batgrbproduct analysis for trigger=894557

batgrbproduct Analysis for Trigger=894557

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 15 downlinks after the trigger.

======================================================================
                  BAT GRB EVENT DATA PROCESSING REPORT
    Process Script Ver: batgrbproduct v2.46
    Process Start Time (local time): Sun Mar 24 18:44:18 EDT 2019
             Host Name: bat1
   Current Working Dir: /local/data/bat1/prebascript/trigger894557/GCN5_download_cron
======================================================================

  Trigger: 00894557      Segment: 000

  BAT Trigger Time: 575065869.824   [s; MET]
      Trigger Stop: 575065869.952   [s; MET]
               UTC: 2019-03-23T20:30:47.204380    [includes UTCF correction] 
       Where From?: TDRSS position message

  BAT 
    RA: 40.1528246982427   Dec: 61.245816597833  [deg; J2000]

     Catalogged Source?: NO
     Point Source?:      YES
     GRB Indicated?:     YES    [ by BAT flight software ]
     Image S/N Ratio:    7.26
     Image Trigger?:     NO
     Rate S/N Ratio:     11.13552872566  [ if not an image trigger ]
     Image S/N Ratio:    7.26

  Flight Position:   [ source = BAT ]
    RA: 40.1528246982427   Dec: 61.245816597833  [deg; J2000]

  Ground Position:   [ source = BAT pre-slew burst ]
    RA: 40.1392757265374   Dec: 61.220942845234  [deg; J2000]  
        { 02h 40m 33.4s , +61d 13' 15.4" }
         +/- 1.77871274244497 [arcmin] (estimated 90% radius based on SNR)
         +/- 0.968343020590824 [arcmin] (formal 1-sigma fit error)
    SNR: 13.3605506165172
 
  Angular difference between Flight and Ground position is 1.542850 arcmin
 
  Partial Coding Fraction: 0.4375    [ including projection effects ]

  Duration
     T90: 16.5639998912811 +/- 1.27769318913387
        Measured from: 0.128000140190125
                   to: 16.6920000314713     [s; relative to TRIGTIME]
     T50: 9.64800000190735 +/- 3.46114666326306
        Measured from: 0.992000102996826
                   to: 10.6400001049042     [s; relative to TRIGTIME]



  Fluence
     Peak Flux  (peak 1 second)
        Measured from: 2.80400002002716     
                   to: 3.80400002002716     [s; relative to TRIGTIME]
     Total Fluence        
        Measured from: -0.567999958992004     
                   to: 17.1280000209808     [s; relative to TRIGTIME]
     
             Band 1     Band 2     Band 3     Band 4
              15-25      25-50     50-100    100-350     keV
 Total     0.574593   0.632683   0.168122  -0.045444
           0.053821   0.055342   0.045511   0.038258 [error]
 Peak      0.159003   0.187983   0.015759   0.005149
           0.015838   0.016699   0.012220   0.009033 [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 2.26e-07 2.43e-07 1.86e-07 2.33e-07 7.43e-07 8.89e-07   erg/cm2
              Error 3.01e-08 2.82e-08 3.93e-08 9.06e-08 9.59e-08 1.49e-07   erg/cm2
Peak flux Power-law 2.10e+00 1.13e+00 3.79e-01 1.65e-01 3.70e+00 3.78e+00   ph/cm2/s
              Error 3.00e-01 1.44e-01 8.73e-02 6.62e-02 4.39e-01 4.49e-01   ph/cm2/s
 
Fluence   Cutoff-PL 2.02e-07 3.14e-07 1.21e-07 6.32e-09 6.44e-07 6.44e-07   erg/cm2
              Error 3.44e-08 4.23e-08 5.23e-08 1.51e-08 8.47e-08 8.55e-08   erg/cm2
Peak flux Cutoff-PL 1.81e+00 1.64e+00 1.45e-01 2.83e-04 3.60e+00 3.60e+00   ph/cm2/s
              Error 3.56e-01 2.40e-01 9.08e-02 1.76e-03 4.34e-01 4.34e-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    2.384    0.203    -      -           4.32e-03 6.81e-04   60.300 57
CPL  -0.241    1.446      30.4    4.9      1.96e-01 1.20e+00   43.730 56
 
The chi2 of BB fit is 45.75 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    2.576    0.221    -      -           1.80e-02 3.24e-03   86.390 57
CPL  -2.081    2.286      28.4    2.9      2.22e+01 9.58e+02   64.560 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   17.696   -0.568   17.128
T90    16.564    0.128   16.692
T50     9.648    0.992   10.640
Peak    1.000    2.804    3.804

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
   40.1393 +61.2209 0.0144   40.1 -139.8       0.9516    13.4  TRIG_00894557       
------------------------------------------
 
Foreground time interval of the image:
 -0.568   8.777 (delta_t =   9.345 [sec])
Background time interval of the image:
-239.824 -117.685 (delta_t = 122.139 [sec])
-116.824  -0.568 (delta_t = 116.256 [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 0.128000

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 0.128000

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 0.128000

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   -0.568 sec. to   17.128 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 2.38389     ( -0.195306   0.210192 )
Norm@50keV  : 4.31972E-03    ( -0.000684057   0.00067793 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          60.30 using 59 PHA bins.
# Reduced chi-squared =          1.058 for     57 degrees of freedom 
# Null hypothesis probability =   3.574881e-01
 
Photon flux (15-150 keV)    in 17.7 sec: 0.791786 ( -0.0857431  0.0857471 ) ph/cm2/s
Energy fluence (15-150 keV)             : 7.43103e-07 ( -9.47642e-08  9.70399e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from   -0.568 sec. to   17.128 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: -0.240813     ( -1.64994   1.24244 )
Epeak [keV] : 30.4299      ( -5.6185 4.13376 )
Norm@50keV  : 0.195972    ( -0.208217   2.18785 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          43.73 using 59 PHA bins.
# Reduced chi-squared =         0.7810 for     56 degrees of freedom 
# Null hypothesis probability =   8.834021e-01
 
Photon flux (15-150 keV)    in 17.7 sec: 0.759386 ( -0.085125  0.08537 ) ph/cm2/s
Energy fluence (15-150 keV)             : 6.43579e-07 ( -8.13386e-08  8.80911e-08 ) ergs/cm2

Band function

Time interval is from   -0.568 sec. to   17.128 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : 0.350944   ( -1.44545   2.22061 )
beta        : -9.15965    ( 9.9957   19.9936 )
Epeak [keV] : 30.5744      ( -3.52348 3.99981 )
Norm@50keV   : 0.230863    ( -0.230863   11.3821 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          43.73 using 59 PHA bins.
# Reduced chi-squared =         0.7952 for     55 degrees of freedom 
# Null hypothesis probability =   8.627947e-01
 
Photon flux (15-150 keV)    in 17.7 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]    : 8.07815  (-0.797142  0.871415)
R^2/D10^2   : 0.886558  (-0.304098   0.467992)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          45.75 using 59 PHA bins.
# Reduced chi-squared =         0.8027 for     57 degrees of freedom 
# Null hypothesis probability =   8.572805e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.865e-07   3.287e-08
25- 50  3.319e-07   4.788e-08
50-150  8.998e-08   2.875e-08
15-150  6.084e-07   8.558e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 35.7727       (-7.33553      9.93279)
Norm        : 5.68608       (-1.04253     1.29925)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          48.48 using 59 PHA bins.
# Reduced chi-squared =         0.8506 for     57 degrees of freedom 
# Null hypothesis probability =   7.817125e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  2.218e-07   3.089e-08
25- 50  2.774e-07   3.744e-08
50-150  1.891e-07   6.315e-08
15-150  6.883e-07   1.003e-07

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 5.05401        (-5.05401      -5.05401)
R1^2/D10^2  : 2.30291        (-2.30291      -2.30291)
kT2 [keV]   : 9.89823        (-9.89823      -9.89823)
R2^2/D10^2  : 0.282167    (-0.282167   0.8114)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          43.72 using 59 PHA bins.
# Reduced chi-squared =         0.7948 for     55 degrees of freedom 
# Null hypothesis probability =   8.632275e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  2.028e-07   1.107e-07
25- 50  3.127e-07   1.668e-07
50-150  1.263e-07   6.862e-08
15-150  6.417e-07   3.384e-07

Peak spectrum fit

Power-law model

Time interval is from    2.804 sec. to    3.804 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 2.57583     ( -0.210006   0.231459 )
Norm@50keV  : 1.79866E-02    ( -0.00325955   0.00321859 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          86.39 using 59 PHA bins.
# Reduced chi-squared =          1.516 for     57 degrees of freedom 
# Null hypothesis probability =   7.236690e-03
 
Photon flux (15-150 keV)    in 1 sec: 3.70415 ( -0.439224  0.439234 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.83782e-07 ( -2.5093e-08  2.5509e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from    2.804 sec. to    3.804 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: -2.08114     ( -2.87961   1.69172 )
Epeak [keV] : 28.4389      ( -3.02422 2.80636 )
Norm@50keV  : 22.2047    ( -24.1601   1891.56 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          64.56 using 59 PHA bins.
# Reduced chi-squared =          1.153 for     56 degrees of freedom 
# Null hypothesis probability =   2.024488e-01
 
Photon flux (15-150 keV)    in 1 sec: 3.59666 ( -0.4337  0.43494 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.58688e-07 ( -1.9824e-08  2.0556e-08 ) ergs/cm2

Band function

Time interval is from    2.804 sec. to    3.804 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : 2.57985   ( -1.38381   -1.61787 )
beta        : -5.51079    ( 4.94426   1.39986 )
Epeak [keV] : 28.6244      ( -3.11199 2.79866 )
Norm@50keV   : 48.0911    ( -48.0829   1045.39 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          64.18 using 59 PHA bins.
# Reduced chi-squared =          1.167 for     55 degrees of freedom 
# Null hypothesis probability =   1.858103e-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]    : 7.22254  (-0.668871  0.716036)
R^2/D10^2   : 6.82854  (-2.26585   3.43609)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          64.69 using 59 PHA bins.
# Reduced chi-squared =          1.135 for     57 degrees of freedom 
# Null hypothesis probability =   2.261112e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  5.905e-08   1.100e-08
25- 50  8.585e-08   1.457e-08
50-150  1.591e-08   6.483e-09
15-150  1.608e-07   2.505e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 27.9642       (-5.59915      7.40848)
Norm        : 33.0002       (-6.89984     8.85777)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          75.68 using 59 PHA bins.
# Reduced chi-squared =          1.328 for     57 degrees of freedom 
# Null hypothesis probability =   4.958023e-02
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  6.468e-08   8.935e-09
25- 50  7.101e-08   1.107e-08
50-150  3.539e-08   1.398e-08
15-150  1.711e-07   2.460e-08

Double BB

------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 200.000        (-200      -200)
R1^2/D10^2  : 1.12114E-04        (-7.21762e-05      0.000272654)
kT2 [keV]   : 7.03340        (-0.635944      0.699781)
R2^2/D10^2  : 7.48534    (-2.49417   3.80598)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          64.69 using 59 PHA bins.
#Fit statistic : Chi-Squared =          58.37 using 59 PHA bins.
# Reduced chi-squared =          1.176 for     55 degrees of freedom 
# Reduced chi-squared =          1.061 for     55 degrees of freedom 
# Null hypothesis probability =   1.743591e-01
# Null hypothesis probability =   3.525593e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  5.904e-08   1.247e+00
25- 50  8.586e-08   9.580e+00
50-150  1.592e-08   2.374e+02
15-150  1.608e-07   2.396e+02

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: 2.44478     ( -0.201691   0.217498 )
Norm@50keV  : 5.55685E-03    ( -0.000942036   0.000938971 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          90.11 using 59 PHA bins.
# Reduced chi-squared =          1.581 for     57 degrees of freedom 
# Null hypothesis probability =   3.400251e-03
 
Photon flux (15-150 keV)    in 9.345 sec: 1.05574 ( -0.120487  0.120489 ) ph/cm2/s
Energy fluence (15-150 keV)             : 5.11799e-07 ( -6.86959e-08  7.04877e-08 ) ergs/cm2

Cutoff power-law model

Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: -1.05752     ( -2.23394   1.43078 )
Epeak [keV] : 29.7390      ( -3.66117 3.29797 )
Norm@50keV  : 1.03449    ( -1.41863   36.1561 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          65.82 using 59 PHA bins.
# Reduced chi-squared =          1.175 for     56 degrees of freedom 
# Null hypothesis probability =   1.734753e-01
 
Photon flux (15-150 keV)    in 9.345 sec: 1.02154 ( -0.118085  0.11831 ) ph/cm2/s
Energy fluence (15-150 keV)             : 4.39622e-07 ( -5.55775e-08  5.87333e-08 ) ergs/cm2

Band function

 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : 1.24596   ( -0.91397   4.04533 )
beta        : -10.0000    ( 10   10 )
Epeak [keV] : 29.9026      ( -3.68794 3.20334 )
Norm@50keV   : 1.36921    ( -1.36979   36.0035 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          65.77 using 59 PHA bins.
# Reduced chi-squared =          1.196 for     55 degrees of freedom 
# Null hypothesis probability =   1.517749e-01
 
Photon flux (15-150 keV)    in 9.345 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)  = 2.43e-07
S(50-100 keV) = 1.86e-07

T90 vs. Hardness ratio plot

T90                                   = 16.5639998912811 sec.
Hardness ratio (energy fluence ratio) = 0.765432

Color vs. Color plot

Count Ratio  (25-50 keV) / (15-25 keV) = 1.1011
Count Ratio (50-100 keV) / (15-25 keV) = 0.292593

Mask shadow pattern

IMX = -6.443540563718642E-01, IMY = 5.443169945274297E-01

TIME vs. PHA plot around the trigger time

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.128000

TIME vs. DetID plot around the trigger time

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.128000

100 us light curve (15-350 keV)

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.128000

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:
-239.824000 -117.684700
-116.824000 -0.568000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
254.2201  35.4370    0.0  39.6   31.7  -0.5205  -0.9   12.9	Her X-1                       
299.5714  35.2114    0.6  39.6  -27.5   7.8950  20.2    1.1	Cyg X-1                       
308.0346  40.9119    5.0  35.4  -40.2   0.9007   2.3    4.2	Cyg X-3                       
325.9139  38.3095   64.5  41.9  -60.1   0.1342   0.2   12.2	Cyg X-2                       
165.2184  54.6304    3.9  44.2  131.0   3.5848   3.0 ------	UNKNOWN                       
220.2717  49.8512    2.8  33.7   79.5   2.3548   4.1 ------	UNKNOWN                       
229.9572  51.2937    3.0  29.7   70.2   1.8709   3.9 ------	UNKNOWN                       
257.0894  25.3711    3.0  49.1   26.0   3.2004   3.8 ------	UNKNOWN                       
260.6096  19.7853    3.1  54.3   21.0   4.9793   3.7 ------	UNKNOWN                       
122.9910  50.7220    3.9  54.8  161.8   6.4591   3.5 ------	UNKNOWN                       
122.9729  50.8749    4.1  54.7  161.8   7.0539   3.8 ------	UNKNOWN                       
 83.0072  52.5767    3.1  53.8 -167.9   3.0058   3.8 ------	UNKNOWN

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

Time interval of the image:
-0.568000 8.776600
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
254.6275  35.3498    3.1  39.6   31.2  -0.3070  -3.7    8.3	Her X-1                       
299.4355  35.1068    6.6  39.6  -27.3  -0.1157  -1.7    9.5	Cyg X-1                       
308.1652  40.8706    9.1  35.4  -40.3  -0.0784  -1.3    5.5	Cyg X-3                       
325.9889  38.2704    4.6  41.9  -60.2   0.3072   2.5    9.1	Cyg X-2                       
 40.1393  61.2209    0.9  40.1 -139.8   0.9510  13.3 ------	UNKNOWN

Post-slew image of 15-350 keV band

Time interval of the image:
68.976590 717.376000
718.176000 962.266000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
 83.6467  22.0146    0.9  49.3  171.3  31.2970  12.3    0.7	Crab                          
308.0878  41.0465    8.2  55.8  -17.1  -5.0064  -1.4    5.7	Cyg X-3                       
326.3386  38.3048    6.0  49.6  -33.4   4.5459   1.9    7.9	Cyg X-2                       
 93.6694  20.5445    2.9  54.9  161.6  18.2177   3.9 ------	UNKNOWN                       
301.2106  65.8295    2.3  39.7    9.3   6.5724   4.9 ------	UNKNOWN

Plot creation:
Sun Mar 24 18:48:16 EDT 2019