batgrbproduct analysis for trigger=440955

batgrbproduct Analysis for Trigger=440955

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): Fri Jan 17 14:57:29 EST 2014
             Host Name: batevent1
   Current Working Dir: /local/data/batevent/batevent_reproc/trigger440955
======================================================================

  Trigger: 00440955      Segment: 000

  BAT Trigger Time: 314861240.256   [s; MET]
      Trigger Stop: 314861240.512   [s; MET]
               UTC: 2010-12-24T05:27:13.761240    [includes UTCF correction] 
       Where From?: TDRSS position message

  BAT 
    RA: 285.926038610832   Dec: 45.7154744502681  [deg; J2000]

     Catalogged Source?: NO
     Point Source?:      YES
     GRB Indicated?:     YES    [ by BAT flight software ]
     Image S/N Ratio:    9.17
     Image Trigger?:     NO
     Rate S/N Ratio:     18.4661853126194  [ if not an image trigger ]
     Image S/N Ratio:    9.17

  Flight Position:   [ source = BAT ]
    RA: 285.926038610832   Dec: 45.7154744502681  [deg; J2000]

  Ground Position:   [ source = BAT pre-slew burst ]
    RA: 285.939544758496   Dec: 45.7061061793522  [deg; J2000]  
        { 19h 03m 45.5s , +45d 42' 22.0" }
         +/- 2.09718152589513 [arcmin] (estimated 90% radius based on SNR)
         +/- 0.905015927662979 [arcmin] (formal 1-sigma fit error)
    SNR: 10.5593782379298
 
  Angular difference between Flight and Ground position is 0.797593 arcmin
 
  Partial Coding Fraction: 0.5390625    [ including projection effects ]

  Duration
     T90: 0.24399995803833 +/- 0.042520585314364
        Measured from: 0.0360000133514404
                   to: 0.279999971389771     [s; relative to TRIGTIME]
     T50: 0.135999977588654 +/- 0.033941109986914
        Measured from: 0.0879999995231628
                   to: 0.223999977111816     [s; relative to TRIGTIME]



  Fluence
     Peak Flux  (peak 1 second)
        Measured from: -0.337999999523163     
                   to: 0.662000000476837     [s; relative to TRIGTIME]
     Total Fluence        
        Measured from: 0.0239999890327454     
                   to: 0.296000003814697     [s; relative to TRIGTIME]
     
             Band 1     Band 2     Band 3     Band 4
              15-25      25-50     50-100    100-350     keV
 Total     0.008106   0.031051   0.039613   0.017654
           0.004590   0.005382   0.005129   0.003901 [error]
 Peak      0.008687   0.036580   0.036461   0.016309
           0.007933   0.008644   0.007795   0.006652 [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 4.43e-09 1.08e-08 2.08e-08 9.92e-08 5.63e-08 1.35e-07   erg/cm2
              Error 1.49e-09 2.39e-09 4.06e-09 3.79e-08 1.08e-08 4.06e-08   erg/cm2
Peak flux Power-law 1.16e-01 1.88e-01 2.30e-01 5.53e-01 6.92e-01 1.09e+00   ph/cm2/s
              Error 7.36e-02 7.44e-02 5.95e-02 3.18e-01 1.94e-01 3.24e-01   ph/cm2/s
 
Fluence   Cutoff-PL 2.38e-09 1.15e-08 2.74e-08 2.74e-08 5.80e-08 6.86e-08   erg/cm2
              Error 1.68e-09 3.19e-09 5.94e-09 2.19e-08 1.13e-08 2.35e-08   erg/cm2
Peak flux Cutoff-PL 9.65e-02 1.93e-01 2.49e-01 3.03e-01 6.79e-01 8.43e-01   ph/cm2/s
              Error 9.59e-02 8.34e-02 7.70e-02 3.51e-01 1.96e-01 3.81e-01   ph/cm2/s
 
Fluence        Band 2.39e-09 1.14e-08 2.73e-08 2.76e-08 5.80e-08 6.89e-08   erg/cm2
              Error -------- 2.70e-09 5.41e-09 -------- -------- --------   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    1.046    0.262    -      -           1.95e-02 3.71e-03   71.540 57
CPL  -0.928    1.519      95.8   35.4      1.18e-01 2.30e-01   62.830 56
 
 
=== 1-s peak spectral analysis ===
 
Model Ph_index Ph_90err Epeak  Epeak_90err Norm     Nomr_90err chi2   dof
PL    0.710    0.485    -      -           5.99e-03 1.80e-03   45.310 57
CPL   0.051    1.297     176.2    0.0      1.15e-02 6.26e-02   44.900 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: 0.192000 sec.
T50 in the 50-300 keV band: 0.128000 sec.

 
=== Table of the duration information ==
 
        Value   tstart    tstop
T100    0.272    0.024    0.296
T90     0.244    0.036    0.280
T50     0.136    0.088    0.224
Peak    1.000   -0.338    0.662

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
  285.9395    45.7061   0.0183    27.1393    47.5341         0.1030458     10.559 TRIG_00440955                 
 
Foreground time interval of the image:
  0.024   0.296 (delta_t =   0.272 [sec])
Background time interval of the image:
-239.256   0.024 (delta_t = 239.280 [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    0.024 sec. to    0.296 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.04639     ( -0.266018   0.258725 )
Norm@50keV  : 1.94644E-02    ( -0.00372087   0.00370128 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          71.54 using 59 PHA bins.
# Reduced chi-squared =          1.255 for     57 degrees of freedom 
# Null hypothesis probability =   9.314857e-02
 
Photon flux (15-150 keV)    in 0.272 sec: 2.24707 ( -0.437678  0.440501 ) ph/cm2/s
Energy fluence (15-150 keV)             : 5.63421e-08 ( -1.07856e-08  1.08112e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from    0.024 sec. to    0.296 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: -0.927587     ( -1.80365   1.23498 )
Epeak [keV] : 95.8109      ( -19.867 50.9007 )
Norm@50keV  : 0.118021    ( -0.117787   0.341803 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          62.83 using 59 PHA bins.
# Reduced chi-squared =          1.122 for     56 degrees of freedom 
# Null hypothesis probability =   2.471778e-01
 
Photon flux (15-150 keV)    in 0.272 sec: 2.17799 ( -0.22121  0.44273 ) ph/cm2/s
Energy fluence (15-150 keV)             : 5.79831e-08 ( -1.12953e-08  1.12627e-08 ) ergs/cm2

Band function

Time interval is from    0.024 sec. to    0.296 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : 0.921023   ( -0.937382   1.56061 )
beta        : -10.0000    ( 10   3.19744e-14 )
Epeak [keV] : 95.9415      ( -19.9673 50.7969 )
Norm@50keV   : 0.117307    ( -0.117307   0.342688 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          62.83 using 59 PHA bins.
# Reduced chi-squared =          1.142 for     55 degrees of freedom 
# Null hypothesis probability =   2.186210e-01
 
Photon flux (15-150 keV)    in 0.272 sec:  (    ) ph/cm2/s
Energy fluence (15-150 keV)             : 5.80067e-08 ( 0  0 ) ergs/cm2

Single BB

 
Spectral model blackbody:
------------------------------------------------------------
Parameters  : value    Lower 90%  Upper 90%
kT [keV]    : 23.5421  (-4.10039  4.91877)
R^2/D10^2   : 7.31014E-02  (-0.0337118   0.0614257)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          62.88 using 59 PHA bins.
# Reduced chi-squared =          1.103 for     57 degrees of freedom 
# Null hypothesis probability =   2.760425e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.974e-09   7.343e-10
25- 50  1.085e-08   3.612e-09
50-150  4.487e-08   1.503e-08
15-150  5.770e-08   1.446e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 200.000       (      )
Norm        : 9.33744       (-1.8393     1.83912)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          79.84 using 59 PHA bins.
# Reduced chi-squared =          1.401 for     57 degrees of freedom 
# Null hypothesis probability =   2.460162e-02
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  6.328e-09   3.691e-09
25- 50  1.217e-08   7.196e-09
50-150  2.670e-08   1.549e-08
15-150  4.520e-08   2.666e-08

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 7.95828        (-7.93751      191.751)
R1^2/D10^2  : 0.373020        (-0.377606      -0.377606)
kT2 [keV]   : 25.2693        (-5.33605      -25.2677)
R2^2/D10^2  : 5.47531E-02    (-0.0547975   0.0695123)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          62.24 using 59 PHA bins.
# Reduced chi-squared =          1.132 for     55 degrees of freedom 
# Null hypothesis probability =   2.342470e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  2.800e-09   1.605e-09
25- 50  1.138e-08   6.450e-09
50-150  4.481e-08   2.671e-08
15-150  5.899e-08   3.366e-08

Peak spectrum fit

Power-law model

Time interval is from   -0.338 sec. to    0.662 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 0.710471     ( -0.528628   0.441991 )
Norm@50keV  : 5.98976E-03    ( -0.00184341   0.00174683 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          45.31 using 59 PHA bins.
# Reduced chi-squared =         0.7950 for     57 degrees of freedom 
# Null hypothesis probability =   8.678575e-01
 
Photon flux (15-150 keV)    in 1 sec: 0.691810 ( -0.192524  0.196157 ) ph/cm2/s
Energy fluence (15-150 keV)             : 7.27709e-08 ( -1.92658e-08  1.93668e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from   -0.338 sec. to    0.662 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 5.08966E-02     ( -2.64219   -0.0477609 )
Epeak [keV] : 176.239      ( -176.086 -176.086 )
Norm@50keV  : 1.14908E-02    ( -0.00707766   0.118108 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          44.90 using 59 PHA bins.
# Reduced chi-squared =         0.8017 for     56 degrees of freedom 
# Null hypothesis probability =   8.562870e-01
 
Photon flux (15-150 keV)    in 1 sec: 0.678882 ( -0.193244  0.198294 ) ph/cm2/s
Energy fluence (15-150 keV)             : 7.09501e-08 ( -2.12456e-08  2.02015e-08 ) ergs/cm2

Band function

Time interval is from   -0.338 sec. to    0.662 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : 5.00000   ( -4.96474   -4.96474 )
beta        : -0.949646    ( -1.13608   0.615288 )
Epeak [keV] : 37.3951      ( -37.3954 31.8883 )
Norm@50keV   : 38.1978    ( -9.66454   854702 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          43.67 using 59 PHA bins.
# Reduced chi-squared =         0.7941 for     55 degrees of freedom 
# Null hypothesis probability =   8.642886e-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]    : 26.1426  (-8.1925  16.8613)
R^2/D10^2   : 1.57436E-02  (-0.0157198   0.03509)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          46.03 using 59 PHA bins.
# Reduced chi-squared =         0.8075 for     57 degrees of freedom 
# Null hypothesis probability =   8.505126e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.825e-09   1.143e-09
25- 50  1.058e-08   6.375e-09
50-150  5.322e-08   3.163e-08
15-150  6.563e-08   4.037e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 200.000       (      )
Norm        : 2.82574       (-0.831016     0.830905)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          54.56 using 59 PHA bins.
# Reduced chi-squared =         0.9572 for     57 degrees of freedom 
# Null hypothesis probability =   5.671242e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  7.035e-09   4.373e-09
25- 50  1.353e-08   8.295e-09
50-150  2.968e-08   1.840e-08
15-150  5.025e-08   3.131e-08

Double BB

R1^2/D10^2  : 4.10052E-04        (      )
kT2 [keV]   : 14.7060        (-14.7075      17.3259)
R2^2/D10^2  : 6.17424E-02    (-0.0617179   -0.0617179)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          44.09 using 59 PHA bins.
#Fit statistic : Chi-Squared =          43.91 using 59 PHA bins.
#Fit statistic : Chi-Squared =          43.90 using 59 PHA bins.
# Reduced chi-squared =         0.8016 for     55 degrees of freedom 
# Reduced chi-squared =         0.7984 for     55 degrees of freedom 
# Reduced chi-squared =         0.7982 for     55 degrees of freedom 
# Null hypothesis probability =   8.540219e-01
# Null hypothesis probability =   8.583971e-01
# Null hypothesis probability =   8.587026e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  3.134e-09   2.289e-09
25- 50  1.276e-08   8.865e-09
50-150  5.597e-08   2.904e-08
15-150  7.187e-08   3.898e-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: 1.04639     ( -0.266018   0.258725 )
Norm@50keV  : 1.94644E-02    ( -0.00372087   0.00370128 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          71.54 using 59 PHA bins.
# Reduced chi-squared =          1.255 for     57 degrees of freedom 
# Null hypothesis probability =   9.314857e-02
 
Photon flux (15-150 keV)    in 0.272 sec: 2.24707 ( -0.437678  0.440501 ) ph/cm2/s
Energy fluence (15-150 keV)             : 5.63421e-08 ( -1.07856e-08  1.08112e-08 ) ergs/cm2

Cutoff power-law model

Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: -0.927587     ( -1.80365   1.23498 )
Epeak [keV] : 95.8109      ( -19.867 50.9007 )
Norm@50keV  : 0.118021    ( -0.117787   0.341803 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          62.83 using 59 PHA bins.
# Reduced chi-squared =          1.122 for     56 degrees of freedom 
# Null hypothesis probability =   2.471778e-01
 
Photon flux (15-150 keV)    in 0.272 sec: 2.17799 ( -0.22121  0.44273 ) ph/cm2/s
Energy fluence (15-150 keV)             : 5.79831e-08 ( -1.12953e-08  1.12627e-08 ) ergs/cm2

Band function

 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : 0.921023   ( -0.937382   1.56061 )
beta        : -10.0000    ( 10   3.55271e-15 )
Epeak [keV] : 95.9415      ( -19.9673 50.7969 )
Norm@50keV   : 0.117307    ( -0.117307   0.342688 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          62.83 using 59 PHA bins.
# Reduced chi-squared =          1.142 for     55 degrees of freedom 
# Null hypothesis probability =   2.186210e-01
 
Photon flux (15-150 keV)    in 0.272 sec:  (    ) ph/cm2/s
Energy fluence (15-150 keV)             : 5.80067e-08 ( 0  0 ) ergs/cm2

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

S(25-50 keV)  = 1.08e-08
S(50-100 keV) = 2.08e-08

T90 vs. Hardness ratio plot

T90                                   = 0.24399995803833 sec.
Hardness ratio (energy fluence ratio) = 1.92593

Color vs. Color plot

Count Ratio  (25-50 keV) / (15-25 keV) = 3.83062
Count Ratio (50-100 keV) / (15-25 keV) = 4.88687

Mask shadow pattern

IMX = 3.460763347837418E-01, IMY = -3.781281415607399E-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:
-239.256000 0.024000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
254.4556  35.2211    5.5  37.6    1.8  -0.6155  -2.1    7.3	Her X-1                       
268.5421  -1.3839    0.0  31.7  -69.2   0.3098   0.9   11.2	SW J1753.5-0127               
274.1522 -14.0282    8.0  38.1  -90.7  -1.0463  -1.4    8.5	GX 17+2                       
288.8019  10.9382    0.6   9.3  -94.2   3.7388  18.7    0.5	GRS 1915+105                  
299.5910  35.2322    2.3  17.0   76.9   1.1889   5.0    1.8	Cyg X-1                       
308.0627  40.9638    2.3  25.2   85.8   1.5659   5.1    2.3	Cyg X-3                       
326.2311  38.3214    7.8  34.4  107.8   0.7757   1.5    2.8	Cyg X-2                       
242.3321   3.6175    2.7  51.9  -42.3   4.9761   4.4 ------	UNKNOWN                       
242.0702   3.6533    3.2  52.2  -42.1   4.4556   3.8 ------	UNKNOWN

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

Time interval of the image:
0.024000 0.296000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
254.3331  35.2434    6.3  37.7    1.8  -0.0185  -1.9    8.5	Her X-1                       
268.2618  -1.4118    7.7  32.0  -68.9  -0.0153  -1.5    6.8	SW J1753.5-0127               
274.0472 -14.0031   27.9  38.2  -90.6   0.0070   0.4    3.1	GX 17+2                       
288.8512  10.7416    0.0   9.4  -95.0  -0.0141  -1.9   12.6	GRS 1915+105                  
299.4988  35.3334   23.2  17.1   76.6   0.0039   0.5    9.1	Cyg X-1                       
308.3618  40.9923    5.7  25.4   86.2   0.0207   2.0   11.6	Cyg X-3                       
326.1416  38.1167    0.0  34.3  108.1  -0.0006  -0.0   12.4	Cyg X-2                       
285.9395  45.7061    1.1  27.1   47.5   0.1031  10.6 ------	UNKNOWN                       
338.3057  -0.1028    2.5  48.3  166.8   0.0903   4.6 ------	UNKNOWN                       
263.4171  21.8690    2.0  27.9  -20.8   0.0419   5.8 ------	UNKNOWN                       
229.2339  27.4189    1.6  58.6  -10.4   0.2825   7.1 ------	UNKNOWN

Post-slew image of 15-350 keV band

Time interval of the image:
61.644600 962.789600
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
254.6623  35.2444   12.5  25.7  -25.8  -0.4507  -0.9   11.6	Her X-1                       
288.8000  10.9387    0.8  34.8 -107.9  12.3897  13.7    0.4	GRS 1915+105                  
299.5806  35.1966    1.7  14.7 -152.3   3.2026   6.8    0.6	Cyg X-1                       
308.1409  40.9893    1.6  16.8  175.4   3.6373   7.0    2.6	Cyg X-3                       
326.0331  38.3131    4.7  30.4  166.7   1.6472   2.5    6.5	Cyg X-2                       
220.2148  21.2871    3.1  58.1  -14.3   9.5353   3.8 ------	UNKNOWN                       
220.7184  18.6301    3.0  59.6  -17.0  12.2976   3.9 ------	UNKNOWN                       
259.3733  11.5397    2.7  40.9  -61.0   6.4081   4.2 ------	UNKNOWN                       
251.3405   9.1650    3.9  47.0  -52.9   6.8963   3.0 ------	UNKNOWN                       
241.7345   9.7991    4.0  52.0  -42.3   8.3374   2.9 ------	UNKNOWN                       
278.9798   5.1757    3.4  41.0  -92.4   7.3041   3.4 ------	UNKNOWN

Plot creation:
Sat May 30 23:19:12 EDT 2015