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
37.8430 59.0467 0.0160 8.9224 -99.6067 1.1422355 11.992 TRIG_01245636
Foreground time interval of the image:
-6.696 53.260 (delta_t = 59.956 [sec])
Background time interval of the image:
-209.499 -6.696 (delta_t = 202.803 [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 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)
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 -6.696 sec. to 53.260 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.49142 ( -0.192386 0.194856 )
Norm@50keV : 1.20809E-03 ( -0.000144777 0.000143681 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 55.71 using 59 bins.
Reduced chi-squared = 0.977368
# Null hypothesis probability of 5.23e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 59.96 sec: 0.150475 ( -0.017406 0.017421 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.88227e-07 ( -9.02122e-08 9.14264e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -6.696 sec. to 53.260 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.644144 ( -0.980129 0.795744 )
Epeak [keV] : 77.5468 ( -20.3857 300.083 )
Norm@50keV : 3.32000E-03 ( -0.00200467 0.00703117 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 52.37 using 59 bins.
Reduced chi-squared = 0.935179
# Null hypothesis probability of 6.13e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 59.96 sec: 0.145603 ( -0.018091 0.018049 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.43904e-07 ( -9.72012e-08 1.00008e-07 ) ergs/cm2
Band function
Time interval is from -6.696 sec. to 53.260 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] : 14.7022 (-1.88991 2.21464)
R^2/D10^2 : 1.87847E-02 (-0.00734269 0.0117287)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 62.13 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.98e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.113e-08 1.062e-08
25- 50 1.994e-07 2.812e-08
50-150 2.907e-07 7.219e-08
15-150 5.412e-07 9.300e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.363 (-78.0457 -199.363)
Norm : 0.618547 (-0.0704628 0.0705274)
------------------------------------------------------------
#Fit statistic : Chi-Squared 53.98 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.89e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.235e-08 5.136e-08
25- 50 1.777e-07 9.869e-08
50-150 3.896e-07 2.133e-07
15-150 6.596e-07 3.580e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.35246 (-2.46141 4.79124)
R1^2/D10^2 : 0.298451 (-0.254605 1.13837)
kT2 [keV] : 19.1681 (-3.90368 9.56134)
R2^2/D10^2 : 6.38554E-03 (-0.00561653 0.00893117)
------------------------------------------------------------
#Fit statistic : Chi-Squared 52.21 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.82e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.428e-08 4.573e-08
25- 50 1.770e-07 8.334e-08
50-150 3.632e-07 1.989e-07
15-150 6.246e-07 2.879e-07
Peak spectrum fit
Power-law model
Time interval is from 5.800 sec. to 6.800 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.86095 ( -0.61334 0.761324 )
Norm@50keV : 2.72566E-03 ( -0.00126984 0.00116489 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 66.40 using 59 bins.
Reduced chi-squared = 1.16491
# Null hypothesis probability of 1.85e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.384859 ( -0.133575 0.133593 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.50634e-08 ( -1.0682e-08 1.14666e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 5.800 sec. to 6.800 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.45348 ( -2.93118 1.2529 )
Epeak [keV] : 59.8252 ( -59.3191 -59.9106 )
Norm@50keV : 4.61200E-03 ( -0.00460228 0.22619 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 66.29 using 59 bins.
Reduced chi-squared = 1.18375
# Null hypothesis probability of 1.63e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.381262 ( -0.134072 0.134698 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.43187e-08 ( -1.07108e-08 1.25689e-08 ) ergs/cm2
Band function
Time interval is from 5.800 sec. to 6.800 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] : 11.5383 (-5.34155 8.18125)
R^2/D10^2 : 0.106668 (-0.103411 0.9206)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 69.08 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.31e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.991e-09 1.858e-09
25- 50 8.980e-09 5.800e-09
50-150 6.996e-09 5.065e-09
15-150 1.897e-08 1.281e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 89.1523 (-89.1523 -89.1523)
Norm : 1.76478 (-0.69509 1.32373)
------------------------------------------------------------
#Fit statistic : Chi-Squared 66.31 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.87e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.603e-09 2.855e-09
25- 50 7.770e-09 4.733e-09
50-150 1.176e-08 9.900e-09
15-150 2.414e-08 1.768e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 4.29803 (-3.82609 6.57522)
R1^2/D10^2 : 3.07647 (-2.98983 -3.07647)
kT2 [keV] : 18.5875 (-18.5869 56.9162)
R2^2/D10^2 : 1.55833E-02 (-0.015445 0.16271)
------------------------------------------------------------
#Fit statistic : Chi-Squared 65.73 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.52e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.988e-09 3.044e-09
25- 50 6.780e-09 3.714e-09
50-150 1.279e-08 9.365e-09
15-150 2.456e-08 1.365e-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: 1.49142 ( -0.192386 0.194856 )
Norm@50keV : 1.20809E-03 ( -0.000144777 0.000143681 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 55.71 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.23e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 59.96 sec: 0.150471 ( -0.0174051 0.01742 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.88143e-07 ( -9.01876e-08 9.14444e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.644143 ( -0.980129 0.795744 )
Epeak [keV] : 77.5468 ( -20.3857 300.083 )
Norm@50keV : 3.32001E-03 ( -0.00200467 0.00703117 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 52.37 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.13e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 59.96 sec: 0.145589 ( -0.018087 0.018045 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.4415e-07 ( -9.71814e-08 1.00091e-07 ) 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) = 1.70e-07
S(50-100 keV) = 2.41e-07
T90 vs. Hardness ratio plot
T90 = 50.1159999370575 sec.
Hardness ratio (energy fluence ratio) = 1.41765
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.37628
Count Ratio (50-100 keV) / (15-25 keV) = 1.04896
Mask shadow pattern
IMX = -2.620016867665400E-02, IMY = 1.547951701735723E-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:
-209.499400 -6.696000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
326.1163 38.4262 4.4 41.7 120.9 -4.0659 -2.6 6.8 Cyg X-2
12.1897 18.3550 2.7 37.0 47.6 2.5405 4.3 ------ UNKNOWN
37.2527 14.5815 2.8 41.0 9.0 1.8758 4.2 ------ UNKNOWN
213.5395 77.1245 2.3 48.5 -154.2 3.1264 5.0 ------ UNKNOWN
105.6884 60.1345 2.7 41.7 -103.7 5.3262 4.2 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-6.696000 53.260000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
326.0261 38.3854 7.8 41.8 120.9 -0.4985 -1.5 7.8 Cyg X-2
316.5715 41.1919 2.4 45.4 130.9 1.9818 4.8 ------ UNKNOWN
37.8430 59.0467 1.0 8.9 -99.6 1.1422 12.0 ------ UNKNOWN
60.0404 8.8620 2.1 53.6 -17.4 1.5918 5.5 ------ UNKNOWN
63.5498 5.1777 2.4 58.5 -19.3 3.0410 4.9 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
111.700600 963.088600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
356.4789 40.6631 2.4 31.6 84.7 10.1592 4.7 ------ UNKNOWN
0.0413 37.8611 3.4 32.1 77.3 7.3294 3.4 ------ UNKNOWN
339.0380 58.8594 2.1 29.3 127.2 9.0144 5.4 ------ UNKNOWN
39.7223 18.1418 2.9 40.9 9.0 6.2670 4.1 ------ UNKNOWN
142.6493 60.0692 3.3 47.3 -127.3 17.6262 3.6 ------ UNKNOWN
Plot creation:
Sat Oct 19 18:21:45 EDT 2024