batgrbproduct analysis for trigger=517469

batgrbproduct Analysis for Trigger=517469

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 05:53:43 EST 2014
             Host Name: batevent1
   Current Working Dir: /local/data/batevent/batevent_reproc/trigger517469
======================================================================

  Trigger: 00517469      Segment: 000

  BAT Trigger Time: 353136826.304   [s; MET]
      Trigger Stop: 353136826.56   [s; MET]
               UTC: 2012-03-11T05:33:38.324140    [includes UTCF correction] 
       Where From?: TDRSS position message

  BAT 
    RA: 273.086737373698   Dec: 14.2755565148965  [deg; J2000]

     Catalogged Source?: NO
     Point Source?:      YES
     GRB Indicated?:     YES    [ by BAT flight software ]
     Image S/N Ratio:    12.99
     Image Trigger?:     NO
     Rate S/N Ratio:     25.0199920063936  [ if not an image trigger ]
     Image S/N Ratio:    12.99

  Flight Position:   [ source = BAT ]
    RA: 273.086737373698   Dec: 14.2755565148965  [deg; J2000]

  Ground Position:   [ source = BAT pre-slew burst ]
    RA: 273.075094741315   Dec: 14.2965464351011  [deg; J2000]  
        { 18h 12m 18.0s , +14d 17' 47.6" }
         +/- 1.12471480168645 [arcmin] (estimated 90% radius based on SNR)
         +/- 0.517870236248799 [arcmin] (formal 1-sigma fit error)
    SNR: 25.7158361797186
 
  Angular difference between Flight and Ground position is 1.429806 arcmin
 
  Partial Coding Fraction: 0.71875    [ including projection effects ]

  Duration
     T90: 3.47999995946884 +/- 0.819795078477236
        Measured from: -0.952000021934509
                   to: 2.52799993753433     [s; relative to TRIGTIME]
     T50: 0.815999984741211 +/- 0.13792750112767
        Measured from: 0.0959999561309814
                   to: 0.911999940872192     [s; relative to TRIGTIME]



  Fluence
     Peak Flux  (peak 1 second)
        Measured from: -0.0720000267028809     
                   to: 0.927999973297119     [s; relative to TRIGTIME]
     Total Fluence        
        Measured from: -1.37600004673004     
                   to: 3.22799998521805     [s; relative to TRIGTIME]
     
             Band 1     Band 2     Band 3     Band 4
              15-25      25-50     50-100    100-350     keV
 Total     0.259436   0.235777   0.089076   0.027720
           0.015187   0.014845   0.011766   0.009414 [error]
 Peak      0.144512   0.150025   0.058510   0.013671
           0.008378   0.008238   0.006104   0.004522 [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 8.38e-08 9.54e-08 7.78e-08 1.06e-07 2.96e-07 3.63e-07   erg/cm2
              Error 8.79e-09 7.22e-09 1.11e-08 2.96e-08 2.54e-08 4.29e-08   erg/cm2
Peak flux Power-law 1.56e+00 1.05e+00 4.61e-01 2.80e-01 3.21e+00 3.35e+00   ph/cm2/s
              Error 1.53e-01 7.03e-02 5.10e-02 5.85e-02 2.20e-01 2.25e-01   ph/cm2/s
 
Fluence   Cutoff-PL 8.16e-08 9.91e-08 7.54e-08 5.48e-08 2.85e-07 3.11e-07   erg/cm2
              Error 9.67e-09 9.64e-09 1.29e-08 7.08e-08 3.04e-08 6.84e-08   erg/cm2
Peak flux Cutoff-PL 1.44e+00 1.14e+00 4.52e-01 1.08e-01 3.11e+00 3.14e+00   ph/cm2/s
              Error 1.76e-01 9.74e-02 5.94e-02 8.37e-02 2.30e-01 2.46e-01   ph/cm2/s
 
Fluence        Band -------- -------- -------- -------- -------- --------   erg/cm2
              Error -------- -------- -------- -------- -------- --------   erg/cm2
Peak flux      Band -------- -------- -------- -------- -------- --------   ph/cm2/s
              Error -------- -------- -------- -------- -------- --------   ph/cm2/s

 
=== Time-averaged spectral analysis ===
 
Model Ph_index Ph_90err Epeak  Epeak_90err Norm     Nomr_90err chi2   dof
PL    2.293    0.154    -      -           6.73e-03 6.92e-04   46.570 57
CPL   1.941    0.381       6.7   15.0      1.09e-02 0.00e+00   45.590 56
 
 
=== 1-s peak spectral analysis ===
 
Model Ph_index Ph_90err Epeak  Epeak_90err Norm     Nomr_90err chi2   dof
PL    2.185    0.126    -      -           1.95e-02 1.64e-03   42.690 57
CPL   1.432    0.594      31.1    0.0      5.33e-02 0.00e+00   37.390 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: 0.512000 sec.
T50 in the 50-300 keV band: 0.256000 sec.

 
=== Table of the duration information ==
 
        Value   tstart    tstop
T100    4.604   -1.376    3.228
T90     3.480   -0.952    2.528
T50     0.816    0.096    0.912
Peak    1.000   -0.072    0.928

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
  273.0751    14.2965   0.0075    21.1147    54.2487         0.6593838     25.716 TRIG_00517469                 
 
Foreground time interval of the image:
 -1.376   3.228 (delta_t =   4.604 [sec])
Background time interval of the image:
-213.003  -1.376 (delta_t = 211.627 [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 0.256000

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 0.256000

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 0.256000

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   -1.376 sec. to    3.228 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 2.29308     ( -0.150109   0.157243 )
Norm@50keV  : 6.73011E-03    ( -0.000698384   0.000686575 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          46.57 using 59 PHA bins.
# Reduced chi-squared =         0.8170 for     57 degrees of freedom 
# Null hypothesis probability =   8.365582e-01
 
Photon flux (15-150 keV)    in 4.604 sec: 1.17164 ( -0.0877726  0.087857 ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.95727e-07 ( -2.52081e-08  2.55681e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from   -1.376 sec. to    3.228 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.94088     ( -0.704285   0.0567269 )
Epeak [keV] : 6.66037      ( -5.53853 24.5235 )
Norm@50keV  : 1.08914E-02    (     )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          45.59 using 59 PHA bins.
# Reduced chi-squared =         0.8142 for     56 degrees of freedom 
# Null hypothesis probability =   8.383667e-01
 
Photon flux (15-150 keV)    in 4.604 sec: 1.15343 ( -0.09299  0.09275 ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.85124e-07 ( -3.0159e-08  3.06065e-08 ) ergs/cm2

Band function

Time interval is from   -1.376 sec. to    3.228 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -1.76941   ( 1.77345   1.77345 )
beta        : -2.58869    ( 2.58823   0.405422 )
Epeak [keV] : 16.3567      ( -16.04 11.9424 )
Norm@50keV   : 1.40890E-02    ( -0.00497673   2600.2 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          45.28 using 59 PHA bins.
# Reduced chi-squared =         0.8232 for     55 degrees of freedom 
# Null hypothesis probability =   8.221186e-01
 
Photon flux (15-150 keV)    in 4.604 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]    : 8.49878  (-0.740657  0.807381)
R^2/D10^2   : 0.967105  (-0.299112   0.438444)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          82.06 using 59 PHA bins.
# Reduced chi-squared =          1.440 for     57 degrees of freedom 
# Null hypothesis probability =   1.650885e-02
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  6.061e-08   7.458e-09
25- 50  1.175e-07   1.008e-08
50-150  3.750e-08   8.939e-09
15-150  2.156e-07   1.814e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 43.4689       (-7.92875      10.5453)
Norm        : 7.07323       (-1.01929     1.22779)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          47.69 using 59 PHA bins.
# Reduced chi-squared =         0.8366 for     57 degrees of freedom 
# Null hypothesis probability =   8.054732e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  7.677e-08   6.906e-09
25- 50  1.046e-07   8.402e-09
50-150  8.838e-08   1.968e-08
15-150  2.697e-07   2.576e-08

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 4.87917        (-1.16743      1.35878)
R1^2/D10^2  : 6.69348        (-3.9871      14.1731)
kT2 [keV]   : 15.5365        (-3.57445      7.63266)
R2^2/D10^2  : 5.85105E-02    (-0.0474153   0.12998)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          47.65 using 59 PHA bins.
# Reduced chi-squared =         0.8663 for     55 degrees of freedom 
# Null hypothesis probability =   7.487219e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  8.142e-08   3.225e-08
25- 50  9.720e-08   3.093e-08
50-150  9.404e-08   5.102e-08
15-150  2.727e-07   7.995e-08

Peak spectrum fit

Power-law model

Time interval is from   -0.072 sec. to    0.928 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 2.18487     ( -0.123834   0.12825 )
Norm@50keV  : 1.95132E-02    ( -0.00164918   0.0016262 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          42.69 using 59 PHA bins.
# Reduced chi-squared =         0.7489 for     57 degrees of freedom 
# Null hypothesis probability =   9.205282e-01
 
Photon flux (15-150 keV)    in 1 sec: 3.20501 ( -0.21994  0.220196 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.83085e-07 ( -1.36701e-08  1.37778e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from   -0.072 sec. to    0.928 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.43186     ( -0.669555   0.519357 )
Epeak [keV] : 31.1084      (   )
Norm@50keV  : 5.33309E-02    (     )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          37.39 using 59 PHA bins.
# Reduced chi-squared =         0.6678 for     56 degrees of freedom 
# Null hypothesis probability =   9.736423e-01
 
Photon flux (15-150 keV)    in 1 sec: 3.11402 ( -0.23038  0.23017 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.71775e-07 ( -1.5486e-08  1.5943e-08 ) ergs/cm2

Band function

Time interval is from   -0.072 sec. to    0.928 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -0.877164   ( -1.18216   0.65658 )
beta        : -2.60621    ( 2.57605   0.340602 )
Epeak [keV] : 31.1541      ( -7.78864 7.36456 )
Norm@50keV   : 0.125086    ( -0.0705784   3324.8 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          35.91 using 59 PHA bins.
# Reduced chi-squared =         0.6530 for     55 degrees of freedom 
# Null hypothesis probability =   9.783694e-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]    : 9.38238  (-0.687298  0.736207)
R^2/D10^2   : 1.86109  (-0.489241   0.665325)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          71.26 using 59 PHA bins.
# Reduced chi-squared =          1.250 for     57 degrees of freedom 
# Null hypothesis probability =   9.690813e-02
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  3.254e-08   3.650e-09
25- 50  7.372e-08   5.840e-09
50-150  3.190e-08   5.980e-09
15-150  1.382e-07   1.080e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 50.9526       (-8.25838      10.9958)
Norm        : 17.9121       (-2.02955     2.46073)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          37.40 using 59 PHA bins.
# Reduced chi-squared =         0.6562 for     57 degrees of freedom 
# Null hypothesis probability =   9.791906e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  4.398e-08   3.910e-09
25- 50  6.359e-08   4.610e-09
50-150  6.285e-08   1.098e-08
15-150  1.704e-07   1.370e-08

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 5.86063        (-1.59253      1.78073)
R1^2/D10^2  : 8.32673        (-4.70291      11.204)
kT2 [keV]   : 16.9832        (-4.4041      14.2773)
R2^2/D10^2  : 0.109905    (-0.0975929   0.327442)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          39.56 using 59 PHA bins.
# Reduced chi-squared =         0.7193 for     55 degrees of freedom 
# Null hypothesis probability =   9.420979e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  4.317e-08   1.350e-08
25- 50  6.332e-08   1.427e-08
50-150  6.166e-08   3.135e-08
15-150  1.682e-07   5.026e-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: 2.29308     ( -0.150109   0.157243 )
Norm@50keV  : 6.73011E-03    ( -0.000698384   0.000686575 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          46.57 using 59 PHA bins.
# Reduced chi-squared =         0.8170 for     57 degrees of freedom 
# Null hypothesis probability =   8.365582e-01
 
Photon flux (15-150 keV)    in 4.604 sec: 1.17164 ( -0.0877726  0.087857 ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.95727e-07 ( -2.52081e-08  2.55681e-08 ) ergs/cm2

Cutoff power-law model

Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.94088     ( -0.704285   0.0567269 )
Epeak [keV] : 6.66037      ( -5.53853 24.5235 )
Norm@50keV  : 1.08914E-02    (     )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          45.59 using 59 PHA bins.
# Reduced chi-squared =         0.8142 for     56 degrees of freedom 
# Null hypothesis probability =   8.383667e-01
 
Photon flux (15-150 keV)    in 4.604 sec: 1.15343 ( -0.09299  0.09275 ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.85124e-07 ( -3.0159e-08  3.07902e-08 ) ergs/cm2

Band function

 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -1.76941   ( 1.77345   1.77345 )
beta        : -2.58869    ( 2.58823   0.405422 )
Epeak [keV] : 16.3567      ( -16.04 11.9424 )
Norm@50keV   : 1.40890E-02    ( -0.00497673   2547.94 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          45.28 using 59 PHA bins.
# Reduced chi-squared =         0.8232 for     55 degrees of freedom 
# Null hypothesis probability =   8.221186e-01
 
Photon flux (15-150 keV)    in 4.604 sec:  (    ) ph/cm2/s
Energy fluence (15-150 keV)             : 0 ( 0  0 ) ergs/cm2

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

S(25-50 keV)  = 9.54e-08
S(50-100 keV) = 7.78e-08

T90 vs. Hardness ratio plot

T90                                   = 3.47999995946884 sec.
Hardness ratio (energy fluence ratio) = 0.815514

Color vs. Color plot

Count Ratio  (25-50 keV) / (15-25 keV) = 0.908806
Count Ratio (50-100 keV) / (15-25 keV) = 0.343345

Mask shadow pattern

IMX = 2.256228773123946E-01, IMY = -3.133946757620175E-01

TIME vs. PHA plot around the trigger time

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.256000

TIME vs. DetID plot around the trigger time

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.256000

100 us light curve (15-350 keV)

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.256000

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:
-213.003410 -1.376000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
254.2679  35.2157    0.0  37.4  100.7  -0.9559  -2.1   12.0	Her X-1                       
263.0190 -24.7624    7.5  55.0   14.9  -1.4704  -1.5    1.1	GX 1+4                        
268.4445  -1.6141    3.4  33.9   30.8   0.7566   3.4   10.7	SW J1753.5-0127               
270.2936 -25.0673    7.6  51.8    7.7   0.7490   1.5    0.9	GX 5-1                        
270.2057 -25.7514    3.6  52.4    7.4  -1.5985  -3.1    5.3	GRS 1758-258                  
273.9347 -13.8500    0.0  40.3   11.1  -0.2765  -1.0   11.9	GX 17+2                       
275.9884 -30.4635    5.4  54.6   -0.8   1.1803   2.1    6.7	H1820-303                     
284.8979 -24.9464    8.2  47.1   -8.6   0.4412   1.4    7.7	HT1900.1-2455                 
288.7939  10.9539    0.6  11.5    6.8   3.0394  19.0    0.6	GRS 1915+105                  
299.5945  35.1993    0.5  14.8  178.2   3.5428  22.6    0.2	Cyg X-1                       
308.0536  40.9868    1.0  23.0 -172.1   1.9899  11.4    3.3	Cyg X-3                       
326.0108  38.3713    8.2  32.3 -149.0   0.2851   1.4    8.1	Cyg X-2                       
257.6417   1.8935    2.2  40.4   46.3   2.0177   5.2 ------	UNKNOWN                       
335.8714  69.2453    2.9  54.2  177.0   2.3759   4.0 ------	UNKNOWN                       
301.1382 -35.9161    2.6  57.6  -26.8   4.5134   4.5 ------	UNKNOWN

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

Time interval of the image:
-1.376000 3.228000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
254.5222  35.4194    5.3  37.2  101.1   0.1456   2.2    5.6	Her X-1                       
262.9398 -24.7226    7.1  55.0   15.0   0.2222   1.6    4.0	GX 1+4                        
268.3288  -1.4560   15.7  33.9   31.1   0.0274   0.7    2.4	SW J1753.5-0127               
270.3614 -25.1565    4.3  51.8    7.6   0.1882   2.7    6.3	GX 5-1                        
270.4018 -25.6309    7.1  52.2    7.3   0.1193   1.6    8.6	GRS 1758-258                  
274.0671 -13.8998    7.9  40.3   10.9  -0.0512  -1.5    8.9	GX 17+2                       
276.0262 -30.3837    7.5  54.5   -0.8   0.1295   1.5    5.3	H1820-303                     
284.8714 -25.0297    5.1  47.1   -8.6   0.1018   2.3   11.1	HT1900.1-2455                 
288.6139  10.8664    4.4  11.6    7.5  -0.0540  -2.6   11.9	GRS 1915+105                  
299.4882  35.3784    4.5  14.9  177.6   0.0550   2.5   11.7	Cyg X-1                       
308.2946  41.0482   54.2  23.2 -171.8   0.0051   0.2   10.1	Cyg X-3                       
326.1654  38.1989    7.8  32.4 -148.7   0.0421   1.5    7.4	Cyg X-2                       
267.6455  12.0441    3.1  26.9   54.2   0.1185   3.8 ------	UNKNOWN                       
273.0751  14.2966    0.5  21.1   54.2   0.6593  25.7 ------	UNKNOWN

Post-slew image of 15-350 keV band

Time interval of the image:
172.796610 962.737000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
264.7465 -44.4502   20.3  54.1  174.1   0.8894   0.6    0.2	4U 1735-44                    
340.7290 -71.9245    3.0  10.8 -167.5   1.5225   3.8 ------	UNKNOWN                       
 57.8012 -41.8056    2.9  36.3   -4.2   2.0560   3.9 ------	UNKNOWN                       
 47.4408 -28.8214    2.2  46.4  -22.0   4.0813   5.2 ------	UNKNOWN                       
  9.9157 -29.7487    3.9  42.4  -69.0   6.7583   3.0 ------	UNKNOWN                       
320.5897 -33.3836    3.0  48.0 -128.9   7.0303   3.8 ------	UNKNOWN

Plot creation:
Sat May 30 20:06:13 EDT 2015