batgrbproduct analysis for trigger=555163

batgrbproduct Analysis for Trigger=555163

Analysis Summary

Notes:

1) No attempt has been made to eliminate the non-significant decimal places.
2) This is a special analysis for ground-detected GRB. The event data duration is likely to be shorter than the burst duration. In such cases, the burst durations are found using the quad-rate data, and spectral analyses are only available for event data range.
3) Some mask-weighted light curve plots might be missing because the time range is not completely covered by the event data range.

Special note:

Due to the low partial coding fraction of this burst, the light curves and burst durations are created using the special DETECTION mask aperture. However, the spectral analysis is done using the default FLUX aperture for more accurate results, and thus the spectral analysis is only available after T+23.572 s (met=389434982.484000 s; see figure below), when the burst came into the BAT calibrated field of view.

FLUX-mask-weighted light curve (pcodethresh=0.05; aperture=CALDB:FLUX)

======================================================================
                  BAT GRB EVENT DATA PROCESSING REPORT
    Process Script Ver: batgrbproduct v2.46
    Process Start Time: Thu Dec 17 15:12:42 EST 2015
             Host Name: bat1
   Current Working Dir: /local/data/bat1/alien/Swift_3rdBATcatalog/event/batevent_reproc/trigger555163
======================================================================

  Trigger: 00555163      Segment: 000

  BAT Trigger Time: 389434958.912   [s; MET]
      Trigger Stop: 389434959.936   [s; MET]
               UTC: 2013-05-05T08:22:28.392980    [includes UTCF correction] 
       Where From?: TDRSS position message

  BAT 
    RA: 137.059762477099   Dec: 17.4850913390281  [deg; J2000]

     Catalogged Source?: NO
     Point Source?:      YES
     GRB Indicated?:     YES    [ by BAT flight software ]
     Image S/N Ratio:    6.59
     Image Trigger?:     NO
     Rate S/N Ratio:     255.998046867549  [ if not an image trigger ]
     Image S/N Ratio:    6.59

  Analysis Position:   [ source = BAT ]
    RA: 137.059762477099   Dec: 17.4850913390281  [deg; J2000]

  Refined Position:   [ source = BAT pre-slew burst ]
    RA: 137.06   Dec: 17.4851  [deg; J2000]
        { 09h 08m 14.4s , +17d 29' 06.4" }
        +/- 1.63568103017 [arcmin] (estimated 90% radius based on SNR)
    SNR: 15.062305751
 
  Angular difference between the GCN position (ra=137.059762477099, dec=17.4850913390281 deg) and this refined position is 0.003 arcmin
 
  Partial Coding Fraction: 0.02636719    [ including projection effects ]

  Duration
     T90: 89.3440000414848 +/- 111.154229439193
        Measured from: -1.14399999380112
                   to: 88.2000000476837     [s; relative to TRIGTIME]
     T50: 13.1840000152588 +/- 2.45682072392117
        Measured from: 0.680000007152557
                   to: 13.8640000224113     [s; relative to TRIGTIME]


======================================================================

=== 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 5.84e-07 9.42e-07 1.15e-06 2.75e-06 3.46e-06 5.42e-06   erg/cm2
              Error 6.91e-08 6.76e-08 1.20e-07 6.10e-07 2.78e-07 7.08e-07   erg/cm2
Peak flux Power-law -------- -------- -------- -------- -------- --------   ph/cm2/s
              Error -------- -------- -------- -------- -------- --------   ph/cm2/s
 
Fluence   Cutoff-PL 5.82e-07 9.43e-07 1.15e-06 2.72e-06 3.44e-06 5.21e-06   erg/cm2
              Error 6.89e-08 6.66e-08 1.19e-07 7.14e-07 2.75e-07 9.57e-07   erg/cm2
Peak flux Cutoff-PL -------- -------- -------- -------- -------- --------   ph/cm2/s
              Error -------- -------- -------- -------- -------- --------   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    1.714    0.133    -      -           1.10e-03 8.35e-05   42.830 57
CPL   1.719    0.155    9999.4   -0.0      1.09e-03 2.62e-04   42.850 56
 
 
(1-s peak is outside the event data range; spectral analysis not available)
 
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

 
=== Table of the duration information ==
 
        Value   tstart    tstop
T100  366.288   -3.032  363.256
T90    89.344   -1.144   88.200
T50    13.184    0.680   13.864
Peak    1.000    1.436    2.436

Click here for the BAT GCN circular template

Special notes of this burst

Image

15.0-350.0 keV image (Event data with DETECTION mask)

#RAcent DECcent POSerr Theta  Phi  Peak_Cts  SNR Name
137.060 17.485 0.000 59.438 -175.872 21.937 15.062 TRIG_00555163
 
Foreground time interval of the image: -3.032 to 13.789 [sec]
Background time interval of the image: -239.912 to -3.032 [sec]

Lightcurves

Notes:

1) The mask-weighted lightcurves have units of either count/det or counts/sec/det, where a det is 0.4 x 0.4 = 0.16 sq cm.
2) 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 (for the best duration plot, slew times are marked by green arrows).
3) For lightcurves in unit of count rate, 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)

Quad-rate summed light curves (from T0-300s to T0+1000s)

Spectral Evolution

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 an average DRM

Power-law model

Time interval is from   23.572 sec. to  364.776 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.71416     ( -0.131849   0.134148 )
Norm@50keV  : 1.09581E-03    ( -8.39691e-05   8.30581e-05 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          42.83 using 59 PHA bins.
# Reduced chi-squared =         0.7514 for     57 degrees of freedom 
# Null hypothesis probability =   9.181458e-01
 
Photon flux (15-150 keV)    in 341.2 sec: 0.146263 ( -0.0105626  0.0105901 ) ph/cm2/s
Energy fluence (15-150 keV)             : 3.45806e-06 ( -2.76915e-07  2.791e-07 ) ergs/cm2

Cutoff power-law model

Time interval is from   23.572 sec. to  364.776 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.71925     ( -0.178759   0.130482 )
Epeak [keV] : 9999.36      ( -9999.35 -9999.36 )
Norm@50keV  : 1.09359E-03    ( -8.33595e-05   0.000441148 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          42.85 using 59 PHA bins.
# Reduced chi-squared =         0.7651 for     56 degrees of freedom 
# Null hypothesis probability =   9.017789e-01
 
Photon flux (15-150 keV)    in 341.2 sec: 0.146458 ( -0.010769  0.010377 ) ph/cm2/s
Energy fluence (15-150 keV)             : 3.44424e-06 ( -2.64399e-07  2.85857e-07 ) ergs/cm2

Band function

Time interval is from   23.572 sec. to  364.776 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -1.28486   ( 1.27978   1.27978 )
beta        : -1.72115    ( 1.72126   0.138199 )
Epeak [keV] : 38.1296      ( -37.518 -37.518 )
Norm@50keV   : 2.36889E-03    ( -0.0011983   225870 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          42.80 using 59 PHA bins.
# Reduced chi-squared =         0.7781 for     55 degrees of freedom 
# Null hypothesis probability =   8.845549e-01
 
Photon flux (15-150 keV)    in 341.2 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]    : 12.6769  (  )
R^2/D10^2   : 2.77314E-02  (   )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =         115.16 using 59 PHA bins.
# Reduced chi-squared =         2.0203 for     57 degrees of freedom 
# Null hypothesis probability =   8.181320e-06
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  3.225e-07   4.371e-08
25- 50  1.081e-06   9.639e-08
50-150  1.081e-06   1.726e-07
15-150  2.484e-06   2.269e-07

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 143.568       (-43.5457      -142.404)
Norm        : 0.596462       (-0.0496613     0.0336728)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          47.47 using 59 PHA bins.
# Reduced chi-squared =         0.8328 for     57 degrees of freedom 
# Null hypothesis probability =   8.118014e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  5.246e-07   5.289e-08
25- 50  9.660e-07   1.320e-07
50-150  1.872e-06   7.140e-07
15-150  3.362e-06   8.318e-07

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 6.11655        (-1.08513      1.26655)
R1^2/D10^2  : 0.303698        (-0.150691      0.344689)
kT2 [keV]   : 26.9274        (-5.49463      9.98221)
R2^2/D10^2  : 1.50556E-03    (-0.000970081   0.00189349)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          44.12 using 59 PHA bins.
# Reduced chi-squared =         0.8022 for     55 degrees of freedom 
# Null hypothesis probability =   8.531427e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  5.914e-07   1.499e-07
25- 50  9.157e-07   1.754e-07
50-150  1.991e-06   7.136e-07
15-150  3.498e-06   8.182e-07

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

S(25-50 keV)  = 9.42e-07
S(50-100 keV) = 1.15e-06

T90 vs. Hardness ratio plot

T90                                   = 89.3440000414848 sec.
Hardness ratio (energy fluence ratio) = 1.22081

Color vs. Color plot

Count Ratio  (25-50 keV) / (15-25 keV) = 1.06704
Count Ratio (50-100 keV) / (15-25 keV) = 0.757932

Mask shadow pattern (with DETECTION mask)

IMX = -1.68907355441, IMY = 0.121915813671

TIME vs. PHA plot around the beginning of event data (event_start to event_start+0.64s) with DETECTION mask

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.024000

TIME vs. DetID plot around the beginning of event data (event_start to event_start+0.64s) with DETECTION mask

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.024000

100 us light curve (15-350 keV; (event_start to event_start+0.64s)

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.024000

Spacecraft aspect plot

Bright source in the event data image

Event data image of 15-350 keV band

Time interval of the image:
-3.032000 13.788590
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
254.4215  35.4725    4.0  44.2   28.3   0.4711   2.9    8.0	Her X-1                       
167.2322   9.1216    2.8  54.8  148.0   5.6520   4.1 ------	UNKNOWN                       
232.4735  62.9561    3.5  17.7   -5.0   0.2674   3.3 ------	UNKNOWN                       
137.0417  17.4809    0.7  59.5 -175.9  23.4004  16.1 ------	UNKNOWN                       
131.2273  35.3489    3.1  47.6 -157.9   0.6429   3.7 ------	UNKNOWN                       
341.5679  68.7920    2.4  49.4  -52.0   2.0840   4.7 ------	UNKNOWN

Webpage updated on:
Tue Jan 12 00:18:13 EST 2016