batgrbproduct analysis for trigger=301981

batgrbproduct Analysis for Trigger=301981

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 v2.46
    Process Start Time (local time): Mon Jan 20 04:59:14 EST 2014
             Host Name: batevent1
   Current Working Dir: /local/data/batevent/batevent_reproc/trigger301981
======================================================================

  Trigger: 00301981      Segment: 000

  BAT Trigger Time: 223279608   [s; MET]
      Trigger Stop: 223279672   [s; MET]
               UTC: 2008-01-29T06:06:45.464120    [includes UTCF correction] 
       Where From?: TDRSS position message

  BAT 
    RA: 105.280011758568   Dec: -7.82688688603851  [deg; J2000]

     Catalogged Source?: NO
     Point Source?:      YES
     GRB Indicated?:     YES    [ by BAT flight software ]
     Image S/N Ratio:    7.51
     Image Trigger?:     YES
     Rate S/N Ratio:     0  [ if not an image trigger ]
     Image S/N Ratio:    7.51

  Flight Position:   [ source = BAT ]
    RA: 105.280011758568   Dec: -7.82688688603851  [deg; J2000]

  Ground Position:   [ source = BAT pre-slew burst ]
    RA: 105.287918693116   Dec: -7.84878702628647  [deg; J2000]  
        { 07h 01m 09.1s , -07d 50' 55.6" }
         +/- 2.0979526670691 [arcmin] (estimated 90% radius based on SNR)
         +/- 1.08096063871601 [arcmin] (formal 1-sigma fit error)
    SNR: 10.5538339688152
 
  Angular difference between Flight and Ground position is 1.395530 arcmin
 
  Partial Coding Fraction: 0.46875    [ including projection effects ]

  Duration
     T90: 50.1800000071526 +/- 9.16545032804407
        Measured from: -1.44400000572205
                   to: 48.7360000014305     [s; relative to TRIGTIME]
     T50: 25.8240000009537 +/- 8.11501521505903
        Measured from: 8.5
                   to: 34.3240000009537     [s; relative to TRIGTIME]



  Fluence
     Peak Flux  (peak 1 second)
        Measured from: 27.0119999945164     
                   to: 28.0119999945164     [s; relative to TRIGTIME]
     Total Fluence        
        Measured from: -3.45600000023842     
                   to: 52.4320000112057     [s; relative to TRIGTIME]
     
             Band 1     Band 2     Band 3     Band 4
              15-25      25-50     50-100    100-350     keV
 Total     0.245843   0.448381   0.393414   0.088385
           0.060115   0.062663   0.054931   0.046762 [error]
 Peak      0.000221   0.031510   0.022339   0.011426
           0.008306   0.008451   0.007610   0.006220 [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-08 1.83e-07 3.05e-07 1.15e-06 8.39e-07 1.72e-06   erg/cm2
              Error 2.54e-08 3.22e-08 5.13e-08 4.43e-07 1.31e-07 4.69e-07   erg/cm2
Peak flux Power-law 1.24e-01 1.66e-01 1.63e-01 2.89e-01 5.48e-01 7.43e-01   ph/cm2/s
              Error 9.37e-02 7.89e-02 5.56e-02 2.19e-01 2.05e-01 2.52e-01   ph/cm2/s
 
Fluence   Cutoff-PL 8.67e-08 1.84e-07 3.05e-07 1.14e-06 8.39e-07 1.71e-06   erg/cm2
              Error 2.52e-08 3.38e-08 5.39e-08 8.22e-07 9.85e-08 5.32e-07   erg/cm2
Peak flux Cutoff-PL 1.13e-01 1.70e-01 1.71e-01 2.06e-01 5.42e-01 6.59e-01   ph/cm2/s
              Error 1.14e-01 8.67e-02 7.02e-02 2.78e-01 2.07e-01 3.06e-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    1.268    0.261    -      -           1.51e-03 2.22e-04   52.570 57
CPL   1.269    0.263    9999.4    0.0      1.51e-03 1.52e-03   52.570 56
 
 
=== 1-s peak spectral analysis ===
 
Model Ph_index Ph_90err Epeak  Epeak_90err Norm     Nomr_90err chi2   dof
PL    1.023    0.629    -      -           4.75e-03 1.74e-03   58.680 57
CPL   3.168    0.000     216.5    0.0      2.38e-09 0.00e+00   58.400 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: 58.752000 sec.
T50 in the 50-300 keV band: 26.176000 sec.

 
=== Table of the duration information ==
 
        Value   tstart    tstop
T100   55.888   -3.456   52.432
T90    50.180   -1.444   48.736
T50    25.824    8.500   34.324
Peak    1.000   27.012   28.012

Click here for the BAT GCN circular template

Image

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

#   RAcent    DECcent   POSerr    Theta     Phi              Peak Cts       SNR   Name
  105.2879    -7.8488   0.0182    41.5279   176.7982         1.3076689     10.554 TRIG_00301981                 
 
Foreground time interval of the image:
 -3.456  52.432 (delta_t =  55.888 [sec])
Background time interval of the image:
-355.699 -264.950 (delta_t =  90.749 [sec])
-239.000  -3.456 (delta_t = 235.544 [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

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 64.000000

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 64.000000

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 64.000000

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

Time interval is from   -3.456 sec. to   52.432 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.26839     ( -0.266422   0.256252 )
Norm@50keV  : 1.50713E-03    ( -0.000221911   0.000221558 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          52.57 using 59 PHA bins.
# Reduced chi-squared =         0.9223 for     57 degrees of freedom 
# Null hypothesis probability =   6.418104e-01
 
Photon flux (15-150 keV)    in 55.89 sec: 0.178799 ( -0.0280672  0.028225 ) ph/cm2/s
Energy fluence (15-150 keV)             : 8.38982e-07 ( -1.30077e-07  1.30968e-07 ) ergs/cm2

Cutoff power-law model

Time interval is from   -3.456 sec. to   52.432 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.26882     ( -0.271355   0.255092 )
Epeak [keV] : 9999.36      ( -9999.36 -9999.36 )
Norm@50keV  : 1.51277E-03    ( -0.000221751   0.0028215 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          52.57 using 59 PHA bins.
# Reduced chi-squared =         0.9388 for     56 degrees of freedom 
# Null hypothesis probability =   6.053569e-01
 
Photon flux (15-150 keV)    in 55.89 sec: 0.178956 ( -0.02833  0.027866 ) ph/cm2/s
Energy fluence (15-150 keV)             : 8.38842e-07 ( -6.6878e-08  1.30196e-07 ) ergs/cm2

Band function

Time interval is from   -3.456 sec. to   52.432 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : 5.18489E-02   ( 0.297423   0.297423 )
beta        : -1.38065    ( 1.36743   0.338048 )
Epeak [keV] : 53.6609      ( -52.9983 256.963 )
Norm@50keV   : 9.95909E-03    ( -0.01164   68.2602 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          51.98 using 59 PHA bins.
# Reduced chi-squared =         0.9452 for     55 degrees of freedom 
# Null hypothesis probability =   5.905659e-01
 
Photon flux (15-150 keV)    in 55.89 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]    : 17.8492  (-3.35954  4.55883)
R^2/D10^2   : 1.15996E-02  (-0.00624754   0.0122783)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          64.64 using 59 PHA bins.
# Reduced chi-squared =          1.134 for     57 degrees of freedom 
# Null hypothesis probability =   2.271975e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  4.146e-08   1.202e-08
25- 50  1.906e-07   4.759e-08
50-150  4.397e-07   1.308e-07
15-150  6.717e-07   1.495e-07

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 200.000       (      )
Norm        : 0.756931       (-0.112641     0.112616)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          56.41 using 59 PHA bins.
# Reduced chi-squared =         0.9897 for     57 degrees of freedom 
# Null hypothesis probability =   4.970690e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.054e-07   5.991e-08
25- 50  2.028e-07   1.121e-07
50-150  4.447e-07   2.485e-07
15-150  7.528e-07   4.264e-07

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 11.4372        (-3.65352      2.61713)
R1^2/D10^2  : 4.33016E-02        (-0.0236239      0.0958474)
kT2 [keV]   : 199.227        (-160.487      -199.281)
R2^2/D10^2  : 2.61256E-05    (-8.36613e-06   0.00126593)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          50.05 using 59 PHA bins.
# Reduced chi-squared =         0.9100 for     55 degrees of freedom 
# Null hypothesis probability =   6.638822e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  6.846e-08   3.471e-08
25- 50  2.137e-07   9.935e-08
50-150  5.367e-07   1.871e-07
15-150  8.188e-07   2.871e-07

Peak spectrum fit

Power-law model

Time interval is from   27.012 sec. to   28.012 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.02299     ( -0.687446   0.569715 )
Norm@50keV  : 4.75369E-03    ( -0.00179388   0.00168954 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          58.68 using 59 PHA bins.
# Reduced chi-squared =          1.030 for     57 degrees of freedom 
# Null hypothesis probability =   4.135409e-01
 
Photon flux (15-150 keV)    in 1 sec: 0.547983 ( -0.202575  0.208272 ) ph/cm2/s
Energy fluence (15-150 keV)             : 5.09921e-08 ( -1.72787e-08  1.73415e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from   27.012 sec. to   28.012 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 3.16763     (     )
Epeak [keV] : 216.489      (   )
Norm@50keV  : 2.37627E-09    (     )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          58.40 using 59 PHA bins.
# Reduced chi-squared =          1.043 for     56 degrees of freedom 
# Null hypothesis probability =   3.871859e-01
 
Photon flux (15-150 keV)    in 1 sec: 0.541947 ( -0.203409  0.210826 ) ph/cm2/s
Energy fluence (15-150 keV)             : 5.04463e-08 ( -9.4626e-09  1.76947e-08 ) ergs/cm2

Band function

Time interval is from   27.012 sec. to   28.012 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : 5.00000   ( -4.94535   -4.94535 )
beta        : -1.34395    ( -1.55927   0.862043 )
Epeak [keV] : 40.9406      ( -40.9408 26.8508 )
Norm@50keV   : 20.9390    ( -6.84543   1.82034e+06 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          57.74 using 59 PHA bins.
# Reduced chi-squared =          1.050 for     55 degrees of freedom 
# Null hypothesis probability =   3.743159e-01
 
Photon flux (15-150 keV)    in 1 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]    : 21.6273  (-7.79111  18.3206)
R^2/D10^2   : 2.07631E-02  (-0.0207092   0.0720597)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          59.91 using 59 PHA bins.
# Reduced chi-squared =          1.051 for     57 degrees of freedom 
# Null hypothesis probability =   3.706718e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.811e-09   1.188e-09
25- 50  9.480e-09   5.895e-09
50-150  3.311e-08   2.159e-08
15-150  4.440e-08   2.837e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 199.361       (-101.893      -199.363)
Norm        : 2.40338       (-0.844471     0.844522)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          61.09 using 59 PHA bins.
# Reduced chi-squared =          1.072 for     57 degrees of freedom 
# Null hypothesis probability =   3.314139e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  5.985e-09   3.828e-09
25- 50  1.151e-08   6.915e-09
50-150  2.525e-08   1.559e-08
15-150  4.275e-08   2.728e-08

Double BB

R1^2/D10^2  : 7.46681E-02        (      )
kT2 [keV]   : 199.363        (-199.363      -199.363)
R2^2/D10^2  : 8.59245E-05    (-8.68374e-05   0.0383313)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          59.57 using 59 PHA bins.
#Fit statistic : Chi-Squared =          57.65 using 59 PHA bins.
#Fit statistic : Chi-Squared =          57.63 using 59 PHA bins.
# Reduced chi-squared =          1.083 for     55 degrees of freedom 
# Reduced chi-squared =          1.048 for     55 degrees of freedom 
# Reduced chi-squared =          1.048 for     55 degrees of freedom 
# Null hypothesis probability =   3.128812e-01
# Null hypothesis probability =   3.775075e-01
# Null hypothesis probability =   3.780934e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  2.494e-09   1.179e-09
25- 50  9.258e-09   5.700e-09
50-150  3.324e-08   2.135e-08
15-150  4.499e-08   2.875e-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: 1.26839     ( -0.266422   0.256252 )
Norm@50keV  : 1.50713E-03    ( -0.000221911   0.000221558 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          52.57 using 59 PHA bins.
# Reduced chi-squared =         0.9223 for     57 degrees of freedom 
# Null hypothesis probability =   6.418104e-01
 
Photon flux (15-150 keV)    in 55.89 sec: 0.178799 ( -0.0280672  0.028225 ) ph/cm2/s
Energy fluence (15-150 keV)             : 8.38982e-07 ( -1.30077e-07  1.30968e-07 ) ergs/cm2

Cutoff power-law model

Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.26882     ( -0.271355   0.255092 )
Epeak [keV] : 9999.36      ( -9999.36 -9999.36 )
Norm@50keV  : 1.51277E-03    ( -0.000221751   0.0028215 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          52.57 using 59 PHA bins.
# Reduced chi-squared =         0.9388 for     56 degrees of freedom 
# Null hypothesis probability =   6.053569e-01
 
Photon flux (15-150 keV)    in 55.89 sec: 0.178956 ( -0.02833  0.027866 ) ph/cm2/s
Energy fluence (15-150 keV)             : 8.38842e-07 ( -6.6878e-08  1.30196e-07 ) ergs/cm2

Band function

 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : 5.18489E-02   ( 0.297423   0.297423 )
beta        : -1.38065    ( 1.36743   0.338048 )
Epeak [keV] : 53.6609      ( -52.9983 257.178 )
Norm@50keV   : 9.95909E-03    ( -0.01164   68.2602 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          51.98 using 59 PHA bins.
# Reduced chi-squared =         0.9452 for     55 degrees of freedom 
# Null hypothesis probability =   5.905659e-01
 
Photon flux (15-150 keV)    in 55.89 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)  = 1.83e-07
S(50-100 keV) = 3.05e-07

T90 vs. Hardness ratio plot

T90                                   = 50.1800000071526 sec.
Hardness ratio (energy fluence ratio) = 1.66667

Color vs. Color plot

Count Ratio  (25-50 keV) / (15-25 keV) = 1.82385
Count Ratio (50-100 keV) / (15-25 keV) = 1.60027

Mask shadow pattern

IMX = -8.842114871837599E-01, IMY = -4.946245927239137E-02

TIME vs. PHA plot around the trigger time

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 64.000000

TIME vs. DetID plot around the trigger time

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 64.000000

100 us light curve (15-350 keV)

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 64.000000

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:
-355.699400 -264.950000
-239.000000 -3.456000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
 83.6300  22.0086    0.3  28.7 -120.5  13.5991  44.6    0.4	Crab                          
125.7051 -10.9129    2.4  45.3  147.5   2.9097   4.9 ------	UNKNOWN                       
187.6852  60.9734    3.5  54.0   19.3   4.7035   3.3 ------	UNKNOWN                       
187.4862  71.6039    2.2  53.9    6.1   4.5239   5.2 ------	UNKNOWN                       
143.5859  64.7696    2.8  36.7    4.9   1.2708   4.2 ------	UNKNOWN                       
100.0023 -22.5409    3.3  57.0  179.3   5.1239   3.5 ------	UNKNOWN                       
102.6388 -12.6533    2.4  46.8  179.1   1.9923   4.8 ------	UNKNOWN                       
106.5517  21.9371    2.0  12.7 -163.9   1.1947   5.7 ------	UNKNOWN                       
 99.8636   6.2452    2.7  29.6 -167.0   0.9927   4.2 ------	UNKNOWN                       
 67.4852  86.5330    2.9  54.8  -19.0   3.0073   4.0 ------	UNKNOWN                       
 11.4319  83.8638    3.1  58.6  -22.9   5.4207   3.7 ------	UNKNOWN

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

Time interval of the image:
-3.456000 52.432000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
 83.4771  21.9852    4.9  28.9 -120.4   0.2316   2.3    8.9	Crab                          
180.1025  51.8281    2.5  50.6   31.2   1.6927   4.7 ------	UNKNOWN                       
132.9909  48.4697    2.9  21.2   21.2   0.3004   4.0 ------	UNKNOWN                       
105.2879  -7.8488    1.1  41.5  176.8   1.3074  10.6 ------	UNKNOWN                       
 88.4594  -9.5723    2.4  48.8 -161.9   0.8114   4.9 ------	UNKNOWN

Post-slew image of 15-350 keV band

Time interval of the image:
404.200600 963.120000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
147.4353  33.2376    3.4  37.7   82.8   3.2002   3.4 ------	UNKNOWN                       
290.9053  88.5164    2.4  23.1 -131.7   1.3903   4.8 ------	UNKNOWN                       
268.2673  56.0982    2.5  41.2  -77.6   6.6444   4.7 ------	UNKNOWN

Plot creation:
Sun May 31 08:28:27 EDT 2015