batgrbproduct analysis for trigger=1202768

batgrbproduct Analysis for Trigger=1202768

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): Sun Dec 17 17:29:21 EST 2023
             Host Name: batproc1
   Current Working Dir: /local/data/bat1/prebascript/trigger1202768/GCN5_download_cron
======================================================================

  Trigger: 01202768      Segment: 000

  BAT Trigger Time: 724457464   [s; MET]
      Trigger Stop: 724457536   [s; MET]
               UTC: 2023-12-16T22:10:31.440080    [includes UTCF correction] 
       Where From?: TDRSS position message

  BAT 
    RA: 245.092742782378   Dec: -15.4292711794308  [deg; J2000]

     Catalogged Source?: YES
     Point Source?:      YES
     GRB Indicated?:     NO    [ by BAT flight software ]
     Image S/N Ratio:    17.89
     Image Trigger?:     YES
     Rate S/N Ratio:     0  [ if not an image trigger ]
     Image S/N Ratio:    17.89

  Flight Position:   [ source = BAT ]
    RA: 245.092742782378   Dec: -15.4292711794308  [deg; J2000]

  Ground Position:   [ source = BAT pre-slew burst ]
    RA: 245.084123729054   Dec: -15.4783873715337  [deg; J2000]  
        { 16h 20m 20.2s , -15d 28' 42.2" }
         +/- 1.26849712199075 [arcmin] (estimated 90% radius based on SNR)
         +/- 0.519038749569769 [arcmin] (formal 1-sigma fit error)
    SNR: 21.6551886325592
 
  Angular difference between Flight and Ground position is 2.988827 arcmin
 
  Partial Coding Fraction: 0.4648438    [ including projection effects ]

  Duration
     T90: 625.111999988556 +/- 173.907989564521
        Measured from: -68.9399999380112
                   to: 556.172000050545     [s; relative to TRIGTIME]
     T50: 320.05999994278 +/- 32.4536326453263
        Measured from: 35.392000079155
                   to: 355.452000021935     [s; relative to TRIGTIME]



  Fluence
     Peak Flux  (peak 1 second)
        Measured from: 205.151999950409     
                   to: 206.151999950409     [s; relative to TRIGTIME]
     Total Fluence        
        Measured from: -93.3200000524521     
                   to: 835.327999949455     [s; relative to TRIGTIME]
     
             Band 1     Band 2     Band 3     Band 4
              15-25      25-50     50-100    100-350     keV
 Total    38.696997   3.857040  -0.474785  -0.215940
           0.314990   0.286223   0.245007   0.218211 [error]
 Peak      0.074740   0.016142   0.016254   0.012960
           0.010526   0.009545   0.008499   0.007182 [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 1.42e-05 1.81e-06 1.00e-07 5.88e-09 1.61e-05 1.61e-05   erg/cm2
              Error -------- -------- -------- -------- -------- --------   erg/cm2
Peak flux Power-law 7.70e-01 1.61e-01 1.68e-02 1.93e-03 9.49e-01 9.50e-01   ph/cm2/s
              Error 1.88e-01 9.43e-02 2.60e-02 6.27e-03 2.44e-01 2.45e-01   ph/cm2/s
 
Fluence   Cutoff-PL 1.34e-05 1.39e-06 1.22e-09 1.98e-16 1.48e-05 1.48e-05   erg/cm2
              Error 1.28e-06 1.90e-07 2.78e-09 3.96e-14 1.29e-06 1.29e-06   erg/cm2
Peak flux Cutoff-PL 7.70e-01 1.58e-01 1.59e-02 1.77e-03 9.45e-01 9.47e-01   ph/cm2/s
              Error 1.87e-01 7.60e-02 1.60e-02 6.22e-03 2.54e-01 2.44e-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    6.170    0.000    -      -           1.19e-04 0.00e+00  118.480 57
CPL   1.000    0.000      50.0    0.0      1.53e-03 0.00e+00  847.040 56
 
The chi2 of BB fit is 87.23 which shows a significant improvement in the fit over a PL.
Check the BB fit.
 
=== 1-s peak spectral analysis ===
 
Model Ph_index Ph_90err Epeak  Epeak_90err Norm     Nomr_90err chi2   dof
PL    4.257    1.105    -      -           1.23e-03 1.51e-03   53.480 57
CPL  -6.480    0.000      16.4    0.0      9.22e+05 0.00e+00   51.550 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: 0.000000 sec.
T50 in the 50-300 keV band: 0.000000 sec.

 
=== Table of the duration information ==
 
        Value   tstart    tstop
T100  928.648  -93.320  835.328
T90   625.112  -68.940  556.172
T50   320.060   35.392  355.452
Peak    1.000  205.152  206.152

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
  245.0841 -15.4784 0.0088   30.2 -111.6      47.8793    21.7  TRIG_01202768       
------------------------------------------
 
Foreground time interval of the image:
-77.699 835.328 (delta_t = 913.027 [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 72.000000

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 72.000000

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 72.000000

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

Time interval is from  -93.320 sec. to  835.328 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 6.17027     (     )
Norm@50keV  : 1.19366E-04    (     )
------------------------------------------------------------
#Fit statistic : Chi-Squared =         118.48 using 59 PHA bins.
# Reduced chi-squared =         2.0786 for     57 degrees of freedom 
# Null hypothesis probability =   3.321717e-06
 
Photon flux (15-150 keV)    in 928.6 sec: 0.583209 (    ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.61327e-05 ( 0  0 ) ergs/cm2

Cutoff power-law model

Time interval is from  -93.320 sec. to  835.328 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.00000     (     )
Epeak [keV] : 50.0000      (   )
Norm@50keV  : 1.52623E-03    (     )
------------------------------------------------------------
#Fit statistic : Chi-Squared =         847.04 using 59 PHA bins.
# Reduced chi-squared =         15.126 for     56 degrees of freedom 
# Null hypothesis probability =  9.647110e-142
 
Photon flux (15-150 keV)    in 928.6 sec: 0.532500 ( -0.052015  0.050992 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.47925e-05 ( -1.30663e-06  1.2797e-06 ) ergs/cm2

Band function

Time interval is from  -93.320 sec. to  835.328 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -9.35794   (     )
beta        : -6.20235    (     )
Epeak [keV] : 249.348      (   )
Norm@50keV   : 1.57656E-02    (     )
------------------------------------------------------------
#Fit statistic : Chi-Squared =         118.54 using 59 PHA bins.
# Reduced chi-squared =         2.1552 for     55 degrees of freedom 
# Null hypothesis probability =   1.473045e-06
 
Photon flux (15-150 keV)    in 928.6 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]    : 2.73099  (-0.113609  0.123508)
R^2/D10^2   : 141.063  (-43.6657   61.7087)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          87.23 using 59 PHA bins.
# Reduced chi-squared =          1.530 for     57 degrees of freedom 
# Null hypothesis probability =   6.126399e-03
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.333e-05   1.398e-06
25- 50  1.383e-06   1.407e-07
50-150  1.000e-09   4.452e-10
15-150  1.472e-05   1.453e-06

Thermal bremsstrahlung (OTTB)

XSPEC12>exit
 XSPEC: quit
 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 4.70822       (-0.281958      0.316434)
Norm        : 160.853       (-42.3373     56.6176)
------------------------------------------------------------
 Reduced chi-squared = 
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.388e-05   1.212e-06
25- 50  1.526e-06   1.704e-07
50-150  5.788e-09   2.411e-09
15-150  1.541e-05   1.263e-06

Double BB

XSPEC12>exit
 XSPEC: quit
 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 2.74253        (-0.113606      0.123512)
R1^2/D10^2  : 135.859        (-43.6666      61.7066)
kT2 [keV]   : 0.492374        (-1.7879      2.2274)
R2^2/D10^2  : 6.04189E+10    (-6.83263e+10   4.37787e+15)
------------------------------------------------------------
 Reduced chi-squared = 
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  0.000e+00   0.000e+00
25- 50  0.000e+00   0.000e+00
50-150  0.000e+00   0.000e+00
15-150  0.000e+00   0.000e+00

Peak spectrum fit

Power-law model

Time interval is from  205.152 sec. to  206.152 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 4.25709     ( -0.973829   1.23601 )
Norm@50keV  : 1.22558E-03    ( -0.00122558   0.00179421 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          53.48 using 59 PHA bins.
# Reduced chi-squared =         0.9382 for     57 degrees of freedom 
# Null hypothesis probability =   6.080617e-01
 
Photon flux (15-150 keV)    in 1 sec: 0.949083 ( -0.24301  0.245601 ) ph/cm2/s
Energy fluence (15-150 keV)             : 3.27468e-08 ( -9.9842e-09  1.18374e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from  205.152 sec. to  206.152 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: -6.47975     (     )
Epeak [keV] : 16.4122      (   )
Norm@50keV  : 9.22349E+05    (     )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          51.55 using 59 PHA bins.
# Reduced chi-squared =         0.9205 for     56 degrees of freedom 
# Null hypothesis probability =   6.438655e-01
 
Photon flux (15-150 keV)    in 1 sec: 0.944838 0.938136 0.929772 (    ) ph/cm2/s
Energy fluence (15-150 keV)             : 9.6105e-16 ( 0  0 ) ergs/cm2

Band function

Time interval is from  205.152 sec. to  206.152 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : 3.70125   ( 1.83871   1.83871 )
beta        : -8.69606    ( 9.61766   19.1066 )
Epeak [keV] : 15.1020      ( -5.73684 3.19652 )
Norm@50keV   : 4267.92    ( -4268.14   66938.8 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          51.69 using 59 PHA bins.
# Reduced chi-squared =         0.9398 for     55 degrees of freedom 
# Null hypothesis probability =   6.020109e-01
 
Photon flux (15-150 keV)    in 1 sec:  (    ) ph/cm2/s
Energy fluence (15-150 keV)             : 0 ( 0  0 ) ergs/cm2

Single BB

 XSPEC: quit
 
 
Spectral model blackbody:
------------------------------------------------------------
Parameters  : value    Lower 90%  Upper 90%
kT [keV]    : 3.30606  (-0.686057  0.817945)
R^2/D10^2   : 73.8450  (-73.845   235.264)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
 Reduced chi-squared = 
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  2.463e-08   1.402e-08
25- 50  4.978e-09   3.201e-09
50-150  1.698e-11   1.746e-11
15-150  2.962e-08   1.695e-08

Thermal bremsstrahlung (OTTB)

XSPEC12>exit
 XSPEC: quit
 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 7.04316       (-2.30226      3.92583)
Norm        : 74.0880       (-47.0387     164.933)
------------------------------------------------------------
 Reduced chi-squared = 
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  2.376e-08   1.345e-08
25- 50  5.961e-09   3.990e-09
50-150  1.351e-10   1.458e-10
15-150  2.985e-08   1.748e-08

Double BB

XSPEC12>exit
 XSPEC: quit
 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 3.21607        (-0.67989      0.789319)
R1^2/D10^2  : 84.9408        (-60.8679      278.581)
kT2 [keV]   : 71.4575        (-50.0953      -71.4589)
R2^2/D10^2  : 5.48518E-04    (-0.000513756   0.0100053)
------------------------------------------------------------
 Reduced chi-squared = 
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  2.438e-08   1.393e-08
25- 50  6.225e-09   3.303e-09
50-150  2.882e-08   1.746e-08
15-150  5.942e-08   3.037e-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: 6.17128     (     )
Norm@50keV  : 1.19237E-04    (     )
------------------------------------------------------------
#Fit statistic : Chi-Squared =         121.33 using 59 PHA bins.
# Reduced chi-squared =         2.1285 for     57 degrees of freedom 
# Null hypothesis probability =   1.509301e-06
 
Photon flux (15-150 keV)    in 913 sec: 0.583159 (    ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.58596e-05 ( 0  0 ) ergs/cm2

Cutoff power-law model

Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.00000     (     )
Epeak [keV] : 50.0000      (   )
Norm@50keV  : 1.52205E-03    (     )
------------------------------------------------------------
#Fit statistic : Chi-Squared =         846.30 using 59 PHA bins.
# Reduced chi-squared =         15.112 for     56 degrees of freedom 
# Null hypothesis probability =  1.366218e-141
 
Photon flux (15-150 keV)    in 913 sec: 0.532461 ( -0.052114  0.051097 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.45419e-05 ( -1.2877e-06  1.26067e-06 ) ergs/cm2

Band function

 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -9.36591   (     )
beta        : -6.20514    (     )
Epeak [keV] : 249.005      (   )
Norm@50keV   : 1.57229E-02    (     )
------------------------------------------------------------
#Fit statistic : Chi-Squared =         121.39 using 59 PHA bins.
# Reduced chi-squared =         2.2071 for     55 degrees of freedom 
# Null hypothesis probability =   6.529143e-07
 
Photon flux (15-150 keV)    in 913 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)  = 1.81e-06
S(50-100 keV) = 1.00e-07

T90 vs. Hardness ratio plot

T90                                   = 625.111999988556 sec.
Hardness ratio (energy fluence ratio) = 0.0552486

Color vs. Color plot

Count Ratio  (25-50 keV) / (15-25 keV) = 0.0996729
Count Ratio (50-100 keV) / (15-25 keV) = -0.0122693

Mask shadow pattern

IMX = -2.137544653424678E-01, IMY = 5.402702161296974E-01

TIME vs. PHA plot around the trigger time

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 72.000000

TIME vs. DetID plot around the trigger time

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 72.000000

100 us light curve (15-350 keV)

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 72.000000

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:
-77.699400 835.328000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
170.4067 -60.6176    4.5  58.2   -8.3  12.8922   2.5    2.7	Cen X-3                       
186.8911 -62.8168   18.5  54.4  -16.9   2.3439   0.6    7.0	GX 301-2                      
245.0621 -15.5320    0.6  30.1 -111.5  43.4270  19.6    8.1	Sco X-1                       
184.0597  -0.1890    3.5  32.2   77.5   8.8460   3.3 ------	UNKNOWN                       
186.2164   2.9822    2.7  31.6   84.7  10.9664   4.3 ------	UNKNOWN                       
226.5893  32.2197    3.8  45.8  162.8  12.4279   3.0 ------	UNKNOWN                       
251.8277  32.2595    2.3  57.0 -173.9  25.5438   5.1 ------	UNKNOWN                       
214.4862 -45.0160    2.6  33.0  -32.2   7.9217   4.4 ------	UNKNOWN                       
201.5610 -57.3772    2.5  46.4  -22.4  11.9725   4.6 ------	UNKNOWN

Post-slew image of 15-350 keV band

Time interval of the image:

Plot creation:
Sun Dec 17 17:32:35 EST 2023