batgrbproduct analysis for trigger=155408

batgrbproduct Analysis for Trigger=155408

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): Wed Jan 22 20:10:23 EST 2014
             Host Name: batevent1
   Current Working Dir: /local/data/batevent/batevent_reproc/trigger155408
======================================================================

  Trigger: 00155408      Segment: 000

  BAT Trigger Time: 148581352   [s; MET]
      Trigger Stop: 148581472   [s; MET]
               UTC: 2005-09-16T16:35:52.267640    [includes UTCF correction] 
       Where From?: TDRSS position message

  BAT 
    RA: 135.992250681767   Dec: -51.4255835934932  [deg; J2000]

     Catalogged Source?: NO
     Point Source?:      YES
     GRB Indicated?:     YES    [ by BAT flight software ]
     Image S/N Ratio:    8.77
     Image Trigger?:     YES
     Rate S/N Ratio:     0  [ if not an image trigger ]
     Image S/N Ratio:    8.77

  Flight Position:   [ source = BAT ]
    RA: 135.992250681767   Dec: -51.4255835934932  [deg; J2000]

  Ground Position:   [ source = BAT pre-slew image ]
    RA: 136.007745125   Dec: -51.4051369862  [deg; J2000]
        { 09h 04m 01.9s , -51d -24' -18.5" }
        +/- 2.08730754188 [arcmin] (estimated 90% radius based on SNR)
    SNR: 10.632199995

 
  Angular difference between Flight and Ground position is 1.356910 arcmin
 
  Partial Coding Fraction: 0.4179688    [ including projection effects ]

  Duration
     T90: 85.1840000152588 +/- 12.7242994355077
        Measured from: 11.4560000002384
                   to: 96.6400000154972     [s; relative to TRIGTIME]
     T50: 32.8960000276566 +/- 22.1224316868661
        Measured from: 25.419999986887
                   to: 58.3160000145435     [s; relative to TRIGTIME]



  Fluence
     Peak Flux  (peak 1 second)
        Measured from: 43.7199999988079     
                   to: 44.7199999988079     [s; relative to TRIGTIME]
     Total Fluence        
        Measured from: 7.38400000333786     
                   to: 105.615999996662     [s; relative to TRIGTIME]
     
             Band 1     Band 2     Band 3     Band 4
              15-25      25-50     50-100    100-350     keV
 Total     0.565474   0.778072   0.377587   0.119276
           0.079290   0.081186   0.071007   0.064000 [error]
 Peak      0.018843   0.029143   0.020229   0.013180
           0.008177   0.008702   0.007838   0.006720 [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 2.07e-07 3.18e-07 3.67e-07 8.11e-07 1.13e-06 1.70e-06   erg/cm2
              Error 4.02e-08 4.07e-08 6.98e-08 3.14e-07 1.65e-07 3.82e-07   erg/cm2
Peak flux Power-law 2.16e-01 2.21e-01 1.59e-01 1.83e-01 6.67e-01 7.78e-01   ph/cm2/s
              Error 1.20e-01 7.83e-02 6.26e-02 1.50e-01 2.22e-01 2.54e-01   ph/cm2/s
 
Fluence   Cutoff-PL 1.88e-07 3.52e-07 3.64e-07 2.29e-07 1.05e-06 1.13e-06   erg/cm2
              Error 4.75e-08 5.78e-08 8.36e-08 5.45e-07 1.95e-07 5.26e-07   erg/cm2
Peak flux Cutoff-PL 1.98e-01 2.36e-01 1.65e-01 8.99e-02 6.54e-01 6.89e-01   ph/cm2/s
              Error 1.40e-01 1.01e-01 7.40e-02 1.60e-01 2.32e-01 2.99e-01   ph/cm2/s
 
Fluence        Band 1.77e-07 3.66e-07 3.47e-07 4.47e-07 1.06e-06 1.33e-06   erg/cm2
              Error -------- -------- 8.08e-08 -------- -------- --------   erg/cm2
Peak flux      Band -------- -------- -------- -------- -------- --------   ph/cm2/s
              Error -------- -------- -------- -------- -------- --------   ph/cm2/s

 
=== Time-averaged spectral analysis ===
 
Model Ph_index Ph_90err Epeak  Epeak_90err Norm     Nomr_90err chi2   dof
PL    1.794    0.225    -      -           1.25e-03 1.78e-04   61.550 57
CPL   0.928    1.245      54.6  -20.2      3.78e-03 1.31e-02   59.690 56
 
 
=== 1-s peak spectral analysis ===
 
Model Ph_index Ph_90err Epeak  Epeak_90err Norm     Nomr_90err chi2   dof
PL    1.474    0.563    -      -           5.38e-03 1.76e-03   58.260 57
CPL   0.851    1.750      87.7    0.0      1.15e-02 7.71e-01   58.110 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: 41.472000 sec.
T50 in the 50-300 keV band: 26.048000 sec.

 
=== Table of the duration information ==
 
        Value   tstart    tstop
T100   98.232    7.384  105.616
T90    85.184   11.456   96.640
T50    32.896   25.420   58.316
Peak    1.000   43.720   44.720

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
136.008 -51.405 0.018 41.407 -145.312 1.941 10.632 TRIG_00155408
 
Image time interval: 0.000 to 120.000 [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 120.000000

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 120.000000

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 120.000000

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    7.384 sec. to  105.616 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.79431     ( -0.220187   0.228971 )
Norm@50keV  : 1.25148E-03    ( -0.000179721   0.000176454 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          61.55 using 59 PHA bins.
# Reduced chi-squared =          1.080 for     57 degrees of freedom 
# Null hypothesis probability =   3.165263e-01
 
Photon flux (15-150 keV)    in 98.23 sec: 0.172072 ( -0.0222627  0.0222917 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.13197e-06 ( -1.63934e-07  1.66453e-07 ) ergs/cm2

Cutoff power-law model

Time interval is from    7.384 sec. to  105.616 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 0.928111     ( -1.50201   0.98817 )
Epeak [keV] : 54.6285      ( -14.2045 -54.6388 )
Norm@50keV  : 3.78348E-03    ( -0.00377996   0.0224925 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          59.69 using 59 PHA bins.
# Reduced chi-squared =          1.066 for     56 degrees of freedom 
# Null hypothesis probability =   3.432236e-01
 
Photon flux (15-150 keV)    in 98.23 sec: 0.166391 ( -0.023733  0.023491 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.04652e-06 ( -1.91232e-07  1.97894e-07 ) ergs/cm2

Band function

Time interval is from    7.384 sec. to  105.616 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -0.354463   ( -1.30554   5.24829 )
beta        : -2.34534    ( 2.34495   0.57572 )
Epeak [keV] : 45.8382      ( -18.8629 39.847 )
Norm@50keV   : 8.59028E-03    ( -0.00945195   1.26566 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          58.50 using 59 PHA bins.
# Reduced chi-squared =          1.064 for     55 degrees of freedom 
# Null hypothesis probability =   3.482048e-01
 
Photon flux (15-150 keV)    in 98.23 sec:  (    ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.05934e-06 ( 0  0 ) ergs/cm2

Single BB

 
Spectral model blackbody:
------------------------------------------------------------
Parameters  : value    Lower 90%  Upper 90%
kT [keV]    : 11.4345  (-1.46074  1.72392)
R^2/D10^2   : 5.05598E-02  (-0.0208756   0.0340708)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          65.59 using 59 PHA bins.
# Reduced chi-squared =          1.151 for     57 degrees of freedom 
# Null hypothesis probability =   2.035029e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.366e-07   3.023e-08
25- 50  4.056e-07   7.181e-08
50-150  3.083e-07   9.543e-08
15-150  8.505e-07   1.350e-07

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 97.2632       (-34.3994      77.7674)
Norm        : 0.769784       (-0.129727     0.163879)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          59.92 using 59 PHA bins.
# Reduced chi-squared =          1.051 for     57 degrees of freedom 
# Null hypothesis probability =   3.701809e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.976e-07   3.561e-08
25- 50  3.398e-07   5.285e-08
50-150  5.419e-07   2.256e-07
15-150  1.079e-06   2.977e-07

Double BB

R1^2/D10^2  : 8.26326E-02        (-0.0393054      0.104169)
kT2 [keV]   : 69.9171        (-37.9821      -56.4871)
R2^2/D10^2  : 7.27087E-05    (   )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          61.46 using 59 PHA bins.
#Fit statistic : Chi-Squared =          58.12 using 59 PHA bins.
#Fit statistic : Chi-Squared =          58.02 using 59 PHA bins.
# Reduced chi-squared =          1.117 for     55 degrees of freedom 
# Reduced chi-squared =          1.057 for     55 degrees of freedom 
# Reduced chi-squared =          1.055 for     55 degrees of freedom 
# Null hypothesis probability =   2.557259e-01
# Null hypothesis probability =   3.610188e-01
# Null hypothesis probability =   3.646781e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.799e-07   7.607e-08
25- 50  3.674e-07   1.302e-07
50-150  3.663e-07   1.423e-07
15-150  9.136e-07   2.775e-07

Peak spectrum fit

Power-law model

Time interval is from   43.720 sec. to   44.720 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.47415     ( -0.567032   0.55993 )
Norm@50keV  : 5.37725E-03    ( -0.00177269   0.00175438 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          58.26 using 59 PHA bins.
# Reduced chi-squared =          1.022 for     57 degrees of freedom 
# Null hypothesis probability =   4.286962e-01
 
Photon flux (15-150 keV)    in 1 sec: 0.666740 ( -0.221769  0.223131 ) ph/cm2/s
Energy fluence (15-150 keV)             : 5.12345e-08 ( -1.78854e-08  1.82885e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from   43.720 sec. to   44.720 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 0.851347     ( -2.18976   1.31107 )
Epeak [keV] : 87.7375      ( -88.5343 -88.5343 )
Norm@50keV  : 1.15064E-02    ( -0.0113344   1.52974 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          58.11 using 59 PHA bins.
# Reduced chi-squared =          1.038 for     56 degrees of freedom 
# Null hypothesis probability =   3.974934e-01
 
Photon flux (15-150 keV)    in 1 sec: 0.653785 ( -0.23515  0.22965 ) ph/cm2/s
Energy fluence (15-150 keV)             : 4.87294e-08 ( -2.03238e-08  2.02897e-08 ) ergs/cm2

Band function

Time interval is from   43.720 sec. to   44.720 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : 5.00000   ( -5   -5 )
beta        : -1.59032    ( -1.47142   0.617747 )
Epeak [keV] : 24.4343      ( -24.4367 60.4136 )
Norm@50keV   : 672.079    ( -213.661   4.60778e+06 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          57.66 using 59 PHA bins.
# Reduced chi-squared =          1.048 for     55 degrees of freedom 
# Null hypothesis probability =   3.772913e-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]    : 14.3784  (-4.58213  7.16557)
R^2/D10^2   : 9.03434E-02  (-0.0902341   0.263096)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          59.27 using 59 PHA bins.
# Reduced chi-squared =          1.040 for     57 degrees of freedom 
# Null hypothesis probability =   3.927787e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  3.934e-09   2.502e-09
25- 50  1.502e-08   9.030e-09
50-150  2.072e-08   1.402e-08
15-150  3.967e-08   2.565e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 199.363       (-199.363      -199.363)
Norm        : 2.75738       (-0.888909     1.16074)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          58.18 using 59 PHA bins.
# Reduced chi-squared =          1.021 for     57 degrees of freedom 
# Null hypothesis probability =   4.315579e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  6.866e-09   4.247e-09
25- 50  1.321e-08   8.135e-09
50-150  2.897e-08   1.761e-08
15-150  4.904e-08   3.007e-08

Double BB

------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 199.141        (      )
R1^2/D10^2  : 7.01904E-05        (-7.07142e-05      0.168002)
kT2 [keV]   : 11.3377        (-8.35904      6.40014)
R2^2/D10^2  : 0.181738    (-0.143354   1.30255)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          58.22 using 59 PHA bins.
#Fit statistic : Chi-Squared =          57.15 using 59 PHA bins.
# Reduced chi-squared =          1.059 for     55 degrees of freedom 
# Reduced chi-squared =          1.039 for     55 degrees of freedom 
# Null hypothesis probability =   3.576344e-01
# Null hypothesis probability =   3.951081e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  5.875e-09   3.814e-09
25- 50  1.425e-08   8.315e-09
50-150  2.704e-08   1.529e-08
15-150  4.717e-08   2.627e-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: 1.79431     ( -0.220187   0.228971 )
Norm@50keV  : 1.25148E-03    ( -0.000179721   0.000176454 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          61.55 using 59 PHA bins.
# Reduced chi-squared =          1.080 for     57 degrees of freedom 
# Null hypothesis probability =   3.165263e-01
 
Photon flux (15-150 keV)    in 98.23 sec: 0.172072 ( -0.0222627  0.0222917 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.13197e-06 ( -1.63934e-07  1.66453e-07 ) ergs/cm2

Cutoff power-law model

Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 0.928111     ( -1.50201   0.98817 )
Epeak [keV] : 54.6285      ( -14.2045 -54.6388 )
Norm@50keV  : 3.78348E-03    ( -0.00377996   0.0224925 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          59.69 using 59 PHA bins.
# Reduced chi-squared =          1.066 for     56 degrees of freedom 
# Null hypothesis probability =   3.432236e-01
 
Photon flux (15-150 keV)    in 98.23 sec: 0.166391 ( -0.023733  0.023491 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.04652e-06 ( -1.91232e-07  1.97894e-07 ) ergs/cm2

Band function

 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -0.354463   ( -1.40458   5.27434 )
beta        : -2.34534    ( 2.34495   0.57572 )
Epeak [keV] : 45.8382      ( -18.8629 39.847 )
Norm@50keV   : 8.59028E-03    ( -0.00945195   1.26566 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          58.50 using 59 PHA bins.
# Reduced chi-squared =          1.064 for     55 degrees of freedom 
# Null hypothesis probability =   3.482048e-01
 
Photon flux (15-150 keV)    in 98.23 sec:  (    ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.05934e-06 ( 0  0 ) ergs/cm2

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

S(25-50 keV)  = 3.18e-07
S(50-100 keV) = 3.67e-07

T90 vs. Hardness ratio plot

T90                                   = 85.1840000152588 sec.
Hardness ratio (energy fluence ratio) = 1.15409

Color vs. Color plot

Count Ratio  (25-50 keV) / (15-25 keV) = 1.37596
Count Ratio (50-100 keV) / (15-25 keV) = 0.667735

Mask shadow pattern

IMX = -0.725101197699, IMY = 0.501860005705

TIME vs. PHA plot around the trigger time

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 120.000000

TIME vs. DetID plot around the trigger time

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 120.000000

100 us light curve (15-350 keV)

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 120.000000

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:
-6.299400 7.384000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
135.5686 -40.5039    6.6  50.8 -137.6  -0.2852  -1.7    3.6	Vela X-1                      
170.4491 -60.7096    5.1  21.7 -130.6   0.0797   2.3    6.5	Cen X-3                       
186.4556 -62.7532    3.7  14.4 -121.6   0.1008   3.1    5.6	GX 301-2                      
244.8821 -15.6442    6.2  54.4   -3.9   0.1926   1.9    5.6	Sco X-1                       
255.8558 -37.8425    6.1  35.9   18.7   0.0912   1.9    6.2	4U 1700-377                   
256.4359 -36.4989  191.3  37.3   18.5   0.0030   0.1    4.6	GX 349+2                      
263.1035 -24.7388    6.3  50.4   20.0   0.2163   1.8    5.2	GX 1+4                        
264.5433 -44.4062   13.0  33.0   34.2  -0.0414  -0.9    8.9	4U 1735-44                    
270.2337 -25.7467    4.2  51.8   28.2   0.4430   2.8    3.7	GRS 1758-258                  
275.8730 -30.4070    6.8  49.5   36.6   0.2774   1.7    3.6	H1820-303                     
263.1258 -33.8899   10.3  41.9   24.8   0.0706   1.1    7.6	GX 354-0                      
230.7250 -70.1032    3.3   5.0   93.3   0.1139   3.5 ------	UNKNOWN                       
 98.1856 -49.1335    2.2  55.3 -171.8   0.5673   5.2 ------	UNKNOWN

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

Time interval of the image:
7.384000 105.616000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
135.5385 -40.5358    5.2  50.8 -137.6   2.7770   2.2    1.2	Vela X-1                      
170.6316 -60.6828    4.8  21.6 -130.3  -0.6512  -2.4   10.0	Cen X-3                       
186.3250 -62.7361    4.6  14.4 -121.6  -0.5883  -2.5    9.3	GX 301-2                      
244.8765 -15.6603    6.9  54.4   -3.9  -1.2802  -1.7    6.1	Sco X-1                       
256.0047 -37.7791   30.5  36.0   18.8   0.1376   0.4    4.0	4U 1700-377                   
256.3599 -36.2663   25.0  37.5   18.2   0.1740   0.5   10.1	GX 349+2                      
263.0396 -24.8892   12.2  50.2   20.0  -0.8336  -0.9    8.8	GX 1+4                        
264.5382 -44.3826    6.2  33.0   34.2   0.6765   1.8    9.7	4U 1735-44                    
270.2682 -25.7571    4.7  51.8   28.3  -2.8943  -2.5    2.0	GRS 1758-258                  
275.8498 -30.4219    6.4  49.5   36.5  -2.1551  -1.8    5.1	H1820-303                     
263.1318 -33.8220   24.5  42.0   24.7  -0.2191  -0.5    7.2	GX 354-0                      
 82.7555 -51.2738    2.6  56.9  176.2   6.5271   4.4 ------	UNKNOWN                       
190.2724 -29.1614    2.9  42.0  -74.0   3.9208   4.0 ------	UNKNOWN

Post-slew image of 15-350 keV band

Time interval of the image:
193.500590 303.096300
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
135.4873 -40.5490    1.5  10.9 -136.3   0.7110   7.9    1.9	Vela X-1                      
170.2854 -60.5128    3.9  20.9   -5.1   0.2988   3.0    6.7	Cen X-3                       
186.7519 -62.8892    5.2  28.9   -1.1   0.2665   2.2    7.6	GX 301-2                      
 78.9403 -71.6009    2.4  31.9   75.9   0.8806   4.7 ------	UNKNOWN                       
 95.7865 -28.8519    2.3  37.4  157.3   0.7803   4.9 ------	UNKNOWN                       
201.3460 -32.8782    2.9  50.0  -39.3   1.5033   4.0 ------	UNKNOWN

Plot creation:
Wed Jul 15 01:04:22 EDT 2015