batgrbproduct analysis for trigger=641698

batgrbproduct Analysis for Trigger=641698

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): Fri Jun 26 00:15:42 EDT 2015
             Host Name: bat1
   Current Working Dir: /local/data/bat1/alien/Swift_3rdBATcatalog/event/batevent_reproc/trigger641698
======================================================================

  Trigger: 00641698      Segment: 000

  BAT Trigger Time: 454402149.44   [s; MET]
      Trigger Stop: 454402149.952   [s; MET]
               UTC: 2015-05-27T06:48:55.804620    [includes UTCF correction] 
       Where From?: TDRSS position message

  BAT 
    RA: 288.957781485581   Dec: 4.19407695074873  [deg; J2000]

     Catalogged Source?: NO
     Point Source?:      YES
     GRB Indicated?:     YES    [ by BAT flight software ]
     Image S/N Ratio:    9.07
     Image Trigger?:     NO
     Rate S/N Ratio:     16.0312195418814  [ if not an image trigger ]
     Image S/N Ratio:    9.07

  Flight Position:   [ source = BAT ]
    RA: 288.957781485581   Dec: 4.19407695074873  [deg; J2000]

  Ground Position:   [ source = BAT pre-slew burst ]
    RA: 288.962786011235   Dec: 4.19625221640243  [deg; J2000]  
        { 19h 15m 51.1s , +04d 11' 46.5" }
         +/- 0.868057129532653 [arcmin] (estimated 90% radius based on SNR)
         +/- 0.288853126344496 [arcmin] (formal 1-sigma fit error)
    SNR: 37.2311551353881
 
  Angular difference between Flight and Ground position is 0.326672 arcmin
 
  Partial Coding Fraction: 1    [ including projection effects ]

  Duration
     T90: 108.800000011921 +/- 84.1058050290632
        Measured from: -106.815999984741
                   to: 1.98400002717972     [s; relative to TRIGTIME]
     T50: 13.0880000591278 +/- 1.67999995946884
        Measured from: -16.3840000033379
                   to: -3.29599994421005     [s; relative to TRIGTIME]



  Fluence
     Peak Flux  (peak 1 second)
        Measured from: -13.8679999709129     
                   to: -12.8679999709129     [s; relative to TRIGTIME]
     Total Fluence        
        Measured from: -111.856000006199     
                   to: 12.1759999990463     [s; relative to TRIGTIME]
     
             Band 1     Band 2     Band 3     Band 4
              15-25      25-50     50-100    100-350     keV
 Total     1.698444   2.277963   1.311061   0.235896
           0.088824   0.090265   0.082060   0.080231 [error]
 Peak      0.088507   0.148304   0.096675   0.018081
           0.008185   0.008800   0.007846   0.006435 [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 5.39e-07 8.73e-07 1.07e-06 2.58e-06 3.21e-06 5.06e-06   erg/cm2
              Error 4.55e-08 4.43e-08 8.11e-08 4.17e-07 1.87e-07 4.84e-07   erg/cm2
Peak flux Power-law 9.00e-01 9.16e-01 6.56e-01 7.50e-01 2.77e+00 3.22e+00   ph/cm2/s
              Error 1.06e-01 6.93e-02 6.18e-02 1.40e-01 2.02e-01 2.41e-01   ph/cm2/s
 
Fluence   Cutoff-PL 5.16e-07 8.99e-07 1.07e-06 1.55e-06 3.11e-06 4.04e-06   erg/cm2
              Error 5.32e-08 5.53e-08 8.49e-08 9.80e-07 2.28e-07 7.24e-07   erg/cm2
Peak flux Cutoff-PL 7.58e-01 1.02e+00 6.97e-01 2.48e-01 2.65e+00 2.72e+00   ph/cm2/s
              Error 1.25e-01 8.98e-02 7.23e-02 1.38e-01 2.09e-01 2.46e-01   ph/cm2/s
 
Fluence        Band 4.90e-07 9.19e-07 1.04e-06 2.19e-06 3.12e-06 4.64e-06   erg/cm2
              Error -------- -------- 8.71e-08 -------- 2.04e-07 --------   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    1.707    0.096    -      -           2.80e-03 1.53e-04   54.420 57
CPL   1.408    0.375      91.2  -30.9      4.04e-03 1.95e-03   52.550 56
 
 
=== 1-s peak spectral analysis ===
 
Model Ph_index Ph_90err Epeak  Epeak_90err Norm     Nomr_90err chi2   dof
PL    1.481    0.120    -      -           2.23e-02 1.68e-03   72.260 57
CPL   0.389    0.597      70.5   18.7      8.29e-02 6.78e-02   59.220 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: 107.456000 sec.
T50 in the 50-300 keV band: 55.296000 sec.

 
=== Table of the duration information ==
 
        Value   tstart    tstop
T100  124.032 -111.856   12.176
T90   108.800 -106.816    1.984
T50    13.088  -16.384   -3.296
Peak    1.000  -13.868  -12.868

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
  288.9628     4.1963   0.0051    10.2673   -91.7735         4.5916489     37.231 TRIG_00641698                 
 
Foreground time interval of the image:
-43.739  10.261 (delta_t =  54.000 [sec])
Background time interval of the image:

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 -111.856 sec. to   12.176 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.70732     ( -0.09593   0.0970521 )
Norm@50keV  : 2.80113E-03    ( -0.000153958   0.000152876 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          54.42 using 59 PHA bins.
# Reduced chi-squared =         0.9547 for     57 degrees of freedom 
# Null hypothesis probability =   5.726275e-01
 
Photon flux (15-150 keV)    in 124 sec: 0.372976 ( -0.0190529  0.0190771 ) ph/cm2/s
Energy fluence (15-150 keV)             : 3.21417e-06 ( -1.86027e-07  1.8775e-07 ) ergs/cm2

Cutoff power-law model

Time interval is from -111.856 sec. to   12.176 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.40772     ( -0.410011   0.339918 )
Epeak [keV] : 91.2379      ( -29.3724 -91.2384 )
Norm@50keV  : 4.04218E-03    ( -0.00132305   0.00258169 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          52.55 using 59 PHA bins.
# Reduced chi-squared =         0.9384 for     56 degrees of freedom 
# Null hypothesis probability =   6.062838e-01
 
Photon flux (15-150 keV)    in 124 sec: 0.366018 ( -0.020841  0.020831 ) ph/cm2/s
Energy fluence (15-150 keV)             : 3.1079e-06 ( -2.27776e-07  2.28668e-07 ) ergs/cm2

Band function

Time interval is from -111.856 sec. to   12.176 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -6.42316E-03   ( -1.52205   3.55392 )
beta        : -1.84518    ( 1.84509   0.152827 )
Epeak [keV] : 36.5556      ( -12.0066 53.462 )
Norm@50keV   : 3.70822E-02    ( -0.0346162   27.6663 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          50.31 using 59 PHA bins.
# Reduced chi-squared =         0.9148 for     55 degrees of freedom 
# Null hypothesis probability =   6.540462e-01
 
Photon flux (15-150 keV)    in 124 sec:  (    ) ph/cm2/s
Energy fluence (15-150 keV)             : 3.11662e-06 ( -3.11575e-06  -2.03546e-07 ) ergs/cm2

Single BB

 
Spectral model blackbody:
------------------------------------------------------------
Parameters  : value    Lower 90%  Upper 90%
kT [keV]    : 12.2103  (  )
R^2/D10^2   : 8.18159E-02  (   )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =         129.21 using 59 PHA bins.
# Reduced chi-squared =         2.2668 for     57 degrees of freedom 
# Null hypothesis probability =   1.581985e-07
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  3.203e-07   3.137e-08
25- 50  1.029e-06   6.039e-08
50-150  9.328e-07   1.167e-07
15-150  2.282e-06   1.364e-07

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 129.917       (-29.1084      37.7653)
Norm        : 1.54542       (-0.0960772     0.115355)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          52.79 using 59 PHA bins.
# Reduced chi-squared =         0.9262 for     57 degrees of freedom 
# Null hypothesis probability =   6.335085e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  4.972e-07   3.980e-08
25- 50  9.015e-07   7.136e-08
50-150  1.671e-06   4.955e-07
15-150  3.070e-06   5.499e-07

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 7.32234        (-1.07192      1.10149)
R1^2/D10^2  : 0.381107        (-0.139033      0.263259)
kT2 [keV]   : 27.0664        (-5.53346      9.7144)
R2^2/D10^2  : 3.35032E-03    (-0.00214411   0.00446537)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          51.01 using 59 PHA bins.
# Reduced chi-squared =         0.9275 for     55 degrees of freedom 
# Null hypothesis probability =   6.277358e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  4.761e-07   7.229e-08
25- 50  9.333e-07   1.264e-07
50-150  1.720e-06   6.044e-07
15-150  3.129e-06   7.490e-07

Peak spectrum fit

Power-law model

Time interval is from  -13.868 sec. to  -12.868 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.48132     ( -0.119248   0.120625 )
Norm@50keV  : 2.22709E-02    ( -0.00168059   0.00167315 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          72.26 using 59 PHA bins.
# Reduced chi-squared =          1.268 for     57 degrees of freedom 
# Null hypothesis probability =   8.385973e-02
 
Photon flux (15-150 keV)    in 1 sec: 2.76655 ( -0.201598  0.201699 ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.11938e-07 ( -1.75978e-08  1.77504e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from  -13.868 sec. to  -12.868 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 0.388872     ( -0.642575   0.550828 )
Epeak [keV] : 70.4717      ( -11.5908 25.8138 )
Norm@50keV  : 8.28881E-02    ( -0.0396161   0.0960289 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          59.22 using 59 PHA bins.
# Reduced chi-squared =          1.058 for     56 degrees of freedom 
# Null hypothesis probability =   3.588502e-01
 
Photon flux (15-150 keV)    in 1 sec: 2.65361 ( -0.20901  0.20899 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.94061e-07 ( -1.9527e-08  1.9827e-08 ) ergs/cm2

Band function

Time interval is from  -13.868 sec. to  -12.868 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -0.388773   ( -0.360648   0.951571 )
beta        : -10.0000    ( 10   20 )
Epeak [keV] : 70.4574      ( -11.5857 25.8067 )
Norm@50keV   : 8.29019E-02    ( -0.03964   0.0961226 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          59.22 using 59 PHA bins.
# Reduced chi-squared =          1.077 for     55 degrees of freedom 
# Null hypothesis probability =   3.242413e-01
 
Photon flux (15-150 keV)    in 1 sec:  (    ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.97222e-07 ( -1.97215e-07  -9.764e-09 ) ergs/cm2

Single BB

 
Spectral model blackbody:
------------------------------------------------------------
Parameters  : value    Lower 90%  Upper 90%
kT [keV]    : 13.9792  (-1.13038  1.26397)
R^2/D10^2   : 0.416379  (-0.109974   0.144813)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          76.99 using 59 PHA bins.
# Reduced chi-squared =          1.351 for     57 degrees of freedom 
# Null hypothesis probability =   4.002520e-02
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.719e-08   2.190e-09
25- 50  6.384e-08   5.850e-09
50-150  8.208e-08   1.236e-08
15-150  1.631e-07   1.340e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 200.000       (      )
Norm        : 11.3865       (-0.817763     0.817748)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          66.55 using 59 PHA bins.
# Reduced chi-squared =          1.167 for     57 degrees of freedom 
# Null hypothesis probability =   1.813481e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  2.836e-08   2.370e-09
25- 50  5.455e-08   7.010e-09
50-150  1.196e-07   3.550e-08
15-150  2.025e-07   4.165e-08

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 9.28608        (-2.15939      1.99357)
R1^2/D10^2  : 1.13810        (-0.463933      1.10802)
kT2 [keV]   : 27.2099        (-7.47917      18.5465)
R2^2/D10^2  : 2.47512E-02    (-0.0207321   0.0464133)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          56.84 using 59 PHA bins.
# Reduced chi-squared =          1.033 for     55 degrees of freedom 
# Null hypothesis probability =   4.064474e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  2.244e-08   7.508e-09
25- 50  6.124e-08   2.377e-08
50-150  1.151e-07   5.477e-08
15-150  1.988e-07   8.260e-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: 1.79336     ( -0.0721314   0.0727758 )
Norm@50keV  : 5.21693E-03    ( -0.000209007   0.000208013 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          66.69 using 59 PHA bins.
# Reduced chi-squared =          1.170 for     57 degrees of freedom 
# Null hypothesis probability =   1.780980e-01
 
Photon flux (15-150 keV)    in 54 sec: 0.717054 ( -0.0277417  0.0277805 ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.59411e-06 ( -1.06393e-07  1.06991e-07 ) ergs/cm2

Cutoff power-law model

Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.33840     ( -0.324112   0.300368 )
Epeak [keV] : 67.7474      ( -11.6881 41.2094 )
Norm@50keV  : 9.02489E-03    ( -0.00268554   0.004236 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          59.77 using 59 PHA bins.
# Reduced chi-squared =          1.067 for     56 degrees of freedom 
# Null hypothesis probability =   3.403797e-01
 
Photon flux (15-150 keV)    in 54 sec: 0.694401 ( -0.031123  0.031179 ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.47097e-06 ( -1.31711e-07  1.32592e-07 ) ergs/cm2

Band function

 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -0.106087   ( -1.57187   3.03038 )
beta        : -1.95326    ( 1.94739   0.124845 )
Epeak [keV] : 37.0336      ( -9.04904 41.9634 )
Norm@50keV   : 6.18388E-02    ( -0.061025   16.9297 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          57.20 using 59 PHA bins.
# Reduced chi-squared =          1.040 for     55 degrees of freedom 
# Null hypothesis probability =   3.933908e-01
 
Photon flux (15-150 keV)    in 54 sec:  (    ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.49712e-06 ( -2.49674e-06  -1.26463e-07 ) ergs/cm2

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

S(25-50 keV)  = 8.73e-07
S(50-100 keV) = 1.07e-06

T90 vs. Hardness ratio plot

T90                                   = 108.800000011921 sec.
Hardness ratio (energy fluence ratio) = 1.22566

Color vs. Color plot

Count Ratio  (25-50 keV) / (15-25 keV) = 1.34121
Count Ratio (50-100 keV) / (15-25 keV) = 0.771919

Mask shadow pattern

IMX = -5.606019335997852E-03, IMY = 1.810553663361952E-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:

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

Time interval of the image:
-43.739400 10.260600
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
244.9747 -15.6343    0.8  38.2  110.9   6.8867  14.9    0.4	Sco X-1                       
254.6596  35.3020   11.1  45.9 -168.4  -0.2408  -1.0   10.2	Her X-1                       
256.5702 -36.4966    6.9  40.7   74.1   0.9313   1.7    7.9	GX 349+2                      
263.0416 -24.6858   42.9  28.1   80.5  -0.0569  -0.3    4.0	GX 1+4                        
268.2875  -1.4248    4.6  13.4  139.0   0.3096   2.5    5.1	SW J1753.5-0127               
270.3381 -25.2163    9.8  24.7   67.6  -0.2085  -1.2    8.7	GX 5-1                        
270.1478 -25.6763    7.5  25.2   67.5   0.2940   1.7    9.3	GRS 1758-258                  
273.9770 -13.9377    4.1  13.3   76.7   0.3278   2.8    6.2	GX 17+2                       
276.0475 -30.4475   15.1  28.0   52.9   0.1362   0.8    8.0	H1820-303                     
285.1132 -24.8012    9.6  22.1   34.1   0.1506   1.2    8.3	HT1900.1-2455                 
288.7909  11.0375    7.2  15.7 -110.6   0.1884   1.6    5.5	GRS 1915+105                  
299.6293  35.2621    3.5  41.8 -115.2   1.4306   3.3    4.1	Cyg X-1                       
263.0234 -33.8815    5.1  35.4   69.8   0.7430   2.3    3.3	GX 354-0                      
288.9628   4.1962    0.3  10.3  -91.8   4.5914  37.2 ------	UNKNOWN

Post-slew image of 15-350 keV band

Time interval of the image:
45.460600 522.760600
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
254.5097  35.3796    3.3  44.5  170.9   3.1131   3.5    3.4	Her X-1                       
262.9098 -24.6519    5.4  38.4   72.0   2.8910   2.1    7.8	GX 1+4                        
268.4352  -1.5768   13.3  21.3  106.7  -0.4142  -0.9    8.5	SW J1753.5-0127               
270.2335 -25.1055    3.3  34.5   62.9   2.9974   3.5    3.2	GX 5-1                        
270.5082 -25.7641    4.4  34.9   61.9   2.1442   2.6   11.2	GRS 1758-258                  
273.9455 -14.0370    3.2  23.5   71.0   1.8691   3.6    3.5	GX 17+2                       
276.0052 -30.2731    4.0  36.6   50.9   2.4390   2.9    7.0	H1820-303                     
285.1921 -24.9209    4.6  29.3   39.0   1.2183   2.5    8.5	HT1900.1-2455                 
288.7922  10.9271    1.5   6.8 -149.3   2.8143   7.6    1.2	GRS 1915+105                  
299.5930  35.1962    0.5  32.5 -131.7  13.6044  22.9    0.3	Cyg X-1                       
308.1614  40.9820    3.4  40.7 -125.6   2.8900   3.3    2.9	Cyg X-3                       
248.1136  44.8750    4.0  54.1  177.1   5.4551   2.9 ------	UNKNOWN                       
286.5856  14.2716    2.8  10.4 -160.9   1.5342   4.1 ------	UNKNOWN                       
328.0953   5.2345    2.8  39.0  -61.2   3.8062   4.2 ------	UNKNOWN                       
290.6787  59.0099    4.9  54.9 -146.9   5.2477   2.4 ------	UNKNOWN

Plot creation:
Fri Jun 26 00:48:23 EDT 2015