batgrbproduct analysis for trigger=661036

batgrbproduct Analysis for Trigger=661036

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): Mon Nov 16 01:24:01 EST 2015
             Host Name: bat1
   Current Working Dir: /local/data/bat1/alien/Swift_3rdBATcatalog/event/batevent_reproc/trigger661036
======================================================================

  Trigger: 00661036      Segment: 000

  BAT Trigger Time: 467215607.424   [s; MET]
      Trigger Stop: 467215615.616   [s; MET]
               UTC: 2015-10-22T14:06:32.116140    [includes UTCF correction] 
       Where From?: TDRSS position message

  BAT 
    RA: 349.212869430113   Dec: 55.813346849863  [deg; J2000]

     Catalogged Source?: NO
     Point Source?:      YES
     GRB Indicated?:     YES    [ by BAT flight software ]
     Image S/N Ratio:    7.24
     Image Trigger?:     NO
     Rate S/N Ratio:     10.0995049383621  [ if not an image trigger ]
     Image S/N Ratio:    7.24

  Flight Position:   [ source = BAT ]
    RA: 349.212869430113   Dec: 55.813346849863  [deg; J2000]

  Ground Position:   [ source = BAT pre-slew burst ]
    RA: 349.232463026896   Dec: 55.8126592306048  [deg; J2000]  
        { 23h 16m 55.8s , +55d 48' 45.6" }
         +/- 2.26827853983666 [arcmin] (estimated 90% radius based on SNR)
         +/- 0.966884123925847 [arcmin] (formal 1-sigma fit error)
    SNR: 9.44018898554026
 
  Angular difference between Flight and Ground position is 0.661861 arcmin
 
  Partial Coding Fraction: 0.3515625    [ including projection effects ]

  Duration
     T90: 117.680000007153 +/- 18.7778933407152
        Measured from: 2.60799998044968
                   to: 120.287999987602     [s; relative to TRIGTIME]
     T50: 67.0720000267029 +/- 23.3560215804344
        Measured from: 10.8159999847412
                   to: 77.8880000114441     [s; relative to TRIGTIME]



  Fluence
     Peak Flux  (peak 1 second)
        Measured from: 10.3719999790192     
                   to: 11.3719999790192     [s; relative to TRIGTIME]
     Total Fluence        
        Measured from: -1.04000002145767     
                   to: 132.847999989986     [s; relative to TRIGTIME]
     
             Band 1     Band 2     Band 3     Band 4
              15-25      25-50     50-100    100-350     keV
 Total     0.674476   0.887534   0.369326   0.170550
           0.104838   0.106113   0.091351   0.081571 [error]
 Peak      0.024354   0.031148   0.027473   0.017126
           0.009438   0.009523   0.008000   0.007405 [error]

     [ fluence units of on-axis counts / fully illuminated detector ] 

======================================================================
 
=== Fluence/Peak Flux Summary ===
 
              Model    Band1    Band2    Band3    Band4    Band5    Total      
                       15-25    25-50   50-100  100-350   15-150   15-350   keV
Fluence   Power-law 2.38e-07 3.45e-07 3.72e-07 7.48e-07 1.19e-06 1.70e-06   erg/cm2
              Error 5.04e-08 5.03e-08 9.03e-08 3.65e-07 2.09e-07 4.60e-07   erg/cm2
Peak flux Power-law 2.17e-01 2.31e-01 1.76e-01 2.17e-01 7.06e-01 8.40e-01   ph/cm2/s
              Error 1.21e-01 8.21e-02 6.43e-02 1.68e-01 2.30e-01 2.64e-01   ph/cm2/s
 
Fluence   Cutoff-PL 2.35e-07 3.56e-07 3.68e-07 4.62e-07 1.15e-06 1.41e-06   erg/cm2
              Error 5.44e-08 6.94e-08 1.06e-07 4.39e-07 2.54e-07 6.38e-07   erg/cm2
Peak flux Cutoff-PL 1.92e-01 2.46e-01 1.86e-01 1.11e-01 6.90e-01 7.35e-01   ph/cm2/s
              Error 1.41e-01 1.01e-01 7.58e-02 1.12e-01 2.38e-01 3.13e-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    1.892    0.273    -      -           9.64e-04 1.71e-04   51.890 57
CPL   1.650    1.100      59.7    0.0      1.34e-03 0.00e+00   51.780 56
 
 
=== 1-s peak spectral analysis ===
 
Model Ph_index Ph_90err Epeak  Epeak_90err Norm     Nomr_90err chi2   dof
PL    1.399    0.546    -      -           5.80e-03 1.81e-03   62.630 57
CPL   0.746    2.799      98.2    0.0      1.23e-02 5.99e-01   62.390 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: 7.808000 sec.
T50 in the 50-300 keV band: 4.288000 sec.

 
=== Table of the duration information ==
 
        Value   tstart    tstop
T100  133.888   -1.040  132.848
T90   117.680    2.608  120.288
T50    67.072   10.816   77.888
Peak    1.000   10.372   11.372

Click here for the BAT GCN circular template

Image

Pre-slew 15.0-350.0 keV image (Event data)

#   RAcent    DECcent   POSerr    Theta     Phi              Peak Cts       SNR   Name
  349.2325    55.8127   0.0204    31.8397    57.1278         2.2593152      9.440 TRIG_00661036                 
 
Foreground time interval of the image:
 -1.040 132.848 (delta_t = 133.888 [sec])
Background time interval of the image:
-501.323 -484.563 (delta_t =  16.761 [sec])
-239.424  -1.040 (delta_t = 238.384 [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 8.192000

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 8.192000

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 8.192000

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   -1.040 sec. to  132.848 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.89181     ( -0.264442   0.280793 )
Norm@50keV  : 9.64012E-04    ( -0.000173639   0.000168312 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          51.89 using 59 PHA bins.
# Reduced chi-squared =         0.9103 for     57 degrees of freedom 
# Null hypothesis probability =   6.667102e-01
 
Photon flux (15-150 keV)    in 133.9 sec: 0.137868 ( -0.0201217  0.0201274 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.18667e-06 ( -2.06098e-07  2.11737e-07 ) ergs/cm2

Cutoff power-law model

Time interval is from   -1.040 sec. to  132.848 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.65039     ( -1.63916   0.561122 )
Epeak [keV] : 59.7454      (   )
Norm@50keV  : 1.33585E-03    (     )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          51.78 using 59 PHA bins.
# Reduced chi-squared =         0.9247 for     56 degrees of freedom 
# Null hypothesis probability =   6.352202e-01
 
Photon flux (15-150 keV)    in 133.9 sec: 0.136635 ( -0.021221  0.020907 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.15274e-06 ( -2.67185e-07  2.40438e-07 ) ergs/cm2

Band function

Time interval is from   -1.040 sec. to  132.848 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : 0.783802   ( -2.57577   -2.57577 )
beta        : -2.11176    ( 2.11996   0.421418 )
Epeak [keV] : 29.5050      ( -27.0962 80.8365 )
Norm@50keV   : 7.27174E-02    ( -0.0729247   49.9781 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          50.73 using 59 PHA bins.
# Reduced chi-squared =         0.9224 for     55 degrees of freedom 
# Null hypothesis probability =   6.383094e-01
 
Photon flux (15-150 keV)    in 133.9 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]    : 9.77927  (-1.50134  1.83053)
R^2/D10^2   : 7.06940E-02  (-0.0341811   0.0631961)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          59.07 using 59 PHA bins.
# Reduced chi-squared =          1.036 for     57 degrees of freedom 
# Null hypothesis probability =   3.997489e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.829e-07   4.646e-08
25- 50  4.405e-07   9.614e-08
50-150  2.154e-07   9.814e-08
15-150  8.388e-07   1.742e-07

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 77.2988       (-29.9229      71.663)
Norm        : 0.655073       (-0.129454     0.179582)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          51.92 using 59 PHA bins.
# Reduced chi-squared =         0.9109 for     57 degrees of freedom 
# Null hypothesis probability =   6.655460e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  2.271e-07   4.419e-08
25- 50  3.707e-07   6.929e-08
50-150  5.111e-07   2.953e-07
15-150  1.109e-06   3.093e-07

Double BB

------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 8.45002        (-2.11992      1.75081)
R1^2/D10^2  : 0.113981        (-0.0613725      0.186025)
kT2 [keV]   : 199.443        (-199.443      -199.443)
R2^2/D10^2  : 1.32085E-05    (-6.86033e-06   0.0025971)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          49.35 using 59 PHA bins.
#Fit statistic : Chi-Squared =          49.20 using 59 PHA bins.
# Reduced chi-squared =         0.8973 for     55 degrees of freedom 
# Reduced chi-squared =         0.8945 for     55 degrees of freedom 
# Null hypothesis probability =   6.893119e-01
# Null hypothesis probability =   6.948296e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  2.116e-07   9.440e-08
25- 50  4.028e-07   1.444e-07
50-150  5.741e-07   3.248e-07
15-150  1.189e-06   4.563e-07

Peak spectrum fit

Power-law model

Time interval is from   10.372 sec. to   11.372 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.39905     ( -0.555454   0.535599 )
Norm@50keV  : 5.79697E-03    ( -0.00180806   0.00180682 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          62.63 using 59 PHA bins.
# Reduced chi-squared =          1.099 for     57 degrees of freedom 
# Null hypothesis probability =   2.834475e-01
 
Photon flux (15-150 keV)    in 1 sec: 0.705810 ( -0.228678  0.230472 ) ph/cm2/s
Energy fluence (15-150 keV)             : 5.60251e-08 ( -1.86415e-08  1.89476e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from   10.372 sec. to   11.372 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 0.745871     ( -4.0009   1.59797 )
Epeak [keV] : 98.2085      ( -98.1845 -98.1845 )
Norm@50keV  : 1.22704E-02    ( -0.012275   1.18588 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          62.39 using 59 PHA bins.
# Reduced chi-squared =          1.114 for     56 degrees of freedom 
# Null hypothesis probability =   2.594450e-01
 
Photon flux (15-150 keV)    in 1 sec: 0.689515 ( -0.238715  0.237354 ) ph/cm2/s
Energy fluence (15-150 keV)             : 5.38217e-08 ( -2.03403e-08  2.03406e-08 ) ergs/cm2

Band function

Time interval is from   10.372 sec. to   11.372 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : 0.169158   ( 0.601292   0.601292 )
beta        : -1.83702    ( 1.66356   0.778789 )
Epeak [keV] : 60.6986      ( -60.2022 213.258 )
Norm@50keV   : 4.08975E-02    ( -0.0423329   600373 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          62.17 using 59 PHA bins.
# Reduced chi-squared =          1.130 for     55 degrees of freedom 
# Null hypothesis probability =   2.360331e-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]    : 15.6845  (-4.70073  8.30737)
R^2/D10^2   : 7.21962E-02  (-0.0718789   0.182505)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          63.71 using 59 PHA bins.
# Reduced chi-squared =          1.118 for     57 degrees of freedom 
# Null hypothesis probability =   2.521814e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  3.688e-09   2.388e-09
25- 50  1.525e-08   9.730e-09
50-150  2.602e-08   1.733e-08
15-150  4.496e-08   2.779e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 199.363       (-126.427      -199.363)
Norm        : 2.95100       (-0.919745     0.919955)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          62.72 using 59 PHA bins.
# Reduced chi-squared =          1.100 for     57 degrees of freedom 
# Null hypothesis probability =   2.807021e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  7.348e-09   4.520e-09
25- 50  1.414e-08   8.535e-09
50-150  3.100e-08   1.944e-08
15-150  5.249e-08   3.219e-08

Double BB

R1^2/D10^2  : 8.84926E-04        (-0.000874986      0.165003)
kT2 [keV]   : 11.2468        (-11.2576      9.08901)
R2^2/D10^2  : 0.178961    (-0.178544   -0.178544)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          62.85 using 59 PHA bins.
#Fit statistic : Chi-Squared =          62.29 using 59 PHA bins.
#Fit statistic : Chi-Squared =          62.17 using 59 PHA bins.
# Reduced chi-squared =          1.143 for     55 degrees of freedom 
# Reduced chi-squared =          1.133 for     55 degrees of freedom 
# Reduced chi-squared =          1.130 for     55 degrees of freedom 
# Null hypothesis probability =   2.181054e-01
# Null hypothesis probability =   2.327459e-01
# Null hypothesis probability =   2.361013e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  5.773e-09   2.742e-09
25- 50  1.355e-08   8.280e-09
50-150  2.866e-08   1.777e-08
15-150  4.799e-08   2.909e-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: 1.89181     ( -0.264442   0.280793 )
Norm@50keV  : 9.64012E-04    ( -0.000173639   0.000168312 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          51.89 using 59 PHA bins.
# Reduced chi-squared =         0.9103 for     57 degrees of freedom 
# Null hypothesis probability =   6.667102e-01
 
Photon flux (15-150 keV)    in 133.9 sec: 0.137868 ( -0.0201217  0.0201274 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.18667e-06 ( -2.06098e-07  2.11737e-07 ) ergs/cm2

Cutoff power-law model

Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.65039     ( -1.63916   0.561158 )
Epeak [keV] : 59.7454      (   )
Norm@50keV  : 1.33585E-03    (     )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          51.78 using 59 PHA bins.
# Reduced chi-squared =         0.9247 for     56 degrees of freedom 
# Null hypothesis probability =   6.352202e-01
 
Photon flux (15-150 keV)    in 133.9 sec: 0.136635 ( -0.021221  0.020907 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.15274e-06 ( -2.67185e-07  2.40438e-07 ) ergs/cm2

Band function

 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : 0.783802   ( -2.57577   -2.57577 )
beta        : -2.11176    ( 2.11996   0.421418 )
Epeak [keV] : 29.5050      ( -27.0962 80.9917 )
Norm@50keV   : 7.27174E-02    ( -0.0729247   49.9674 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          50.73 using 59 PHA bins.
# Reduced chi-squared =         0.9224 for     55 degrees of freedom 
# Null hypothesis probability =   6.383094e-01
 
Photon flux (15-150 keV)    in 133.9 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)  = 3.45e-07
S(50-100 keV) = 3.72e-07

T90 vs. Hardness ratio plot

T90                                   = 117.680000007153 sec.
Hardness ratio (energy fluence ratio) = 1.07826

Color vs. Color plot

Count Ratio  (25-50 keV) / (15-25 keV) = 1.31589
Count Ratio (50-100 keV) / (15-25 keV) = 0.547575

Mask shadow pattern

IMX = 3.370504102847328E-01, IMY = -5.215546828021406E-01

TIME vs. PHA plot around the trigger time

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 8.192000

TIME vs. DetID plot around the trigger time

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 8.192000

100 us light curve (15-350 keV)

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 8.192000

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:
-501.323400 -484.562600
-239.424000 -1.040000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
254.3987  35.1506    0.0  36.9  -82.8  -0.7345  -1.3   11.9	Her X-1                       
288.8733  10.9802    5.1  35.2 -152.8   0.5992   2.2    4.9	GRS 1915+105                  
299.5960  35.2141    0.6   9.4 -164.9   4.0395  18.6    0.8	Cyg X-1                       
308.1293  40.9624    1.1   6.0  128.9   2.3136  10.9    1.0	Cyg X-3                       
326.1451  38.3392   15.6  19.3  105.1   0.1798   0.7    1.6	Cyg X-2                       
  0.6585  65.8287    1.9  37.9   40.1   2.5882   6.1 ------	UNKNOWN                       
342.1291  63.0899    2.3  29.5   41.8   1.4065   5.0 ------	UNKNOWN                       
278.4687  29.8740    2.1  23.3 -115.7   1.3599   5.4 ------	UNKNOWN                       
225.8886  64.5838    3.2  44.9  -30.9   1.5125   3.6 ------	UNKNOWN                       
266.4793  12.6423    3.0  43.7 -120.5   3.4121   3.9 ------	UNKNOWN                       
221.1093  53.1930    2.9  50.8  -44.5   4.6755   4.0 ------	UNKNOWN                       
269.1993   5.6699    2.8  48.0 -129.0   4.0969   4.1 ------	UNKNOWN

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

Time interval of the image:
-1.040000 132.848000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
254.6764  35.3484   13.7  36.6  -82.6  -0.2838  -0.8   10.7	Her X-1                       
288.6962  10.9138    3.9  35.3 -152.6   0.5334   3.0    6.3	GRS 1915+105                  
299.6686  35.3063    4.0   9.3 -165.1  -0.4007  -2.9    7.4	Cyg X-1                       
308.0591  41.1015    6.7   5.8  128.2  -0.2422  -1.7    9.2	Cyg X-3                       
325.9965  38.3941   14.6  19.2  105.1  -0.1360  -0.8    9.3	Cyg X-2                       
349.2306  55.8138    1.2  31.8   57.1   2.2540   9.4 ------	UNKNOWN                       
319.7270  15.2546    2.6  33.0  151.7   0.8418   4.4 ------	UNKNOWN                       
296.8492  57.0517    2.3  12.9   -6.4   0.6882   5.0 ------	UNKNOWN                       
285.2039  -2.1567    2.9  48.9 -152.9   1.2449   4.0 ------	UNKNOWN

Post-slew image of 15-350 keV band

Time interval of the image:
284.276600 962.627900
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
299.6003  35.1896    0.8  39.3 -142.0   9.5773  13.8    0.9	Cyg X-1                       
308.1180  40.9514    0.9  30.5 -143.3   6.3749  12.6    0.4	Cyg X-3                       
326.1701  38.3156    3.5  23.3 -170.7   1.3185   3.2    0.4	Cyg X-2                       
 60.6619  40.5666    3.7  47.6   35.5   6.1074   3.1 ------	UNKNOWN                       
 19.6384  63.7513    0.6  17.0    8.3   8.8624  20.5 ------	UNKNOWN                       
273.4283  62.1386    3.3  37.3  -90.1   4.8526   3.5 ------	UNKNOWN                       
284.3712  34.9256    3.0  48.0 -129.1   7.6671   3.8 ------	UNKNOWN

Plot creation:
Mon Nov 16 15:48:38 EST 2015