batgrbproduct analysis for trigger=933515

batgrbproduct Analysis for Trigger=933515

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): Wed Nov 27 11:54:33 EST 2019
             Host Name: bat1
   Current Working Dir: /local/data/bat1/alien/Swift_3rdBATcatalog/event/batevent_reproc/trigger933515
======================================================================

  Trigger: 00933515      Segment: 000

  BAT Trigger Time: 594742547.776   [s; MET]
      Trigger Stop: 594742548.288   [s; MET]
               UTC: 2019-11-06T14:15:23.900640    [includes UTCF correction] 
       Where From?: TDRSS position message

  BAT 
    RA: 269.349636887849   Dec: 46.0518248196464  [deg; J2000]

     Catalogged Source?: NO
     Point Source?:      YES
     GRB Indicated?:     YES    [ by BAT flight software ]
     Image S/N Ratio:    7.85
     Image Trigger?:     NO
     Rate S/N Ratio:     20.5669638012031  [ if not an image trigger ]
     Image S/N Ratio:    7.85

  Flight Position:   [ source = BAT ]
    RA: 269.349636887849   Dec: 46.0518248196464  [deg; J2000]

  Ground Position:   [ source = BAT pre-slew burst ]
    RA: 269.359318636608   Dec: 46.0473276332839  [deg; J2000]  
        { 17h 57m 26.2s , +46d 02' 50.4" }
         +/- 1.63859635698673 [arcmin] (estimated 90% radius based on SNR)
         +/- 0.741387568123865 [arcmin] (formal 1-sigma fit error)
    SNR: 15.0220716823996
 
  Angular difference between Flight and Ground position is 0.485133 arcmin
 
  Partial Coding Fraction: 0.953125    [ including projection effects ]

  Duration
     T90: 3.43599987030029 +/- 0.324863016551151
        Measured from: -1.25199997425079
                   to: 2.1839998960495     [s; relative to TRIGTIME]
     T50: 1.64799988269806 +/- 0.720988169553211
        Measured from: -0.00800001621246338
                   to: 1.6399998664856     [s; relative to TRIGTIME]



  Fluence
     Peak Flux  (peak 1 second)
        Measured from: -0.0479999780654907     
                   to: 0.952000021934509     [s; relative to TRIGTIME]
     Total Fluence        
        Measured from: -1.35600006580353     
                   to: 2.37999999523163     [s; relative to TRIGTIME]
     
             Band 1     Band 2     Band 3     Band 4
              15-25      25-50     50-100    100-350     keV
 Total     0.056877   0.157930   0.156001   0.053594
           0.013764   0.014639   0.013370   0.011352 [error]
 Peak      0.020252   0.054813   0.053791   0.023784
           0.007093   0.007917   0.007290   0.005981 [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 2.07e-08 5.49e-08 1.18e-07 6.58e-07 3.18e-07 8.52e-07   erg/cm2
              Error 4.33e-09 6.82e-09 1.23e-08 1.63e-07 3.31e-08 1.68e-07   erg/cm2
Peak flux Power-law 2.01e-01 3.13e-01 3.67e-01 8.32e-01 1.13e+00 1.71e+00   ph/cm2/s
              Error 7.01e-02 6.59e-02 5.51e-02 2.89e-01 1.72e-01 2.98e-01   ph/cm2/s
 
Fluence   Cutoff-PL 1.92e-08 5.60e-08 1.22e-07 4.33e-07 3.12e-07 6.31e-07   erg/cm2
              Error 5.16e-09 7.48e-09 1.48e-08 3.21e-07 3.57e-08 2.59e-07   erg/cm2
Peak flux Cutoff-PL 2.01e-01 3.14e-01 3.68e-01 8.31e-01 1.13e+00 1.71e+00   ph/cm2/s
              Error 6.13e-02 6.07e-02 6.29e-02 3.45e-01 1.73e-01 4.21e-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    0.900    0.174    -      -           7.59e-03 7.52e-04   45.040 57
CPL   0.595    0.572     263.3    0.0      1.04e-02 7.45e-03   44.420 56
 
 
=== 1-s peak spectral analysis ===
 
Model Ph_index Ph_90err Epeak  Epeak_90err Norm     Nomr_90err chi2   dof
PL    0.770    0.278    -      -           9.78e-03 1.54e-03   44.710 57
CPL   0.765    0.307    9999.2    0.0      9.85e-03 9.67e-03   44.710 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: 3.392000 sec.
T50 in the 50-300 keV band: 1.856000 sec.

 
=== Table of the duration information ==
 
        Value   tstart    tstop
T100    3.736   -1.356    2.380
T90     3.436   -1.252    2.184
T50     1.648   -0.008    1.640
Peak    1.000   -0.048    0.952

Click here for the BAT GCN circular template

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
  269.3593    46.0473   0.0127    15.4453    42.2249         0.4180388     15.022 TRIG_00933515                 
 
Foreground time interval of the image:
 -1.356   2.380 (delta_t =   3.736 [sec])
Background time interval of the image:
-255.275  -1.356 (delta_t = 253.919 [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

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.512000

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 0.512000

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 0.512000

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   -1.356 sec. to    2.380 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 0.899935     ( -0.177779   0.170793 )
Norm@50keV  : 7.58511E-03    ( -0.000754777   0.000749447 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          45.04 using 59 PHA bins.
# Reduced chi-squared =         0.7901 for     57 degrees of freedom 
# Null hypothesis probability =   8.742222e-01
 
Photon flux (15-150 keV)    in 3.736 sec: 0.870592 ( -0.086489  0.08674 ) ph/cm2/s
Energy fluence (15-150 keV)             : 3.18073e-07 ( -3.29666e-08  3.31451e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from   -1.356 sec. to    2.380 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 0.594798     ( -0.758631   0.386119 )
Epeak [keV] : 263.338      ( -263.34 -263.34 )
Norm@50keV  : 1.03824E-02    ( -0.00339088   0.0115012 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          44.42 using 59 PHA bins.
# Reduced chi-squared =         0.7933 for     56 degrees of freedom 
# Null hypothesis probability =   8.677069e-01
 
Photon flux (15-150 keV)    in 3.736 sec: 0.859520 ( -0.089846  0.089876 ) ph/cm2/s
Energy fluence (15-150 keV)             : 3.12491e-07 ( -3.60404e-08  3.53473e-08 ) ergs/cm2

Band function

Time interval is from   -1.356 sec. to    2.380 sec.
 
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       :    (     )
beta        :     (     )
Epeak [keV] :       (   )
Norm@50keV   :     (     )
------------------------------------------------------------
 
Photon flux (15-150 keV)    in  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]    : 22.9660  (-3.05942  3.78692)
R^2/D10^2   : 2.75637E-02  (-0.0102565   0.0155051)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          58.50 using 59 PHA bins.
# Reduced chi-squared =          1.026 for     57 degrees of freedom 
# Null hypothesis probability =   4.201221e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  9.850e-09   1.900e-09
25- 50  5.340e-08   8.238e-09
50-150  2.104e-07   3.729e-08
15-150  2.736e-07   3.531e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 200.000       (-17.191      -200)
Norm        : 3.51859       (-0.359853     0.359853)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          82.68 using 59 PHA bins.
# Reduced chi-squared =          1.450 for     57 degrees of freedom 
# Null hypothesis probability =   1.474318e-02
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  3.272e-08   1.706e-08
25- 50  6.294e-08   2.340e-08
50-150  1.380e-07   7.493e-08
15-150  2.337e-07   1.270e-07

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 8.04744E-02        (0.822496      -0.0804744)
R1^2/D10^2  : 4.78220E+17        (-4.7822e+17      -4.7822e+17)
kT2 [keV]   : 22.9726        (-3.06126      3.78507)
R2^2/D10^2  : 2.75399E-02    (-0.0102567   0.0155087)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          58.50 using 59 PHA bins.
# Reduced chi-squared =          1.064 for     55 degrees of freedom 
# Null hypothesis probability =   3.482216e-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   -0.048 sec. to    0.952 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 0.770450     ( -0.288489   0.266657 )
Norm@50keV  : 9.78014E-03    ( -0.00155785   0.00152135 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          44.71 using 59 PHA bins.
# Reduced chi-squared =         0.7845 for     57 degrees of freedom 
# Null hypothesis probability =   8.813884e-01
 
Photon flux (15-150 keV)    in 1 sec: 1.12543 ( -0.171089  0.1722 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.15744e-07 ( -1.80158e-08  1.81281e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from   -0.048 sec. to    0.952 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 0.764559     ( -0.346776   0.267689 )
Epeak [keV] : 9999.19      ( -9999.32 -9999.32 )
Norm@50keV  : 9.85439E-03    ( -0.00146476   0.0178813 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          44.71 using 59 PHA bins.
# Reduced chi-squared =         0.7985 for     56 degrees of freedom 
# Null hypothesis probability =   8.607360e-01
 
Photon flux (15-150 keV)    in 1 sec: 1.12552 ( -0.174944  0.17087 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.15776e-07 ( -1.89527e-08  1.69848e-08 ) ergs/cm2

Band function

Time interval is from   -0.048 sec. to    0.952 sec.
 
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       :    (     )
beta        :     (     )
Epeak [keV] :       (   )
Norm@50keV   :     (     )
------------------------------------------------------------
 
Photon flux (15-150 keV)    in  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]    : 26.4764  (-5.63269  8.32639)
R^2/D10^2   : 2.38036E-02  (-0.0128486   0.0250011)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          52.46 using 59 PHA bins.
# Reduced chi-squared =         0.9204 for     57 degrees of freedom 
# Null hypothesis probability =   6.458178e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  2.809e-09   9.800e-10
25- 50  1.640e-08   4.728e-09
50-150  8.435e-08   2.525e-08
15-150  1.035e-07   2.369e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 200.000       (-32.0395      -200)
Norm        : 4.46402       (-0.714004     0.714004)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          67.40 using 59 PHA bins.
# Reduced chi-squared =          1.182 for     57 degrees of freedom 
# Null hypothesis probability =   1.631040e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.111e-08   6.385e-09
25- 50  2.137e-08   1.214e-08
50-150  4.688e-08   2.677e-08
15-150  7.936e-08   4.494e-08

Double BB

------------------------------------------------------------
#Fit statistic : Chi-Squared =          49.38 using 59 PHA bins.
#Fit statistic : Chi-Squared =          48.63 using 59 PHA bins.
#Fit statistic : Chi-Squared =          48.59 using 59 PHA bins.
#Fit statistic : Chi-Squared =          48.58 using 59 PHA bins.
# Reduced chi-squared =         0.8979 for     55 degrees of freedom 
# Reduced chi-squared =         0.8841 for     55 degrees of freedom 
# Reduced chi-squared =         0.8835 for     55 degrees of freedom 
# Reduced chi-squared =         0.8832 for     55 degrees of freedom 
# Null hypothesis probability =   6.881526e-01
# Null hypothesis probability =   7.151680e-01
# Null hypothesis probability =   7.163438e-01
# Null hypothesis probability =   7.169789e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  2.992e-09   9.365e-10
25- 50  1.590e-08   3.825e-09
50-150  8.528e-08   2.381e-08
15-150  1.042e-07   2.770e-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: 0.899935     ( -0.177779   0.170793 )
Norm@50keV  : 7.58511E-03    ( -0.000754777   0.000749447 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          45.04 using 59 PHA bins.
# Reduced chi-squared =         0.7901 for     57 degrees of freedom 
# Null hypothesis probability =   8.742222e-01
 
Photon flux (15-150 keV)    in 3.736 sec: 0.870600 ( -0.0864854  0.0867333 ) ph/cm2/s
Energy fluence (15-150 keV)             : 3.18033e-07 ( -3.29561e-08  3.31566e-08 ) ergs/cm2

Cutoff power-law model

Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 0.594767     ( -0.758623   0.386178 )
Epeak [keV] : 263.308      ( -263.339 -263.339 )
Norm@50keV  : 1.03828E-02    ( -0.00339088   0.0115011 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          44.42 using 59 PHA bins.
# Reduced chi-squared =         0.7933 for     56 degrees of freedom 
# Null hypothesis probability =   8.677069e-01
 
Photon flux (15-150 keV)    in 3.736 sec: 0.859493 ( -0.089827  0.08987 ) ph/cm2/s
Energy fluence (15-150 keV)             : 3.12639e-07 ( -3.60539e-08  3.53609e-08 ) ergs/cm2

Band function

 
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       :    (     )
beta        :     (     )
Epeak [keV] :       (   )
Norm@50keV   :     (     )
------------------------------------------------------------
 
Photon flux (15-150 keV)    in  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)  = 5.49e-08
S(50-100 keV) = 1.18e-07

T90 vs. Hardness ratio plot

T90                                   = 3.43599987030029 sec.
Hardness ratio (energy fluence ratio) = 2.14936

Color vs. Color plot

Count Ratio  (25-50 keV) / (15-25 keV) = 2.77669
Count Ratio (50-100 keV) / (15-25 keV) = 2.74278

Mask shadow pattern

IMX = 2.046010439575555E-01, IMY = -1.856828444633533E-01

TIME vs. PHA plot around the trigger time

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.512000

TIME vs. DetID plot around the trigger time

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.512000

100 us light curve (15-350 keV)

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.512000

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:
-255.275400 -1.356000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
254.4700  35.2473    1.9  11.1  -27.9   1.7257   6.2    5.7	Her X-1                       
268.5298  -1.4401    8.1  32.2 -148.6  -0.5673  -1.4    9.7	SW J1753.5-0127               
270.4356 -25.1158    6.6  56.0 -149.2   2.6191   1.8    8.5	GX 5-1                        
273.9642 -14.0594    4.9  45.4 -155.0   1.4597   2.4    2.8	GX 17+2                       
288.8617  10.8100   12.3  28.7  164.2  -0.3098  -0.9    8.9	GRS 1915+105                  
299.5563  35.1937    1.0  27.9  107.0   4.6540  11.4    1.7	Cyg X-1                       
308.2028  40.8826    3.6  34.9   96.4   1.8649   3.2    5.9	Cyg X-3                       
213.0592  68.5524    3.1  48.5   11.9   2.0388   3.7 ------	UNKNOWN                       
285.1331  -2.9833    2.9  38.1 -175.9   1.6024   3.9 ------	UNKNOWN                       
242.9187  22.8422    2.5  22.5  -69.8   1.6527   4.6 ------	UNKNOWN                       
209.8413  43.6866    3.3  46.1  -22.1   1.9984   3.5 ------	UNKNOWN                       
224.9744  26.7740    2.7  36.5  -50.6   2.0520   4.2 ------	UNKNOWN                       
267.9030 -23.6577    2.4  54.4 -146.4   6.8042   4.9 ------	UNKNOWN

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

Time interval of the image:
-1.356000 2.380000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
254.4590  35.3436 1190.8  11.2  -27.5  -0.0002  -0.0    0.1	Her X-1                       
268.3930  -1.2707    0.0  32.1 -148.4   0.0447   1.4   11.0	SW J1753.5-0127               
270.2303 -25.1237   31.8  56.0 -148.9  -0.0550  -0.4    4.0	GX 5-1                        
273.9449 -13.9059    8.0  45.2 -155.0  -0.0817  -1.4    8.6	GX 17+2                       
288.7308  10.7722   38.7  28.6  164.5   0.0095   0.3   11.1	GRS 1915+105                  
299.4602  35.0235    0.0  27.8  107.4   0.0490   1.3   12.5	Cyg X-1                       
308.2039  40.8408    6.8  34.9   96.5   0.0998   1.7    7.9	Cyg X-3                       
295.1017  25.9336    2.5  25.5  128.8   0.1527   4.7 ------	UNKNOWN                       
269.3593  46.0473    0.8  15.4   42.2   0.4181  15.0 ------	UNKNOWN

Post-slew image of 15-350 keV band

Time interval of the image:
54.124600 719.219200
720.224000 962.302000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
254.4813  35.3577    1.6  15.5  -85.7   6.4521   7.4    1.5	Her X-1                       
268.2480  -1.5230    7.7  47.6 -135.8  -4.2663  -1.5    8.3	SW J1753.5-0127               
288.8317  11.1021    4.5  38.7 -168.9   3.1589   2.6    9.6	GRS 1915+105                  
299.5940  35.1935    0.8  25.2  147.4  14.3810  15.4    0.5	Cyg X-1                       
308.1590  40.9529    1.6  28.3  128.9   7.5852   7.2    2.2	Cyg X-3                       
326.0507  38.2818    6.3  41.9  122.4   7.3496   1.8    6.2	Cyg X-2                       
123.7953  86.6736    4.1  46.7   40.2   6.3375   2.8 ------	UNKNOWN                       
292.6151  13.4441    4.1  38.1 -175.9   3.1052   2.8 ------	UNKNOWN

Plot creation:
Wed Nov 27 16:18:40 EST 2019