batgrbproduct analysis for trigger=175942

batgrbproduct Analysis for Trigger=175942

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 19:10:33 EST 2014
             Host Name: batevent1
   Current Working Dir: /local/data/batevent/batevent_reproc/trigger175942
======================================================================

  Trigger: 00175942      Segment: 000

  BAT Trigger Time: 158136568.384   [s; MET]
      Trigger Stop: 158136569.408   [s; MET]
               UTC: 2006-01-05T06:49:27.446760    [includes UTCF correction] 
       Where From?: TDRSS position message

  BAT 
    RA: 297.473683880003   Dec: 46.3625146711849  [deg; J2000]

     Catalogged Source?: NO
     Point Source?:      YES
     GRB Indicated?:     YES    [ by BAT flight software ]
     Image S/N Ratio:    14.4
     Image Trigger?:     NO
     Rate S/N Ratio:     77.7045687202497  [ if not an image trigger ]
     Image S/N Ratio:    14.4

  Flight Position:   [ source = BAT ]
    RA: 297.473683880003   Dec: 46.3625146711849  [deg; J2000]

  Ground Position:   [ source = BAT pre-slew burst ]
    RA: 297.490792296574   Dec: 46.3553167009083  [deg; J2000]  
        { 19h 49m 57.8s , +46d 21' 19.1" }
         +/- 0.909580578003676 [arcmin] (estimated 90% radius based on SNR)
         +/- 0.264805068930653 [arcmin] (formal 1-sigma fit error)
    SNR: 34.8270505702139
 
  Angular difference between Flight and Ground position is 0.829694 arcmin
 
  Partial Coding Fraction: 0.2851562    [ including projection effects ]

  Duration
     T90: 54.3760000169277 +/- 1.42005071887118
        Measured from: -17.8760000169277
                   to: 36.5     [s; relative to TRIGTIME]
     T50: 25.944000005722 +/- 0.413879213185527
        Measured from: 4.17199999094009
                   to: 30.1159999966621     [s; relative to TRIGTIME]



  Fluence
     Peak Flux  (peak 1 second)
        Measured from: 30.4160000085831     
                   to: 31.4160000085831     [s; relative to TRIGTIME]
     Total Fluence        
        Measured from: -21.0480000078678     
                   to: 66.5399999916553     [s; relative to TRIGTIME]
     
             Band 1     Band 2     Band 3     Band 4
              15-25      25-50     50-100    100-350     keV
 Total     4.145485   7.699234   8.605156   3.526818
           0.089326   0.100687   0.099278   0.085742 [error]
 Peak      0.137210   0.285700   0.350326   0.144956
           0.011097   0.013568   0.014763   0.011720 [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 1.46e-06 3.50e-06 6.71e-06 3.14e-05 1.82e-05 4.31e-05   erg/cm2
              Error 5.83e-08 8.26e-08 1.14e-07 1.30e-06 3.01e-07 1.32e-06   erg/cm2
Peak flux Power-law 1.48e+00 2.12e+00 2.27e+00 4.52e+00 7.28e+00 1.04e+01   ph/cm2/s
              Error 1.51e-01 1.32e-01 1.14e-01 4.96e-01 3.57e-01 5.59e-01   ph/cm2/s
 
Fluence   Cutoff-PL 1.45e-06 3.51e-06 6.72e-06 3.12e-05 1.82e-05 4.28e-05   erg/cm2
              Error 4.96e-08 8.16e-08 1.13e-07 2.09e-06 3.00e-07 2.06e-06   erg/cm2
Peak flux Cutoff-PL 1.39e+00 2.14e+00 2.34e+00 3.65e+00 7.22e+00 9.53e+00   ph/cm2/s
              Error 1.45e-01 1.39e-01 1.49e-01 1.04e+00 3.64e-01 1.10e+00   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    1.062    0.032    -      -           1.96e-02 3.49e-04   37.300 57
CPL   1.057    0.032    9999.4    0.0      1.97e-02 1.11e-03   37.340 56
 
 
=== 1-s peak spectral analysis ===
 
Model Ph_index Ph_90err Epeak  Epeak_90err Norm     Nomr_90err chi2   dof
PL    0.903    0.084    -      -           6.34e-02 3.09e-03   65.090 57
CPL   0.682    0.268     359.7    0.0      7.88e-02 2.40e-02   63.690 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: 53.312000 sec.
T50 in the 50-300 keV band: 25.536000 sec.

 
=== Table of the duration information ==
 
        Value   tstart    tstop
T100   87.588  -21.048   66.540
T90    54.376  -17.876   36.500
T50    25.944    4.172   30.116
Peak    1.000   30.416   31.416

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
  297.4908    46.3553   0.0056    42.9199    20.8052        11.9637806     34.827 TRIG_00175942                 
 
Foreground time interval of the image:
-21.048  15.317 (delta_t =  36.365 [sec])
Background time interval of the image:
-27.483 -21.048 (delta_t =   6.435 [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 1.024000

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 1.024000

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 1.024000

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  -21.048 sec. to   66.540 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.06218     ( -0.0316875   0.0315247 )
Norm@50keV  : 1.95825E-02    ( -0.000349956   0.000348495 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          37.30 using 59 PHA bins.
# Reduced chi-squared =         0.6544 for     57 degrees of freedom 
# Null hypothesis probability =   9.798102e-01
 
Photon flux (15-150 keV)    in 87.59 sec: 2.26385 ( -0.042938  0.0431194 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.81556e-05 ( -3.007e-07  3.0081e-07 ) ergs/cm2

Cutoff power-law model

Time interval is from  -21.048 sec. to   66.540 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.05657     ( -0.032354   0.0313775 )
Epeak [keV] : 9999.36      ( -9999.36 -9999.36 )
Norm@50keV  : 1.96906E-02    ( -0.000330926   0.00188551 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          37.34 using 59 PHA bins.
# Reduced chi-squared =         0.6669 for     56 degrees of freedom 
# Null hypothesis probability =   9.740240e-01
 
Photon flux (15-150 keV)    in 87.59 sec: 2.26360 (    ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.81608e-05 ( -2.9912e-07  3.0131e-07 ) ergs/cm2

Band function

Time interval is from  -21.048 sec. to   66.540 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -9.46757E-02   ( 0.850922   0.850922 )
beta        : -1.07073    ( -0.0315236   0.0316885 )
Epeak [keV] : 54.1719      ( -54.1346 212.663 )
Norm@50keV   : 9.27009E-02    ( -0.0933352   730147 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          36.21 using 59 PHA bins.
# Reduced chi-squared =         0.6584 for     55 degrees of freedom 
# Null hypothesis probability =   9.763475e-01
 
Photon flux (15-150 keV)    in 87.59 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]    : 24.7417  (  )
R^2/D10^2   : 5.40107E-02  (   )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =         680.26 using 59 PHA bins.
# Reduced chi-squared =         11.934 for     57 degrees of freedom 
# Null hypothesis probability =  1.515975e-107
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  5.058e-07   1.857e-08
25- 50  2.855e-06   7.620e-08
50-150  1.298e-05   2.890e-07
15-150  1.634e-05   3.022e-07

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 199.363       (      )
Norm        : 10.0821       (     )
------------------------------------------------------------
#Fit statistic : Chi-Squared =         851.05 using 59 PHA bins.
# Reduced chi-squared =         14.931 for     57 degrees of freedom 
# Null hypothesis probability =  5.784507e-142
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  2.199e-06   4.248e-08
25- 50  4.230e-06   8.014e-08
50-150  9.278e-06   1.752e-07
15-150  1.571e-05   2.978e-07

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 8.96322        (-0.639568      0.685385)
R1^2/D10^2  : 0.790041        (-0.164963      0.218446)
kT2 [keV]   : 39.4713        (-2.55049      3.14237)
R2^2/D10^2  : 1.10446E-02    (-0.00229058   0.0025498)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          36.36 using 59 PHA bins.
# Reduced chi-squared =         0.6611 for     55 degrees of freedom 
# Null hypothesis probability =   9.752823e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.276e-06   8.803e-08
25- 50  3.615e-06   1.340e-07
50-150  1.340e-05   3.635e-07
15-150  1.829e-05   4.993e-07

Peak spectrum fit

Power-law model

Time interval is from   30.416 sec. to   31.416 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 0.902569     ( -0.084061   0.0829502 )
Norm@50keV  : 6.34001E-02    ( -0.00309872   0.00308937 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          65.09 using 59 PHA bins.
# Reduced chi-squared =          1.142 for     57 degrees of freedom 
# Null hypothesis probability =   2.159046e-01
 
Photon flux (15-150 keV)    in 1 sec: 7.27703 ( -0.356349  0.356776 ) ph/cm2/s
Energy fluence (15-150 keV)             : 7.1081e-07 ( -3.65337e-08  3.66087e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from   30.416 sec. to   31.416 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 0.681830     ( -0.340988   0.19535 )
Epeak [keV] : 359.678      ( -359.689 -359.689 )
Norm@50keV  : 7.88115E-02    ( -0.0178765   0.0301428 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          63.69 using 59 PHA bins.
# Reduced chi-squared =          1.137 for     56 degrees of freedom 
# Null hypothesis probability =   2.241186e-01
 
Photon flux (15-150 keV)    in 1 sec: 7.22458 ( -0.36387  0.3641 ) ph/cm2/s
Energy fluence (15-150 keV)             : 7.06768e-07 ( -3.7579e-08  3.7433e-08 ) ergs/cm2

Band function

Time interval is from   30.416 sec. to   31.416 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : 4.99998   ( -4.99998   -4.99998 )
beta        : -0.934831    ( -0.0894287   0.0893581 )
Epeak [keV] : 26.6266      ( -26.6266 5.36745 )
Norm@50keV   : 2723.30    ( -128.682   7.33351e+06 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          63.15 using 59 PHA bins.
# Reduced chi-squared =          1.148 for     55 degrees of freedom 
# Null hypothesis probability =   2.105331e-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]    : 24.3845  (  )
R^2/D10^2   : 0.196306  (   )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =         128.19 using 59 PHA bins.
# Reduced chi-squared =         2.2489 for     57 degrees of freedom 
# Null hypothesis probability =   2.129692e-07
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  2.054e-08   2.010e-09
25- 50  1.151e-07   8.800e-09
50-150  5.089e-07   3.650e-08
15-150  6.445e-07   3.855e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 199.363       (      )
Norm        : 29.0047       (     )
------------------------------------------------------------
#Fit statistic : Chi-Squared =         225.59 using 59 PHA bins.
# Reduced chi-squared =         3.9577 for     57 degrees of freedom 
# Null hypothesis probability =   6.500153e-22
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  7.222e-08   3.880e-09
25- 50  1.389e-07   7.600e-09
50-150  3.047e-07   4.470e-08
15-150  5.159e-07   3.370e-08

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 8.89645        (-1.98429      2.43278)
R1^2/D10^2  : 2.16454        (-1.05025      2.54934)
kT2 [keV]   : 37.7854        (-6.03048      11.5394)
R2^2/D10^2  : 4.54457E-02    (-0.0248162   0.0272084)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          63.46 using 59 PHA bins.
# Reduced chi-squared =          1.154 for     55 degrees of freedom 
# Null hypothesis probability =   2.027781e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  4.187e-08   1.021e-08
25- 50  1.276e-07   2.401e-08
50-150  5.452e-07   1.109e-07
15-150  7.147e-07   1.232e-07

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: 0.961186     ( -0.0430026   0.0426608 )
Norm@50keV  : 2.28154E-02    ( -0.000551798   0.000549727 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          31.22 using 59 PHA bins.
# Reduced chi-squared =         0.5478 for     57 degrees of freedom 
# Null hypothesis probability =   9.978530e-01
 
Photon flux (15-150 keV)    in 36.36 sec: 2.62224 ( -0.0648676  0.0650663 ) ph/cm2/s
Energy fluence (15-150 keV)             : 9.09724e-06 ( -2.07832e-07  2.07926e-07 ) ergs/cm2

Cutoff power-law model

Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 0.957206     ( -0.0455187   0.0410945 )
Epeak [keV] : 9999.36      ( -9999.36 -9999.36 )
Norm@50keV  : 2.29537E-02    ( -0.000515153   0.00220839 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          31.34 using 59 PHA bins.
# Reduced chi-squared =         0.5597 for     56 degrees of freedom 
# Null hypothesis probability =   9.968782e-01
 
Photon flux (15-150 keV)    in 36.36 sec: 2.62108 (    ) ph/cm2/s
Energy fluence (15-150 keV)             : 9.09774e-06 ( -2.06525e-07  2.09615e-07 ) ergs/cm2

Band function

 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -0.497174   ( 0.792182   0.792182 )
beta        : -0.966432    ( -0.0426585   0.0430068 )
Epeak [keV] : 89.1927      ( -88.7285 338.919 )
Norm@50keV   : 4.81207E-02    ( -0.0264261   0.437014 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          30.98 using 59 PHA bins.
# Reduced chi-squared =         0.5633 for     55 degrees of freedom 
# Null hypothesis probability =   9.963312e-01
 
Photon flux (15-150 keV)    in 36.36 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)  = 3.50e-06
S(50-100 keV) = 6.71e-06

T90 vs. Hardness ratio plot

T90                                   = 54.3760000169277 sec.
Hardness ratio (energy fluence ratio) = 1.91714

Color vs. Color plot

Count Ratio  (25-50 keV) / (15-25 keV) = 1.85726
Count Ratio (50-100 keV) / (15-25 keV) = 2.07579

Mask shadow pattern

IMX = 8.692680592359927E-01, IMY = -3.302945234494673E-01

TIME vs. PHA plot around the trigger time

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.024000

TIME vs. DetID plot around the trigger time

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.024000

100 us light curve (15-350 keV)

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.024000

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:
-27.483400 -21.048000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
288.8145  10.9732    3.0  37.8  -35.9   0.1359   3.8    1.9	GRS 1915+105                  
299.6374  35.1920    1.5  34.4    8.8   0.2470   7.9    2.4	Cyg X-1                       
308.1896  40.7799    0.0  33.7   24.4  -0.0637  -1.9   11.0	Cyg X-3                       
326.1115  38.3725   52.5  26.7   48.9   0.0066   0.2    4.2	Cyg X-2                       
334.4990  47.3408    2.6  36.2   59.3   0.2560   4.5 ------	UNKNOWN                       
 14.5090  -4.7581    2.8  49.7  157.7   0.3147   4.1 ------	UNKNOWN                       
276.3041  39.5650    2.5  52.9    2.4   0.3543   4.6 ------	UNKNOWN                       
307.9951  27.6616    2.4  24.2    5.3   0.1211   4.9 ------	UNKNOWN                       
352.6488 -28.2649    2.8  46.8 -159.9   0.1854   4.1 ------	UNKNOWN                       
316.8707 -13.1302    2.6  26.9 -105.8   0.1377   4.4 ------	UNKNOWN

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

Time interval of the image:
-21.048000 15.316620
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
288.7627  10.9694 1547.7  37.8  -35.9  -0.0017  -0.0    2.5	GRS 1915+105                  
299.8137  35.2521    7.4  34.3    9.1  -0.3358  -1.5   11.4	Cyg X-1                       
307.9616  41.0473   62.0  34.0   24.5  -0.0455  -0.2    8.8	Cyg X-3                       
326.1975  38.1318    0.0  26.5   49.1  -0.0859  -0.4   11.5	Cyg X-2                       
330.5127  48.4691    2.3  36.9   54.6   1.9190   5.0 ------	UNKNOWN                       
297.4908  46.3553    0.3  42.9   20.8  11.9638  34.8 ------	UNKNOWN                       
300.4955  38.2015    2.1  35.8   13.7   1.2333   5.5 ------	UNKNOWN                       
339.4576 -20.1625    2.1  34.0 -149.5   0.9876   5.4 ------	UNKNOWN

Post-slew image of 15-350 keV band

Time interval of the image:
76.716590 302.672800
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
254.4487  35.2769    7.1  33.9  -14.6   0.3417   1.6    4.0	Her X-1                       
288.7847  10.9430    1.7  36.2  -86.7   3.1661   7.0    0.8	GRS 1915+105                  
299.5954  35.2005    0.2  11.3 -110.1   8.5628  51.8    0.3	Cyg X-1                       
308.0772  40.9720    1.4   9.4 -159.9   1.3565   8.3    1.9	Cyg X-3                       
326.0841  38.4460    3.2  22.4  179.2   0.5818   3.6    8.5	Cyg X-2                       
261.9401  52.3445    2.2  23.6   16.5   0.9282   5.1 ------	UNKNOWN                       
352.4429  24.0744    1.9  48.9  176.2   2.3139   6.0 ------	UNKNOWN                       
297.3729  46.3538    2.3   0.1  -23.4   0.8229   4.9 ------	UNKNOWN                       
265.2287  34.5538    2.5  27.0  -25.6   0.7697   4.7 ------	UNKNOWN                       
230.3134  23.0171    2.6  58.0  -10.4   4.2701   4.5 ------	UNKNOWN

Plot creation:
Sun May 31 14:47:12 EDT 2015