batgrbproduct analysis for trigger=1218967

batgrbproduct Analysis for Trigger=1218967

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): Thu Mar  7 07:06:09 EST 2024
             Host Name: batproc1
   Current Working Dir: /local/data/bat1/prebascript/trigger1218967/GCN5_download_cron
======================================================================

  Trigger: 01218967      Segment: 000

  BAT Trigger Time: 731420376   [s; MET]
      Trigger Stop: 731420440   [s; MET]
               UTC: 2024-03-06T12:19:02.962900    [includes UTCF correction] 
       Where From?: TDRSS position message

  BAT 
    RA: 299.313254986747   Dec: 35.2294425424692  [deg; J2000]

     Catalogged Source?: NO
     Point Source?:      YES
     GRB Indicated?:     YES    [ by BAT flight software ]
     Image S/N Ratio:    13.7
     Image Trigger?:     YES
     Rate S/N Ratio:     0  [ if not an image trigger ]
     Image S/N Ratio:    13.7

  Flight Position:   [ source = BAT ]
    RA: 299.313254986747   Dec: 35.2294425424692  [deg; J2000]

  Ground Position:   [ source = BAT pre-slew burst ]
    RA: 299.170408996303   Dec: 35.269222818869  [deg; J2000]  
        { 19h 56m 40.9s , +35d 16' 09.2" }
         +/- 3.33070186561729 [arcmin] (estimated 90% radius based on SNR)
         +/- 2.49128002932106 [arcmin] (formal 1-sigma fit error)
    SNR: 5.45304048970484
 
  Angular difference between Flight and Ground position is 7.395068 arcmin
 
  Partial Coding Fraction: 0.984375    [ including projection effects ]

  Duration
     T90: 204.031999826431 +/- 24.9145227511739
        Measured from: -6.7519998550415
                   to: 197.27999997139     [s; relative to TRIGTIME]
     T50: 104.767999887466 +/- 31.9188090033259
        Measured from: 35.296000123024
                   to: 140.06400001049     [s; relative to TRIGTIME]



  Fluence
     Peak Flux  (peak 1 second)
        Measured from: 106.764000058174     
                   to: 107.764000058174     [s; relative to TRIGTIME]
     Total Fluence        
        Measured from: -22.3680000305176     
                   to: 203.871999979019     [s; relative to TRIGTIME]
     
             Band 1     Band 2     Band 3     Band 4
              15-25      25-50     50-100    100-350     keV
 Total     2.828348   3.194260   1.949277   0.290226
           0.100113   0.101187   0.084907   0.070420 [error]
 Peak      0.032316   0.031269   0.017219   0.006063
           0.006615   0.006535   0.005548   0.004554 [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 8.77e-07 1.34e-06 1.52e-06 3.32e-06 4.73e-06 7.06e-06   erg/cm2
              Error 6.00e-08 5.38e-08 8.62e-08 4.06e-07 2.00e-07 4.71e-07   erg/cm2
Peak flux Power-law 3.19e-01 2.36e-01 1.16e-01 8.07e-02 7.09e-01 7.51e-01   ph/cm2/s
              Error 9.37e-02 5.19e-02 4.38e-02 5.77e-02 1.54e-01 1.67e-01   ph/cm2/s
 
Fluence   Cutoff-PL 8.52e-07 1.36e-06 1.53e-06 2.50e-06 4.65e-06 6.25e-06   erg/cm2
              Error 7.14e-08 6.34e-08 8.92e-08 9.29e-07 2.34e-07 9.84e-07   erg/cm2
Peak flux Cutoff-PL 3.04e-01 2.55e-01 1.14e-01 3.38e-02 6.97e-01 7.07e-01   ph/cm2/s
              Error 1.02e-01 6.95e-02 5.12e-02 5.48e-02 1.17e-01 1.77e-01   ph/cm2/s
 
Fluence        Band 8.25e-07 1.37e-06 1.51e-06 2.99e-06 4.64e-06 6.70e-06   erg/cm2
              Error -------- -------- 9.12e-08 -------- -------- --------   erg/cm2
Peak flux      Band 3.07e-01 2.50e-01 1.17e-01 4.65e-02 7.03e-01 7.22e-01   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    1.809    0.075    -      -           2.28e-03 9.46e-05   54.370 57
CPL   1.632    0.268     100.2  -32.0      2.82e-03 8.91e-04   53.240 56
 
 
=== 1-s peak spectral analysis ===
 
Model Ph_index Ph_90err Epeak  Epeak_90err Norm     Nomr_90err chi2   dof
PL    2.026    0.413    -      -           4.67e-03 1.35e-03   78.220 57
CPL   1.386    1.416      39.1    0.0      1.12e-02 0.00e+00   77.680 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  226.240  -22.368  203.872
T90   204.032   -6.752  197.280
T50   104.768   35.296  140.064
Peak    1.000  106.764  107.764

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
  299.1704 +35.2692 0.0351   21.2 -176.5       1.2159     5.5  TRIG_01218967       
------------------------------------------
 
Foreground time interval of the image:
-22.368  27.560 (delta_t =  49.928 [sec])
 29.000  71.301 (delta_t =  42.301 [sec])
Background time interval of the image:
-60.000 -55.198 (delta_t =   4.802 [sec])
-54.000 -22.368 (delta_t =  31.632 [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 64.000000

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 64.000000

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 64.000000

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
-22.368000 27.560000
29.000000 203.872000
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.80935     ( -0.0749223   0.0756047 )
Norm@50keV  : 2.28497E-03    ( -9.4811e-05   9.43857e-05 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          54.37 using 59 PHA bins.
# Reduced chi-squared =         0.9538 for     57 degrees of freedom 
# Null hypothesis probability =   5.744099e-01
 
Photon flux (15-150 keV)    in 224.8 sec: 0.316012 ( -0.0130919  0.0131278 ) ph/cm2/s
Energy fluence (15-150 keV)             : 4.72732e-06 ( -1.99475e-07  2.00258e-07 ) ergs/cm2

Cutoff power-law model

Multiple GTIs in the spectrum
tstart tstop
-22.368000 27.560000
29.000000 203.872000
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.63163     ( -0.303054   0.232983 )
Epeak [keV] : 100.189      ( -36.1186 -100.196 )
Norm@50keV  : 2.81805E-03    ( -0.000603282   0.00117947 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          53.24 using 59 PHA bins.
# Reduced chi-squared =         0.9508 for     56 degrees of freedom 
# Null hypothesis probability =   5.798198e-01
 
Photon flux (15-150 keV)    in 224.8 sec: 0.312169 ( -0.01436  0.014385 ) ph/cm2/s
Energy fluence (15-150 keV)             : 4.65242e-06 ( -2.34242e-07  2.33297e-07 ) ergs/cm2

Band function

Multiple GTIs in the spectrum
tstart tstop
-22.368000 27.560000
29.000000 203.872000
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : 0.966883   ( 0.100168   0.100168 )
beta        : -1.85439    ( 1.85548   0.0933074 )
Epeak [keV] : 26.1675      ( -29.3001 37.2966 )
Norm@50keV   : 0.276509    ( -0.275074   214.163 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          52.08 using 59 PHA bins.
# Reduced chi-squared =         0.9470 for     55 degrees of freedom 
# Null hypothesis probability =   5.867537e-01
 
Photon flux (15-150 keV)    in 224.8 sec:  (    ) ph/cm2/s
Energy fluence (15-150 keV)             : 4.64309e-06 ( 0  0 ) ergs/cm2

Single BB

 
Spectral model blackbody:
------------------------------------------------------------
Parameters  : value    Lower 90%  Upper 90%
kT [keV]    : 12.5975  (  )
R^2/D10^2   : 6.00493E-02  (   )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =         207.41 using 59 PHA bins.
# Reduced chi-squared =         3.6387 for     57 degrees of freedom 
# Null hypothesis probability =   5.881542e-19
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  4.543e-07   3.260e-08
25- 50  1.512e-06   6.856e-08
50-150  1.488e-06   1.288e-07
15-150  3.454e-06   1.551e-07

Thermal bremsstrahlung (OTTB)

XSPEC12>exit
 XSPEC: quit
 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 107.464       (-15.8758      21.0055)
Norm        : 1.34847       (-0.0786547     0.0856101)
------------------------------------------------------------
 Reduced chi-squared = 
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  7.920e-07   6.025e-08
25- 50  1.389e-06   7.520e-08
50-150  2.342e-06   6.098e-07
15-150  4.523e-06   6.362e-07

Double BB

XSPEC12>exit
 XSPEC: quit
 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 6.65250        (-0.846525      0.903136)
R1^2/D10^2  : 0.456163        (-0.162541      0.29329)
kT2 [keV]   : 24.1992        (-3.37519      4.90995)
R2^2/D10^2  : 4.06321E-03    (-0.00199541   0.00319143)
------------------------------------------------------------
 Reduced chi-squared = 
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  7.839e-07   1.016e-07
25- 50  1.381e-06   1.225e-07
50-150  2.415e-06   4.621e-07
15-150  4.580e-06   4.946e-07

Peak spectrum fit

Power-law model

Time interval is from  106.764 sec. to  107.764 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 2.02637     ( -0.385056   0.440878 )
Norm@50keV  : 4.66608E-03    ( -0.00138295   0.00132117 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          78.22 using 59 PHA bins.
# Reduced chi-squared =          1.372 for     57 degrees of freedom 
# Null hypothesis probability =   3.257825e-02
 
Photon flux (15-150 keV)    in 1 sec: 0.708534 ( -0.153927  0.153928 ) ph/cm2/s
Energy fluence (15-150 keV)             : 4.30964e-08 ( -1.14355e-08  1.19919e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from  106.764 sec. to  107.764 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.38619     ( -2.0802   0.751518 )
Epeak [keV] : 39.1283      (   )
Norm@50keV  : 1.11572E-02    (     )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          77.68 using 59 PHA bins.
# Reduced chi-squared =          1.387 for     56 degrees of freedom 
# Null hypothesis probability =   2.917726e-02
 
Photon flux (15-150 keV)    in 1 sec: 0.697352 ( -0.155192  0.078202 ) ph/cm2/s
Energy fluence (15-150 keV)             : 4.0637e-08 ( -1.17732e-08  1.31799e-08 ) ergs/cm2

Band function

Time interval is from  106.764 sec. to  107.764 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -1.38422   ( -1.19823   2.32258 )
beta        : -10.0000    ( 10   3.55271e-15 )
Epeak [keV] : 39.1101      ( -27.2534 -39.1101 )
Norm@50keV   : 1.11877E-02    ( -0.0111877   0.199446 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          77.68 using 59 PHA bins.
# Reduced chi-squared =          1.412 for     55 degrees of freedom 
# Null hypothesis probability =   2.367977e-02
 
Photon flux (15-150 keV)    in 1 sec: 0.703091 (    ) ph/cm2/s
Energy fluence (15-150 keV)             : 4.06757e-08 ( 0  0 ) ergs/cm2

Single BB

 XSPEC: quit
 
 
Spectral model blackbody:
------------------------------------------------------------
Parameters  : value    Lower 90%  Upper 90%
kT [keV]    : 9.47557  (-2.44492  3.13454)
R^2/D10^2   : 0.408943  (-0.269986   0.86892)
(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  7.325e-09   4.067e-09
25- 50  1.684e-08   6.433e-09
50-150  7.505e-09   4.349e-09
15-150  3.167e-08   1.188e-08

Thermal bremsstrahlung (OTTB)

XSPEC12>exit
 XSPEC: quit
 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 62.0080       (-28.8092      81.5282)
Norm        : 3.69263       (-1.1101     1.68477)
------------------------------------------------------------
 Reduced chi-squared = 
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  9.328e-09   3.004e-09
25- 50  1.434e-08   4.416e-09
50-150  1.676e-08   1.114e-08
15-150  4.043e-08   1.667e-08

Double BB

XSPEC12>exit
 XSPEC: quit
 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 5.11491        (-2.79599      3.60704)
R1^2/D10^2  : 2.95196        (-2.55921      112.959)
kT2 [keV]   : 16.9518        (-14.6259      33.9921)
R2^2/D10^2  : 3.09625E-02    (-0.0312439   0.248332)
------------------------------------------------------------
 Reduced chi-squared = 
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  9.669e-09   5.675e-09
25- 50  1.343e-08   7.085e-09
50-150  1.666e-08   1.054e-08
15-150  3.976e-08   2.145e-08

Pre-slew spectrum (Pre-slew PHA with pre-slew DRM)

Power-law model

 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.65991     ( -0.107253   0.108283 )
Norm@50keV  : 2.31449E-03    ( -0.000142541   0.000141722 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          45.73 using 59 PHA bins.
# Reduced chi-squared =         0.8024 for     57 degrees of freedom 
# Null hypothesis probability =   8.577663e-01
 
Photon flux (15-150 keV)    in 92.23 sec: 0.303211 ( -0.018291  0.0183347 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.98338e-06 ( -1.29367e-07  1.30186e-07 ) ergs/cm2

Cutoff power-law model

Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.55506     ( -0.427409   0.203286 )
Epeak [keV] : 205.883      ( -205.937 -205.937 )
Norm@50keV  : 2.62248E-03    ( -0.000606767   0.00168656 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          45.53 using 59 PHA bins.
# Reduced chi-squared =         0.8131 for     56 degrees of freedom 
# Null hypothesis probability =   8.399157e-01
 
Photon flux (15-150 keV)    in 92.23 sec: 0.301477 ( -0.01935  0.019299 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.96596e-06 ( -1.47273e-07  1.4279e-07 ) ergs/cm2

Band function

 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -1.24712   ( 1.17547   1.17547 )
beta        : -1.74465    ( 1.74552   0.179729 )
Epeak [keV] : 69.2682      ( -63.8735 -63.8735 )
Norm@50keV   : 4.06825E-03    ( -0.00182672   176.151 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          45.09 using 59 PHA bins.
# Reduced chi-squared =         0.8198 for     55 degrees of freedom 
# Null hypothesis probability =   8.274205e-01
 
Photon flux (15-150 keV)    in 92.23 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)  = 1.34e-06
S(50-100 keV) = 1.52e-06

T90 vs. Hardness ratio plot

T90                                   = 204.031999826431 sec.
Hardness ratio (energy fluence ratio) = 1.13433

Color vs. Color plot

Count Ratio  (25-50 keV) / (15-25 keV) = 1.12937
Count Ratio (50-100 keV) / (15-25 keV) = 0.689193

Mask shadow pattern

IMX = -3.877468266728697E-01, IMY = 2.392547724977371E-02

TIME vs. PHA plot around the trigger time

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 64.000000

TIME vs. DetID plot around the trigger time

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 64.000000

100 us light curve (15-350 keV)

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 64.000000

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:
-60.000000 -55.197800
-54.000000 -22.368000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
254.6206  35.2204    0.0  36.5  109.4   0.3951   1.9   10.8	Her X-1                       
263.1196 -24.6300   40.3  48.0   13.7   0.0587   0.3    9.2	GX 1+4                        
268.4657  -1.6410    0.0  27.1   32.4   0.1594   1.4   12.7	SW J1753.5-0127               
270.3417 -25.1336    4.5  45.1    5.5   0.4078   2.6    4.5	GX 5-1                        
270.2402 -25.5886    6.2  45.5    5.4   0.3017   1.9    9.9	GRS 1758-258                  
274.1187 -14.0952    5.5  33.6    8.3   0.2399   2.1    7.5	GX 17+2                       
276.0267 -30.4175   17.1  48.1   -3.6   0.1242   0.7    6.1	H1820-303                     
285.1125 -24.7863    7.0  40.9  -13.2   0.2140   1.6    9.1	HT1900.1-2455                 
288.7731  11.1125    9.8   4.9  -12.4  -0.1072  -1.2   10.1	GRS 1915+105                  
299.4462  35.1684    0.8  21.2 -175.8   1.3589  15.2    7.3	Cyg X-1                       
308.1276  41.0316   16.2  29.9 -169.9  -0.0713  -0.7    4.8	Cyg X-3                       
326.0088  38.2448    5.3  39.1 -151.1  -0.2938  -2.2    8.9	Cyg X-2                       
263.0831 -33.8723    5.3  55.7    7.3  -1.0303  -2.2    5.2	GX 354-0                      
247.6501   2.4517    3.2  43.2   57.1   1.2388   3.7 ------	UNKNOWN                       
306.4131 -12.5594    2.3  33.1  -50.7   0.6624   5.1 ------	UNKNOWN

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

Time interval of the image:
-22.368000 27.560000
29.000000 71.300590
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
254.6171  35.2203   20.2  36.5  109.4  -0.2903  -0.6   10.7	Her X-1                       
262.9261 -24.6257   61.7  48.1   13.9   0.1037   0.2    8.5	GX 1+4                        
268.3843  -1.6124    6.7  27.2   32.5  -0.4501  -1.7    9.6	SW J1753.5-0127               
270.3693 -25.1053    4.6  45.0    5.5  -1.0346  -2.5    4.9	GX 5-1                        
270.2464 -25.5627    8.2  45.5    5.4  -0.5944  -1.4   11.2	GRS 1758-258                  
274.0118 -14.0154    7.5  33.6    8.6  -0.4188  -1.5    1.3	GX 17+2                       
275.7769 -30.4125    7.9  48.2   -3.3   0.6722   1.5    8.1	H1820-303                     
285.0315 -24.8899    3.8  41.0  -13.1  -0.9626  -3.0    1.9	HT1900.1-2455                 
288.9388  10.8870   11.1   5.1  -14.5  -0.2226  -1.0    9.0	GRS 1915+105                  
299.6745  35.0930    2.6  21.3 -175.2  -0.9736  -4.4    7.7	Cyg X-1                       
308.2793  40.9153    5.2  29.9 -169.6   0.5349   2.2    8.0	Cyg X-3                       
326.0138  38.2413    4.5  39.1 -151.1   0.8670   2.6    8.9	Cyg X-2                       
263.0345 -33.9103    9.7  55.8    7.3   1.4995   1.2    5.1	GX 354-0                      
246.8553  15.5670    2.2  40.8   76.4   4.6244   5.2 ------	UNKNOWN

Post-slew image of 15-350 keV band

Time interval of the image:
131.500600 243.092500
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
254.5329  35.2076   15.1  36.3   71.8  -0.4160  -0.8    8.9	Her X-1                       
268.2839  -1.3618  152.9  46.7   13.6  -0.0277  -0.1    7.4	SW J1753.5-0127               
274.0152 -14.2075    0.0  54.9   -1.1   0.9777   1.6   10.3	GX 17+2                       
288.6618  10.9810    3.9  26.1   -7.2   0.5999   2.9    8.3	GRS 1915+105                  
299.3808  35.2097    0.7   0.1 -117.4   2.9407  15.4   10.3	Cyg X-1                       
308.3856  40.9827    0.0   9.2 -163.2  -0.1765  -0.9   12.6	Cyg X-3                       
326.0257  38.2321    4.4  21.5 -137.5   0.5654   2.6    8.7	Cyg X-2                       
  5.8715  52.6491    2.3  49.0 -164.1   2.3155   4.9 ------	UNKNOWN                       
299.2234  -9.0947    2.3  44.3  -31.4   1.8314   5.0 ------	UNKNOWN

Plot creation:
Thu Mar  7 07:09:59 EST 2024