batgrbproduct analysis for trigger=686443

batgrbproduct Analysis for Trigger=686443

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): Tue May 17 17:56:24 EDT 2016
             Host Name: bat1
   Current Working Dir: /local/data/bat1/prebascript/trigger686443/GCN5_download_cron
======================================================================

  Trigger: 00686443      Segment: 000

  BAT Trigger Time: 485124603.26   [s; MET]
      Trigger Stop: 485124603.276   [s; MET]
               UTC: 2016-05-16T20:49:46.981860    [includes UTCF correction] 
       Where From?: (*SHORT BURST*) TDRSS scaled map message

  BAT 
    RA: 293.704102098376   Dec: 21.8799242647327  [deg; J2000]

     Catalogged Source?: YES
     Point Source?:      YES
     GRB Indicated?:     NO    [ by BAT flight software ]
     Image S/N Ratio:    9.21
     Image Trigger?:     NO
     Rate S/N Ratio:     42.8952211790544  [ if not an image trigger ]
     Image S/N Ratio:    9.21

  Flight Position:   [ source = BAT ]
    RA: 293.704102098376   Dec: 21.8799242647327  [deg; J2000]

  Ground Position:   [ source = BAT pre-slew burst ]
    RA: 293.731746221103   Dec: 21.8823287360038  [deg; J2000]  
        { 19h 34m 55.6s , +21d 52' 56.4" }
         +/- 2.16653014226968 [arcmin] (estimated 90% radius based on SNR)
         +/- 1.32753716540423 [arcmin] (formal 1-sigma fit error)
    SNR: 10.0798593445696
 
  Angular difference between Flight and Ground position is 1.545903 arcmin
 
  Partial Coding Fraction: 0.2382812    [ including projection effects ]

  Duration
     T90: 0.0279999375343323 +/- 0.0113137314268704
        Measured from: -0.0119998455047607
                   to: 0.0160000920295715     [s; relative to TRIGTIME]
     T50: 0.0079999566078186 +/- 0.00400000810623169
        Measured from: -0.00399988889694214
                   to: 0.00400006771087646     [s; relative to TRIGTIME]



  Fluence
     Peak Flux  (peak 1 second)
        Measured from: -0.495999991893768     
                   to: 0.504000008106232     [s; relative to TRIGTIME]
     Total Fluence        
        Measured from: -0.015999972820282     
                   to: 0.0199999809265137     [s; relative to TRIGTIME]
     
             Band 1     Band 2     Band 3     Band 4
              15-25      25-50     50-100    100-350     keV
 Total     0.052209   0.042752   0.015764  -0.000316
           0.007330   0.006367   0.004136   0.001735 [error]
 Peak      0.054357   0.018000   0.015661  -0.002993
           0.014665   0.014723   0.010493   0.009347 [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 9.64e-09 4.08e-09 1.02e-09 3.15e-10 1.49e-08 1.50e-08   erg/cm2
              Error 2.76e-09 1.26e-09 5.11e-10 2.57e-10 4.09e-09 4.13e-09   erg/cm2
Peak flux Power-law 4.87e-01 2.68e-01 9.25e-02 4.17e-02 8.70e-01 8.89e-01   ph/cm2/s
              Error 2.39e-01 1.27e-01 8.15e-02 7.77e-02 3.46e-01 3.58e-01   ph/cm2/s
 
Fluence   Cutoff-PL 1.38e-08 1.49e-08 1.63e-10 9.26e-17 2.89e-08 2.89e-08   erg/cm2
              Error 3.84e-09 3.87e-09 1.74e-10 3.34e-15 5.50e-09 5.50e-09   erg/cm2
Peak flux Cutoff-PL 4.86e-01 2.68e-01 9.27e-02 4.16e-02 8.69e-01 8.89e-01   ph/cm2/s
              Error 1.79e-01 1.30e-01 8.31e-02 5.66e-02 3.46e-01 3.56e-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    3.987    0.422    -      -           1.90e-02 7.83e-03   96.740 57
CPL   1.000    0.000      50.0    0.0      2.87e-02 0.00e+00  128.500 56
 
The chi2 of BB fit is 68.38 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    2.534    1.021    -      -           4.34e-03 3.64e-03   66.360 57
CPL  -8.303    0.000      21.2    0.0      2.18e+06 0.00e+00   66.040 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: 0.000000 sec.
T50 in the 50-300 keV band: 0.000000 sec.

 
=== Table of the duration information ==
 
        Value   tstart    tstop
T100    0.036   -0.016    0.020
T90     0.028   -0.012    0.016
T50     0.008   -0.004    0.004
Peak    1.000   -0.496    0.504

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
  293.7317 +21.8823 0.0190   34.2   77.7       0.1174    10.1  TRIG_00686443       
------------------------------------------
 
Foreground time interval of the image:
 -0.016   0.020 (delta_t =   0.036 [sec])
Background time interval of the image:
-239.260  -0.016 (delta_t = 239.244 [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   -0.016 sec. to    0.020 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 3.98707     ( -0.394098   0.449953 )
Norm@50keV  : 1.90176E-02    ( -0.00770539   0.00795124 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          96.74 using 59 PHA bins.
# Reduced chi-squared =          1.697 for     57 degrees of freedom 
# Null hypothesis probability =   7.996933e-04
 
Photon flux (15-150 keV)    in 0.036 sec: 11.6103 ( -3.19627  3.19987 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.4935e-08 ( -4.0847e-09  4.09212e-09 ) ergs/cm2

Cutoff power-law model

Time interval is from   -0.016 sec. to    0.020 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.00000     (     )
Epeak [keV] : 50.0000      (   )
Norm@50keV  : 2.87473E-02    (     )
------------------------------------------------------------
#Fit statistic : Chi-Squared =         128.50 using 59 PHA bins.
# Reduced chi-squared =         2.2947 for     56 degrees of freedom 
# Null hypothesis probability =   1.260993e-07
 
Photon flux (15-150 keV)    in 0.036 sec: 20.3005 ( -4.1134  4.1386 ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.88945e-08 ( -5.49846e-09  5.49886e-09 ) ergs/cm2

Band function

Time interval is from   -0.016 sec. to    0.020 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : 5.00000   ( -1.36866   -5 )
beta        : -10.0000    ( 10   10 )
Epeak [keV] : 23.3420      ( -1.57645 1.51129 )
Norm@50keV   : 5.53961E+04    ( -10682.6   40106.7 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          60.60 using 59 PHA bins.
# Reduced chi-squared =          1.102 for     55 degrees of freedom 
# Null hypothesis probability =   2.809119e-01
 
Photon flux (15-150 keV)    in 0.036 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]    : 5.00802  (-0.428039  0.41668)
R^2/D10^2   : 169.416  (-66.7284   102.801)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          68.38 using 59 PHA bins.
# Reduced chi-squared =          1.200 for     57 degrees of freedom 
# Null hypothesis probability =   1.436534e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.493e-08   3.685e-09
25- 50  9.788e-09   2.686e-09
50-150  4.011e-10   2.056e-10
15-150  2.512e-08   5.783e-09

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 11.4604       (-1.82761      2.1807)
Norm        : 422.808       (-154.925     208.489)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          81.91 using 59 PHA bins.
# Reduced chi-squared =          1.437 for     57 degrees of freedom 
# Null hypothesis probability =   1.698688e-02
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.280e-08   3.560e-09
25- 50  6.554e-09   1.847e-09
50-150  6.393e-10   3.602e-10
15-150  1.999e-08   5.166e-09

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 5.00795        (-0.427971      0.416748)
R1^2/D10^2  : 169.429        (-66.7403      102.789)
kT2 [keV]   : 3.93769E-02        (-0.0393769      -0.0393769)
R2^2/D10^2  : 4.83808E-04    (-0.000483808   -0.000483808)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          68.38 using 59 PHA bins.
# Reduced chi-squared =          1.243 for     55 degrees of freedom 
# Null hypothesis probability =   1.060795e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  0.000e+00   0.000e+00
25- 50  0.000e+00   0.000e+00
50-150  0.000e+00   0.000e+00
15-150  0.000e+00   0.000e+00

Peak spectrum fit

Power-law model

Time interval is from   -0.496 sec. to    0.504 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 2.53371     ( -0.83042   1.21179 )
Norm@50keV  : 4.33558E-03    ( -0.00433558   0.00293844 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          66.36 using 59 PHA bins.
# Reduced chi-squared =          1.164 for     57 degrees of freedom 
# Null hypothesis probability =   1.855418e-01
 
Photon flux (15-150 keV)    in 1 sec: 0.869600 ( -0.346647  0.346014 ) ph/cm2/s
Energy fluence (15-150 keV)             : 4.37586e-08 ( -2.14948e-08  2.35724e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from   -0.496 sec. to    0.504 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: -8.30250     (     )
Epeak [keV] : 21.1707      (   )
Norm@50keV  : 2.18499E+06    (     )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          66.04 using 59 PHA bins.
# Reduced chi-squared =          1.179 for     56 degrees of freedom 
# Null hypothesis probability =   1.687015e-01
 
Photon flux (15-150 keV)    in 1 sec: 0.869362 ( -0.346271  0.344758 ) ph/cm2/s
Energy fluence (15-150 keV)             : 4.3126e-08 ( -4.3126e-08  2.42303e-08 ) ergs/cm2

Band function

Time interval is from   -0.496 sec. to    0.504 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : 2.90815   ( 1.49576   1.49576 )
beta        : -2.88099    ( 2.66705   0.939475 )
Epeak [keV] : 18.7766      ( -11.8017 -11.8017 )
Norm@50keV   : 137.713    ( -138.272   10500.7 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          65.82 using 59 PHA bins.
# Reduced chi-squared =          1.197 for     55 degrees of freedom 
# Null hypothesis probability =   1.506539e-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]    : 4.78980  (-1.46737  2.32928)
R^2/D10^2   : 8.69027  (-8.69027   42.76)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          66.85 using 59 PHA bins.
# Reduced chi-squared =          1.173 for     57 degrees of freedom 
# Null hypothesis probability =   1.747287e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.774e-08   1.107e-08
25- 50  1.041e-08   6.880e-09
50-150  3.422e-10   3.712e-10
15-150  2.849e-08   1.788e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 20.5207       (-13.1089      132.258)
Norm        : 9.87381       (-9.75815     34.1509)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          67.33 using 59 PHA bins.
# Reduced chi-squared =          1.181 for     57 degrees of freedom 
# Null hypothesis probability =   1.644581e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.565e-08   1.013e-08
25- 50  1.397e-08   8.975e-09
50-150  4.368e-09   4.603e-09
15-150  3.399e-08   2.247e-08

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 4.48329        (-1.43627      1.93065)
R1^2/D10^2  : 11.0874        (-5.51205      65.5335)
kT2 [keV]   : 36.2046        (-34.487      -35.9458)
R2^2/D10^2  : 2.26395E-03    (-0.00228345   0.0224412)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          63.58 using 59 PHA bins.
# Reduced chi-squared =          1.156 for     55 degrees of freedom 
# Null hypothesis probability =   1.999876e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.748e-08   1.110e-08
25- 50  1.115e-08   6.765e-09
50-150  2.301e-08   1.543e-08
15-150  5.164e-08   2.463e-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: 3.98707     ( -0.394098   0.449953 )
Norm@50keV  : 1.90176E-02    ( -0.00770539   0.00795124 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          96.74 using 59 PHA bins.
# Reduced chi-squared =          1.697 for     57 degrees of freedom 
# Null hypothesis probability =   7.996933e-04
 
Photon flux (15-150 keV)    in 0.036 sec: 11.6103 ( -3.19627  3.19987 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.4935e-08 ( -4.0847e-09  4.09212e-09 ) ergs/cm2

Cutoff power-law model

Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.00000     (     )
Epeak [keV] : 50.0000      (   )
Norm@50keV  : 2.87473E-02    (     )
------------------------------------------------------------
#Fit statistic : Chi-Squared =         128.50 using 59 PHA bins.
# Reduced chi-squared =         2.2947 for     56 degrees of freedom 
# Null hypothesis probability =   1.260993e-07
 
Photon flux (15-150 keV)    in 0.036 sec: 20.3005 ( -4.1134  4.1386 ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.88945e-08 ( -5.49846e-09  5.49886e-09 ) ergs/cm2

Band function

 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : 5.00000   ( -1.36866   -5 )
beta        : -10.0000    ( 10   10 )
Epeak [keV] : 23.3420      ( -1.57645 1.51129 )
Norm@50keV   : 5.53961E+04    ( -10682.6   40106.7 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          60.60 using 59 PHA bins.
# Reduced chi-squared =          1.102 for     55 degrees of freedom 
# Null hypothesis probability =   2.809119e-01
 
Photon flux (15-150 keV)    in 0.036 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)  = 4.08e-09
S(50-100 keV) = 1.02e-09

T90 vs. Hardness ratio plot

T90                                   = 0.0279999375343323 sec.
Hardness ratio (energy fluence ratio) = 0.25

Color vs. Color plot

Count Ratio  (25-50 keV) / (15-25 keV) = 0.818863
Count Ratio (50-100 keV) / (15-25 keV) = 0.30194

Mask shadow pattern

IMX = 1.451002951008835E-01, IMY = -6.632310588058992E-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:
-239.260000 -0.016000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
299.5906  35.1967    0.4  21.7   92.9   8.0324  28.2    0.3	Cyg X-1                       
308.1191  40.9420    2.0  13.2  101.4   1.3551   5.6    0.8	Cyg X-3                       
326.1002  38.3295    6.8   5.2   13.2   0.3677   1.7    3.4	Cyg X-2                       
289.8368  17.6065    2.4  39.8   77.4   3.9837   4.9 ------	UNKNOWN                       
305.4637  -1.2946    2.5  48.4   44.2   4.6334   4.7 ------	UNKNOWN                       
277.3748  39.3415    2.5  36.0  117.0   2.3583   4.6 ------	UNKNOWN                       
266.4949  67.8216    3.3  38.9  165.6   1.2259   3.5 ------	UNKNOWN                       
239.3510  75.4149    2.6  47.3  176.6   2.1832   4.4 ------	UNKNOWN                       
342.8811  13.7682    2.4  33.2  -14.9   1.2821   4.9 ------	UNKNOWN                       
119.2792  77.4122    3.6  57.9 -156.8   5.0296   3.2 ------	UNKNOWN

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

Time interval of the image:
-0.016000 0.020000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
299.6803  35.3632   10.4  21.6   93.2   0.0061   1.1   10.6	Cyg X-1                       
308.1334  40.7979  123.4  13.3  100.7  -0.0004  -0.1    9.3	Cyg X-3                       
326.0682  38.1417    7.5   5.4   13.6   0.0053   1.5   11.9	Cyg X-2                       
293.7318  21.8823    1.1  34.2   77.7   0.1173  10.1 ------	UNKNOWN                       
348.7880  55.8988    2.4  19.2 -121.4   0.0152   4.9 ------	UNKNOWN

Post-slew image of 15-350 keV band

Time interval of the image:
62.140600 512.840590
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
254.4558  35.3423  197.7  36.7  151.3   0.0389   0.1    0.1	Her X-1                       
268.2336  -1.4208    5.9  34.1   81.1  -1.5509  -2.0    8.3	SW J1753.5-0127               
274.1826 -14.0918    3.8  40.8   60.8   3.5860   3.0   10.8	GX 17+2                       
285.1936 -24.8925    6.9  47.5   41.5  -2.3289  -1.7    8.7	HT1900.1-2455                 
288.7559  10.9692    1.6  11.9   55.3   2.3159   7.2    2.9	GRS 1915+105                  
299.5944  35.2016    0.3  14.3 -129.2  15.1710  43.1    0.2	Cyg X-1                       
308.1146  40.9743    1.4  22.6 -119.8   3.2246   8.4    1.3	Cyg X-3                       
326.3938  38.2511    6.8  32.4  -96.7   1.1140   1.7   11.3	Cyg X-2                       
292.4756  33.2561    3.1  11.4 -154.3   1.3494   3.7 ------	UNKNOWN                       
328.7590 -25.4906    2.7  58.3   -6.5   8.2414   4.3 ------	UNKNOWN                       
261.5798  77.7489    3.7  57.9 -156.7   7.6568   3.2 ------	UNKNOWN

Plot creation:
Tue May 17 18:01:44 EDT 2016