batgrbproduct analysis for trigger=743086

batgrbproduct Analysis for Trigger=743086

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): Thu Apr 13 16:33:48 EDT 2017
             Host Name: bat1
   Current Working Dir: /local/data/bat1/alien/Swift_3rdBATcatalog/event/batevent_reproc/trigger743086
======================================================================

  Trigger: 00743086      Segment: 000

  BAT Trigger Time: 511543691.328   [s; MET]
      Trigger Stop: 511543691.84   [s; MET]
               UTC: 2017-03-18T15:27:52.554820    [includes UTCF correction] 
       Where From?: TDRSS position message

  BAT 
    RA: 284.279322271095   Dec: 6.26950020290672  [deg; J2000]

     Catalogged Source?: NO
     Point Source?:      YES
     GRB Indicated?:     YES    [ by BAT flight software ]
     Image S/N Ratio:    7.21
     Image Trigger?:     NO
     Rate S/N Ratio:     14.9331845230681  [ if not an image trigger ]
     Image S/N Ratio:    7.21

  Flight Position:   [ source = BAT ]
    RA: 284.279322271095   Dec: 6.26950020290672  [deg; J2000]

  Ground Position:   [ source = BAT pre-slew burst ]
    RA: 284.292349987551   Dec: 6.31685800630574  [deg; J2000]  
        { 18h 57m 10.2s , +06d 19' 00.7" }
         +/- 2.21816638960067 [arcmin] (estimated 90% radius based on SNR)
         +/- 1.03037939340942 [arcmin] (formal 1-sigma fit error)
    SNR: 9.74632894653276
 
  Angular difference between Flight and Ground position is 2.945776 arcmin
 
  Partial Coding Fraction: 0.6796875    [ including projection effects ]

  Duration
     T90: 1.07199990749359 +/- 0.221846764251316
        Measured from: -0.46399998664856
                   to: 0.607999920845032     [s; relative to TRIGTIME]
     T50: 0.555999934673309 +/- 0.297617258995808
        Measured from: -0.100000023841858
                   to: 0.455999910831451     [s; relative to TRIGTIME]



  Fluence
     Peak Flux  (peak 1 second)
        Measured from: -0.364000022411346     
                   to: 0.635999977588654     [s; relative to TRIGTIME]
     Total Fluence        
        Measured from: -0.5     
                   to: 0.643999993801117     [s; relative to TRIGTIME]
     
             Band 1     Band 2     Band 3     Band 4
              15-25      25-50     50-100    100-350     keV
 Total     0.031774   0.047054   0.069911   0.019985
           0.009041   0.009812   0.009560   0.008166 [error]
 Peak      0.030110   0.045104   0.057211   0.015219
           0.008480   0.009271   0.009042   0.007743 [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 7.30e-09 2.10e-08 4.92e-08 3.13e-07 1.33e-07 3.91e-07   erg/cm2
              Error 3.06e-09 5.18e-09 8.59e-09 1.40e-07 2.36e-08 1.42e-07   erg/cm2
Peak flux Power-law 2.25e-01 3.29e-01 3.58e-01 7.29e-01 1.14e+00 1.64e+00   ph/cm2/s
              Error 9.79e-02 8.56e-02 6.95e-02 3.32e-01 2.21e-01 3.49e-01   ph/cm2/s
 
Fluence   Cutoff-PL 1.65e-09 2.51e-09 2.56e-09 5.33e-09 1.03e-08 1.77e-08   erg/cm2
              Error -------- -------- -------- -------- -------- --------   erg/cm2
Peak flux Cutoff-PL 2.33e-01 3.31e-01 3.57e-01 7.85e-01 1.14e+00 1.64e+00   ph/cm2/s
              Error 1.08e-01 8.59e-02 7.59e-02 -------- 2.49e-01 4.22e-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    0.773    0.335    -      -           9.83e-03 1.85e-03   51.150 57
CPL   0.773    0.338    9999.3    0.0      9.91e-03 9.75e-03   51.160 56
 
 
=== 1-s peak spectral analysis ===
 
Model Ph_index Ph_90err Epeak  Epeak_90err Norm     Nomr_90err chi2   dof
PL    0.878    0.359    -      -           9.90e-03 1.94e-03   48.950 57
CPL   0.802    0.000     989.2    0.0      1.06e-02 0.00e+00   49.030 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: 1.088000 sec.
T50 in the 50-300 keV band: 0.576000 sec.

 
=== Table of the duration information ==
 
        Value   tstart    tstop
T100    1.144   -0.500    0.644
T90     1.072   -0.464    0.608
T50     0.556   -0.100    0.456
Peak    1.000   -0.364    0.636

Click here for the BAT GCN circular template

Estimated redshift from machine learning (Ukwatta et al. 2016) - may take a few minute to calcaulte

Special notes of this burst

Image

Pre-slew 15.0-350.0 keV image (Event data)

#   RAcent    DECcent   POSerr    Theta     Phi              Peak Cts       SNR   Name
  284.2923     6.3169   0.0198    29.9372    25.9351         0.1699870      9.746 TRIG_00743086                 
 
Foreground time interval of the image:
 -0.500   0.644 (delta_t =   1.144 [sec])
Background time interval of the image:
-239.328  -0.500 (delta_t = 238.828 [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   -0.500 sec. to    0.644 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 0.772853     ( -0.349206   0.321574 )
Norm@50keV  : 9.82661E-03    ( -0.00188396   0.0018102 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          51.15 using 59 PHA bins.
# Reduced chi-squared =         0.8974 for     57 degrees of freedom 
# Null hypothesis probability =   6.931728e-01
 
Photon flux (15-150 keV)    in 1.144 sec: 1.13064 ( -0.203431  0.20488 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.32906e-07 ( -2.35722e-08  2.36266e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from   -0.500 sec. to    0.644 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 0.773466     ( -0.359579   0.31731 )
Epeak [keV] : 9999.33      ( -9999.36 -9999.36 )
Norm@50keV  : 9.90778E-03    ( -0.00174531   0.0177629 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          51.16 using 59 PHA bins.
# Reduced chi-squared =         0.9135 for     56 degrees of freedom 
# Null hypothesis probability =   6.583249e-01
 
Photon flux (15-150 keV)    in 1.144 sec: 1.13282 ( -0.2082  0.20058 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.03294e-08 ( 0  0 ) ergs/cm2

Band function

Time interval is from   -0.500 sec. to    0.644 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]    : 30.2949  (-6.52368  10.4244)
R^2/D10^2   : 1.64552E-02  (-0.00918443   0.0171587)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          55.72 using 59 PHA bins.
# Reduced chi-squared =         0.9775 for     57 degrees of freedom 
# Null hypothesis probability =   5.233705e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  2.687e-09   1.183e-09
25- 50  1.664e-08   5.275e-09
50-150  1.075e-07   3.616e-08
15-150  1.268e-07   4.112e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 200.000       (-40.3814      -200)
Norm        : 4.59465       (-0.848516     0.848516)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          67.90 using 59 PHA bins.
# Reduced chi-squared =          1.191 for     57 degrees of freedom 
# Null hypothesis probability =   1.530261e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.309e-08   7.653e-09
25- 50  2.517e-08   1.432e-08
50-150  5.521e-08   3.178e-08
15-150  9.348e-08   5.376e-08

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 4.27752        (-2.32667      4.04323)
R1^2/D10^2  : 5.62578        (-5.29628      517.961)
kT2 [keV]   : 35.5834        (-8.87173      18.7939)
R2^2/D10^2  : 9.99797E-03    (-0.00667349   0.0128258)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          48.25 using 59 PHA bins.
# Reduced chi-squared =         0.8772 for     55 degrees of freedom 
# Null hypothesis probability =   7.283510e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.005e-08   6.138e-09
25- 50  1.683e-08   7.137e-09
50-150  1.095e-07   5.403e-08
15-150  1.363e-07   6.151e-08

Peak spectrum fit

Power-law model

Time interval is from   -0.364 sec. to    0.636 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 0.878173     ( -0.372809   0.345318 )
Norm@50keV  : 9.90319E-03    ( -0.00196394   0.00191268 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          48.95 using 59 PHA bins.
# Reduced chi-squared =         0.8587 for     57 degrees of freedom 
# Null hypothesis probability =   7.672239e-01
 
Photon flux (15-150 keV)    in 1 sec: 1.13656 ( -0.220728  0.22183 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.12106e-07 ( -2.22473e-08  2.23468e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from   -0.364 sec. to    0.636 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 0.802397     (     )
Epeak [keV] : 989.203      (   )
Norm@50keV  : 1.06322E-02    (     )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          49.03 using 59 PHA bins.
# Reduced chi-squared =         0.8756 for     56 degrees of freedom 
# Null hypothesis probability =   7.336663e-01
 
Photon flux (15-150 keV)    in 1 sec: 1.14439 ( -0.257828  0.2395 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.12336e-07 ( -2.49363e-08  2.45913e-08 ) ergs/cm2

Band function

Time interval is from   -0.364 sec. to    0.636 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]    : 27.9911  (-6.55163  10.566)
R^2/D10^2   : 2.00908E-02  (-0.0119963   0.0246788)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          54.42 using 59 PHA bins.
# Reduced chi-squared =         0.9547 for     57 degrees of freedom 
# Null hypothesis probability =   5.725845e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  2.567e-09   1.118e-09
25- 50  1.537e-08   6.417e-09
50-150  8.713e-08   3.451e-08
15-150  1.051e-07   3.894e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 200.000       (-50.2518      -200)
Norm        : 4.61017       (-0.914276     0.914276)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          59.81 using 59 PHA bins.
# Reduced chi-squared =          1.049 for     57 degrees of freedom 
# Null hypothesis probability =   3.740775e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.148e-08   6.715e-09
25- 50  2.208e-08   1.283e-08
50-150  4.843e-08   2.762e-08
15-150  8.199e-08   4.849e-08

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 5.21744        (-2.49341      4.56845)
R1^2/D10^2  : 2.59030        (-2.38058      54.5228)
kT2 [keV]   : 35.6047        (-10.205      27.6179)
R2^2/D10^2  : 9.37519E-03    (-0.00722401   0.0168881)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          46.99 using 59 PHA bins.
# Reduced chi-squared =         0.8544 for     55 degrees of freedom 
# Null hypothesis probability =   7.702651e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  9.110e-09   5.575e-09
25- 50  1.633e-08   8.690e-09
50-150  9.010e-08   5.115e-08
15-150  1.155e-07   6.125e-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: 0.772853     ( -0.349206   0.321574 )
Norm@50keV  : 9.82661E-03    ( -0.00188396   0.0018102 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          51.15 using 59 PHA bins.
# Reduced chi-squared =         0.8974 for     57 degrees of freedom 
# Null hypothesis probability =   6.931728e-01
 
Photon flux (15-150 keV)    in 1.144 sec: 1.13063 ( -0.203403  0.204899 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.32892e-07 ( -2.3568e-08  2.36384e-08 ) ergs/cm2

Cutoff power-law model

Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 0.776181     ( -0.361501   0.315694 )
Epeak [keV] : 9999.36      ( -9999.36 -9999.36 )
Norm@50keV  : 9.91479E-03    ( -0.00174706   0.0178168 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          51.16 using 59 PHA bins.
# Reduced chi-squared =         0.9136 for     56 degrees of freedom 
# Null hypothesis probability =   6.582757e-01
 
Photon flux (15-150 keV)    in 1.144 sec: 1.13249 ( -0.207909  0.20209 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.32739e-07 ( -2.33898e-08  2.38009e-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)  = 2.10e-08
S(50-100 keV) = 4.92e-08

T90 vs. Hardness ratio plot

T90                                   = 1.07199990749359 sec.
Hardness ratio (energy fluence ratio) = 2.34286

Color vs. Color plot

Count Ratio  (25-50 keV) / (15-25 keV) = 1.4809
Count Ratio (50-100 keV) / (15-25 keV) = 2.20026

Mask shadow pattern

IMX = 5.178916333020426E-01, IMY = -2.518671730167600E-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:
-239.328000 -0.500000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
268.2842  -1.3754    4.9  46.6   36.1   1.8653   2.4    6.8	SW J1753.5-0127               
273.9583 -13.9921    4.2  52.3   19.6   2.6440   2.7    3.8	GX 17+2                       
284.9856 -24.7979    5.3  56.8    2.0  -2.8634  -2.2    7.9	HT1900.1-2455                 
288.8017  10.9015    1.3  23.6   24.8   2.1573   8.9    2.6	GRS 1915+105                  
299.5642  35.2070    0.4   8.5  123.8   6.3921  26.2    1.3	Cyg X-1                       
308.0048  41.1453    0.0  12.9  167.5   0.5488   2.4   12.5	Cyg X-3                       
326.0513  38.3880    5.2  19.7 -146.2   0.5192   2.2    6.9	Cyg X-2                       
278.8041 -16.2873    2.2  51.7   13.0   4.0443   5.3 ------	UNKNOWN                       
294.2095  -5.2822    2.2  35.5   -0.6   1.6114   5.3 ------	UNKNOWN                       
325.1451 -18.5324    3.5  50.6  -44.7   4.2051   3.3 ------	UNKNOWN

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

Time interval of the image:
-0.500000 0.644000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
268.3690  -1.4524   19.0  46.6   36.0  -0.0278  -0.6    0.1	SW J1753.5-0127               
273.9108 -13.9525  249.5  52.3   19.6  -0.0031  -0.0    7.5	GX 17+2                       
284.9594 -24.9132   10.9  56.9    2.0   0.0944   1.0    4.2	HT1900.1-2455                 
288.8055  11.0977   11.0  23.4   25.1   0.0163   1.0    9.1	GRS 1915+105                  
299.7081  35.0235  636.5   8.3  123.7  -0.0003  -0.0   12.2	Cyg X-1                       
308.3658  41.0370    0.0  12.8  168.8   0.0150   1.0   12.6	Cyg X-3                       
325.9330  38.2688   40.4  19.5 -146.0  -0.0039  -0.3   11.7	Cyg X-2                       
284.2923   6.3168    1.2  29.9   25.9   0.1699   9.7 ------	UNKNOWN                       
304.4703  16.7388    2.8  11.7  -15.0   0.0535   4.2 ------	UNKNOWN                       
293.7264 -28.9071    2.4  58.4   -8.3   0.4338   4.9 ------	UNKNOWN

Post-slew image of 15-350 keV band

Time interval of the image:
62.572600 962.744600
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
254.5485  35.3431    4.7  39.9  138.6   3.2982   2.4    4.4	Her X-1                       
256.1273 -38.0342    0.0  51.5   26.1   1.7209   0.7   13.2	4U 1700-377                   
256.4914 -36.3739   72.8  50.0   27.1  -0.3419  -0.2    4.0	GX 349+2                      
262.9816 -24.6664    5.4  37.2   30.8   1.8143   2.1    5.0	GX 1+4                        
264.8750 -44.4089   15.1  53.6   14.8   1.7463   0.8    6.2	4U 1735-44                    
268.2208  -1.3050    8.5  17.7   63.0  -0.7991  -1.3   12.5	SW J1753.5-0127               
270.3550 -24.9649   24.1  34.0   20.6  -0.3426  -0.5    7.9	GX 5-1                        
270.3196 -25.7280    3.5  34.7   20.1   2.4280   3.3    1.3	GRS 1758-258                  
273.9256 -13.9737    4.3  22.7   24.6   1.5349   2.7    6.0	GX 17+2                       
275.8769 -30.2124    6.0  37.3    9.7   1.4621   1.9    9.6	H1820-303                     
285.1693 -25.0740    0.0  31.3   -3.8  -0.5060  -0.8   11.7	HT1900.1-2455                 
288.7862  10.9145    0.9   6.4 -139.1   5.8512  12.3    2.0	GRS 1915+105                  
299.5869  35.1942    0.5  32.2 -158.5  15.8535  24.8    0.5	Cyg X-1                       
308.1639  41.0909    7.5  40.8 -154.5  -1.4732  -1.5    8.6	Cyg X-3                       
326.2073  38.3708   17.3  49.6 -138.9   1.7582   0.7    3.4	Cyg X-2                       
262.8552 -33.9554   12.1  45.0   23.0  -1.1084  -1.0    9.8	GX 354-0                      
251.5019 -25.0290    2.5  44.7   41.9   7.3514   4.6 ------	UNKNOWN                       
259.8983 -25.0263    0.8  39.3   33.9  14.1991  14.3 ------	UNKNOWN                       
282.3701  55.1292    3.1  48.9  176.2   5.0347   3.7 ------	UNKNOWN                       
306.2214  57.2935    4.0  53.9 -167.9   5.7814   2.9 ------	UNKNOWN                       
324.2290  10.3690    4.3  39.7 -101.0   6.7780   2.7 ------	UNKNOWN                       
	UNKNOWN                       
	UNKNOWN

Plot creation:
Thu Apr 13 21:15:16 EDT 2017