batgrbproduct analysis for trigger=309096

batgrbproduct Analysis for Trigger=309096

Analysis Summary

Notes:

1) No attempt has been made to eliminate the non-significant decimal places.
2) This batgrbproduct analysis is done using the HEASARC data.
3) This batgrbproduct analysis is using the flight position for the mask-weighting calculation.

======================================================================
                  BAT GRB EVENT DATA PROCESSING REPORT
    Process Script Ver: batgrbproduct v2.46
    Process Start Time (local time): Mon Jan 20 02:46:00 EST 2014
             Host Name: batevent1
   Current Working Dir: /local/data/batevent/batevent_reproc/trigger309096
======================================================================

  Trigger: 00309096      Segment: 000

  BAT Trigger Time: 229748062.016   [s; MET]
      Trigger Stop: 229748062.528   [s; MET]
               UTC: 2008-04-13T02:54:19.302440    [includes UTCF correction] 
       Where From?: TDRSS position message

  BAT 
    RA: 287.289929388104   Dec: -27.679225960068  [deg; J2000]

     Catalogged Source?: NO
     Point Source?:      YES
     GRB Indicated?:     YES    [ by BAT flight software ]
     Image S/N Ratio:    9.06
     Image Trigger?:     NO
     Rate S/N Ratio:     15.6524758424985  [ if not an image trigger ]
     Image S/N Ratio:    9.06

  Flight Position:   [ source = BAT ]
    RA: 287.289929388104   Dec: -27.679225960068  [deg; J2000]

  Ground Position:   [ source = BAT pre-slew burst ]
    RA: 287.299178959777   Dec: -27.67775699745  [deg; J2000]  
        { 19h 09m 11.8s , -27d 40' 39.9" }
         +/- 0.64947967629121 [arcmin] (estimated 90% radius based on SNR)
         +/- 0.170347385175325 [arcmin] (formal 1-sigma fit error)
    SNR: 56.3484348898179
 
  Angular difference between Flight and Ground position is 0.499308 arcmin
 
  Partial Coding Fraction: 0.8125    [ including projection effects ]

  Duration
     T90: 46.3600000143051 +/- 0.481215117373871
        Measured from: 1.11599999666214
                   to: 47.4760000109673     [s; relative to TRIGTIME]
     T50: 15.4759999811649 +/- 0.798979370890493
        Measured from: 2.84400001168251
                   to: 18.3199999928474     [s; relative to TRIGTIME]



  Fluence
     Peak Flux  (peak 1 second)
        Measured from: 1.64399999380112     
                   to: 2.64399999380112     [s; relative to TRIGTIME]
     Total Fluence        
        Measured from: -0.0800000131130219     
                   to: 50.33599999547     [s; relative to TRIGTIME]
     
             Band 1     Band 2     Band 3     Band 4
              15-25      25-50     50-100    100-350     keV
 Total     1.538148   2.201969   1.573177   0.387463
           0.046508   0.044330   0.039610   0.037403 [error]
 Peak      0.134871   0.251607   0.242727   0.069710
           0.008356   0.009030   0.008725   0.006521 [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 4.90e-07 8.84e-07 1.22e-06 3.53e-06 3.52e-06 6.13e-06   erg/cm2
              Error 2.62e-08 2.67e-08 4.18e-08 2.80e-07 9.99e-08 3.02e-07   erg/cm2
Peak flux Power-law 1.37e+00 1.72e+00 1.57e+00 2.50e+00 5.52e+00 7.17e+00   ph/cm2/s
              Error 1.09e-01 8.27e-02 6.96e-02 2.40e-01 2.25e-01 3.01e-01   ph/cm2/s
 
Fluence   Cutoff-PL 4.79e-07 8.90e-07 1.23e-06 3.02e-06 3.49e-06 5.62e-06   erg/cm2
              Error 3.37e-08 2.88e-08 4.45e-08 6.82e-07 8.68e-08 7.58e-07   erg/cm2
Peak flux Cutoff-PL 1.24e+00 1.76e+00 1.64e+00 1.70e+00 5.42e+00 6.34e+00   ph/cm2/s
              Error 1.37e-01 8.97e-02 8.47e-02 4.63e-01 2.35e-01 5.21e-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    1.530    0.052    -      -           7.40e-03 1.96e-04   75.380 57
CPL   1.426    0.181     291.2    0.0      8.28e-03 1.56e-03   74.630 56
 
 
=== 1-s peak spectral analysis ===
 
Model Ph_index Ph_90err Epeak  Epeak_90err Norm     Nomr_90err chi2   dof
PL    1.130    0.070    -      -           4.74e-02 1.87e-03   52.670 57
CPL   0.744    0.283     182.1  165.8      7.11e-02 2.09e-02   46.720 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: 44.544000 sec.
T50 in the 50-300 keV band: 14.656000 sec.

 
=== Table of the duration information ==
 
        Value   tstart    tstop
T100   50.416   -0.080   50.336
T90    46.360    1.116   47.476
T50    15.476    2.844   18.320
Peak    1.000    1.644    2.644

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
  287.2992   -27.6778   0.0034    16.7003   -90.6024         2.8883762     56.348 TRIG_00309096                 
 
Foreground time interval of the image:
 -0.080  10.685 (delta_t =  10.765 [sec])
Background time interval of the image:
-239.016  -0.080 (delta_t = 238.936 [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 0.512000

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 0.512000

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 0.512000

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   -0.080 sec. to   50.336 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.52958     ( -0.0523745   0.0523954 )
Norm@50keV  : 7.39868E-03    ( -0.000196032   0.000195954 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          75.38 using 59 PHA bins.
# Reduced chi-squared =          1.322 for     57 degrees of freedom 
# Null hypothesis probability =   5.198109e-02
 
Photon flux (15-150 keV)    in 50.42 sec: 0.931188 ( -0.0270238  0.0271126 ) ph/cm2/s
Energy fluence (15-150 keV)             : 3.52241e-06 ( -9.97408e-08  9.99738e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from   -0.080 sec. to   50.336 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.42567     ( -0.211446   0.149592 )
Epeak [keV] : 291.209      ( -291.233 -291.233 )
Norm@50keV  : 8.28452E-03    ( -0.00103163   0.00208143 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          74.63 using 59 PHA bins.
# Reduced chi-squared =          1.333 for     56 degrees of freedom 
# Null hypothesis probability =   4.873906e-02
 
Photon flux (15-150 keV)    in 50.42 sec: 0.923336 ( -0.030718  0.030471 ) ph/cm2/s
Energy fluence (15-150 keV)             : 3.49175e-06 ( -1.18069e-07  5.55376e-08 ) ergs/cm2

Band function

Time interval is from   -0.080 sec. to   50.336 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -0.566449   ( -0.6512   5.85508 )
beta        : -1.59293    ( -0.0997443   0.0792028 )
Epeak [keV] : 50.4693      ( -24.4449 109.298 )
Norm@50keV   : 2.93195E-02    ( -0.0294483   436.129 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          71.01 using 59 PHA bins.
# Reduced chi-squared =          1.291 for     55 degrees of freedom 
# Null hypothesis probability =   7.194038e-02
 
Photon flux (15-150 keV)    in 50.42 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]    : 15.7066  (  )
R^2/D10^2   : 8.44770E-02  (   )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =         360.37 using 59 PHA bins.
# Reduced chi-squared =         6.3223 for     57 degrees of freedom 
# Null hypothesis probability =   1.235400e-45
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  2.181e-07   1.132e-08
25- 50  9.033e-07   3.252e-08
50-150  1.546e-06   8.647e-08
15-150  2.668e-06   8.546e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 200.000       (      )
Norm        : 3.77770       (-0.0996702     0.0996691)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          79.06 using 59 PHA bins.
# Reduced chi-squared =          1.387 for     57 degrees of freedom 
# Null hypothesis probability =   2.822487e-02
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  4.744e-07   1.412e-08
25- 50  9.126e-07   2.697e-08
50-150  2.001e-06   5.899e-08
15-150  3.388e-06   1.006e-07

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 7.90670        (-0.765418      0.825652)
R1^2/D10^2  : 0.644462        (-0.175173      0.260937)
kT2 [keV]   : 30.3189        (-3.6523      5.34211)
R2^2/D10^2  : 6.79956E-03    (-0.0028227   0.00386768)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          79.81 using 59 PHA bins.
# Reduced chi-squared =          1.451 for     55 degrees of freedom 
# Null hypothesis probability =   1.605551e-02
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  4.131e-07   3.915e-08
25- 50  9.278e-07   5.597e-08
50-150  2.120e-06   2.050e-07
15-150  3.461e-06   2.564e-07

Peak spectrum fit

Power-law model

Time interval is from    1.644 sec. to    2.644 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.13034     ( -0.0698127   0.0694003 )
Norm@50keV  : 4.74207E-02    ( -0.00186898   0.00186845 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          52.67 using 59 PHA bins.
# Reduced chi-squared =         0.9241 for     57 degrees of freedom 
# Null hypothesis probability =   6.380408e-01
 
Photon flux (15-150 keV)    in 1 sec: 5.51778 ( -0.224819  0.225082 ) ph/cm2/s
Energy fluence (15-150 keV)             : 4.91099e-07 ( -2.12068e-08  2.12654e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from    1.644 sec. to    2.644 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 0.743651     ( -0.292455   0.274113 )
Epeak [keV] : 182.090      ( -54.9172 276.598 )
Norm@50keV  : 7.10963E-02    ( -0.0173063   0.0244968 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          46.72 using 59 PHA bins.
# Reduced chi-squared =         0.8342 for     56 degrees of freedom 
# Null hypothesis probability =   8.070488e-01
 
Photon flux (15-150 keV)    in 1 sec: 5.41686 ( -0.23516  0.23535 ) ph/cm2/s
Energy fluence (15-150 keV)             : 4.80698e-07 ( -2.2889e-08  2.2767e-08 ) ergs/cm2

Band function

Time interval is from    1.644 sec. to    2.644 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : 0.791259   ( -1.04579   4.34625 )
beta        : -1.26244    ( 1.26081   0.109896 )
Epeak [keV] : 50.3713      ( -26.5419 143.09 )
Norm@50keV   : 0.719158    ( -0.708657   229.356 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          43.93 using 59 PHA bins.
# Reduced chi-squared =         0.7988 for     55 degrees of freedom 
# Null hypothesis probability =   8.578479e-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]    : 20.1147  (  )
R^2/D10^2   : 0.253052  (   )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =         143.31 using 59 PHA bins.
# Reduced chi-squared =         2.5143 for     57 degrees of freedom 
# Null hypothesis probability =   2.215363e-09
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.969e-08   1.610e-09
25- 50  9.846e-08   5.715e-09
50-150  2.956e-07   1.915e-08
15-150  4.137e-07   1.930e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 199.363       (      )
Norm        : 22.8600       (     )
------------------------------------------------------------
#Fit statistic : Chi-Squared =         148.57 using 59 PHA bins.
# Reduced chi-squared =         2.6065 for     57 degrees of freedom 
# Null hypothesis probability =   4.221413e-10
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  5.692e-08   2.285e-09
25- 50  1.095e-07   4.550e-09
50-150  2.401e-07   1.030e-08
15-150  4.066e-07   1.915e-08

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 8.94105        (-1.40546      1.62976)
R1^2/D10^2  : 1.93964        (-0.714858      1.27063)
kT2 [keV]   : 33.5011        (-4.89172      8.57419)
R2^2/D10^2  : 4.00994E-02    (-0.0208065   0.0286337)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          44.14 using 59 PHA bins.
# Reduced chi-squared =         0.8025 for     55 degrees of freedom 
# Null hypothesis probability =   8.526876e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  3.665e-08   6.075e-09
25- 50  1.055e-07   1.333e-08
50-150  3.418e-07   6.125e-08
15-150  4.840e-07   8.750e-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: 1.43520     ( -0.0530179   0.0529807 )
Norm@50keV  : 1.74315E-02    ( -0.000486325   0.000486292 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          69.42 using 59 PHA bins.
# Reduced chi-squared =          1.218 for     57 degrees of freedom 
# Null hypothesis probability =   1.251428e-01
 
Photon flux (15-150 keV)    in 10.76 sec: 2.14041 ( -0.0644829  0.0646414 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.79981e-06 ( -5.40923e-08  5.42126e-08 ) ergs/cm2

Cutoff power-law model

Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.20661     ( -0.217922   0.207364 )
Epeak [keV] : 185.670      ( -65.0348 946.672 )
Norm@50keV  : 2.23109E-02    ( -0.00435986   0.00575198 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          65.87 using 59 PHA bins.
# Reduced chi-squared =          1.176 for     56 degrees of freedom 
# Null hypothesis probability =   1.722400e-01
 
Photon flux (15-150 keV)    in 10.76 sec: 2.10607 ( -0.07097  0.07115 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.76873e-06 ( -6.16333e-08  6.13428e-08 ) ergs/cm2

Band function

 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : 0.914364   ( -2.1232   3.54877 )
beta        : -1.51086    ( -0.0787732   0.0717536 )
Epeak [keV] : 36.8903      ( -7.78054 63.1771 )
Norm@50keV   : 0.657077    ( -0.65401   361.463 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          60.43 using 59 PHA bins.
# Reduced chi-squared =          1.099 for     55 degrees of freedom 
# Null hypothesis probability =   2.860090e-01
 
Photon flux (15-150 keV)    in 10.76 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)  = 8.84e-07
S(50-100 keV) = 1.22e-06

T90 vs. Hardness ratio plot

T90                                   = 46.3600000143051 sec.
Hardness ratio (energy fluence ratio) = 1.38009

Color vs. Color plot

Count Ratio  (25-50 keV) / (15-25 keV) = 1.43157
Count Ratio (50-100 keV) / (15-25 keV) = 1.02277

Mask shadow pattern

IMX = -3.154197460994845E-03, IMY = 3.000031334939362E-01

TIME vs. PHA plot around the trigger time

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.512000

TIME vs. DetID plot around the trigger time

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.512000

100 us light curve (15-350 keV)

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.512000

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:
-239.016000 -0.080000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
244.9793 -15.6510    0.2  24.4  101.7  29.0852  73.8    0.6	Sco X-1                       
255.9920 -37.8634    0.8  15.7   30.1   3.8463  14.1    1.2	4U 1700-377                   
256.4768 -36.4483    2.2  14.4   33.2   1.4106   5.1    2.5	GX 349+2                      
263.0161 -24.8901    8.0   5.2   95.3  -0.4252  -1.4    8.7	GX 1+4                        
264.8956 -44.6255    0.0  18.5   -1.1   0.4298   1.5   12.4	4U 1735-44                    
268.4241  -1.4979    4.7  24.8  170.1   0.7234   2.5    4.3	SW J1753.5-0127               
270.2547 -25.0364    2.7   2.0 -140.0   1.2664   4.3    3.0	GX 5-1                        
270.3625 -25.7779   10.6   1.7 -118.3   0.3226   1.1    3.9	GRS 1758-258                  
274.0066 -13.9546    3.0  13.4 -166.2   1.0893   3.8    4.9	GX 17+2                       
275.9642 -30.3283    4.7   7.6  -66.1   0.7091   2.5    3.1	H1820-303                     
284.9650 -25.0426   68.3  14.8 -100.9  -0.0540  -0.2    8.3	HT1900.1-2455                 
288.8035  10.9399   21.5  42.1 -159.1   0.2858   0.5    0.5	GRS 1915+105                  
262.8933 -33.7581    6.4   8.9   22.8   0.5218   1.8    6.6	GX 354-0                      
258.7705 -32.5657    2.4  10.6   42.1   1.3380   4.9 ------	UNKNOWN                       
266.7974 -27.3312    1.4   1.9   48.2   2.4231   8.2 ------	UNKNOWN                       
292.2447 -56.4132    2.4  34.5  -32.5   1.7288   4.9 ------	UNKNOWN                       
312.9417 -19.4465    4.5  41.2  -99.5   4.5716   2.6 ------	UNKNOWN

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

Time interval of the image:
-0.080000 10.684600
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
244.9785 -15.6938    2.0  24.4  101.6  -0.3733  -5.9    3.2	Sco X-1                       
256.1557 -37.9089    4.0  15.6   29.7   0.1333   2.9    8.9	4U 1700-377                   
256.2850 -36.3083    7.6  14.5   34.0   0.0717   1.5   10.0	GX 349+2                      
262.8603 -24.6593   23.5   5.4   97.2   0.0218   0.5    9.6	GX 1+4                        
264.8390 -44.6173    7.3  18.5   -1.0  -0.0730  -1.6   10.8	4U 1735-44                    
268.3140  -1.2931    7.1  25.0  169.9   0.0858   1.6   10.1	SW J1753.5-0127               
270.4292 -25.2129    5.0   2.0 -133.2  -0.1070  -2.3   11.2	GX 5-1                        
270.2268 -25.8843    4.8   1.5 -116.1  -0.1105  -2.4    9.4	GRS 1758-258                  
273.9221 -14.1763    9.1  13.1 -166.1  -0.0547  -1.3    9.7	GX 17+2                       
276.0314 -30.4209  108.9   7.7  -65.7  -0.0047  -0.1    6.4	H1820-303                     
285.1985 -24.9982    4.0  15.0 -100.9   0.1366   2.9   10.0	HT1900.1-2455                 
288.9177  11.0478    7.5  42.3 -159.0  -0.1182  -1.5    9.3	GRS 1915+105                  
262.8282 -33.7504    4.0   8.9   23.1  -0.1249  -2.9    9.5	GX 354-0                      
261.3894  23.4008    2.1  50.2  161.9   0.8482   5.4 ------	UNKNOWN                       
287.2992 -27.6778    0.2  16.7  -90.6   2.8883  56.3 ------	UNKNOWN                       
319.5195 -43.7127    3.3  44.4  -62.8   0.6981   3.5 ------	UNKNOWN

Post-slew image of 15-350 keV band

Time interval of the image:
50.084590 352.184600
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
255.9987 -37.8360    0.6  28.0   67.0   6.2099  18.2    0.8	4U 1700-377                   
256.5895 -36.5529   32.6  27.3   69.5  -0.1140  -0.4   10.8	GX 349+2                      
262.8827 -24.7630    6.0  22.0   98.3  -0.5990  -1.9    7.0	GX 1+4                        
264.7910 -44.6011    8.2  24.7   47.0   0.4060   1.4    9.3	4U 1735-44                    
268.4091  -1.4416    5.7  31.9  148.5   0.7968   2.0    2.6	SW J1753.5-0127               
270.2838 -25.0762    2.2  15.4  102.1   1.3467   5.3    0.2	GX 5-1                        
270.2300 -25.7009    5.0  15.3   99.8   0.6211   2.4    4.7	GRS 1758-258                  
274.1075 -14.0762    2.0  18.3  141.6   1.4200   5.6    6.4	GX 17+2                       
275.8915 -30.3202    3.1  10.3   78.7   0.8808   3.8    3.3	H1820-303                     
285.0207 -24.8505    4.4   3.5  150.3   0.6019   2.6    4.3	HT1900.1-2455                 
288.8397  10.9619    9.9  38.7 -171.3   0.4138   1.2    2.6	GRS 1915+105                  
262.9023 -33.8327    8.9  21.8   73.8   0.3674   1.3    4.3	GX 354-0                      
257.1472  14.3043    2.6  51.2  147.6   5.9903   4.5 ------	UNKNOWN                       
266.8168 -27.3714    1.2  18.1   92.5   2.5919   9.6 ------	UNKNOWN                       
277.3268 -23.7997    2.1   9.8  117.5   1.3313   5.5 ------	UNKNOWN                       
348.2448 -46.7216    3.7  50.7  -44.5   5.2914   3.1 ------	UNKNOWN                       
333.1977 -24.1351    3.8  41.2  -77.9   3.8289   3.1 ------	UNKNOWN                       
320.9516   4.9619    2.8  46.1 -123.7   5.8598   4.1 ------	UNKNOWN

Plot creation:
Sun May 31 07:49:42 EDT 2015