Special notes of this burst
Image
Pre-slew 15.0-350.0 keV image (Event data)
# RAcent DECcent POSerr Theta Phi Peak Cts SNR Name
335.3405 51.5573 0.0052 48.1586 -151.9850 16.4036322 37.075 TRIG_01231488
Foreground time interval of the image:
-37.219 16.381 (delta_t = 53.600 [sec])
Background time interval of the image:
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 -70.916 sec. to 227.452 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.60396 ( -0.0439333 0.0440338 )
Norm@50keV : 7.38710E-03 ( -0.000164388 0.000164387 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 61.25 using 59 bins.
Reduced chi-squared = 1.07456
# Null hypothesis probability of 3.26e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 298.4 sec: 0.950477 ( -0.024867 0.024981 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.06081e-05 ( -4.70478e-07 4.70326e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -70.916 sec. to 227.452 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.60168 ( -0.139923 0.0443068 )
Epeak [keV] : 9998.06 ( -9998.47 -9998.47 )
Norm@50keV : 7.40469E-03 ( -0.000164768 0.001102 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 61.26 using 59 bins.
Reduced chi-squared = 1.09393
# Null hypothesis probability of 2.93e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 298.4 sec: 0.953303 ( -0.038457 0.030165 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.06518e-05 ( -6.6525e-07 3.97024e-07 ) ergs/cm2
Band function
Time interval is from -70.916 sec. to 227.452 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] : 16.5199 ( )
R^2/D10^2 : 7.06463E-02 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 540.52 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.14e-80 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.181e-06 5.550e-08
25- 50 5.103e-06 1.671e-07
50-150 9.849e-06 3.596e-07
15-150 1.613e-05 3.969e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-18.454 -200)
Norm : 3.78884 (-0.0844122 0.0844123)
------------------------------------------------------------
#Fit statistic : Chi-Squared 73.61 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.85e-02 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.816e-06 7.281e-08
25- 50 5.417e-06 1.343e-07
50-150 1.188e-05 3.118e-07
15-150 2.012e-05 5.431e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.61695 (-0.64989 0.693537)
R1^2/D10^2 : 0.767923 (-0.198451 0.290561)
kT2 [keV] : 29.8377 (-2.69531 3.50558)
R2^2/D10^2 : 7.03015E-03 (-0.00224213 0.0028529)
------------------------------------------------------------
#Fit statistic : Chi-Squared 84.61 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.31e-03 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.605e-06 2.077e-07
25- 50 5.514e-06 2.298e-07
50-150 1.220e-05 7.385e-07
15-150 2.032e-05 8.475e-07
Peak spectrum fit
Power-law model
Time interval is from 0.168 sec. to 1.168 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.42166 ( -0.128547 0.128931 )
Norm@50keV : 6.31156E-02 ( -0.00494287 0.00493576 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 58.18 using 59 bins.
Reduced chi-squared = 1.0207
# Null hypothesis probability of 4.32e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 7.72510 ( -0.62524 0.62614 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.07309e-07 ( -5.11871e-08 5.13945e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.168 sec. to 1.168 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.10546 ( -0.534364 0.379958 )
Epeak [keV] : 150.699 ( -64.5153 -150.7 )
Norm@50keV : 8.99989E-02 ( -0.0301849 0.0710592 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 56.92 using 59 bins.
Reduced chi-squared = 1.01643
# Null hypothesis probability of 4.41e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 7.65274 ( -0.63516 0.63564 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.99639e-07 ( -5.35292e-08 5.31007e-08 ) ergs/cm2
Band function
Time interval is from 0.168 sec. to 1.168 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] : 16.4408 (-1.63435 1.84062)
R^2/D10^2 : 0.659313 (-0.203669 0.289626)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 95.58 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.04e-03 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.661e-08 5.310e-09
25- 50 1.576e-07 1.695e-08
50-150 3.008e-07 4.560e-08
15-150 4.951e-07 4.750e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-30.8008 -200)
Norm : 32.1507 (-2.50861 2.50861)
------------------------------------------------------------
#Fit statistic : Chi-Squared 60.34 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.56e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.008e-08 7.800e-09
25- 50 1.540e-07 2.270e-08
50-150 3.378e-07 1.234e-07
15-150 5.719e-07 9.260e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 8.15788 (-2.02742 2.38746)
R1^2/D10^2 : 4.78660 (-2.57167 7.05535)
kT2 [keV] : 31.3443 (-7.70901 20.0223)
R2^2/D10^2 : 5.49466E-02 (-0.043444 0.0579648)
------------------------------------------------------------
#Fit statistic : Chi-Squared 56.36 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.24e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.664e-08 2.317e-08
25- 50 1.573e-07 4.085e-08
50-150 3.811e-07 1.812e-07
15-150 6.051e-07 2.171e-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: 1.42955 ( -0.0499788 0.0499026 )
Norm@50keV : 2.19831E-02 ( -0.000592903 0.000592631 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 60.02 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.67e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 53.6 sec: 2.69564 ( -0.0822291 0.0826486 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.13189e-05 ( -3.13526e-07 3.13721e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.42779 ( -0.270677 0.0486277 )
Epeak [keV] : 9342.79 ( -9079.3 -9079.3 )
Norm@50keV : 2.20673E-02 ( -0.000597487 0.00674286 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 59.99 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.33e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 53.6 sec: 2.68337 ( -0.08949 0.045 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.12911e-05 ( -3.30819e-07 3.29426e-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) = 5.34e-06
S(50-100 keV) = 7.04e-06
T90 vs. Hardness ratio plot
T90 = 158.971999883652 sec.
Hardness ratio (energy fluence ratio) = 1.31835
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.30406
Count Ratio (50-100 keV) / (15-25 keV) = 1.00512
Mask shadow pattern
IMX = -9.859501710022455E-01, IMY = 5.245699676983058E-01
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:
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-37.219410 16.380600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
288.8613 11.1571 0.0 42.5 127.2 0.3992 0.8 13.2 GRS 1915+105
299.6300 35.1838 3.1 43.0 165.8 1.3180 3.8 2.2 Cyg X-1
308.2321 41.0091 6.4 42.7 178.9 0.5603 1.8 6.5 Cyg X-3
326.1144 38.2094 45.1 35.0 -162.4 -0.0518 -0.3 7.3 Cyg X-2
346.8636 -47.3994 3.1 52.8 11.1 1.7508 3.8 ------ UNKNOWN
0.8108 -35.6424 2.5 48.0 -8.3 1.2137 4.6 ------ UNKNOWN
13.6209 -33.2493 4.6 54.4 -19.5 1.0496 2.5 ------ UNKNOWN
344.2351 36.1665 2.4 34.8 -136.8 1.2162 4.8 ------ UNKNOWN
335.3405 51.5573 0.3 48.2 -152.0 16.4024 37.1 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
107.180670 962.780600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
299.5610 35.2195 1.1 30.3 86.4 14.2034 10.3 1.8 Cyg X-1
308.2004 40.9485 17.5 21.4 85.9 -0.6062 -0.7 4.1 Cyg X-3
325.9234 38.4061 0.0 14.7 45.3 1.1638 1.8 12.7 Cyg X-2
304.4402 43.0770 2.9 22.4 94.9 3.7764 4.0 ------ UNKNOWN
335.1454 29.4769 2.1 22.1 15.4 3.7741 5.5 ------ UNKNOWN
286.7340 74.9237 2.5 30.3 172.2 3.7026 4.6 ------ UNKNOWN
324.9970 64.6742 2.6 14.2 176.6 2.9484 4.5 ------ UNKNOWN
335.5604 51.5770 2.3 0.1 -84.5 3.6057 4.9 ------ UNKNOWN
286.6107 88.4444 2.1 37.4 -167.0 4.7705 5.4 ------ UNKNOWN
2.8309 73.5890 2.7 24.9 -147.0 3.0187 4.2 ------ UNKNOWN
142.3827 70.9059 2.2 57.2 -160.1 16.7461 5.3 ------ UNKNOWN
60.9783 61.3360 2.3 44.8 -122.3 15.3820 5.0 ------ UNKNOWN
28.8494 33.5595 2.2 42.2 -71.3 14.3838 5.1 ------ UNKNOWN
Plot creation:
Sat Nov 16 12:25:31 EST 2024