batgrbproduct analysis for trigger=518200

batgrbproduct Analysis for Trigger=518200

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 05:27:20 EST 2014
             Host Name: batevent1
   Current Working Dir: /local/data/batevent/batevent_reproc/trigger518200
======================================================================

  Trigger: 00518200      Segment: 000

  BAT Trigger Time: 353937383.616   [s; MET]
      Trigger Stop: 353937410.496   [s; MET]
               UTC: 2012-03-20T11:56:15.603640    [includes UTCF correction] 
       Where From?: TDRSS position message

  BAT 
    RA: 212.53789490183   Dec: 8.68498369747149  [deg; J2000]

     Catalogged Source?: NO
     Point Source?:      YES
     GRB Indicated?:     YES    [ by BAT flight software ]
     Image S/N Ratio:    10.06
     Image Trigger?:     NO
     Rate S/N Ratio:     12.9614813968157  [ if not an image trigger ]
     Image S/N Ratio:    10.06

  Flight Position:   [ source = BAT ]
    RA: 212.53789490183   Dec: 8.68498369747149  [deg; J2000]

  Ground Position:   [ source = BAT pre-slew burst ]
    RA: 212.51656289908   Dec: 8.68152229462087  [deg; J2000]  
        { 14h 10m 04.0s , +08d 40' 53.5" }
         +/- 1.60948988386926 [arcmin] (estimated 90% radius based on SNR)
         +/- 0.741459408410574 [arcmin] (formal 1-sigma fit error)
    SNR: 15.4116610679366
 
  Angular difference between Flight and Ground position is 1.282182 arcmin
 
  Partial Coding Fraction: 0.6015625    [ including projection effects ]

  Duration
     T90: 24.9759999513626 +/- 3.54538684013936
        Measured from: 0.84799998998642
                   to: 25.823999941349     [s; relative to TRIGTIME]
     T50: 16.9359999299049 +/- 2.80228762218953
        Measured from: 6.27200001478195
                   to: 23.2079999446869     [s; relative to TRIGTIME]



  Fluence
     Peak Flux  (peak 1 second)
        Measured from: 24.0960000157356     
                   to: 25.0960000157356     [s; relative to TRIGTIME]
     Total Fluence        
        Measured from: -0.015999972820282     
                   to: 29.8560000061989     [s; relative to TRIGTIME]
     
             Band 1     Band 2     Band 3     Band 4
              15-25      25-50     50-100    100-350     keV
 Total     0.290419   0.380584   0.281643   0.039128
           0.041247   0.037120   0.032255   0.027736 [error]
 Peak      0.020071   0.014868   0.025458   0.010549
           0.007453   0.006923   0.005914   0.005137 [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 8.96e-08 1.58e-07 2.12e-07 5.86e-07 6.16e-07 1.05e-06   erg/cm2
              Error 1.58e-08 1.75e-08 3.08e-08 1.78e-07 7.45e-08 2.04e-07   erg/cm2
Peak flux Power-law 1.32e-01 1.62e-01 1.45e-01 2.23e-01 5.16e-01 6.62e-01   ph/cm2/s
              Error 8.04e-02 6.05e-02 4.72e-02 1.65e-01 1.62e-01 2.04e-01   ph/cm2/s
 
Fluence   Cutoff-PL 7.41e-08 1.78e-07 2.17e-07 1.24e-07 5.53e-07 5.93e-07   erg/cm2
              Error 1.87e-08 2.30e-08 3.67e-08 1.36e-07 8.24e-08 1.58e-07   erg/cm2
Peak flux Cutoff-PL 1.15e-01 1.70e-01 1.53e-01 1.16e-01 5.00e-01 5.54e-01   ph/cm2/s
              Error 1.09e-01 7.24e-02 5.91e-02 1.35e-01 1.91e-01 2.78e-01   ph/cm2/s
 
Fluence        Band 7.33e-08 1.77e-07 2.17e-07 1.31e-07 5.53e-07 6.03e-07   erg/cm2
              Error 1.82e-08 2.26e-08 -------- -------- -------- --------   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    1.572    0.184    -      -           2.20e-03 2.46e-04   64.130 57
CPL   0.314    0.947      63.3   23.9      9.96e-03 1.55e-02   56.990 56
 
 
=== 1-s peak spectral analysis ===
 
Model Ph_index Ph_90err Epeak  Epeak_90err Norm     Nomr_90err chi2   dof
PL    1.163    0.553    -      -           4.42e-03 1.32e-03   66.160 57
CPL   0.530    8.010     122.9    0.0      8.86e-03 1.93e+01   66.050 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: 26.752000 sec.
T50 in the 50-300 keV band: 19.008000 sec.

 
=== Table of the duration information ==
 
        Value   tstart    tstop
T100   29.872   -0.016   29.856
T90    24.976    0.848   25.824
T50    16.936    6.272   23.208
Peak    1.000   24.096   25.096

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
  212.5166     8.6815   0.0125    23.7030   117.8942         1.1165221     15.412 TRIG_00518200                 
 
Foreground time interval of the image:
 -0.016  29.856 (delta_t =  29.872 [sec])
Background time interval of the image:
-239.616  -0.016 (delta_t = 239.600 [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 26.880000

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 26.880000

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 26.880000

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   -0.016 sec. to   29.856 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.57166     ( -0.182645   0.184875 )
Norm@50keV  : 2.19649E-03    ( -0.000246774   0.00024529 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          64.13 using 59 PHA bins.
# Reduced chi-squared =          1.125 for     57 degrees of freedom 
# Null hypothesis probability =   2.408850e-01
 
Photon flux (15-150 keV)    in 29.87 sec: 0.279837 ( -0.0307238  0.0307924 ) ph/cm2/s
Energy fluence (15-150 keV)             : 6.15833e-07 ( -7.40471e-08  7.50194e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from   -0.016 sec. to   29.856 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 0.313765     ( -1.05251   0.841526 )
Epeak [keV] : 63.2855      ( -11.9922 35.8908 )
Norm@50keV  : 9.96298E-03    ( -0.00626168   0.0248162 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          56.99 using 59 PHA bins.
# Reduced chi-squared =          1.018 for     56 degrees of freedom 
# Null hypothesis probability =   4.379510e-01
 
Photon flux (15-150 keV)    in 29.87 sec: 0.263654 ( -0.032336  0.032451 ) ph/cm2/s
Energy fluence (15-150 keV)             : 5.52831e-07 ( -8.05086e-08  8.43559e-08 ) ergs/cm2

Band function

Time interval is from   -0.016 sec. to   29.856 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -0.313642   ( -0.661396   1.14057 )
beta        : -10.0000    ( 10   0 )
Epeak [keV] : 63.2727      ( -11.0067 35.8849 )
Norm@50keV   : 9.96515E-03    ( -0.00626419   0.0248946 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          56.99 using 59 PHA bins.
# Reduced chi-squared =          1.036 for     55 degrees of freedom 
# Null hypothesis probability =   4.008561e-01
 
Photon flux (15-150 keV)    in 29.87 sec: 0.266353 (    ) ph/cm2/s
Energy fluence (15-150 keV)             : 5.53443e-07 ( 0  0 ) ergs/cm2

Single BB

 
Spectral model blackbody:
------------------------------------------------------------
Parameters  : value    Lower 90%  Upper 90%
kT [keV]    : 13.7346  (-1.60299  1.8561)
R^2/D10^2   : 4.35044E-02  (-0.0159825   0.0246372)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          64.04 using 59 PHA bins.
# Reduced chi-squared =          1.124 for     57 degrees of freedom 
# Null hypothesis probability =   2.431191e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  5.186e-08   1.141e-08
25- 50  1.892e-07   2.646e-08
50-150  2.327e-07   5.073e-08
15-150  4.738e-07   7.049e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 163.938       (-62.7132      -162.677)
Norm        : 1.16241       (-0.134983     0.15765)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          60.53 using 59 PHA bins.
# Reduced chi-squared =          1.062 for     57 degrees of freedom 
# Null hypothesis probability =   3.496688e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  8.845e-08   4.938e-08
25- 50  1.660e-07   8.852e-08
50-150  3.395e-07   1.925e-07
15-150  5.939e-07   3.230e-07

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 7.47994        (-3.29541      42.7455)
R1^2/D10^2  : 0.193159        (-0.131885      1.03765)
kT2 [keV]   : 20.2756        (-5.45242      29.9442)
R2^2/D10^2  : 7.88115E-03    (-0.00762453   0.0137839)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          56.44 using 59 PHA bins.
# Reduced chi-squared =          1.026 for     55 degrees of freedom 
# Null hypothesis probability =   4.208066e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  7.382e-08   4.143e-08
25- 50  1.790e-07   9.095e-08
50-150  3.027e-07   1.701e-07
15-150  5.556e-07   2.839e-07

Peak spectrum fit

Power-law model

Time interval is from   24.096 sec. to   25.096 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.16338     ( -0.577085   0.528555 )
Norm@50keV  : 4.41818E-03    ( -0.00132342   0.00131253 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          66.16 using 59 PHA bins.
# Reduced chi-squared =          1.161 for     57 degrees of freedom 
# Null hypothesis probability =   1.900653e-01
 
Photon flux (15-150 keV)    in 1 sec: 0.516098 ( -0.160381  0.162797 ) ph/cm2/s
Energy fluence (15-150 keV)             : 4.53002e-08 ( -1.41784e-08  1.44294e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from   24.096 sec. to   25.096 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 0.530083     ( -8.64316   7.37686 )
Epeak [keV] : 122.852      ( -122.768 -122.768 )
Norm@50keV  : 8.86316E-03    ( -0.00887209   38.6465 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          66.05 using 59 PHA bins.
# Reduced chi-squared =          1.179 for     56 degrees of freedom 
# Null hypothesis probability =   1.685527e-01
 
Photon flux (15-150 keV)    in 1 sec: 0.500255 ( -0.207998  0.17449 ) ph/cm2/s
Energy fluence (15-150 keV)             : 4.31361e-08 ( -1.89485e-08  1.62391e-08 ) ergs/cm2

Band function

Time interval is from   24.096 sec. to   25.096 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : 0.505867   ( 0.0910513   0.0910513 )
beta        : -1.86986    ( 1.62965   0.972762 )
Epeak [keV] : 76.5099      ( -76.3016 240.122 )
Norm@50keV   : 2.77164E-02    ( -0.0278759   16.0961 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          65.53 using 59 PHA bins.
# Reduced chi-squared =          1.191 for     55 degrees of freedom 
# Null hypothesis probability =   1.564958e-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]    : 17.6493  (-4.82662  8.78835)
R^2/D10^2   : 3.64944E-02  (-0.0364937   0.0726985)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          66.53 using 59 PHA bins.
# Reduced chi-squared =          1.167 for     57 degrees of freedom 
# Null hypothesis probability =   1.816584e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  2.290e-09   1.454e-09
25- 50  1.044e-08   6.201e-09
50-150  2.347e-08   1.598e-08
15-150  3.619e-08   2.214e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 199.363       (-106.734      -199.363)
Norm        : 2.18385       (-0.65887     0.65887)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          67.58 using 59 PHA bins.
# Reduced chi-squared =          1.186 for     57 degrees of freedom 
# Null hypothesis probability =   1.593932e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  5.438e-09   3.369e-09
25- 50  1.046e-08   6.420e-09
50-150  2.294e-08   1.414e-08
15-150  3.884e-08   2.344e-08

Double BB

------------------------------------------------------------
#Fit statistic : Chi-Squared =          66.26 using 59 PHA bins.
#Fit statistic : Chi-Squared =          64.82 using 59 PHA bins.
#Fit statistic : Chi-Squared =          64.64 using 59 PHA bins.
#Fit statistic : Chi-Squared =          64.53 using 59 PHA bins.
# Reduced chi-squared =          1.205 for     55 degrees of freedom 
# Reduced chi-squared =          1.179 for     55 degrees of freedom 
# Reduced chi-squared =          1.175 for     55 degrees of freedom 
# Reduced chi-squared =          1.173 for     55 degrees of freedom 
# Null hypothesis probability =   1.421082e-01
# Null hypothesis probability =   1.713575e-01
# Null hypothesis probability =   1.753614e-01
# Null hypothesis probability =   1.777370e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  3.346e-09   1.825e-09
25- 50  9.952e-09   5.995e-09
50-150  2.439e-08   1.576e-08
15-150  3.769e-08   2.223e-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: 1.57166     ( -0.182645   0.184875 )
Norm@50keV  : 2.19649E-03    ( -0.000246774   0.00024529 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          64.13 using 59 PHA bins.
# Reduced chi-squared =          1.125 for     57 degrees of freedom 
# Null hypothesis probability =   2.408850e-01
 
Photon flux (15-150 keV)    in 29.87 sec: 0.279837 ( -0.0307238  0.0307924 ) ph/cm2/s
Energy fluence (15-150 keV)             : 6.15833e-07 ( -7.40471e-08  7.50194e-08 ) ergs/cm2

Cutoff power-law model

Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 0.313765     ( -1.05251   0.841526 )
Epeak [keV] : 63.2855      ( -11.9922 35.8908 )
Norm@50keV  : 9.96298E-03    ( -0.00626168   0.0248162 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          56.99 using 59 PHA bins.
# Reduced chi-squared =          1.018 for     56 degrees of freedom 
# Null hypothesis probability =   4.379510e-01
 
Photon flux (15-150 keV)    in 29.87 sec: 0.263654 ( -0.032336  0.032451 ) ph/cm2/s
Energy fluence (15-150 keV)             : 5.52831e-07 ( -8.05086e-08  8.43559e-08 ) ergs/cm2

Band function

 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -0.313642   ( -0.661396   1.14057 )
beta        : -10.0000    ( 10   20 )
Epeak [keV] : 63.2727      ( -11.0067 35.8849 )
Norm@50keV   : 9.96515E-03    ( -0.00626419   0.0248946 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          56.99 using 59 PHA bins.
# Reduced chi-squared =          1.036 for     55 degrees of freedom 
# Null hypothesis probability =   4.008561e-01
 
Photon flux (15-150 keV)    in 29.87 sec: 0.266353 (    ) ph/cm2/s
Energy fluence (15-150 keV)             : 5.53443e-07 ( 0  0 ) ergs/cm2

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

S(25-50 keV)  = 1.58e-07
S(50-100 keV) = 2.12e-07

T90 vs. Hardness ratio plot

T90                                   = 24.9759999513626 sec.
Hardness ratio (energy fluence ratio) = 1.34177

Color vs. Color plot

Count Ratio  (25-50 keV) / (15-25 keV) = 1.31047
Count Ratio (50-100 keV) / (15-25 keV) = 0.969782

Mask shadow pattern

IMX = -2.053962601929236E-01, IMY = -3.880213364858037E-01

TIME vs. PHA plot around the trigger time

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 26.880000

TIME vs. DetID plot around the trigger time

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 26.880000

100 us light curve (15-350 keV)

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 26.880000

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:
-239.616000 -0.016000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
244.9728 -15.6387    0.2  17.6  -86.9  17.6455  69.0    0.4	Sco X-1                       
254.4611  35.3767    4.9  50.9 -172.7   1.4637   2.4    2.1	Her X-1                       
256.0729 -37.9751    7.4  38.2  -56.9   0.7358   1.6    8.9	4U 1700-377                   
256.5297 -36.3130    6.8  37.4  -59.3   0.8297   1.7    8.0	GX 349+2                      
262.8184 -24.8450    0.0  36.5  -80.4   0.8863   1.6   12.0	GX 1+4                        
268.3585  -1.5706    4.9  40.6 -118.7   1.4202   2.3    7.1	SW J1753.5-0127               
262.8927 -33.7747   10.6  40.3  -67.4  -0.7150  -1.1    6.0	GX 354-0                      
197.0102  18.2257    4.2  41.2  111.3   2.5349   2.7 ------	UNKNOWN                       
217.0223 -47.6052    2.5  39.6   -8.5   1.4571   4.6 ------	UNKNOWN                       
266.3770  31.8104    2.7  54.8 -160.4   3.0835   4.2 ------	UNKNOWN                       
269.8885  30.8267    3.0  56.5 -157.1   3.8119   3.8 ------	UNKNOWN

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

Time interval of the image:
-0.016000 29.856000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
245.1360 -15.5360    4.3  17.7  -87.4   0.1747   2.7   11.0	Sco X-1                       
254.4214  35.4891    8.3  51.0 -172.8   0.2042   1.4    9.0	Her X-1                       
255.9988 -37.7160    8.2  38.0  -57.1  -0.1615  -1.4    7.7	4U 1700-377                   
256.5541 -36.2997  112.9  37.4  -59.3   0.0116   0.1    9.4	GX 349+2                      
263.1903 -24.6862    6.1  36.7  -80.9  -0.2492  -1.9   10.5	GX 1+4                        
268.3156  -1.4148   56.6  40.6 -118.9   0.0317   0.2    3.9	SW J1753.5-0127               
263.1368 -33.9566    0.0  40.5  -67.3  -0.5541  -3.2   10.4	GX 354-0                      
212.5166   8.6816    0.7  23.7  117.9   1.1165  15.4 ------	UNKNOWN                       
201.0140 -54.3044    2.3  50.1    0.0   0.6867   5.1 ------	UNKNOWN                       
210.0382 -54.8055    2.6  47.9   -6.3   0.4909   4.4 ------	UNKNOWN                       
222.0925 -56.4712    2.3  47.6  -15.8   0.5673   5.0 ------	UNKNOWN                       
254.4001 -54.3792    2.4  49.8  -40.0   0.9586   4.7 ------	UNKNOWN

Post-slew image of 15-350 keV band

Time interval of the image:
154.684590 962.510000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
244.9754 -15.6332    0.3  40.3  -39.2  37.1548  42.1    0.5	Sco X-1                       
207.6997  13.1204    3.1   6.5  147.2   1.6755   3.8 ------	UNKNOWN                       
224.5604 -41.5813    2.4  51.5    2.4   5.9154   4.9 ------	UNKNOWN                       
211.1101  59.3227    3.5  50.7 -167.1   4.2325   3.3 ------	UNKNOWN

Plot creation:
Sat May 30 20:00:09 EDT 2015