Estimated redshift from machine learning (Ukwatta et al. 2016) - may take a few minute to calcaulte
Image
Pre-slew 15.0-350.0 keV image (Event data)
# RAcent DECcent POSerr Theta Phi Peak Cts SNR Name
327.9049 -56.6530 0.0132 11.7816 -178.0595 1.7457008 14.562 TRIG_01270788
Foreground time interval of the image:
-20.832 9.128 (delta_t = 29.960 [sec])
Background time interval of the image:
-60.848 -20.832 (delta_t = 40.016 [sec])
Lightcurves
Notes:
- 1) The mask-weighted light curves are using the flight position.
- 2) Multiple plots of different time binning/intervals are shown to cover all scenarios of short/long GRBs, rate/image triggers, and real/false positives.
- 3) 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.
- 4) 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.
- 5) 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 1.024000
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 1.024000
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 1.024000
SN=5 or 10 sec. binning (whichever binning is satisfied first)
SN=5 or 10 sec. binning (T < 200 sec)
Quad-rate summed light curves (from T0-300s to T0+1000s)
Spectral Evolution
Spectra
Notes:
- 1) The fitting includes the systematic errors.
- 2) When the burst includes telescope slew time periods, the fitting uses an average response file made from multiple 5-s response files through out the slew time plus single time preiod for the non-slew times, and weighted by the total counts in the corresponding time period using addrmf. An average response file is needed becuase a spectral fit using 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.
Time averaged spectrum fit using the average DRM
Power-law model
Time interval is from -20.832 sec. to 9.128 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.64244 ( -0.203156 0.220313 )
Norm@50keV : 2.37771E-03 ( -0.000390756 0.000396471 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 62.10 using 59 bins.
Reduced chi-squared = 1.08947
# Null hypothesis probability of 2.99e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 29.96 sec: 0.511092 ( -0.043704 0.043715 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.43415e-07 ( -8.18211e-08 8.54456e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -20.832 sec. to 9.128 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.07937 ( -1.30529 0.721866 )
Epeak [keV] : 19.3976 ( -18.2754 6.92696 )
Norm@50keV : 2.52724E-02 ( -0.0252763 0.165643 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 55.07 using 59 bins.
Reduced chi-squared = 0.983393
# Null hypothesis probability of 5.10e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 29.96 sec: 0.487031 ( -0.044612 0.04514 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.49952e-07 ( -7.60316e-08 8.96391e-08 ) ergs/cm2
Band function
Time interval is from -20.832 sec. to 9.128 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : ( )
beta : ( )
Epeak [keV] : ( )
Norm@50keV : ( )
------------------------------------------------------------
Photon flux (15-150 keV) in 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] : 6.82149 (-0.647518 0.698447)
R^2/D10^2 : 1.04796 (-0.350768 0.55163)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 64.88 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.21e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.283e-07 3.409e-08
25- 50 2.972e-07 4.066e-08
50-150 4.482e-08 1.575e-08
15-150 5.704e-07 6.202e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 26.4858 (-4.94139 6.432)
Norm : 4.54603 (-0.84411 1.11047)
------------------------------------------------------------
#Fit statistic : Chi-Squared 55.25 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.41e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.586e-07 2.852e-08
25- 50 2.748e-07 3.183e-08
50-150 1.270e-07 4.650e-08
15-150 6.605e-07 7.595e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 3.19780 (-1.49437 1.71374)
R1^2/D10^2 : 15.7632 (-13.0996 879.159)
kT2 [keV] : 8.83832 (-1.56914 3.03062)
R2^2/D10^2 : 0.281280 (-0.223618 0.447428)
------------------------------------------------------------
#Fit statistic : Chi-Squared 53.93 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.15e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.568e-07 1.324e-07
25- 50 2.857e-07 1.516e-07
50-150 9.466e-08 5.710e-08
15-150 6.372e-07 3.204e-07
Peak spectrum fit
Power-law model
Time interval is from 0.092 sec. to 1.092 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.04404 ( -0.194017 0.206551 )
Norm@50keV : 1.51864E-02 ( -0.00223061 0.00219207 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 51.09 using 59 bins.
Reduced chi-squared = 0.896316
# Null hypothesis probability of 6.95e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 2.32551 ( -0.23848 0.23854 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.40456e-07 ( -1.87309e-08 1.9382e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.092 sec. to 1.092 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.31410 ( -1.19106 0.837091 )
Epeak [keV] : 34.3958 ( -28.9335 -34.3956 )
Norm@50keV : 4.36945E-02 ( -0.0436996 0.220904 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 48.93 using 59 bins.
Reduced chi-squared = 0.87375
# Null hypothesis probability of 7.37e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 2.26476 ( -0.24693 0.24802 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.26561e-07 ( -2.24875e-08 2.47638e-08 ) ergs/cm2
Band function
Time interval is from 0.092 sec. to 1.092 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : ( )
beta : ( )
Epeak [keV] : ( )
Norm@50keV : ( )
------------------------------------------------------------
Photon flux (15-150 keV) in 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] : 8.05380 (-0.901977 1.0456)
R^2/D10^2 : 2.49564 (-0.946005 1.48412)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 59.10 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.99e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.942e-08 5.005e-09
25- 50 5.209e-08 7.200e-09
50-150 1.398e-08 4.812e-09
15-150 9.548e-08 1.285e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 54.7080 (-15.4441 23.4471)
Norm : 12.7606 (-1.29777 1.29777)
------------------------------------------------------------
#Fit statistic : Chi-Squared 48.84 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.70e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.154e-08 4.705e-09
25- 50 4.661e-08 1.364e-08
50-150 4.900e-08 2.828e-08
15-150 1.271e-07 4.666e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.32040 (-1.09358 1.18453)
R1^2/D10^2 : 5.34026 (-2.4037 3.69)
kT2 [keV] : 24.7255 (-9.02167 25.932)
R2^2/D10^2 : 1.99052E-02 (-0.0180149 0.0941651)
------------------------------------------------------------
#Fit statistic : Chi-Squared 43.36 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.72e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.256e-08 9.645e-09
25- 50 4.591e-08 1.541e-08
50-150 5.828e-08 3.336e-08
15-150 1.368e-07 5.157e-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: 2.64244 ( -0.203156 0.220313 )
Norm@50keV : 2.37771E-03 ( -0.000390756 0.000396471 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 62.10 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.99e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 29.96 sec: 0.511008 ( -0.0436982 0.0437092 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.43215e-07 ( -8.17941e-08 8.54984e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.07933 ( -1.30527 0.724954 )
Epeak [keV] : 19.3979 ( -18.2174 6.92683 )
Norm@50keV : 2.52738E-02 ( -0.025277 0.165643 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 55.07 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.10e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 29.96 sec: 0.486877 ( -0.044579 0.045107 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.5e-07 ( -7.60235e-08 8.95864e-08 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : ( )
beta : ( )
Epeak [keV] : ( )
Norm@50keV : ( )
------------------------------------------------------------
Photon flux (15-150 keV) in 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) = 2.49e-07
S(50-100 keV) = 1.60e-07
T90 vs. Hardness ratio plot
T90 = 25.9879999160767 sec.
Hardness ratio (energy fluence ratio) = 0.64257
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 0.817144
Count Ratio (50-100 keV) / (15-25 keV) = 0.121661
Mask shadow pattern
IMX = -2.084561767038293E-01, IMY = 7.062541447758889E-03
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.024000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.024000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.024000
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:
-60.848000 -20.832000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
275.9963 -30.5009 38.3 40.8 -77.5 0.2331 0.3 8.8 H1820-303
284.9004 -24.8379 52.6 38.2 -62.8 -0.0866 -0.2 8.9 HT1900.1-2455
345.8896 -14.8719 2.5 34.8 45.8 1.5057 4.7 ------ UNKNOWN
330.2406 -18.4470 2.8 26.9 19.6 0.8980 4.1 ------ UNKNOWN
96.9967 -78.9781 2.1 52.9 178.8 3.5419 5.5 ------ UNKNOWN
297.6690 3.8331 2.2 54.7 -25.4 3.4731 5.2 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-20.832000 9.128000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
275.8403 -30.2839 158.2 41.1 -77.4 0.0412 0.1 6.6 H1820-303
285.0418 -24.9205 278.0 38.0 -62.8 -0.0120 -0.0 0.3 HT1900.1-2455
327.9049 -56.6530 0.8 11.8 -178.1 1.7452 14.6 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
54.852600 639.352590
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
186.6516 -62.8026 7.2 56.8 -152.8 8.6373 1.6 1.9 GX 301-2
264.8612 -44.3726 4.6 40.3 -92.9 -9.5328 -2.5 6.9 4U 1735-44
284.8764 -25.0123 5.8 44.2 -55.4 -7.2473 -2.0 10.3 HT1900.1-2455
339.5995 -13.5962 2.6 44.0 23.6 6.2636 4.4 ------ UNKNOWN
306.9126 -0.7944 2.5 58.4 -17.7 13.0109 4.7 ------ UNKNOWN
280.9980 -27.0789 2.6 44.4 -61.2 18.7804 4.4 ------ UNKNOWN
Plot creation:
Wed Dec 18 17:40:12 EST 2024