batgrbproduct analysis for trigger=631051

batgrbproduct Analysis for Trigger=631051

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 Mar  1 23:02:15 EST 2015
             Host Name: bat1
   Current Working Dir: /local/data/bat1/alien/Swift_3rdBATcatalog/event/batevent_reproc/trigger631051
======================================================================

  Trigger: 00631051      Segment: 000

  BAT Trigger Time: 445559504   [s; MET]
      Trigger Stop: 445559568   [s; MET]
               UTC: 2015-02-13T22:31:30.817240    [includes UTCF correction] 
       Where From?: TDRSS position message

  BAT 
    RA: 253.42510590632   Dec: 34.1786965238723  [deg; J2000]

     Catalogged Source?: NO
     Point Source?:      YES
     GRB Indicated?:     YES    [ by BAT flight software ]
     Image S/N Ratio:    8.03
     Image Trigger?:     YES
     Rate S/N Ratio:     0  [ if not an image trigger ]
     Image S/N Ratio:    8.03

  Flight Position:   [ source = BAT ]
    RA: 253.42510590632   Dec: 34.1786965238723  [deg; J2000]

  Ground Position:   [ source = BAT pre-slew burst ]
    RA: 253.447648236967   Dec: 34.1630797570746  [deg; J2000]  
        { 16h 53m 47.4s , +34d 09' 47.1" }
         +/- 1.80899661834305 [arcmin] (estimated 90% radius based on SNR)
         +/- 0.869108927567478 [arcmin] (formal 1-sigma fit error)
    SNR: 13.0421790621574
 
  Angular difference between Flight and Ground position is 1.459535 arcmin
 
  Partial Coding Fraction: 0.1367188    [ including projection effects ]

  Duration
     T90: 209 +/- 74.2428447730823
        Measured from: 9
                   to: 218     [s; relative to TRIGTIME]
     T50: 74 +/- 15.2315462117278
        Measured from: 26
                   to: 100     [s; relative to TRIGTIME]



  Fluence
     Peak Flux  (peak 1 second)
        Measured from: 18     
                   to: 19     [s; relative to TRIGTIME]
     Total Fluence        
        Measured from: 4     
                   to: 291     [s; relative to TRIGTIME]
     
             Band 1     Band 2     Band 3     Band 4
              15-25      25-50     50-100    100-350     keV
 Total     1.458925   2.391896   1.173747   0.509223
           0.167675   0.163898   0.137259   0.111195 [error]
 Peak      0.068577   0.035709   0.000135   0.017264
           0.016608   0.016114   0.012700   0.011725 [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 5.58e-07 8.84e-07 1.06e-06 2.45e-06 3.21e-06 4.95e-06   erg/cm2
              Error 7.58e-08 7.87e-08 1.31e-07 6.19e-07 3.16e-07 7.43e-07   erg/cm2
Peak flux Power-law 6.71e-01 2.77e-01 6.74e-02 2.00e-02 1.03e+00 1.03e+00   ph/cm2/s
              Error 2.99e-01 1.52e-01 8.30e-02 5.12e-02 4.14e-01 4.21e-01   ph/cm2/s
 
Fluence   Cutoff-PL 4.99e-07 1.01e-06 1.03e-06 5.14e-07 2.89e-06 3.05e-06   erg/cm2
              Error 8.60e-08 1.16e-07 1.67e-07 5.81e-07 3.73e-07 6.83e-07   erg/cm2
Peak flux Cutoff-PL 7.63e-01 1.83e-01 8.97e-05 1.13e-13 9.46e-01 9.45e-01   ph/cm2/s
              Error 3.50e-01 2.35e-01 6.29e-02 0.00e+00 3.94e-01 3.95e-01   ph/cm2/s
 
Fluence        Band 4.43e-07 1.08e-06 9.63e-07 1.39e-06 2.99e-06 3.88e-06   erg/cm2
              Error 9.59e-08 1.20e-07 1.51e-07 6.33e-07 3.28e-07 7.47e-07   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    1.744    0.148    -      -           1.21e-03 1.15e-04   65.930 57
CPL   0.642    0.840      53.6   17.1      5.01e-03 7.72e-03   58.700 56
 
The chi2 of BB fit is -------- which shows a significant improvement in the fit over a PL.
Check the BB fit.
 
=== 1-s peak spectral analysis ===
 
Model Ph_index Ph_90err Epeak  Epeak_90err Norm     Nomr_90err chi2   dof
PL    3.038    1.130    -      -           3.63e-03 3.13e-03   62.990 57
CPL   1.000    0.000      50.0    0.0      1.78e-02 0.00e+00   68.790 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: 101.504000 sec.
T50 in the 50-300 keV band: 43.520000 sec.

 
=== Table of the duration information ==
 
        Value   tstart    tstop
T100  287.000    4.000  291.000
T90   209.000    9.000  218.000
T50    74.000   26.000  100.000
Peak    1.000   18.000   19.000

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
  253.4476    34.1631   0.0147    38.7182   119.5005         3.7300498     13.042 TRIG_00631051                 
 
Foreground time interval of the image:
  4.000  72.901 (delta_t =  68.901 [sec])
Background time interval of the image:
-463.499 -447.733 (delta_t =  15.766 [sec])
-239.000   4.000 (delta_t = 243.000 [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 64.000000

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 64.000000

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 64.000000

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    4.000 sec. to  291.000 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.74370     ( -0.147091   0.149564 )
Norm@50keV  : 1.21036E-03    ( -0.000115319   0.000114355 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          65.93 using 59 PHA bins.
# Reduced chi-squared =          1.157 for     57 degrees of freedom 
# Null hypothesis probability =   1.954873e-01
 
Photon flux (15-150 keV)    in 287 sec: 0.163283 ( -0.0146667  0.0146852 ) ph/cm2/s
Energy fluence (15-150 keV)             : 3.20656e-06 ( -3.14239e-07  3.17212e-07 ) ergs/cm2

Cutoff power-law model

Time interval is from    4.000 sec. to  291.000 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 0.642495     ( -0.944664   0.734674 )
Epeak [keV] : 53.5753      ( -9.16207 25.106 )
Norm@50keV  : 5.01459E-03    ( -0.0030534   0.0123877 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          58.70 using 59 PHA bins.
# Reduced chi-squared =          1.048 for     56 degrees of freedom 
# Null hypothesis probability =   3.766434e-01
 
Photon flux (15-150 keV)    in 287 sec: 0.156917 ( -0.015306  0.015279 ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.89095e-06 ( -3.67983e-07  3.77835e-07 ) ergs/cm2

Band function

Time interval is from    4.000 sec. to  291.000 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : 4.45417   ( -4.54949   -4.45417 )
beta        : -2.22802    ( -0.298677   0.253806 )
Epeak [keV] : 32.0475      ( -3.23027 3.24272 )
Norm@50keV   : 16.1408    ( -1.39066   77.823 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          51.30 using 59 PHA bins.
# Reduced chi-squared =         0.9328 for     55 degrees of freedom 
# Null hypothesis probability =   6.166646e-01
 
Photon flux (15-150 keV)    in 287 sec:  (    ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.98842e-06 ( -2.98641e-06  -3.2689e-07 ) ergs/cm2

Single BB

 
Spectral model blackbody:
------------------------------------------------------------
Parameters  : value    Lower 90%  Upper 90%
kT [keV]    : 11.2763  (-1.03553  1.17564)
R^2/D10^2   : 5.11506E-02  (-0.0161309   0.022639)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          70.06 using 59 PHA bins.
# Reduced chi-squared =          1.229 for     57 degrees of freedom 
# Null hypothesis probability =   1.147005e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  3.918e-07   6.257e-08
25- 50  1.143e-06   1.279e-07
50-150  8.367e-07   1.739e-07
15-150  2.372e-06   2.483e-07

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 99.9206       (-23.8452      55.3762)
Norm        : 0.731458       (-0.0939969     0.0906947)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          60.64 using 59 PHA bins.
# Reduced chi-squared =          1.064 for     57 degrees of freedom 
# Null hypothesis probability =   3.461153e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  5.487e-07   7.677e-08
25- 50  9.486e-07   1.017e-07
50-150  1.537e-06   5.779e-07
15-150  3.034e-06   5.815e-07

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 8.73514        (-1.53554      1.50367)
R1^2/D10^2  : 0.108126        (-0.0383119      0.102542)
kT2 [keV]   : 34.1643        (-18.2471      -40.9684)
R2^2/D10^2  : 4.66123E-04    (-0.000250289   0.00146552)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          50.60 using 59 PHA bins.
# Reduced chi-squared =         0.9201 for     55 degrees of freedom 
# Null hypothesis probability =   6.431243e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  4.760e-07   1.456e-07
25- 50  1.065e-06   3.044e-07
50-150  1.449e-06   7.545e-07
15-150  2.990e-06   9.594e-07

Peak spectrum fit

Power-law model

Time interval is from   18.000 sec. to   19.000 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 3.03850     ( -0.941901   1.3188 )
Norm@50keV  : 3.63091E-03    ( -0.00269752   0.00357028 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          62.99 using 59 PHA bins.
# Reduced chi-squared =          1.105 for     57 degrees of freedom 
# Null hypothesis probability =   2.727227e-01
 
Photon flux (15-150 keV)    in 1 sec: 1.02699 ( -0.413108  0.415303 ) ph/cm2/s
Energy fluence (15-150 keV)             : 4.44143e-08 ( -2.09505e-08  2.54287e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from   18.000 sec. to   19.000 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.00000     (     )
Epeak [keV] : 50.0000      (   )
Norm@50keV  : 1.77842E-02    (     )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          68.79 using 59 PHA bins.
# Reduced chi-squared =          1.228 for     56 degrees of freedom 
# Null hypothesis probability =   1.171336e-01
 
Photon flux (15-150 keV)    in 1 sec: 0.946047 ( -0.366121  0.422623 ) ph/cm2/s
Energy fluence (15-150 keV)             : 3.21549e-08 ( -1.26798e-08  2.95824e-08 ) ergs/cm2

Band function

Time interval is from   18.000 sec. to   19.000 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : 4.93857   ( -4.93857   -4.93857 )
beta        : -4.86781    ( 4.86781   2.44285 )
Epeak [keV] : 19.8205      ( -19.8205 6.19999 )
Norm@50keV   : 7613.41    ( -2897.09   5.45116e+07 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          61.39 using 59 PHA bins.
# Reduced chi-squared =          1.116 for     55 degrees of freedom 
# Null hypothesis probability =   2.578139e-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]    : 4.79696  (-1.52181  2.39385)
R^2/D10^2   : 10.7929  (-10.7929   63.8485)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          61.82 using 59 PHA bins.
# Reduced chi-squared =          1.085 for     57 degrees of freedom 
# Null hypothesis probability =   3.080241e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  2.217e-08   1.374e-08
25- 50  1.305e-08   9.965e-09
50-150  4.325e-10   4.676e-10
15-150  3.566e-08   2.227e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 14.7593       (-7.63055      22.2277)
Norm        : 18.7513       (-18.7515     49.7012)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          62.35 using 59 PHA bins.
# Reduced chi-squared =          1.094 for     57 degrees of freedom 
# Null hypothesis probability =   2.918940e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  2.137e-08   1.365e-08
25- 50  1.434e-08   9.585e-09
50-150  2.445e-09   2.579e-09
15-150  3.816e-08   2.419e-08

Double BB

------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 197.839        (      )
R1^2/D10^2  : 1.04777E-04        (-9.80572e-05      0.00343254)
kT2 [keV]   : 4.65523        (-1.45987      1.5267)
R2^2/D10^2  : 12.1451    (-10.154   55.9558)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          61.81 using 59 PHA bins.
#Fit statistic : Chi-Squared =          58.73 using 59 PHA bins.
# Reduced chi-squared =          1.124 for     55 degrees of freedom 
# Reduced chi-squared =          1.068 for     55 degrees of freedom 
# Null hypothesis probability =   2.459907e-01
# Null hypothesis probability =   3.403439e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  2.214e-08   1.021e-07
25- 50  1.335e-08   2.284e-07
50-150  8.577e-10   7.050e-08
15-150  3.634e-08   2.921e-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: 1.58325     ( -0.193247   0.193898 )
Norm@50keV  : 3.26697E-03    ( -0.000385694   0.000384196 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          52.32 using 59 PHA bins.
# Reduced chi-squared =         0.9178 for     57 degrees of freedom 
# Null hypothesis probability =   6.511678e-01
 
Photon flux (15-150 keV)    in 68.9 sec: 0.417674 ( -0.0502589  0.0504287 ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.10952e-06 ( -2.62789e-07  2.64779e-07 ) ergs/cm2

Cutoff power-law model

Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 0.794562     ( -1.05795   0.827371 )
Epeak [keV] : 73.0216      ( -20.0469 -73.0266 )
Norm@50keV  : 8.47034E-03    ( -0.00527759   0.0219218 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          49.72 using 59 PHA bins.
# Reduced chi-squared =         0.8879 for     56 degrees of freedom 
# Null hypothesis probability =   7.099725e-01
 
Photon flux (15-150 keV)    in 68.9 sec: 0.405225 ( -0.052122  0.052168 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.98545e-06 ( -3.00259e-07  2.9893e-07 ) ergs/cm2

Band function

 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : 4.12486   ( -4.81004   -4.12485 )
beta        : -1.95891    ( -0.417676   0.320911 )
Epeak [keV] : 33.7623      ( -6.09536 18.7308 )
Norm@50keV   : 17.8945    ( -17.8827   12.994 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          45.50 using 59 PHA bins.
# Reduced chi-squared =         0.8273 for     55 degrees of freedom 
# Null hypothesis probability =   8.156433e-01
 
Photon flux (15-150 keV)    in 68.9 sec:  (    ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.00261e-06 ( -2.00213e-06  -2.71149e-07 ) ergs/cm2

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

S(25-50 keV)  = 8.84e-07
S(50-100 keV) = 1.06e-06

T90 vs. Hardness ratio plot

T90                                   = 209 sec.
Hardness ratio (energy fluence ratio) = 1.1991

Color vs. Color plot

Count Ratio  (25-50 keV) / (15-25 keV) = 1.63949
Count Ratio (50-100 keV) / (15-25 keV) = 0.804529

Mask shadow pattern

IMX = -3.947685319726116E-01, IMY = -6.977378766001685E-01

TIME vs. PHA plot around the trigger time

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 64.000000

TIME vs. DetID plot around the trigger time

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 64.000000

100 us light curve (15-350 keV)

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 64.000000

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:
-463.499400 -447.732900
-239.000000 4.000000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
244.9985 -15.6596    1.2  46.1   41.7   6.6532   9.3    1.6	Sco X-1                       
254.5092  35.3948    4.2  38.7  121.9   1.6944   2.8    4.0	Her X-1                       
256.0040 -37.8568    1.6  53.4   11.2   5.7547   7.0    1.1	4U 1700-377                   
256.3895 -36.4260    4.2  52.0   11.9   2.0749   2.8    2.2	GX 349+2                      
262.9827 -24.7640   63.9  39.3   15.1   0.0575   0.2    1.8	GX 1+4                        
264.7163 -44.3314    6.8  55.6    0.2   1.4953   1.7    7.2	4U 1735-44                    
268.3891  -1.4371    3.6  19.0   43.0   0.6562   3.1    1.6	SW J1753.5-0127               
270.3359 -25.0757    6.2  36.2    5.4   0.5417   1.8    2.8	GX 5-1                        
270.4063 -25.7213    3.7  36.7    4.9   0.9046   3.1    5.8	GRS 1758-258                  
274.0254 -14.1147    2.7  24.8    8.5   0.8568   4.2    4.8	GX 17+2                       
275.9629 -30.3661    3.6  39.5   -5.1   0.9138   3.2    2.0	H1820-303                     
284.9334 -24.8027    5.5  33.1  -17.4   0.5100   2.1    9.0	HT1900.1-2455                 
288.8097  10.9233    1.0   4.8 -141.1   2.2904  11.8    1.5	GRS 1915+105                  
299.5700  35.2050    1.2  30.2 -172.5   2.0818   9.6    1.0	Cyg X-1                       
308.1064  40.9546    3.9  38.7 -168.5   0.8608   3.0    0.2	Cyg X-3                       
326.2487  38.1812   56.7  47.8 -152.4  -0.0974  -0.2    9.2	Cyg X-2                       
262.9952 -33.8497    6.4  46.9    7.9   0.7607   1.8    1.0	GX 354-0                      
249.1237 -14.8876    2.6  42.2   39.8   2.1580   4.5 ------	UNKNOWN                       
305.5889  63.0902    2.4  56.9  174.0   6.2109   4.9 ------	UNKNOWN                       
277.3834 -23.7898    2.0  32.8   -4.6   1.3989   5.7 ------	UNKNOWN                       
283.5763 -49.4661    2.6  57.7  -16.2   3.9122   4.4 ------	UNKNOWN                       
	UNKNOWN                       
	UNKNOWN                       
	UNKNOWN

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

Time interval of the image:
4.000000 72.900600
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
245.0957 -15.7382    7.7  46.0   41.5  -0.5539  -1.5    8.9	Sco X-1                       
254.6260  35.4124    5.0  38.7  122.0  -0.6364  -2.3    9.2	Her X-1                       
255.9823 -37.9220   53.8  53.4   11.2  -0.0909  -0.2    4.7	4U 1700-377                   
256.5290 -36.5010    7.0  52.0   11.8   0.5969   1.6    6.5	GX 349+2                      
262.9829 -24.6609    4.4  39.2   15.2   0.4230   2.6    5.3	GX 1+4                        
264.8555 -44.4772    6.2  55.7    0.0   0.7913   1.8    5.1	4U 1735-44                    
268.5024  -1.5146   15.7  18.9   42.6   0.0776   0.7    8.9	SW J1753.5-0127               
270.4488 -25.0130    5.6  36.1    5.3  -0.2572  -2.0    9.8	GX 5-1                        
270.3404 -25.7637    9.4  36.8    4.9   0.1614   1.2    2.4	GRS 1758-258                  
274.0593 -14.0226   45.1  24.7    8.5   0.0253   0.3    3.2	GX 17+2                       
275.7478 -30.4457    6.4  39.7   -4.9   0.2429   1.8   10.3	H1820-303                     
284.9018 -25.0421    4.4  33.3  -17.3   0.3024   2.6   10.3	HT1900.1-2455                 
288.9249  10.8424    6.5   4.9 -139.6  -0.1568  -1.8    9.7	GRS 1915+105                  
299.7035  35.0819    5.4  30.1 -172.2  -0.2189  -2.1    9.1	Cyg X-1                       
308.2632  40.9206   11.1  38.8 -168.3  -0.1284  -1.0    7.2	Cyg X-3                       
326.1567  38.3361 2700.0  47.8 -152.7   0.0002   0.0    1.1	Cyg X-2                       
263.1532 -33.7332   11.1  46.7    7.8   0.2189   1.0   10.2	GX 354-0                      
253.4477  34.1630    0.9  38.7  119.5   3.7293  13.0 ------	UNKNOWN                       
264.0282 -32.5575    2.0  45.3    7.7   1.0528   5.7 ------	UNKNOWN

Post-slew image of 15-350 keV band

Time interval of the image:
132.500600 533.000590
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
244.9777 -15.6358    0.7  50.5   -9.3   8.9817  16.8    0.3	Sco X-1                       
254.4326  35.3264    1.2   1.4 -164.9   2.2631   9.8    1.6	Her X-1                       
268.2566  -1.4467    4.7  38.2  -44.3   0.9342   2.5    6.7	SW J1753.5-0127               
288.7086  10.8981    3.0  39.7  -82.5   3.4297   3.9    6.0	GRS 1915+105                  
299.5953  35.2279    1.5  37.6 -125.1   3.3514   8.0    1.6	Cyg X-1                       
308.1185  40.9590   14.2  43.2 -135.7   0.4182   0.8    0.5	Cyg X-3                       
224.8332  63.7427    2.5  34.4  138.1   1.7711   4.6 ------	UNKNOWN                       
262.9803  58.4323    3.3  25.1  171.9   0.9261   3.5 ------	UNKNOWN                       
255.6443 -13.1452    2.4  47.4  -22.8   2.2420   4.8 ------	UNKNOWN

Plot creation:
Thu May 28 13:26:46 EDT 2015