batgrbproduct analysis for trigger=342121

batgrbproduct Analysis for Trigger=342121

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): Sun Jan 19 18:49:22 EST 2014
             Host Name: batevent1
   Current Working Dir: /local/data/batevent/batevent_reproc/trigger342121
======================================================================

  Trigger: 00342121      Segment: 000

  BAT Trigger Time: 255567799.296   [s; MET]
      Trigger Stop: 255567803.392   [s; MET]
               UTC: 2009-02-05T23:03:14.820740    [includes UTCF correction] 
       Where From?: TDRSS position message

  BAT 
    RA: 220.925433877431   Dec: -27.8637399346592  [deg; J2000]

     Catalogged Source?: NO
     Point Source?:      YES
     GRB Indicated?:     YES    [ by BAT flight software ]
     Image S/N Ratio:    8.16
     Image Trigger?:     NO
     Rate S/N Ratio:     15.1327459504216  [ if not an image trigger ]
     Image S/N Ratio:    8.16

  Flight Position:   [ source = BAT ]
    RA: 220.925433877431   Dec: -27.8637399346592  [deg; J2000]

  Ground Position:   [ source = BAT pre-slew burst ]
    RA: 220.91650989556   Dec: -27.8492183299414  [deg; J2000]  
        { 14h 43m 40.0s , -27d 50' 57.2" }
         +/- 1.99605923167749 [arcmin] (estimated 90% radius based on SNR)
         +/- 0.89193218931916 [arcmin] (formal 1-sigma fit error)
    SNR: 11.3318078597344
 
  Angular difference between Flight and Ground position is 0.991594 arcmin
 
  Partial Coding Fraction: 1.015625    [ including projection effects ]

  Duration
     T90: 8.8120000064373 +/- 1.77945720942472
        Measured from: -2.60400000214577
                   to: 6.20800000429153     [s; relative to TRIGTIME]
     T50: 4.33200001716614 +/- 1.06734248169701
        Measured from: 0.00799998641014099
                   to: 4.34000000357628     [s; relative to TRIGTIME]



  Fluence
     Peak Flux  (peak 1 second)
        Measured from: 4.0799999833107     
                   to: 5.0799999833107     [s; relative to TRIGTIME]
     Total Fluence        
        Measured from: -2.9200000166893     
                   to: 6.62399998307228     [s; relative to TRIGTIME]
     
             Band 1     Band 2     Band 3     Band 4
              15-25      25-50     50-100    100-350     keV
 Total     0.164760   0.171229   0.062367  -0.011050
           0.016961   0.016448   0.013997   0.011884 [error]
 Peak      0.030009   0.021611   0.009052   0.001841
           0.005569   0.005361   0.004557   0.003763 [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 4.53e-08 6.12e-08 6.10e-08 1.10e-07 2.03e-07 2.77e-07   erg/cm2
              Error 7.09e-09 7.20e-09 1.24e-08 4.32e-08 2.89e-08 5.77e-08   erg/cm2
Peak flux Power-law 2.11e-01 1.60e-01 8.11e-02 5.90e-02 4.79e-01 5.11e-01   ph/cm2/s
              Error 7.20e-02 4.07e-02 3.37e-02 4.68e-02 1.21e-01 1.32e-01   ph/cm2/s
 
Fluence   Cutoff-PL 4.09e-08 7.29e-08 5.09e-08 1.04e-08 1.74e-07 1.75e-07   erg/cm2
              Error 8.12e-09 1.07e-08 1.70e-08 2.29e-08 3.00e-08 3.74e-08   erg/cm2
Peak flux Cutoff-PL 1.99e-01 2.10e-01 3.37e-02 3.03e-04 4.42e-01 4.42e-01   ph/cm2/s
              Error 8.12e-02 6.50e-02 5.09e-02 2.54e-02 1.16e-01 1.16e-01   ph/cm2/s
 
Fluence        Band 4.04e-08 7.30e-08 5.00e-08 2.57e-08 1.77e-07 1.90e-07   erg/cm2
              Error 7.97e-09 1.07e-08 -------- 3.06e-08 -------- 5.53e-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    2.005    0.212    -      -           2.31e-03 3.45e-04   68.410 57
CPL   0.393    1.300      38.4    8.8      2.17e-02 8.81e-02   61.590 56
 
 
=== 1-s peak spectral analysis ===
 
Model Ph_index Ph_90err Epeak  Epeak_90err Norm     Nomr_90err chi2   dof
PL    1.980    0.457    -      -           3.23e-03 1.04e-03   52.550 57
CPL  -1.005    4.407      32.4    0.0      3.25e-01 0.00e+00   50.330 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: 0.000000 sec.
T50 in the 50-300 keV band: 0.000000 sec.

 
=== Table of the duration information ==
 
        Value   tstart    tstop
T100    9.544   -2.920    6.624
T90     8.812   -2.604    6.208
T50     4.332    0.008    4.340
Peak    1.000    4.080    5.080

Click here for the BAT GCN circular template

Special notes of this burst

Image

Pre-slew 15.0-350.0 keV image (Event data)

#   RAcent    DECcent   POSerr    Theta     Phi              Peak Cts       SNR   Name
  220.9165   -27.8492   0.0170    10.6095   -28.1507         0.3474018     11.332 TRIG_00342121                 
 
Foreground time interval of the image:
 -2.920   6.624 (delta_t =   9.544 [sec])
Background time interval of the image:
-239.296  -2.920 (delta_t = 236.376 [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)

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   -2.920 sec. to    6.624 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 2.00539     ( -0.206298   0.218288 )
Norm@50keV  : 2.30738E-03    ( -0.000347606   0.000341427 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          68.41 using 59 PHA bins.
# Reduced chi-squared =          1.200 for     57 degrees of freedom 
# Null hypothesis probability =   1.432287e-01
 
Photon flux (15-150 keV)    in 9.544 sec: 0.346968 ( -0.0401275  0.0401291 ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.03136e-07 ( -2.84415e-08  2.92824e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from   -2.920 sec. to    6.624 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 0.392538     ( -1.48315   1.11738 )
Epeak [keV] : 38.4188      ( -7.62232 9.93531 )
Norm@50keV  : 2.16896E-02    ( -0.0216898   0.154543 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          61.59 using 59 PHA bins.
# Reduced chi-squared =          1.100 for     56 degrees of freedom 
# Null hypothesis probability =   2.830215e-01
 
Photon flux (15-150 keV)    in 9.544 sec: 0.329564 ( -0.040995  0.041283 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.73588e-07 ( -2.75707e-08  3.24162e-08 ) ergs/cm2

Band function

Time interval is from   -2.920 sec. to    6.624 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -0.397089   ( -0.998138   1.82468 )
beta        : -9.99999    ( 9.99999   20 )
Epeak [keV] : 38.4233      ( -6.58103 10.2549 )
Norm@50keV   : 2.15477E-02    ( -0.0215477   0.154947 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          61.59 using 59 PHA bins.
# Reduced chi-squared =          1.120 for     55 degrees of freedom 
# Null hypothesis probability =   2.521842e-01
 
Photon flux (15-150 keV)    in 9.544 sec:  (    ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.77486e-07 ( 0  0 ) ergs/cm2

Single BB

 
Spectral model blackbody:
------------------------------------------------------------
Parameters  : value    Lower 90%  Upper 90%
kT [keV]    : 9.57664  (-1.09526  1.24632)
R^2/D10^2   : 0.196841  (-0.0745255   0.118382)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          66.03 using 59 PHA bins.
# Reduced chi-squared =          1.158 for     57 degrees of freedom 
# Null hypothesis probability =   1.930577e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  3.452e-08   7.144e-09
25- 50  8.064e-08   1.378e-08
50-150  3.708e-08   1.233e-08
15-150  1.522e-07   2.305e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 59.4585       (-16.763      27.8495)
Norm        : 1.84477       (-0.32582     0.390133)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          63.33 using 59 PHA bins.
# Reduced chi-squared =          1.111 for     57 degrees of freedom 
# Null hypothesis probability =   2.631161e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  4.418e-08   6.996e-09
25- 50  6.706e-08   8.876e-09
50-150  7.573e-08   2.758e-08
15-150  1.870e-07   3.584e-08

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 4.64554        (-2.64554      -4.64895)
R1^2/D10^2  : 1.30010        (-1.10705      69.2036)
kT2 [keV]   : 12.0874        (-2.61875      -12.0933)
R2^2/D10^2  : 6.45993E-02    (-0.0643658   0.131253)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          61.65 using 59 PHA bins.
# Reduced chi-squared =          1.121 for     55 degrees of freedom 
# Null hypothesis probability =   2.503952e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  4.134e-08   2.190e-08
25- 50  7.259e-08   3.794e-08
50-150  5.375e-08   3.226e-08
15-150  1.677e-07   8.580e-08

Peak spectrum fit

Power-law model

Time interval is from    4.080 sec. to    5.080 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.97980     ( -0.436086   0.478599 )
Norm@50keV  : 3.22511E-03    ( -0.00105012   0.00102182 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          52.55 using 59 PHA bins.
# Reduced chi-squared =         0.9219 for     57 degrees of freedom 
# Null hypothesis probability =   6.426421e-01
 
Photon flux (15-150 keV)    in 1 sec: 0.479327 ( -0.121119  0.12112 ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.97148e-08 ( -8.89447e-09  9.46552e-09 ) ergs/cm2

Cutoff power-law model

Time interval is from    4.080 sec. to    5.080 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: -1.00527     ( -5.66656   3.14782 )
Epeak [keV] : 32.3553      (   )
Norm@50keV  : 0.325059    (     )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          50.33 using 59 PHA bins.
# Reduced chi-squared =         0.8988 for     56 degrees of freedom 
# Null hypothesis probability =   6.882595e-01
 
Photon flux (15-150 keV)    in 1 sec: 0.442273 ( -0.114448  0.1184 ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.10853e-08 ( -6.0779e-09  1.25492e-08 ) ergs/cm2

Band function

Time interval is from    4.080 sec. to    5.080 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : 5.00000   ( -5.95219   -5 )
beta        : -2.52114    ( -2.02031   0.665093 )
Epeak [keV] : 24.7411      ( -5.90291 6.52825 )
Norm@50keV   : 651.642    ( -156.478   3141.14 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          48.03 using 59 PHA bins.
# Reduced chi-squared =         0.8733 for     55 degrees of freedom 
# Null hypothesis probability =   7.357903e-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]    : 8.20700  (-1.74294  2.31286)
R^2/D10^2   : 0.505706  (-0.319724   0.801003)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          50.36 using 59 PHA bins.
# Reduced chi-squared =         0.8836 for     57 degrees of freedom 
# Null hypothesis probability =   7.205042e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  6.273e-09   3.281e-09
25- 50  1.147e-08   6.495e-09
50-150  3.274e-09   2.365e-09
15-150  2.102e-08   1.062e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 55.4047       (-27.5519      102.059)
Norm        : 2.64205       (-0.942694     1.55597)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          51.54 using 59 PHA bins.
# Reduced chi-squared =         0.9042 for     57 degrees of freedom 
# Null hypothesis probability =   6.793783e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  6.547e-09   2.614e-09
25- 50  9.715e-09   4.916e-09
50-150  1.033e-08   7.465e-09
15-150  2.659e-08   1.515e-08

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 7.43773        (-7.43682      2.29753)
R1^2/D10^2  : 0.688953        (-0.689224      1.5144)
kT2 [keV]   : 55.4873        (-55.3737      -55.3737)
R2^2/D10^2  : 3.40793E-04    (-0.000342441   0.00783196)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          48.15 using 59 PHA bins.
# Reduced chi-squared =         0.8755 for     55 degrees of freedom 
# Null hypothesis probability =   7.316460e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  6.598e-09   3.858e-09
25- 50  1.075e-08   6.490e-09
50-150  1.254e-08   6.165e-09
15-150  2.989e-08   1.422e-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: 2.00539     ( -0.206298   0.218288 )
Norm@50keV  : 2.30738E-03    ( -0.000347606   0.000341427 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          68.41 using 59 PHA bins.
# Reduced chi-squared =          1.200 for     57 degrees of freedom 
# Null hypothesis probability =   1.432287e-01
 
Photon flux (15-150 keV)    in 9.544 sec: 0.346968 ( -0.0401275  0.0401291 ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.03136e-07 ( -2.84415e-08  2.92824e-08 ) ergs/cm2

Cutoff power-law model

Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 0.392538     ( -1.48315   1.11738 )
Epeak [keV] : 38.4188      ( -7.62232 9.93525 )
Norm@50keV  : 2.16896E-02    ( -0.0216898   0.154543 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          61.59 using 59 PHA bins.
# Reduced chi-squared =          1.100 for     56 degrees of freedom 
# Null hypothesis probability =   2.830215e-01
 
Photon flux (15-150 keV)    in 9.544 sec: 0.329564 ( -0.040995  0.041283 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.73588e-07 ( -2.75707e-08  3.24162e-08 ) ergs/cm2

Band function

 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -0.397089   ( -0.998138   1.82468 )
beta        : -9.99999    ( 9.99999   20 )
Epeak [keV] : 38.4233      ( -6.58103 10.2549 )
Norm@50keV   : 2.15477E-02    ( -0.0215477   0.154947 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          61.59 using 59 PHA bins.
# Reduced chi-squared =          1.120 for     55 degrees of freedom 
# Null hypothesis probability =   2.521842e-01
 
Photon flux (15-150 keV)    in 9.544 sec:  (    ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.77486e-07 ( 0  0 ) ergs/cm2

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

S(25-50 keV)  = 6.12e-08
S(50-100 keV) = 6.10e-08

T90 vs. Hardness ratio plot

T90                                   = 8.8120000064373 sec.
Hardness ratio (energy fluence ratio) = 0.996732

Color vs. Color plot

Count Ratio  (25-50 keV) / (15-25 keV) = 1.03926
Count Ratio (50-100 keV) / (15-25 keV) = 0.378532

Mask shadow pattern

IMX = 1.651591959193517E-01, IMY = 8.837470254186201E-02

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 -2.920000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
170.2797 -60.5372    6.6  56.1    0.6   1.7050   1.7    5.3	Cen X-3                       
186.8535 -62.8233    5.2  51.2   -7.5   1.0728   2.2    6.3	GX 301-2                      
244.9670 -15.6373    0.3  23.4 -116.9   9.1958  41.4    0.7	Sco X-1                       
255.9805 -37.7941    1.8  37.2  -75.8   3.0398   6.4    3.0	4U 1700-377                   
256.4624 -36.3036   14.1  37.0  -78.3   0.3825   0.8    7.3	GX 349+2                      
263.1632 -24.8185   36.9  40.3  -98.2   0.2970   0.3    9.5	GX 1+4                        
196.4051 -26.3488    3.0  24.2   37.2   0.7688   3.8 ------	UNKNOWN                       
167.5647 -59.6132    3.0  56.9    2.3   3.8744   3.8 ------	UNKNOWN                       
221.7988 -22.4933    2.1   5.4  -38.7   0.9725   5.6 ------	UNKNOWN                       
250.4023  10.6094    3.0  40.6 -157.8   1.0367   3.9 ------	UNKNOWN                       
254.7683 -29.6631    2.5  33.6  -88.5   1.6575   4.6 ------	UNKNOWN

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

Time interval of the image:
-2.920000 6.624000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
170.3808 -60.6216    4.1  56.1    0.5  -0.4436  -2.8    1.9	Cen X-3                       
186.7226 -62.6324   26.4  51.1   -7.3  -0.0343  -0.4    8.5	GX 301-2                      
244.9716 -15.4864    7.0  23.5 -117.3  -0.0629  -1.6    9.2	Sco X-1                       
256.0712 -37.8905    3.6  37.3  -75.7  -0.2475  -3.2    4.9	4U 1700-377                   
256.6043 -36.4096    2.9  37.1  -78.2  -0.2995  -3.9    8.2	GX 349+2                      
262.8754 -24.8359    4.9  40.0  -98.2   0.2826   2.3    9.1	GX 1+4                        
199.2786   4.0488    2.2  29.9  106.9   0.2609   5.2 ------	UNKNOWN                       
220.9165 -27.8492    1.0  10.6  -28.2   0.3475  11.3 ------	UNKNOWN                       
254.3822   5.9580    2.5  40.7 -148.4   0.2306   4.7 ------	UNKNOWN                       
227.8518 -65.6710    2.8  48.7  -30.5   0.3070   4.2 ------	UNKNOWN

Post-slew image of 15-350 keV band

Time interval of the image:
71.404590 962.775200
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
170.1857 -60.8082    5.6  47.1   13.3  -2.9303  -2.1   11.8	Cen X-3                       
186.7585 -62.7192    7.6  41.3    5.2   1.5554   1.5    4.2	GX 301-2                      
244.9709 -15.6459    0.2  25.4 -131.5  40.3182  62.5    0.6	Sco X-1                       
255.9982 -37.8216    0.8  30.9  -79.9  12.8250  14.2    1.5	4U 1700-377                   
256.3423 -36.4486    2.7  31.0  -82.6   4.0202   4.3    4.7	GX 349+2                      
263.1342 -24.6335   51.6  37.8 -102.7   0.3767   0.2    9.6	GX 1+4                        
264.6194 -44.4804    6.3  38.4  -70.2   2.6731   1.9    5.6	4U 1735-44                    
262.9114 -33.9073    5.3  36.3  -87.5   3.5469   2.2    5.8	GX 354-0                      
194.9534 -33.8193    3.4  23.0   50.8   2.3720   3.4 ------	UNKNOWN                       
225.7527  26.7976    3.9  54.9  167.6  12.0272   3.0 ------	UNKNOWN

Plot creation:
Sun May 31 04:52:17 EDT 2015