batgrbproduct analysis for trigger=1227767

batgrbproduct Analysis for Trigger=1227767

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 v2.48
    Process Start Time (local time): Sun May 12 20:30:28 EDT 2024
             Host Name: batproc1
   Current Working Dir: /local/data/bat1/prebascript/trigger1227767/GCN5_download_cron
======================================================================

  Trigger: 01227767      Segment: 000

  BAT Trigger Time: 737143646.656   [s; MET]
      Trigger Stop: 737143648.704   [s; MET]
               UTC: 2024-05-11T18:06:53.226840    [includes UTCF correction] 
       Where From?: TDRSS position message

  BAT 
    RA: 336.664509948977   Dec: 8.51351293746527  [deg; J2000]

     Catalogged Source?: NO
     Point Source?:      YES
     GRB Indicated?:     YES    [ by BAT flight software ]
     Image S/N Ratio:    8.52
     Image Trigger?:     NO
     Rate S/N Ratio:     14.8996644257513  [ if not an image trigger ]
     Image S/N Ratio:    8.52

  Flight Position:   [ source = BAT ]
    RA: 336.664509948977   Dec: 8.51351293746527  [deg; J2000]

  Ground Position:   [ source = BAT pre-slew burst ]
    RA: 336.668521076857   Dec: 8.51416525750696  [deg; J2000]  
        { 22h 26m 40.4s , +08d 30' 51.0" }
         +/- 0.689232651612834 [arcmin] (estimated 90% radius based on SNR)
         +/- 0.235260275407324 [arcmin] (formal 1-sigma fit error)
    SNR: 51.7635815640006
 
  Angular difference between Flight and Ground position is 0.241212 arcmin
 
  Partial Coding Fraction: 0.8515625    [ including projection effects ]

  Duration
     T90: 148.536000013351 +/- 17.0657857031545
        Measured from: -44.8279999494553
                   to: 103.708000063896     [s; relative to TRIGTIME]
     T50: 59.9880000352859 +/- 2.39597334507173
        Measured from: -15.095999956131
                   to: 44.892000079155     [s; relative to TRIGTIME]



  Fluence
     Peak Flux  (peak 1 second)
        Measured from: 35.1480000019073     
                   to: 36.1480000019073     [s; relative to TRIGTIME]
     Total Fluence        
        Measured from: -92.0119999647141     
                   to: 203.703999996185     [s; relative to TRIGTIME]
     
             Band 1     Band 2     Band 3     Band 4
              15-25      25-50     50-100    100-350     keV
 Total     4.891166   6.502661   4.679380   1.151685
           0.099978   0.104191   0.089568   0.072790 [error]
 Peak      0.074694   0.123857   0.094247   0.022257
           0.007559   0.008561   0.007527   0.005405 [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 1.55e-06 2.72e-06 3.64e-06 9.92e-06 1.06e-05 1.78e-05   erg/cm2
              Error 7.04e-08 7.03e-08 9.61e-08 6.13e-07 2.36e-07 6.55e-07   erg/cm2
Peak flux Power-law 8.11e-01 8.47e-01 6.26e-01 7.46e-01 2.57e+00 3.03e+00   ph/cm2/s
              Error 1.09e-01 7.11e-02 5.99e-02 1.45e-01 2.03e-01 2.39e-01   ph/cm2/s
 
Fluence   Cutoff-PL 1.48e-06 2.74e-06 3.69e-06 7.87e-06 1.04e-05 1.58e-05   erg/cm2
              Error 9.36e-08 7.46e-08 1.09e-07 1.70e-06 2.65e-07 1.72e-06   erg/cm2
Peak flux Cutoff-PL 7.81e-01 8.66e-01 6.40e-01 5.78e-01 2.55e+00 2.86e+00   ph/cm2/s
              Error 1.26e-01 8.45e-02 6.84e-02 2.33e-01 2.07e-01 3.23e-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    1.582    0.042    -      -           4.39e-03 9.56e-05   42.730 57
CPL   1.403    0.171     185.6 1222.7      5.29e-03 9.17e-04   39.450 56
 
 
=== 1-s peak spectral analysis ===
 
Model Ph_index Ph_90err Epeak  Epeak_90err Norm     Nomr_90err chi2   dof
PL    1.437    0.131    -      -           2.09e-02 1.64e-03   60.620 57
CPL   1.220    0.421     182.9    0.0      2.69e-02 1.56e-02   60.090 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: 104.064000 sec.
T50 in the 50-300 keV band: 52.544000 sec.

 
=== Table of the duration information ==
 
        Value   tstart    tstop
T100  295.716  -92.012  203.704
T90   148.536  -44.828  103.708
T50    59.988  -15.096   44.892
Peak    1.000   35.148   36.148

Click here for the BAT GCN circular template

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

Special notes of this burst

Image

Pre-slew 15.0-350.0 keV image (Event data)

#   RAcent    DECcent   POSerr    Theta     Phi              Peak Cts       SNR   Name
  336.6685     8.5142   0.0037    28.3846  -173.5370         9.1260616     51.764 TRIG_01227767                 
 
Foreground time interval of the image:
-92.012 -13.852 (delta_t =  78.160 [sec])
-12.656 -12.426 (delta_t =   0.230 [sec])
-11.656 -11.546 (delta_t =   0.110 [sec])
-10.656   8.174 (delta_t =  18.830 [sec])
 21.344  24.845 (delta_t =   3.501 [sec])
Background time interval of the image:
-239.656 -92.012 (delta_t = 147.644 [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

Multiple GTIs in the spectrum
tstart tstop
-92.012000 -13.851700
-12.656000 -12.426000
-11.656000 -11.546000
-10.656000 8.174000
21.344000 155.994000
157.344000 157.454000
158.344000 158.584000
159.344000 159.924000
180.344000 203.704000
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.58165     ( -0.042186   0.0421925 )
Norm@50keV  : 4.39358E-03    ( -9.55954e-05   9.55953e-05 )
------------------------------------------------------------
#Fit statistic  : Chi-Squared                   42.73     using 59 bins.
 Reduced chi-squared = 0.749649
# Null hypothesis probability of 9.20e-01 with 57 degrees of freedom
 
Photon flux (15-150 keV)    in 256.3 sec: 0.561451 ( -0.014184  0.014242 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.05569e-05 ( -2.36259e-07  2.36214e-07 ) ergs/cm2

Cutoff power-law model

Multiple GTIs in the spectrum
tstart tstop
-92.012000 -13.851700
-12.656000 -12.426000
-11.656000 -11.546000
-10.656000 8.174000
21.344000 155.994000
157.344000 157.454000
158.344000 158.584000
159.344000 159.924000
180.344000 203.704000
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.40316     ( -0.17447   0.167626 )
Epeak [keV] : 185.591      ( -64.74 2380.65 )
Norm@50keV  : 5.28886E-03    ( -0.000811855   0.00102247 )
------------------------------------------------------------
#Fit statistic  : Chi-Squared                   39.45     using 59 bins.
 Reduced chi-squared = 0.704464
# Null hypothesis probability of 9.54e-01 with 56 degrees of freedom
 
Photon flux (15-150 keV)    in 256.3 sec: 0.552947 ( -0.01607  0.01617 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.04287e-05 ( -2.65278e-07  2.64309e-07 ) ergs/cm2

Band function

Multiple GTIs in the spectrum
tstart tstop
-92.012000 -13.851700
-12.656000 -12.426000
-11.656000 -11.546000
-10.656000 8.174000
21.344000 155.994000
157.344000 157.454000
158.344000 158.584000
159.344000 159.924000
180.344000 203.704000
 
 
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]    : 16.3244  (  )
R^2/D10^2   : 4.41784E-02  (   )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic  : Chi-Squared                  466.77     using 59 bins.
 Reduced chi-squared = 
# Null hypothesis probability of 1.15e-65 with 57 degrees of freedom
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  6.210e-07   2.947e-08
25- 50  2.658e-06   8.073e-08
50-150  4.988e-06   1.986e-07
15-150  8.267e-06   2.050e-07

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 200.000       (-16.1176      -200)
Norm        : 2.25628       (-0.0490902     0.0490902)
------------------------------------------------------------
#Fit statistic  : Chi-Squared                   41.62     using 59 bins.
 Reduced chi-squared = 
# Null hypothesis probability of 9.37e-01 with 57 degrees of freedom
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.441e-06   3.985e-08
25- 50  2.771e-06   7.048e-08
50-150  6.077e-06   1.538e-07
15-150  1.029e-05   2.512e-07

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 8.21513        (-0.640255      0.662153)
R1^2/D10^2  : 0.339655        (-0.0758764      0.106487)
kT2 [keV]   : 30.2956        (-2.76697      3.59306)
R2^2/D10^2  : 3.86417E-03    (-0.00124943   0.00160783)
------------------------------------------------------------
#Fit statistic  : Chi-Squared                   46.36     using 59 bins.
 Reduced chi-squared = 
# Null hypothesis probability of 7.90e-01 with 55 degrees of freedom
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.224e-06   9.214e-08
25- 50  2.859e-06   1.320e-07
50-150  6.222e-06   4.447e-07
15-150  1.030e-05   5.805e-07

Peak spectrum fit

Power-law model

Time interval is from   35.148 sec. to   36.148 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.43659     ( -0.130348   0.13097 )
Norm@50keV  : 2.09284E-02    ( -0.00163986   0.00163574 )
------------------------------------------------------------
#Fit statistic  : Chi-Squared                   60.62     using 59 bins.
 Reduced chi-squared = 1.06351
# Null hypothesis probability of 3.47e-01 with 57 degrees of freedom
 
Photon flux (15-150 keV)    in 1 sec: 2.57072 ( -0.20277  0.20296 ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.00798e-07 ( -1.72372e-08  1.73444e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from   35.148 sec. to   36.148 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.22001     ( -0.554746   0.287691 )
Epeak [keV] : 182.912      ( -182.933 -182.933 )
Norm@50keV  : 2.69440E-02    ( -0.00741363   0.0237355 )
------------------------------------------------------------
#Fit statistic  : Chi-Squared                   60.09     using 59 bins.
 Reduced chi-squared = 1.07304
# Null hypothesis probability of 3.30e-01 with 56 degrees of freedom
 
Photon flux (15-150 keV)    in 1 sec: 2.55294 ( -0.20712  0.20704 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.98089e-07 ( -1.86363e-08  1.8437e-08 ) ergs/cm2

Band function

Time interval is from   35.148 sec. to   36.148 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]    : 15.2901  (-1.49136  1.68526)
R^2/D10^2   : 0.279037  (-0.0857059   0.120619)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic  : Chi-Squared                   99.34     using 59 bins.
 Reduced chi-squared = 
# Null hypothesis probability of 4.40e-04 with 57 degrees of freedom
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.361e-08   2.065e-09
25- 50  5.504e-08   5.370e-09
50-150  8.831e-08   1.411e-08
15-150  1.570e-07   1.550e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 200.000       (-35.4724      -200)
Norm        : 10.6170       (-0.81861     0.81861)
------------------------------------------------------------
#Fit statistic  : Chi-Squared                   62.32     using 59 bins.
 Reduced chi-squared = 
# Null hypothesis probability of 2.93e-01 with 57 degrees of freedom
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  2.644e-08   2.360e-09
25- 50  5.086e-08   5.640e-09
50-150  1.116e-07   3.783e-08
15-150  1.889e-07   5.128e-08

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 8.56309        (-2.04468      2.34577)
R1^2/D10^2  : 1.44722        (-0.725943      1.71891)
kT2 [keV]   : 35.0054        (-10.9992      52.5391)
R2^2/D10^2  : 1.22581E-02    (-0.0109099   0.0285083)
------------------------------------------------------------
#Fit statistic  : Chi-Squared                   59.67     using 59 bins.
 Reduced chi-squared = 
# Null hypothesis probability of 3.10e-01 with 55 degrees of freedom
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  2.222e-08   6.165e-09
25- 50  5.334e-08   1.327e-08
50-150  1.244e-07   5.799e-08
15-150  2.000e-07   7.355e-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: 1.38736     ( -0.0464571   0.0463426 )
Norm@50keV  : 6.28078E-03    ( -0.000155386   0.000155344 )
------------------------------------------------------------
#Fit statistic  : Chi-Squared                   40.67     using 59 bins.
 Reduced chi-squared = 
# Null hypothesis probability of 9.50e-01 with 57 degrees of freedom
 
Photon flux (15-150 keV)    in 100.8 sec: 0.762717 ( -0.021116  0.0211816 ) ph/cm2/s
Energy fluence (15-150 keV)             : 6.13348e-06 ( -1.57227e-07  1.57354e-07 ) ergs/cm2

Cutoff power-law model

Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.20065     ( -0.188224   0.175004 )
Epeak [keV] : 244.667      ( -93.9355 2719.8 )
Norm@50keV  : 7.59438E-03    ( -0.00124952   0.00155321 )
------------------------------------------------------------
#Fit statistic  : Chi-Squared                   37.57     using 59 bins.
 Reduced chi-squared = 
# Null hypothesis probability of 9.72e-01 with 56 degrees of freedom
 
Photon flux (15-150 keV)    in 100.8 sec: 0.752346 ( -0.023124  0.023221 ) ph/cm2/s
Energy fluence (15-150 keV)             : 6.07159e-06 ( -1.70342e-07  1.69445e-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)  = 2.72e-06
S(50-100 keV) = 3.64e-06

T90 vs. Hardness ratio plot

T90                                   = 148.536000013351 sec.
Hardness ratio (energy fluence ratio) = 1.33824

Color vs. Color plot

Count Ratio  (25-50 keV) / (15-25 keV) = 1.32947
Count Ratio (50-100 keV) / (15-25 keV) = 0.9567

Mask shadow pattern

IMX = -5.369171108225050E-01, IMY = 6.082231970598598E-02

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:
-239.656000 -92.012000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
309.7853 -32.6420    4.3  32.1   77.4   1.0743   2.7 ------	UNKNOWN                       
331.7526  29.0190    2.5  49.4 -173.8   2.2340   4.6 ------	UNKNOWN                       
349.1950  26.9756    2.1  46.7 -153.2   2.2087   5.5 ------	UNKNOWN

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

Time interval of the image:
-92.012000 -13.851700
-12.656000 -12.426000
-11.656000 -11.546000
-10.656000 8.174000
21.344000 24.844590
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
336.6685   8.5142    0.2  28.4 -173.5   9.1261  51.8 ------	UNKNOWN

Post-slew image of 15-350 keV band

Time interval of the image:
91.044580 155.994000
157.344000 157.454000
158.344000 158.584000
159.344000 159.924000
180.344000 232.454000
233.344000 327.594000
328.344000 647.330200
660.344000 712.104000
720.344000 758.434000
765.344000 773.984000
780.344000 799.153200
800.344000 809.964000
817.344000 822.834000
829.344000 846.004000
849.344000 863.764000
866.344000 866.814000
868.344000 882.554000
884.344000 962.416100
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
299.5934  35.1950    1.2  43.1  150.4  27.1416   9.5    0.4	Cyg X-1                       
308.0864  40.9302    3.4  41.1  163.2   6.3680   3.4    1.7	Cyg X-3                       
326.2560  38.5072    0.0  31.4 -179.2  -2.4647  -2.1   11.8	Cyg X-2                       
308.7583  -7.4394    3.8  32.1   77.5   6.1289   3.0 ------	UNKNOWN                       
 11.5511   8.9950    2.5  34.5  -77.0   8.3959   4.6 ------	UNKNOWN                       
 18.5808   8.1630    2.2  41.4  -76.2  18.9880   5.2 ------	UNKNOWN

Plot creation:
Sat Nov 16 18:13:22 EST 2024