batgrbproduct analysis for trigger=1187225

batgrbproduct Analysis for Trigger=1187225

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 v2.48
    Process Start Time (local time): Sat Aug 26 19:38:09 EDT 2023
             Host Name: batproc1
   Current Working Dir: /local/data/bat1/prebascript/trigger1187225/GCN5_download_cron
======================================================================

  Trigger: 01187225      Segment: 000

  BAT Trigger Time: 714699144   [s; MET]
      Trigger Stop: 714699360   [s; MET]
               UTC: 2023-08-25T23:31:52.107840    [includes UTCF correction] 
       Where From?: TDRSS position message

  BAT 
    RA: 261.947481520388   Dec: -16.2178211607624  [deg; J2000]

     Catalogged Source?: YES
     Point Source?:      YES
     GRB Indicated?:     NO    [ by BAT flight software ]
     Image S/N Ratio:    31.44
     Image Trigger?:     YES
     Rate S/N Ratio:     0  [ if not an image trigger ]
     Image S/N Ratio:    31.44

  Flight Position:   [ source = BAT ]
    RA: 261.947481520388   Dec: -16.2178211607624  [deg; J2000]

  Ground Position:   [ source = BAT pre-slew burst ]
    RA: 261.939760486986   Dec: -16.2133893598014  [deg; J2000]  
        { 17h 27m 45.5s , -16d 12' 48.2" }
         +/- 0.598010675615263 [arcmin] (estimated 90% radius based on SNR)
         +/- 0.196341165275051 [arcmin] (formal 1-sigma fit error)
    SNR: 63.4023875995734
 
  Angular difference between Flight and Ground position is 0.518250 arcmin
 
  Partial Coding Fraction: 0.6640625    [ including projection effects ]

  Duration
     T90: 116.075999975204 +/- 4.4890231152698
        Measured from: -68.1039998531342
                   to: 47.9720001220703     [s; relative to TRIGTIME]
     T50: 57.0719999074936 +/- 6.23264822897981
        Measured from: -35.0839998722076
                   to: 21.9880000352859     [s; relative to TRIGTIME]



  Fluence
     Peak Flux  (peak 1 second)
        Measured from: -4.10800004005432     
                   to: -3.10800004005432     [s; relative to TRIGTIME]
     Total Fluence        
        Measured from: -71.8240000009537     
                   to: 174.468000054359     [s; relative to TRIGTIME]
     
             Band 1     Band 2     Band 3     Band 4
              15-25      25-50     50-100    100-350     keV
 Total    26.884458  21.227467   5.638664   0.409565
           0.166014   0.155622   0.116080   0.092324 [error]
 Peak      0.172129   0.143448   0.030497   0.007651
           0.011388   0.010415   0.007544   0.005815 [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 1.14e-05 8.95e-06 4.74e-06 3.64e-06 2.67e-05 2.87e-05   erg/cm2
              Error 4.11e-07 1.77e-07 1.37e-07 2.26e-07 5.50e-07 5.44e-07   erg/cm2
Peak flux Power-law 2.01e+00 9.98e-01 3.03e-01 1.17e-01 3.38e+00 3.43e+00   ph/cm2/s
              Error 2.37e-01 9.58e-02 5.88e-02 4.09e-02 3.05e-01 3.07e-01   ph/cm2/s
 
Fluence   Cutoff-PL 9.99e-06 9.29e-06 4.62e-06 1.51e-06 2.50e-05 2.54e-05   erg/cm2
              Error 5.30e-07 2.02e-07 1.54e-07 3.33e-07 7.02e-07 8.25e-07   erg/cm2
Peak flux Cutoff-PL 1.86e+00 1.12e+00 2.58e-01 2.22e-02 3.25e+00 3.25e+00   ph/cm2/s
              Error 2.67e-01 1.31e-01 7.88e-02 3.80e-02 3.17e-01 3.20e-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    2.918    0.041    -      -           1.00e-02 2.10e-04   95.980 57
CPL   1.984   -0.947       0.8    0.0      3.10e-02 1.36e-03   56.700 56
 
 
=== 1-s peak spectral analysis ===
 
Model Ph_index Ph_90err Epeak  Epeak_90err Norm     Nomr_90err chi2   dof
PL    2.718    0.198    -      -           1.50e-02 2.20e-03   74.510 57
CPL   1.493    0.850      14.9   12.2      8.75e-02 0.00e+00   68.990 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  246.292  -71.824  174.468
T90   116.076  -68.104   47.972
T50    57.072  -35.084   21.988
Peak    1.000   -4.108   -3.108

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
  261.9398 -16.2134 0.0030   30.7 -142.6      46.1274    63.4  TRIG_01187225       
------------------------------------------
 
Foreground time interval of the image:
-13.699  35.830 (delta_t =  49.529 [sec])
 37.000 102.260 (delta_t =  65.260 [sec])
103.000 174.468 (delta_t =  71.468 [sec])
Background time interval of the image:

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 216.000000

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 216.000000

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 216.000000

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

Multiple GTIs in the spectrum
tstart tstop
-71.824000 -56.795800
-42.000000 35.830000
37.000000 102.260000
103.000000 174.468000
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 2.91820     ( -0.0414084   0.0415888 )
Norm@50keV  : 1.00458E-02    ( -0.000210132   0.000209567 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          95.98 using 59 PHA bins.
# Reduced chi-squared =          1.684 for     57 degrees of freedom 
# Null hypothesis probability =   9.492130e-04
 
Photon flux (15-150 keV)    in 229.6 sec: 2.60482 ( -0.0713196  0.0720277 ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.67211e-05 ( -5.4885e-07  5.50689e-07 ) ergs/cm2

Cutoff power-law model

Multiple GTIs in the spectrum
tstart tstop
-71.824000 -56.795800
-42.000000 35.830000
37.000000 102.260000
103.000000 174.468000
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.98428     ( -0.0894332   -1.98428 )
Epeak [keV] : 0.751808      ( -0.039258 0.041974 )
Norm@50keV  : 3.10184E-02    ( -0.00109997   0.00162011 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          56.70 using 59 PHA bins.
# Reduced chi-squared =          1.013 for     56 degrees of freedom 
# Null hypothesis probability =   4.486035e-01
 
Photon flux (15-150 keV)    in 229.6 sec: 2.39801 ( -0.08631  0.08746 ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.49552e-05 ( -6.99591e-07  7.04413e-07 ) ergs/cm2

Band function

Multiple GTIs in the spectrum
tstart tstop
-71.824000 -56.795800
-42.000000 35.830000
37.000000 102.260000
103.000000 174.468000
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -1.75065   (     )
beta        : -8.24944    (     )
Epeak [keV] : 12.1064      (   )
Norm@50keV   : 3.18068E-02    (     )
------------------------------------------------------------
#Fit statistic : Chi-Squared =         130.70 using 59 PHA bins.
# Reduced chi-squared =         2.3764 for     55 degrees of freedom 
# Null hypothesis probability =   4.187461e-08
 
Photon flux (15-150 keV)    in 229.6 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]    : 8.70090  (  )
R^2/D10^2   : 1.48391  (   )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =         513.75 using 59 PHA bins.
# Reduced chi-squared =         9.0131 for     57 degrees of freedom 
# Null hypothesis probability =   9.966982e-75
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  4.930e-06   2.043e-07
25- 50  9.931e-06   1.894e-07
50-150  3.413e-06   1.481e-07
15-150  1.827e-05   3.765e-07

Thermal bremsstrahlung (OTTB)

XSPEC12>exit
 XSPEC: quit
 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 29.4209       (-1.05402      1.10966)
Norm        : 18.1998       (-0.940824     0.990832)
------------------------------------------------------------
 Reduced chi-squared = 
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  8.419e-06   2.973e-07
25- 50  9.516e-06   1.975e-07
50-150  5.079e-06   2.078e-07
15-150  2.302e-05   4.512e-07

Double BB

XSPEC12>exit
 XSPEC: quit
 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 6.04578        (-0.295833      0.289018)
R1^2/D10^2  : 6.46558        (-1.16888      1.55227)
kT2 [keV]   : 17.4808        (-1.40769      1.65342)
R2^2/D10^2  : 3.55428E-02    (-0.0123532   0.0180271)
------------------------------------------------------------
 Reduced chi-squared = 
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  7.792e-06   4.799e-07
25- 50  9.668e-06   3.054e-07
50-150  5.712e-06   4.339e-07
15-150  2.317e-05   8.576e-07

Peak spectrum fit

Power-law model

Time interval is from   -4.108 sec. to   -3.108 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 2.71777     ( -0.190554   0.205873 )
Norm@50keV  : 1.49731E-02    ( -0.00221229   0.00219625 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          74.51 using 59 PHA bins.
# Reduced chi-squared =          1.307 for     57 degrees of freedom 
# Null hypothesis probability =   5.961953e-02
 
Photon flux (15-150 keV)    in 1 sec: 3.38147 ( -0.304513  0.304824 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.60288e-07 ( -1.60165e-08  1.62745e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from   -4.108 sec. to   -3.108 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.49341     ( -1.20945   0.490333 )
Epeak [keV] : 14.8801      ( -13.7631 10.6539 )
Norm@50keV  : 8.75076E-02    (     )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          68.99 using 59 PHA bins.
# Reduced chi-squared =          1.232 for     56 degrees of freedom 
# Null hypothesis probability =   1.140749e-01
 
Photon flux (15-150 keV)    in 1 sec: 3.25188 ( -0.31706  0.31788 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.47584e-07 ( -1.657e-08  1.7277e-08 ) ergs/cm2

Band function

Time interval is from   -4.108 sec. to   -3.108 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -1.49456   ( -0.531911   2.74019 )
beta        : -10.0000    ( 10   1.77636e-15 )
Epeak [keV] : 14.8567      ( -8.10067 10.6601 )
Norm@50keV   : 8.73536E-02    ( -0.050585   0.442564 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          68.99 using 59 PHA bins.
# Reduced chi-squared =          1.254 for     55 degrees of freedom 
# Null hypothesis probability =   9.730352e-02
 
Photon flux (15-150 keV)    in 1 sec:  (    ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.48549e-07 ( 0  0 ) ergs/cm2

Single BB

 XSPEC: quit
 
 
Spectral model blackbody:
------------------------------------------------------------
Parameters  : value    Lower 90%  Upper 90%
kT [keV]    : 7.05133  (-0.653562  0.709924)
R^2/D10^2   : 5.96783  (-2.03314   3.15863)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
 Reduced chi-squared = 
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  4.803e-08   7.390e-09
25- 50  6.671e-08   8.680e-09
50-150  1.135e-08   3.784e-09
15-150  1.261e-07   1.395e-08

Thermal bremsstrahlung (OTTB)

XSPEC12>exit
 XSPEC: quit
 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 27.2191       (-4.79649      6.05532)
Norm        : 29.1968       (-5.52421     7.15638)
------------------------------------------------------------
 Reduced chi-squared = 
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  5.634e-08   6.840e-09
25- 50  6.088e-08   6.385e-09
50-150  2.923e-08   9.065e-09
15-150  1.464e-07   1.540e-08

Double BB

XSPEC12>exit
 XSPEC: quit
 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 4.82931        (-3.29999      1.44353)
R1^2/D10^2  : 21.6899        (-12.9773      19726.9)
kT2 [keV]   : 12.2078        (-4.60377      8.69438)
R2^2/D10^2  : 0.317852    (-0.289684   0.546799)
------------------------------------------------------------
 Reduced chi-squared = 
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  5.584e-08   2.950e-08
25- 50  5.964e-08   2.752e-08
50-150  3.013e-08   1.747e-08
15-150  1.456e-07   7.380e-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: 2.91827     ( -0.0419793   0.0421967 )
Norm@50keV  : 1.02588E-02    ( -0.000219854   0.000219225 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =         101.32 using 59 PHA bins.
# Reduced chi-squared =         1.7776 for     57 degrees of freedom 
# Null hypothesis probability =   2.750623e-04
 
Photon flux (15-150 keV)    in 186.3 sec: 2.66020 ( -0.0731797  0.0739059 ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.21423e-05 ( -4.58509e-07  4.60008e-07 ) ergs/cm2

Cutoff power-law model

Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.98416     ( -0.139836   -1.98416 )
Epeak [keV] : 0.755378      ( -0.0396667 0.0426595 )
Norm@50keV  : 3.17934E-02    ( -0.000599668   0.00171338 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          49.35 using 59 PHA bins.
# Reduced chi-squared =         0.8813 for     56 degrees of freedom 
# Null hypothesis probability =   7.228460e-01
 
Photon flux (15-150 keV)    in 186.3 sec: 2.42041 ( -0.08858  0.0898 ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.04889e-05 ( -5.82933e-07  5.8759e-07 ) ergs/cm2

Band function

 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -1.15906   ( -0.474237   0.83407 )
beta        : -3.24211    ( -0.152861   0.111265 )
Epeak [keV] : 18.0697      ( -9.36781 4.83495 )
Norm@50keV   : 0.108017    ( -0.0615772   0.279437 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          36.70 using 59 PHA bins.
# Reduced chi-squared =         0.6673 for     55 degrees of freedom 
# Null hypothesis probability =   9.726882e-01
 
Photon flux (15-150 keV)    in 186.3 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)  = 8.95e-06
S(50-100 keV) = 4.74e-06

T90 vs. Hardness ratio plot

T90                                   = 116.075999975204 sec.
Hardness ratio (energy fluence ratio) = 0.529609

Color vs. Color plot

Count Ratio  (25-50 keV) / (15-25 keV) = 0.789581
Count Ratio (50-100 keV) / (15-25 keV) = 0.209737

Mask shadow pattern

IMX = -4.721665436117246E-01, IMY = 3.609669977645035E-01

TIME vs. PHA plot around the trigger time

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 216.000000

TIME vs. DetID plot around the trigger time

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 216.000000

100 us light curve (15-350 keV)

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 216.000000

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:
-10.000000 -4.292000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
245.0755 -15.5633    3.9  44.0 -126.7   0.3650   2.9    7.2	Sco X-1                       
254.4754  35.3491  113.2  40.6  -46.1   0.0079   0.1    1.0	Her X-1                       
256.0454 -37.8627   14.8  50.5 -158.9   0.0716   0.8    3.0	4U 1700-377                   
256.3296 -36.5207    7.4  49.3 -158.1   0.1306   1.6    7.8	GX 349+2                      
263.1127 -24.6216    3.3  36.3 -154.2   0.1714   3.5    9.3	GX 1+4                        
264.8683 -44.4797    6.3  52.7 -170.5   0.1752   1.8    5.7	4U 1735-44                    
268.2346  -1.3025   34.9  17.2 -119.9  -0.0137  -0.3   12.0	SW J1753.5-0127               
270.4336 -25.0254    5.9  33.2 -164.6   0.0861   2.0    8.7	GX 5-1                        
270.1579 -25.7644   16.7  33.9 -164.8  -0.0311  -0.7    7.9	GRS 1758-258                  
274.0063 -14.0363  190.6  21.8 -160.4   0.0022   0.1    0.0	GX 17+2                       
276.0540 -30.2349    3.4  36.4 -175.9   0.1735   3.4   10.4	H1820-303                     
285.1662 -24.7933    4.3  30.1  170.4  -0.1184  -2.7   10.4	HT1900.1-2455                 
288.7629  10.9357   11.8   7.2   31.2   0.0340   1.0    2.2	GRS 1915+105                  
299.7272  35.1712    2.8  33.1   16.0   0.1961   4.1    7.0	Cyg X-1                       
308.0222  41.0444    2.8  41.6   19.7   0.2804   4.1    6.8	Cyg X-3                       
326.1941  38.2859   15.5  50.4   35.4   0.1585   0.7    2.4	Cyg X-2                       
262.9523 -33.9575    5.8  44.1 -162.2  -0.1246  -2.0    7.6	GX 354-0                      
262.0032 -16.2030    0.3  30.7 -142.6   1.6378  34.1 ------	UNKNOWN

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

Time interval of the image:
-13.699380 35.830000
37.000000 102.260000
103.000000 174.468000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
244.9549 -15.6151    2.9  44.0 -126.7   7.0210   3.9    2.1	Sco X-1                       
254.2961  35.3377  267.0  40.6  -46.1   0.0475   0.0    7.9	Her X-1                       
256.0993 -37.9897    8.3  50.5 -159.1   1.9202   1.4   10.2	4U 1700-377                   
256.3524 -36.5351    7.0  49.2 -158.1   2.1292   1.7    7.8	GX 349+2                      
263.1490 -24.6309    6.4  36.2 -154.4   1.3922   1.8   10.3	GX 1+4                        
264.8777 -44.4373   15.9  52.7 -170.5   1.1213   0.7    5.8	4U 1735-44                    
268.5016  -1.5998   15.0  17.0 -121.3  -0.4609  -0.8   11.9	SW J1753.5-0127               
270.3775 -25.1437    5.4  33.3 -164.7   1.4293   2.1    6.4	GX 5-1                        
270.4362 -25.7978   23.5  33.8 -165.3   0.3461   0.5    7.9	GRS 1758-258                  
274.1161 -14.0546    5.3  21.8 -160.8   1.1800   2.2    6.5	GX 17+2                       
276.0341 -30.5351  175.5  36.7 -176.1   0.0525   0.1   11.6	H1820-303                     
285.2046 -24.7867    0.0  30.1  170.3  -1.4307  -1.9   12.2	HT1900.1-2455                 
288.9533  10.9562   35.0   7.4   32.7  -0.1675  -0.3    9.2	GRS 1915+105                  
299.5898  35.2294    1.4  33.1   15.9   6.5678   8.2    1.7	Cyg X-1                       
308.0048  41.1437    0.0  41.7   19.6   1.2841   1.2   12.4	Cyg X-3                       
326.2852  38.3978   13.7  50.5   35.3  -2.6858  -0.8    7.0	Cyg X-2                       
263.0224 -33.7447   12.9  43.9 -162.2   0.8070   0.9    5.7	GX 354-0                      
323.3555  -5.9901    3.0  40.8   97.9   7.7030   3.8 ------	UNKNOWN                       
324.8528   3.6386    3.7  40.7   82.9   6.6599   3.1 ------	UNKNOWN                       
304.4843  44.9711    2.8  43.5   13.3   4.9677   4.1 ------	UNKNOWN                       
267.4969 -51.2032    3.5  58.3 -175.6  11.1147   3.3 ------	UNKNOWN                       
	UNKNOWN                       
	UNKNOWN                       
	UNKNOWN                       
	UNKNOWN

Post-slew image of 15-350 keV band

Time interval of the image:
-60.000000 -56.795800
-10.000000 35.830000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
244.9544 -15.5449    5.8  44.1 -126.8   1.0191   2.0    5.9	Sco X-1                       
254.6243  35.3622    5.4  40.4  -46.0   0.6759   2.1    8.2	Her X-1                       
256.1157 -37.8691    4.8  50.5 -159.1   0.9418   2.4    6.3	4U 1700-377                   
256.3456 -36.4048    3.9  49.2 -158.1   1.0591   2.9    4.5	GX 349+2                      
262.9992 -24.8593    3.2  36.6 -154.5  -0.8001  -3.7    6.8	GX 1+4                        
264.7482 -44.3120    5.9  52.7 -170.4   0.8435   2.0    8.3	4U 1735-44                    
268.5247  -1.3821    9.7  17.0 -120.9  -0.2044  -1.2   10.3	SW J1753.5-0127               
270.1434 -25.0727    5.2  33.4 -164.4   0.4339   2.2    7.7	GX 5-1                        
270.1863 -25.5672    0.0  33.8 -164.8  -0.2971  -1.5   12.3	GRS 1758-258                  
274.1341 -13.9588    4.0  21.8 -160.8   0.4450   2.9    8.8	GX 17+2                       
275.9128 -30.5175   15.0  36.8 -175.9  -0.1769  -0.8    9.1	H1820-303                     
285.0356 -24.9208   36.4  30.4  170.6   0.0693   0.3    0.0	HT1900.1-2455                 
288.7717  10.8434   16.5   7.1   32.5  -0.1068  -0.7    6.3	GRS 1915+105                  
299.6585  35.3068    1.7  33.2   15.9   1.5277   6.9    7.1	Cyg X-1                       
308.1297  40.9260   99.4  41.5   20.0  -0.0350  -0.1    1.8	Cyg X-3                       
326.0694  38.4886  151.1  50.4   35.1   0.0740   0.1   11.1	Cyg X-2                       
262.9518 -33.8720   15.2  44.1 -162.2  -0.2076  -0.8    2.9	GX 354-0                      
311.8317  55.1459    2.9  54.5   11.4   3.3352   4.0 ------	UNKNOWN                       
261.9470 -16.1147    0.2  30.7 -142.6  11.5204  58.7 ------	UNKNOWN                       
259.9468   1.0536    2.8  24.5 -107.2   0.8286   4.1 ------	UNKNOWN                       
249.5256 -31.7410    2.2  49.6 -148.5   2.0962   5.2 ------	UNKNOWN

Plot creation:
Sat Aug 26 19:40:11 EDT 2023