batgrbproduct analysis for trigger=1180060

batgrbproduct Analysis for Trigger=1180060

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 21 11:56:14 EDT 2023
             Host Name: batproc1
   Current Working Dir: /local/data/bat1/prebascript/trigger1180060/GCN5_download_cron
======================================================================

  Trigger: 01180060      Segment: 000

  BAT Trigger Time: 711531992   [s; MET]
      Trigger Stop: 711532104   [s; MET]
               UTC: 2023-07-20T07:46:00.324520    [includes UTCF correction] 
       Where From?: TDRSS position message

  BAT 
    RA: 47.6704340786371   Dec: 59.7950276979517  [deg; J2000]

     Catalogged Source?: NO
     Point Source?:      YES
     GRB Indicated?:     YES    [ by BAT flight software ]
     Image S/N Ratio:    10.7
     Image Trigger?:     YES
     Rate S/N Ratio:     0  [ if not an image trigger ]
     Image S/N Ratio:    10.7

  Flight Position:   [ source = BAT ]
    RA: 47.6704340786371   Dec: 59.7950276979517  [deg; J2000]

  Ground Position:   [ source = BAT pre-slew burst ]
    RA: 47.6053267914638   Dec: 59.7652550813726  [deg; J2000]  
        { 03h 10m 25.3s , +59d 45' 54.9" }
         +/- 2.34286017616718 [arcmin] (estimated 90% radius based on SNR)
         +/- 1.12536715562001 [arcmin] (formal 1-sigma fit error)
    SNR: 9.01382826645089
 
  Angular difference between Flight and Ground position is 2.656493 arcmin
 
  Partial Coding Fraction: 0.640625    [ including projection effects ]

  Duration
     T90: 112 +/- 
        Measured from: 0
                   to: 112     [s; relative to TRIGTIME]
     T50: 112 +/- 
        Measured from: 0
                   to: 112     [s; relative to TRIGTIME]

    WARNING: battblocks failed.  Used TDRSS fore/background intervals

  Fluence
     Peak Flux  (peak 112 second)
        Measured from: 0     
                   to: 112     [s; relative to TRIGTIME]
     Total Fluence        
        Measured from: 0     
                   to: 112     [s; relative to TRIGTIME]
     
             Band 1     Band 2     Band 3     Band 4
              15-25      25-50     50-100    100-350     keV
 Total     2.108307   1.789102   0.336290   0.027712
           0.105109   0.111426   0.100531   0.106165 [error]
 Peak      2.108307   1.789102   0.336290   0.027712
           0.105109   0.111426   0.100531   0.106165 [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 7.00e-07 6.76e-07 4.56e-07 4.81e-07 2.03e-06 2.31e-06   erg/cm2
              Error 6.79e-08 5.79e-08 8.14e-08 1.61e-07 1.87e-07 2.76e-07   erg/cm2
Peak flux Power-law 2.06e-01 1.11e-01 3.75e-02 1.64e-02 3.64e-01 3.71e-01   ph/cm2/s
              Error 2.05e-02 9.19e-03 6.46e-03 5.13e-03 2.73e-02 2.78e-02   ph/cm2/s
 
Fluence   Cutoff-PL 6.54e-07 7.60e-07 3.20e-07 3.74e-08 1.77e-06 1.77e-06   erg/cm2
              Error 7.59e-08 7.78e-08 1.15e-07 7.88e-08 1.98e-07 2.14e-07   erg/cm2
Peak flux Cutoff-PL 1.90e-01 1.25e-01 2.79e-02 1.75e-03 3.44e-01 3.45e-01   ph/cm2/s
              Error 2.32e-02 1.25e-02 9.07e-03 3.28e-03 2.88e-02 2.90e-02   ph/cm2/s
 
Fluence        Band 1.33e-06 2.45e-06 2.03e-06 2.79e-06 6.86e-06 8.66e-06   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    2.568    0.175    -      -           1.77e-03 2.30e-04   53.230 57
CPL   1.047    0.935      21.3   12.8      1.69e-02 4.87e-02   44.800 56
 
 
=== 1-s peak spectral analysis ===
 
Model Ph_index Ph_90err Epeak  Epeak_90err Norm     Nomr_90err chi2   dof
PL    2.568    0.175    -      -           1.77e-03 2.30e-04   53.230 57
CPL   1.047    0.935      21.3   12.8      1.69e-02 4.87e-02   44.800 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  112.000    0.000  112.000
T90   112.000    0.000  112.000
T50   112.000    0.000  112.000
Peak  112.000    0.000  112.000

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
   47.6053 +59.7653 0.0213   24.8 -113.3       4.2638     9.0  TRIG_01180060       
------------------------------------------
 
Foreground time interval of the image:
  0.000 112.000 (delta_t = 112.000 [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

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)

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    0.000 sec. to  112.000 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 2.56845     ( -0.169721   0.180145 )
Norm@50keV  : 1.77479E-03    ( -0.000229712   0.000230001 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          53.23 using 59 PHA bins.
# Reduced chi-squared =         0.9339 for     57 degrees of freedom 
# Null hypothesis probability =   6.171700e-01
 
Photon flux (15-150 keV)    in 112 sec: 0.363801 ( -0.0272992  0.027304 ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.02655e-06 ( -1.84539e-07  1.89801e-07 ) ergs/cm2

Cutoff power-law model

Time interval is from    0.000 sec. to  112.000 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.04711     ( -1.15938   0.710631 )
Epeak [keV] : 21.3365      ( -19.4181 6.1907 )
Norm@50keV  : 1.68810E-02    ( -0.016881   0.0804194 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          44.80 using 59 PHA bins.
# Reduced chi-squared =         0.8000 for     56 degrees of freedom 
# Null hypothesis probability =   8.586819e-01
 
Photon flux (15-150 keV)    in 112 sec: 0.344409 ( -0.028714  0.028982 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.76783e-06 ( -1.83019e-07  2.1233e-07 ) ergs/cm2

Band function

Time interval is from    0.000 sec. to  112.000 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -1.08166   ( -0.914342   0.78036 )
beta        : -9.37167    ( 9.37167   19.3716 )
Epeak [keV] : 21.1153      ( -4.45041 6.41066 )
Norm@50keV   : 1.59722E-02    ( -0.0159775   0.218584 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          44.80 using 59 PHA bins.
# Reduced chi-squared =         0.8146 for     55 degrees of freedom 
# Null hypothesis probability =   8.352578e-01
 
Photon flux (15-150 keV)    in 112 sec:  (    ) ph/cm2/s
Energy fluence (15-150 keV)             : 6.86112e-06 ( 0  0 ) ergs/cm2

Single BB

 
Spectral model blackbody:
------------------------------------------------------------
Parameters  : value    Lower 90%  Upper 90%
kT [keV]    : 7.21353  (-0.574664  0.615573)
R^2/D10^2   : 0.587964  (-0.17162   0.24866)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          56.78 using 59 PHA bins.
# Reduced chi-squared =         0.9961 for     57 degrees of freedom 
# Null hypothesis probability =   4.834610e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  5.673e-07   7.375e-08
25- 50  8.229e-07   8.008e-08
50-150  1.518e-07   4.419e-08
15-150  1.542e-06   1.428e-07

Thermal bremsstrahlung (OTTB)

XSPEC12>exit
 XSPEC: quit
 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 29.0919       (-4.76541      6.04229)
Norm        : 2.96246       (-0.477585     0.595217)
------------------------------------------------------------
 Reduced chi-squared = 
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  6.645e-07   6.938e-08
25- 50  7.464e-07   7.067e-08
50-150  3.924e-07   1.094e-07
15-150  1.803e-06   1.730e-07

Double BB

XSPEC12>exit
 XSPEC: quit
 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 3.66305        (-1.61037      1.93458)
R1^2/D10^2  : 5.53610        (-4.33      133.902)
kT2 [keV]   : 9.38921        (-1.62059      4.48229)
R2^2/D10^2  : 0.150096    (-0.132763   0.195298)
------------------------------------------------------------
 Reduced chi-squared = 
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  6.566e-07   3.387e-07
25- 50  7.688e-07   4.004e-07
50-150  2.903e-07   1.735e-07
15-150  1.716e-06   8.463e-07

Peak spectrum fit

Power-law model

Time interval is from    0.000 sec. to  112.000 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 2.56845     ( -0.169721   0.180145 )
Norm@50keV  : 1.77479E-03    ( -0.000229712   0.000230001 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          53.23 using 59 PHA bins.
# Reduced chi-squared =         0.9339 for     57 degrees of freedom 
# Null hypothesis probability =   6.171700e-01
 
Photon flux (15-150 keV)    in 112 sec: 0.363801 ( -0.0272992  0.027304 ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.02655e-06 ( -1.84539e-07  1.89801e-07 ) ergs/cm2

Cutoff power-law model

Time interval is from    0.000 sec. to  112.000 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.04711     ( -1.15938   0.710631 )
Epeak [keV] : 21.3365      ( -19.4181 6.1907 )
Norm@50keV  : 1.68810E-02    ( -0.016881   0.0804194 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          44.80 using 59 PHA bins.
# Reduced chi-squared =         0.8000 for     56 degrees of freedom 
# Null hypothesis probability =   8.586819e-01
 
Photon flux (15-150 keV)    in 112 sec: 0.344409 ( -0.028714  0.028982 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.76783e-06 ( -1.83019e-07  2.1233e-07 ) ergs/cm2

Band function

Time interval is from    0.000 sec. to  112.000 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -1.08166   ( -0.914342   0.78036 )
beta        : -9.37167    ( 9.37167   19.3716 )
Epeak [keV] : 21.1153      ( -4.45041 6.41066 )
Norm@50keV   : 1.59722E-02    ( -0.0159775   0.216739 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          44.80 using 59 PHA bins.
# Reduced chi-squared =         0.8146 for     55 degrees of freedom 
# Null hypothesis probability =   8.352578e-01
 
Photon flux (15-150 keV)    in 112 sec:  (    ) ph/cm2/s
Energy fluence (15-150 keV)             : 6.77139e-06 ( -6.7706e-06  -2.24458e-06 ) ergs/cm2

Single BB

 XSPEC: quit
 
 
Spectral model blackbody:
------------------------------------------------------------
Parameters  : value    Lower 90%  Upper 90%
kT [keV]    : 7.21353  (-0.574664  0.615573)
R^2/D10^2   : 0.587964  (-0.17162   0.24866)
(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  5.673e-07   6.283e-08
25- 50  8.229e-07   7.806e-08
50-150  1.518e-07   4.608e-08
15-150  1.542e-06   1.523e-07

Thermal bremsstrahlung (OTTB)

XSPEC12>exit
 XSPEC: quit
 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 29.0919       (-4.76541      6.04229)
Norm        : 2.96246       (-0.477585     0.595217)
------------------------------------------------------------
 Reduced chi-squared = 
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  6.645e-07   6.910e-08
25- 50  7.464e-07   7.577e-08
50-150  3.924e-07   1.130e-07
15-150  1.803e-06   1.848e-07

Double BB

XSPEC12>exit
 XSPEC: quit
 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 3.66305        (-1.61037      1.93458)
R1^2/D10^2  : 5.53610        (-4.33      133.902)
kT2 [keV]   : 9.38921        (-1.62059      4.48229)
R2^2/D10^2  : 0.150096    (-0.132763   0.195298)
------------------------------------------------------------
 Reduced chi-squared = 
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  6.566e-07   3.412e-07
25- 50  7.688e-07   4.021e-07
50-150  2.903e-07   1.692e-07
15-150  1.716e-06   8.725e-07

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: 2.56845     ( -0.169721   0.180145 )
Norm@50keV  : 1.77479E-03    ( -0.000229712   0.000230001 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          53.23 using 59 PHA bins.
# Reduced chi-squared =         0.9339 for     57 degrees of freedom 
# Null hypothesis probability =   6.171700e-01
 
Photon flux (15-150 keV)    in 112 sec: 0.363801 ( -0.0272992  0.027304 ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.02655e-06 ( -1.84539e-07  1.89801e-07 ) ergs/cm2

Cutoff power-law model

Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.04711     ( -1.15938   0.710631 )
Epeak [keV] : 21.3365      ( -19.4181 6.1907 )
Norm@50keV  : 1.68810E-02    ( -0.016881   0.0804194 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          44.80 using 59 PHA bins.
# Reduced chi-squared =         0.8000 for     56 degrees of freedom 
# Null hypothesis probability =   8.586819e-01
 
Photon flux (15-150 keV)    in 112 sec: 0.344409 ( -0.028714  0.028982 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.76783e-06 ( -1.83019e-07  2.1233e-07 ) ergs/cm2

Band function

 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -1.08166   ( -0.914342   0.78036 )
beta        : -9.37167    ( 9.37167   19.3716 )
Epeak [keV] : 21.1153      ( -4.45041 6.41066 )
Norm@50keV   : 1.59722E-02    ( -0.0159775   0.218312 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          44.80 using 59 PHA bins.
# Reduced chi-squared =         0.8146 for     55 degrees of freedom 
# Null hypothesis probability =   8.352578e-01
 
Photon flux (15-150 keV)    in 112 sec:  (    ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.95955e-06 ( -1.95877e-06  -2.7823e-07 ) ergs/cm2

S(25-50 keV) vs. S(50-100 keV) plot

S(25-50 keV)  = 6.76e-07
S(50-100 keV) = 4.56e-07

T90 vs. Hardness ratio plot

T90                                   = 112 sec.
Hardness ratio (energy fluence ratio) = 0.674556

Color vs. Color plot

Count Ratio  (25-50 keV) / (15-25 keV) = 0.848597
Count Ratio (50-100 keV) / (15-25 keV) = 0.159507

Mask shadow pattern

IMX = -1.830214404239196E-01, IMY = 4.241309234369235E-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:
-119.000000 -74.210000
-73.000000 65.576000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
326.1977  38.1276   38.9  36.0  121.5   0.5597   0.3   11.7	Cyg X-2                       
344.4404  24.3719    2.1  31.6   84.6   6.9525   5.5 ------	UNKNOWN                       
  1.0843  26.2167    3.4  21.5   58.8   3.1415   3.5 ------	UNKNOWN                       
300.5056  68.6933    2.7  43.0  174.5   6.7806   4.3 ------	UNKNOWN                       
 50.1438   9.5180    2.6  47.1  -27.2   8.2672   4.5 ------	UNKNOWN                       
 62.0944  13.7450    2.5  51.1  -42.8  25.5198   4.7 ------	UNKNOWN

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

Time interval of the image:
0.000000 112.000000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
326.1777  38.1865   22.3  36.0  121.6   0.4983   0.5    8.1	Cyg X-2                       
344.4371  24.3880    2.2  31.6   84.6   3.4528   5.2 ------	UNKNOWN                       
 25.0181  33.8503    3.2  13.9  -15.5   1.3084   3.6 ------	UNKNOWN                       
 47.6053  59.7652    1.3  24.8 -113.3   4.2602   9.0 ------	UNKNOWN                       
 50.1437   9.5161    2.4  47.1  -27.2   3.8139   4.8 ------	UNKNOWN                       
 60.5862  44.8334    2.9  32.4  -81.4   2.6923   4.0 ------	UNKNOWN                       
 66.6053  28.2337    2.3  44.4  -61.1   9.1994   5.0 ------	UNKNOWN

Post-slew image of 15-350 keV band

Time interval of the image:
184.000620 416.820000
418.000000 475.990000
477.000000 513.700000
515.000000 572.440000
574.000000 582.181300
583.000000 603.070800
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
 83.5625  22.1508    5.7  45.3  -54.4   6.8517   2.0    9.1	Crab                          
 14.3210  30.0858    3.0  37.2   47.3   6.1871   3.9 ------	UNKNOWN                       
 47.8927  59.8426    0.6   0.1 -128.7  14.9324  19.2 ------	UNKNOWN                       
179.0894  78.5811    2.4  38.6 -170.9   5.7933   4.9 ------	UNKNOWN

Plot creation:
Fri Jul 21 11:59:31 EDT 2023