batgrbproduct analysis for trigger=1059494

batgrbproduct Analysis for Trigger=1059494

Analysis Summary

Notes:

1) No attempt has been made to eliminate the non-significant decimal places.
2) This batgrbproduct analysis is done of the amount of data for this trigger downloaded to date.
3) This batgrbproduct analysis is using the flight position for the mask-weighting calculation.
4) This page will be updated for up to 15 downlinks after the trigger.

======================================================================
                  BAT GRB EVENT DATA PROCESSING REPORT
    Process Script Ver: batgrbproduct v2.48
    Process Start Time (local time): Fri Jul  9 15:24:41 EDT 2021
             Host Name: batproc1
   Current Working Dir: /local/data/bat1/prebascript/trigger1059494/GCN5_download_cron
======================================================================

  Trigger: 01059494      Segment: 000

  BAT Trigger Time: 647443432   [s; MET]
      Trigger Stop: 647443496   [s; MET]
               UTC: 2021-07-08T13:23:24.666240    [includes UTCF correction] 
       Where From?: TDRSS position message

  BAT 
    RA: 142.579045529825   Dec: 14.4712178294586  [deg; J2000]

     Catalogged Source?: NO
     Point Source?:      YES
     GRB Indicated?:     YES    [ by BAT flight software ]
     Image S/N Ratio:    10.51
     Image Trigger?:     YES
     Rate S/N Ratio:     0  [ if not an image trigger ]
     Image S/N Ratio:    10.51

  Flight Position:   [ source = BAT ]
    RA: 142.579045529825   Dec: 14.4712178294586  [deg; J2000]

  Ground Position:   [ source = BAT pre-slew burst ]
    RA: 142.593802920625   Dec: 14.5229538938038  [deg; J2000]  
        { 09h 30m 22.5s , +14d 31' 22.6" }
         +/- 2.50056034464392 [arcmin] (estimated 90% radius based on SNR)
         +/- 1.10546229995544 [arcmin] (formal 1-sigma fit error)
    SNR: 8.21284467116698
 
  Angular difference between Flight and Ground position is 3.220359 arcmin
 
  Partial Coding Fraction: 0.7421875    [ including projection effects ]

  Duration
     T90: 298.431999921799 +/- 47.3189010708561
        Measured from: -74.6479998826981
                   to: 223.784000039101     [s; relative to TRIGTIME]
     T50: 115.007999897003 +/- 39.3778950267522
        Measured from: -12.2479999065399
                   to: 102.759999990463     [s; relative to TRIGTIME]



  Fluence
     Peak Flux  (peak 1 second)
        Measured from: 2.83599996566772     
                   to: 3.83599996566772     [s; relative to TRIGTIME]
     Total Fluence        
        Measured from: -99.8639999628067     
                   to: 263.72000002861     [s; relative to TRIGTIME]
     
             Band 1     Band 2     Band 3     Band 4
              15-25      25-50     50-100    100-350     keV
 Total     1.337306   1.157020   1.120498   0.436199
           0.147194   0.155000   0.144746   0.150750 [error]
 Peak      0.017554   0.011381   0.021867   0.028796
           0.008374   0.008887   0.008174   0.008031 [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 3.37e-07 5.75e-07 7.46e-07 1.96e-06 2.19e-06 3.61e-06   erg/cm2
              Error 7.10e-08 7.07e-08 1.55e-07 8.92e-07 3.51e-07 1.02e-06   erg/cm2
Peak flux Power-law 5.50e-022.46e-05 9.62e-023.26e-04 1.28e-013.96e-03 3.51e-011.21e+00 3.74e-011.86e-02 6.27e-014.05e-01   ph/cm2/s
              Error 8.87e-02 9.13e-02 6.57e-02 1.21e+00 2.91e-01 1.18e+00   ph/cm2/s
 
Fluence   Cutoff-PL 3.41e-07 5.75e-07 7.37e-07 1.88e-06 2.18e-06 3.53e-06   erg/cm2
              Error 6.75e-08 7.05e-08 1.51e-07 7.18e-07 3.49e-07 1.23e-06   erg/cm2
Peak flux Cutoff-PL 6.80e-02 1.07e-01 1.27e-01 2.88e-01 3.85e-01 5.88e-01   ph/cm2/s
              Error 8.70e-02 9.16e-02 6.63e-02 -------- 2.92e-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    1.623    0.264    -      -           6.68e-04 9.58e-05   85.550 57
CPL   1.624    0.279    10000.0   -0.0      6.69e-04 -2.85e-04   85.570 56
 
 
=== 1-s peak spectral analysis ===
 
Model Ph_index Ph_90err Epeak  Epeak_90err Norm     Nomr_90err chi2   dof
PL   -2.596    0.899    -      -           2.64e-05 1.27e-05   47.440 57
CPL  -3.088    0.450    10000.0    0.0      6.68e-05 0.00e+00   46.470 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: 106.944000 sec.
T50 in the 50-300 keV band: 59.968000 sec.

 
=== Table of the duration information ==
 
        Value   tstart    tstop
T100  363.584  -99.864  263.720
T90   298.432  -74.648  223.784
T50   115.008  -12.248  102.760
Peak    1.000    2.836    3.836

Click here for the BAT GCN circular template

Estimated redshift from machine learning (Ukwatta et al. 2016) - may take a few minutes to calcaulte

Image

Pre-slew 15-350 keV image (Event data; bkg subtracted)

#   RAcent  DECcent POSerr  Theta    Phi     Peak Cts     SNR  Name
  142.5938 +14.5230 0.0234   19.9  -72.8       3.6430     8.2  TRIG_01059494       
------------------------------------------
 
Foreground time interval of the image:
-75.899 -10.430 (delta_t =  65.469 [sec])
-10.000  36.780 (delta_t =  46.780 [sec])
 39.000 117.490 (delta_t =  78.490 [sec])
119.000 126.840 (delta_t =   7.840 [sec])
131.000 141.922 (delta_t =  10.922 [sec])
145.000 263.720 (delta_t = 118.720 [sec])
Background time interval of the image:

Lightcurves

Notes:

1) All plots contain as much data as has been downloaded to date.
2) The mask-weighted light curves are using the flight position.
3) Multiple plots of different time binning/intervals are shown to cover all scenarios of short/long GRBs, rate/image triggers, and real/false positives.
4) 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.
5) 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.
6) 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)

Spectra

Notes:

1) The fitting includes the systematic errors.
2) For long bursts, a spectral fit of 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.
4) For short bursts (T90<1sec), the specrtum is also fit with Blackbody, OTTB, and Double Blackbody.

Time averaged spectrum fit using the pre-slew DRM

Power-law model

Multiple GTIs in the spectrum
tstart tstop
-99.864000 -10.430000
-10.000000 36.780000
39.000000 117.490000
119.000000 126.840000
131.000000 141.921600
145.000000 263.720000
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.62347     ( -0.259192   0.269483 )
Norm@50keV  : 6.67652E-04    ( -9.7866e-05   9.37554e-05 )
------------------------------------------------------------
#Fit statistic  : Chi-Squared                   85.55     using 59 bins.
 Reduced chi-squared = 
# Null hypothesis probability of 8.54e-03 with 57 degrees of freedom
 
Photon flux (15-150 keV)    in 352.2 sec: 8.64317E-02 ( -0.0106083  0.0106113 ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.19308e-06 ( -3.45823e-07  3.55542e-07 ) ergs/cm2

Cutoff power-law model

Multiple GTIs in the spectrum
tstart tstop
-99.864000 -10.430000
-10.000000 36.780000
39.000000 117.490000
119.000000 126.840000
131.000000 141.921600
145.000000 263.720000
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.62357     ( -0.312347   0.246177 )
Epeak [keV] : 1.00000E+04      ( -9999.99 -10000 )
Norm@50keV  : 6.68753E-04    ( -9.85404e-05   -0.000668759 )
------------------------------------------------------------
#Fit statistic  : Chi-Squared                   85.57     using 59 bins.
 Reduced chi-squared = 
# Null hypothesis probability of 6.67e-03 with 56 degrees of freedom
 
Photon flux (15-150 keV)    in 352.2 sec: 8.63968E-02 ( -0.010578  0.0105806 ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.17754e-06 ( -3.2551e-07  3.71571e-07 ) ergs/cm2

Band function

Multiple GTIs in the spectrum
tstart tstop
-99.864000 -10.430000
-10.000000 36.780000
39.000000 117.490000
119.000000 126.840000
131.000000 141.921600
145.000000 263.720000
XSPEC12>exit
 XSPEC: quit
 
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -1.28847   ( 1.28931   1.28931 )
beta        : -1.62340    ( -0.269734   0.259161 )
Epeak [keV] : 25.6516      ( -25.2215 -25.2215 )
Norm@50keV   : 1.50209E-03    ( -0.000925856   1.4298 )
------------------------------------------------------------
 
Photon flux (15-150 keV)    in 352.2 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]    : 11.5985  (  )
R^2/D10^2   : 2.15565E-02  (   )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic  : Chi-Squared                  124.60     using 59 bins.
 Reduced chi-squared = 
# Null hypothesis probability of 5.99e-07 with 57 degrees of freedom
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  2.152e-07   5.869e-08
25- 50  6.504e-07   1.386e-07
50-150  5.139e-07   1.691e-07
15-150  1.380e-06   2.513e-07

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 199.363       (-98.3838      -199.363)
Norm        : 0.346336       (-0.0427982     0.0428068)
------------------------------------------------------------
#Fit statistic  : Chi-Squared                   89.00     using 59 bins.
 Reduced chi-squared = 
# Null hypothesis probability of 4.28e-03 with 57 degrees of freedom
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  3.037e-07   1.678e-07
25- 50  5.843e-07   3.216e-07
50-150  1.281e-06   7.030e-07
15-150  2.169e-06   1.188e-06

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 5.16735        (-1.26018      1.47651)
R1^2/D10^2  : 0.375287        (-0.241029      0.780291)
kT2 [keV]   : 35.5762        (-10.4352      24.1932)
R2^2/D10^2  : 4.90914E-04    (-0.000356854   0.00088177)
------------------------------------------------------------
#Fit statistic  : Chi-Squared                   78.46     using 59 bins.
 Reduced chi-squared = 
# Null hypothesis probability of 2.06e-02 with 55 degrees of freedom
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  3.967e-07   2.072e-07
25- 50  4.605e-07   1.745e-07
50-150  1.665e-06   9.206e-07
15-150  2.522e-06   1.063e-06

Peak spectrum fit

Power-law model

Time interval is from    2.836 sec. to    3.836 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: -2.59584     ( 2.59584   4.39473 )
Norm@50keV  : 2.63724E-05    ( -1.26528e-05   1.26528e-05 )
------------------------------------------------------------
#Fit statistic  : Chi-Squared                   47.44     using 59 bins.
 Reduced chi-squared = 
# Null hypothesis probability of 8.13e-01 with 57 degrees of freedom
 
Photon flux (15-150 keV)    in 1 sec: 0.373880 1.86031E-02 ( -0.37388  0.208043 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.44026e-16 ( -4.12164e-08  2.17977e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from    2.836 sec. to    3.836 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: -3.08834     ( 3.08834   3.98741 )
Epeak [keV] : 1.00000E+04      ( -10000 -10000 )
Norm@50keV  : 6.68197E-05    ( -6.68188e-05   -6.68188e-05 )
------------------------------------------------------------
#Fit statistic  : Chi-Squared                   46.47     using 59 bins.
 Reduced chi-squared = 
# Null hypothesis probability of 8.14e-01 with 56 degrees of freedom
 
Photon flux (15-150 keV)    in 1 sec: 0.385161 2.34561E-02 (    ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.72241e-16 ( 0  0 ) ergs/cm2

Band function

Time interval is from    2.836 sec. to    3.836 sec.
XSPEC12>exit
 XSPEC: quit
 
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -9.99999   ( 9.99999   9.99999 )
beta        : -0.585272    ( -1.25729   0.579998 )
Epeak [keV] : 16.9685      ( -16.9685 -16.9685 )
Norm@50keV   : 0.434687    ( -0.433856   0.253471 )
------------------------------------------------------------
 
Photon flux (15-150 keV)    in 1 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]    : 199.438  (-199.438  -199.438)
R^2/D10^2   : 1.49572E-04  (-0.000149572   0.0184181)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic  : Chi-Squared                   48.67     using 59 bins.
 Reduced chi-squared = 
# Null hypothesis probability of 7.76e-01 with 57 degrees of freedom
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  2.721e-10   1.971e-10
25- 50  2.128e-09   1.490e-09
50-150  3.650e-08   2.441e-08
15-150  3.890e-08   2.616e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 199.363       (-199.363      -199.363)
Norm        : 1.55753       (-0.825806     0.825828)
------------------------------------------------------------
#Fit statistic  : Chi-Squared                   49.55     using 59 bins.
 Reduced chi-squared = 
# Null hypothesis probability of 7.48e-01 with 57 degrees of freedom
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  3.878e-09   2.645e-09
25- 50  7.461e-09   5.060e-09
50-150  1.636e-08   1.155e-08
15-150  2.770e-08   1.965e-08

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 6.29316        (-2.88716      10.7487)
R1^2/D10^2  : 0.689812        (-0.822757      6.87509)
kT2 [keV]   : 200.000        (-200      -200)
R2^2/D10^2  : 1.37178E-04    (-7.55766e-05   0.000692877)
------------------------------------------------------------
#Fit statistic  : Chi-Squared                   44.76     using 59 bins.
 Reduced chi-squared = 
# Null hypothesis probability of 8.36e-01 with 55 degrees of freedom
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  4.144e-09   2.698e-09
25- 50  5.649e-09   3.673e-09
50-150  3.702e-08   2.775e-08
15-150  4.682e-08   3.365e-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: 1.68562     ( -0.253087   0.264488 )
Norm@50keV  : 6.80601E-04    ( -0.000102467   9.82038e-05 )
------------------------------------------------------------
#Fit statistic  : Chi-Squared                   84.62     using 59 bins.
 Reduced chi-squared = 
# Null hypothesis probability of 1.02e-02 with 57 degrees of freedom
 
Photon flux (15-150 keV)    in 328.2 sec: 8.99421E-02 ( -0.0109884  0.0109899 ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.07059e-06 ( -3.26279e-07  3.36261e-07 ) ergs/cm2

Cutoff power-law model

Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.69889     ( -0.283926   0.253289 )
Epeak [keV] : 9999.34      ( -9999.35 -9999.36 )
Norm@50keV  : 6.78275E-04    ( -9.97044e-05   0.00032041 )
------------------------------------------------------------
#Fit statistic  : Chi-Squared                   84.64     using 59 bins.
 Reduced chi-squared = 
# Null hypothesis probability of 8.02e-03 with 56 degrees of freedom
 
Photon flux (15-150 keV)    in 328.2 sec: 8.98974E-02 ( -0.010972  0.0109796 ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.0629e-06 ( -3.1883e-07  3.18807e-07 ) ergs/cm2

Band function

XSPEC12>exit
 XSPEC: quit
 
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -1.33573   ( 1.33625   1.33625 )
beta        : -1.68556    ( 1.68559   0.253026 )
Epeak [keV] : 22.7901      ( -22.691 -22.691 )
Norm@50keV   : 1.59081E-03    ( -0.000999064   12.349 )
------------------------------------------------------------
 
Photon flux (15-150 keV)    in 328.2 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)  = 5.75e-07
S(50-100 keV) = 7.46e-07

T90 vs. Hardness ratio plot

T90                                   = 298.431999921799 sec.
Hardness ratio (energy fluence ratio) = 1.29739

Color vs. Color plot

Count Ratio  (25-50 keV) / (15-25 keV) = 0.865187
Count Ratio (50-100 keV) / (15-25 keV) = 0.837877

Mask shadow pattern

IMX = 1.068418225591300E-01, IMY = 3.453715854325352E-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:

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

Time interval of the image:
-75.899410 -10.430000
-10.000000 36.780000
39.000000 117.490000
119.000000 126.840000
131.000000 141.921600
145.000000 263.720000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
135.6536 -40.4379   23.3  45.7  176.1   0.4417   0.5    9.0	Vela X-1                      
147.1217 -52.0891    2.8  53.6  160.8   7.9829   4.2 ------	UNKNOWN                       
142.0510 -42.6755    3.0  45.6  168.7   3.5268   3.8 ------	UNKNOWN                       
142.5938  14.5230    1.4  19.9  -72.8   3.6424   8.2 ------	UNKNOWN                       
126.7199  11.6044    2.8  32.1  -96.1   2.7460   4.1 ------	UNKNOWN

Post-slew image of 15-350 keV band

Time interval of the image:

Plot creation:
Fri Jul  9 15:30:13 EDT 2021