batgrbproduct analysis for trigger=665268

batgrbproduct Analysis for Trigger=665268

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): Sun Dec 13 15:47:51 EST 2015
             Host Name: bat1
   Current Working Dir: /local/data/bat1/alien/Swift_3rdBATcatalog/event/batevent_reproc/trigger665268
======================================================================

  Trigger: 00665268      Segment: 000

  BAT Trigger Time: 470308145.28   [s; MET]
      Trigger Stop: 470308145.536   [s; MET]
               UTC: 2015-11-27T09:08:49.807240    [includes UTCF correction] 
       Where From?: TDRSS position message

  BAT 
    RA: 19.7778363516866   Dec: -82.773849221241  [deg; J2000]

     Catalogged Source?: NO
     Point Source?:      YES
     GRB Indicated?:     YES    [ by BAT flight software ]
     Image S/N Ratio:    6.86
     Image Trigger?:     NO
     Rate S/N Ratio:     12.5299640861417  [ if not an image trigger ]
     Image S/N Ratio:    6.86

  Flight Position:   [ source = BAT ]
    RA: 19.7778363516866   Dec: -82.773849221241  [deg; J2000]

  Ground Position:   [ source = BAT pre-slew burst ]
    RA: 19.6606456422828   Dec: -82.7616121566521  [deg; J2000]  
        { 01h 18m 38.6s , -82d 45' 41.8" }
         +/- 2.79318077851476 [arcmin] (estimated 90% radius based on SNR)
         +/- 1.34551489332188 [arcmin] (formal 1-sigma fit error)
    SNR: 7.01187282003185
 
  Angular difference between Flight and Ground position is 1.150073 arcmin
 
  Partial Coding Fraction: 0.9609375    [ including projection effects ]

  Duration
     T90: 0.187999904155731 +/- 0.042520585314364
        Measured from: 0.0240000486373901
                   to: 0.211999952793121     [s; relative to TRIGTIME]
     T50: 0.0959999561309814 +/- 0.042520585314364
        Measured from: 0.0760000348091125
                   to: 0.171999990940094     [s; relative to TRIGTIME]



  Fluence
     Peak Flux  (peak 1 second)
        Measured from: -0.379999995231628     
                   to: 0.620000004768372     [s; relative to TRIGTIME]
     Total Fluence        
        Measured from: 0.0160000324249268     
                   to: 0.220000028610229     [s; relative to TRIGTIME]
     
             Band 1     Band 2     Band 3     Band 4
              15-25      25-50     50-100    100-350     keV
 Total     0.006509   0.014960   0.016288   0.002608
           0.002752   0.003119   0.003042   0.002395 [error]
 Peak      0.007012   0.025647   0.015450   0.001306
           0.005877   0.006077   0.005501   0.004809 [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 2.37e-09 5.06e-09 8.45e-09 3.22e-08 2.33e-08 4.81e-08   erg/cm2
              Error 9.27e-10 1.32e-09 2.17e-09 1.64e-08 5.64e-09 1.80e-08   erg/cm2
Peak flux Power-law 8.79e-02 1.18e-01 1.16e-01 2.07e-01 3.90e-01 5.29e-01   ph/cm2/s
              Error 6.13e-02 5.14e-02 4.27e-02 1.78e-01 1.37e-01 1.98e-01   ph/cm2/s
 
Fluence   Cutoff-PL 1.78e-09 5.88e-09 1.02e-08 8.67e-09 2.31e-08 2.65e-08   erg/cm2
              Error 1.06e-09 1.68e-09 2.93e-09 1.35e-08 5.74e-09 1.42e-08   erg/cm2
Peak flux Cutoff-PL 8.70e-02 1.19e-01 1.17e-01 2.05e-01 3.89e-01 5.14e-01   ph/cm2/s
              Error 6.17e-02 6.81e-02 4.65e-02 1.55e-01 1.38e-01 2.29e-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    1.257    0.334    -      -           1.14e-02 2.66e-03   47.170 57
CPL  -0.184    1.625      84.4  163.8      5.45e-02 1.63e-01   43.860 56
 
 
=== 1-s peak spectral analysis ===
 
Model Ph_index Ph_90err Epeak  Epeak_90err Norm     Nomr_90err chi2   dof
PL    1.018    0.636    -      -           3.38e-03 1.17e-03   54.190 57
CPL   0.964    2.900     953.7    0.0      3.61e-03 1.68e+01   54.190 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    0.204    0.016    0.220
T90     0.188    0.024    0.212
T50     0.096    0.076    0.172
Peak    1.000   -0.380    0.620

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
   19.6606   -82.7616   0.0274    20.0095    -2.2689         0.0405565      7.012 TRIG_00665268                 
 
Foreground time interval of the image:
  0.016   0.220 (delta_t =   0.204 [sec])
Background time interval of the image:
-203.579   0.016 (delta_t = 203.595 [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 0.256000

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 0.256000

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 0.256000

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    0.016 sec. to    0.220 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.25691     ( -0.339758   0.327775 )
Norm@50keV  : 1.14104E-02    ( -0.00266162   0.00265882 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          47.17 using 59 PHA bins.
# Reduced chi-squared =         0.8276 for     57 degrees of freedom 
# Null hypothesis probability =   8.202085e-01
 
Photon flux (15-150 keV)    in 0.204 sec: 1.35117 ( -0.32696  0.32837 ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.32546e-08 ( -5.63317e-09  5.6469e-09 ) ergs/cm2

Cutoff power-law model

Time interval is from    0.016 sec. to    0.220 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: -0.184442     ( -1.88889   1.36026 )
Epeak [keV] : 84.4096      ( -23.6382 303.932 )
Norm@50keV  : 5.44938E-02    ( -0.0544866   0.27109 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          43.86 using 59 PHA bins.
# Reduced chi-squared =         0.7832 for     56 degrees of freedom 
# Null hypothesis probability =   8.806826e-01
 
Photon flux (15-150 keV)    in 0.204 sec: 1.34644 ( -0.32768  0.32937 ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.3143e-08 ( -5.73132e-09  5.74852e-09 ) ergs/cm2

Band function

Time interval is from    0.016 sec. to    0.220 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : 0.179035   ( -0.939039   2.64568 )
beta        : -10.0000    ( 10   3.55271e-15 )
Epeak [keV] : 84.4985      ( -22.319 163.208 )
Norm@50keV   : 5.42063E-02    ( -0.0542063   0.270792 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          43.86 using 59 PHA bins.
# Reduced chi-squared =         0.7974 for     55 degrees of freedom 
# Null hypothesis probability =   8.597643e-01
 
Photon flux (15-150 keV)    in 0.204 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]    : 19.2804  (-4.20111  5.17691)
R^2/D10^2   : 7.80300E-02  (-0.0443694   0.100415)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          45.19 using 59 PHA bins.
# Reduced chi-squared =         0.7929 for     57 degrees of freedom 
# Null hypothesis probability =   8.706078e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.157e-09   5.073e-10
25- 50  5.621e-09   2.516e-09
50-150  1.540e-08   6.572e-09
15-150  2.218e-08   8.309e-09

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 200.000       (-78.2346      -200)
Norm        : 5.75281       (-1.35424     1.35424)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          48.29 using 59 PHA bins.
# Reduced chi-squared =         0.8471 for     57 degrees of freedom 
# Null hypothesis probability =   7.877031e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  2.923e-09   1.763e-09
25- 50  5.622e-09   3.329e-09
50-150  1.233e-08   7.279e-09
15-150  2.087e-08   1.241e-08

Double BB

R1^2/D10^2  : 0.608268        (-0.632406      2.3986)
kT2 [keV]   : 23.4749        (-23.4586      -23.4586)
R2^2/D10^2  : 3.33036E-02    (-0.0335773   0.0848769)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          45.19 using 59 PHA bins.
#Fit statistic : Chi-Squared =          43.28 using 59 PHA bins.
#Fit statistic : Chi-Squared =          43.20 using 59 PHA bins.
# Reduced chi-squared =         0.8217 for     55 degrees of freedom 
# Reduced chi-squared =         0.7870 for     55 degrees of freedom 
# Reduced chi-squared =         0.7854 for     55 degrees of freedom 
# Null hypothesis probability =   8.244753e-01
# Null hypothesis probability =   8.735422e-01
# Null hypothesis probability =   8.755486e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  0.000e+00   0.000e+00
25- 50  0.000e+00   0.000e+00
50-150  0.000e+00   0.000e+00
15-150  0.000e+00   0.000e+00

Peak spectrum fit

Power-law model

Time interval is from   -0.380 sec. to    0.620 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.01810     ( -0.694368   0.57732 )
Norm@50keV  : 3.38101E-03    ( -0.00118241   0.00115818 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          54.19 using 59 PHA bins.
# Reduced chi-squared =         0.9507 for     57 degrees of freedom 
# Null hypothesis probability =   5.812403e-01
 
Photon flux (15-150 keV)    in 1 sec: 0.389650 ( -0.136437  0.137794 ) ph/cm2/s
Energy fluence (15-150 keV)             : 3.63329e-08 ( -1.31248e-08  1.34626e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from   -0.380 sec. to    0.620 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 0.964329     ( -6.51227   -0.712281 )
Epeak [keV] : 953.736      ( -968.882 -968.882 )
Norm@50keV  : 3.60803E-03    ( -0.00135698   33.5202 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          54.19 using 59 PHA bins.
# Reduced chi-squared =         0.9676 for     56 degrees of freedom 
# Null hypothesis probability =   5.437866e-01
 
Photon flux (15-150 keV)    in 1 sec: 0.389122 ( -0.137702  0.137945 ) ph/cm2/s
Energy fluence (15-150 keV)             : 3.61393e-08 ( -1.96254e-08  1.35485e-08 ) ergs/cm2

Band function

Time interval is from   -0.380 sec. to    0.620 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : 4.95652   ( -4.95652   -4.95652 )
beta        : -1.51669    ( -1.80092   0.872149 )
Epeak [keV] : 35.4131      ( -31.4563 17.649 )
Norm@50keV   : 37.5060    ( -12.1226   817651 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          51.99 using 59 PHA bins.
# Reduced chi-squared =         0.9453 for     55 degrees of freedom 
# Null hypothesis probability =   5.902681e-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]    : 15.2527  (-5.42052  18.9076)
R^2/D10^2   : 4.43291E-02  (-0.0439421   0.15987)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          55.91 using 59 PHA bins.
# Reduced chi-squared =         0.9810 for     57 degrees of freedom 
# Null hypothesis probability =   5.158422e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  2.153e-09   1.434e-09
25- 50  8.686e-09   5.450e-09
50-150  1.385e-08   9.500e-09
15-150  2.469e-08   1.582e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 199.361       (-112.628      -199.362)
Norm        : 1.60855       (-0.568639     0.568632)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          56.21 using 59 PHA bins.
# Reduced chi-squared =         0.9862 for     57 degrees of freedom 
# Null hypothesis probability =   5.045140e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  4.005e-09   2.547e-09
25- 50  7.705e-09   4.897e-09
50-150  1.690e-08   1.060e-08
15-150  2.861e-08   1.817e-08

Double BB

------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 10.4962        (-3.69767      6.0038)
R1^2/D10^2  : 0.128926        (-0.10782      0.391269)
kT2 [keV]   : 198.983        (-174.626      -199.113)
R2^2/D10^2  : 7.47647E-05    (-5.14489e-05   0.00672119)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          55.91 using 59 PHA bins.
#Fit statistic : Chi-Squared =          51.46 using 59 PHA bins.
# Reduced chi-squared =          1.017 for     55 degrees of freedom 
# Reduced chi-squared =         0.9356 for     55 degrees of freedom 
# Null hypothesis probability =   4.402852e-01
# Null hypothesis probability =   6.108256e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  0.000e+00   0.000e+00
25- 50  0.000e+00   0.000e+00
50-150  0.000e+00   0.000e+00
15-150  0.000e+00   0.000e+00

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: 1.25691     ( -0.339758   0.327775 )
Norm@50keV  : 1.14104E-02    ( -0.00266162   0.00265882 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          47.17 using 59 PHA bins.
# Reduced chi-squared =         0.8276 for     57 degrees of freedom 
# Null hypothesis probability =   8.202085e-01
 
Photon flux (15-150 keV)    in 0.204 sec: 1.35111 ( -0.32691  0.328398 ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.32521e-08 ( -5.63209e-09  5.65612e-09 ) ergs/cm2

Cutoff power-law model

Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: -0.184121     ( -1.88884   1.36033 )
Epeak [keV] : 84.4159      ( -23.638 304.038 )
Norm@50keV  : 5.44760E-02    ( -0.0544867   0.271105 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          43.86 using 59 PHA bins.
# Reduced chi-squared =         0.7832 for     56 degrees of freedom 
# Null hypothesis probability =   8.806826e-01
 
Photon flux (15-150 keV)    in 0.204 sec: 1.34640 ( -0.32766  0.32933 ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.3153e-08 ( -5.73389e-09  5.75137e-09 ) ergs/cm2

Band function

 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : 0.179035   ( -0.939039   2.64568 )
beta        : -10.0000    ( 10   7.10543e-15 )
Epeak [keV] : 84.4985      ( -22.319 163.211 )
Norm@50keV   : 5.42063E-02    ( -0.0542063   0.270792 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          43.86 using 59 PHA bins.
# Reduced chi-squared =         0.7974 for     55 degrees of freedom 
# Null hypothesis probability =   8.597643e-01
 
Photon flux (15-150 keV)    in 0.204 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)  = 5.06e-09
S(50-100 keV) = 8.45e-09

T90 vs. Hardness ratio plot

T90                                   = 0.187999904155731 sec.
Hardness ratio (energy fluence ratio) = 1.66996

Color vs. Color plot

Count Ratio  (25-50 keV) / (15-25 keV) = 2.29836
Count Ratio (50-100 keV) / (15-25 keV) = 2.50238

Mask shadow pattern

IMX = 3.638718056106555E-01, IMY = 1.441658461201686E-02

TIME vs. PHA plot around the trigger time

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.256000

TIME vs. DetID plot around the trigger time

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.256000

100 us light curve (15-350 keV)

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.256000

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:
-203.579410 0.016000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
135.5551 -40.6059    3.2  33.6  158.1   1.1350   3.6    3.3	Vela X-1                      
170.2996 -60.6235    1.6  18.5 -140.3   1.3286   7.0    0.5	Cen X-3                       
186.8384 -62.8406    4.1  20.9 -117.1   0.6206   2.8    6.5	GX 301-2                      
178.4973 -62.5154    2.8  18.9 -126.8   0.8535   4.1 ------	UNKNOWN                       
207.6417 -77.0289    3.2  16.9  -68.8   0.7556   3.7 ------	UNKNOWN                       
201.2977 -60.9540    2.5  26.4 -105.9   1.2090   4.6 ------	UNKNOWN                       
181.9710 -23.7274    3.2  56.0 -148.7   4.4104   3.7 ------	UNKNOWN                       
186.1118 -26.8173    2.9  53.9 -143.4   5.0088   4.0 ------	UNKNOWN                       
210.8132 -45.6014    2.8  42.5 -109.9   3.5411   4.1 ------	UNKNOWN                       
196.4193 -35.6798    2.7  48.0 -129.2   4.5444   4.3 ------	UNKNOWN

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

Time interval of the image:
0.016000 0.220000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
135.4424 -40.3948    4.4  33.8  157.9   0.0218   2.6   10.4	Vela X-1                      
170.6735 -60.7430    0.0  18.5 -139.6  -0.0063  -1.1   12.7	Cen X-3                       
186.3680 -62.8374    7.8  20.8 -117.6   0.0091   1.5    8.9	GX 301-2                      
 25.6561 -46.5731    2.5  50.6   35.1   0.1261   4.6 ------	UNKNOWN                       
 19.6603 -82.7615    1.6  20.0   -2.3   0.0405   7.0 ------	UNKNOWN                       
170.5801 -20.1961    2.3  57.2 -162.0   0.1309   5.1 ------	UNKNOWN

Post-slew image of 15-350 keV band

Time interval of the image:
57.820600 962.760000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
135.6446 -40.5690    3.7  52.9  169.7   7.2748   3.1    5.4	Vela X-1                      
170.3144 -60.5774    1.7  35.9 -155.6   5.8880   7.0    2.7	Cen X-3                       
186.3721 -62.8242    3.7  34.2 -142.1   2.4688   3.1    8.4	GX 301-2                      
 24.1365 -72.6115    2.6  10.2   56.1   2.5154   4.5 ------	UNKNOWN                       
 78.6394 -85.1540    2.9   6.3 -172.8   2.2179   4.0 ------	UNKNOWN                       
344.1703 -71.4784    2.9  13.3   -4.7   2.1454   4.0 ------	UNKNOWN                       
327.2915 -30.6638    2.9  55.1   -7.5   7.0212   3.9 ------	UNKNOWN                       
180.7007 -70.0255    2.6  26.9 -145.6   2.9512   4.4 ------	UNKNOWN                       
318.6399 -28.7925    3.5  57.9  -16.2   9.8095   3.3 ------	UNKNOWN                       
292.6058 -39.2397    3.9  50.8  -44.4  10.7020   3.0 ------	UNKNOWN                       
202.2818 -49.2261    3.0  48.0 -129.1  12.5855   3.8 ------	UNKNOWN

Plot creation:
Mon May  2 14:51:45 EDT 2016