batgrbproduct analysis for trigger=324805

batgrbproduct Analysis for Trigger=324805

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 22:40:37 EST 2014
             Host Name: batevent1
   Current Working Dir: /local/data/batevent/batevent_reproc/trigger324805
======================================================================

  Trigger: 00324805      Segment: 000

  BAT Trigger Time: 243186818.24   [s; MET]
      Trigger Stop: 243186818.368   [s; MET]
               UTC: 2008-09-15T15:53:35.140100    [includes UTCF correction] 
       Where From?: TDRSS position message

  BAT 
    RA: 213.078560327715   Dec: -11.4732707538459  [deg; J2000]

     Catalogged Source?: NO
     Point Source?:      YES
     GRB Indicated?:     YES    [ by BAT flight software ]
     Image S/N Ratio:    10.57
     Image Trigger?:     NO
     Rate S/N Ratio:     23.473389188611  [ if not an image trigger ]
     Image S/N Ratio:    10.57

  Flight Position:   [ source = BAT ]
    RA: 213.078560327715   Dec: -11.4732707538459  [deg; J2000]

  Ground Position:   [ source = BAT pre-slew burst ]
    RA: 213.087987204382   Dec: -11.4904661441536  [deg; J2000]  
        { 14h 12m 21.1s , -11d 29' 25.7" }
         +/- 0.779382872910783 [arcmin] (estimated 90% radius based on SNR)
         +/- 0.245163071345694 [arcmin] (formal 1-sigma fit error)
    SNR: 43.4270182902908
 
  Angular difference between Flight and Ground position is 1.171194 arcmin
 
  Partial Coding Fraction: 0.7421875    [ including projection effects ]

  Duration
     T90: 4.05200001597404 +/- 0.607328571222746
        Measured from: -0.156000018119812
                   to: 3.89599999785423     [s; relative to TRIGTIME]
     T50: 1.07600000500679 +/- 0.101980397051727
        Measured from: 0.412000000476837
                   to: 1.48800000548363     [s; relative to TRIGTIME]



  Fluence
     Peak Flux  (peak 1 second)
        Measured from: 0.175999999046326     
                   to: 1.17599999904633     [s; relative to TRIGTIME]
     Total Fluence        
        Measured from: -0.532000005245209     
                   to: 6.14800000190735     [s; relative to TRIGTIME]
     
             Band 1     Band 2     Band 3     Band 4
              15-25      25-50     50-100    100-350     keV
 Total     0.652910   0.767040   0.428383   0.045302
           0.019846   0.021759   0.020417   0.021377 [error]
 Peak      0.273363   0.393802   0.244957   0.056357
           0.009807   0.011115   0.010015   0.008859 [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 2.34e-07 3.26e-07 3.36e-07 6.33e-07 1.10e-06 1.53e-06   erg/cm2
              Error 1.48e-08 1.24e-08 2.07e-08 8.20e-08 4.67e-08 9.99e-08   erg/cm2
Peak flux Power-law 3.28e+00 2.89e+00 1.75e+00 1.59e+00 8.60e+00 9.51e+00   ph/cm2/s
              Error 2.08e-01 1.12e-01 8.70e-02 1.62e-01 3.29e-01 3.48e-01   ph/cm2/s
 
Fluence   Cutoff-PL 2.17e-07 3.41e-07 3.32e-07 2.79e-07 1.04e-06 1.17e-06   erg/cm2
              Error 1.75e-08 1.55e-08 2.27e-08 1.33e-07 5.77e-08 1.48e-07   erg/cm2
Peak flux Cutoff-PL 2.95e+00 3.04e+00 1.80e+00 8.11e-01 8.30e+00 8.60e+00   ph/cm2/s
              Error 2.52e-01 1.34e-01 9.58e-02 2.49e-01 3.54e-01 4.45e-01   ph/cm2/s
 
Fluence        Band 2.07e-07 3.46e-07 3.21e-07 5.06e-07 1.05e-06 1.38e-06   erg/cm2
              Error 1.97e-08 1.70e-08 2.30e-08 -------- 5.28e-08 --------   erg/cm2
Peak flux      Band 2.73e+00 3.17e+00 1.71e+00 1.25e+00 8.19e+00 8.86e+00   ph/cm2/s
              Error 2.98e-01 1.55e-01 9.31e-02 2.05e-01 3.62e-01 4.17e-01   ph/cm2/s

 
=== Time-averaged spectral analysis ===
 
Model Ph_index Ph_90err Epeak  Epeak_90err Norm     Nomr_90err chi2   dof
PL    1.957    0.077    -      -           1.78e-02 7.82e-04   71.980 57
CPL   1.439    0.325      48.3    9.9      3.40e-02 1.41e-02   63.500 56
 
 
=== 1-s peak spectral analysis ===
 
Model Ph_index Ph_90err Epeak  Epeak_90err Norm     Nomr_90err chi2   dof
PL    1.728    0.067    -      -           6.41e-02 2.48e-03   73.090 57
CPL   1.118    0.299      69.2   15.2      1.33e-01 4.80e-02   59.030 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: 1.408000 sec.
T50 in the 50-300 keV band: 0.640000 sec.

 
=== Table of the duration information ==
 
        Value   tstart    tstop
T100    6.680   -0.532    6.148
T90     4.052   -0.156    3.896
T50     1.076    0.412    1.488
Peak    1.000    0.176    1.176

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
  213.0880   -11.4905   0.0044    32.3197   -26.1081         1.9945508     43.427 TRIG_00324805                 
 
Foreground time interval of the image:
 -0.532   6.148 (delta_t =   6.680 [sec])
Background time interval of the image:
-60.240  -0.532 (delta_t =  59.708 [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 0.128000

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 0.128000

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 0.128000

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   -0.532 sec. to    6.148 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.95677     ( -0.0762457   0.0773066 )
Norm@50keV  : 1.78414E-02    ( -0.0007852   0.000779724 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          71.98 using 59 PHA bins.
# Reduced chi-squared =          1.263 for     57 degrees of freedom 
# Null hypothesis probability =   8.740461e-02
 
Photon flux (15-150 keV)    in 6.68 sec: 2.62440 ( -0.104163  0.1044 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.09702e-06 ( -4.65851e-08  4.68957e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from   -0.532 sec. to    6.148 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.43893     ( -0.338298   0.311964 )
Epeak [keV] : 48.3311      ( -7.59374 12.136 )
Norm@50keV  : 3.39555E-02    ( -0.0107   0.0175358 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          63.50 using 59 PHA bins.
# Reduced chi-squared =          1.134 for     56 degrees of freedom 
# Null hypothesis probability =   2.290997e-01
 
Photon flux (15-150 keV)    in 6.68 sec: 2.53206 ( -0.11629  0.11658 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.03672e-06 ( -5.72877e-08  5.80492e-08 ) ergs/cm2

Band function

Time interval is from   -0.532 sec. to    6.148 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -1.43898   ( -0.23473   0.459997 )
beta        : -10.0000    ( 10   1.77636e-15 )
Epeak [keV] : 48.3216      ( -7.58637 12.1339 )
Norm@50keV   : 3.39482E-02    ( -0.010707   0.0175478 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          63.50 using 59 PHA bins.
# Reduced chi-squared =          1.155 for     55 degrees of freedom 
# Null hypothesis probability =   2.018530e-01
 
Photon flux (15-150 keV)    in 6.68 sec: 2.55089 ( 4.44911  -0.1399 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.0501e-06 ( -1.05005e-06  -5.28856e-08 ) ergs/cm2

Single BB

 
Spectral model blackbody:
------------------------------------------------------------
Parameters  : value    Lower 90%  Upper 90%
kT [keV]    : 10.8936  (  )
R^2/D10^2   : 0.836173  (   )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =         179.73 using 59 PHA bins.
# Reduced chi-squared =         3.1532 for     57 degrees of freedom 
# Null hypothesis probability =   1.237194e-14
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.382e-07   9.452e-09
25- 50  3.860e-07   1.593e-08
50-150  2.568e-07   2.879e-08
15-150  7.810e-07   3.240e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 75.4347       (-9.45062      11.716)
Norm        : 12.3028       (-0.803544     0.879784)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          63.80 using 59 PHA bins.
# Reduced chi-squared =          1.119 for     57 degrees of freedom 
# Null hypothesis probability =   2.497225e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  2.123e-07   1.239e-08
25- 50  3.445e-07   1.296e-08
50-150  4.671e-07   4.335e-08
15-150  1.024e-06   4.409e-08

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 6.55147        (-0.728185      0.740649)
R1^2/D10^2  : 4.18084        (-1.30447      2.19637)
kT2 [keV]   : 21.6947        (-3.02602      4.13012)
R2^2/D10^2  : 4.24813E-02    (-0.0208773   0.0356961)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          58.85 using 59 PHA bins.
# Reduced chi-squared =          1.070 for     55 degrees of freedom 
# Null hypothesis probability =   3.363357e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  2.037e-07   2.351e-08
25- 50  3.451e-07   3.434e-08
50-150  4.863e-07   1.046e-07
15-150  1.035e-06   1.500e-07

Peak spectrum fit

Power-law model

Time interval is from    0.176 sec. to    1.176 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.72755     ( -0.0667085   0.0672488 )
Norm@50keV  : 6.41221E-02    ( -0.00248469   0.00247648 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          73.09 using 59 PHA bins.
# Reduced chi-squared =          1.282 for     57 degrees of freedom 
# Null hypothesis probability =   7.410017e-02
 
Photon flux (15-150 keV)    in 1 sec: 8.59975 ( -0.329203  0.329735 ) ph/cm2/s
Energy fluence (15-150 keV)             : 5.92504e-07 ( -2.38715e-08  2.39625e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from    0.176 sec. to    1.176 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.11781     ( -0.309358   0.288002 )
Epeak [keV] : 69.2192      ( -9.52149 20.8592 )
Norm@50keV  : 0.132540    ( -0.0377867   0.0581493 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          59.03 using 59 PHA bins.
# Reduced chi-squared =          1.054 for     56 degrees of freedom 
# Null hypothesis probability =   3.653336e-01
 
Photon flux (15-150 keV)    in 1 sec: 8.30166 ( -0.35421  0.35477 ) ph/cm2/s
Energy fluence (15-150 keV)             : 5.61973e-07 ( -2.7705e-08  2.7766e-08 ) ergs/cm2

Band function

Time interval is from    0.176 sec. to    1.176 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -6.35612E-02   ( -0.85794   2.27157 )
beta        : -1.97798    ( -0.191373   0.136893 )
Epeak [keV] : 42.4145      ( -7.78393 14.7927 )
Norm@50keV   : 0.645858    ( -1.0059   24.3332 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          53.03 using 59 PHA bins.
# Reduced chi-squared =         0.9641 for     55 degrees of freedom 
# Null hypothesis probability =   5.504155e-01
 
Photon flux (15-150 keV)    in 1 sec: 8.18646 ( -1.18646  -0.36063 ) ph/cm2/s
Energy fluence (15-150 keV)             : 5.6656e-07 ( -5.66553e-07  -2.5793e-08 ) ergs/cm2

Single BB

 
Spectral model blackbody:
------------------------------------------------------------
Parameters  : value    Lower 90%  Upper 90%
kT [keV]    : 12.7970  (  )
R^2/D10^2   : 1.62059  (   )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =         177.10 using 59 PHA bins.
# Reduced chi-squared =         3.1069 for     57 degrees of freedom 
# Null hypothesis probability =   3.100754e-14
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  5.629e-08   3.790e-09
25- 50  1.906e-07   7.600e-09
50-150  1.955e-07   1.640e-08
15-150  4.423e-07   2.025e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 123.456       (      )
Norm        : 36.1584       (-1.67214     2.13343)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          59.69 using 59 PHA bins.
# Reduced chi-squared =          1.047 for     57 degrees of freedom 
# Null hypothesis probability =   3.782556e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  9.265e-08   6.320e-09
25- 50  1.674e-07   8.850e-09
50-150  3.073e-07   7.760e-08
15-150  5.673e-07   8.555e-08

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 7.83650        (-0.894481      0.907514)
R1^2/D10^2  : 6.77964        (-1.94828      3.14861)
kT2 [keV]   : 26.0919        (-4.07276      6.26613)
R2^2/D10^2  : 8.10477E-02    (-0.0441245   0.0769802)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          53.42 using 59 PHA bins.
# Reduced chi-squared =         0.9713 for     55 degrees of freedom 
# Null hypothesis probability =   5.351769e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  8.348e-08   8.645e-09
25- 50  1.794e-07   1.780e-08
50-150  3.027e-07   6.700e-08
15-150  5.655e-07   8.615e-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: 1.95677     ( -0.0762457   0.0773066 )
Norm@50keV  : 1.78414E-02    ( -0.0007852   0.000779724 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          71.98 using 59 PHA bins.
# Reduced chi-squared =          1.263 for     57 degrees of freedom 
# Null hypothesis probability =   8.740461e-02
 
Photon flux (15-150 keV)    in 6.68 sec: 2.62440 ( -0.104163  0.1044 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.09702e-06 ( -4.65851e-08  4.68957e-08 ) ergs/cm2

Cutoff power-law model

Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.43893     ( -0.338298   0.311964 )
Epeak [keV] : 48.3311      ( -7.59374 12.136 )
Norm@50keV  : 3.39555E-02    ( -0.0107   0.0175358 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          63.50 using 59 PHA bins.
# Reduced chi-squared =          1.134 for     56 degrees of freedom 
# Null hypothesis probability =   2.290997e-01
 
Photon flux (15-150 keV)    in 6.68 sec: 2.53206 ( -0.11629  0.11658 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.03672e-06 ( -5.72877e-08  5.80492e-08 ) ergs/cm2

Band function

 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -1.43898   ( -0.23473   0.459997 )
beta        : -10.0000    ( 10   7.10543e-15 )
Epeak [keV] : 48.3216      ( -7.58637 12.1339 )
Norm@50keV   : 3.39482E-02    ( -0.010707   0.0175478 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          63.50 using 59 PHA bins.
# Reduced chi-squared =          1.155 for     55 degrees of freedom 
# Null hypothesis probability =   2.018530e-01
 
Photon flux (15-150 keV)    in 6.68 sec: 2.55089 ( 4.44911  -0.1399 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.0501e-06 ( -1.05005e-06  -5.28856e-08 ) ergs/cm2

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

S(25-50 keV)  = 3.26e-07
S(50-100 keV) = 3.36e-07

T90 vs. Hardness ratio plot

T90                                   = 4.05200001597404 sec.
Hardness ratio (energy fluence ratio) = 1.03067

Color vs. Color plot

Count Ratio  (25-50 keV) / (15-25 keV) = 1.1748
Count Ratio (50-100 keV) / (15-25 keV) = 0.656113

Mask shadow pattern

IMX = 5.681019625274246E-01, IMY = 2.784099831101502E-01

TIME vs. PHA plot around the trigger time

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.128000

TIME vs. DetID plot around the trigger time

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.128000

100 us light curve (15-350 keV)

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.128000

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:
-60.240000 -0.532000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
135.5550 -40.4964    9.7  45.1 -170.2   0.1432   1.2    3.7	Vela X-1                      
170.5941 -60.6347    4.8  25.9  149.6  -0.1964  -2.4    8.2	Cen X-3                       
186.6346 -62.6564    6.9  23.3  131.6   0.1457   1.7    6.9	GX 301-2                      
245.0368 -15.6376    2.7  49.1   15.8   0.9539   4.3    3.3	Sco X-1                       
256.0396 -37.8918   12.8  46.0   48.6   0.2982   0.9    3.8	4U 1700-377                   
229.6159 -17.6900    2.7  36.7    3.4   0.4056   4.3 ------	UNKNOWN                       
199.3564   6.7896    2.5  46.9  -54.3   1.5655   4.6 ------	UNKNOWN

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

Time interval of the image:
-0.532000 6.148000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
135.5066 -40.5455   16.3  45.1 -170.3   0.0480   0.7    1.1	Vela X-1                      
170.3148 -60.6247   37.4  26.0  149.8   0.0137   0.3    0.1	Cen X-3                       
186.7850 -62.9028   12.0  23.6  131.2  -0.0463  -1.0    8.7	GX 301-2                      
245.0751 -15.6864   15.2  49.1   15.8   0.0893   0.8    6.2	Sco X-1                       
255.9022 -37.7509    7.3  45.9   48.4   0.2691   1.6    6.9	4U 1700-377                   
213.0880 -11.4905    0.3  32.3  -26.1   1.9945  43.4 ------	UNKNOWN                       
147.8453 -19.3603    2.5  45.8 -136.9   0.4129   4.7 ------	UNKNOWN

Post-slew image of 15-350 keV band

Time interval of the image:
185.260600 842.842800
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
244.9817 -15.6333    0.6  41.0  -49.2  21.7045  19.6    0.4	Sco X-1                       
255.9908 -37.8274    0.6  22.1  -79.8  11.3359  20.0    1.0	4U 1700-377                   
256.6235 -36.5406    4.1  21.8  -76.2   1.5646   2.8   11.5	GX 349+2                      
263.1484 -24.5762   14.1  22.2  -40.5   0.3922   0.8   12.7	GX 1+4                        
264.9394 -44.3573    4.1  15.8 -101.5   1.3326   2.8   10.1	4U 1735-44                    
268.3285  -1.4575    3.4  39.2   -6.7   2.2951   3.4    2.4	SW J1753.5-0127               
270.2395 -25.0279    2.3  17.4  -27.7   2.2791   5.0    3.9	GX 5-1                        
270.1768 -25.7659    2.5  16.9  -29.4   2.0139   4.6    6.9	GRS 1758-258                  
274.0050 -14.0569    1.6  25.5   -4.5   4.1784   7.2    1.2	GX 17+2                       
275.9535 -30.3040    2.5  10.2  -25.2   2.1925   4.7    4.1	H1820-303                     
285.1531 -25.0423    5.1  12.9   23.0   0.9857   2.3    9.7	HT1900.1-2455                 
288.8290  10.9700    2.0  49.1   24.9  10.0910   5.8    2.3	GRS 1915+105                  
263.0240 -33.8319    3.8  17.5  -64.2   1.4885   3.0    1.7	GX 354-0                      
280.6153 -11.4337    1.6  26.7   11.1   3.6442   7.1 ------	UNKNOWN                       
270.8837  -5.0162    3.7  35.0   -4.6   1.9382   3.1 ------	UNKNOWN

Plot creation:
Sun May 31 06:24:31 EDT 2015