batgrbproduct analysis for trigger=686761

batgrbproduct Analysis for Trigger=686761

Analysis Summary

Notes:

1) No attempt has been made to eliminate the non-significant decimal places.
2) This batgrbproduct analysis is done of the amount of data for this trigger downloaded to date.
3) This batgrbproduct analysis is using the flight position for the mask-weighting calculation.
4) This page will be updated for up to 10 downlinks after the trigger.

======================================================================
                  BAT GRB EVENT DATA PROCESSING REPORT
    Process Script Ver: batgrbproduct v2.46
    Process Start Time (local time): Thu May 19 12:16:32 EDT 2016
             Host Name: bat1
   Current Working Dir: /local/data/bat1/prebascript/trigger686761/GCN5_download_cron
======================================================================

  Trigger: 00686761      Segment: 000

  BAT Trigger Time: 485255380.244   [s; MET]
      Trigger Stop: 485255380.26   [s; MET]
               UTC: 2016-05-18T09:09:23.958660    [includes UTCF correction] 
       Where From?: (*SHORT BURST*) TDRSS scaled map message

  BAT 
    RA: 293.722461595314   Dec: 21.8910956484575  [deg; J2000]

     Catalogged Source?: YES
     Point Source?:      YES
     GRB Indicated?:     NO    [ by BAT flight software ]
     Image S/N Ratio:    24.16
     Image Trigger?:     NO
     Rate S/N Ratio:     255.998046867549  [ if not an image trigger ]
     Image S/N Ratio:    24.16

  Flight Position:   [ source = BAT ]
    RA: 293.722461595314   Dec: 21.8910956484575  [deg; J2000]

  Ground Position:   [ source = BAT pre-slew burst ]
    RA: 293.72753769189   Dec: 21.8914024205546  [deg; J2000]  
        { 19h 34m 54.6s , +21d 53' 29.0" }
         +/- 0.455095527860558 [arcmin] (estimated 90% radius based on SNR)
         +/- 0.148013191766966 [arcmin] (formal 1-sigma fit error)
    SNR: 93.657655736819
 
  Angular difference between Flight and Ground position is 0.283203 arcmin
 
  Partial Coding Fraction: 0.984375    [ including projection effects ]

  Duration
     T90: 0.12799996137619 +/- 0.004
        Measured from: -0.0479999184608459
                   to: 0.0800000429153442     [s; relative to TRIGTIME]
     T50: 0.0679999589920044 +/- 0.004
        Measured from: -0.0199999213218689
                   to: 0.0480000376701355     [s; relative to TRIGTIME]



  Fluence
     Peak Flux  (peak 1 second)
        Measured from: -0.486000001430511     
                   to: 0.513999998569489     [s; relative to TRIGTIME]
     Total Fluence        
        Measured from: -0.0720000267028809     
                   to: 0.0959999561309814     [s; relative to TRIGTIME]
     
             Band 1     Band 2     Band 3     Band 4
              15-25      25-50     50-100    100-350     keV
 Total     2.032181   2.162640   0.445415   0.008820
           0.021684   0.022189   0.010383   0.002215 [error]
 Peak      2.033533   2.166442   0.449657   0.007714
           0.022385   0.022852   0.011460   0.004706 [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 9.98e-07 6.48e-07 2.72e-07 1.57e-07 2.00e-06 2.07e-06   erg/cm2
              Error -------- -------- -------- -------- -------- --------   erg/cm2
Peak flux Power-law 3.09e+01 1.30e+01 3.24e+00 9.88e-01 4.77e+01 4.81e+01   ph/cm2/s
              Error -------- -------- -------- -------- -------- --------   ph/cm2/s
 
Fluence   Cutoff-PL 6.00e-07 8.97e-07 3.29e-07 1.59e-08 1.84e-06 1.84e-06   erg/cm2
              Error 3.55e-08 2.15e-08 1.27e-08 2.98e-09 4.78e-08 4.79e-08   erg/cm2
Peak flux Cutoff-PL 1.94e+01 1.64e+01 3.33e+00 9.45e-02 3.93e+01 3.93e+01   ph/cm2/s
              Error 1.23e+00 4.09e-01 1.35e-01 2.07e-02 1.39e+00 1.39e+00   ph/cm2/s
 
Fluence        Band -------- -------- -------- -------- -------- --------   erg/cm2
              Error -------- -------- -------- -------- -------- --------   erg/cm2
Peak flux      Band -------- -------- -------- -------- -------- --------   ph/cm2/s
              Error -------- -------- -------- -------- -------- --------   ph/cm2/s

 
=== Time-averaged spectral analysis ===
 
Model Ph_index Ph_90err Epeak  Epeak_90err Norm     Nomr_90err chi2   dof
PL    3.249    0.000    -      -           8.73e-01 0.00e+00 1114.720 57
CPL  -0.242    0.260      29.5    1.2      6.42e+01 2.11e+01   60.120 56
 
The chi2 of BB fit is 130.78 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    3.005    0.000    -      -           1.73e-01 0.00e+00  682.570 57
CPL  -0.165    0.290      29.4    1.3      9.71e+00 3.66e+00   59.990 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: 0.128000 sec.
T50 in the 50-300 keV band: 0.064000 sec.

 
=== Table of the duration information ==
 
        Value   tstart    tstop
T100    0.168   -0.072    0.096
T90     0.128   -0.048    0.080
T50     0.068   -0.020    0.048
Peak    1.000   -0.486    0.514

Click here for the BAT GCN circular template

Estimated redshift from machine learning (Ukwatta et al. 2016) - may take a few minutes to calcaulte

Image

Pre-slew 15-350 keV image (Event data; bkg subtracted)

#   RAcent  DECcent POSerr  Theta    Phi     Peak Cts     SNR  Name
  293.7275 +21.8914 0.0021   12.0 -120.5       4.7825    93.7  TRIG_00686761       
------------------------------------------
 
Foreground time interval of the image:
 -0.072   0.096 (delta_t =   0.168 [sec])
Background time interval of the image:
-239.244  -0.072 (delta_t = 239.172 [sec])

Lightcurves

Notes:

1) All plots contain as much data as has been downloaded to date.
2) The mask-weighted light curves are using the flight position.
3) Multiple plots of different time binning/intervals are shown to cover all scenarios of short/long GRBs, rate/image triggers, and real/false positives.
4) 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.
5) 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.
6) 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 0.016000

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 0.016000

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 0.016000

SN=5 or 10 sec. binning (whichever binning is satisfied first)

SN=5 or 10 sec. binning (T < 200 sec)

Spectra

Notes:

1) The fitting includes the systematic errors.
2) For long bursts, a spectral fit of 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.
4) For short bursts (T90<1sec), the specrtum is also fit with Blackbody, OTTB, and Double Blackbody.

Time averaged spectrum fit using the pre-slew DRM

Power-law model

Time interval is from   -0.072 sec. to    0.096 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 3.24866     (     )
Norm@50keV  : 0.873192    (     )
------------------------------------------------------------
#Fit statistic : Chi-Squared =        1114.72 using 59 PHA bins.
# Reduced chi-squared =        19.5565 for     57 degrees of freedom 
# Null hypothesis probability =  5.298077e-196
 
Photon flux (15-150 keV)    in 0.168 sec: 289.424 (    ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.99656e-06 ( 0  0 ) ergs/cm2

Cutoff power-law model

Time interval is from   -0.072 sec. to    0.096 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: -0.241560     ( -0.266435   0.253222 )
Epeak [keV] : 29.5420      ( -1.28799 1.1803 )
Norm@50keV  : 64.2241    ( -17.1506   24.9553 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          60.12 using 59 PHA bins.
# Reduced chi-squared =          1.074 for     56 degrees of freedom 
# Null hypothesis probability =   3.290575e-01
 
Photon flux (15-150 keV)    in 0.168 sec: 232.329 ( -8.019  8.103 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.84187e-06 ( 0  0 ) ergs/cm2

Band function

Time interval is from   -0.072 sec. to    0.096 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : 0.237143   ( -0.239013   0.281906 )
beta        : -10.0000    ( 10   10 )
Epeak [keV] : 29.5151      ( -1.2685 1.20242 )
Norm@50keV   : 63.9143    ( -16.7599   25.5357 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          60.12 using 59 PHA bins.
# Reduced chi-squared =          1.093 for     55 degrees of freedom 
# Null hypothesis probability =   2.955675e-01
 
Photon flux (15-150 keV)    in 0.168 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]    : 8.65223  (  )
R^2/D10^2   : 194.090  (   )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =         130.78 using 59 PHA bins.
# Reduced chi-squared =         2.2943 for     57 degrees of freedom 
# Null hypothesis probability =   9.984940e-08
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  4.650e-07   1.806e-08
25- 50  9.283e-07   2.134e-08
50-150  3.134e-07   1.294e-08
15-150  1.707e-06   3.830e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 25.3858       (      )
Norm        : 2583.22       (     )
------------------------------------------------------------
#Fit statistic : Chi-Squared =         205.77 using 59 PHA bins.
# Reduced chi-squared =         3.6101 for     57 degrees of freedom 
# Null hypothesis probability =   1.074447e-18
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  8.027e-07   2.495e-08
25- 50  8.308e-07   1.831e-08
50-150  3.613e-07   1.386e-08
15-150  1.995e-06   4.368e-08

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 6.09721        (-0.852644      0.812092)
R1^2/D10^2  : 477.039        (-127.055      255.022)
kT2 [keV]   : 10.6720        (-0.75452      1.18042)
R2^2/D10^2  : 44.7650    (-25.4812   32.9941)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          57.95 using 59 PHA bins.
# Reduced chi-squared =          1.054 for     55 degrees of freedom 
# Null hypothesis probability =   3.670847e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  5.828e-07   5.947e-08
25- 50  9.013e-07   7.896e-08
50-150  3.444e-07   4.964e-08
15-150  1.829e-06   1.695e-07

Peak spectrum fit

Power-law model

Time interval is from   -0.486 sec. to    0.514 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 3.00450     (     )
Norm@50keV  : 0.172940    (     )
------------------------------------------------------------
#Fit statistic : Chi-Squared =         682.57 using 59 PHA bins.
# Reduced chi-squared =         11.975 for     57 degrees of freedom 
# Null hypothesis probability =  5.262400e-108
 
Photon flux (15-150 keV)    in 1 sec: 47.7171 (    ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.08222e-06 ( 0  0 ) ergs/cm2

Cutoff power-law model

Time interval is from   -0.486 sec. to    0.514 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: -0.165448     ( -0.296652   0.282391 )
Epeak [keV] : 29.3748      ( -1.40573 1.25808 )
Norm@50keV  : 9.71383    ( -2.9075   4.41524 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          59.99 using 59 PHA bins.
# Reduced chi-squared =          1.071 for     56 degrees of freedom 
# Null hypothesis probability =   3.330984e-01
 
Photon flux (15-150 keV)    in 1 sec: 39.2562 ( -1.3826  1.3971 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.85301e-06 ( 0  0 ) ergs/cm2

Band function

Time interval is from   -0.486 sec. to    0.514 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : 0.434609   ( -0.420301   0.329406 )
beta        : -5.41709    ( -1.05985   0.452095 )
Epeak [keV] : 30.0230      ( -1.46127 0.901632 )
Norm@50keV   : 13.9860    ( -5.07049   7.74099 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          55.75 using 59 PHA bins.
# Reduced chi-squared =          1.014 for     55 degrees of freedom 
# Null hypothesis probability =   4.462507e-01
 
Photon flux (15-150 keV)    in 1 sec:  (    ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.85418e-06 ( 0  0 ) ergs/cm2

Single BB

 
Spectral model blackbody:
------------------------------------------------------------
Parameters  : value    Lower 90%  Upper 90%
kT [keV]    : 8.58626  (  )
R^2/D10^2   : 33.8319  (   )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =         123.70 using 59 PHA bins.
# Reduced chi-squared =         2.1702 for     57 degrees of freedom 
# Null hypothesis probability =   7.735324e-07
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  4.730e-07   1.920e-08
25- 50  9.325e-07   2.185e-08
50-150  3.074e-07   1.350e-08
15-150  1.713e-06   3.950e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 26.9234       (      )
Norm        : 404.330       (     )
------------------------------------------------------------
#Fit statistic : Chi-Squared =         159.37 using 59 PHA bins.
# Reduced chi-squared =         2.7960 for     57 degrees of freedom 
# Null hypothesis probability =   1.264511e-11
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  7.753e-07   2.735e-08
25- 50  8.322e-07   2.005e-08
50-150  3.935e-07   1.690e-08
15-150  2.001e-06   4.250e-08

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 6.46117        (-0.98398      0.849981)
R1^2/D10^2  : 73.5394        (-18.4371      37.6015)
kT2 [keV]   : 11.4407        (-1.28458      2.52588)
R2^2/D10^2  : 4.63522    (-3.52225   6.47288)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          56.76 using 59 PHA bins.
# Reduced chi-squared =          1.032 for     55 degrees of freedom 
# Null hypothesis probability =   4.093440e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  5.780e-07   5.575e-08
25- 50  9.046e-07   9.705e-08
50-150  3.533e-07   9.865e-08
15-150  1.836e-06   2.340e-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: 3.24866     (     )
Norm@50keV  : 0.873192    (     )
------------------------------------------------------------
#Fit statistic : Chi-Squared =        1114.72 using 59 PHA bins.
# Reduced chi-squared =        19.5565 for     57 degrees of freedom 
# Null hypothesis probability =  5.298077e-196
 
Photon flux (15-150 keV)    in 0.168 sec: 289.424 (    ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.99656e-06 ( 0  0 ) ergs/cm2

Cutoff power-law model

Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: -0.241560     ( -0.266435   0.253222 )
Epeak [keV] : 29.5420      ( -1.28799 1.1803 )
Norm@50keV  : 64.2241    ( -17.1506   24.9553 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          60.12 using 59 PHA bins.
# Reduced chi-squared =          1.074 for     56 degrees of freedom 
# Null hypothesis probability =   3.290575e-01
 
Photon flux (15-150 keV)    in 0.168 sec: 232.329 ( -8.019  8.103 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.84187e-06 ( 0  0 ) ergs/cm2

Band function

 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : 0.237143   ( -0.239013   0.281906 )
beta        : -10.0000    ( 10   10 )
Epeak [keV] : 29.5151      ( -1.2685 1.20242 )
Norm@50keV   : 63.9143    ( -16.7599   25.5357 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          60.12 using 59 PHA bins.
# Reduced chi-squared =          1.093 for     55 degrees of freedom 
# Null hypothesis probability =   2.955675e-01
 
Photon flux (15-150 keV)    in 0.168 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)  = 6.48e-07
S(50-100 keV) = 2.72e-07

T90 vs. Hardness ratio plot

T90                                   = 0.12799996137619 sec.
Hardness ratio (energy fluence ratio) = 0.419753

Color vs. Color plot

Count Ratio  (25-50 keV) / (15-25 keV) = 1.0642
Count Ratio (50-100 keV) / (15-25 keV) = 0.219181

Mask shadow pattern

IMX = -1.076574603843445E-01, IMY = 1.828344656944240E-01

TIME vs. PHA plot around the trigger time

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.016000

TIME vs. DetID plot around the trigger time

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.016000

100 us light curve (15-350 keV)

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.016000

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:
-239.244000 -0.072000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
254.4393  35.2001    5.5  39.6  170.7   0.8308   2.1    8.6	Her X-1                       
268.2697  -1.5700    6.8  23.9   97.0  -0.5308  -1.7    9.2	SW J1753.5-0127               
270.3151 -24.9847  183.0  40.1   63.6  -0.0508  -0.1    5.9	GX 5-1                        
270.2891 -25.7288    9.9  40.8   63.1   0.9846   1.2    1.1	GRS 1758-258                  
274.0677 -14.0144    2.8  28.9   67.9   1.5896   4.1    3.8	GX 17+2                       
275.6724 -30.3335    0.0  43.1   53.8   1.0296   1.2   13.2	H1820-303                     
285.0405 -24.9135   86.3  36.0   43.0   0.0584   0.1    0.5	HT1900.1-2455                 
288.7536  10.9563    1.2   0.1  175.6   2.2813   9.8    2.7	GRS 1915+105                  
299.5886  35.2040    0.4  26.2 -122.7   8.1138  28.4    0.2	Cyg X-1                       
308.1770  40.8508    4.5  34.5 -116.6   1.0522   2.5    6.8	Cyg X-3                       
276.1395 -17.7668    3.2  31.3   60.9   1.3476   3.6 ------	UNKNOWN                       
280.4751  -8.7570    2.3  21.3   60.4   1.3414   5.1 ------	UNKNOWN                       
301.5906 -21.4697    3.7  34.7   15.9   1.0029   3.1 ------	UNKNOWN                       
299.2571 -17.7199    3.5  30.4   17.2   0.9045   3.3 ------	UNKNOWN                       
253.4434  52.2823    2.9  50.3 -170.3   2.5417   4.0 ------	UNKNOWN                       
243.7743  56.7223    2.7  57.4 -170.3   5.2523   4.3 ------	UNKNOWN                       
307.9748  54.9437    3.3  46.6 -127.9   3.6498   3.5 ------	UNKNOWN                       
332.1681  18.9994    2.9  42.5  -69.2   4.1618   4.0 ------	UNKNOWN

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

Time interval of the image:
-0.072000 0.096000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
254.4586  35.3424   34.7  39.6  170.9  -0.0286  -0.3    0.0	Her X-1                       
268.2171  -1.4149    4.6  23.9   97.4  -0.1764  -2.5    9.3	SW J1753.5-0127               
270.2916 -25.0872    6.4  40.2   63.6   0.3355   1.8    0.6	GX 5-1                        
270.3530 -25.8397  116.6  40.9   62.9  -0.0193  -0.1    6.4	GRS 1758-258                  
274.0526 -14.1673   14.9  29.0   67.8  -0.0658  -0.8    8.3	GX 17+2                       
275.9762 -30.3496    7.8  43.0   53.4   0.2984   1.5    2.8	H1820-303                     
285.1745 -24.8571  158.5  35.9   42.8   0.0074   0.1    8.4	HT1900.1-2455                 
288.9591  10.8769   69.9   0.1  -57.7   0.0087   0.2   10.3	GRS 1915+105                  
299.4921  35.2546    5.5  26.2 -122.9  -0.1236  -2.1    5.8	Cyg X-1                       
308.1178  40.9798    8.6  34.6 -116.8   0.1224   1.3    1.7	Cyg X-3                       
302.8289 -32.4375    2.4  45.3   20.4   0.5181   4.8 ------	UNKNOWN                       
245.8418  39.7262    2.3  47.7  171.9   0.6469   5.0 ------	UNKNOWN                       
293.7275  21.8914    0.1  12.0 -120.5   4.7822  93.7 ------	UNKNOWN                       
335.2736  -6.1752    2.0  49.3  -34.9   0.8442   5.6 ------	UNKNOWN

Post-slew image of 15-350 keV band

Time interval of the image:
42.656590 320.056600
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
254.4737  35.1529  172.7  36.7  152.1   0.0329   0.1   11.4	Her X-1                       
268.4636  -1.5380    7.5  34.0   81.8   0.8455   1.5    7.7	SW J1753.5-0127               
273.8862 -14.1203    7.8  40.9   62.3   1.3431   1.5    8.6	GX 17+2                       
284.8026 -24.8630    6.8  47.5   43.1  -1.8365  -1.7   13.2	HT1900.1-2455                 
288.7657  10.9401    1.3  11.9   56.4   2.2611   8.9    2.0	GRS 1915+105                  
299.6013  35.1977    0.3  14.3 -128.1  10.4457  40.2    0.6	Cyg X-1                       
308.0680  40.9946    3.2  22.6 -118.8   1.1081   3.6    3.2	Cyg X-3                       
326.1981  38.1958    5.7  32.3  -95.7   0.9417   2.0    7.7	Cyg X-2                       
252.1874  11.1157    2.7  41.1  113.8   4.3597   4.3 ------	UNKNOWN                       
319.3614 -20.3786    2.6  49.1   -0.3   2.2924   4.4 ------	UNKNOWN

Plot creation:
Thu May 19 12:21:15 EDT 2016