batgrbproduct analysis for trigger=1180055

batgrbproduct Analysis for Trigger=1180055

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): Fri Jul 21 12:02:04 EDT 2023
             Host Name: batproc1
   Current Working Dir: /local/data/bat1/prebascript/trigger1180055/GCN5_download_cron
======================================================================

  Trigger: 01180055      Segment: 000

  BAT Trigger Time: 711530336   [s; MET]
      Trigger Stop: 711530400   [s; MET]
               UTC: 2023-07-20T07:18:24.324620    [includes UTCF correction] 
       Where From?: TDRSS position message

  BAT 
    RA: 245.960257202829   Dec: -12.7263795644008  [deg; J2000]

     Catalogged Source?: NO
     Point Source?:      YES
     GRB Indicated?:     YES    [ by BAT flight software ]
     Image S/N Ratio:    17.5
     Image Trigger?:     YES
     Rate S/N Ratio:     0  [ if not an image trigger ]
     Image S/N Ratio:    17.5

  Flight Position:   [ source = BAT ]
    RA: 245.960257202829   Dec: -12.7263795644008  [deg; J2000]

  Ground Position:   [ source = BAT pre-slew burst ]
    RA: 245.9526927222   Dec: -12.7257091973197  [deg; J2000]  
        { 16h 23m 48.6s , -12d 43' 32.6" }
         +/- 1.39619062878339 [arcmin] (estimated 90% radius based on SNR)
         +/- 0.610546833068761 [arcmin] (formal 1-sigma fit error)
    SNR: 18.8822827284352
 
  Angular difference between Flight and Ground position is 0.444543 arcmin
 
  Partial Coding Fraction: 0.625    [ including projection effects ]

  Duration
     T90: 486.767999887466 +/- 22.6768734530433
        Measured from: -22.4199998378754
                   to: 464.348000049591     [s; relative to TRIGTIME]
     T50: 209.896000027657 +/- 12.6336700654128
        Measured from: 68.9480000734329
                   to: 278.844000101089     [s; relative to TRIGTIME]



  Fluence
     Peak Flux  (peak 1 second)
        Measured from: -23.6720000505447     
                   to: -22.6720000505447     [s; relative to TRIGTIME]
     Total Fluence        
        Measured from: -44.5360000133514     
                   to: 538.728000044823     [s; relative to TRIGTIME]
     
             Band 1     Band 2     Band 3     Band 4
              15-25      25-50     50-100    100-350     keV
 Total    26.273468   1.791065  -0.174968  -0.135322
           0.211536   0.184818   0.157146   0.141290 [error]
 Peak      0.069842   0.034946   0.003339   0.009040
           0.010269   0.009053   0.007902   0.007361 [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 9.08e-06 8.56e-07 3.23e-08 1.26e-09 9.97e-06 9.97e-06   erg/cm2
              Error 7.26e-07 8.94e-08 8.88e-09 5.94e-10 7.18e-07 7.18e-07   erg/cm2
Peak flux Power-law 7.44e-01 1.81e-01 2.28e-02 3.21e-03 9.50e-01 9.50e-01   ph/cm2/s
              Error 1.83e-01 1.42e-01 3.32e-02 9.81e-03 2.31e-01 2.32e-01   ph/cm2/s
 
Fluence   Cutoff-PL 8.51e-06 5.87e-07 7.24e-11 6.04e-20 9.10e-06 9.10e-06   erg/cm2
              Error 8.92e-07 1.00e-07 2.84e-10 1.11e-16 9.00e-07 9.00e-07   erg/cm2
Peak flux Cutoff-PL 7.44e-01 1.79e-01 2.23e-02 3.09e-03 9.48e-01 9.49e-01   ph/cm2/s
              Error 1.83e-01 -------- -------- -------- 2.31e-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    6.729    0.260    -      -           6.87e-05 1.56e-05   84.230 57
CPL   1.000    0.000      50.0    0.0      1.26e-03 0.00e+00  726.660 56
 
The chi2 of BB fit is 52.41 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    3.987    1.179    -      -           1.56e-03 1.62e-03   63.150 57
CPL   1.898    0.000       1.2    0.0      6.42e-02 0.00e+00   65.240 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  583.264  -44.536  538.728
T90   486.768  -22.420  464.348
T50   209.896   68.948  278.844
Peak    1.000  -23.672  -22.672

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
  245.9527 -12.7257 0.0101   23.0  114.0       5.5269    18.9  TRIG_01180055       
------------------------------------------
 
Foreground time interval of the image:
-19.499  73.701 (delta_t =  93.200 [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 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
-44.536000 178.740000
180.000000 228.960000
230.000000 306.760000
308.000000 330.480000
332.000000 393.650000
395.000000 538.728000
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 6.72940     ( -0.260534   0.259947 )
Norm@50keV  : 6.86737E-05    ( -1.41368e-05   1.70565e-05 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          84.23 using 59 PHA bins.
# Reduced chi-squared =          1.478 for     57 degrees of freedom 
# Null hypothesis probability =   1.100608e-02
 
Photon flux (15-150 keV)    in 576.9 sec: 0.593556 ( -0.0458944  0.0463797 ) ph/cm2/s
Energy fluence (15-150 keV)             : 9.9682e-06 ( -7.14594e-07  7.20681e-07 ) ergs/cm2

Cutoff power-law model

Multiple GTIs in the spectrum
tstart tstop
-44.536000 178.740000
180.000000 228.960000
230.000000 306.760000
308.000000 330.480000
332.000000 393.650000
395.000000 538.728000
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.00000     (     )
Epeak [keV] : 50.0000      (   )
Norm@50keV  : 1.26197E-03    (     )
------------------------------------------------------------
#Fit statistic : Chi-Squared =         726.66 using 59 PHA bins.
# Reduced chi-squared =         12.976 for     56 degrees of freedom 
# Null hypothesis probability =  2.151332e-117
 
Photon flux (15-150 keV)    in 576.9 sec: 0.537139 ( -0.05952  0.057559 ) ph/cm2/s
Energy fluence (15-150 keV)             : 9.0991e-06 ( -9.15079e-07  8.85311e-07 ) ergs/cm2

Band function

Multiple GTIs in the spectrum
tstart tstop
-44.536000 178.740000
180.000000 228.960000
230.000000 306.760000
308.000000 330.480000
332.000000 393.650000
395.000000 538.728000
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : 4.60485   ( -6.31526   -4.60485 )
beta        : -9.99061    ( 9.99061   19.8936 )
Epeak [keV] : 12.6669      ( -0.53003 0.452576 )
Norm@50keV   : 8.87552E+04    ( -5200.8   214526 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          52.57 using 59 PHA bins.
# Reduced chi-squared =         0.9558 for     55 degrees of freedom 
# Null hypothesis probability =   5.680950e-01
 
Photon flux (15-150 keV)    in 576.9 sec: 0.657527 ( 6.34247  -0.063195 ) 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]    : 2.48046  (-0.105451  0.114526)
R^2/D10^2   : 290.480  (-96.1767   140.21)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          52.41 using 59 PHA bins.
# Reduced chi-squared =         0.9195 for     57 degrees of freedom 
# Null hypothesis probability =   6.476233e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  8.681e-06   1.038e-06
25- 50  6.182e-07   7.852e-08
50-150  1.808e-10   8.887e-11
15-150  9.300e-06   1.064e-06

Thermal bremsstrahlung (OTTB)

XSPEC12>exit
 XSPEC: quit
 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 4.07332       (-0.244146      0.274006)
Norm        : 298.682       (-86.5039     119.257)
------------------------------------------------------------
 Reduced chi-squared = 
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  8.975e-06   9.288e-07
25- 50  6.863e-07   8.054e-08
50-150  1.133e-09   5.620e-10
15-150  9.662e-06   9.980e-07

Double BB

XSPEC12>exit
 XSPEC: quit
 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 0.409147        (-2.49366      -2.49366)
R1^2/D10^2  : 1.38445E+13        (-1.55895e+13      1.48597e+18)
kT2 [keV]   : 2.49532        (-0.114604      0.124594)
R2^2/D10^2  : 274.463    (-97.4128   146.902)
------------------------------------------------------------
 Reduced chi-squared = 
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  8.677e-06   9.340e+02
25- 50  6.191e-07   8.310e+03
50-150  1.827e-10   2.230e+05
15-150  9.296e-06   1.952e+05

Peak spectrum fit

Power-law model

Time interval is from  -23.672 sec. to  -22.672 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 3.98742     ( -0.960477   1.3971 )
Norm@50keV  : 1.55678E-03    ( -0.00119255   0.00205314 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          63.15 using 59 PHA bins.
# Reduced chi-squared =          1.108 for     57 degrees of freedom 
# Null hypothesis probability =   2.680053e-01
 
Photon flux (15-150 keV)    in 1 sec: 0.949520 ( -0.231459  0.231232 ) ph/cm2/s
Energy fluence (15-150 keV)             : 3.39767e-08 ( -1.05243e-08  1.23898e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from  -23.672 sec. to  -22.672 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.89776     (     )
Epeak [keV] : 1.16083      (   )
Norm@50keV  : 6.41816E-02    (     )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          65.24 using 59 PHA bins.
# Reduced chi-squared =          1.165 for     56 degrees of freedom 
# Null hypothesis probability =   1.863006e-01
 
Photon flux (15-150 keV)    in 1 sec: 0.948003 ( -0.230601  0.232027 ) ph/cm2/s
Energy fluence (15-150 keV)             : 3.30907e-08 ( -9.6208e-09  1.33374e-08 ) ergs/cm2

Band function

Time interval is from  -23.672 sec. to  -22.672 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -9.81589   ( 9.81589   9.81589 )
beta        : -3.98774    ( -1.39759   0.959314 )
Epeak [keV] : 1.89599      ( -1.89599 -1.89599 )
Norm@50keV   : 0.211525    ( -0.162094   0.279025 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          63.15 using 59 PHA bins.
# Reduced chi-squared =          1.148 for     55 degrees of freedom 
# Null hypothesis probability =   2.104163e-01
 
Photon flux (15-150 keV)    in 1 sec:  (    ) ph/cm2/s
Energy fluence (15-150 keV)             : 0 ( 0  0 ) ergs/cm2

Single BB

 XSPEC: quit
 
 
Spectral model blackbody:
------------------------------------------------------------
Parameters  : value    Lower 90%  Upper 90%
kT [keV]    : 2.98089  (-0.82651  1.4373)
R^2/D10^2   : 126.213  (-126.929   1050.96)
(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  2.267e-08   1.301e-08
25- 50  3.232e-09   2.101e-09
50-150  4.942e-12   5.345e-12
15-150  2.591e-08   1.506e-08

Thermal bremsstrahlung (OTTB)

XSPEC12>exit
 XSPEC: quit
 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 8.21926       (-3.98548      9.97805)
Norm        : 48.3785       (-47.5866     288.049)
------------------------------------------------------------
 Reduced chi-squared = 
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  2.221e-08   1.257e-08
25- 50  7.197e-09   4.344e-09
50-150  2.767e-10   2.961e-10
15-150  2.968e-08   1.745e-08

Double BB

XSPEC12>exit
 XSPEC: quit
 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 2.25287        (-0.838529      1.05514)
R1^2/D10^2  : 615.032        (-1091.21      84117.5)
kT2 [keV]   : 9.39034        (-3.77314      8.26784)
R2^2/D10^2  : 0.260186    (-0.305569   2.38057)
------------------------------------------------------------
 Reduced chi-squared = 
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.986e-08   1.138e-08
25- 50  1.107e-08   7.070e-09
50-150  4.486e-09   3.972e-09
15-150  3.541e-08   1.884e-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: 6.02827     ( -0.378738   0.38726 )
Norm@50keV  : 1.52890E-04    ( -4.7015e-05   6.23894e-05 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          54.35 using 59 PHA bins.
# Reduced chi-squared =         0.9535 for     57 degrees of freedom 
# Null hypothesis probability =   5.750422e-01
 
Photon flux (15-150 keV)    in 93.2 sec: 0.647314 ( -0.0587243  0.0590187 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.80942e-06 ( -1.52615e-07  1.53078e-07 ) ergs/cm2

Cutoff power-law model

Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.00000     (     )
Epeak [keV] : 50.0000      (   )
Norm@50keV  : 3.07596E-03    (     )
------------------------------------------------------------
#Fit statistic : Chi-Squared =         368.11 using 59 PHA bins.
# Reduced chi-squared =         6.5734 for     56 degrees of freedom 
# Null hypothesis probability =   1.782209e-47
 
Photon flux (15-150 keV)    in 93.2 sec: 0.624945 ( -0.067192  0.065292 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.72333e-06 ( -1.70817e-07  1.66977e-07 ) ergs/cm2

Band function

 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : 0.966870   ( -0.0396735   0.447483 )
beta        : -9.13722    ( 8.01468   1.60807 )
Epeak [keV] : 8.85241      ( -0.322424 0.148652 )
Norm@50keV   : 86.0486    ( -83.516   59296.5 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          45.81 using 59 PHA bins.
# Reduced chi-squared =         0.8329 for     55 degrees of freedom 
# Null hypothesis probability =   8.067250e-01
 
Photon flux (15-150 keV)    in 93.2 sec:  (    ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.57648e-06 ( 0  0 ) ergs/cm2

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

S(25-50 keV)  = 8.56e-07
S(50-100 keV) = 3.23e-08

T90 vs. Hardness ratio plot

T90                                   = 486.767999887466 sec.
Hardness ratio (energy fluence ratio) = 0.0377336

Color vs. Color plot

Count Ratio  (25-50 keV) / (15-25 keV) = 0.0681701
Count Ratio (50-100 keV) / (15-25 keV) = -0.00665949

Mask shadow pattern

IMX = -1.724983452830623E-01, IMY = -3.871876579202563E-01

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:

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

Time interval of the image:
-19.499400 73.700600
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
245.0430 -15.6730    5.3  24.8  120.2  -0.6670  -2.2    4.2	Sco X-1                       
254.5821  35.4538   19.2  37.5    6.2  -0.1971  -0.6    9.0	Her X-1                       
268.4283  -1.5474  149.0  37.9   72.8   0.0530   0.1    6.7	SW J1753.5-0127               
245.9527 -12.7257    0.6  23.0  114.0   5.5237  19.0 ------	UNKNOWN                       
198.3828 -38.7165    2.5  53.0 -174.2   3.1670   4.7 ------	UNKNOWN                       
211.3804 -17.2239    2.5  29.4 -165.1   1.1548   4.6 ------	UNKNOWN                       
190.4074  14.7760    3.0  41.2  -99.1   3.6626   3.9 ------	UNKNOWN

Post-slew image of 15-350 keV band

Time interval of the image:
137.500590 178.740000
180.000000 228.960000
230.000000 306.760000
308.000000 330.480000
332.000000 393.650000
395.000000 881.930000
885.000000 885.030000
894.000000 963.170000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
245.1219 -15.7047    7.1   3.1  179.5   6.9748   1.6    9.1	Sco X-1                       
254.4272  35.4804    5.5  48.9   -7.1 -17.0893  -2.1    8.4	Her X-1                       
255.7902 -37.9668   16.0  26.7  146.4  -3.7438  -0.7   11.9	4U 1700-377                   
256.5843 -36.5212    6.4  25.6  143.8  -9.1138  -1.8    9.3	GX 349+2                      
263.0319 -24.7846  249.0  20.1  113.0  -0.2633  -0.0    2.7	GX 1+4                        
264.5953 -44.3082    0.0  35.4  140.5  -6.8198  -0.8   10.6	4U 1735-44                    
268.4968  -1.4985   13.3  25.0   48.8   4.8481   0.9    8.2	SW J1753.5-0127               
270.1680 -24.9301    7.2  25.9  105.4  10.7365   1.6   11.0	GX 5-1                        
270.1124 -25.8611    0.0  26.2  107.4  10.2868   1.6   12.5	GRS 1758-258                  
274.0094 -14.0385   45.1  27.3   79.8  -1.6988  -0.3    0.2	GX 17+2                       
275.8406 -30.2357    7.5  32.7  110.9  12.0054   1.5    9.0	H1820-303                     
285.1326 -24.8087    4.8  38.8   97.7 -38.2417  -2.4    8.5	HT1900.1-2455                 
263.1468 -33.9087    9.9  26.3  130.2   6.7734   1.2    9.0	GX 354-0                      
278.4862 -16.4560    3.1  31.6   84.5  29.2587   3.8 ------	UNKNOWN                       
245.7776 -12.7498    1.4   0.2 -109.5  36.6106   8.1 ------	UNKNOWN                       
229.2508 -27.8347    2.9  21.7 -152.8  17.5120   4.1 ------	UNKNOWN                       
219.7464 -38.9525    2.8  35.0 -159.4  23.9385   4.2 ------	UNKNOWN                       
221.5670  32.7173    2.7  51.1  -42.8 113.7160   4.4 ------	UNKNOWN

Plot creation:
Fri Jul 21 12:08:29 EDT 2023