batgrbproduct analysis for trigger=826428

batgrbproduct Analysis for Trigger=826428

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 May 11 17:59:21 EDT 2018
             Host Name: bat1
   Current Working Dir: /local/data/bat1/alien/Swift_3rdBATcatalog/event/batevent_reproc/trigger826428
======================================================================

  Trigger: 00826428      Segment: 000

  BAT Trigger Time: 545726666.816   [s; MET]
      Trigger Stop: 545726667.264   [s; MET]
               UTC: 2018-04-18T06:44:06.012000    [includes UTCF correction] 
       Where From?: (*SHORT BURST*) Expanded to TRIGTIME - 64 ms to TRIGTIME + 320 ms

  BAT 
    RA: 170.112382201695   Dec: 24.9562917733818  [deg; J2000]

     Catalogged Source?: NO
     Point Source?:      YES
     GRB Indicated?:     YES    [ by BAT flight software ]
     Image S/N Ratio:    8.81
     Image Trigger?:     NO
     Rate S/N Ratio:     22.8473193175917  [ if not an image trigger ]
     Image S/N Ratio:    8.81

  Flight Position:   [ source = BAT ]
    RA: 170.112382201695   Dec: 24.9562917733818  [deg; J2000]

  Ground Position:   [ source = BAT pre-slew burst ]
    RA: 170.128590124768   Dec: 24.9270362960537  [deg; J2000]  
        { 11h 20m 30.9s , +24d 55' 37.3" }
         +/- 1.3625519161545 [arcmin] (estimated 90% radius based on SNR)
         +/- 0.508540245299671 [arcmin] (formal 1-sigma fit error)
    SNR: 19.5517411474932
 
  Angular difference between Flight and Ground position is 1.964361 arcmin
 
  Partial Coding Fraction: 1    [ including projection effects ]

  Duration
     T90: 4.40799999237061 +/- 2.49110413778446
        Measured from: 0.279999971389771
                   to: 4.68799996376038     [s; relative to TRIGTIME]
     T50: 0.787999987602234 +/- 0.188509894903112
        Measured from: 0.480000019073486
                   to: 1.26800000667572     [s; relative to TRIGTIME]



  Fluence
     Peak Flux  (peak 1 second)
        Measured from: 0.236000061035156     
                   to: 1.23600006103516     [s; relative to TRIGTIME]
     Total Fluence        
        Measured from: 0.0959999561309814     
                   to: 7.16799998283386     [s; relative to TRIGTIME]
     
             Band 1     Band 2     Band 3     Band 4
              15-25      25-50     50-100    100-350     keV
 Total     0.122150   0.214889   0.163279   0.049147
           0.014874   0.015816   0.014133   0.011788 [error]
 Peak      0.097779   0.153141   0.101117   0.041370
           0.006913   0.007981   0.007038   0.005314 [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 3.91e-08 7.85e-08 1.22e-07 4.21e-07 3.42e-07 6.61e-07   erg/cm2
              Error 5.66e-09 7.07e-09 1.34e-08 9.77e-08 3.31e-08 1.08e-07   erg/cm2
Peak flux Power-law 9.34e-01 9.93e-01 7.48e-01 9.16e-01 3.02e+00 3.59e+00   ph/cm2/s
              Error 1.01e-01 6.52e-02 5.79e-02 1.47e-01 1.86e-01 2.26e-01   ph/cm2/s
 
Fluence   Cutoff-PL 3.34e-08 8.70e-08 1.28e-07 1.12e-07 3.13e-07 3.60e-07   erg/cm2
              Error 6.75e-09 9.41e-09 1.54e-08 9.98e-08 3.79e-08 1.05e-07   erg/cm2
Peak flux Cutoff-PL 9.33e-01 9.95e-01 7.49e-01 9.08e-01 3.02e+00 3.57e+00   ph/cm2/s
              Error 1.01e-01 7.21e-02 6.19e-02 2.32e-01 1.90e-01 3.26e-01   ph/cm2/s
 
Fluence        Band 3.22e-08 8.98e-08 1.75e-07 7.02e-07 3.18e-07 3.03e-07   erg/cm2
              Error 7.31e-09 1.09e-08 1.71e-08 -------- 3.79e-08 1.69e-07   erg/cm2
Peak flux      Band 9.14e-01 1.03e+00 7.42e-01 7.18e-01 2.94e+00 2.74e+00   ph/cm2/s
              Error 1.32e-01 7.13e-02 5.74e-02 2.32e-01 1.90e-01 3.23e-01   ph/cm2/s

 
=== Time-averaged spectral analysis ===
 
Model Ph_index Ph_90err Epeak  Epeak_90err Norm     Nomr_90err chi2   dof
PL    1.358    0.143    -      -           4.95e-03 4.28e-04   62.170 57
CPL   0.343    0.739      79.7   39.4      1.64e-02 1.71e-02   55.160 56
 
 
=== 1-s peak spectral analysis ===
 
Model Ph_index Ph_90err Epeak  Epeak_90err Norm     Nomr_90err chi2   dof
PL    1.408    0.107    -      -           2.48e-02 1.53e-03   60.840 57
CPL   1.405    0.268    9996.8    0.0      2.49e-02 8.61e-03   60.840 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: 1.024000 sec.
T50 in the 50-300 keV band: 0.512000 sec.

 
=== Table of the duration information ==
 
        Value   tstart    tstop
T100    7.072    0.096    7.168
T90     4.408    0.280    4.688
T50     0.788    0.480    1.268
Peak    1.000    0.236    1.236

Click here for the BAT GCN circular template

Special notes of this burst

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

Image

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

#   RAcent    DECcent   POSerr    Theta     Phi              Peak Cts       SNR   Name
  170.1286    24.9270   0.0098    14.4701   167.3957         0.5726498     19.552 TRIG_00826428                 
 
Foreground time interval of the image:
  0.096   7.168 (delta_t =   7.072 [sec])
Background time interval of the image:
-238.816   0.096 (delta_t = 238.912 [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

8 ms binning

From T100_start-3 s to T100_start+3 s

2 ms binning

From T100_start-1 s to T100_start+1 s

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    0.096 sec. to    7.168 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.35790     ( -0.142475   0.142761 )
Norm@50keV  : 4.95128E-03    ( -0.000428222   0.000427196 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          62.17 using 59 PHA bins.
# Reduced chi-squared =          1.091 for     57 degrees of freedom 
# Null hypothesis probability =   2.972892e-01
 
Photon flux (15-150 keV)    in 7.072 sec: 0.597474 ( -0.05141  0.051453 ) ph/cm2/s
Energy fluence (15-150 keV)             : 3.41431e-07 ( -3.29397e-08  3.33028e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from    0.096 sec. to    7.168 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 0.343053     ( -0.802183   0.676202 )
Epeak [keV] : 79.6850      ( -16.8081 61.9121 )
Norm@50keV  : 1.64226E-02    ( -0.00891734   0.0252565 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          55.16 using 59 PHA bins.
# Reduced chi-squared =         0.9850 for     56 degrees of freedom 
# Null hypothesis probability =   5.065749e-01
 
Photon flux (15-150 keV)    in 7.072 sec: 0.572963 ( -0.054105  0.053972 ) ph/cm2/s
Energy fluence (15-150 keV)             : 3.12912e-07 ( -3.74623e-08  3.82458e-08 ) ergs/cm2

Band function

Time interval is from    0.096 sec. to    7.168 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : 3.32716E-03   ( -0.895717   -0.0187777 )
beta        : -1.97665    ( 1.9742   0.516076 )
Epeak [keV] : 66.3725      ( -32.0621 47.21 )
Norm@50keV   : 2.65544E-02    ( -0.0298881   37.9082 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          53.93 using 59 PHA bins.
# Reduced chi-squared =         0.9805 for     55 degrees of freedom 
# Null hypothesis probability =   5.155915e-01
 
Photon flux (15-150 keV)    in 7.072 sec: 0.573209 ( -0.053441  0.053406 ) ph/cm2/s
Energy fluence (15-150 keV)             : 3.1837e-07 ( -3.7431e-08  3.84606e-08 ) ergs/cm2

Single BB

 
Spectral model blackbody:
------------------------------------------------------------
Parameters  : value    Lower 90%  Upper 90%
kT [keV]    : 15.3010  (-1.44532  1.63888)
R^2/D10^2   : 6.67661E-02  (-0.0198773   0.0274116)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          66.59 using 59 PHA bins.
# Reduced chi-squared =          1.168 for     57 degrees of freedom 
# Null hypothesis probability =   1.803176e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  2.306e-08   3.692e-09
25- 50  9.332e-08   9.653e-09
50-150  1.500e-07   2.458e-08
15-150  2.664e-07   2.967e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 200.000       (-35.4379      -200)
Norm        : 2.46521       (-0.209662     0.209662)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          63.17 using 59 PHA bins.
# Reduced chi-squared =          1.108 for     57 degrees of freedom 
# Null hypothesis probability =   2.675214e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  4.341e-08   5.633e-09
25- 50  8.350e-08   1.529e-08
50-150  1.831e-07   8.296e-08
15-150  3.100e-07   9.505e-08

Double BB

------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 44.6545        (-4.63957      3.73757)
R1^2/D10^2  : 1.09304E-03        (-0.0985203      0.551247)
kT2 [keV]   : 11.3108        (-5.49416      2.78897)
R2^2/D10^2  : 0.145086    (-0.0671274   0.555565)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          54.55 using 59 PHA bins.
#Fit statistic : Chi-Squared =          54.45 using 59 PHA bins.
# Reduced chi-squared =         0.9919 for     55 degrees of freedom 
# Reduced chi-squared =         0.9901 for     55 degrees of freedom 
# Null hypothesis probability =   4.916418e-01
# Null hypothesis probability =   4.954164e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  3.049e-08   1.116e-08
25- 50  9.235e-08   3.731e-08
50-150  1.978e-07   9.900e-08
15-150  3.206e-07   1.458e-07

Peak spectrum fit

Power-law model

Time interval is from    0.236 sec. to    1.236 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.40810     ( -0.106841   0.107329 )
Norm@50keV  : 2.47880E-02    ( -0.0015341   0.00152981 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          60.84 using 59 PHA bins.
# Reduced chi-squared =          1.067 for     57 degrees of freedom 
# Null hypothesis probability =   3.395533e-01
 
Photon flux (15-150 keV)    in 1 sec: 3.02436 ( -0.18601  0.18618 ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.39155e-07 ( -1.65679e-08  1.668e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from    0.236 sec. to    1.236 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.40509     ( -0.374541   0.161177 )
Epeak [keV] : 9996.82      ( -9996.71 -9996.71 )
Norm@50keV  : 2.48765E-02    ( -0.00152908   0.0156944 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          60.84 using 59 PHA bins.
# Reduced chi-squared =          1.086 for     56 degrees of freedom 
# Null hypothesis probability =   3.060837e-01
 
Photon flux (15-150 keV)    in 1 sec: 3.02263 ( -0.19223  0.18788 ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.38864e-07 ( -1.82668e-08  1.69534e-08 ) ergs/cm2

Band function

Time interval is from    0.236 sec. to    1.236 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -0.667762   ( 0.764112   5.76297 )
beta        : -1.51999    ( -0.245351   0.184245 )
Epeak [keV] : 65.8917      ( -65.8917 249.081 )
Norm@50keV   : 6.95979E-02    ( -0.0695979   2.15725e+06 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          59.40 using 59 PHA bins.
# Reduced chi-squared =          1.080 for     55 degrees of freedom 
# Null hypothesis probability =   3.182885e-01
 
Photon flux (15-150 keV)    in 1 sec: 2.94041 ( -0.13235  0.24846 ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.39155e-07 ( -1.65679e-08  1.668e-08 ) ergs/cm2

Single BB

 
Spectral model blackbody:
------------------------------------------------------------
Parameters  : value    Lower 90%  Upper 90%
kT [keV]    : 14.7829  (  )
R^2/D10^2   : 0.363518  (   )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =         129.10 using 59 PHA bins.
# Reduced chi-squared =         2.2650 for     57 degrees of freedom 
# Null hypothesis probability =   1.631690e-07
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.667e-08   1.910e-09
25- 50  6.534e-08   5.110e-09
50-150  9.655e-08   1.280e-08
15-150  1.786e-07   1.330e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 200.000       (-23.0663      -200)
Norm        : 12.4275       (-0.753736     0.753736)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          66.65 using 59 PHA bins.
# Reduced chi-squared =          1.169 for     57 degrees of freedom 
# Null hypothesis probability =   1.790314e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  3.095e-08   2.115e-09
25- 50  5.953e-08   4.520e-09
50-150  1.306e-07   2.893e-08
15-150  2.211e-07   3.920e-08

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 9.31436        (-1.41597      1.44518)
R1^2/D10^2  : 1.36785        (-0.485185      0.885711)
kT2 [keV]   : 49.6352        (-16.6488      71.9034)
R2^2/D10^2  : 5.55810E-03    (-0.00442022   0.0126784)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          57.26 using 59 PHA bins.
# Reduced chi-squared =          1.041 for     55 degrees of freedom 
# Null hypothesis probability =   3.913296e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  2.500e-08   4.280e-09
25- 50  6.349e-08   9.295e-09
50-150  1.539e-07   6.654e-08
15-150  2.424e-07   7.371e-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: 1.35790     ( -0.142475   0.142761 )
Norm@50keV  : 4.95128E-03    ( -0.000428222   0.000427196 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          62.17 using 59 PHA bins.
# Reduced chi-squared =          1.091 for     57 degrees of freedom 
# Null hypothesis probability =   2.972892e-01
 
Photon flux (15-150 keV)    in 7.072 sec: 0.597465 ( -0.0514083  0.0514502 ) ph/cm2/s
Energy fluence (15-150 keV)             : 3.41389e-07 ( -3.29886e-08  3.33049e-08 ) ergs/cm2

Cutoff power-law model

Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 0.343032     ( -0.802178   0.676207 )
Epeak [keV] : 79.6842      ( -16.808 61.9121 )
Norm@50keV  : 1.64231E-02    ( -0.00891736   0.0252565 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          55.16 using 59 PHA bins.
# Reduced chi-squared =         0.9850 for     56 degrees of freedom 
# Null hypothesis probability =   5.065749e-01
 
Photon flux (15-150 keV)    in 7.072 sec: 0.572920 ( -0.054096  0.054025 ) ph/cm2/s
Energy fluence (15-150 keV)             : 3.13031e-07 ( -3.7495e-08  3.82765e-08 ) ergs/cm2

Band function

 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : 3.32716E-03   ( -0.895717   -0.0187777 )
beta        : -1.97665    ( 1.9742   0.516076 )
Epeak [keV] : 66.3725      ( -32.0621 47.21 )
Norm@50keV   : 2.65544E-02    ( -0.0298881   37.9082 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          53.93 using 59 PHA bins.
# Reduced chi-squared =         0.9805 for     55 degrees of freedom 
# Null hypothesis probability =   5.155915e-01
 
Photon flux (15-150 keV)    in 7.072 sec: 0.573209 ( -0.053441  0.053406 ) ph/cm2/s
Energy fluence (15-150 keV)             : 3.1837e-07 ( -3.7431e-08  3.84606e-08 ) ergs/cm2

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

S(25-50 keV)  = 7.85e-08
S(50-100 keV) = 1.22e-07

T90 vs. Hardness ratio plot

T90                                   = 4.40799999237061 sec.
Hardness ratio (energy fluence ratio) = 1.55414

Color vs. Color plot

Count Ratio  (25-50 keV) / (15-25 keV) = 1.75922
Count Ratio (50-100 keV) / (15-25 keV) = 1.33671

Mask shadow pattern

IMX = -2.518425959351169E-01, IMY = -5.631317706837238E-02

TIME vs. PHA plot around the trigger time

TIME vs. DetID plot around the trigger time

100 us light curve (15-350 keV)

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:
-238.816000 0.096000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
254.5044  35.4151    7.1  57.2   -5.0  -1.4757  -1.6    4.9	Her X-1                       
191.0885  16.4902    3.0  18.0   85.3   0.7999   3.9 ------	UNKNOWN                       
134.2644   0.3504    3.3  56.8  173.9   4.6709   3.5 ------	UNKNOWN                       
127.7262   8.2839    2.8  57.2 -173.8   5.0046   4.2 ------	UNKNOWN                       
124.8780  26.4324    2.6  50.9 -152.5   2.7407   4.5 ------	UNKNOWN                       
171.7109  72.7484    3.3  40.0  -76.8   3.0193   3.5 ------	UNKNOWN                       
133.8516  58.5737    2.9  41.6 -108.3   3.4717   4.1 ------	UNKNOWN                       
122.3030  44.2015    3.0  48.1 -129.2   3.9731   3.9 ------	UNKNOWN

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

Time interval of the image:
0.096000 7.168000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
254.3737  35.2865   14.0  57.1   -4.9  -0.1122  -0.8    5.3	Her X-1                       
198.9368  17.6143    2.3  20.7   63.7   0.1661   5.1 ------	UNKNOWN                       
247.2324  22.8140    2.2  56.2   11.8   0.9273   5.3 ------	UNKNOWN                       
170.1286  24.9271    0.6  14.5  167.4   0.5725  19.5 ------	UNKNOWN                       
153.0066  35.3017    2.3  25.4 -147.9   0.1572   4.9 ------	UNKNOWN

Post-slew image of 15-350 keV band

Time interval of the image:
272.084600 963.276800
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
244.9705 -15.6366    0.7  25.0   95.8  22.5001  16.2    0.6	Sco X-1                       
254.4896  35.3542   49.3  55.6  167.9  -1.2725  -0.2    1.7	Her X-1                       
256.0230 -37.8131    2.6  23.7   34.7   4.7663   4.4    2.5	4U 1700-377                   
256.6137 -36.3063   17.2  22.2   36.1   0.6817   0.7   11.1	GX 349+2                      
263.0217 -24.6314    7.1   9.9   51.2   1.4921   1.6    6.9	GX 1+4                        
264.5628 -44.5975    0.0  27.1   14.3   2.5790   2.4   11.7	4U 1735-44                    
268.2156  -1.3128    0.0  17.0  174.7   1.4788   1.5   12.4	SW J1753.5-0127               
270.1184 -25.0662    8.2   7.1   10.6   1.2632   1.4    9.0	GX 5-1                        
270.2307 -25.6985    2.9   7.7    9.3   3.9476   4.3    4.7	GRS 1758-258                  
274.0641 -13.8812    3.5   5.1 -140.0   3.1739   3.3    9.9	GX 17+2                       
275.9108 -30.3773    4.0  13.1  -14.8   2.5744   2.8    1.0	H1820-303                     
285.0311 -24.8137   22.6  14.7  -56.0  -0.5101  -0.5    6.4	HT1900.1-2455                 
288.8058  10.9616    1.9  33.9 -143.2   8.2858   6.2    1.1	GRS 1915+105                  
262.8635 -33.8072    2.4  17.4   27.4   4.4263   4.9    6.5	GX 354-0                      
275.0902   7.1830    0.1  25.6 -166.3  96.4887  93.5 ------	UNKNOWN                       
297.4221 -47.3215    2.3  36.4  -26.4   6.3187   5.1 ------	UNKNOWN                       
319.5309 -45.8613    3.1  48.6  -39.8  14.0591   3.8 ------	UNKNOWN                       
320.4426 -35.8338    2.4  47.0  -53.2  23.4153   4.8 ------	UNKNOWN                       
305.3106  16.1417    3.1  48.1 -129.1  18.7146   3.7 ------	UNKNOWN

Plot creation:
Sun May 13 07:46:58 EDT 2018