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
300.3044 +35.3116 0.0121 40.3 -16.5 2.8261 15.9 TRIG_01217732
------------------------------------------
Foreground time interval of the image:
0.000 64.000 (delta_t = 64.000 [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
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 0.000 sec. to 64.000 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.76125 ( -0.154408 0.157885 )
Norm@50keV : 2.79035E-03 ( -0.000251534 0.000247939 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 76.89 using 59 PHA bins.
# Reduced chi-squared = 1.349 for 57 degrees of freedom
# Null hypothesis probability = 4.068838e-02
Photon flux (15-150 keV) in 64 sec: 0.378878 ( -0.0318986 0.0319988 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.64683e-06 ( -1.52543e-07 1.53834e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.000 sec. to 64.000 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.14890 ( -0.577032 0.0692953 )
Epeak [keV] : 60.0621 ( )
Norm@50keV : 1.74196E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 75.70 using 59 PHA bins.
# Reduced chi-squared = 1.352 for 56 degrees of freedom
# Null hypothesis probability = 4.085469e-02
Photon flux (15-150 keV) in 64 sec: 0.379706 ( -0.032846 0.031262 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.64849e-06 ( -1.54138e-07 1.46035e-07 ) ergs/cm2
Band function
Time interval is from 0.000 sec. to 64.000 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.42917 ( 1.42917 1.42917 )
beta : -1.76123 ( 1.76123 0.154407 )
Epeak [keV] : 18.5388 ( -18.5388 -18.5388 )
Norm@50keV : 6.47271E-03 ( -0.00391616 85.9464 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 76.89 using 59 PHA bins.
# Reduced chi-squared = 1.398 for 55 degrees of freedom
# Null hypothesis probability = 2.726222e-02
Photon flux (15-150 keV) in 64 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] : 11.7947 ( )
R^2/D10^2 : 9.30374E-02 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 132.16 using 59 PHA bins.
# Reduced chi-squared = 2.3185 for 57 degrees of freedom
# Null hypothesis probability = 6.635076e-08
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.749e-07 3.056e-08
25- 50 5.393e-07 5.805e-08
50-150 4.459e-07 9.302e-08
15-150 1.160e-06 1.216e-07
Thermal bremsstrahlung (OTTB)
XSPEC12>exit
XSPEC: quit
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 129.903 (-41.612 71.0491)
Norm : 1.55874 (-0.160222 0.215874)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.588e-07 3.069e-08
25- 50 4.693e-07 6.314e-08
50-150 8.698e-07 3.444e-07
15-150 1.598e-06 3.846e-07
Double BB
XSPEC12>exit
XSPEC: quit
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.11676 (-1.3187 1.41693)
R1^2/D10^2 : 0.493755 (-0.235677 0.303223)
kT2 [keV] : 37.4036 (-12.1286 38.6667)
R2^2/D10^2 : 1.26960E-03 (-0.00105084 0.00326064)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.769e-07 6.922e-08
25- 50 4.725e-07 1.005e-07
50-150 9.670e-07 4.844e-07
15-150 1.716e-06 5.536e-07
Peak spectrum fit
Power-law model
Time interval is from 0.000 sec. to 64.000 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.76125 ( -0.154408 0.157885 )
Norm@50keV : 2.79035E-03 ( -0.000251534 0.000247939 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 76.89 using 59 PHA bins.
# Reduced chi-squared = 1.349 for 57 degrees of freedom
# Null hypothesis probability = 4.068838e-02
Photon flux (15-150 keV) in 64 sec: 0.378878 ( -0.0318986 0.0319988 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.64683e-06 ( -1.52543e-07 1.53834e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.000 sec. to 64.000 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.14379 ( -0.571914 0.0683794 )
Epeak [keV] : 58.1462 ( )
Norm@50keV : 1.75181E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 75.70 using 59 PHA bins.
# Reduced chi-squared = 1.352 for 56 degrees of freedom
# Null hypothesis probability = 4.085295e-02
Photon flux (15-150 keV) in 64 sec: 0.379706 ( -0.032846 0.031262 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.64849e-06 ( -1.54138e-07 1.46035e-07 ) ergs/cm2
Band function
Time interval is from 0.000 sec. to 64.000 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.42917 ( 1.42917 1.42917 )
beta : -1.76123 ( 1.76123 0.154407 )
Epeak [keV] : 18.5388 ( -18.5388 -18.5388 )
Norm@50keV : 6.47271E-03 ( -0.00391616 378.255 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 76.89 using 59 PHA bins.
# Reduced chi-squared = 1.398 for 55 degrees of freedom
# Null hypothesis probability = 2.726222e-02
Photon flux (15-150 keV) in 64 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] : 11.7947 ( )
R^2/D10^2 : 9.30374E-02 ( )
(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 1.749e-07 2.755e-08
25- 50 5.393e-07 6.016e-08
50-150 4.459e-07 8.496e-08
15-150 1.160e-06 1.174e-07
Thermal bremsstrahlung (OTTB)
XSPEC12>exit
XSPEC: quit
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 129.903 (-41.612 71.0491)
Norm : 1.55874 (-0.160222 0.215874)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.588e-07 3.226e-08
25- 50 4.693e-07 6.086e-08
50-150 8.698e-07 3.479e-07
15-150 1.598e-06 4.227e-07
Double BB
XSPEC12>exit
XSPEC: quit
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.11676 (-1.3187 1.41693)
R1^2/D10^2 : 0.493755 (-0.235677 0.303223)
kT2 [keV] : 37.4036 (-12.1286 38.6667)
R2^2/D10^2 : 1.26960E-03 (-0.00105084 0.00326064)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.769e-07 6.339e-08
25- 50 4.725e-07 1.034e-07
50-150 9.670e-07 4.770e-07
15-150 1.716e-06 5.635e-07
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: 1.76125 ( -0.154408 0.157885 )
Norm@50keV : 2.79035E-03 ( -0.000251534 0.000247939 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 76.89 using 59 PHA bins.
# Reduced chi-squared = 1.349 for 57 degrees of freedom
# Null hypothesis probability = 4.068838e-02
Photon flux (15-150 keV) in 64 sec: 0.378878 ( -0.0318986 0.0319988 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.64683e-06 ( -1.52543e-07 1.53834e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.14927 ( -0.577401 0.0693636 )
Epeak [keV] : 60.1980 ( )
Norm@50keV : 1.74116E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 75.70 using 59 PHA bins.
# Reduced chi-squared = 1.352 for 56 degrees of freedom
# Null hypothesis probability = 4.085473e-02
Photon flux (15-150 keV) in 64 sec: 0.379706 ( -0.032846 0.031262 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.64849e-06 ( -1.54138e-07 1.46035e-07 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.42917 ( 1.42917 1.42917 )
beta : -1.76123 ( 1.76123 0.154407 )
Epeak [keV] : 18.5388 ( -18.5388 -18.5388 )
Norm@50keV : 6.47271E-03 ( -0.00391616 670.556 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 76.89 using 59 PHA bins.
# Reduced chi-squared = 1.398 for 55 degrees of freedom
# Null hypothesis probability = 2.726222e-02
Photon flux (15-150 keV) in 64 sec: ( ) 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) = 4.57e-07
S(50-100 keV) = 5.39e-07
T90 vs. Hardness ratio plot
T90 = 64 sec.
Hardness ratio (energy fluence ratio) = 1.17943
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.23681
Count Ratio (50-100 keV) / (15-25 keV) = 0.779644
Mask shadow pattern
IMX = 8.143423724256850E-01, IMY = 2.410459874545546E-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:
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
0.000000 64.000000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
299.6611 35.3004 4.1 40.8 -16.1 0.5294 2.8 6.9 Cyg X-1
308.3051 40.9773 6.3 32.1 -13.0 0.2771 1.8 9.0 Cyg X-3
325.9826 38.1891 0.0 21.1 -32.4 -0.1990 -1.6 11.9 Cyg X-2
26.3701 68.8021 2.9 28.4 94.6 0.7492 4.0 ------ UNKNOWN
282.0631 35.0746 2.7 53.0 -5.5 1.2364 4.2 ------ UNKNOWN
300.3037 35.3115 0.7 40.3 -16.5 2.8208 16.0 ------ UNKNOWN
39.7413 3.8837 2.3 58.6 -169.2 3.4738 5.1 ------ UNKNOWN
31.8309 2.7670 2.5 55.1 -160.7 2.0188 4.6 ------ UNKNOWN
296.8414 18.7373 2.6 53.1 -31.8 2.2624 4.5 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
167.700620 243.122500
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.3923 35.4963 5.2 37.1 62.5 0.7352 2.2 9.8 Her X-1
268.3236 -1.4391 10.6 47.3 4.4 0.3004 1.1 2.8 SW J1753.5-0127
274.0199 -14.0188 6.9 55.2 -10.1 0.7206 1.6 1.3 GX 17+2
288.8014 10.9378 5.8 26.5 -15.6 0.2988 2.0 0.5 GRS 1915+105
299.3420 35.1973 25.8 0.8 42.0 -0.0666 -0.5 12.2 Cyg X-1
308.0557 40.9264 104.1 8.3 -176.7 -0.0148 -0.1 2.9 Cyg X-3
326.3870 38.3261 12.5 21.0 -147.7 0.1311 0.9 10.1 Cyg X-2
15.9243 38.6982 2.2 58.7 -159.4 4.6841 5.2 ------ UNKNOWN
Plot creation:
Wed Feb 28 00:28:24 EST 2024