batgrbproduct analysis for trigger=706052

batgrbproduct Analysis for Trigger=706052

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 Aug 22 15:49:26 EDT 2016
             Host Name: bat1
   Current Working Dir: /local/data/bat1/alien/Swift_3rdBATcatalog/event/batevent_reproc/trigger706052
======================================================================

  Trigger: 00706052      Segment: 000

  BAT Trigger Time: 491189664.288   [s; MET]
      Trigger Stop: 491189664.32   [s; MET]
               UTC: 2016-07-26T01:34:07.673500    [includes UTCF correction] 
       Where From?: (*SHORT BURST*) TDRSS scaled map message

  BAT 
    RA: 98.8207862266102   Dec: -6.64457301434871  [deg; J2000]

     Catalogged Source?: NO
     Point Source?:      YES
     GRB Indicated?:     YES    [ by BAT flight software ]
     Image S/N Ratio:    7.6
     Image Trigger?:     NO
     Rate S/N Ratio:     24.2899156029822  [ if not an image trigger ]
     Image S/N Ratio:    7.6

  Flight Position:   [ source = BAT ]
    RA: 98.8207862266102   Dec: -6.64457301434871  [deg; J2000]

  Ground Position:   [ source = BAT pre-slew burst ]
    RA: 98.8097713403672   Dec: -6.61705628207127  [deg; J2000]  
        { 06h 35m 14.3s , -06d 37' 01.4" }
         +/- 1.28567004748997 [arcmin] (estimated 90% radius based on SNR)
         +/- 0.400102829777201 [arcmin] (formal 1-sigma fit error)
    SNR: 21.2431569048477
 
  Angular difference between Flight and Ground position is 1.776730 arcmin
 
  Partial Coding Fraction: 0.5859375    [ including projection effects ]

  Duration
     T90: 0.727999925613403 +/- 0.0430813282857434
        Measured from: 0.0160000324249268
                   to: 0.74399995803833     [s; relative to TRIGTIME]
     T50: 0.179999947547913 +/- 0.168760170863201
        Measured from: 0.495999991893768
                   to: 0.675999939441681     [s; relative to TRIGTIME]



  Fluence
     Peak Flux  (peak 1 second)
        Measured from: -0.103999972343445     
                   to: 0.896000027656555     [s; relative to TRIGTIME]
     Total Fluence        
        Measured from: 0.00400000810623169     
                   to: 0.787999987602234     [s; relative to TRIGTIME]
     
             Band 1     Band 2     Band 3     Band 4
              15-25      25-50     50-100    100-350     keV
 Total     0.070635   0.125319   0.133469   0.053616
           0.008490   0.010123   0.009806   0.007128 [error]
 Peak      0.075867   0.131073   0.138061   0.052557
           0.009349   0.010854   0.010349   0.007611 [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 2.39e-08 5.50e-08 9.96e-08 4.31e-07 2.71e-07 6.10e-07   erg/cm2
              Error 3.70e-09 5.14e-09 9.20e-09 8.87e-08 2.37e-08 9.41e-08   erg/cm2
Peak flux Power-law 8.21e-01 1.00e+00 8.89e-01 1.36e+00 3.19e+00 4.07e+00   ph/cm2/s
              Error 1.32e-01 9.92e-02 8.25e-02 2.64e-01 2.73e-01 3.53e-01   ph/cm2/s
 
Fluence   Cutoff-PL 2.30e-08 5.57e-08 1.02e-07 3.40e-07 2.70e-07 5.21e-07   erg/cm2
              Error 4.10e-09 5.68e-09 1.08e-08 1.37e-07 2.43e-08 1.42e-07   erg/cm2
Peak flux Cutoff-PL 7.59e-01 1.03e+00 9.26e-01 9.87e-01 3.15e+00 3.70e+00   ph/cm2/s
              Error 1.61e-01 1.08e-01 1.02e-01 4.19e-01 2.79e-01 5.32e-01   ph/cm2/s
 
Fluence        Band 2.39e-08 5.50e-08 9.96e-08 4.31e-07 2.71e-07 6.10e-07   erg/cm2
              Error 3.70e-09 5.14e-09 9.20e-09 8.87e-08 2.37e-08 9.41e-08   erg/cm2
Peak flux      Band 7.88e-01 1.06e+00 9.72e-01 1.06e+00 3.30e+00 3.81e+00   ph/cm2/s
              Error 7.55e-02 9.48e-02 7.79e-02 3.91e-01 2.67e-01 3.28e-01   ph/cm2/s

 
=== Time-averaged spectral analysis ===
 
Model Ph_index Ph_90err Epeak  Epeak_90err Norm     Nomr_90err chi2   dof
PL    1.138    0.137    -      -           3.35e-02 2.69e-03   57.990 57
CPL   0.961    0.389     333.1    0.0      4.04e-02 1.89e-02   57.600 56
 
 
=== 1-s peak spectral analysis ===
 
Model Ph_index Ph_90err Epeak  Epeak_90err Norm     Nomr_90err chi2   dof
PL    1.175    0.140    -      -           2.72e-02 2.25e-03   63.030 57
CPL   0.851    0.486     200.5    0.0      3.83e-02 2.16e-02   61.900 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: 0.704000 sec.
T50 in the 50-300 keV band: 0.128000 sec.

 
=== Table of the duration information ==
 
        Value   tstart    tstop
T100    0.784    0.004    0.788
T90     0.728    0.016    0.744
T50     0.180    0.496    0.676
Peak    1.000   -0.104    0.896

Click here for the BAT GCN circular template

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

Image

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

#   RAcent    DECcent   POSerr    Theta     Phi              Peak Cts       SNR   Name
   98.8098    -6.6171   0.0091    38.0763   -26.0833         0.3905527     21.243 TRIG_00706052                 
 
Foreground time interval of the image:
  0.004   0.788 (delta_t =   0.784 [sec])
Background time interval of the image:
-239.288   0.004 (delta_t = 239.292 [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 0.032000

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 0.032000

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 0.032000

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    0.004 sec. to    0.788 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.13810     ( -0.137543   0.135857 )
Norm@50keV  : 3.35173E-02    ( -0.00268748   0.002685 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          57.99 using 59 PHA bins.
# Reduced chi-squared =          1.017 for     57 degrees of freedom 
# Null hypothesis probability =   4.387337e-01
 
Photon flux (15-150 keV)    in 0.784 sec: 3.90340 ( -0.32275  0.32317 ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.71516e-07 ( -2.36681e-08  2.37786e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from    0.004 sec. to    0.788 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 0.960741     ( -0.531645   0.246724 )
Epeak [keV] : 333.080      ( -333.08 -333.08 )
Norm@50keV  : 4.04008E-02    ( -0.0091464   0.0286824 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          57.60 using 59 PHA bins.
# Reduced chi-squared =          1.029 for     56 degrees of freedom 
# Null hypothesis probability =   4.158373e-01
 
Photon flux (15-150 keV)    in 0.784 sec: 3.88145 ( -0.32833  0.32848 ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.69828e-07 ( -2.44043e-08  2.42865e-08 ) ergs/cm2

Band function

Time interval is from    0.004 sec. to    0.788 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : 4.30134   ( -4.30249   -4.30249 )
beta        : -1.17505    ( -0.154586   0.150989 )
Epeak [keV] : 25.3866      ( -25.3842 182.269 )
Norm@50keV   : 716.470    ( -717.084   281.395 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          57.22 using 59 PHA bins.
# Reduced chi-squared =          1.040 for     55 degrees of freedom 
# Null hypothesis probability =   3.925977e-01
 
Photon flux (15-150 keV)    in 0.784 sec: 4.26293 ( -0.69251  -0.06698 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.19059e-13 ( 0  0 ) ergs/cm2

Single BB

 
Spectral model blackbody:
------------------------------------------------------------
Parameters  : value    Lower 90%  Upper 90%
kT [keV]    : 20.9750  (-2.28562  2.63624)
R^2/D10^2   : 0.157631  (-0.0499065   0.0715043)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          92.03 using 59 PHA bins.
# Reduced chi-squared =          1.615 for     57 degrees of freedom 
# Null hypothesis probability =   2.261568e-03
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.028e-08   1.725e-09
25- 50  5.279e-08   6.515e-09
50-150  1.731e-07   2.411e-08
15-150  2.361e-07   2.681e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 200.000       (-15.8512      -200)
Norm        : 16.1060       (-1.3272     1.3272)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          83.20 using 59 PHA bins.
# Reduced chi-squared =          1.460 for     57 degrees of freedom 
# Null hypothesis probability =   1.337668e-02
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  3.145e-08   3.132e-09
25- 50  6.050e-08   9.643e-09
50-150  1.327e-07   5.408e-08
15-150  2.246e-07   7.127e-08

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 7.41809        (-1.77075      2.3095)
R1^2/D10^2  : 2.63487        (-1.52216      4.16813)
kT2 [keV]   : 32.6190        (-6.06567      11.2476)
R2^2/D10^2  : 3.31107E-02    (-0.0199322   0.0321337)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          55.33 using 59 PHA bins.
# Reduced chi-squared =          1.006 for     55 degrees of freedom 
# Null hypothesis probability =   4.622073e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  2.342e-08   1.115e-08
25- 50  5.565e-08   2.056e-08
50-150  1.951e-07   6.660e-08
15-150  2.742e-07   8.197e-08

Peak spectrum fit

Power-law model

Time interval is from   -0.104 sec. to    0.896 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.17500     ( -0.140989   0.139434 )
Norm@50keV  : 2.72276E-02    ( -0.00225133   0.00224993 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          63.03 using 59 PHA bins.
# Reduced chi-squared =          1.106 for     57 degrees of freedom 
# Null hypothesis probability =   2.715878e-01
 
Photon flux (15-150 keV)    in 1 sec: 3.18519 ( -0.27267  0.27311 ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.78253e-07 ( -2.49269e-08  2.50523e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from   -0.104 sec. to    0.896 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 0.850843     ( -0.58184   0.391086 )
Epeak [keV] : 200.510      ( -200.51 -200.51 )
Norm@50keV  : 3.83119E-02    ( -0.012652   0.0305909 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          61.90 using 59 PHA bins.
# Reduced chi-squared =          1.105 for     56 degrees of freedom 
# Null hypothesis probability =   2.736216e-01
 
Photon flux (15-150 keV)    in 1 sec: 3.14952 ( -0.27895  0.27909 ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.74897e-07 ( -2.59425e-08  2.58006e-08 ) ergs/cm2

Band function

Time interval is from   -0.104 sec. to    0.896 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -0.866799   ( -0.287476   0.242749 )
beta        : -9.37167    ( 9.37167   19.3717 )
Epeak [keV] : 209.437      ( -70.9352 -209.34 )
Norm@50keV   : 3.76270E-02    ( -0.0077681   0.0106114 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          61.91 using 59 PHA bins.
# Reduced chi-squared =          1.126 for     55 degrees of freedom 
# Null hypothesis probability =   2.432424e-01
 
Photon flux (15-150 keV)    in 1 sec: 3.29510 ( -0.40901  0.12512 ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.78234e-07 ( -2.29521e-08  2.50503e-08 ) ergs/cm2

Single BB

 
Spectral model blackbody:
------------------------------------------------------------
Parameters  : value    Lower 90%  Upper 90%
kT [keV]    : 20.2472  (-2.16084  2.49389)
R^2/D10^2   : 0.143566  (-0.0453264   0.0644845)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          89.26 using 59 PHA bins.
# Reduced chi-squared =          1.566 for     57 degrees of freedom 
# Null hypothesis probability =   4.056505e-03
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.129e-08   1.810e-09
25- 50  5.669e-08   7.640e-09
50-150  1.726e-07   2.355e-08
15-150  2.406e-07   2.440e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 200.000       (-17.7305      -200)
Norm        : 13.2293       (-1.11939     1.11939)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          82.51 using 59 PHA bins.
# Reduced chi-squared =          1.448 for     57 degrees of freedom 
# Null hypothesis probability =   1.520436e-02
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  3.293e-08   3.395e-09
25- 50  6.336e-08   1.146e-08
50-150  1.390e-07   5.584e-08
15-150  2.352e-07   6.910e-08

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 7.25476        (-2.08088      2.83966)
R1^2/D10^2  : 2.20239        (-1.4106      4.95238)
kT2 [keV]   : 29.8196        (-5.54672      10.9585)
R2^2/D10^2  : 3.50431E-02    (-0.022605   0.0361603)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          60.96 using 59 PHA bins.
# Reduced chi-squared =          1.108 for     55 degrees of freedom 
# Null hypothesis probability =   2.701649e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  2.419e-08   1.139e-08
25- 50  5.840e-08   2.041e-08
50-150  1.949e-07   8.193e-08
15-150  2.775e-07   8.480e-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: 1.13810     ( -0.137543   0.135857 )
Norm@50keV  : 3.35173E-02    ( -0.00268748   0.002685 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          57.99 using 59 PHA bins.
# Reduced chi-squared =          1.017 for     57 degrees of freedom 
# Null hypothesis probability =   4.387337e-01
 
Photon flux (15-150 keV)    in 0.784 sec: 3.90337 ( -0.322721  0.323186 ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.71494e-07 ( -2.37044e-08  2.37741e-08 ) ergs/cm2

Cutoff power-law model

Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 0.960741     ( -0.531645   0.246724 )
Epeak [keV] : 333.079      ( -333.079 -333.079 )
Norm@50keV  : 4.04008E-02    ( -0.00914641   0.0286824 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          57.60 using 59 PHA bins.
# Reduced chi-squared =          1.029 for     56 degrees of freedom 
# Null hypothesis probability =   4.158373e-01
 
Photon flux (15-150 keV)    in 0.784 sec: 3.88120 ( -0.32828  0.3284 ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.6995e-07 ( -2.44208e-08  2.42977e-08 ) ergs/cm2

Band function

 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : 4.30134   ( -4.30249   -4.30249 )
beta        : -1.17505    ( -0.154586   0.150989 )
Epeak [keV] : 25.3866      ( -25.3842 182.269 )
Norm@50keV   : 716.470    ( -717.084   281.395 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          57.22 using 59 PHA bins.
# Reduced chi-squared =          1.040 for     55 degrees of freedom 
# Null hypothesis probability =   3.925977e-01
 
Photon flux (15-150 keV)    in 0.784 sec: 4.26293 ( -0.69251  -0.06698 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.19059e-13 ( 0  0 ) ergs/cm2

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

S(25-50 keV)  = 5.50e-08
S(50-100 keV) = 9.96e-08

T90 vs. Hardness ratio plot

T90                                   = 0.727999925613403 sec.
Hardness ratio (energy fluence ratio) = 1.81091

Color vs. Color plot

Count Ratio  (25-50 keV) / (15-25 keV) = 1.77418
Count Ratio (50-100 keV) / (15-25 keV) = 1.88956

Mask shadow pattern

IMX = 7.036455956279711E-01, IMY = 3.444578927201825E-01

TIME vs. PHA plot around the trigger time

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.032000

TIME vs. DetID plot around the trigger time

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.032000

100 us light curve (15-350 keV)

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.032000

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:
-239.288000 0.004000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
 83.6261  22.0179    0.2  10.7  -77.0   9.8473  48.0    0.4	Crab                          
 39.1429  35.9405    2.2  32.4  144.6   1.6249   5.2 ------	UNKNOWN                       
 19.5494  67.9833    3.3  56.9  179.3   4.3130   3.5 ------	UNKNOWN                       
100.1169  61.6554    2.7  44.9 -141.6   2.1659   4.3 ------	UNKNOWN                       
116.9649   3.4875    3.7  46.9  -54.2   3.3593   3.1 ------	UNKNOWN

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

Time interval of the image:
0.004000 0.788000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
 83.6459  21.8643    5.7  10.7  -76.2   0.0260   2.0    9.0	Crab                          
 70.1698 -25.9052    2.4  47.0   22.6   0.1473   4.7 ------	UNKNOWN                       
 98.8098  -6.6170    0.5  38.1  -26.1   0.3906  21.3 ------	UNKNOWN                       
104.3029  17.7719    2.7  30.4  -69.3   0.0858   4.2 ------	UNKNOWN

Post-slew image of 15-350 keV band

Time interval of the image:
188.412600 456.012590
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
135.5442 -40.5596    1.1  23.0 -103.7   3.0344  11.0    0.8	Vela X-1                      
170.5139 -60.6896    4.3   8.0   32.6   0.6325   2.7    7.1	Cen X-3                       
186.6796 -62.7655    0.6  15.4   46.9   4.4230  19.2    0.7	GX 301-2                      
204.7187 -33.9688    2.8  41.8    8.5   1.4776   4.1 ------	UNKNOWN                       
199.7751 -17.2419    2.9  54.1   -8.0   2.7123   4.0 ------	UNKNOWN                       
172.7465 -10.3283    2.7  52.1  -42.0   5.5706   4.3 ------	UNKNOWN

Plot creation:
Mon Aug 22 16:25:16 EDT 2016