to 65.064 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -6.79550 ( )
Epeak [keV] : 34.5274 ( )
Norm@50keV : 195.773 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared 72.14 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.20e-02 with 56 degrees of freedom
Photon flux (15-150 keV) in 39.36 sec: 7.56024E-02 ( -0.0229161 0.0304656 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.50334e-07 ( -4.56844e-08 1.3045e-07 ) ergs/cm2
Band function
Time interval is from 25.704 sec. to 65.064 sec.
XSPEC12>exit
XSPEC: quit
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 4.31338 ( -2.35328 3.43075 )
beta : -2.85419 ( 9.37167 19.3713 )
Epeak [keV] : 35.1489 ( -9.50392 7.91459 )
Norm@50keV : 5.18113 ( -5.05007 1.73924 )
------------------------------------------------------------
Photon flux (15-150 keV) in 39.36 sec: 8.80879E-02 ( 6.91191 -0.0243435 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.17467e-07 ( 0 0 ) ergs/cm2
Single BB
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 10.6694 (-2.59815 4.26133)
R^2/D10^2 : 3.66329E-02 (-0.0262598 0.0673138)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 73.02 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.49e-02 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.406e-08 2.084e-08
25- 50 9.256e-08 5.440e-08
50-150 5.810e-08 4.180e-08
15-150 1.847e-07 9.691e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 141.038 (-83.1505 -131.519)
Norm : 0.368009 (-0.117251 0.178727)
------------------------------------------------------------
#Fit statistic : Chi-Squared 75.20 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.35e-02 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.738e-08 2.257e-08
25- 50 6.866e-08 4.080e-08
50-150 1.320e-07 8.325e-08
15-150 2.381e-07 1.496e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 27.1773 (-24.7373 -24.7373)
R1^2/D10^2 : 5.50757E-04 (-0.000591208 0.0757785)
kT2 [keV] : 8.67108 (-8.6551 4.60065)
R2^2/D10^2 : 6.24099E-02 (-0.0629174 -0.0629174)
------------------------------------------------------------
#Fit statistic : Chi-Squared 71.61 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.56e-02 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.805e-08 2.783e-08
25- 50 8.620e-08 6.410e-08
50-150 1.082e-07 6.386e-08
15-150 2.324e-07 1.504e-07
Peak spectrum fit
Power-law model
Time interval is from 61.140 sec. to 62.140 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.12603 ( -1.01906 1.6223 )
Norm@50keV : 1.75149E-03 ( -0.00141462 0.00140784 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 65.07 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.16e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.279155 ( -0.163092 0.163895 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.63207e-08 ( -1.09841e-08 1.30719e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 61.140 sec. to 62.140 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.235976 ( )
Epeak [keV] : 34.8400 ( )
Norm@50keV : 2.60770E-02 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared 64.59 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.02e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.270790 ( -0.27079 0.161767 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.40202e-08 ( -8.78923e-09 1.40873e-08 ) ergs/cm2
Band function
Time interval is from 61.140 sec. to 62.140 sec.
XSPEC12>exit
XSPEC: quit
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.308772 ( 1.18576 1.18576 )
beta : -9.94534 ( 9.45745 19.4575 )
Epeak [keV] : 34.4249 ( -20.9109 159.171 )
Norm@50keV : 2.36598E-02 ( -0.0269825 1.05093e+06 )
------------------------------------------------------------
Photon flux (15-150 keV) in 1 sec: 6.72280E-02 ( 6.93277 -0.0198307 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.04172e-09 ( 0 0 ) ergs/cm2
Single BB
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 8.96172 (-4.43981 7.96999)
R^2/D10^2 : 0.214204 (-0.214203 2.8122)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 64.66 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.27e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.342e-09 2.303e-09
25- 50 7.056e-09 4.815e-09
50-150 2.657e-09 2.565e-09
15-150 1.306e-08 9.125e-09
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 48.4798 (-48.4646 -48.4646)
Norm : 1.65383 (-1.65405 4.09292)
------------------------------------------------------------
#Fit statistic : Chi-Squared 64.74 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.25e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.014e-09 2.636e-09
25- 50 5.702e-09 3.738e-09
50-150 5.375e-09 5.370e-09
15-150 1.509e-08 1.212e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 3.23601 (-3.22133 35.4149)
R1^2/D10^2 : 3.88361 (-3.94361 -3.94361)
kT2 [keV] : 10.0399 (-10.0407 -10.0407)
R2^2/D10^2 : 0.123795 (-0.123799 2.616)
------------------------------------------------------------
#Fit statistic : Chi-Squared 64.52 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.78e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.690e-09 2.221e-09
25- 50 6.579e-09 5.030e-09
50-150 3.360e-09 2.355e-09
15-150 1.363e-08 1.171e-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: 1.59176 ( -0.452071 0.463763 )
Norm@50keV : 6.95629E-04 ( -0.000217484 0.00021468 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 76.35 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.45e-02 with 57 degrees of freedom
Photon flux (15-150 keV) in 39.36 sec: 8.91551E-02 ( -0.0261479 0.0262119 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.56437e-07 ( -8.32153e-08 8.69502e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -6.79550 ( )
Epeak [keV] : 34.5274 ( )
Norm@50keV : 195.773 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared 72.14 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.20e-02 with 56 degrees of freedom
Photon flux (15-150 keV) in 39.36 sec: 7.56024E-02 ( -0.0229161 0.0304656 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.50334e-07 ( -4.56844e-08 1.3045e-07 ) ergs/cm2
Band function
XSPEC12>exit
XSPEC: quit
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 4.31338 ( -2.35328 3.43075 )
beta : -2.85419 ( 9.37167 19.3713 )
Epeak [keV] : 35.1489 ( -9.50392 7.91459 )
Norm@50keV : 5.18113 ( -5.05007 1.73924 )
------------------------------------------------------------
Photon flux (15-150 keV) in 39.36 sec: 8.80879E-02 ( 6.91191 -0.0243435 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.17467e-07 ( 0 0 ) ergs/cm2
S(25-50 keV) vs. S(50-100 keV) plot
S(25-50 keV) = 6.62e-08
S(50-100 keV) = 8.79e-08
T90 vs. Hardness ratio plot
T90 = 22.4639998674393 sec.
Hardness ratio (energy fluence ratio) = 1.32779
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.82289
Count Ratio (50-100 keV) / (15-25 keV) = 0.610241
Mask shadow pattern
IMX = 3.635848841923888E-01, IMY = 2.155625906870272E-01
TIME vs. PHA plot around the trigger time
TIME vs. DetID plot around the trigger time
100 us light curve (15-350 keV)
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:
-239.000000 25.704000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.4748 35.2491 5.9 40.8 -16.0 0.8432 1.9 5.7 Her X-1
288.8195 11.0258 4.2 32.3 -83.8 1.5592 2.7 5.0 GRS 1915+105
299.6030 35.2321 2.6 6.7 -62.9 1.3963 4.4 1.9 Cyg X-1
308.1461 40.9449 2.2 2.2 104.2 1.5077 5.2 1.7 Cyg X-3
325.9111 38.3046 0.0 15.3 150.4 -0.1624 -0.5 12.3 Cyg X-2
311.5742 49.7400 2.9 11.1 81.1 1.1847 4.0 ------ UNKNOWN
288.3306 54.3611 2.7 19.3 30.0 1.3627 4.3 ------ UNKNOWN
354.1544 10.6603 2.5 51.2 173.4 4.9829 4.5 ------ UNKNOWN
232.5418 35.1329 2.5 57.2 -6.3 6.3476 4.5 ------ UNKNOWN
321.1793 11.7078 2.9 30.6 -146.9 1.5023 4.1 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
25.704000 65.064000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.2509 35.4560 0.0 40.9 -15.6 -0.1918 -1.7 12.2 Her X-1
288.7249 11.1323 0.0 32.2 -83.5 -0.1281 -0.8 12.0 GRS 1915+105
299.4940 35.3985 0.0 6.6 -61.3 0.0613 0.8 12.7 Cyg X-1
308.2779 40.8718 6.0 2.2 107.4 0.1566 1.9 9.0 Cyg X-3
326.1657 38.1595 5.9 15.6 150.8 -0.1612 -2.0 9.7 Cyg X-2
355.5638 11.7476 2.3 51.5 171.2 1.4928 5.1 ------ UNKNOWN
311.7970 3.2144 2.0 36.5 -126.5 0.8119 5.7 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
116.300600 455.970000
457.000000 491.160000
492.000000 849.000620
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.5091 35.2044 30.5 19.4 0.9 -1.0098 -0.4 8.7 Her X-1
268.4791 -1.6167 0.0 37.2 -82.0 -9.9028 -1.2 11.9 SW J1753.5-0127
288.7975 10.9455 20.7 25.4 -123.1 1.8171 0.6 0.1 GRS 1915+105
299.6025 35.3366 3.5 17.5 162.7 8.2969 3.3 8.1 Cyg X-1
308.1454 40.9439 4.7 24.4 147.4 7.1116 2.5 1.7 Cyg X-3
326.2604 38.3000 7.9 38.5 151.6 -7.1170 -1.5 4.4 Cyg X-2
236.5464 60.9384 3.3 37.5 49.7 16.9126 4.1 ------ UNKNOWN
237.0632 60.8493 4.2 37.2 49.8 14.6991 3.6 ------ UNKNOWN
213.0998 31.3372 2.7 53.8 8.0 32.5017 4.3 ------ UNKNOWN
Plot creation:
Tue Dec 22 17:19:49 EST 2020