batgrbproduct analysis for trigger=323870

batgrbproduct Analysis for Trigger=323870

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 23:10:40 EST 2014
             Host Name: batevent1
   Current Working Dir: /local/data/batevent/batevent_reproc/trigger323870
======================================================================

  Trigger: 00323870      Segment: 000

  BAT Trigger Time: 242308738.048   [s; MET]
      Trigger Stop: 242308738.304   [s; MET]
               UTC: 2008-09-05T11:58:54.973940    [includes UTCF correction] 
       Where From?: TDRSS position message

  BAT 
    RA: 287.661676067797   Dec: -18.8772722987606  [deg; J2000]

     Catalogged Source?: NO
     Point Source?:      YES
     GRB Indicated?:     YES    [ by BAT flight software ]
     Image S/N Ratio:    6.87
     Image Trigger?:     NO
     Rate S/N Ratio:     29.0344622819159  [ if not an image trigger ]
     Image S/N Ratio:    6.87

  Flight Position:   [ source = BAT ]
    RA: 287.661676067797   Dec: -18.8772722987606  [deg; J2000]

  Ground Position:   [ source = BAT pre-slew burst ]
    RA: 287.667070239253   Dec: -18.8666914609386  [deg; J2000]  
        { 19h 10m 40.1s , -18d 52' 00.1" }
         +/- 2.08491945537207 [arcmin] (estimated 90% radius based on SNR)
         +/- 0.764992847180635 [arcmin] (formal 1-sigma fit error)
    SNR: 10.6482085549777
 
  Angular difference between Flight and Ground position is 0.704858 arcmin
 
  Partial Coding Fraction: 0.5625    [ including projection effects ]

  Duration
     T90: 1.01600003242493 +/- 0.0815843255901954
        Measured from: 0.0479999780654907
                   to: 1.06400001049042     [s; relative to TRIGTIME]
     T50: 0.768000036478043 +/- 0.120000004768375
        Measured from: 0.179999977350235
                   to: 0.948000013828278     [s; relative to TRIGTIME]



  Fluence
     Peak Flux  (peak 1 second)
        Measured from: 0.0399999916553497     
                   to: 1.03999999165535     [s; relative to TRIGTIME]
     Total Fluence        
        Measured from: 0.0399999916553497     
                   to: 1.12799999117851     [s; relative to TRIGTIME]
     
             Band 1     Band 2     Band 3     Band 4
              15-25      25-50     50-100    100-350     keV
 Total     0.011610   0.062965   0.065322   0.036225
           0.007346   0.008028   0.007953   0.007170 [error]
 Peak      0.009954   0.056345   0.058198   0.034752
           0.007015   0.007665   0.007648   0.006936 [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 7.96e-09 2.26e-08 5.21e-08 3.24e-07 1.41e-07 4.07e-07   erg/cm2
              Error 2.49e-09 4.25e-09 6.99e-09 1.04e-07 1.91e-08 1.06e-07   erg/cm2
Peak flux Power-law 2.13e-01 3.39e-01 4.06e-01 9.51e-01 1.23e+00 1.91e+00   ph/cm2/s
              Error 7.42e-02 7.25e-02 5.66e-02 2.94e-01 1.86e-01 3.01e-01   ph/cm2/s
 
Fluence   Cutoff-PL 7.60e-09 2.28e-08 5.33e-08 2.63e-07 1.40e-07 3.46e-07   erg/cm2
              Error 2.91e-09 4.48e-09 8.60e-09 1.93e-07 1.95e-08 1.68e-07   erg/cm2
Peak flux Cutoff-PL 2.07e-01 3.40e-01 4.12e-01 8.66e-01 1.23e+00 1.82e+00   ph/cm2/s
              Error 8.53e-02 7.43e-02 6.96e-02 4.50e-01 1.88e-01 4.53e-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    0.795    0.242    -      -           1.10e-02 1.61e-03   50.300 57
CPL   0.627    0.830     499.3    0.0      1.30e-02 1.19e-02   50.200 56
 
 
=== 1-s peak spectral analysis ===
 
Model Ph_index Ph_90err Epeak  Epeak_90err Norm     Nomr_90err chi2   dof
PL    0.738    0.261    -      -           1.07e-02 1.70e-03   49.120 57
CPL   0.641    0.709     854.9    0.0      1.17e-02 1.09e-02   49.090 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: 1.024000 sec.
T50 in the 50-300 keV band: 0.832000 sec.

 
=== Table of the duration information ==
 
        Value   tstart    tstop
T100    1.088    0.040    1.128
T90     1.016    0.048    1.064
T50     0.768    0.180    0.948
Peak    1.000    0.040    1.040

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
  287.6671   -18.8667   0.0181    39.6253    -6.5243         0.1762158     10.648 TRIG_00323870                 
 
Foreground time interval of the image:
  0.040   1.128 (delta_t =   1.088 [sec])
Background time interval of the image:
-749.147 -701.951 (delta_t =  47.196 [sec])
-239.048   0.040 (delta_t = 239.088 [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)

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    0.040 sec. to    1.128 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 0.794886     ( -0.250689   0.232794 )
Norm@50keV  : 1.10396E-02    ( -0.00162854   0.00158856 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          50.30 using 59 PHA bins.
# Reduced chi-squared =         0.8825 for     57 degrees of freedom 
# Null hypothesis probability =   7.226038e-01
 
Photon flux (15-150 keV)    in 1.088 sec: 1.26905 ( -0.179082  0.180275 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.40663e-07 ( -1.90668e-08  1.9113e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from    0.040 sec. to    1.128 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 0.626821     ( -1.03686   0.623252 )
Epeak [keV] : 499.274      ( -500.136 -500.136 )
Norm@50keV  : 1.29966E-02    ( -0.00309096   0.0207787 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          50.20 using 59 PHA bins.
# Reduced chi-squared =         0.8964 for     56 degrees of freedom 
# Null hypothesis probability =   6.930456e-01
 
Photon flux (15-150 keV)    in 1.088 sec: 1.26276 ( -0.18127  0.18215 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.40128e-07 ( -1.96721e-08  1.93729e-08 ) ergs/cm2

Band function

Time interval is from    0.040 sec. to    1.128 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -0.732639   ( 0.732639   0.732639 )
beta        : -0.794892    ( -0.232794   0.250667 )
Epeak [keV] : 15.6074      ( -15.6074 -15.6074 )
Norm@50keV   : 1.64507E-02    ( -0.00698771   0 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          50.30 using 59 PHA bins.
# Reduced chi-squared =         0.9146 for     55 degrees of freedom 
# Null hypothesis probability =   6.544156e-01
 
Photon flux (15-150 keV)    in 1.088 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]    : 26.2349  (-4.68402  6.61428)
R^2/D10^2   : 2.79009E-02  (-0.0135686   0.0232666)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          58.43 using 59 PHA bins.
# Reduced chi-squared =          1.025 for     57 degrees of freedom 
# Null hypothesis probability =   4.227845e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  3.536e-09   1.023e-09
25- 50  2.054e-08   5.881e-09
50-150  1.040e-07   2.488e-08
15-150  1.281e-07   2.870e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 200.000       (      )
Norm        : 5.22581       (-0.754041     0.753965)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          78.92 using 59 PHA bins.
# Reduced chi-squared =          1.385 for     57 degrees of freedom 
# Null hypothesis probability =   2.891036e-02
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.416e-08   7.926e-09
25- 50  2.724e-08   1.528e-08
50-150  5.975e-08   3.313e-08
15-150  1.012e-07   5.679e-08

Double BB

------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 12.9498        (-4.76298      6.15529)
R1^2/D10^2  : 0.160526        (      )
kT2 [keV]   : 91.2881        (-57.4877      -92.9548)
R2^2/D10^2  : 9.39722E-04    (-0.000638179   0.00499623)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          47.87 using 59 PHA bins.
#Fit statistic : Chi-Squared =          47.37 using 59 PHA bins.
# Reduced chi-squared =         0.8704 for     55 degrees of freedom 
# Reduced chi-squared =         0.8613 for     55 degrees of freedom 
# Null hypothesis probability =   7.411581e-01
# Null hypothesis probability =   7.578704e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  6.924e-09   4.158e-09
25- 50  2.511e-08   1.382e-08
50-150  1.037e-07   5.723e-08
15-150  1.358e-07   6.958e-08

Peak spectrum fit

Power-law model

Time interval is from    0.040 sec. to    1.040 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 0.738146     ( -0.272623   0.249928 )
Norm@50keV  : 1.06965E-02    ( -0.00172456   0.00167041 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          49.12 using 59 PHA bins.
# Reduced chi-squared =         0.8617 for     57 degrees of freedom 
# Null hypothesis probability =   7.617646e-01
 
Photon flux (15-150 keV)    in 1 sec: 1.23309 ( -0.185473  0.186882 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.28367e-07 ( -1.83384e-08  1.83745e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from    0.040 sec. to    1.040 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 0.641251     ( -1.09045   0.328106 )
Epeak [keV] : 854.855      ( -880.208 -880.208 )
Norm@50keV  : 1.17384E-02    ( -0.00219335   0.0196178 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          49.09 using 59 PHA bins.
# Reduced chi-squared =         0.8766 for     56 degrees of freedom 
# Null hypothesis probability =   7.317923e-01
 
Photon flux (15-150 keV)    in 1 sec: 1.22977 ( -0.18737  0.18861 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.28181e-07 ( -1.8728e-08  1.8542e-08 ) ergs/cm2

Band function

Time interval is from    0.040 sec. to    1.040 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : 5.00000   ( -5   -5 )
beta        : -0.938096    ( -0.435504   0.329859 )
Epeak [keV] : 40.6480      ( -39.3867 13.9288 )
Norm@50keV   : 40.8400    ( -5.60651   971916 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          46.59 using 59 PHA bins.
# Reduced chi-squared =         0.8471 for     55 degrees of freedom 
# Null hypothesis probability =   7.830389e-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]    : 27.8681  (-5.41154  8.00281)
R^2/D10^2   : 2.29869E-02  (-0.0119027   0.0212839)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          56.59 using 59 PHA bins.
# Reduced chi-squared =         0.9928 for     57 degrees of freedom 
# Null hypothesis probability =   4.904672e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  2.919e-09   9.395e-10
25- 50  1.744e-08   5.198e-09
50-150  9.813e-08   2.363e-08
15-150  1.185e-07   2.568e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 200.000       (      )
Norm        : 5.05396       (-0.783744     0.78367)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          78.01 using 59 PHA bins.
# Reduced chi-squared =          1.369 for     57 degrees of freedom 
# Null hypothesis probability =   3.372452e-02
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.258e-08   7.175e-09
25- 50  2.419e-08   1.377e-08
50-150  5.306e-08   2.952e-08
15-150  8.983e-08   5.135e-08

Double BB

R1^2/D10^2  : 0.136162        (-0.0728608      0.344042)
kT2 [keV]   : 163.800        (-163.803      -163.803)
R2^2/D10^2  : 3.61492E-04    (   )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          55.21 using 59 PHA bins.
#Fit statistic : Chi-Squared =          46.37 using 59 PHA bins.
#Fit statistic : Chi-Squared =          46.34 using 59 PHA bins.
# Reduced chi-squared =          1.004 for     55 degrees of freedom 
# Reduced chi-squared =         0.8431 for     55 degrees of freedom 
# Reduced chi-squared =         0.8425 for     55 degrees of freedom 
# Null hypothesis probability =   4.668134e-01
# Null hypothesis probability =   7.897459e-01
# Null hypothesis probability =   7.907981e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  2.876e-09   9.685e-10
25- 50  1.724e-08   4.775e-09
50-150  9.803e-08   2.257e-08
15-150  1.181e-07   2.724e-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: 0.794886     ( -0.250689   0.232794 )
Norm@50keV  : 1.10396E-02    ( -0.00162854   0.00158856 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          50.30 using 59 PHA bins.
# Reduced chi-squared =         0.8825 for     57 degrees of freedom 
# Null hypothesis probability =   7.226038e-01
 
Photon flux (15-150 keV)    in 1.088 sec: 1.26905 ( -0.179082  0.180275 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.40663e-07 ( -1.90668e-08  1.9113e-08 ) ergs/cm2

Cutoff power-law model

Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 0.626821     ( -1.03686   0.623252 )
Epeak [keV] : 499.274      ( -500.136 -500.136 )
Norm@50keV  : 1.29966E-02    ( -0.00309096   0.0207787 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          50.20 using 59 PHA bins.
# Reduced chi-squared =         0.8964 for     56 degrees of freedom 
# Null hypothesis probability =   6.930456e-01
 
Photon flux (15-150 keV)    in 1.088 sec: 1.26276 ( -0.18127  0.18215 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.40128e-07 ( -1.96721e-08  1.93729e-08 ) ergs/cm2

Band function

 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -0.732639   ( 0.732639   0.732639 )
beta        : -0.794892    ( -0.232794   0.250667 )
Epeak [keV] : 15.6074      ( -15.6074 -15.6074 )
Norm@50keV   : 1.64507E-02    ( -0.00698718   0 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          50.30 using 59 PHA bins.
# Reduced chi-squared =         0.9146 for     55 degrees of freedom 
# Null hypothesis probability =   6.544156e-01
 
Photon flux (15-150 keV)    in 1.088 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)  = 2.26e-08
S(50-100 keV) = 5.21e-08

T90 vs. Hardness ratio plot

T90                                   = 1.01600003242493 sec.
Hardness ratio (energy fluence ratio) = 2.30531

Color vs. Color plot

Count Ratio  (25-50 keV) / (15-25 keV) = 5.42334
Count Ratio (50-100 keV) / (15-25 keV) = 5.62636

Mask shadow pattern

IMX = 8.226525908598192E-01, IMY = 9.408322069180867E-02

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:
-749.147400 -701.951500
-239.048000 0.040000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
270.3177 -25.0077   28.7  52.3  -22.9  -0.2000  -0.4    4.7	GX 5-1                        
270.3433 -25.7713    6.1  52.0  -23.8   0.9280   1.9    2.8	GRS 1758-258                  
273.9756 -14.0916    6.1  53.5   -8.6  -0.9896  -1.9    3.7	GX 17+2                       
275.9018 -30.3141    3.7  46.0  -27.7   1.1091   3.2    3.4	H1820-303                     
285.1834 -24.9763    5.4  39.5  -16.8   0.5618   2.1    8.7	HT1900.1-2455                 
  0.3101 -52.9875    2.3  31.8 -138.9   1.1531   5.1 ------	UNKNOWN

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

Time interval of the image:
0.040000 1.128000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
270.3121 -25.2938    0.0  52.2  -23.3  -0.0543  -1.8   13.0	GX 5-1                        
270.4466 -25.7473    4.9  51.9  -23.7   0.0684   2.4    7.8	GRS 1758-258                  
273.9731 -14.0226   14.2  53.5   -8.6   0.0259   0.8    2.1	GX 17+2                       
275.9173 -30.2673   13.6  46.0  -27.6   0.0165   0.8    6.0	H1820-303                     
284.9193 -24.9871    5.4  39.8  -16.9   0.0325   2.1    7.5	HT1900.1-2455                 
 28.4955 -22.3963    2.6  52.7  173.1   0.1482   4.5 ------	UNKNOWN                       
287.6671 -18.8667    1.1  39.6   -6.5   0.1762  10.6 ------	UNKNOWN

Post-slew image of 15-350 keV band

Time interval of the image:
94.452600 962.978400
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
244.9777 -15.6512    0.9  40.8  -87.5  24.9027  12.4    0.7	Sco X-1                       
255.9144 -37.7923    4.0  33.5 -126.3   1.9060   2.9    4.6	4U 1700-377                   
256.4657 -36.3822    1.4  32.5 -124.2   5.2754   8.1    2.9	GX 349+2                      
263.0138 -24.8204    5.1  23.6 -104.2   1.1876   2.3    4.5	GX 1+4                        
264.9163 -44.5856   11.8  32.0 -143.8   0.5275   1.0   11.0	4U 1735-44                    
268.3629  -1.4420    1.1  25.7  -44.8   4.9142  10.3    0.7	SW J1753.5-0127               
270.3110 -25.0896    1.2  17.3 -109.4   3.8270   9.8    1.6	GX 5-1                        
270.2558 -25.7373    2.8  17.5 -111.4   1.6676   4.2    2.5	GRS 1758-258                  
274.0613 -14.0838    2.7  13.9  -67.1   1.8255   4.3    4.3	GX 17+2                       
275.9486 -30.3227    2.4  15.6 -134.5   1.8855   4.8    2.9	H1820-303                     
285.0024 -24.8518    3.6   6.5 -153.1   1.2571   3.2    4.5	HT1900.1-2455                 
288.7996  10.9520    0.5  29.8    7.0  12.5672  25.0    0.4	GRS 1915+105                  
262.9681 -33.8361    1.6  26.6 -124.4   3.6752   7.1    1.0	GX 354-0                      
282.0408  15.8770    3.6  35.2   -4.6   1.7749   3.2 ------	UNKNOWN                       
277.3167 -23.7832    1.7  10.8 -114.0   2.8978   6.9 ------	UNKNOWN                       
272.4305  22.3529    2.7  43.8  -15.8   3.0446   4.3 ------	UNKNOWN                       
270.0787 -13.1252    3.6  17.9  -69.1   1.4339   3.3 ------	UNKNOWN                       
266.8384 -27.3566    1.5  20.9 -113.0   3.6434   7.7 ------	UNKNOWN                       
255.2011 -41.6439    2.3  35.8 -131.8   3.4721   5.1 ------	UNKNOWN                       
258.7210   2.8784    2.4  35.8  -50.9   3.0206   4.9 ------	UNKNOWN

Plot creation:
Sun May 31 06:35:49 EDT 2015