batgrbproduct analysis for trigger=761119

batgrbproduct Analysis for Trigger=761119

Analysis Summary

Notes:

1) No attempt has been made to eliminate the non-significant decimal places.
2) This batgrbproduct analysis is done using the HEASARC data.
3) This batgrbproduct analysis is using the flight position for the mask-weighting calculation.

======================================================================
                  BAT GRB EVENT DATA PROCESSING REPORT
    Process Script Ver: batgrbproduct v2.46
    Process Start Time (local time): Wed Aug  2 14:57:46 EDT 2017
             Host Name: bat1
   Current Working Dir: /local/data/bat1/alien/Swift_3rdBATcatalog/event/batevent_reproc/trigger761119
======================================================================

  Trigger: 00761119      Segment: 000

  BAT Trigger Time: 521340363.968   [s; MET]
      Trigger Stop: 521340368.064   [s; MET]
               UTC: 2017-07-10T00:45:44.623200    [includes UTCF correction] 
       Where From?: TDRSS position message

  BAT 
    RA: 231.81245248794   Dec: -38.5470762478186  [deg; J2000]

     Catalogged Source?: NO
     Point Source?:      YES
     GRB Indicated?:     YES    [ by BAT flight software ]
     Image S/N Ratio:    6.88
     Image Trigger?:     NO
     Rate S/N Ratio:     7.87400787401181  [ if not an image trigger ]
     Image S/N Ratio:    6.88

  Flight Position:   [ source = BAT ]
    RA: 231.81245248794   Dec: -38.5470762478186  [deg; J2000]

  Ground Position:   [ source = BAT pre-slew burst ]
    RA: 231.849844108435   Dec: -38.5227185855827  [deg; J2000]  
        { 15h 27m 24.0s , -38d 31' 21.8" }
         +/- 2.51906033302231 [arcmin] (estimated 90% radius based on SNR)
         +/- 1.31900280964353 [arcmin] (formal 1-sigma fit error)
    SNR: 8.12681594328101
 
  Angular difference between Flight and Ground position is 2.283777 arcmin
 
  Partial Coding Fraction: 0.2285156    [ including projection effects ]

  Duration
     T90: 33.1200000047684 +/- 10.8611601354231
        Measured from: 0.568000018596649
                   to: 33.688000023365     [s; relative to TRIGTIME]
     T50: 15.9679999947548 +/- 7.83892645512002
        Measured from: 3.19200003147125
                   to: 19.160000026226     [s; relative to TRIGTIME]



  Fluence
     Peak Flux  (peak 1 second)
        Measured from: 0.491999983787537     
                   to: 1.49199998378754     [s; relative to TRIGTIME]
     Total Fluence        
        Measured from: 0.167999982833862     
                   to: 36.7919999957085     [s; relative to TRIGTIME]
     
             Band 1     Band 2     Band 3     Band 4
              15-25      25-50     50-100    100-350     keV
 Total     0.419266   0.497776   0.326038   0.055708
           0.085266   0.084466   0.074213   0.067624 [error]
 Peak      0.016995   0.029650   0.047331   0.034167
           0.014286   0.013706   0.013653   0.011141 [error]

     [ fluence units of on-axis counts / fully illuminated detector ] 

======================================================================
 
=== Fluence/Peak Flux Summary ===
 
              Model    Band1    Band2    Band3    Band4    Band5    Total      
                       15-25    25-50   50-100  100-350   15-150   15-350   keV
Fluence   Power-law 1.54e-07 2.23e-07 2.40e-07 4.80e-07 7.65e-07 1.10e-06   erg/cm2
              Error 4.22e-08 4.09e-08 7.43e-08 3.07e-07 1.70e-07 3.82e-07   erg/cm2
Peak flux Power-law 1.95e-01 2.82e-01 3.03e-01 6.08e-01 9.68e-01 1.39e+00   ph/cm2/s
              Error 1.51e-01 1.32e-01 9.72e-02 4.70e-01 3.35e-01 4.79e-01   ph/cm2/s
 
Fluence   Cutoff-PL 1.55e-07 2.20e-07 2.40e-07 5.27e-07 7.69e-07 1.09e-06   erg/cm2
              Error 4.43e-08 4.76e-08 8.12e-08 2.80e-07 1.53e-07 3.50e-07   erg/cm2
Peak flux Cutoff-PL 2.10e-01 2.82e-01 3.02e-01 6.35e-01 9.73e-01 1.41e+00   ph/cm2/s
              Error -------- 1.37e-01 1.13e-01 -------- 3.41e-01 5.80e-01   ph/cm2/s
 
Fluence        Band -------- -------- -------- -------- -------- --------   erg/cm2
              Error -------- -------- -------- -------- -------- --------   erg/cm2
Peak flux      Band -------- -------- -------- -------- -------- --------   ph/cm2/s
              Error -------- -------- -------- -------- -------- --------   ph/cm2/s

 
=== Time-averaged spectral analysis ===
 
Model Ph_index Ph_90err Epeak  Epeak_90err Norm     Nomr_90err chi2   dof
PL    1.892    0.359    -      -           2.27e-03 5.11e-04   48.730 57
CPL   1.892    0.000    9999.2    0.0      2.27e-03 0.00e+00   48.730 56
 
 
=== 1-s peak spectral analysis ===
 
Model Ph_index Ph_90err Epeak  Epeak_90err Norm     Nomr_90err chi2   dof
PL    0.894    0.644    -      -           8.43e-03 2.97e-03   43.260 57
CPL   0.896    0.650    9999.4    0.0      8.50e-03 3.46e-02   43.260 56
 
Model      : spectral model: simple power-law (PL) and cutoff power-law (CPL)
Ph_index   : photon index: E^-{Ph_index} (minus sign is not included in the index)
Ph_90err   : 90% error of the photon index
Epeak      : Epeak in keV
Epeak_90err: 90% error of Epeak
Norm       : normalization at 50 keV in PL model and at 1 keV in CPL model
Nomr_90err : 90% error of the normalization
chi2       : Chi-Squared
dof        : degree of freedom

 
=== T90/T50 calculation in the 50-300 keV band (BATSE band) using 64 ms lc ===
 
T90 in the 50-300 keV band: 3.328000 sec.
T50 in the 50-300 keV band: 1.920000 sec.

 
=== Table of the duration information ==
 
        Value   tstart    tstop
T100   36.624    0.168   36.792
T90    33.120    0.568   33.688
T50    15.968    3.192   19.160
Peak    1.000    0.492    1.492

Click here for the BAT GCN circular template

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
  231.8498   -38.5227   0.0235    35.3359   125.6589         1.2712620      8.127 TRIG_00761119                 
 
Foreground time interval of the image:
  0.168  36.792 (delta_t =  36.624 [sec])
Background time interval of the image:
-606.567 -589.275 (delta_t =  17.292 [sec])
-239.968   0.168 (delta_t = 240.136 [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

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)

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    0.168 sec. to   36.792 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.89223     ( -0.344352   0.374249 )
Norm@50keV  : 2.27124E-03    ( -0.000522515   0.000498601 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          48.73 using 59 PHA bins.
# Reduced chi-squared =         0.8549 for     57 degrees of freedom 
# Null hypothesis probability =   7.740993e-01
 
Photon flux (15-150 keV)    in 36.62 sec: 0.324897 ( -0.06001  0.060058 ) ph/cm2/s
Energy fluence (15-150 keV)             : 7.64765e-07 ( -1.67443e-07  1.72707e-07 ) ergs/cm2

Cutoff power-law model

Time interval is from    0.168 sec. to   36.792 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.89247     (     )
Epeak [keV] : 9999.16      (   )
Norm@50keV  : 2.27217E-03    (     )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          48.73 using 59 PHA bins.
# Reduced chi-squared =         0.8702 for     56 degrees of freedom 
# Null hypothesis probability =   7.439363e-01
 
Photon flux (15-150 keV)    in 36.62 sec: 0.325938 ( -0.063032  0.060564 ) ph/cm2/s
Energy fluence (15-150 keV)             : 7.70049e-07 ( -1.78081e-07  1.28824e-07 ) ergs/cm2

Band function

Time interval is from    0.168 sec. to   36.792 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]    : 9.44249  (-2.14442  3.36623)
R^2/D10^2   : 0.182252  (-0.123987   0.312962)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          58.57 using 59 PHA bins.
# Reduced chi-squared =          1.028 for     57 degrees of freedom 
# Null hypothesis probability =   4.175775e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.185e-07   4.819e-08
25- 50  2.711e-07   9.800e-08
50-150  1.196e-07   5.790e-08
15-150  5.092e-07   1.647e-07

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 85.5354       (-40.8452      -85.537)
Norm        : 1.48297       (-0.364294     0.545907)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          49.48 using 59 PHA bins.
# Reduced chi-squared =         0.8681 for     57 degrees of freedom 
# Null hypothesis probability =   7.499895e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.414e-07   3.911e-08
25- 50  2.365e-07   6.255e-08
50-150  3.488e-07   2.246e-07
15-150  7.268e-07   3.250e-07

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 6.29880        (-1.96325      2.24616)
R1^2/D10^2  : 0.686780        (-0.469612      2.27095)
kT2 [keV]   : 28.0027        (-23.5221      75.5465)
R2^2/D10^2  : 2.45666E-03    (-0.00241348   0.0153423)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          47.60 using 59 PHA bins.
# Reduced chi-squared =         0.8654 for     55 degrees of freedom 
# Null hypothesis probability =   7.504250e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.532e-07   8.957e-08
25- 50  2.257e-07   1.196e-07
50-150  4.082e-07   2.377e-07
15-150  7.871e-07   4.119e-07

Peak spectrum fit

Power-law model

Time interval is from    0.492 sec. to    1.492 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 0.893892     ( -0.686477   0.601316 )
Norm@50keV  : 8.43425E-03    ( -0.0030785   0.00285363 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          43.26 using 59 PHA bins.
# Reduced chi-squared =         0.7590 for     57 degrees of freedom 
# Null hypothesis probability =   9.105124e-01
 
Photon flux (15-150 keV)    in 1 sec: 0.968013 ( -0.330753  0.339177 ) ph/cm2/s
Energy fluence (15-150 keV)             : 9.48899e-08 ( -3.07187e-08  3.0852e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from    0.492 sec. to    1.492 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 0.896011     ( -0.700208   0.599183 )
Epeak [keV] : 9999.35      ( -9999.36 -9999.36 )
Norm@50keV  : 8.50147E-03    ( -0.00282104   0.0663482 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          43.26 using 59 PHA bins.
# Reduced chi-squared =         0.7725 for     56 degrees of freedom 
# Null hypothesis probability =   8.934256e-01
 
Photon flux (15-150 keV)    in 1 sec: 0.972524 ( -0.343549  0.338016 ) ph/cm2/s
Energy fluence (15-150 keV)             : 9.49883e-08 ( -3.12926e-08  3.11683e-08 ) ergs/cm2

Band function

Time interval is from    0.492 sec. to    1.492 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]    : 29.7024  (-10.7212  25.4123)
R^2/D10^2   : 1.42638E-02  (-0.0142615   0.0411116)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          44.97 using 59 PHA bins.
# Reduced chi-squared =         0.7889 for     57 degrees of freedom 
# Null hypothesis probability =   8.758100e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.981e-09   1.281e-09
25- 50  1.217e-08   7.675e-09
50-150  7.612e-08   4.775e-08
15-150  9.027e-08   5.530e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 199.363       (-99.7591      -199.363)
Norm        : 4.14250       (-1.38768     1.38768)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          46.94 using 59 PHA bins.
# Reduced chi-squared =         0.8234 for     57 degrees of freedom 
# Null hypothesis probability =   8.266911e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.032e-08   6.520e-09
25- 50  1.984e-08   1.258e-08
50-150  4.352e-08   2.631e-08
15-150  7.368e-08   4.598e-08

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 6.16538        (-6.17664      84.4965)
R1^2/D10^2  : 1.24004        (-1.23489      -1.23489)
kT2 [keV]   : 38.3048        (-38.3297      -38.3297)
R2^2/D10^2  : 6.33631E-03    (-0.0063243   0.0271373)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          42.58 using 59 PHA bins.
# Reduced chi-squared =         0.7742 for     55 degrees of freedom 
# Null hypothesis probability =   8.891561e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  7.743e-09   5.245e-09
25- 50  1.521e-08   7.895e-09
50-150  7.609e-08   4.538e-08
15-150  9.905e-08   5.415e-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: 1.89223     ( -0.344352   0.374249 )
Norm@50keV  : 2.27124E-03    ( -0.000522515   0.000498601 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          48.73 using 59 PHA bins.
# Reduced chi-squared =         0.8549 for     57 degrees of freedom 
# Null hypothesis probability =   7.740993e-01
 
Photon flux (15-150 keV)    in 36.62 sec: 0.324877 ( -0.0600053  0.0600528 ) ph/cm2/s
Energy fluence (15-150 keV)             : 7.64622e-07 ( -1.67346e-07  1.72828e-07 ) ergs/cm2

Cutoff power-law model

Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.82545     ( -1.25916   0.599464 )
Epeak [keV] : 117.446      (   )
Norm@50keV  : 2.47269E-03    (     )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          48.75 using 59 PHA bins.
# Reduced chi-squared =         0.8706 for     56 degrees of freedom 
# Null hypothesis probability =   7.431231e-01
 
Photon flux (15-150 keV)    in 36.62 sec: 0.324917 ( -0.060448  0.059897 ) ph/cm2/s
Energy fluence (15-150 keV)             : 7.62824e-07 ( -1.83001e-07  1.72568e-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)  = 2.23e-07
S(50-100 keV) = 2.40e-07

T90 vs. Hardness ratio plot

T90                                   = 33.1200000047684 sec.
Hardness ratio (energy fluence ratio) = 1.07623

Color vs. Color plot

Count Ratio  (25-50 keV) / (15-25 keV) = 1.18726
Count Ratio (50-100 keV) / (15-25 keV) = 0.77764

Mask shadow pattern

IMX = -4.133066594442243E-01, IMY = -5.760480846399125E-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:
-606.567400 -589.275000
-239.968000 0.168000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
244.9882 -15.6674    0.9  35.3   80.6   8.2998  12.5    1.7	Sco X-1                       
213.9751 -34.1794    3.7  25.0  147.7   0.8152   3.2 ------	UNKNOWN                       
215.9474  46.8908    4.1  56.7  -17.7   2.8655   2.8 ------	UNKNOWN                       
168.8013  -6.0153    2.5  40.3 -111.2   3.1666   4.6 ------	UNKNOWN                       
169.9136   2.2390    3.5  41.0  -98.4   3.4398   3.3 ------	UNKNOWN                       
160.5223 -18.1715    2.5  48.0 -129.1   5.3371   4.6 ------	UNKNOWN

Pre-slew background subtracted image of 15-350 keV band

Time interval of the image:
0.168000 36.792000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
244.9864 -15.6760  411.0  35.3   80.6  -0.0054  -0.0    2.2	Sco X-1                       
231.8498 -38.5227    1.4  35.3  125.7   1.2711   8.1 ------	UNKNOWN                       
169.7641 -10.6872    2.4  38.9 -118.4   0.7451   4.8 ------	UNKNOWN

Post-slew image of 15-350 keV band

Time interval of the image:
112.532590 662.312000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
170.4060 -60.7702    4.9  43.4 -140.3  -6.0024  -2.3    9.2	Cen X-3                       
186.9684 -62.7837   26.9  36.1 -145.7  -0.7328  -0.4    8.6	GX 301-2                      
244.9835 -15.6094    1.3  25.7   31.6  14.9639   9.2    1.9	Sco X-1                       
255.9906 -37.8151    1.5  19.0   96.5  12.7819   7.7    1.8	4U 1700-377                   
256.4214 -36.5592    5.5  19.6   93.0   3.4271   2.1    8.2	GX 349+2                      
262.8326 -24.7068    6.4  29.6   72.5   4.4921   1.8    9.9	GX 1+4                        
264.7328 -44.6006   19.8  25.2  115.7  -1.0887  -0.6    9.0	4U 1735-44                    
270.2837 -25.0787   10.0  35.1   80.1   4.0566   1.2    0.0	GX 5-1                        
270.3598 -25.8555 2591.3  34.7   81.3  -0.0127  -0.0    7.4	GRS 1758-258                  
276.1008 -30.3349    6.1  37.1   92.1  -7.8289  -1.9    9.3	H1820-303                     
263.0762 -33.7968    4.1  25.6   90.2   5.9022   2.9    4.9	GX 354-0                      
207.5189 -58.2888    3.2  25.2 -148.4   5.1359   3.6 ------	UNKNOWN                       
215.4495  16.0927    4.0  56.7  -17.7  20.5571   2.9 ------	UNKNOWN                       
136.6005 -67.4833    2.4  56.7 -151.8  39.4523   4.9 ------	UNKNOWN                       
163.3957 -52.3266    3.0  48.0 -129.0  26.9153   3.9 ------	UNKNOWN

Plot creation:
Wed Aug  2 18:52:33 EDT 2017