batgrbproduct analysis for trigger=1273106

batgrbproduct Analysis for Trigger=1273106

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): Tue Dec 10 11:49:26 EST 2024
             Host Name: batproc1
   Current Working Dir: /local/data/bat1/prebascript/trigger1273106/GCN5_download_cron
======================================================================

  Trigger: 01273106      Segment: 000

  BAT Trigger Time: 755434821.12   [s; MET]
      Trigger Stop: 755434822.144   [s; MET]
               UTC: 2024-12-09T10:59:46.438980    [includes UTCF correction] 
       Where From?: TDRSS position message

  BAT 
    RA: 190.110870775986   Dec: -2.87869882402428  [deg; J2000]

     Catalogged Source?: NO
     Point Source?:      YES
     GRB Indicated?:     YES    [ by BAT flight software ]
     Image S/N Ratio:    12.99
     Image Trigger?:     NO
     Rate S/N Ratio:     29.9833287011299  [ if not an image trigger ]
     Image S/N Ratio:    12.99

  Flight Position:   [ source = BAT ]
    RA: 190.110870775986   Dec: -2.87869882402428  [deg; J2000]

  Ground Position:   [ source = BAT pre-slew burst ]
    RA: 190.10000245361   Dec: -2.88129393680302  [deg; J2000]  
        { 12h 40m 24.0s , -02d 52' 52.7" }
         +/- 0.783342667491334 [arcmin] (estimated 90% radius based on SNR)
         +/- 0.249739486884726 [arcmin] (formal 1-sigma fit error)
    SNR: 43.1137534146606
 
  Angular difference between Flight and Ground position is 0.669630 arcmin
 
  Partial Coding Fraction: 0.65625    [ including projection effects ]

  Duration
     T90: 50.1560000181198 +/- 3.32103896194526
        Measured from: -0.0999999046325684
                   to: 50.0560001134872     [s; relative to TRIGTIME]
     T50: 23.6440000534058 +/- 0.9848857985775
        Measured from: 7.3840000629425
                   to: 31.0280001163483     [s; relative to TRIGTIME]



  Fluence
     Peak Flux  (peak 1 second)
        Measured from: 3.58799993991852     
                   to: 4.58799993991852     [s; relative to TRIGTIME]
     Total Fluence        
        Measured from: -2.66799998283386     
                   to: 68.1879999637604     [s; relative to TRIGTIME]
     
             Band 1     Band 2     Band 3     Band 4
              15-25      25-50     50-100    100-350     keV
 Total     2.475728   3.838868   3.096316   0.601370
           0.067423   0.074129   0.066971   0.051950 [error]
 Peak      0.053362   0.098738   0.124157   0.037122
           0.008864   0.010240   0.010034   0.007448 [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 8.66e-07 1.62e-06 2.32e-06 7.09e-06 6.61e-06 1.19e-05   erg/cm2
              Error 4.21e-08 4.62e-08 7.02e-08 4.82e-07 1.73e-07 5.21e-07   erg/cm2
Peak flux Power-law 5.24e-01 7.08e-01 7.06e-01 1.27e+00 2.35e+00 3.21e+00   ph/cm2/s
              Error 1.00e-01 8.59e-02 7.65e-02 2.79e-01 2.41e-01 3.51e-01   ph/cm2/s
 
Fluence   Cutoff-PL 7.48e-07 1.67e-06 2.44e-06 3.46e-06 6.37e-06 8.33e-06   erg/cm2
              Error 5.40e-08 5.16e-08 8.17e-08 7.39e-07 1.91e-07 7.52e-07   erg/cm2
Peak flux Cutoff-PL 3.69e-01 7.61e-01 8.24e-01 4.61e-01 2.26e+00 2.42e+00   ph/cm2/s
              Error 1.23e-01 1.03e-01 1.03e-01 2.46e-01 2.47e-01 3.43e-01   ph/cm2/s
 
Fluence        Band 7.41e-07 1.67e-06 2.44e-06 3.79e-06 6.37e-06 8.77e-06   erg/cm2
              Error -------- -------- 7.79e-08 -------- -------- --------   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    1.475    0.045    -      -           9.80e-03 2.43e-04   83.370 57
CPL   0.868    0.203     102.4   18.2      1.86e-02 3.92e-03   53.780 56
 
 
=== 1-s peak spectral analysis ===
 
Model Ph_index Ph_90err Epeak  Epeak_90err Norm     Nomr_90err chi2   dof
PL    1.006    0.159    -      -           2.04e-02 2.06e-03   69.170 57
CPL  -0.353    0.846      99.2   36.1      8.22e-02 7.99e-02   58.690 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: 38.720000 sec.
T50 in the 50-300 keV band: 20.736000 sec.

 
=== Table of the duration information ==
 
        Value   tstart    tstop
T100   70.856   -2.668   68.188
T90    50.156   -0.100   50.056
T50    23.644    7.384   31.028
Peak    1.000    3.588    4.588

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
  190.1000  -2.8813 0.0045   26.9   37.5       3.9072    43.1  TRIG_01273106       
------------------------------------------
 
Foreground time interval of the image:
 -2.668  14.381 (delta_t =  17.049 [sec])
Background time interval of the image:
-239.120 -76.317 (delta_t = 162.803 [sec])
-75.120  -2.668 (delta_t =  72.452 [sec])

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 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)

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   -2.668 sec. to   68.188 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.47510     ( -0.0452343   0.0452552 )
Norm@50keV  : 9.79680E-03    ( -0.0002434   0.000243397 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          83.37 using 59 PHA bins.
# Reduced chi-squared =          1.463 for     57 degrees of freedom 
# Null hypothesis probability =   1.294488e-02
 
Photon flux (15-150 keV)    in 70.86 sec: 1.21502 ( -0.0330447  0.0331225 ) ph/cm2/s
Energy fluence (15-150 keV)             : 6.61324e-06 ( -1.73284e-07  1.7349e-07 ) ergs/cm2

Cutoff power-law model

Time interval is from   -2.668 sec. to   68.188 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 0.867869     ( -0.207674   0.198644 )
Epeak [keV] : 102.358      ( -13.0447 23.3929 )
Norm@50keV  : 1.85731E-02    ( -0.00342553   0.00441171 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          53.78 using 59 PHA bins.
# Reduced chi-squared =         0.9603 for     56 degrees of freedom 
# Null hypothesis probability =   5.594035e-01
 
Photon flux (15-150 keV)    in 70.86 sec: 1.16564 ( -0.036  0.0362 ) ph/cm2/s
Energy fluence (15-150 keV)             : 6.37306e-06 ( -1.91627e-07  1.91244e-07 ) ergs/cm2

Band function

Time interval is from   -2.668 sec. to   68.188 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -0.873372   ( -0.186122   0.18597 )
beta        : -9.36563    ( 9.37032   19.3703 )
Epeak [keV] : 103.033      ( -8.46163 22.105 )
Norm@50keV   : 1.84385E-02    ( -0.00327344   0.00268353 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          53.78 using 59 PHA bins.
# Reduced chi-squared =         0.9779 for     55 degrees of freedom 
# Null hypothesis probability =   5.211573e-01
 
Photon flux (15-150 keV)    in 70.86 sec: 1.16579 (    ) ph/cm2/s
Energy fluence (15-150 keV)             : 6.37303e-06 ( 0  0 ) ergs/cm2

Single BB

 
Spectral model blackbody:
------------------------------------------------------------
Parameters  : value    Lower 90%  Upper 90%
kT [keV]    : 16.8802  (  )
R^2/D10^2   : 9.08832E-02  (   )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =         275.33 using 59 PHA bins.
# Reduced chi-squared =         4.8304 for     57 degrees of freedom 
# Null hypothesis probability =   2.329174e-30
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  3.744e-07   1.903e-08
25- 50  1.647e-06   5.208e-08
50-150  3.344e-06   1.399e-07
15-150  5.366e-06   1.492e-07

Thermal bremsstrahlung (OTTB)

XSPEC12>exit
 XSPEC: quit
 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 200.000       (-7.15648      -200)
Norm        : 5.02447       (-0.124695     0.124695)
------------------------------------------------------------
 Reduced chi-squared = 
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  8.867e-07   2.586e-08
25- 50  1.706e-06   4.677e-08
50-150  3.741e-06   9.814e-08
15-150  6.334e-06   1.704e-07

Double BB

XSPEC12>exit
 XSPEC: quit
 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 7.52674        (-0.882128      0.970825)
R1^2/D10^2  : 0.809014        (-0.25458      0.418848)
kT2 [keV]   : 24.9779        (-2.0158      2.69232)
R2^2/D10^2  : 1.85508E-02    (-0.00611233   0.00729704)
------------------------------------------------------------
 Reduced chi-squared = 
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  7.016e-07   7.125e-08
25- 50  1.686e-06   1.098e-07
50-150  3.928e-06   2.916e-07
15-150  6.315e-06   3.642e-07

Peak spectrum fit

Power-law model

Time interval is from    3.588 sec. to    4.588 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.00639     ( -0.160784   0.157424 )
Norm@50keV  : 2.04098E-02    ( -0.00206349   0.00206048 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          69.17 using 59 PHA bins.
# Reduced chi-squared =          1.213 for     57 degrees of freedom 
# Null hypothesis probability =   1.295173e-01
 
Photon flux (15-150 keV)    in 1 sec: 2.35017 ( -0.240315  0.24152 ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.20183e-07 ( -2.38481e-08  2.40086e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from    3.588 sec. to    4.588 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: -0.352648     ( -0.929159   0.762462 )
Epeak [keV] : 99.1933      ( -19.2342 52.9545 )
Norm@50keV  : 8.21541E-02    ( -0.0435125   0.116218 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          58.69 using 59 PHA bins.
# Reduced chi-squared =          1.048 for     56 degrees of freedom 
# Null hypothesis probability =   3.772286e-01
 
Photon flux (15-150 keV)    in 1 sec: 2.25977 ( -0.24742  0.24737 ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.0977e-07 ( -2.5253e-08  2.5333e-08 ) ergs/cm2

Band function

Time interval is from    3.588 sec. to    4.588 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : 0.352961   ( -0.604284   0.793477 )
beta        : -10.0000    ( 10   1.42109e-14 )
Epeak [keV] : 99.1715      ( -14.1301 52.959 )
Norm@50keV   : 8.21891E-02    ( -0.0435037   0.116504 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          58.69 using 59 PHA bins.
# Reduced chi-squared =          1.067 for     55 degrees of freedom 
# Null hypothesis probability =   3.418967e-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]    : 21.2764  (-2.29166  2.67596)
R^2/D10^2   : 9.87827E-02  (-0.0312382   0.0437583)
(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  8.400e-09   1.531e-09
25- 50  4.353e-08   7.040e-09
50-150  1.470e-07   2.075e-08
15-150  1.989e-07   2.660e-08

Thermal bremsstrahlung (OTTB)

XSPEC12>exit
 XSPEC: quit
 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 200.000       (-18.7713      -200)
Norm        : 9.42317       (-0.995445     0.995445)
------------------------------------------------------------
 Reduced chi-squared = 
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  2.347e-08   6.015e-09
25- 50  4.514e-08   2.122e-08
50-150  9.901e-08   5.470e-08
15-150  1.676e-07   9.100e-08

Double BB

XSPEC12>exit
 XSPEC: quit
 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 7.12218        (-4.06904      10.2513)
R1^2/D10^2  : 0.786040        (-0.730654      21.1784)
kT2 [keV]   : 24.3666        (-3.80888      17.1472)
R2^2/D10^2  : 5.87055E-02    (-0.05385   0.0493797)
------------------------------------------------------------
 Reduced chi-squared = 
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.266e-08   6.410e-09
25- 50  4.359e-08   1.753e-08
50-150  1.534e-07   6.235e-08
15-150  2.096e-07   9.651e-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: 1.09040     ( -0.0572299   0.0568585 )
Norm@50keV  : 1.57684E-02    ( -0.000523328   0.000522863 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          59.70 using 59 PHA bins.
# Reduced chi-squared =          1.047 for     57 degrees of freedom 
# Null hypothesis probability =   3.777800e-01
 
Photon flux (15-150 keV)    in 17.05 sec: 1.82735 ( -0.0629202  0.0630274 ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.81958e-06 ( -9.88486e-08  9.89846e-08 ) ergs/cm2

Cutoff power-law model

Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 0.436275     ( -0.267099   0.251687 )
Epeak [keV] : 139.049      ( -24.0971 49.4927 )
Norm@50keV  : 3.04549E-02    ( -0.00663813   0.00902258 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          38.25 using 59 PHA bins.
# Reduced chi-squared =         0.6830 for     56 degrees of freedom 
# Null hypothesis probability =   9.665546e-01
 
Photon flux (15-150 keV)    in 17.05 sec: 1.77267 ( -0.06587  0.066 ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.74191e-06 ( -1.0571e-07  1.05164e-07 ) ergs/cm2

Band function

 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -0.440837   ( -0.240008   0.203069 )
beta        : -9.36269    ( 9.37063   19.3706 )
Epeak [keV] : 139.928      ( -13.3026 35.5502 )
Norm@50keV   : 3.02747E-02    ( -0.00635298   0.00488617 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          38.25 using 59 PHA bins.
# Reduced chi-squared =         0.6954 for     55 degrees of freedom 
# Null hypothesis probability =   9.582512e-01
 
Photon flux (15-150 keV)    in 17.05 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)  = 1.62e-06
S(50-100 keV) = 2.32e-06

T90 vs. Hardness ratio plot

T90                                   = 50.1560000181198 sec.
Hardness ratio (energy fluence ratio) = 1.4321

Color vs. Color plot

Count Ratio  (25-50 keV) / (15-25 keV) = 1.5506
Count Ratio (50-100 keV) / (15-25 keV) = 1.25067

Mask shadow pattern

IMX = 4.024509322672266E-01, IMY = -3.083503906805937E-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:
-239.120000 -76.317500
-75.120000 -2.668000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
244.9602 -15.6425    0.8  35.5  -90.0  14.6150  14.1    1.1	Sco X-1                       
254.3921  35.4350   27.5  46.8 -171.9  -0.3657  -0.4    6.4	Her X-1                       
170.3078 -25.5951    2.7  53.7   16.9   6.6210   4.2 ------	UNKNOWN                       
185.4700 -23.3288    2.8  41.0    9.0   2.7797   4.1 ------	UNKNOWN

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

Time interval of the image:
-2.668000 14.380600
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
245.1273 -15.6511   13.0  35.6  -90.1  -0.1414  -0.9    8.6	Sco X-1                       
254.4015  35.1556    0.0  46.6 -171.5   0.1466   1.1   11.5	Her X-1                       
190.1000  -2.8813    0.3  26.9   37.5   3.9069  43.1 ------	UNKNOWN                       
264.1397   5.6508    2.7  48.1 -129.2   1.3268   4.3 ------	UNKNOWN

Post-slew image of 15-350 keV band

Time interval of the image:
80.680600 283.680610
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
173.6600  30.6805    2.8  37.1  132.8   3.4050   4.2 ------	UNKNOWN                       
165.4181 -31.8799    2.9  37.1   12.6   2.1089   4.0 ------	UNKNOWN                       
162.1643 -49.2225    2.8  52.1   -0.6   3.0048   4.2 ------	UNKNOWN                       
220.0958  15.5809    3.2  35.0 -146.2   1.8275   3.7 ------	UNKNOWN                       
220.4038   7.4765    2.1  32.0 -132.5   2.7020   5.5 ------	UNKNOWN

Plot creation:
Tue Dec 10 11:54:47 EST 2024