batgrbproduct analysis for trigger=975998

batgrbproduct Analysis for Trigger=975998

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 v2.47
    Process Start Time (local time): Fri Jun  5 09:14:28 EDT 2020
             Host Name: bat1
   Current Working Dir: /local/data/bat1/prebascript/trigger975998/GCN5_download_cron
======================================================================

  Trigger: 00975998      Segment: 000

  BAT Trigger Time: 612962346.276   [s; MET]
      Trigger Stop: 612962346.34   [s; MET]
               UTC: 2020-06-04T11:18:41.219420    [includes UTCF correction] 
       Where From?: (*SHORT BURST*) TDRSS scaled map message

  BAT 
    RA: 257.19483619524   Dec: -40.127019493857  [deg; J2000]

     Catalogged Source?: YES
     Point Source?:      YES
     GRB Indicated?:     NO    [ by BAT flight software ]
     Image S/N Ratio:    16.03
     Image Trigger?:     NO
     Rate S/N Ratio:     78.2496006379585  [ if not an image trigger ]
     Image S/N Ratio:    16.03

  Flight Position:   [ source = BAT ]
    RA: 257.19483619524   Dec: -40.127019493857  [deg; J2000]

  Ground Position:   [ source = BAT pre-slew burst ]
    RA: 257.08921095358   Dec: -40.1341335113953  [deg; J2000]  
        { 17h 08m 21.4s , -40d 08' 02.9" }
         +/- 2.39859394376899 [arcmin] (estimated 90% radius based on SNR)
         +/- 1.29736760837517 [arcmin] (formal 1-sigma fit error)
    SNR: 8.71611692174575
 
  Angular difference between Flight and Ground position is 4.864285 arcmin
 
  Partial Coding Fraction: 0.890625    [ including projection effects ]

  Duration
     T90: 52 +/- 15.0332963783729
        Measured from: -0.275999903678894
                   to: 51.7240000963211     [s; relative to TRIGTIME]
     T50: 21 +/- 13
        Measured from: -0.275999903678894
                   to: 20.7240000963211     [s; relative to TRIGTIME]



  Fluence
     Peak Flux  (peak 1 second)
        Measured from: -0.276000022888184     
                   to: 0.723999977111816     [s; relative to TRIGTIME]
     Total Fluence        
        Measured from: -0.276000022888184     
                   to: 59.7239999771118     [s; relative to TRIGTIME]
     
             Band 1     Band 2     Band 3     Band 4
              15-25      25-50     50-100    100-350     keV
 Total     0.624746   0.596951   0.059609   0.038299
           0.056003   0.053356   0.044848   0.040967 [error]
 Peak      0.134089   0.215273   0.060797  -0.002175
           0.009450   0.010328   0.007043   0.005499 [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 1.90e-07 1.96e-07 1.43e-07 1.66e-07 5.94e-07 6.95e-07   erg/cm2
              Error 2.62e-08 2.50e-08 3.51e-08 7.56e-08 8.37e-08 1.28e-07   erg/cm2
Peak flux Power-law 1.50e+00 1.10e+00 5.39e-01 3.73e-01 3.32e+00 3.52e+00   ph/cm2/s
              Error -------- -------- -------- -------- -------- --------   ph/cm2/s
 
Fluence   Cutoff-PL 1.71e-07 2.54e-07 6.17e-08 9.48e-10 4.87e-07 4.87e-07   erg/cm2
              Error 3.02e-08 3.62e-08 3.78e-08 4.35e-09 6.53e-08 6.53e-08   erg/cm2
Peak flux Cutoff-PL 1.17e+00 1.60e+00 4.46e-01 1.20e-02 3.23e+00 3.23e+00   ph/cm2/s
              Error 1.62e-01 1.29e-01 8.23e-02 -------- 2.30e-01 2.30e-01   ph/cm2/s
 
Fluence        Band 1.63e-07 2.25e-07 7.24e-08 1.45e-08 4.72e-07 4.77e-07   erg/cm2
              Error 2.84e-08 -------- -------- -------- 8.37e-08 --------   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    2.461    0.233    -      -           1.00e-03 1.82e-04   57.440 57
CPL  -0.866    1.958      28.5    4.0      1.52e-01 3.43e+00   41.220 56
 
The chi2 of BB fit is 41.28 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    2.034    0.000    -      -           2.18e-02 0.00e+00  133.520 57
CPL  -1.474    0.921      38.5    2.3      2.79e+00 5.59e+00   54.220 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: 0.320000 sec.
T50 in the 50-300 keV band: 0.192000 sec.

 
=== Table of the duration information ==
 
        Value   tstart    tstop
T100   60.000   -0.276   59.724
T90    52.000   -0.276   51.724
T50    21.000   -0.276   20.724
Peak    1.000   -0.276    0.724

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
  257.0892 -40.1341 0.0221   14.5  119.0       1.5136     8.7  TRIG_00975998       
------------------------------------------
 
Foreground time interval of the image:
 -0.276  59.724 (delta_t =  60.000 [sec])
Background time interval of the image:
-28.975  -0.276 (delta_t =  28.699 [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 0.064000

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 0.064000

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 0.064000

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   -0.276 sec. to   59.724 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 2.46094     ( -0.224119   0.242878 )
Norm@50keV  : 9.99723E-04    ( -0.000181704   0.000182297 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          57.44 using 59 PHA bins.
# Reduced chi-squared =          1.008 for     57 degrees of freedom 
# Null hypothesis probability =   4.588468e-01
 
Photon flux (15-150 keV)    in 60 sec: 0.191786 ( -0.0216434  0.0216456 ) ph/cm2/s
Energy fluence (15-150 keV)             : 5.93698e-07 ( -8.20536e-08  8.53548e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from   -0.276 sec. to   59.724 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: -0.865644     ( -2.45908   1.45644 )
Epeak [keV] : 28.4660      ( -4.38811 3.59064 )
Norm@50keV  : 0.151632    ( -0.185761   6.67968 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          41.22 using 59 PHA bins.
# Reduced chi-squared =         0.7360 for     56 degrees of freedom 
# Null hypothesis probability =   9.303605e-01
 
Photon flux (15-150 keV)    in 60 sec: 0.179686 ( -0.021198  0.021311 ) ph/cm2/s
Energy fluence (15-150 keV)             : 4.87135e-07 ( -6.25278e-08  6.80232e-08 ) ergs/cm2

Band function

Time interval is from   -0.276 sec. to   59.724 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : 1.10426   ( -1.84277   -0.866056 )
beta        : -9.99866    ( 9.99866   0.0013684 )
Epeak [keV] : 28.6635      ( -3.02539 3.34911 )
Norm@50keV   : 0.218441    ( -0.023748   6.45711 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          41.15 using 59 PHA bins.
# Reduced chi-squared =         0.7483 for     55 degrees of freedom 
# Null hypothesis probability =   9.170812e-01
 
Photon flux (15-150 keV)    in 60 sec:  (    ) ph/cm2/s
Energy fluence (15-150 keV)             : 4.72282e-07 ( -4.71862e-07  -7.338e-08 ) ergs/cm2

Single BB

 
Spectral model blackbody:
------------------------------------------------------------
Parameters  : value    Lower 90%  Upper 90%
kT [keV]    : 7.46775  (-0.731013  0.802545)
R^2/D10^2   : 0.291507  (-0.101309   0.1562)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          41.28 using 59 PHA bins.
# Reduced chi-squared =         0.7242 for     57 degrees of freedom 
# Null hypothesis probability =   9.419122e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.668e-07   3.210e-08
25- 50  2.581e-07   3.939e-08
50-150  5.374e-08   2.069e-08
15-150  4.786e-07   7.368e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 30.7898       (-6.56968      9.1474)
Norm        : 1.53141       (-0.312947     0.405961)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          47.56 using 59 PHA bins.
# Reduced chi-squared =         0.8345 for     57 degrees of freedom 
# Null hypothesis probability =   8.090474e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.895e-07   2.766e-08
25- 50  2.196e-07   3.288e-08
50-150  1.244e-07   4.716e-08
15-150  5.335e-07   8.541e-08

Double BB

# Reduced chi-squared =         0.7156 for     55 degrees of freedom 
# Reduced chi-squared =         0.7146 for     55 degrees of freedom 
# Reduced chi-squared =         0.7140 for     55 degrees of freedom 
# Reduced chi-squared =         0.7137 for     55 degrees of freedom 
# Reduced chi-squared =         0.7135 for     55 degrees of freedom 
# Null hypothesis probability =   9.382481e-01
# Null hypothesis probability =   9.414330e-01
# Null hypothesis probability =   9.435312e-01
# Null hypothesis probability =   9.448590e-01
# Null hypothesis probability =   9.456104e-01
# Null hypothesis probability =   9.460309e-01
# Null hypothesis probability =   9.462544e-01
# Null hypothesis probability =   9.463912e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.660e-07   3.555e-08
25- 50  2.566e-07   4.902e-08
50-150  5.853e-08   2.413e-08
15-150  4.811e-07   8.616e-08

Peak spectrum fit

Power-law model

Time interval is from   -0.276 sec. to    0.724 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 2.03425     (     )
Norm@50keV  : 2.17751E-02    (     )
------------------------------------------------------------
#Fit statistic : Chi-Squared =         133.52 using 59 PHA bins.
# Reduced chi-squared =         2.3425 for     57 degrees of freedom 
# Null hypothesis probability =   4.419054e-08
 
Photon flux (15-150 keV)    in 1 sec: 3.31875 (    ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.0124e-07 ( 0  0 ) ergs/cm2

Cutoff power-law model

Time interval is from   -0.276 sec. to    0.724 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: -1.47362     ( -0.991564   0.850221 )
Epeak [keV] : 38.4625      ( -2.15648 2.38841 )
Norm@50keV  : 2.78864    ( -2.78929   8.39163 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          54.22 using 59 PHA bins.
# Reduced chi-squared =         0.9682 for     56 degrees of freedom 
# Null hypothesis probability =   5.425751e-01
 
Photon flux (15-150 keV)    in 1 sec: 3.22620 ( -0.22934  0.22982 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.74059e-07 ( -1.3292e-08  1.3756e-08 ) ergs/cm2

Band function

Time interval is from   -0.276 sec. to    0.724 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : 2.43045   ( -1.19871   2.51407 )
beta        : -3.65620    ( 3.84762   0.732211 )
Epeak [keV] : 36.2934      ( -2.73657 3.15632 )
Norm@50keV   : 12.4073    ( -11.2527   212.192 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          52.60 using 59 PHA bins.
# Reduced chi-squared =         0.9564 for     55 degrees of freedom 
# Null hypothesis probability =   5.668829e-01
 
Photon flux (15-150 keV)    in 1 sec:  (    ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.83399e-07 ( -1.83392e-07  -1.7812e-08 ) ergs/cm2

Single BB

 
Spectral model blackbody:
------------------------------------------------------------
Parameters  : value    Lower 90%  Upper 90%
kT [keV]    : 9.88263  (-0.546227  0.578469)
R^2/D10^2   : 1.86273  (-0.380017   0.469661)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          54.82 using 59 PHA bins.
# Reduced chi-squared =         0.9618 for     57 degrees of freedom 
# Null hypothesis probability =   5.571444e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  3.690e-08   3.990e-09
25- 50  9.021e-08   6.315e-09
50-150  4.550e-08   7.720e-09
15-150  1.726e-07   1.280e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 56.8551       (-8.58813      10.3177)
Norm        : 18.7198       (-1.90601     1.98044)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          95.96 using 59 PHA bins.
# Reduced chi-squared =          1.684 for     57 degrees of freedom 
# Null hypothesis probability =   9.530390e-04
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  4.661e-08   4.445e-09
25- 50  6.976e-08   4.810e-09
50-150  7.583e-08   1.271e-08
15-150  1.922e-07   1.515e-08

Double BB

------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 9.66700        (-9.45268      0.844813)
R1^2/D10^2  : 1.99668        (-0.546539      0.902219)
kT2 [keV]   : 193.098        (-190.782      -190.782)
R2^2/D10^2  : 5.52590E-05    (-5.59448e-05   2.33669)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          53.14 using 59 PHA bins.
#Fit statistic : Chi-Squared =          52.98 using 59 PHA bins.
# Reduced chi-squared =         0.9661 for     55 degrees of freedom 
# Reduced chi-squared =         0.9633 for     55 degrees of freedom 
# Null hypothesis probability =   5.460859e-01
# Null hypothesis probability =   5.520693e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  3.807e-08   4.600e-09
25- 50  8.882e-08   1.787e-08
50-150  5.570e-08   2.217e-08
15-150  1.826e-07   4.050e-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: 2.46094     ( -0.224119   0.242878 )
Norm@50keV  : 9.99723E-04    ( -0.000181704   0.000182297 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          57.44 using 59 PHA bins.
# Reduced chi-squared =          1.008 for     57 degrees of freedom 
# Null hypothesis probability =   4.588468e-01
 
Photon flux (15-150 keV)    in 60 sec: 0.191786 ( -0.0216434  0.0216456 ) ph/cm2/s
Energy fluence (15-150 keV)             : 5.93698e-07 ( -8.20536e-08  8.53548e-08 ) ergs/cm2

Cutoff power-law model

Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: -0.865644     ( -2.45908   1.45644 )
Epeak [keV] : 28.4660      ( -4.38811 3.59064 )
Norm@50keV  : 0.151632    ( -0.185761   6.67968 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          41.22 using 59 PHA bins.
# Reduced chi-squared =         0.7360 for     56 degrees of freedom 
# Null hypothesis probability =   9.303605e-01
 
Photon flux (15-150 keV)    in 60 sec: 0.179686 ( -0.021198  0.021311 ) ph/cm2/s
Energy fluence (15-150 keV)             : 4.87135e-07 ( -6.25278e-08  6.80232e-08 ) ergs/cm2

Band function

 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : 1.10426   ( -1.84277   -0.866056 )
beta        : -9.99866    ( 9.99866   0.00142787 )
Epeak [keV] : 28.6635      ( -3.02539 3.34911 )
Norm@50keV   : 0.218441    ( -0.023748   6.45711 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          41.15 using 59 PHA bins.
# Reduced chi-squared =         0.7483 for     55 degrees of freedom 
# Null hypothesis probability =   9.170812e-01
 
Photon flux (15-150 keV)    in 60 sec:  (    ) ph/cm2/s
Energy fluence (15-150 keV)             : 4.72282e-07 ( -4.71862e-07  -7.338e-08 ) ergs/cm2

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

S(25-50 keV)  = 1.96e-07
S(50-100 keV) = 1.43e-07

T90 vs. Hardness ratio plot

T90                                   = 52 sec.
Hardness ratio (energy fluence ratio) = 0.729592

Color vs. Color plot

Count Ratio  (25-50 keV) / (15-25 keV) = 0.95551
Count Ratio (50-100 keV) / (15-25 keV) = 0.0954132

Mask shadow pattern

IMX = -1.255400537819071E-01, IMY = -2.267216342563589E-01

TIME vs. PHA plot around the trigger time

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.064000

TIME vs. DetID plot around the trigger time

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.064000

100 us light curve (15-350 keV)

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.064000

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:
-28.975400 -0.276000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
170.6316 -60.4902    0.0  40.0  -73.1   0.5450   2.2   12.3	Cen X-3                       
186.6345 -62.8348    1.3  32.1  -75.2   1.0728   9.1    3.9	GX 301-2                      
244.9659 -15.6478    1.7  33.6   67.8   0.8874   6.9    0.9	Sco X-1                       
255.9798 -37.7991    4.5  15.6  110.4   0.2002   2.6    2.7	4U 1700-377                   
256.4634 -36.5382    5.2  16.9  108.7   0.1711   2.2    7.0	GX 349+2                      
263.0060 -24.8094    5.9  29.8  104.2  -0.2110  -2.0    3.8	GX 1+4                        
264.9502 -44.4572    3.8  17.0  144.2   0.2200   3.0    8.9	4U 1735-44                    
270.1484 -25.0108    7.7  33.1  114.9   0.1918   1.5    8.4	GX 5-1                        
270.4260 -25.9221    0.0  32.5  116.2  -0.1210  -1.0   12.6	GRS 1758-258                  
275.9701 -30.2747    5.0  32.4  128.4   0.2758   2.3    6.0	H1820-303                     
285.0343 -24.9225  251.3  41.9  131.9  -0.0100  -0.0    0.2	HT1900.1-2455                 
262.9535 -33.8622    6.0  22.3  116.0   0.1443   1.9    2.4	GX 354-0                      
200.7998 -11.9164    2.4  49.7    5.0   0.7920   4.8 ------	UNKNOWN                       
176.7346 -20.0166    2.1  58.2  -23.6   2.3051   5.5 ------	UNKNOWN                       
  1.2057 -72.5765    2.3  51.6 -138.6   1.7993   5.1 ------	UNKNOWN

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

Time interval of the image:
-0.276000 59.724000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
170.2042 -60.5094   14.1  40.2  -73.3  -0.4847  -0.8    7.6	Cen X-3                       
186.6688 -62.9031    5.1  32.1  -75.3  -0.6754  -2.2    8.0	GX 301-2                      
244.8950 -15.5984   12.6  33.6   67.7  -0.2833  -0.9    5.5	Sco X-1                       
255.8726 -37.6536    0.0  15.7  109.8   0.3090   1.7   12.6	4U 1700-377                   
256.3226 -36.5494    7.1  16.8  108.4  -0.2918  -1.6    9.3	GX 349+2                      
263.0818 -24.8038    4.1  29.8  104.3   0.7028   2.8    5.3	GX 1+4                        
264.7748 -44.4377    6.5  16.9  144.0  -0.3128  -1.8    1.6	4U 1735-44                    
270.1557 -24.9568   24.2  33.2  114.8  -0.1482  -0.5   10.1	GX 5-1                        
270.4494 -25.7405   12.6  32.7  116.1   0.2831   0.9    7.9	GRS 1758-258                  
276.0267 -30.3105    4.3  32.4  128.5  -0.7366  -2.7    6.3	H1820-303                     
285.1894 -24.9821    9.0  41.9  132.1   0.6204   1.3    9.1	HT1900.1-2455                 
262.8139 -33.9465    4.5  22.2  115.9  -0.4699  -2.5   11.0	GX 354-0                      
244.5678  -7.5795    2.4  41.6   66.2   3.2312   4.8 ------	UNKNOWN                       
228.2996 -19.9486    2.4  30.8   37.1   1.0962   4.8 ------	UNKNOWN                       
257.0892 -40.1341    1.3  14.5  119.0   1.5138   8.8 ------	UNKNOWN                       
168.9023 -52.4988    2.3  43.7  -62.5   3.3472   5.0 ------	UNKNOWN

Post-slew image of 15-350 keV band

Time interval of the image:

Plot creation:
Fri Jun  5 09:18:37 EDT 2020