batgrbproduct analysis for trigger=449399

batgrbproduct Analysis for Trigger=449399

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 13 23:42:52 EST 2014
             Host Name: batevent1
   Current Working Dir: /local/data/batevent/batevent_reproc/trigger449399
======================================================================

  Trigger: 00449399      Segment: 000

  BAT Trigger Time: 321926231.296   [s; MET]
      Trigger Stop: 321926235.392   [s; MET]
               UTC: 2011-03-15T23:57:04.537480    [includes UTCF correction] 
       Where From?: TDRSS position message

  BAT 
    RA: 279.191126332668   Dec: 17.5321484999389  [deg; J2000]

     Catalogged Source?: NO
     Point Source?:      YES
     GRB Indicated?:     YES    [ by BAT flight software ]
     Image S/N Ratio:    11.06
     Image Trigger?:     NO
     Rate S/N Ratio:     9.74679434480896  [ if not an image trigger ]
     Image S/N Ratio:    11.06

  Flight Position:   [ source = BAT ]
    RA: 279.191126332668   Dec: 17.5321484999389  [deg; J2000]

  Ground Position:   [ source = BAT pre-slew burst ]
    RA: 279.204684110321   Dec: 17.5367582609684  [deg; J2000]  
        { 18h 36m 49.1s , +17d 32' 12.3" }
         +/- 1.03659230859771 [arcmin] (estimated 90% radius based on SNR)
         +/- 0.361548924956912 [arcmin] (formal 1-sigma fit error)
    SNR: 28.8949044519654
 
  Angular difference between Flight and Ground position is 0.823507 arcmin
 
  Partial Coding Fraction: 0.5703125    [ including projection effects ]

  Duration
     T90: 87.6759999394417 +/- 11.8267709656415
        Measured from: -60.6359999775887
                   to: 27.039999961853     [s; relative to TRIGTIME]
     T50: 32.5839999318123 +/- 2.15692374081893
        Measured from: -20.7519999742508
                   to: 11.8319999575615     [s; relative to TRIGTIME]



  Fluence
     Peak Flux  (peak 1 second)
        Measured from: 3.12800002098083     
                   to: 4.12800002098083     [s; relative to TRIGTIME]
     Total Fluence        
        Measured from: -66.7639999985695     
                   to: 38.839999973774     [s; relative to TRIGTIME]
     
             Band 1     Band 2     Band 3     Band 4
              15-25      25-50     50-100    100-350     keV
 Total     2.083191   2.569981   1.654212   0.375730
           0.095410   0.088663   0.076001   0.068294 [error]
 Peak      0.059155   0.078618   0.041313   0.021078
           0.009719   0.009618   0.008157   0.006943 [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 7.26e-07 1.13e-06 1.33e-06 3.03e-06 4.08e-06 6.22e-06   erg/cm2
              Error 5.58e-08 5.05e-08 7.70e-08 3.86e-07 1.81e-07 4.37e-07   erg/cm2
Peak flux Power-law 6.24e-01 5.72e-01 3.62e-01 3.52e-01 1.70e+00 1.91e+00   ph/cm2/s
              Error 1.47e-01 8.49e-02 6.69e-02 1.31e-01 2.48e-01 2.69e-01   ph/cm2/s
 
Fluence   Cutoff-PL 7.11e-07 1.14e-06 1.34e-06 2.56e-06 4.04e-06 5.75e-06   erg/cm2
              Error 6.72e-08 4.35e-08 8.08e-08 9.19e-07 2.06e-07 8.86e-07   erg/cm2
Peak flux Cutoff-PL 5.77e-01 6.02e-01 3.74e-01 1.98e-01 1.67e+00 1.75e+00   ph/cm2/s
              Error 1.79e-01 1.10e-01 7.47e-02 2.38e-01 2.61e-01 3.54e-01   ph/cm2/s
 
Fluence        Band 6.88e-07 1.15e-06 1.33e-06 2.82e-06 4.03e-06 6.00e-06   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    1.767    0.081    -      -           4.19e-03 1.81e-04   48.500 57
CPL   1.655    0.255     155.6  -17.1      4.76e-03 1.45e-03   48.120 56
 
 
=== 1-s peak spectral analysis ===
 
Model Ph_index Ph_90err Epeak  Epeak_90err Norm     Nomr_90err chi2   dof
PL    1.658    0.245    -      -           1.30e-02 1.91e-03   69.980 57
CPL   1.153    1.097      80.3  -23.3      2.40e-02 7.05e-02   69.390 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: 90.880000 sec.
T50 in the 50-300 keV band: 35.776000 sec.

 
=== Table of the duration information ==
 
        Value   tstart    tstop
T100  105.604  -66.764   38.840
T90    87.676  -60.636   27.040
T50    32.584  -20.752   11.832
Peak    1.000    3.128    4.128

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
  279.2047    17.5368   0.0066    40.4920  -170.6491         6.5049972     28.895 TRIG_00449399                 
 
Foreground time interval of the image:
-66.764  35.405 (delta_t = 102.169 [sec])
Background time interval of the image:
-239.296 -66.764 (delta_t = 172.532 [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 4.096000

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 4.096000

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 4.096000

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)

The mask-weighted light curves based on cleaned DPHs

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  -66.764 sec. to   38.840 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.76706     ( -0.080343   0.0809815 )
Norm@50keV  : 4.18892E-03    ( -0.000181151   0.000180617 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          48.50 using 59 PHA bins.
# Reduced chi-squared =         0.8508 for     57 degrees of freedom 
# Null hypothesis probability =   7.812731e-01
 
Photon flux (15-150 keV)    in 105.6 sec: 0.570017 ( -0.026015  0.0261223 ) ph/cm2/s
Energy fluence (15-150 keV)             : 4.07801e-06 ( -1.80796e-07  1.81564e-07 ) ergs/cm2

Cutoff power-law model

Time interval is from  -66.764 sec. to   38.840 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.65500     ( -0.326616   0.183155 )
Epeak [keV] : 155.583      ( -121.496 -155.627 )
Norm@50keV  : 4.75905E-03    ( -0.000807806   0.00208478 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          48.12 using 59 PHA bins.
# Reduced chi-squared =         0.8593 for     56 degrees of freedom 
# Null hypothesis probability =   7.639419e-01
 
Photon flux (15-150 keV)    in 105.6 sec: 0.565348 ( -0.028746  0.028694 ) ph/cm2/s
Energy fluence (15-150 keV)             : 4.04282e-06 ( -2.07831e-07  2.03966e-07 ) ergs/cm2

Band function

Time interval is from  -66.764 sec. to   38.840 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -1.36403   ( 1.32344   1.32344 )
beta        : -1.84170    ( 1.84042   0.138598 )
Epeak [keV] : 62.2259      ( -59.5713 -59.5713 )
Norm@50keV   : 7.12656E-03    ( -0.00277262   0 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          47.55 using 59 PHA bins.
# Reduced chi-squared =         0.8646 for     55 degrees of freedom 
# Null hypothesis probability =   7.518871e-01
 
Photon flux (15-150 keV)    in 105.6 sec:  (    ) ph/cm2/s
Energy fluence (15-150 keV)             : 4.02824e-06 ( 0  0 ) ergs/cm2

Single BB

 
Spectral model blackbody:
------------------------------------------------------------
Parameters  : value    Lower 90%  Upper 90%
kT [keV]    : 13.5134  (  )
R^2/D10^2   : 8.43312E-02  (   )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =         183.37 using 59 PHA bins.
# Reduced chi-squared =         3.2169 for     57 degrees of freedom 
# Null hypothesis probability =   3.460110e-15
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  3.444e-07   2.814e-08
25- 50  1.236e-06   6.970e-08
50-150  1.458e-06   1.220e-07
15-150  3.039e-06   1.373e-07

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 125.813       (      )
Norm        : 2.34911       (-0.129898     0.16978)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          51.49 using 59 PHA bins.
# Reduced chi-squared =         0.9034 for     57 degrees of freedom 
# Null hypothesis probability =   6.809554e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  6.372e-07   4.736e-08
25- 50  1.154e-06   6.970e-08
50-150  2.130e-06   5.660e-07
15-150  3.920e-06   6.172e-07

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 7.01976        (-1.03417      1.11438)
R1^2/D10^2  : 0.664416        (-0.260528      0.51415)
kT2 [keV]   : 25.8047        (-4.10292      6.63993)
R2^2/D10^2  : 5.98055E-03    (-0.00334668   0.00565731)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          55.75 using 59 PHA bins.
# Reduced chi-squared =          1.014 for     55 degrees of freedom 
# Null hypothesis probability =   4.463110e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  6.289e-07   9.684e-08
25- 50  1.181e-06   1.376e-07
50-150  2.162e-06   4.213e-07
15-150  3.972e-06   5.364e-07

Peak spectrum fit

Power-law model

Time interval is from    3.128 sec. to    4.128 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.65803     ( -0.241913   0.247375 )
Norm@50keV  : 1.30166E-02    ( -0.0019233   0.00190256 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          69.98 using 59 PHA bins.
# Reduced chi-squared =          1.228 for     57 degrees of freedom 
# Null hypothesis probability =   1.159081e-01
 
Photon flux (15-150 keV)    in 1 sec: 1.70417 ( -0.24768  0.248434 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.20963e-07 ( -1.86652e-08  1.8862e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from    3.128 sec. to    4.128 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.15265     ( -1.47313   0.720856 )
Epeak [keV] : 80.2540      ( -33.6925 -80.3556 )
Norm@50keV  : 2.39910E-02    ( -0.0239457   0.117049 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          69.39 using 59 PHA bins.
# Reduced chi-squared =          1.239 for     56 degrees of freedom 
# Null hypothesis probability =   1.078292e-01
 
Photon flux (15-150 keV)    in 1 sec: 1.67029 ( -0.26208  0.25927 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.16475e-07 ( -2.17825e-08  2.1249e-08 ) ergs/cm2

Band function

Time interval is from    3.128 sec. to    4.128 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -0.520124   ( 0.796768   0.796768 )
beta        : -2.09769    ( 2.08095   0.586532 )
Epeak [keV] : 56.2379      ( -56.2773 62.452 )
Norm@50keV   : 5.51962E-02    ( -0.055609   985.078 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          68.43 using 59 PHA bins.
# Reduced chi-squared =          1.244 for     55 degrees of freedom 
# Null hypothesis probability =   1.054099e-01
 
Photon flux (15-150 keV)    in 1 sec:  (    ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.15656e-07 ( 0  0 ) ergs/cm2

Single BB

 
Spectral model blackbody:
------------------------------------------------------------
Parameters  : value    Lower 90%  Upper 90%
kT [keV]    : 13.0726  (-1.87131  2.27422)
R^2/D10^2   : 0.311749  (-0.140011   0.239049)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          75.87 using 59 PHA bins.
# Reduced chi-squared =          1.331 for     57 degrees of freedom 
# Null hypothesis probability =   4.806056e-02
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.130e-08   2.815e-09
25- 50  3.915e-08   8.000e-09
50-150  4.243e-08   1.287e-08
15-150  9.288e-08   1.855e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 154.598       (-71.5311      -152.583)
Norm        : 6.98510       (-1.08453     1.53578)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          69.41 using 59 PHA bins.
# Reduced chi-squared =          1.218 for     57 degrees of freedom 
# Null hypothesis probability =   1.252623e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.789e-08   9.840e-09
25- 50  3.331e-08   1.794e-08
50-150  6.657e-08   3.854e-08
15-150  1.178e-07   6.600e-08

Double BB

R1^2/D10^2  : 0.537062        (-0.283896      0.523638)
kT2 [keV]   : 200.000        (      )
R2^2/D10^2  : 1.45948E-04    (-6.83082e-05   0.000534002)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          71.18 using 59 PHA bins.
#Fit statistic : Chi-Squared =          67.37 using 59 PHA bins.
#Fit statistic : Chi-Squared =          67.15 using 59 PHA bins.
# Reduced chi-squared =          1.294 for     55 degrees of freedom 
# Reduced chi-squared =          1.225 for     55 degrees of freedom 
# Reduced chi-squared =          1.221 for     55 degrees of freedom 
# Null hypothesis probability =   7.003431e-02
# Null hypothesis probability =   1.223483e-01
# Null hypothesis probability =   1.261302e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.766e-08   8.929e-09
25- 50  3.451e-08   1.582e-08
50-150  5.042e-08   2.356e-08
15-150  1.026e-07   4.362e-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: 1.76598     ( -0.0805935   0.0812189 )
Norm@50keV  : 4.26710E-03    ( -0.000184433   0.000183886 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          49.08 using 59 PHA bins.
# Reduced chi-squared =         0.8611 for     57 degrees of freedom 
# Null hypothesis probability =   7.628397e-01
 
Photon flux (15-150 keV)    in 102.2 sec: 0.580422 ( -0.0265086  0.0266192 ) ph/cm2/s
Energy fluence (15-150 keV)             : 4.02059e-06 ( -1.7821e-07  1.78967e-07 ) ergs/cm2

Cutoff power-law model

Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.71094     ( -0.321074   0.356583 )
Epeak [keV] : 264.393      (   )
Norm@50keV  : 4.54350E-03    (     )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          48.99 using 59 PHA bins.
# Reduced chi-squared =         0.8749 for     56 degrees of freedom 
# Null hypothesis probability =   7.350596e-01
 
Photon flux (15-150 keV)    in 102.2 sec: 0.578056 ( -0.029252  0.02814 ) ph/cm2/s
Energy fluence (15-150 keV)             : 4.00454e-06 ( -2.04472e-07  1.92524e-07 ) ergs/cm2

Band function

 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -1.42544   ( 1.33629   1.33629 )
beta        : -1.82376    ( -1.20018   0.120772 )
Epeak [keV] : 65.2075      ( -57.3482 103.703 )
Norm@50keV   : 6.71793E-03    ( -0.00227637   0 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          48.43 using 59 PHA bins.
# Reduced chi-squared =         0.8805 for     55 degrees of freedom 
# Null hypothesis probability =   7.220789e-01
 
Photon flux (15-150 keV)    in 102.2 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)  = 1.13e-06
S(50-100 keV) = 1.33e-06

T90 vs. Hardness ratio plot

T90                                   = 87.6759999394417 sec.
Hardness ratio (energy fluence ratio) = 1.17699

Color vs. Color plot

Count Ratio  (25-50 keV) / (15-25 keV) = 1.23368
Count Ratio (50-100 keV) / (15-25 keV) = 0.794076

Mask shadow pattern

IMX = -8.424927693442371E-01, IMY = 1.387327467616037E-01

TIME vs. PHA plot around the trigger time

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 4.096000

TIME vs. DetID plot around the trigger time

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 4.096000

100 us light curve (15-350 keV)

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 4.096000

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:
-239.296000 -66.764000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
244.9813 -15.6396    0.4  26.0   98.2   7.2703  28.4    0.1	Sco X-1                       
255.9185 -37.8373    1.4  20.6   35.6   1.5295   8.0    3.3	4U 1700-377                   
256.3032 -36.4328    4.9  19.4   37.9   0.4407   2.3    6.4	GX 349+2                      
263.0921 -24.7381    2.0   8.2   69.0   0.9593   5.7    4.6	GX 1+4                        
264.5677 -44.2850    0.0  22.8   11.3   0.3553   2.0   12.4	4U 1735-44                    
268.4029  -1.4177    4.3  21.1  169.2   0.5183   2.7    3.0	SW J1753.5-0127               
270.2820 -25.0678    2.6   3.1   21.5   0.8424   4.5    0.7	GX 5-1                        
270.2121 -25.7243    4.5   3.7   18.3   0.4879   2.6    5.0	GRS 1758-258                  
274.1583 -14.0741    6.2   8.5 -165.0   0.3360   1.9    9.2	GX 17+2                       
275.7520 -30.5174    0.0   9.0  -25.1   0.2403   1.4   12.7	H1820-303                     
285.2083 -25.0269    4.1  12.7  -76.7   0.5053   2.9   11.3	HT1900.1-2455                 
288.7978  10.9331    1.5  37.2 -153.2   1.8614   7.8    0.7	GRS 1915+105                  
262.9226 -33.7791    2.5  13.8   29.9   0.7627   4.6    4.7	GX 354-0                      
238.7225 -14.2669    2.8  32.2   96.8   1.3778   4.1 ------	UNKNOWN                       
303.7665  23.2510    2.9  55.2 -145.3   5.1629   4.0 ------	UNKNOWN

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

Time interval of the image:
-66.764000 35.404600
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
245.0054 -15.5518    2.5  26.0   98.5   1.0023   4.6    5.5	Sco X-1                       
256.0181 -37.8361  187.2  20.5   35.4  -0.0098  -0.1    1.6	4U 1700-377                   
256.4355 -36.4234    4.7  19.3   37.7   0.3839   2.5    0.0	GX 349+2                      
263.1589 -24.9078    0.0   8.2   67.7  -0.1132  -0.8   12.7	GX 1+4                        
264.7258 -44.3397    6.9  22.8   11.0   0.2513   1.7    6.7	4U 1735-44                    
268.5000  -1.6065    0.0  20.9  169.4   0.2843   1.8   12.2	SW J1753.5-0127               
270.4251 -24.9344    8.3   2.9   20.2   0.1992   1.4   11.6	GX 5-1                        
270.4748 -25.6065    4.8   3.5   15.3   0.3582   2.5   12.4	GRS 1758-258                  
273.9717 -13.9578    3.7   8.6 -166.4   0.4312   3.1    5.1	GX 17+2                       
275.8936 -30.2176   11.8   8.8  -26.7  -0.1358  -1.0    9.1	H1820-303                     
284.9679 -25.0468    4.7  12.5  -76.4  -0.3596  -2.5    8.4	HT1900.1-2455                 
288.6538  11.1028    0.0  37.3 -153.5   0.4243   2.1   12.7	GRS 1915+105                  
263.0800 -33.6935    6.4  13.7   29.7  -0.2431  -1.8    9.6	GX 354-0                      
228.9457 -42.1475    2.7  40.6   48.7   1.7341   4.2 ------	UNKNOWN                       
279.2047  17.5367    0.4  40.5 -170.6   6.5046  28.9 ------	UNKNOWN

Post-slew image of 15-350 keV band

Time interval of the image:
93.804590 559.304600
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
244.9749 -15.6469    0.8  47.3   41.5  18.9665  13.6    0.5	Sco X-1                       
254.4593  35.3465   19.1  28.3  128.0  -0.2761  -0.6    0.3	Her X-1                       
262.9863 -24.7232    3.2  45.1   15.0   2.4604   3.6    1.8	GX 1+4                        
268.4278  -1.4826    2.3  21.8   24.3   1.5682   5.0    4.0	SW J1753.5-0127               
270.2438 -25.1034    3.7  43.5    5.9   1.6705   3.1    2.6	GX 5-1                        
270.1980 -25.6868    4.2  44.1    5.7   1.5347   2.7    6.6	GRS 1758-258                  
273.9243 -14.0241    3.2  32.0    3.7   1.4073   3.6    4.8	GX 17+2                       
275.8884 -30.4985    5.4  48.1   -2.1  -1.5225  -2.2    8.1	H1820-303                     
284.9562 -24.9355    9.3  42.8  -13.6   0.6147   1.3    4.4	HT1900.1-2455                 
288.8081  10.9442    0.5  11.4  -62.0   7.4452  24.6    0.6	GRS 1915+105                  
299.6094  35.1995    2.2  25.3 -144.1   1.6935   5.2    0.9	Cyg X-1                       
308.0637  41.1269   14.0  34.2 -145.6   0.3553   0.8   10.7	Cyg X-3                       
326.3090  38.3049    7.2  45.9 -132.7   1.7817   1.6    6.5	Cyg X-2                       
263.0931 -33.9582    5.0  53.7   10.6   3.1858   2.3    9.0	GX 354-0                      
239.8359  17.0201    3.4  37.5   89.4   3.7733   3.4 ------	UNKNOWN                       
245.3513  18.2019    2.2  32.2   90.6   3.7251   5.3 ------	UNKNOWN                       
268.3370  23.7797    3.2  11.9  117.6   1.1412   3.6 ------	UNKNOWN                       
286.5694  71.5135    3.5  54.2  177.0   4.2523   3.3 ------	UNKNOWN                       
303.5440  39.8085    3.0  30.7 -147.5   1.2951   3.9 ------	UNKNOWN                       
335.6099  50.0656    5.6  55.3 -145.3   5.0587   2.1 ------	UNKNOWN

Plot creation:
Sat May 30 22:45:47 EDT 2015