batgrbproduct analysis for trigger=421962

batgrbproduct Analysis for Trigger=421962

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 18:31:07 EST 2014
             Host Name: batevent1
   Current Working Dir: /local/data/batevent/batevent_reproc/trigger421962
======================================================================

  Trigger: 00421962      Segment: 000

  BAT Trigger Time: 295556043.968   [s; MET]
      Trigger Stop: 295556047.04   [s; MET]
               UTC: 2010-05-14T18:53:58.170320    [includes UTCF correction] 
       Where From?: TDRSS position message

  BAT 
    RA: 328.820890294865   Dec: 29.170486033985  [deg; J2000]

     Catalogged Source?: NO
     Point Source?:      YES
     GRB Indicated?:     YES    [ by BAT flight software ]
     Image S/N Ratio:    7.06
     Image Trigger?:     NO
     Rate S/N Ratio:     9.64365076099295  [ if not an image trigger ]
     Image S/N Ratio:    7.06

  Flight Position:   [ source = BAT ]
    RA: 328.820890294865   Dec: 29.170486033985  [deg; J2000]

  Ground Position:   [ source = BAT pre-slew burst ]
    RA: 328.76149612411   Dec: 29.1706248836181  [deg; J2000]  
        { 21h 55m 02.8s , +29d 10' 14.2" }
         +/- 2.38409317937589 [arcmin] (estimated 90% radius based on SNR)
         +/- 0.949646049234544 [arcmin] (formal 1-sigma fit error)
    SNR: 8.79194982687489
 
  Angular difference between Flight and Ground position is 3.111693 arcmin
 
  Partial Coding Fraction: 0.765625    [ including projection effects ]

  Duration
     T90: 23.0159999132156 +/- 6.614585413369
        Measured from: 2.24800002574921
                   to: 25.2639999389648     [s; relative to TRIGTIME]
     T50: 8.73599994182587 +/- 5.68785684938173
        Measured from: 3.75200003385544
                   to: 12.4879999756813     [s; relative to TRIGTIME]



  Fluence
     Peak Flux  (peak 1 second)
        Measured from: 6.20800000429153     
                   to: 7.20800000429153     [s; relative to TRIGTIME]
     Total Fluence        
        Measured from: 0.304000020027161     
                   to: 30.283999979496     [s; relative to TRIGTIME]
     
             Band 1     Band 2     Band 3     Band 4
              15-25      25-50     50-100    100-350     keV
 Total     0.236004   0.289097   0.172599   0.007115
           0.034181   0.034819   0.030661   0.026034 [error]
 Peak      0.025861   0.034656   0.016038   0.007236
           0.006291   0.006469   0.005722   0.004719 [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 8.71e-08 1.19e-07 1.21e-07 2.23e-07 3.99e-07 5.50e-07   erg/cm2
              Error 1.61e-08 1.64e-08 2.87e-08 1.03e-07 6.66e-08 1.36e-07   erg/cm2
Peak flux Power-law 2.77e-01 2.23e-01 1.22e-01 9.70e-02 6.65e-01 7.19e-01   ph/cm2/s
              Error 9.12e-02 5.25e-02 4.61e-02 7.08e-02 1.56e-01 1.73e-01   ph/cm2/s
 
Fluence   Cutoff-PL 7.94e-08 1.36e-07 1.16e-07 4.73e-08 3.64e-07 3.78e-07   erg/cm2
              Error 1.84e-08 2.30e-08 3.45e-08 1.05e-07 7.00e-08 1.25e-07   erg/cm2
Peak flux Cutoff-PL 2.56e-01 2.50e-01 1.18e-01 2.86e-02 6.46e-01 6.53e-01   ph/cm2/s
              Error 1.01e-01 7.57e-02 6.18e-02 -------- 1.60e-01 1.87e-01   ph/cm2/s
 
Fluence        Band -------- -------- -------- -------- -------- --------   erg/cm2
              Error -------- -------- -------- -------- -------- --------   erg/cm2
Peak flux      Band -------- -------- -------- -------- -------- --------   ph/cm2/s
              Error -------- -------- -------- -------- -------- --------   ph/cm2/s

 
=== Time-averaged spectral analysis ===
 
Model Ph_index Ph_90err Epeak  Epeak_90err Norm     Nomr_90err chi2   dof
PL    1.981    0.252    -      -           1.45e-03 2.51e-04   44.110 57
CPL   0.915    1.195      42.5   33.1      5.95e-03 1.84e-02   40.990 56
 
 
=== 1-s peak spectral analysis ===
 
Model Ph_index Ph_90err Epeak  Epeak_90err Norm     Nomr_90err chi2   dof
PL    1.876    0.431    -      -           4.68e-03 1.37e-03   50.120 57
CPL   0.932    2.371      46.2    0.0      1.68e-02 0.00e+00   49.310 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: 8.448000 sec.
T50 in the 50-300 keV band: 4.608000 sec.

 
=== Table of the duration information ==
 
        Value   tstart    tstop
T100   29.980    0.304   30.284
T90    23.016    2.248   25.264
T50     8.736    3.752   12.488
Peak    1.000    6.208    7.208

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
  328.7615    29.1706   0.0219    27.7743   -35.1405         0.7010708      8.792 TRIG_00421962                 
 
Foreground time interval of the image:
  0.304  30.284 (delta_t =  29.980 [sec])
Background time interval of the image:
-44.667   0.304 (delta_t =  44.971 [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 3.072000

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 3.072000

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 3.072000

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    0.304 sec. to   30.284 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.98122     ( -0.242065   0.261079 )
Norm@50keV  : 1.44507E-03    ( -0.000254833   0.000248075 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          44.11 using 59 PHA bins.
# Reduced chi-squared =         0.7738 for     57 degrees of freedom 
# Null hypothesis probability =   8.941584e-01
 
Photon flux (15-150 keV)    in 29.98 sec: 0.214909 ( -0.0290895  0.0290909 ) ph/cm2/s
Energy fluence (15-150 keV)             : 3.9916e-07 ( -6.56103e-08  6.7637e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from    0.304 sec. to   30.284 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 0.914635     ( -1.35453   1.03623 )
Epeak [keV] : 42.5082      ( -25.1186 40.9887 )
Norm@50keV  : 5.95164E-03    ( -0.0059515   0.0308757 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          40.99 using 59 PHA bins.
# Reduced chi-squared =         0.7320 for     56 degrees of freedom 
# Null hypothesis probability =   9.338111e-01
 
Photon flux (15-150 keV)    in 29.98 sec: 0.207656 ( -0.029694  0.029789 ) ph/cm2/s
Energy fluence (15-150 keV)             : 3.64494e-07 ( -6.66192e-08  7.3469e-08 ) ergs/cm2

Band function

Time interval is from    0.304 sec. to   30.284 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -0.916513   ( -0.641243   1.90914 )
beta        : -10.0000    ( 10   3.55271e-15 )
Epeak [keV] : 42.5136      ( -24.7923 40.922 )
Norm@50keV   : 5.93531E-03    ( -0.00593531   0.0309651 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          40.99 using 59 PHA bins.
# Reduced chi-squared =         0.7453 for     55 degrees of freedom 
# Null hypothesis probability =   9.199252e-01
 
Photon flux (15-150 keV)    in 29.98 sec: 0.209867 ( 6.79013  -0.032415 ) 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]    : 10.2546  (-1.50206  1.7622)
R^2/D10^2   : 9.31084E-02  (-0.0421113   0.0764138)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          48.21 using 59 PHA bins.
# Reduced chi-squared =         0.8458 for     57 degrees of freedom 
# Null hypothesis probability =   7.900431e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  6.027e-08   1.498e-08
25- 50  1.552e-07   2.764e-08
50-150  8.707e-08   3.167e-08
15-150  3.025e-07   5.441e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 66.5907       (-21.9335      41.2963)
Norm        : 1.08645       (-0.211224     0.262569)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          41.36 using 59 PHA bins.
# Reduced chi-squared =         0.7256 for     57 degrees of freedom 
# Null hypothesis probability =   9.407648e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  8.309e-08   1.550e-08
25- 50  1.304e-07   2.184e-08
50-150  1.613e-07   7.039e-08
15-150  3.747e-07   8.550e-08

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 4.73032        (-3.44715      3.55048)
R1^2/D10^2  : 0.937824        (-0.783967      2536.83)
kT2 [keV]   : 14.4767        (-4.09973      11.0935)
R2^2/D10^2  : 1.98049E-02    (-0.0183249   0.0633006)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          40.93 using 59 PHA bins.
# Reduced chi-squared =         0.7442 for     55 degrees of freedom 
# Null hypothesis probability =   9.209416e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  8.067e-08   4.449e-08
25- 50  1.316e-07   6.780e-08
50-150  1.422e-07   8.462e-08
15-150  3.544e-07   1.838e-07

Peak spectrum fit

Power-law model

Time interval is from    6.208 sec. to    7.208 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.87630     ( -0.407094   0.455029 )
Norm@50keV  : 4.68128E-03    ( -0.00139488   0.00133636 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          50.12 using 59 PHA bins.
# Reduced chi-squared =         0.8793 for     57 degrees of freedom 
# Null hypothesis probability =   7.286934e-01
 
Photon flux (15-150 keV)    in 1 sec: 0.665155 ( -0.156132  0.156133 ) ph/cm2/s
Energy fluence (15-150 keV)             : 4.30347e-08 ( -1.21846e-08  1.28061e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from    6.208 sec. to    7.208 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 0.932495     ( -3.5128   1.22916 )
Epeak [keV] : 46.2103      (   )
Norm@50keV  : 1.67826E-02    (     )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          49.31 using 59 PHA bins.
# Reduced chi-squared =         0.8805 for     56 degrees of freedom 
# Null hypothesis probability =   7.244005e-01
 
Photon flux (15-150 keV)    in 1 sec: 0.646058 ( -0.159535  0.159985 ) ph/cm2/s
Energy fluence (15-150 keV)             : 3.90141e-08 ( -1.29841e-08  1.47321e-08 ) ergs/cm2

Band function

Time interval is from    6.208 sec. to    7.208 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : 1.50133   ( 1.01978   2.20262 )
beta        : -2.52699    ( 8.50389   18.5039 )
Epeak [keV] : 34.2648      ( -46.9894 -46.9894 )
Norm@50keV   : 0.721372    ( -0.66524   82.9382 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          48.63 using 59 PHA bins.
# Reduced chi-squared =         0.8843 for     55 degrees of freedom 
# Null hypothesis probability =   7.149237e-01
 
Photon flux (15-150 keV)    in 1 sec:  (    ) ph/cm2/s
Energy fluence (15-150 keV)             : 3.93935e-08 ( 0  0 ) ergs/cm2

Single BB

 
Spectral model blackbody:
------------------------------------------------------------
Parameters  : value    Lower 90%  Upper 90%
kT [keV]    : 9.68891  (-2.22774  3.26557)
R^2/D10^2   : 0.361044  (-0.241742   0.616136)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          51.27 using 59 PHA bins.
# Reduced chi-squared =         0.8995 for     57 degrees of freedom 
# Null hypothesis probability =   6.888619e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  6.823e-09   3.383e-09
25- 50  1.621e-08   6.810e-09
50-150  7.716e-09   4.682e-09
15-150  3.075e-08   1.347e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 77.3940       (-39.6419      -77.394)
Norm        : 3.18911       (-0.928465     1.44156)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          49.40 using 59 PHA bins.
# Reduced chi-squared =         0.8667 for     57 degrees of freedom 
# Null hypothesis probability =   7.527024e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  8.256e-09   3.786e-09
25- 50  1.348e-08   5.846e-09
50-150  1.861e-08   1.556e-08
15-150  4.035e-08   2.614e-08

Double BB

------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 7.43647        (-7.11537      3.57628)
R1^2/D10^2  : 0.761086        (      )
kT2 [keV]   : 25.0525        (-24.6761      -24.6763)
R2^2/D10^2  : 5.60569E-03    (-0.00624548   0.350289)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          48.57 using 59 PHA bins.
#Fit statistic : Chi-Squared =          48.53 using 59 PHA bins.
# Reduced chi-squared =         0.8830 for     55 degrees of freedom 
# Reduced chi-squared =         0.8824 for     55 degrees of freedom 
# Null hypothesis probability =   7.173240e-01
# Null hypothesis probability =   7.184623e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  7.945e-09   4.854e-09
25- 50  1.444e-08   8.285e-09
50-150  1.800e-08   1.024e-08
15-150  4.038e-08   2.093e-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: 1.98122     ( -0.242065   0.261079 )
Norm@50keV  : 1.44507E-03    ( -0.000254833   0.000248075 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          44.11 using 59 PHA bins.
# Reduced chi-squared =         0.7738 for     57 degrees of freedom 
# Null hypothesis probability =   8.941584e-01
 
Photon flux (15-150 keV)    in 29.98 sec: 0.214909 ( -0.0290895  0.0290909 ) ph/cm2/s
Energy fluence (15-150 keV)             : 3.9916e-07 ( -6.56103e-08  6.7637e-08 ) ergs/cm2

Cutoff power-law model

Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 0.914635     ( -1.35453   1.03623 )
Epeak [keV] : 42.5082      ( -25.1186 40.9887 )
Norm@50keV  : 5.95164E-03    ( -0.0059515   0.0308757 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          40.99 using 59 PHA bins.
# Reduced chi-squared =         0.7320 for     56 degrees of freedom 
# Null hypothesis probability =   9.338111e-01
 
Photon flux (15-150 keV)    in 29.98 sec: 0.207656 ( -0.029694  0.029789 ) ph/cm2/s
Energy fluence (15-150 keV)             : 3.64494e-07 ( -6.66192e-08  7.3469e-08 ) ergs/cm2

Band function

 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -0.916512   ( -0.641247   3.48596 )
beta        : -10.0000    ( 10   1.77636e-15 )
Epeak [keV] : 42.5136      ( -24.9992 40.9369 )
Norm@50keV   : 5.93532E-03    ( -0.00593531   0.0309651 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          40.99 using 59 PHA bins.
# Reduced chi-squared =         0.7453 for     55 degrees of freedom 
# Null hypothesis probability =   9.199252e-01
 
Photon flux (15-150 keV)    in 29.98 sec: 0.209867 ( 6.79013  -0.032415 ) 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)  = 1.19e-07
S(50-100 keV) = 1.21e-07

T90 vs. Hardness ratio plot

T90                                   = 23.0159999132156 sec.
Hardness ratio (energy fluence ratio) = 1.01681

Color vs. Color plot

Count Ratio  (25-50 keV) / (15-25 keV) = 1.22497
Count Ratio (50-100 keV) / (15-25 keV) = 0.731339

Mask shadow pattern

IMX = 4.306790018847859E-01, IMY = 3.031407496949320E-01

TIME vs. PHA plot around the trigger time

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 3.072000

TIME vs. DetID plot around the trigger time

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 3.072000

100 us light curve (15-350 keV)

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 3.072000

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:
-44.667400 0.304000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
254.5689  35.1995    4.0  34.5  129.3   0.3698   2.9   10.2	Her X-1                       
288.8838  10.9817    5.4  32.4   54.0   0.2438   2.1    5.5	GRS 1915+105                  
299.5822  35.2001    0.5   7.2   28.4   1.6041  22.3    0.4	Cyg X-1                       
308.0353  40.9152    4.0   7.4  -45.5   0.2194   2.9    4.1	Cyg X-3                       
326.0786  38.4443   72.3  21.4  -52.3  -0.0119  -0.2    8.6	Cyg X-2                       
312.9026  -3.9205    2.6  48.1   16.8   0.8129   4.4 ------	UNKNOWN                       
344.2541  14.4666    2.8  48.2  -32.4   0.7153   4.2 ------	UNKNOWN

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

Time interval of the image:
0.304000 30.284000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
254.4896  35.2062    4.9  34.5  129.4  -0.3108  -2.3    8.3	Her X-1                       
288.8201  11.1245    6.3  32.3   54.1  -0.2198  -1.8   10.8	GRS 1915+105                  
299.6142  35.2450    5.6   7.2   28.1  -0.1417  -2.0    2.9	Cyg X-1                       
308.3789  40.8977    0.0   7.6  -45.9  -0.0431  -0.6   12.6	Cyg X-3                       
326.2245  38.4898    9.7  21.5  -52.6   0.0935   1.2   10.4	Cyg X-2                       
328.7614  29.1706    1.3  27.8  -35.1   0.7009   8.8 ------	UNKNOWN                       
246.1119  81.7751    2.3  43.0 -153.1   0.5883   5.0 ------	UNKNOWN                       
172.8428  79.6703    2.4  54.1 -153.9   1.1896   4.9 ------	UNKNOWN

Post-slew image of 15-350 keV band

Time interval of the image:
90.132610 962.106200
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
299.5835  35.2019    0.3  25.4  124.8  30.5739  43.8    0.3	Cyg X-1                       
308.0831  40.9854    2.2  20.6  144.1   3.3146   5.4    2.3	Cyg X-3                       
326.1159  38.4042    3.8   9.5 -179.4   1.6974   3.0    5.6	Cyg X-2                       
309.6194  -8.8503    2.6  42.3   42.4   6.2042   4.5 ------	UNKNOWN                       
359.3267  36.3645    3.1  26.5 -100.2   2.4990   3.7 ------	UNKNOWN                       
  0.8967  50.8821    3.4  32.3 -127.7   2.6788   3.4 ------	UNKNOWN                       
 18.9773  41.3452    3.2  42.1 -107.2  10.4706   3.6 ------	UNKNOWN

Plot creation:
Sun May 31 01:34:01 EDT 2015