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
284.6961 -8.1950 0.0446 6.7 -116.0 2.6429 4.3 TRIG_00889483
------------------------------------------
Foreground time interval of the image:
14.836 123.111 (delta_t = 108.275 [sec])
177.000 304.716 (delta_t = 127.716 [sec])
Background time interval of the image:
-14.899 14.836 (delta_t = 29.735 [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
Multiple GTIs in the spectrum
tstart tstop
14.836000 123.110600
177.000000 304.716000
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.31396 ( -0.357221 0.398327 )
Norm@50keV : 3.35629E-04 ( -9.6344e-05 9.61149e-05 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 66.11 using 59 PHA bins.
# Reduced chi-squared = 1.160 for 57 degrees of freedom
# Null hypothesis probability = 1.912077e-01
Photon flux (15-150 keV) in 236 sec: 5.91132E-02 ( -0.0112042 0.0112071 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.58931e-07 ( -1.75948e-07 1.86976e-07 ) ergs/cm2
Cutoff power-law model
Multiple GTIs in the spectrum
tstart tstop
14.836000 123.110600
177.000000 304.716000
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -0.876943 ( -8.82056 2.70552 )
Epeak [keV] : 27.1940 ( )
Norm@50keV : 5.45463E-02 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 62.00 using 59 PHA bins.
# Reduced chi-squared = 1.107 for 56 degrees of freedom
# Null hypothesis probability = 2.709276e-01
Photon flux (15-150 keV) in 236 sec: 5.49910E-02 ( -0.0110077 0.0111667 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.57805e-07 ( -1.30314e-07 1.91495e-07 ) ergs/cm2
Band function
Multiple GTIs in the spectrum
tstart tstop
14.836000 123.110600
177.000000 304.716000
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 5.00000 ( -5.09774 -5 )
beta : -3.37853 ( -2.93864 0.849701 )
Epeak [keV] : 25.5447 ( -4.67205 3.63311 )
Norm@50keV : 72.5305 ( -13.1441 200.898 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 59.02 using 59 PHA bins.
# Reduced chi-squared = 1.073 for 55 degrees of freedom
# Null hypothesis probability = 3.309533e-01
Photon flux (15-150 keV) in 236 sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 6.56734e-07 ( -6.55082e-07 -1.67673e-07 ) ergs/cm2
Single BB
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 6.97184 (-1.12726 1.40002)
R^2/D10^2 : 0.119176 (-0.0639816 0.131118)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 61.96 using 59 PHA bins.
# Reduced chi-squared = 1.087 for 57 degrees of freedom
# Null hypothesis probability = 3.035863e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.187e-07 7.645e-08
25- 50 2.972e-07 1.036e-07
50-150 4.853e-08 3.284e-08
15-150 5.644e-07 1.835e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 33.6259 (-11.8032 23.4287)
Norm : 0.438730 (-0.141999 0.218736)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 63.80 using 59 PHA bins.
# Reduced chi-squared = 1.119 for 57 degrees of freedom
# Null hypothesis probability = 2.497581e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.224e-07 5.907e-08
25- 50 2.699e-07 7.856e-08
50-150 1.708e-07 1.140e-07
15-150 6.630e-07 1.979e-07
Double BB
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.64037 (-1.31481 1.20991)
R1^2/D10^2 : 0.141244 (-0.0616625 0.167578)
kT2 [keV] : 200.000 (-200 -200)
R2^2/D10^2 : 3.86417E-06 (-3.56052e-06 3.40182e-05)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 59.01 using 59 PHA bins.
#Fit statistic : Chi-Squared = 58.98 using 59 PHA bins.
# Reduced chi-squared = 1.073 for 55 degrees of freedom
# Reduced chi-squared = 1.072 for 55 degrees of freedom
# Null hypothesis probability = 3.311651e-01
# Null hypothesis probability = 3.321750e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.201e-07 1.096e-07
25- 50 2.893e-07 1.229e-07
50-150 2.703e-07 4.462e-08
15-150 7.797e-07 2.316e-07
Peak spectrum fit
Power-law model
Time interval is from 186.108 sec. to 187.108 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.20786 ( -0.900416 1.36679 )
Norm@50keV : 2.28328E-03 ( -0.00228328 0.0014641 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 40.88 using 59 PHA bins.
# Reduced chi-squared = 0.7172 for 57 degrees of freedom
# Null hypothesis probability = 9.471287e-01
Photon flux (15-150 keV) in 1 sec: 0.379574 ( -0.168713 0.168744 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.14917e-08 ( -1.17078e-08 1.30886e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 186.108 sec. to 187.108 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.77978 ( )
Epeak [keV] : 27.1061 ( )
Norm@50keV : 3.74921E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 40.99 using 59 PHA bins.
# Reduced chi-squared = 0.7320 for 56 degrees of freedom
# Null hypothesis probability = 9.338291e-01
Photon flux (15-150 keV) in 1 sec: 0.379355 ( -0.168684 0.16843 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.12516e-08 ( -1.16238e-08 1.3153e-08 ) ergs/cm2
Band function
Time interval is from 186.108 sec. to 187.108 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.61348 ( 1.61495 1.61495 )
beta : -2.20594 ( 2.20693 0.896742 )
Epeak [keV] : 9.13364 ( -8.73463 -8.73463 )
Norm@50keV : 8.78415E-03 ( -0.00897501 58.6821 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 40.88 using 59 PHA bins.
# Reduced chi-squared = 0.7432 for 55 degrees of freedom
# Null hypothesis probability = 9.218642e-01
Photon flux (15-150 keV) in 1 sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 2.78277e-09 ( -2.77577e-09 -7.1048e-10 ) ergs/cm2
Single BB
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 10.1331 (-6.17582 7.2914)
R^2/D10^2 : 0.163189 (-0.162864 7.61486)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 42.64 using 59 PHA bins.
# Reduced chi-squared = 0.7481 for 57 degrees of freedom
# Null hypothesis probability = 9.213176e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.428e-09 2.242e-09
25- 50 8.682e-09 5.680e-09
50-150 4.707e-09 4.309e-09
15-150 1.682e-08 1.117e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 50.6390 (-50.6385 -50.6385)
Norm : 2.12307 (-1.20419 4.82739)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 41.15 using 59 PHA bins.
# Reduced chi-squared = 0.7219 for 57 degrees of freedom
# Null hypothesis probability = 9.436124e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.206e-09 3.381e-09
25- 50 7.511e-09 4.840e-09
50-150 7.380e-09 6.460e-09
15-150 2.010e-08 1.428e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 2.83743 (-2.83743 26.1158)
R1^2/D10^2 : 30.5619 (-30.5621 -30.5621)
kT2 [keV] : 13.3886 (-13.3886 -13.3886)
R2^2/D10^2 : 4.61637E-02 (-0.0461638 0.284605)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 40.07 using 59 PHA bins.
# Reduced chi-squared = 0.7285 for 55 degrees of freedom
# Null hypothesis probability = 9.348289e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.762e-09 2.691e-09
25- 50 6.710e-09 4.260e-09
50-150 7.182e-09 5.145e-09
15-150 1.965e-08 1.133e-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: 2.31396 ( -0.357221 0.398327 )
Norm@50keV : 3.35629E-04 ( -9.6344e-05 9.61149e-05 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 66.11 using 59 PHA bins.
# Reduced chi-squared = 1.160 for 57 degrees of freedom
# Null hypothesis probability = 1.912077e-01
Photon flux (15-150 keV) in 236 sec: 5.91132E-02 ( -0.0112042 0.0112071 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.58931e-07 ( -1.75948e-07 1.86976e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -0.876943 ( -8.82056 2.70552 )
Epeak [keV] : 27.1940 ( )
Norm@50keV : 5.45463E-02 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 62.00 using 59 PHA bins.
# Reduced chi-squared = 1.107 for 56 degrees of freedom
# Null hypothesis probability = 2.709276e-01
Photon flux (15-150 keV) in 236 sec: 5.49910E-02 ( -0.0110077 0.0111667 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.57805e-07 ( -1.30314e-07 1.91495e-07 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 5.00000 ( -5.09774 -5 )
beta : -3.37853 ( -2.93864 0.849701 )
Epeak [keV] : 25.5447 ( -4.67205 3.63311 )
Norm@50keV : 72.5305 ( -13.1441 200.898 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 59.02 using 59 PHA bins.
# Reduced chi-squared = 1.073 for 55 degrees of freedom
# Null hypothesis probability = 3.309533e-01
Photon flux (15-150 keV) in 236 sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 6.56734e-07 ( -6.55082e-07 -1.67673e-07 ) ergs/cm2
S(25-50 keV) vs. S(50-100 keV) plot
S(25-50 keV) = 2.46e-07
S(50-100 keV) = 1.98e-07
T90 vs. Hardness ratio plot
T90 = 254.81199991703 sec.
Hardness ratio (energy fluence ratio) = 0.804878
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.00207
Count Ratio (50-100 keV) / (15-25 keV) = 0.234869
Mask shadow pattern
IMX = -5.112628115423513E-02, IMY = 1.049913011029837E-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:
-14.899400 14.836000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
244.9920 -15.6239 0.8 32.9 71.9 2.4784 14.2 1.2 Sco X-1
254.4088 35.2788 4.2 51.1 149.2 1.2433 2.8 4.5 Her X-1
255.7988 -37.9281 9.0 34.0 27.2 0.1611 1.3 10.2 4U 1700-377
256.4325 -36.3789 3.8 32.6 28.4 0.3822 3.0 2.7 GX 349+2
263.0716 -24.8260 3.1 20.4 37.9 0.3193 3.7 5.9 GX 1+4
264.6101 -44.2775 6.8 35.7 11.4 0.2058 1.7 11.8 4U 1735-44
268.3676 -1.4440 118.8 13.5 126.2 -0.0087 -0.1 0.5 SW J1753.5-0127
270.2351 -24.9212 8.1 16.3 21.7 0.1177 1.4 9.8 GX 5-1
270.4817 -25.6174 0.0 16.8 19.8 0.1882 2.3 12.3 GRS 1758-258
273.8478 -14.0604 10.8 5.6 45.7 0.0802 1.1 9.3 GX 17+2
275.9439 -30.4106 10.4 20.0 0.6 0.0901 1.1 2.8 H1820-303
284.8819 -24.8396 14.8 15.5 -28.1 0.0632 0.8 9.7 HT1900.1-2455
288.8014 10.9418 4.1 23.9 -159.6 0.2544 2.8 0.3 GRS 1915+105
299.5574 35.2008 2.0 50.0 -162.9 1.2127 5.7 1.6 Cyg X-1
263.1767 -33.7212 0.0 27.0 23.1 0.1905 2.0 11.6 GX 354-0
245.0537 2.2804 2.3 35.6 103.7 1.0279 5.0 ------ UNKNOWN
239.3269 -30.0699 2.8 41.2 50.3 1.0543 4.1 ------ UNKNOWN
267.1510 -32.2753 2.1 24.1 18.2 0.4750 5.4 ------ UNKNOWN
310.2202 36.0414 2.3 55.4 -154.4 1.8344 5.1 ------ UNKNOWN
316.2549 -48.6900 2.8 49.5 -37.8 1.0250 4.2 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
14.836000 123.110600
177.000000 304.716000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
244.9920 -15.7384 3.3 32.9 71.7 4.6803 3.5 5.9 Sco X-1
254.4355 35.2887 3.5 51.1 149.2 -11.3201 -3.3 3.4 Her X-1
255.7948 -37.9448 0.0 34.1 27.1 -0.6427 -0.7 10.9 4U 1700-377
256.4214 -36.3729 3.4 32.6 28.4 -3.2744 -3.4 3.1 GX 349+2
263.1407 -24.9210 0.0 20.4 37.6 -1.2917 -1.9 12.7 GX 1+4
264.8634 -44.5419 6.7 35.9 10.9 1.6092 1.7 7.5 4U 1735-44
268.4969 -1.6141 0.0 13.3 126.1 -1.3434 -2.0 12.4 SW J1753.5-0127
270.1690 -24.9118 8.6 16.3 21.9 -0.8892 -1.3 11.8 GX 5-1
270.1285 -25.8306 6.7 17.1 20.4 1.1438 1.7 10.8 GRS 1758-258
273.8405 -14.1682 259.7 5.7 44.9 -0.0274 -0.0 12.5 GX 17+2
275.7972 -30.2103 7.3 19.8 1.0 -1.0188 -1.6 11.5 H1820-303
285.1885 -25.0211 10.8 15.8 -28.8 -0.6647 -1.1 10.3 HT1900.1-2455
288.9480 11.0604 64.5 24.0 -159.4 -0.1234 -0.2 11.2 GRS 1915+105
299.5430 35.2063 8.0 50.0 -163.0 -2.2402 -1.5 2.3 Cyg X-1
263.0747 -34.0043 10.3 27.3 22.9 0.8605 1.1 11.0 GX 354-0
266.2499 33.5674 2.3 45.6 160.2 8.0729 5.1 ------ UNKNOWN
282.8612 38.3883 2.1 49.1 179.0 8.6950 5.4 ------ UNKNOWN
307.2528 -40.8062 2.4 39.5 -40.7 4.9922 4.9 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
426.400600 438.900600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.4015 35.2277 5.0 41.9 30.9 -0.2477 -2.3 7.4 Her X-1
268.5519 -1.4723 6.0 55.9 -18.5 -0.3148 -1.9 11.1 SW J1753.5-0127
288.7431 11.0661 796.0 34.8 -34.1 -0.0009 -0.0 7.9 GRS 1915+105
299.6237 35.1562 1.4 9.1 -19.7 0.3742 8.3 3.2 Cyg X-1
308.1653 41.1296 42.9 0.3 -83.2 0.0126 0.3 10.9 Cyg X-3
326.2090 38.2758 5.7 14.3 -151.8 -0.0925 -2.0 3.3 Cyg X-2
12.8674 49.4390 2.8 44.7 168.0 0.4509 4.2 ------ UNKNOWN
Plot creation:
Tue Feb 19 08:20:09 EST 2019