batgrbproduct analysis for trigger=205851

batgrbproduct Analysis for Trigger=205851

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): Wed Jan 22 17:29:14 EST 2014
             Host Name: batevent1
   Current Working Dir: /local/data/batevent/batevent_reproc/trigger205851
======================================================================

  Trigger: 00205851      Segment: 000

  BAT Trigger Time: 167022369.344   [s; MET]
      Trigger Stop: 167022370.368   [s; MET]
               UTC: 2006-04-18T03:06:08.204500    [includes UTCF correction] 
       Where From?: TDRSS position message

  BAT 
    RA: 236.419948391906   Dec: -3.64343384352562  [deg; J2000]

     Catalogged Source?: NO
     Point Source?:      YES
     GRB Indicated?:     YES    [ by BAT flight software ]
     Image S/N Ratio:    10.8
     Image Trigger?:     NO
     Rate S/N Ratio:     28.9309522829789  [ if not an image trigger ]
     Image S/N Ratio:    10.8

  Flight Position:   [ source = BAT ]
    RA: 236.419948391906   Dec: -3.64343384352562  [deg; J2000]

  Ground Position:   [ source = BAT pre-slew burst ]
    RA: 236.430661828296   Dec: -3.63965249246618  [deg; J2000]  
        { 15h 45m 43.4s , -03d 38' 22.7" }
         +/- 0.969578605224568 [arcmin] (estimated 90% radius based on SNR)
         +/- 0.500532965683523 [arcmin] (formal 1-sigma fit error)
    SNR: 31.7896311502763
 
  Angular difference between Flight and Ground position is 0.680447 arcmin
 
  Partial Coding Fraction: 0.3046875    [ including projection effects ]

  Duration
     T90: 109.080000013113 +/- 46.7255162820641
        Measured from: -45.6200000047684
                   to: 63.4600000083447     [s; relative to TRIGTIME]
     T50: 25.4920000135899 +/- 0.68913860008981
        Measured from: 2.0799999833107
                   to: 27.5719999969006     [s; relative to TRIGTIME]



  Fluence
     Peak Flux  (peak 1 second)
        Measured from: 27.4519999921322     
                   to: 28.4519999921322     [s; relative to TRIGTIME]
     Total Fluence        
        Measured from: -82.4560000002384     
                   to: 136.619999974966     [s; relative to TRIGTIME]
     
             Band 1     Band 2     Band 3     Band 4
              15-25      25-50     50-100    100-350     keV
 Total     4.234725   5.224577   3.668461   0.930035
           0.127418   0.117749   0.102110   0.090026 [error]
 Peak      0.215832   0.289826   0.235451   0.053250
           0.012172   0.012617   0.011528   0.008156 [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 1.37e-06 2.26e-06 2.81e-06 6.97e-06 8.40e-06 1.34e-05   erg/cm2
              Error 7.71e-08 7.19e-08 1.07e-07 6.01e-07 2.52e-07 6.61e-07   erg/cm2
Peak flux Power-law 2.16e+00 2.18e+00 1.54e+00 1.73e+00 6.56e+00 7.61e+00   ph/cm2/s
              Error 1.95e-01 1.18e-01 9.48e-02 2.25e-01 3.34e-01 3.73e-01   ph/cm2/s
 
Fluence   Cutoff-PL 1.33e-06 2.28e-06 2.84e-06 5.79e-06 8.31e-06 1.22e-05   erg/cm2
              Error 9.90e-08 7.85e-08 1.14e-07 1.42e-06 2.90e-07 1.49e-06   erg/cm2
Peak flux Cutoff-PL 2.07e+00 2.21e+00 1.57e+00 1.41e+00 6.49e+00 7.26e+00   ph/cm2/s
              Error 2.44e-01 1.30e-01 1.08e-01 4.68e-01 3.55e-01 5.39e-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    1.681    0.056    -      -           4.13e-03 1.19e-04   59.350 57
CPL   1.553    0.194     182.8  -35.3      4.76e-03 1.00e-03   58.330 56
 
 
=== 1-s peak spectral analysis ===
 
Model Ph_index Ph_90err Epeak  Epeak_90err Norm     Nomr_90err chi2   dof
PL    1.498    0.089    -      -           5.26e-02 2.60e-03   54.680 57
CPL   1.313    0.296     195.0    0.0      6.46e-02 0.00e+00   53.800 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: 36.864000 sec.
T50 in the 50-300 keV band: 18.880000 sec.

 
=== Table of the duration information ==
 
        Value   tstart    tstop
T100  219.076  -82.456  136.620
T90   109.080  -45.620   63.460
T50    25.492    2.080   27.572
Peak    1.000   27.452   28.452

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
  236.4307    -3.6397   0.0060    31.2072    94.9614         7.9157465     31.790 TRIG_00205851                 
 
Foreground time interval of the image:
-82.456  11.957 (delta_t =  94.413 [sec])
Background time interval of the image:
-239.344 -82.456 (delta_t = 156.888 [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 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) 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  -82.456 sec. to  136.620 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.68100     ( -0.0563754   0.0565556 )
Norm@50keV  : 4.13366E-03    ( -0.000119507   0.00011936 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          59.35 using 59 PHA bins.
# Reduced chi-squared =          1.041 for     57 degrees of freedom 
# Null hypothesis probability =   3.898786e-01
 
Photon flux (15-150 keV)    in 219.1 sec: 0.545402 ( -0.0174575  0.0175305 ) ph/cm2/s
Energy fluence (15-150 keV)             : 8.39878e-06 ( -2.52254e-07  2.52721e-07 ) ergs/cm2

Cutoff power-law model

Time interval is from  -82.456 sec. to  136.620 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.55263     ( -0.225666   0.16272 )
Epeak [keV] : 182.819      ( -112.15 -182.827 )
Norm@50keV  : 4.75657E-03    ( -0.000708026   0.00129188 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          58.33 using 59 PHA bins.
# Reduced chi-squared =          1.042 for     56 degrees of freedom 
# Null hypothesis probability =   3.897251e-01
 
Photon flux (15-150 keV)    in 219.1 sec: 0.539536 ( -0.019799  0.009967 ) ph/cm2/s
Energy fluence (15-150 keV)             : 8.31401e-06 ( -2.92718e-07  2.87722e-07 ) ergs/cm2

Band function

Time interval is from  -82.456 sec. to  136.620 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -0.459672   ( -0.671746   -0.671746 )
beta        : -1.71811    ( 1.71423   0.0699246 )
Epeak [keV] : 36.7815      ( -36.7697 159.691 )
Norm@50keV   : 2.78506E-02    ( -0.0277998   477.106 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          57.14 using 59 PHA bins.
# Reduced chi-squared =          1.039 for     55 degrees of freedom 
# Null hypothesis probability =   3.956894e-01
 
Photon flux (15-150 keV)    in 219.1 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]    : 14.8131  (  )
R^2/D10^2   : 5.84565E-02  (   )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =         325.94 using 59 PHA bins.
# Reduced chi-squared =         5.7182 for     57 degrees of freedom 
# Null hypothesis probability =   2.382853e-39
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  5.896e-07   3.648e-08
25- 50  2.315e-06   8.107e-08
50-150  3.438e-06   1.906e-07
15-150  6.343e-06   2.005e-07

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 152.416       (      )
Norm        : 2.21033       (-0.0894358     0.0820329)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          62.32 using 59 PHA bins.
# Reduced chi-squared =          1.093 for     57 degrees of freedom 
# Null hypothesis probability =   2.926370e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.222e-06   6.913e-08
25- 50  2.286e-06   1.418e-07
50-150  4.629e-06   1.099e-06
15-150  8.137e-06   1.215e-06

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 6.82560        (-0.719845      0.803154)
R1^2/D10^2  : 0.658091        (-0.211527      0.336996)
kT2 [keV]   : 25.3870        (-2.56259      3.48902)
R2^2/D10^2  : 6.70222E-03    (-0.00251308   0.00331175)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          67.50 using 59 PHA bins.
# Reduced chi-squared =          1.227 for     55 degrees of freedom 
# Null hypothesis probability =   1.200838e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.214e-06   1.238e-07
25- 50  2.302e-06   1.528e-07
50-150  4.652e-06   4.031e-07
15-150  8.167e-06   4.941e-07

Peak spectrum fit

Power-law model

Time interval is from   27.452 sec. to   28.452 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.49841     ( -0.0885831   0.0891434 )
Norm@50keV  : 5.25714E-02    ( -0.00259986   0.00259292 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          54.68 using 59 PHA bins.
# Reduced chi-squared =         0.9593 for     57 degrees of freedom 
# Null hypothesis probability =   5.625071e-01
 
Photon flux (15-150 keV)    in 1 sec: 6.56017 ( -0.333336  0.333952 ) ph/cm2/s
Energy fluence (15-150 keV)             : 4.98849e-07 ( -2.68248e-08  2.69267e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from   27.452 sec. to   28.452 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.31253     ( -0.360116   0.231006 )
Epeak [keV] : 194.982      (   )
Norm@50keV  : 6.46111E-02    (     )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          53.80 using 59 PHA bins.
# Reduced chi-squared =         0.9608 for     56 degrees of freedom 
# Null hypothesis probability =   5.584751e-01
 
Photon flux (15-150 keV)    in 1 sec: 6.49121 ( -0.35452  0.35479 ) ph/cm2/s
Energy fluence (15-150 keV)             : 4.92983e-07 ( -2.9274e-08  2.9079e-08 ) ergs/cm2

Band function

Time interval is from   27.452 sec. to   28.452 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -1.28372   ( 1.28346   1.19725 )
beta        : -1.69764    ( 1.68588   0.258403 )
Epeak [keV] : 170.274      ( -170.848 -170.848 )
Norm@50keV   : 6.68932E-02    ( -0.0130801   4.9321 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          53.73 using 59 PHA bins.
# Reduced chi-squared =         0.9768 for     55 degrees of freedom 
# Null hypothesis probability =   5.234282e-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]    : 15.9165  (  )
R^2/D10^2   : 0.594370  (   )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =         146.73 using 59 PHA bins.
# Reduced chi-squared =         2.5742 for     57 degrees of freedom 
# Null hypothesis probability =   7.572516e-10
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  3.117e-08   3.170e-09
25- 50  1.306e-07   8.100e-09
50-150  2.307e-07   2.220e-08
15-150  3.925e-07   2.345e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 200.000       (      )
Norm        : 26.8510       (-1.30515     1.30514)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          56.03 using 59 PHA bins.
# Reduced chi-squared =         0.9830 for     57 degrees of freedom 
# Null hypothesis probability =   5.113971e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  6.686e-08   3.425e-09
25- 50  1.286e-07   7.250e-09
50-150  2.821e-07   1.530e-08
15-150  4.776e-07   2.685e-08

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 6.26841        (-1.18317      1.4569)
R1^2/D10^2  : 9.34830        (-4.78245      11.4823)
kT2 [keV]   : 24.5082        (-3.17393      4.9399)
R2^2/D10^2  : 0.110790    (-0.0544199   0.0749424)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          58.41 using 59 PHA bins.
# Reduced chi-squared =          1.062 for     55 degrees of freedom 
# Null hypothesis probability =   3.511168e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  6.352e-08   1.430e-08
25- 50  1.224e-07   1.660e-08
50-150  2.991e-07   4.335e-08
15-150  4.850e-07   6.780e-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: 1.55242     ( -0.0771666   0.0772871 )
Norm@50keV  : 5.09884E-03    ( -0.000210013   0.000209728 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          61.41 using 59 PHA bins.
# Reduced chi-squared =          1.077 for     57 degrees of freedom 
# Null hypothesis probability =   3.211195e-01
 
Photon flux (15-150 keV)    in 94.41 sec: 0.645936 ( -0.0283959  0.0284856 ) ph/cm2/s
Energy fluence (15-150 keV)             : 4.53023e-06 ( -1.99094e-07  1.9973e-07 ) ergs/cm2

Cutoff power-law model

Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.40928     ( -0.311718   0.188366 )
Epeak [keV] : 214.751      ( -214.756 -214.756 )
Norm@50keV  : 5.97840E-03    ( -0.00104705   0.00239996 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          60.72 using 59 PHA bins.
# Reduced chi-squared =          1.084 for     56 degrees of freedom 
# Null hypothesis probability =   3.096575e-01
 
Photon flux (15-150 keV)    in 94.41 sec: 0.639631 ( -0.030997  0.030165 ) ph/cm2/s
Energy fluence (15-150 keV)             : 4.48102e-06 ( -2.26178e-07  2.18323e-07 ) ergs/cm2

Band function

 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : 2.42296E-02   ( 0.848623   0.848623 )
beta        : -1.60870    ( 1.59867   0.0982589 )
Epeak [keV] : 37.3805      ( -37.2414 165.845 )
Norm@50keV   : 6.04379E-02    ( -0.060174   409.406 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          59.27 using 59 PHA bins.
# Reduced chi-squared =          1.078 for     55 degrees of freedom 
# Null hypothesis probability =   3.228144e-01
 
Photon flux (15-150 keV)    in 94.41 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)  = 2.26e-06
S(50-100 keV) = 2.81e-06

T90 vs. Hardness ratio plot

T90                                   = 109.080000013113 sec.
Hardness ratio (energy fluence ratio) = 1.24336

Color vs. Color plot

Count Ratio  (25-50 keV) / (15-25 keV) = 1.23375
Count Ratio (50-100 keV) / (15-25 keV) = 0.866281

Mask shadow pattern

IMX = -5.239178584497276E-02, IMY = -6.035240817613787E-01

TIME vs. PHA plot around the trigger time

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

TIME vs. DetID plot around the trigger time

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

100 us light curve (15-350 keV)

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

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:
-239.344000 -82.456000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
244.9781 -15.6278    0.3  23.9   67.1   6.8594  35.8    0.8	Sco X-1                       
254.3211  35.3424    6.2  43.9  165.2   0.5819   1.9    6.7	Her X-1                       
255.9455 -37.8894    3.4  32.9   18.0   0.6284   3.4    3.3	4U 1700-377                   
256.3866 -36.3937    5.3  31.4   18.4   0.3623   2.2    2.9	GX 349+2                      
262.9669 -24.5953    4.1  18.4   14.4   0.3776   2.8    9.3	GX 1+4                        
264.7473 -44.5106    9.5  37.9    4.2   0.2643   1.2    3.6	4U 1735-44                    
268.3036  -1.5047    4.6   5.3 -171.6   0.3654   2.5    5.0	SW J1753.5-0127               
270.3350 -25.0962    2.5  18.6   -6.9   0.7062   4.6    2.9	GX 5-1                        
270.2648 -25.7389    3.3  19.2   -6.4   0.5427   3.6    2.1	GRS 1758-258                  
273.8524 -14.0349   13.0   9.5  -38.5   0.1252   0.9    8.9	GX 17+2                       
275.9071 -30.4166    3.0  24.9  -16.3   0.6043   3.8    3.1	H1820-303                     
285.0994 -24.8645    7.0  24.7  -39.9   0.2632   1.6    4.8	HT1900.1-2455                 
288.7798  10.9541    1.4  27.5 -129.0   1.3882   8.1    1.2	GRS 1915+105                  
299.6208  35.1701    1.4  51.6 -145.6   4.0054   8.2    2.4	Cyg X-1                       
263.0387 -33.8458    3.7  27.5    9.2   0.4696   3.1    2.6	GX 354-0                      
251.4811  44.0414    2.6  52.8  166.4   2.5274   4.5 ------	UNKNOWN                       
253.2473 -39.2713    2.4  35.0   20.4   0.9961   4.8 ------	UNKNOWN                       
289.2056 -24.2070    2.9  27.1  -46.6   0.7304   4.0 ------	UNKNOWN

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

Time interval of the image:
-82.456000 11.956590
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
245.1284 -15.7938    0.0  23.8   66.6   0.1845   1.0   12.6	Sco X-1                       
254.3420  35.4568    8.5  44.0  165.3  -0.3538  -1.4    8.9	Her X-1                       
255.8224 -37.9600   44.0  33.0   18.1  -0.0445  -0.3   10.4	4U 1700-377                   
256.5441 -36.4667   83.6  31.4   18.1   0.0217   0.1    5.9	GX 349+2                      
263.1481 -24.7875    4.0  18.6   13.7  -0.3561  -2.9    8.0	GX 1+4                        
264.9118 -44.6026    0.0  38.0    4.0  -0.1689  -0.9   11.7	4U 1735-44                    
268.5148  -1.3003    0.0   5.5 -169.7   0.0381   0.3   12.7	SW J1753.5-0127               
270.1294 -25.1772    6.0  18.6   -6.2  -0.2528  -1.9   10.3	GX 5-1                        
270.4561 -25.5882    0.0  19.1   -7.0   0.1534   1.2   12.5	GRS 1758-258                  
274.0191 -13.8866    3.0   9.5  -39.9   0.4754   3.9    9.0	GX 17+2                       
275.7941 -30.4320    9.4  24.9  -16.0   0.1580   1.2    7.8	H1820-303                     
284.9257 -24.9459    4.6  24.6  -39.4   0.3365   2.5    6.2	HT1900.1-2455                 
288.6570  10.8600    5.9  27.3 -129.0  -0.2746  -2.0    9.8	GRS 1915+105                  
299.6120  35.0867    8.4  51.5 -145.5  -0.5809  -1.4    7.0	Cyg X-1                       
263.0509 -33.9860    5.3  27.6    9.1  -0.3070  -2.2    9.6	GX 354-0                      
236.4307  -3.6397    0.4  31.2   95.0   7.9173  31.8 ------	UNKNOWN                       
271.0559 -42.6712    2.9  36.1   -3.4   0.6795   4.0 ------	UNKNOWN                       
309.6710 -18.6791    1.7  42.6  -68.7   2.9783   6.6 ------	UNKNOWN

Post-slew image of 15-350 keV band

Time interval of the image:
66.956610 962.700700
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
244.9814 -15.6313    0.1  14.6  -19.5  41.8577  81.9    0.5	Sco X-1                       
254.4296  35.4641   24.5  42.6 -143.3   0.4481   0.5    7.4	Her X-1                       
256.0316 -37.8175    2.1  38.6  -10.2   3.8914   5.6    2.7	4U 1700-377                   
256.4971 -36.3853    1.9  37.6  -12.0   4.0038   6.0    3.7	GX 349+2                      
263.0814 -24.6629    5.2  33.2  -33.2   1.3638   2.2    6.3	GX 1+4                        
264.8293 -44.3251    7.7  47.7  -12.4   1.6075   1.5    8.4	4U 1735-44                    
268.3106  -1.4618    9.7  31.9  -78.2   1.1075   1.2    3.5	SW J1753.5-0127               
270.2353 -25.0214    2.6  38.9  -38.5   3.7457   4.5    4.4	GX 5-1                        
270.3915 -25.6288    3.1  39.3  -37.7   3.0498   3.7    8.4	GRS 1758-258                  
273.8968 -13.9921    3.8  38.4  -57.0   3.0965   3.0    6.9	GX 17+2                       
275.9481 -30.3265    5.5  45.8  -35.0   2.1694   2.1    2.7	H1820-303                     
263.1204 -33.7780    8.7  39.1  -21.4   1.0387   1.3    7.4	GX 354-0                      
236.4629  -3.6669    2.3   0.0  -23.4   2.5251   4.9 ------	UNKNOWN                       
242.4398 -12.6261    3.2  10.8  -18.1   1.7041   3.6 ------	UNKNOWN                       
265.4115   4.4208    3.3  30.0  -90.4   2.9733   3.5 ------	UNKNOWN

Plot creation:
Sun May 31 13:41:31 EDT 2015