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
244.7753 -15.7763 0.0169 19.1 -45.9 2.5133 11.4 TRIG_01220155
------------------------------------------
Foreground time interval of the image:
-20.499 72.601 (delta_t = 93.100 [sec])
Background time interval of the image:
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
Time interval is from -40.512 sec. to 221.312 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 6.23316 ( -0.399479 0.406942 )
Norm@50keV : 6.00175E-05 ( -1.92792e-05 2.61905e-05 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 51.52 using 59 PHA bins.
# Reduced chi-squared = 0.9038 for 57 degrees of freedom
# Null hypothesis probability = 6.800908e-01
Photon flux (15-150 keV) in 261.8 sec: 0.312464 ( -0.0289975 0.0291464 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.42994e-06 ( -2.09159e-07 2.09921e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -40.512 sec. to 221.312 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.00000 ( )
Epeak [keV] : 50.0000 ( )
Norm@50keV : 1.35758E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 367.59 using 59 PHA bins.
# Reduced chi-squared = 6.5641 for 56 degrees of freedom
# Null hypothesis probability = 2.224538e-47
Photon flux (15-150 keV) in 261.8 sec: 0.306520 ( -0.031854 0.031225 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.35465e-06 ( -2.29051e-07 2.23928e-07 ) ergs/cm2
Band function
Time interval is from -40.512 sec. to 221.312 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 1.47245 ( -7.48523 4.31506 )
beta : -7.62566 ( 7.61427 1.23602 )
Epeak [keV] : 9.08970 ( -1.10098 0.812308 )
Norm@50keV : 165.121 ( -105.48 56418.4 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 46.40 using 59 PHA bins.
# Reduced chi-squared = 0.8436 for 55 degrees of freedom
# Null hypothesis probability = 7.889087e-01
Photon flux (15-150 keV) in 261.8 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] : 2.48578 (-0.169301 0.191107)
R^2/D10^2 : 157.015 (-71.6502 128.741)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 47.99 using 59 PHA bins.
# Reduced chi-squared = 0.8420 for 57 degrees of freedom
# Null hypothesis probability = 7.964825e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.163e-06 4.080e-07
25- 50 1.554e-07 3.786e-08
50-150 4.642e-11 3.583e-11
15-150 2.319e-06 4.184e-07
Thermal bremsstrahlung (OTTB)
XSPEC12>exit
XSPEC: quit
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 4.28463 (-0.426059 0.512324)
Norm : 129.044 (-51.8165 85.7826)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.174e-06 3.665e-07
25- 50 1.896e-07 4.389e-08
50-150 4.241e-10 2.800e-10
15-150 2.364e-06 3.983e-07
Double BB
XSPEC12>exit
XSPEC: quit
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.71824 (-5.5434 -5.5434)
R1^2/D10^2 : 9.61239E-02 (-0.117225 226.021)
kT2 [keV] : 2.33185 (-2.31838 0.280883)
R2^2/D10^2 : 244.170 (-147.473 -254.641)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.184e-06 1.136e-06
25- 50 2.057e-07 1.093e-07
50-150 6.844e-09 7.447e-09
15-150 2.396e-06 1.267e-06
Peak spectrum fit
Power-law model
Time interval is from 116.048 sec. to 117.048 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 3.69270 ( -0.877056 1.24002 )
Norm@50keV : 1.27085E-03 ( -0.000927689 0.00145334 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 55.82 using 59 PHA bins.
# Reduced chi-squared = 0.9793 for 57 degrees of freedom
# Null hypothesis probability = 5.194892e-01
Photon flux (15-150 keV) in 1 sec: 0.602494 ( -0.168457 0.169652 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.26097e-08 ( -7.88103e-09 9.34072e-09 ) ergs/cm2
Cutoff power-law model
Time interval is from 116.048 sec. to 117.048 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.00000 ( )
Epeak [keV] : 50.0000 ( )
Norm@50keV : 1.01029E-02 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 72.56 using 59 PHA bins.
# Reduced chi-squared = 1.296 for 56 degrees of freedom
# Null hypothesis probability = 6.752025e-02
Photon flux (15-150 keV) in 1 sec: 0.601116 ( -0.167602 0.168782 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.23767e-08 ( -8.0354e-09 9.2339e-09 ) ergs/cm2
Band function
Time interval is from 116.048 sec. to 117.048 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.62967 ( 1.55257 1.55257 )
beta : -3.70363 ( 3.78973 0.966492 )
Epeak [keV] : 3.34531 ( -3.8838 146.431 )
Norm@50keV : 7.57409E-02 ( -0.0985776 1.2878e+07 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 55.81 using 59 PHA bins.
# Reduced chi-squared = 1.015 for 55 degrees of freedom
# Null hypothesis probability = 4.441107e-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] : 3.62695 (-1.03507 1.50269)
R^2/D10^2 : 25.8572 (-25.8715 161.955)
(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 1.434e-08 8.185e-09
25- 50 3.879e-09 2.598e-09
50-150 2.532e-11 2.830e-11
15-150 1.824e-08 1.056e-08
Thermal bremsstrahlung (OTTB)
XSPEC12>exit
XSPEC: quit
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 9.82294 (-4.40755 9.26184)
Norm : 21.2589 (-21.2537 67.7367)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.385e-08 8.145e-09
25- 50 5.822e-09 3.780e-09
50-150 3.802e-10 3.870e-10
15-150 2.005e-08 1.163e-08
Double BB
XSPEC12>exit
XSPEC: quit
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 2.71298 (-2.66878 2.23261)
R1^2/D10^2 : 108.508 (-117.974 -117.974)
kT2 [keV] : 8.31725 (-8.1482 -8.1482)
R2^2/D10^2 : 0.233178 (-0.261015 68.4885)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.356e-08 7.560e-09
25- 50 6.676e-09 4.118e-09
50-150 1.671e-09 1.041e-09
15-150 2.191e-08 1.092e-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: 5.95628 ( -0.491679 0.514129 )
Norm@50keV : 8.11428E-05 ( -3.25428e-05 4.79417e-05 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 57.44 using 59 PHA bins.
# Reduced chi-squared = 1.008 for 57 degrees of freedom
# Null hypothesis probability = 4.586194e-01
Photon flux (15-150 keV) in 93.1 sec: 0.319594 ( -0.0332204 0.0332703 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.95614e-07 ( -9.01346e-08 9.01352e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 6.13638E-02 ( )
Epeak [keV] : 6.59737 ( )
Norm@50keV : 7.17514 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 54.62 using 59 PHA bins.
# Reduced chi-squared = 0.9754 for 56 degrees of freedom
# Null hypothesis probability = 5.270833e-01
Photon flux (15-150 keV) in 93.1 sec: 0.316423 ( -0.034929 0.034566 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.67888e-07 ( -9.22844e-08 9.15545e-08 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -8.81616 ( 4.1771 8.81616 )
beta : -6.01531 ( -0.46864 0.543749 )
Epeak [keV] : 417.490 ( -417.49 -417.49 )
Norm@50keV : 1.03964E-02 ( -0.00400761 0.00698146 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 57.48 using 59 PHA bins.
# Reduced chi-squared = 1.045 for 55 degrees of freedom
# Null hypothesis probability = 3.833705e-01
Photon flux (15-150 keV) in 93.1 sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 7.3656e-07 ( -7.35908e-07 -7.3656e-07 ) ergs/cm2
S(25-50 keV) vs. S(50-100 keV) plot
S(25-50 keV) = 2.65e-07
S(50-100 keV) = 1.41e-08
T90 vs. Hardness ratio plot
T90 = 220.755999922752 sec.
Hardness ratio (energy fluence ratio) = 0.0532075
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 0.0845595
Count Ratio (50-100 keV) / (15-25 keV) = -0.0192924
Mask shadow pattern
IMX = 2.412903893973802E-01, IMY = 2.489330140662139E-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:
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-20.499400 72.600600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
244.7991 -15.7627 0.0 19.1 -46.0 2.4678 11.2 12.7 Sco X-1
254.2831 35.2506 5.6 40.3 -164.8 0.5721 2.0 10.2 Her X-1
255.8348 -37.8019 4.0 42.9 -37.3 0.9912 2.9 7.6 4U 1700-377
256.4304 -36.4372 3.6 42.0 -39.0 1.1280 3.2 0.9 GX 349+2
263.0296 -24.6168 9.4 37.5 -58.4 -0.4610 -1.2 7.8 GX 1+4
264.6288 -44.6043 3.8 52.3 -38.9 -2.8493 -3.1 10.5 4U 1735-44
268.3165 -1.5681 7.3 34.7 -98.7 0.6073 1.6 7.6 SW J1753.5-0127
270.1017 -25.2132 5.3 43.2 -63.0 -1.5170 -2.2 12.8 GX 5-1
270.2854 -25.8638 6.2 43.7 -62.3 -1.3449 -1.9 7.3 GRS 1758-258
262.9799 -33.8399 45.7 43.5 -47.5 -0.1118 -0.3 0.6 GX 354-0
192.2675 -13.4772 2.8 43.1 58.9 2.9214 4.1 ------ UNKNOWN
201.4518 -0.8354 3.7 32.2 77.4 1.1202 3.2 ------ UNKNOWN
231.4139 -47.1637 2.3 47.1 -9.2 1.6162 5.1 ------ UNKNOWN
251.5423 -54.4516 2.6 56.3 -23.7 3.7870 4.5 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
125.100600 363.130000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
244.8060 -15.7577 3.8 0.1 -117.5 1.4309 3.0 12.3 Sco X-1
254.4276 35.3676 7.3 52.0 -177.6 -2.3518 -1.6 2.1 Her X-1
255.8063 -37.8637 2.3 24.1 -29.4 2.4833 4.9 8.6 4U 1700-377
256.6101 -36.4407 6.0 23.2 -32.5 -0.9536 -1.9 8.5 GX 349+2
262.8446 -24.7556 5.8 19.2 -66.9 1.0755 2.0 9.0 GX 1+4
264.8492 -44.5434 5.0 33.4 -34.1 -1.2942 -2.3 7.2 4U 1735-44
268.4644 -1.6056 5.5 27.4 -126.5 -1.1623 -2.1 10.8 SW J1753.5-0127
270.2432 -25.2182 8.2 25.6 -71.9 -0.8776 -1.4 8.6 GX 5-1
270.4123 -25.6166 26.2 25.9 -71.1 -0.3233 -0.5 9.6 GRS 1758-258
274.1015 -14.1702 12.7 28.4 -97.0 -0.6239 -0.9 9.8 GX 17+2
275.8836 -30.5056 10.8 32.0 -64.8 -0.7720 -1.1 8.6 H1820-303
285.1143 -24.8563 5.4 38.8 -77.4 -2.8719 -2.1 5.7 HT1900.1-2455
262.9592 -33.9544 9.4 24.5 -46.4 -0.6891 -1.2 7.3 GX 354-0
213.3792 16.5190 2.5 44.7 127.2 11.4253 4.6 ------ UNKNOWN
197.7922 -40.3035 2.9 47.4 41.6 5.3409 3.9 ------ UNKNOWN
255.2916 -60.4321 3.3 45.3 -15.0 2.5230 3.5 ------ UNKNOWN
280.5054 20.2228 2.8 50.3 -142.2 5.8085 4.0 ------ UNKNOWN
282.9536 -11.4373 2.3 37.4 -99.4 6.5135 5.1 ------ UNKNOWN
289.3313 -60.9925 2.6 55.2 -32.1 11.2752 4.4 ------ UNKNOWN
Plot creation:
Sat Mar 16 06:36:35 EDT 2024