batgrbproduct analysis for trigger=586071

batgrbproduct Analysis for Trigger=586071

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): Mon Mar  3 22:41:25 EST 2014
             Host Name: batevent1
   Current Working Dir: /local/data/batevent/batevent_reproc/trigger586071
======================================================================

  Trigger: 00586071      Segment: 000

  BAT Trigger Time: 413623869.504   [s; MET]
      Trigger Stop: 413623870.016   [s; MET]
               UTC: 2014-02-09T07:30:57.881180    [includes UTCF correction] 
       Where From?: TDRSS position message

  BAT 
    RA: 81.3347420112946   Dec: 32.477013277617  [deg; J2000]

     Catalogged Source?: NO
     Point Source?:      YES
     GRB Indicated?:     YES    [ by BAT flight software ]
     Image S/N Ratio:    9.74
     Image Trigger?:     NO
     Rate S/N Ratio:     15.7797338380595  [ if not an image trigger ]
     Image S/N Ratio:    9.74

  Flight Position:   [ source = BAT ]
    RA: 81.3347420112946   Dec: 32.477013277617  [deg; J2000]

  Ground Position:   [ source = BAT pre-slew burst ]
    RA: 81.3274012559897   Dec: 32.4884721348062  [deg; J2000]  
        { 05h 25m 18.6s , +32d 29' 18.5" }
         +/- 0.783788501459089 [arcmin] (estimated 90% radius based on SNR)
         +/- 0.222804485578225 [arcmin] (formal 1-sigma fit error)
    SNR: 43.0787234971595
 
  Angular difference between Flight and Ground position is 0.781499 arcmin
 
  Partial Coding Fraction: 0.3828125    [ including projection effects ]

  Duration
     T90: 20.432000041008 +/- 9.62708178563028
        Measured from: 1.7039999961853
                   to: 22.1360000371933     [s; relative to TRIGTIME]
     T50: 0.592000067234039 +/- 0.0815843022113378
        Measured from: 1.95999997854233
                   to: 2.55200004577637     [s; relative to TRIGTIME]



  Fluence
     Peak Flux  (peak 1 second)
        Measured from: 1.69199997186661     
                   to: 2.69199997186661     [s; relative to TRIGTIME]
     Total Fluence        
        Measured from: 0.15200001001358     
                   to: 27.6240000128746     [s; relative to TRIGTIME]
     
             Band 1     Band 2     Band 3     Band 4
              15-25      25-50     50-100    100-350     keV
 Total     1.335441   2.107094   1.933753   0.576608
           0.062658   0.067747   0.060738   0.047570 [error]
 Peak      0.774136   1.555758   1.577069   0.479485
           0.024895   0.033797   0.034685   0.022406 [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 5.16e-07 9.90e-07 1.47e-06 4.70e-06 4.15e-06 7.68e-06   erg/cm2
              Error 3.61e-08 4.11e-08 6.05e-08 4.36e-07 1.52e-07 4.67e-07   erg/cm2
Peak flux Power-law 1.04e+01 1.22e+01 1.04e+01 1.51e+01 3.84e+01 4.82e+01   ph/cm2/s
              Error 5.34e-01 3.89e-01 2.87e-01 8.72e-01 1.05e+00 1.24e+00   ph/cm2/s
 
Fluence   Cutoff-PL 4.83e-07 1.01e-06 1.51e-06 3.38e-06 4.10e-06 6.39e-06   erg/cm2
              Error 4.65e-08 4.46e-08 7.23e-08 1.00e-06 1.60e-07 7.30e-07   erg/cm2
Peak flux Cutoff-PL 9.03e+00 1.25e+01 1.11e+01 1.01e+01 3.76e+01 4.27e+01   ph/cm2/s
              Error 6.87e-01 4.17e-01 3.82e-01 1.47e+00 1.09e+00 1.86e+00   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    1.429    0.063    -      -           1.57e-02 5.53e-04   52.370 57
CPL   1.162    0.255     178.3  564.5      2.07e-02 5.40e-03   48.990 56
 
 
=== 1-s peak spectral analysis ===
 
Model Ph_index Ph_90err Epeak  Epeak_90err Norm     Nomr_90err chi2   dof
PL    1.230    0.043    -      -           3.26e-01 8.36e-03   58.650 57
CPL   0.739    0.186     152.4   40.1      5.32e-01 9.69e-02   36.280 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: 0.832000 sec.
T50 in the 50-300 keV band: 0.256000 sec.

 
=== Table of the duration information ==
 
        Value   tstart    tstop
T100   27.472    0.152   27.624
T90    20.432    1.704   22.136
T50     0.592    1.960    2.552
Peak    1.000    1.692    2.692

Click here for the BAT GCN circular template

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
   81.3274    32.4885   0.0045    44.8609  -159.5211         6.3778061     43.079 TRIG_00586071                 
 
Foreground time interval of the image:
  0.152  27.624 (delta_t =  27.472 [sec])
Background time interval of the image:
-375.203 -322.332 (delta_t =  52.871 [sec])
-239.504   0.152 (delta_t = 239.656 [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    0.152 sec. to   27.624 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.42939     ( -0.0629735   0.0628625 )
Norm@50keV  : 1.57204E-02    ( -0.000552818   0.00055273 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          52.37 using 59 PHA bins.
# Reduced chi-squared =         0.9188 for     57 degrees of freedom 
# Null hypothesis probability =   6.490061e-01
 
Photon flux (15-150 keV)    in 27.47 sec: 1.92762 ( -0.0749455  0.07517 ) ph/cm2/s
Energy fluence (15-150 keV)             : 4.14846e-06 ( -1.51773e-07  1.51915e-07 ) ergs/cm2

Cutoff power-law model

Time interval is from    0.152 sec. to   27.624 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.16201     ( -0.262499   0.248105 )
Epeak [keV] : 178.253      ( -60.8906 1068.01 )
Norm@50keV  : 2.07227E-02    ( -0.00456411   0.00623632 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          48.99 using 59 PHA bins.
# Reduced chi-squared =         0.8748 for     56 degrees of freedom 
# Null hypothesis probability =   7.352638e-01
 
Photon flux (15-150 keV)    in 27.47 sec: 1.89603 ( -0.07987  0.08028 ) ph/cm2/s
Energy fluence (15-150 keV)             : 4.10119e-06 ( -1.59766e-07  1.59244e-07 ) ergs/cm2

Band function

Time interval is from    0.152 sec. to   27.624 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -1.17570   ( -0.0952509   0.164762 )
beta        : -9.35460    ( 9.36969   19.3697 )
Epeak [keV] : 185.374      ( -39.2394 230.127 )
Norm@50keV   : 2.04141E-02    ( -0.000716466   0.00595393 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          49.00 using 59 PHA bins.
# Reduced chi-squared =         0.8908 for     55 degrees of freedom 
# Null hypothesis probability =   7.020996e-01
 
Photon flux (15-150 keV)    in 27.47 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]    : 18.1653  (  )
R^2/D10^2   : 0.113492  (   )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =         210.39 using 59 PHA bins.
# Reduced chi-squared =         3.6910 for     57 degrees of freedom 
# Null hypothesis probability =   1.954641e-19
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  2.054e-07   1.498e-08
25- 50  9.563e-07   5.109e-08
50-150  2.296e-06   1.303e-07
15-150  3.457e-06   1.456e-07

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 200.000       (      )
Norm        : 8.06888       (-0.284385     0.28431)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          66.73 using 59 PHA bins.
# Reduced chi-squared =          1.171 for     57 degrees of freedom 
# Null hypothesis probability =   1.772911e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  5.521e-07   2.143e-08
25- 50  1.062e-06   4.244e-08
50-150  2.329e-06   9.175e-08
15-150  3.943e-06   1.525e-07

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 7.10882        (-1.006      1.14909)
R1^2/D10^2  : 1.68627        (-0.667337      1.24341)
kT2 [keV]   : 27.2590        (-2.68185      3.71996)
R2^2/D10^2  : 2.33083E-02    (-0.00867561   0.0109178)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          52.63 using 59 PHA bins.
# Reduced chi-squared =         0.9569 for     55 degrees of freedom 
# Null hypothesis probability =   5.656806e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  4.608e-07   6.991e-08
25- 50  1.005e-06   8.900e-08
50-150  2.619e-06   2.404e-07
15-150  4.085e-06   3.090e-07

Peak spectrum fit

Power-law model

Time interval is from    1.692 sec. to    2.692 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.22966     ( -0.0431811   0.0430742 )
Norm@50keV  : 0.325954    ( -0.00835745   0.00835286 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          58.65 using 59 PHA bins.
# Reduced chi-squared =          1.029 for     57 degrees of freedom 
# Null hypothesis probability =   4.146372e-01
 
Photon flux (15-150 keV)    in 1 sec: 38.4277 ( -1.05287  1.05436 ) ph/cm2/s
Energy fluence (15-150 keV)             : 3.2799e-06 ( -8.69858e-08  8.70318e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from    1.692 sec. to    2.692 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 0.739282     ( -0.189512   0.182245 )
Epeak [keV] : 152.383      ( -26.4766 53.6952 )
Norm@50keV  : 0.532085    ( -0.0864664   0.107242 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          36.28 using 59 PHA bins.
# Reduced chi-squared =         0.6479 for     56 degrees of freedom 
# Null hypothesis probability =   9.810974e-01
 
Photon flux (15-150 keV)    in 1 sec: 37.5933 ( -1.0858  1.0886 ) ph/cm2/s
Energy fluence (15-150 keV)             : 3.24085e-06 ( 0  0 ) ergs/cm2

Band function

Time interval is from    1.692 sec. to    2.692 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -0.290797   ( -0.616709   1.36193 )
beta        : -1.43564    ( 1.43352   0.11062 )
Epeak [keV] : 85.9866      ( -37.2037 114.54 )
Norm@50keV   : 0.969261    ( -0.553075   6.88336 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          35.84 using 59 PHA bins.
# Reduced chi-squared =         0.6515 for     55 degrees of freedom 
# Null hypothesis probability =   9.788873e-01
 
Photon flux (15-150 keV)    in 1 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]    : 20.2574  (  )
R^2/D10^2   : 1.72270  (   )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =         271.20 using 59 PHA bins.
# Reduced chi-squared =         4.7579 for     57 degrees of freedom 
# Null hypothesis probability =   1.217851e-29
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.356e-07   6.900e-09
25- 50  6.811e-07   2.495e-08
50-150  2.075e-06   8.100e-08
15-150  2.892e-06   7.950e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 199.363       (      )
Norm        : 163.902       (     )
------------------------------------------------------------
#Fit statistic : Chi-Squared =         221.01 using 59 PHA bins.
# Reduced chi-squared =         3.8773 for     57 degrees of freedom 
# Null hypothesis probability =   3.679039e-21
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  4.081e-07   1.085e-08
25- 50  7.851e-07   2.150e-08
50-150  1.722e-06   4.500e-08
15-150  2.915e-06   7.700e-08

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 9.14927        (-1.01018      1.09839)
R1^2/D10^2  : 12.8029        (-3.48647      5.32511)
kT2 [keV]   : 32.2967        (-3.00156      4.17875)
R2^2/D10^2  : 0.292162    (-0.101753   0.123894)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          34.87 using 59 PHA bins.
# Reduced chi-squared =         0.6340 for     55 degrees of freedom 
# Null hypothesis probability =   9.844311e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  2.559e-07   2.615e-08
25- 50  7.478e-07   4.595e-08
50-150  2.245e-06   1.640e-07
15-150  3.249e-06   2.030e-07

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: 1.42939     ( -0.0629735   0.0628625 )
Norm@50keV  : 1.57204E-02    ( -0.000552818   0.00055273 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          52.37 using 59 PHA bins.
# Reduced chi-squared =         0.9188 for     57 degrees of freedom 
# Null hypothesis probability =   6.490061e-01
 
Photon flux (15-150 keV)    in 27.47 sec: 1.92762 ( -0.0749455  0.07517 ) ph/cm2/s
Energy fluence (15-150 keV)             : 4.14846e-06 ( -1.51773e-07  1.51915e-07 ) ergs/cm2

Cutoff power-law model

Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.16201     ( -0.262499   0.248105 )
Epeak [keV] : 178.253      ( -60.8906 1068.01 )
Norm@50keV  : 2.07227E-02    ( -0.00456411   0.00623632 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          48.99 using 59 PHA bins.
# Reduced chi-squared =         0.8748 for     56 degrees of freedom 
# Null hypothesis probability =   7.352638e-01
 
Photon flux (15-150 keV)    in 27.47 sec: 1.89603 ( -0.07987  0.08028 ) ph/cm2/s
Energy fluence (15-150 keV)             : 4.10119e-06 ( -1.59766e-07  1.59244e-07 ) ergs/cm2

Band function

 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -1.17570   ( -0.0952509   0.164762 )
beta        : -9.35460    ( 9.36969   19.3697 )
Epeak [keV] : 185.374      ( -39.2394 230.023 )
Norm@50keV   : 2.04141E-02    ( -0.000716466   0.00595393 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          49.00 using 59 PHA bins.
# Reduced chi-squared =         0.8908 for     55 degrees of freedom 
# Null hypothesis probability =   7.020996e-01
 
Photon flux (15-150 keV)    in 27.47 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)  = 9.90e-07
S(50-100 keV) = 1.47e-06

T90 vs. Hardness ratio plot

T90                                   = 20.432000041008 sec.
Hardness ratio (energy fluence ratio) = 1.48485

Color vs. Color plot

Count Ratio  (25-50 keV) / (15-25 keV) = 1.57783
Count Ratio (50-100 keV) / (15-25 keV) = 1.44803

Mask shadow pattern

IMX = -9.322627058378252E-01, IMY = 3.481684036310416E-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:
-375.203410 -322.332200
-239.504000 0.152000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
 83.6266  22.0095    0.6  50.4 -171.9  11.9818  18.3    0.5	Crab                          
115.8749  40.4632    2.6  17.7 -179.1   1.1101   4.4 ------	UNKNOWN

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

Time interval of the image:
0.152000 27.624000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
 83.6289  21.8250    0.0  50.5 -172.1   0.2378   1.1   11.4	Crab                          
139.2645   9.1754    2.4  39.4  107.9   1.3863   4.8 ------	UNKNOWN                       
157.4625  28.5758    2.2  24.9   65.9   0.5421   5.2 ------	UNKNOWN                       
190.5623  29.8086    2.6  43.8   25.2   0.7146   4.4 ------	UNKNOWN                       
 94.2929   8.5477    2.9  54.2  167.2   1.6855   4.0 ------	UNKNOWN                       
114.4034  45.7126    2.4  16.3 -161.3   0.3633   4.8 ------	UNKNOWN                       
 81.3274  32.4885    0.3  44.9 -159.5   6.3777  43.1 ------	UNKNOWN                       
 70.4680  26.3525    2.2  56.0 -157.6   1.8459   5.3 ------	UNKNOWN                       
 63.3025  37.7057    2.1  53.4 -142.2   2.2706   5.4 ------	UNKNOWN

Post-slew image of 15-350 keV band

Time interval of the image:
466.896600 722.646000
900.496000 962.567900
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
244.8271 -15.6195    5.0  24.3   63.3   8.4976   2.3    8.9	Sco X-1                       
254.3807  35.3569    6.1  47.4  152.9 -19.7876  -1.9    3.9	Her X-1                       
256.0303 -38.0119  178.0  30.4    9.8   0.2101   0.1   10.3	4U 1700-377                   
256.4524 -36.4299    5.4  28.8   10.6  -6.8057  -2.1    0.9	GX 349+2                      
263.0813 -24.7537   10.0  15.8    9.5   3.1960   1.2    4.0	GX 1+4                        
264.5637 -44.5760    7.1  34.8   -5.2   5.9202   1.6   10.8	4U 1735-44                    
268.2187  -1.4426    6.5   8.6  163.5  -5.1257  -1.8    9.0	SW J1753.5-0127               
270.1483 -24.9517   10.1  15.0  -14.6  -3.2417  -1.1   10.6	GX 5-1                        
270.1354 -25.8238    4.9  15.9  -14.3   6.5279   2.4   10.2	GRS 1758-258                  
273.9523 -13.9625    5.2   6.2  -60.5   6.7260   2.2    5.4	GX 17+2                       
275.9011 -30.2156    5.8  21.2  -27.3   6.0130   2.0    9.2	H1820-303                     
284.9110 -24.7687   10.1  21.1  -54.3   3.6429   1.1   11.4	HT1900.1-2455                 
288.7259  10.8141   20.6  28.5 -147.1  -2.0419  -0.6    9.0	GRS 1915+105                  
299.7056  35.2258   11.2  53.7 -159.7 -10.2409  -1.0    5.8	Cyg X-1                       
262.9925 -33.8340   29.1  24.5    1.5  -1.2851  -0.4    0.2	GX 354-0                      
229.6578  -7.0049    3.3  39.1   80.4  44.0240   3.5 ------	UNKNOWN                       
233.4884 -19.6604    2.8  35.7   59.3  26.2445   4.1 ------	UNKNOWN                       
236.8420 -27.1063    3.2  34.9   45.4  18.5416   3.6 ------	UNKNOWN                       
274.3514 -22.1354    2.8  13.2  -32.8  11.9053   4.1 ------	UNKNOWN                       
259.8167 -66.3876    2.5  56.8   -6.4  56.0883   4.6 ------	UNKNOWN                       
284.8201 -68.5502    3.7  59.5  -17.4  59.9582   3.1 ------	UNKNOWN                       
	UNKNOWN                       
	UNKNOWN

Plot creation:
Sat May 30 14:28:29 EDT 2015