batgrbproduct analysis for trigger=586289

batgrbproduct Analysis for Trigger=586289

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): Tue Mar  4 10:49:02 EST 2014
             Host Name: batevent1
   Current Working Dir: /local/data/batevent/batevent_reproc/trigger586289
======================================================================

  Trigger: 00586289      Segment: 000

  BAT Trigger Time: 413814195.456   [s; MET]
      Trigger Stop: 413814203.648   [s; MET]
               UTC: 2014-02-11T12:23:03.824220    [includes UTCF correction] 
       Where From?: TDRSS position message

  BAT 
    RA: 124.230447244537   Dec: 20.2436200277782  [deg; J2000]

     Catalogged Source?: NO
     Point Source?:      YES
     GRB Indicated?:     YES    [ by BAT flight software ]
     Image S/N Ratio:    10.26
     Image Trigger?:     NO
     Rate S/N Ratio:     13.228756555323  [ if not an image trigger ]
     Image S/N Ratio:    10.26

  Flight Position:   [ source = BAT ]
    RA: 124.230447244537   Dec: 20.2436200277782  [deg; J2000]

  Ground Position:   [ source = BAT pre-slew burst ]
    RA: 124.232921756996   Dec: 20.235449467908  [deg; J2000]  
        { 08h 16m 55.9s , +20d 14' 07.6" }
         +/- 1.39216314473229 [arcmin] (estimated 90% radius based on SNR)
         +/- 0.63613875310429 [arcmin] (formal 1-sigma fit error)
    SNR: 18.9603680045216
 
  Angular difference between Flight and Ground position is 0.509641 arcmin
 
  Partial Coding Fraction: 0.8125    [ including projection effects ]

  Duration
     T90: 109.531999945641 +/- 26.249381548809
        Measured from: -14.2759999632835
                   to: 95.255999982357     [s; relative to TRIGTIME]
     T50: 48.2399999499321 +/- 6.60201180093168
        Measured from: 1.04800003767014
                   to: 49.2879999876022     [s; relative to TRIGTIME]



  Fluence
     Peak Flux  (peak 1 second)
        Measured from: 0.904000043869019     
                   to: 1.90400004386902     [s; relative to TRIGTIME]
     Total Fluence        
        Measured from: -19.2399999499321     
                   to: 121.808000028133     [s; relative to TRIGTIME]
     
             Band 1     Band 2     Band 3     Band 4
              15-25      25-50     50-100    100-350     keV
 Total     1.482067   1.372972   0.657660   0.117068
           0.082786   0.084315   0.073460   0.066047 [error]
 Peak      0.044365   0.028315   0.015222   0.005832
           0.007202   0.007511   0.006426   0.005673 [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 4.45e-07 5.78e-07 5.51e-07 9.30e-07 1.88e-06 2.50e-06   erg/cm2
              Error 4.65e-08 4.10e-08 7.04e-08 2.37e-07 1.58e-07 3.12e-07   erg/cm2
Peak flux Power-law 3.88e-01 2.42e-01 9.67e-02 5.22e-02 7.53e-01 7.79e-01   ph/cm2/s
              Error 1.06e-01 6.09e-02 4.53e-02 4.46e-02 1.73e-01 1.84e-01   ph/cm2/s
 
Fluence   Cutoff-PL 4.28e-07 6.04e-07 5.39e-07 4.58e-07 1.80e-06 2.03e-06   erg/cm2
              Error 5.24e-08 5.44e-08 7.81e-08 -------- 1.90e-07 5.16e-07   erg/cm2
Peak flux Cutoff-PL 3.74e-01 2.84e-01 7.61e-02 6.02e-03 7.39e-01 7.39e-01   ph/cm2/s
              Error 1.14e-01 8.27e-02 6.17e-02 4.09e-02 1.69e-01 1.70e-01   ph/cm2/s
 
Fluence        Band -------- -------- -------- -------- -------- --------   erg/cm2
              Error -------- -------- -------- -------- -------- --------   erg/cm2
Peak flux      Band -------- -------- -------- -------- -------- --------   ph/cm2/s
              Error -------- -------- -------- -------- -------- --------   ph/cm2/s

 
=== Time-averaged spectral analysis ===
 
Model Ph_index Ph_90err Epeak  Epeak_90err Norm     Nomr_90err chi2   dof
PL    2.071    0.143    -      -           1.44e-03 1.32e-04   48.030 57
CPL   1.676    0.593      34.2   -2.8      2.43e-03 2.14e-03   46.580 56
 
 
=== 1-s peak spectral analysis ===
 
Model Ph_index Ph_90err Epeak  Epeak_90err Norm     Nomr_90err chi2   dof
PL    2.321    0.462    -      -           4.26e-03 1.54e-03   51.970 57
CPL   0.847    2.603      27.0    0.0      3.89e-02 0.00e+00   50.140 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: 24.192000 sec.
T50 in the 50-300 keV band: 11.456000 sec.

 
=== Table of the duration information ==
 
        Value   tstart    tstop
T100  141.048  -19.240  121.808
T90   109.532  -14.276   95.256
T50    48.240    1.048   49.288
Peak    1.000    0.904    1.904

Click here for the BAT GCN circular template

Image

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

#   RAcent    DECcent   POSerr    Theta     Phi              Peak Cts       SNR   Name
  124.2329    20.2354   0.0101    24.7213    20.0118         3.7022089     18.960 TRIG_00586289                 
 
Foreground time interval of the image:
-19.240 121.808 (delta_t = 141.048 [sec])
Background time interval of the image:
-439.255 -423.944 (delta_t =  15.311 [sec])
-239.456 -19.240 (delta_t = 220.216 [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 8.192000

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 8.192000

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 8.192000

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  -19.240 sec. to  121.808 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 2.07054     ( -0.140061   0.145355 )
Norm@50keV  : 1.44182E-03    ( -0.000132607   0.000130401 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          48.03 using 59 PHA bins.
# Reduced chi-squared =         0.8426 for     57 degrees of freedom 
# Null hypothesis probability =   7.954841e-01
 
Photon flux (15-150 keV)    in 141 sec: 0.223594 ( -0.0159231  0.0159352 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.88383e-06 ( -1.57143e-07  1.5965e-07 ) ergs/cm2

Cutoff power-law model

Time interval is from  -19.240 sec. to  121.808 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.67629     ( -0.633818   0.552595 )
Epeak [keV] : 34.2175      ( -28.5475 -34.2175 )
Norm@50keV  : 2.42716E-03    ( -0.00113773   0.00314609 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          46.58 using 59 PHA bins.
# Reduced chi-squared =         0.8318 for     56 degrees of freedom 
# Null hypothesis probability =   8.110583e-01
 
Photon flux (15-150 keV)    in 141 sec: 0.219146 ( -0.017037  0.017026 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.80329e-06 ( -1.86966e-07  1.93889e-07 ) ergs/cm2

Band function

Time interval is from  -19.240 sec. to  121.808 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -1.67632   ( 1.7719   0.618417 )
beta        : -10.00000    ( 10   5.00933e-13 )
Epeak [keV] : 34.2101      ( -10.1071 -34.2101 )
Norm@50keV   : 2.42658E-03    ( -0.000170604   0.0031504 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          46.58 using 59 PHA bins.
# Reduced chi-squared =         0.8469 for     55 degrees of freedom 
# Null hypothesis probability =   7.833635e-01
 
Photon flux (15-150 keV)    in 141 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]    : 9.74941  (-0.840207  0.923905)
R^2/D10^2   : 0.109769  (-0.0326324   0.0464719)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          87.12 using 59 PHA bins.
# Reduced chi-squared =          1.528 for     57 degrees of freedom 
# Null hypothesis probability =   6.263747e-03
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  2.969e-07   3.553e-08
25- 50  7.118e-07   5.802e-08
50-150  3.450e-07   7.071e-08
15-150  1.354e-06   1.156e-07

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 60.1753       (-12.1083      16.7616)
Norm        : 1.15432       (-0.141411     0.155654)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          47.52 using 59 PHA bins.
# Reduced chi-squared =         0.8336 for     57 degrees of freedom 
# Null hypothesis probability =   8.104069e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  4.093e-07   4.174e-08
25- 50  6.234e-07   4.660e-08
50-150  7.111e-07   1.304e-07
15-150  1.744e-06   1.607e-07

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 4.84821        (-1.15231      1.37224)
R1^2/D10^2  : 1.13586        (-0.684908      2.75975)
kT2 [keV]   : 16.1937        (-3.00482      5.13481)
R2^2/D10^2  : 1.16658E-02    (-0.00796231   0.0132834)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          47.64 using 59 PHA bins.
# Reduced chi-squared =         0.8661 for     55 degrees of freedom 
# Null hypothesis probability =   7.491065e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  4.327e-07   1.554e-07
25- 50  5.860e-07   1.680e-07
50-150  7.035e-07   2.721e-07
15-150  1.722e-06   5.257e-07

Peak spectrum fit

Power-law model

Time interval is from    0.904 sec. to    1.904 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 2.32110     ( -0.420349   0.503322 )
Norm@50keV  : 4.26110E-03    ( -0.00154219   0.00153709 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          51.97 using 59 PHA bins.
# Reduced chi-squared =         0.9118 for     57 degrees of freedom 
# Null hypothesis probability =   6.636302e-01
 
Photon flux (15-150 keV)    in 1 sec: 0.753498 ( -0.173063  0.173372 ) ph/cm2/s
Energy fluence (15-150 keV)             : 4.08806e-08 ( -1.18017e-08  1.2768e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from    0.904 sec. to    1.904 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 0.846559     ( -3.72313   1.48223 )
Epeak [keV] : 26.9885      (   )
Norm@50keV  : 3.88637E-02    (     )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          50.14 using 59 PHA bins.
# Reduced chi-squared =         0.8954 for     56 degrees of freedom 
# Null hypothesis probability =   6.951274e-01
 
Photon flux (15-150 keV)    in 1 sec: 0.738820 ( -0.167514  0.170821 ) ph/cm2/s
Energy fluence (15-150 keV)             : 3.60104e-08 ( -1.07786e-08  1.33484e-08 ) ergs/cm2

Band function

Time interval is from    0.904 sec. to    1.904 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : 5.00000   ( -8.55449   -5 )
beta        : -2.92132    ( -1.4715   0.702719 )
Epeak [keV] : 23.3759      ( -5.24375 4.43671 )
Norm@50keV   : 1620.25    ( -355.914   7124.14 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          48.18 using 59 PHA bins.
# Reduced chi-squared =         0.8761 for     55 degrees of freedom 
# Null hypothesis probability =   7.306161e-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]    : 7.08636  (-1.68674  2.3553)
R^2/D10^2   : 1.39690  (-0.951165   2.84893)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          52.08 using 59 PHA bins.
# Reduced chi-squared =         0.9137 for     57 degrees of freedom 
# Null hypothesis probability =   6.596660e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.141e-08   5.154e-09
25- 50  1.600e-08   8.398e-09
50-150  2.771e-09   2.033e-09
15-150  3.018e-08   1.437e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 36.7580       (-15.5131      33.5305)
Norm        : 5.27797       (-1.82935     3.20122)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          50.28 using 59 PHA bins.
# Reduced chi-squared =         0.8822 for     57 degrees of freedom 
# Null hypothesis probability =   7.231953e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.176e-08   3.834e-09
25- 50  1.489e-08   5.633e-09
50-150  1.048e-08   7.230e-09
15-150  3.713e-08   1.602e-08

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 5.01889        (-2.01565      2.4773)
R1^2/D10^2  : 4.10912        (-3.13389      22.7979)
kT2 [keV]   : 14.2602        (-7.37055      37.1578)
R2^2/D10^2  : 4.83856E-02    (-0.0475538   0.950561)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          48.87 using 59 PHA bins.
# Reduced chi-squared =         0.8886 for     55 degrees of freedom 
# Null hypothesis probability =   7.064602e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.222e-08   7.035e-09
25- 50  1.454e-08   7.490e-09
50-150  1.089e-08   8.075e-09
15-150  3.766e-08   2.061e-08

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

Power-law model

 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 2.07054     ( -0.140061   0.145355 )
Norm@50keV  : 1.44182E-03    ( -0.000132607   0.000130401 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          48.03 using 59 PHA bins.
# Reduced chi-squared =         0.8426 for     57 degrees of freedom 
# Null hypothesis probability =   7.954841e-01
 
Photon flux (15-150 keV)    in 141 sec: 0.223594 ( -0.0159231  0.0159352 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.88383e-06 ( -1.57143e-07  1.5965e-07 ) ergs/cm2

Cutoff power-law model

Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.67629     ( -0.633818   0.552595 )
Epeak [keV] : 34.2175      ( -28.5475 -34.2175 )
Norm@50keV  : 2.42716E-03    ( -0.00115768   0.00314477 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          46.58 using 59 PHA bins.
# Reduced chi-squared =         0.8318 for     56 degrees of freedom 
# Null hypothesis probability =   8.110583e-01
 
Photon flux (15-150 keV)    in 141 sec: 0.219146 ( -0.017037  0.017026 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.80329e-06 ( -1.86966e-07  1.93889e-07 ) ergs/cm2

Band function

 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -1.67632   ( 1.7719   0.618417 )
beta        : -10.00000    ( 10   3.55271e-15 )
Epeak [keV] : 34.2101      ( -10.1071 -34.2101 )
Norm@50keV   : 2.42658E-03    ( -0.000170604   0.0031504 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          46.58 using 59 PHA bins.
# Reduced chi-squared =         0.8469 for     55 degrees of freedom 
# Null hypothesis probability =   7.833635e-01
 
Photon flux (15-150 keV)    in 141 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)  = 5.78e-07
S(50-100 keV) = 5.51e-07

T90 vs. Hardness ratio plot

T90                                   = 109.531999945641 sec.
Hardness ratio (energy fluence ratio) = 0.953287

Color vs. Color plot

Count Ratio  (25-50 keV) / (15-25 keV) = 0.92639
Count Ratio (50-100 keV) / (15-25 keV) = 0.443745

Mask shadow pattern

IMX = 4.326020253788569E-01, IMY = -1.575552783659648E-01

TIME vs. PHA plot around the trigger time

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 8.192000

TIME vs. DetID plot around the trigger time

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 8.192000

100 us light curve (15-350 keV)

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 8.192000

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:
-439.255400 -423.944400
-239.456000 -19.240000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
 83.6136  22.0169    0.9  51.4  -27.0   6.4418  12.7    1.1	Crab                          
135.5305 -40.5557    0.9  37.0 -157.9   3.5211  13.4    0.1	Vela X-1                      
 97.1589 -34.8762    3.1  42.6 -109.9   2.9837   3.7 ------	UNKNOWN                       
 83.8420  -3.4463    2.4  44.9  -60.3   4.1175   4.8 ------	UNKNOWN

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

Time interval of the image:
-19.240000 121.808000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
 83.6279  22.0512    5.4  51.4  -26.9   1.0678   2.1    2.2	Crab                          
135.4021 -40.5711    4.1  37.0 -157.8   0.6885   2.8    5.8	Vela X-1                      
124.2329  20.2355    0.6  24.7   20.0   3.7021  19.0 ------	UNKNOWN                       
 85.6352  -7.3368    2.7  43.1  -65.9   3.1271   4.3 ------	UNKNOWN

Post-slew image of 15-350 keV band

Time interval of the image:
605.744590 826.444600
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
245.0061 -15.6515    0.7  28.0   85.7   7.4330  16.8    1.7	Sco X-1                       
254.5389  35.4263   16.6  52.8  162.7  -0.8717  -0.7    6.4	Her X-1                       
256.0399 -37.7042    7.9  28.5   33.4  -0.4788  -1.5    8.8	4U 1700-377                   
256.5681 -36.5847    6.2  27.4   34.2   0.5927   1.9   11.6	GX 349+2                      
263.0388 -24.7369    1.7  14.8   45.0   1.7910   6.8    1.7	GX 1+4                        
264.9253 -44.5202    6.9  31.4   15.1   0.5092   1.7    8.9	4U 1735-44                    
268.4366  -1.5160    4.6  13.7  158.5   0.6248   2.5    5.6	SW J1753.5-0127               
270.3180 -24.9290    5.5  11.4   19.8   0.5978   2.1    9.2	GX 5-1                        
270.3868 -25.6964    3.0  12.1   18.3   1.0852   3.8    5.3	GRS 1758-258                  
274.0428 -13.9290    2.8   0.2 -163.0   1.1019   4.2    6.8	GX 17+2                       
275.9527 -30.3822    3.5  16.4   -3.4   0.9074   3.3    1.7	H1820-303                     
284.8767 -24.9542   46.1  14.9  -39.0   0.0638   0.2    8.9	HT1900.1-2455                 
288.7793  10.9524    1.0  29.0 -146.3   3.1691  11.4    1.2	GRS 1915+105                  
299.6181  35.0962    7.2  54.8 -151.8   2.1818   1.6    6.5	Cyg X-1                       
263.0131 -33.7927    4.0  22.1   27.5   0.8264   2.9    2.8	GX 354-0                      
266.1372 -28.7580    1.6  16.4   27.8   1.7788   7.1 ------	UNKNOWN                       
267.1112   7.7646    2.5  22.9  164.8   1.1818   4.6 ------	UNKNOWN                       
266.9363  40.0509    2.9  54.5  176.0   4.4482   3.9 ------	UNKNOWN                       
274.1951  -0.1502    3.1  13.9 -176.6   0.9391   3.8 ------	UNKNOWN                       
281.8305 -58.6647    3.0  45.0   -3.1   1.7526   3.8 ------	UNKNOWN                       
290.8883  -2.5085    2.8  20.3 -120.6   1.1106   4.1 ------	UNKNOWN                       
	UNKNOWN

Plot creation:
Sat May 30 14:26:21 EDT 2015