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
154.1819 -21.4096 0.0121 12.4010 -123.1216 1.6085380 15.872 TRIG_00430094
Foreground time interval of the image:
-74.608 10.893 (delta_t = 85.501 [sec])
Background time interval of the image:
-239.808 -74.608 (delta_t = 165.200 [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)
The mask-weighted light curves based on cleaned DPHs
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 -74.608 sec. to 29.840 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.80865 ( -0.125385 0.128332 )
Norm@50keV : 1.25243E-03 ( -9.66337e-05 9.53768e-05 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 82.01 using 59 PHA bins.
# Reduced chi-squared = 1.439 for 57 degrees of freedom
# Null hypothesis probability = 1.667272e-02
Photon flux (15-150 keV) in 104.4 sec: 0.173165 ( -0.0115276 0.0115352 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.20339e-06 ( -9.41014e-08 9.53683e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -74.608 sec. to 29.840 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.47153 ( -0.547272 0.423193 )
Epeak [keV] : 69.5253 ( -21.0777 -69.5255 )
Norm@50keV : 1.92046E-03 ( -0.000734201 0.00188436 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 80.63 using 59 PHA bins.
# Reduced chi-squared = 1.440 for 56 degrees of freedom
# Null hypothesis probability = 1.725037e-02
Photon flux (15-150 keV) in 104.4 sec: 0.170062 ( -0.01235 0.012324 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.15898e-06 ( -1.12533e-07 1.14339e-07 ) ergs/cm2
Band function
Time interval is from -74.608 sec. to 29.840 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.34668 ( 1.35175 1.35175 )
beta : -2.07499 ( 2.07253 0.348866 )
Epeak [keV] : 58.5866 ( -58.6279 -58.6279 )
Norm@50keV : 2.29895E-03 ( -0.0010884 0 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 80.49 using 59 PHA bins.
# Reduced chi-squared = 1.463 for 55 degrees of freedom
# Null hypothesis probability = 1.414290e-02
Photon flux (15-150 keV) in 104.4 sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 1.16248e-06 ( 0 0 ) ergs/cm2
Single BB
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 11.3792 ( )
R^2/D10^2 : 4.90831E-02 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 127.03 using 59 PHA bins.
# Reduced chi-squared = 2.2286 for 57 degrees of freedom
# Null hypothesis probability = 2.982185e-07
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.395e-07 1.712e-08
25- 50 4.116e-07 3.028e-08
50-150 3.088e-07 5.215e-08
15-150 8.599e-07 6.478e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 97.3212 (-22.4369 35.2081)
Norm : 0.764615 (-0.0381138 0.0832601)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 80.92 using 59 PHA bins.
# Reduced chi-squared = 1.420 for 57 degrees of freedom
# Null hypothesis probability = 2.032778e-02
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.086e-07 2.312e-08
25- 50 3.587e-07 2.840e-08
50-150 5.724e-07 1.929e-07
15-150 1.140e-06 2.194e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.82198 (-1.32737 1.54936)
R1^2/D10^2 : 0.391844 (-0.213915 0.644686)
kT2 [keV] : 20.1508 (-4.01916 7.56801)
R2^2/D10^2 : 4.50069E-03 (-0.00316023 0.00648266)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 82.12 using 59 PHA bins.
# Reduced chi-squared = 1.493 for 55 degrees of freedom
# Null hypothesis probability = 1.033450e-02
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.129e-07 6.814e-08
25- 50 3.480e-07 9.495e-08
50-150 5.664e-07 2.463e-07
15-150 1.127e-06 3.491e-07
Peak spectrum fit
Power-law model
Time interval is from 1.332 sec. to 2.332 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.71558 ( -0.185776 0.192624 )
Norm@50keV : 8.89560E-03 ( -0.00109248 0.00107293 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 65.17 using 59 PHA bins.
# Reduced chi-squared = 1.143 for 57 degrees of freedom
# Null hypothesis probability = 2.138199e-01
Photon flux (15-150 keV) in 1 sec: 1.18794 ( -0.125126 0.125144 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.22659e-08 ( -1.04852e-08 1.07141e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 1.332 sec. to 2.332 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.08032 ( -0.871224 0.705122 )
Epeak [keV] : 63.0442 ( -17.8588 -63.0442 )
Norm@50keV : 2.02451E-02 ( -0.0117882 0.0426242 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 62.92 using 59 PHA bins.
# Reduced chi-squared = 1.124 for 56 degrees of freedom
# Null hypothesis probability = 2.446049e-01
Photon flux (15-150 keV) in 1 sec: 1.15814 ( -0.12922 0.06509 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.67841e-08 ( -1.18461e-08 1.23209e-08 ) ergs/cm2
Band function
Time interval is from 1.332 sec. to 2.332 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.08038 ( -0.553937 0.776732 )
beta : -10.0000 ( 10 0 )
Epeak [keV] : 63.0337 ( -17.3637 -63.0337 )
Norm@50keV : 2.02420E-02 ( -0.0117873 0.0426334 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 62.92 using 59 PHA bins.
# Reduced chi-squared = 1.144 for 55 degrees of freedom
# Null hypothesis probability = 2.162423e-01
Photon flux (15-150 keV) in 1 sec: 1.16197 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 7.67208e-08 ( 0 0 ) ergs/cm2
Single BB
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 11.2195 (-1.4849 1.78412)
R^2/D10^2 : 0.368329 (-0.153079 0.253113)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 79.44 using 59 PHA bins.
# Reduced chi-squared = 1.394 for 57 degrees of freedom
# Null hypothesis probability = 2.640313e-02
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.723e-09 1.844e-09
25- 50 2.819e-08 4.215e-09
50-150 2.035e-08 5.705e-09
15-150 5.826e-08 8.840e-09
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 115.431 (-40.5944 83.1254)
Norm : 5.09553 (-0.644701 0.826157)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 63.10 using 59 PHA bins.
# Reduced chi-squared = 1.107 for 57 degrees of freedom
# Null hypothesis probability = 2.695850e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.329e-08 1.970e-09
25- 50 2.362e-08 4.925e-09
50-150 4.133e-08 1.912e-08
15-150 7.824e-08 2.485e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.37418 (-1.73078 1.98775)
R1^2/D10^2 : 1.85973 (-0.947955 1.41923)
kT2 [keV] : 20.8912 (-6.02351 13.2304)
R2^2/D10^2 : 2.57022E-02 (-0.0166182 0.0485397)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 60.76 using 59 PHA bins.
# Reduced chi-squared = 1.105 for 55 degrees of freedom
# Null hypothesis probability = 2.762372e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.302e-08 7.445e-09
25- 50 2.324e-08 1.247e-08
50-150 3.683e-08 2.178e-08
15-150 7.309e-08 3.860e-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: 1.81609 ( -0.147124 0.151501 )
Norm@50keV : 1.12199E-03 ( -0.000106166 0.000104483 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 78.00 using 59 PHA bins.
# Reduced chi-squared = 1.368 for 57 degrees of freedom
# Null hypothesis probability = 3.380116e-02
Photon flux (15-150 keV) in 85.5 sec: 0.155583 ( -0.0123307 0.0123342 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.82685e-07 ( -8.41269e-08 8.55804e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.40502 ( -0.651114 0.507203 )
Epeak [keV] : 62.5363 ( -17.0806 -62.5363 )
Norm@50keV : 1.91221E-03 ( -0.000859045 0.00250189 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 76.48 using 59 PHA bins.
# Reduced chi-squared = 1.366 for 56 degrees of freedom
# Null hypothesis probability = 3.588360e-02
Photon flux (15-150 keV) in 85.5 sec: 0.152596 ( -0.012974 0.012963 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.42028e-07 ( -9.88089e-08 1.01516e-07 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 4.72890 ( -4.7289 -4.7289 )
beta : -1.90823 ( -0.183248 0.170342 )
Epeak [keV] : 22.2593 ( -5.86729 3.92069 )
Norm@50keV : 202.206 ( -15.9105 993209 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 75.82 using 59 PHA bins.
# Reduced chi-squared = 1.378 for 55 degrees of freedom
# Null hypothesis probability = 3.287420e-02
Photon flux (15-150 keV) in 85.5 sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 8.62233e-07 ( 0 0 ) ergs/cm2
S(25-50 keV) vs. S(50-100 keV) plot
S(25-50 keV) = 3.40e-07
S(50-100 keV) = 3.88e-07
T90 vs. Hardness ratio plot
T90 = 71.8999999165535 sec.
Hardness ratio (energy fluence ratio) = 1.14118
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.15095
Count Ratio (50-100 keV) / (15-25 keV) = 0.656951
Mask shadow pattern
IMX = -1.201474119564260E-01, IMY = 1.841542455666287E-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:
-239.808000 -74.608000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.4102 -40.5238 6.9 29.2 178.2 0.2218 1.7 5.7 Vela X-1
170.3880 -60.6205 12.3 34.1 121.2 0.2179 0.9 2.1 Cen X-3
186.9335 -62.7113 35.7 38.5 109.7 0.1347 0.3 8.4 GX 301-2
193.9563 -1.6048 2.7 36.3 -4.4 0.7163 4.2 ------ UNKNOWN
111.2922 -13.2450 2.5 53.2 -142.3 3.0644 4.6 ------ UNKNOWN
168.2178 20.4419 4.2 47.1 -53.2 1.5660 2.7 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-74.608000 10.892600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.5193 -40.5433 8.6 29.1 178.1 0.1494 1.3 0.8 Vela X-1
170.1760 -60.7013 6.5 34.2 121.4 0.3414 1.8 6.2 Cen X-3
186.5859 -62.8166 4.1 38.5 110.0 0.9457 2.8 3.4 GX 301-2
192.4021 -51.9517 2.6 31.9 94.0 0.8458 4.4 ------ UNKNOWN
154.1819 -21.4096 0.7 12.4 -123.1 1.6082 15.8 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
45.492600 349.644000
351.192000 962.281300
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.2900 -40.5290 6.2 25.0 161.5 -0.9624 -1.8 11.0 Vela X-1
170.4094 -60.7373 5.4 41.0 113.9 3.5109 2.1 7.4 Cen X-3
89.9845 -35.7208 3.7 57.2 -173.7 7.0857 3.1 ------ UNKNOWN
Plot creation:
Sun May 31 00:45:21 EDT 2015