batgrbproduct analysis for trigger=436429

batgrbproduct Analysis for Trigger=436429

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): Fri Jan 17 15:39:08 EST 2014
             Host Name: batevent1
   Current Working Dir: /local/data/batevent/batevent_reproc/trigger436429
======================================================================

  Trigger: 00436429      Segment: 000

  BAT Trigger Time: 309004373.696   [s; MET]
      Trigger Stop: 309004374.72   [s; MET]
               UTC: 2010-10-17T10:32:47.416220    [includes UTCF correction] 
       Where From?: TDRSS position message

  BAT 
    RA: 291.377889105661   Dec: -35.1409002465417  [deg; J2000]

     Catalogged Source?: NO
     Point Source?:      YES
     GRB Indicated?:     YES    [ by BAT flight software ]
     Image S/N Ratio:    20.22
     Image Trigger?:     NO
     Rate S/N Ratio:     95.7548954362125  [ if not an image trigger ]
     Image S/N Ratio:    20.22

  Flight Position:   [ source = BAT ]
    RA: 291.377889105661   Dec: -35.1409002465417  [deg; J2000]

  Ground Position:   [ source = BAT pre-slew burst ]
    RA: 291.376741931395   Dec: -35.1404334548356  [deg; J2000]  
        { 19h 25m 30.4s , -35d 08' 25.6" }
         +/- 0.531248327955595 [arcmin] (estimated 90% radius based on SNR)
         +/- 0.107271035281423 [arcmin] (formal 1-sigma fit error)
    SNR: 75.0845209126248
 
  Angular difference between Flight and Ground position is 0.062869 arcmin
 
  Partial Coding Fraction: 0.4375    [ including projection effects ]

  Duration
     T90: 72.2319999337196 +/- 3.66001587388552
        Measured from: -1.87199997901917
                   to: 70.3599999547005     [s; relative to TRIGTIME]
     T50: 20.4479999542236 +/- 0.517006751342904
        Measured from: 4.64399999380112
                   to: 25.0919999480247     [s; relative to TRIGTIME]



  Fluence
     Peak Flux  (peak 1 second)
        Measured from: 2.58000004291534     
                   to: 3.58000004291534     [s; relative to TRIGTIME]
     Total Fluence        
        Measured from: -5.4879999756813     
                   to: 130.568000018597     [s; relative to TRIGTIME]
     
             Band 1     Band 2     Band 3     Band 4
              15-25      25-50     50-100    100-350     keV
 Total     6.318273   9.463312   7.943354   2.415513
           0.086072   0.093788   0.087256   0.069807 [error]
 Peak      0.206983   0.374560   0.420962   0.147216
           0.012394   0.015207   0.016297   0.013200 [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 2.17e-06 4.17e-06 6.20e-06 1.99e-05 1.75e-05 3.24e-05   erg/cm2
              Error 7.79e-08 8.67e-08 1.06e-07 8.18e-07 2.74e-07 8.42e-07   erg/cm2
Peak flux Power-law 2.25e+00 2.88e+00 2.69e+00 4.43e+00 9.30e+00 1.22e+01   ph/cm2/s
              Error 1.91e-01 1.48e-01 1.31e-01 4.64e-01 4.09e-01 5.77e-01   ph/cm2/s
 
Fluence   Cutoff-PL 2.13e-06 4.18e-06 6.25e-06 1.85e-05 1.75e-05 3.11e-05   erg/cm2
              Error 7.83e-08 7.67e-08 1.30e-07 1.91e-06 2.99e-07 2.02e-06   erg/cm2
Peak flux Cutoff-PL 2.03e+00 2.93e+00 2.82e+00 3.06e+00 9.16e+00 1.08e+01   ph/cm2/s
              Error 2.43e-01 1.60e-01 1.65e-01 8.44e-01 4.23e-01 9.46e-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    1.427    0.030    -      -           1.34e-02 2.15e-04   36.020 57
CPL   1.424    0.000    10000.0    0.0      1.34e-02 2.12e-04   35.980 56
 
 
=== 1-s peak spectral analysis ===
 
Model Ph_index Ph_90err Epeak  Epeak_90err Norm     Nomr_90err chi2   dof
PL    1.096    0.075    -      -           8.02e-02 3.45e-03   53.280 57
CPL   0.707    0.300     191.8  202.6      1.20e-01 3.64e-02   47.890 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: 72.128000 sec.
T50 in the 50-300 keV band: 18.368000 sec.

 
=== Table of the duration information ==
 
        Value   tstart    tstop
T100  136.056   -5.488  130.568
T90    72.232   -1.872   70.360
T50    20.448    4.644   25.092
Peak    1.000    2.580    3.580

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
  291.3767   -35.1404   0.0026    36.6142   -48.5428        12.8687436     75.085 TRIG_00436429                 
 
Foreground time interval of the image:
 -5.488  12.405 (delta_t =  17.893 [sec])
Background time interval of the image:
-87.795  -5.488 (delta_t =  82.307 [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 1.024000

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 1.024000

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 1.024000

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)

The mask-weighted light curves based on cleaned DPHs

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   -5.488 sec. to  130.568 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.42713     ( -0.030278   0.0302075 )
Norm@50keV  : 1.33772E-02    ( -0.000214991   0.000214654 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          36.02 using 59 PHA bins.
# Reduced chi-squared =         0.6319 for     57 degrees of freedom 
# Null hypothesis probability =   9.865024e-01
 
Photon flux (15-150 keV)    in 136.1 sec: 1.63941 ( -0.031373  0.0314961 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.74976e-05 ( -2.73818e-07  2.73855e-07 ) ergs/cm2

Cutoff power-law model

Time interval is from   -5.488 sec. to  130.568 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.42362     (     )
Epeak [keV] : 9999.99      (   )
Norm@50keV  : 1.34227E-02    ( -0.000215035   0.000208628 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          35.98 using 59 PHA bins.
# Reduced chi-squared =         0.6424 for     56 degrees of freedom 
# Null hypothesis probability =   9.828119e-01
 
Photon flux (15-150 keV)    in 136.1 sec: 1.63401 ( -0.02877  0.03474 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.74541e-05 ( -2.76691e-07  3.20379e-07 ) ergs/cm2

Band function

Time interval is from   -5.488 sec. to  130.568 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -0.493232   ( 0.915504   5.8696 )
beta        : -1.44426    ( -0.773623   0.0427149 )
Epeak [keV] : 49.1722      ( -49.1795 174.541 )
Norm@50keV   : 5.48758E-02    ( -0.0548315   709.259 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          33.47 using 59 PHA bins.
# Reduced chi-squared =         0.6086 for     55 degrees of freedom 
# Null hypothesis probability =   9.903499e-01
 
Photon flux (15-150 keV)    in 136.1 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]    : 19.5521  (  )
R^2/D10^2   : 7.26192E-02  (   )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =         890.06 using 59 PHA bins.
# Reduced chi-squared =         15.615 for     57 degrees of freedom 
# Null hypothesis probability =  6.690086e-150
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  7.348e-07   2.613e-08
25- 50  3.605e-06   9.459e-08
50-150  1.018e-05   2.361e-07
15-150  1.452e-05   2.450e-07

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 199.363       (      )
Norm        : 6.94484       (     )
------------------------------------------------------------
#Fit statistic : Chi-Squared =         154.68 using 59 PHA bins.
# Reduced chi-squared =         2.7137 for     57 degrees of freedom 
# Null hypothesis probability =   5.887692e-11
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  2.354e-06   4.287e-08
25- 50  4.528e-06   8.234e-08
50-150  9.930e-06   1.858e-07
15-150  1.681e-05   3.062e-07

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 8.66415        (-0.544395      0.576045)
R1^2/D10^2  : 0.778635        (-0.147071      0.19079)
kT2 [keV]   : 34.0804        (-2.31092      2.86622)
R2^2/D10^2  : 8.92801E-03    (-0.00210801   0.00244532)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          57.98 using 59 PHA bins.
# Reduced chi-squared =          1.054 for     55 degrees of freedom 
# Null hypothesis probability =   3.659596e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.720e-06   1.007e-07
25- 50  4.352e-06   1.313e-07
50-150  1.120e-05   3.641e-07
15-150  1.728e-05   4.491e-07

Peak spectrum fit

Power-law model

Time interval is from    2.580 sec. to    3.580 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.09646     ( -0.075028   0.0748746 )
Norm@50keV  : 8.02229E-02    ( -0.00345279   0.00345226 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          53.28 using 59 PHA bins.
# Reduced chi-squared =         0.9347 for     57 degrees of freedom 
# Null hypothesis probability =   6.155339e-01
 
Photon flux (15-150 keV)    in 1 sec: 9.30216 ( -0.409251  0.409525 ) ph/cm2/s
Energy fluence (15-150 keV)             : 8.39698e-07 ( -4.03225e-08  4.04299e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from    2.580 sec. to    3.580 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 0.706629     ( -0.310236   0.29027 )
Epeak [keV] : 191.833      ( -60.0286 345.224 )
Norm@50keV  : 0.119514    ( -0.0299849   0.0428076 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          47.89 using 59 PHA bins.
# Reduced chi-squared =         0.8551 for     56 degrees of freedom 
# Null hypothesis probability =   7.713113e-01
 
Photon flux (15-150 keV)    in 1 sec: 9.15548 ( -0.42247  0.42265 ) ph/cm2/s
Energy fluence (15-150 keV)             : 8.27242e-07 ( -4.2201e-08  4.2072e-08 ) ergs/cm2

Band function

Time interval is from    2.580 sec. to    3.580 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -0.706515   ( -0.22881   0.328143 )
beta        : -10.0000    ( 10   20 )
Epeak [keV] : 191.760      ( -59.9722 345.313 )
Norm@50keV   : 0.119525    ( -0.030036   0.0427917 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          47.89 using 59 PHA bins.
# Reduced chi-squared =         0.8707 for     55 degrees of freedom 
# Null hypothesis probability =   7.406721e-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]    : 21.1862  (  )
R^2/D10^2   : 0.371171  (   )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =         130.11 using 59 PHA bins.
# Reduced chi-squared =         2.2826 for     57 degrees of freedom 
# Null hypothesis probability =   1.215812e-07
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  3.136e-08   2.570e-09
25- 50  1.621e-07   9.650e-09
50-150  5.425e-07   3.785e-08
15-150  7.360e-07   3.895e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 199.363       (      )
Norm        : 37.8443       (     )
------------------------------------------------------------
#Fit statistic : Chi-Squared =         149.26 using 59 PHA bins.
# Reduced chi-squared =         2.6186 for     57 degrees of freedom 
# Null hypothesis probability =   3.388591e-10
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  9.424e-08   4.595e-09
25- 50  1.813e-07   8.750e-09
50-150  3.976e-07   2.075e-08
15-150  6.731e-07   3.480e-08

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 7.06178        (-1.20601      1.4093)
R1^2/D10^2  : 6.23824        (-2.802      5.88838)
kT2 [keV]   : 29.7346        (-3.01533      4.05097)
R2^2/D10^2  : 0.110712    (-0.0383038   0.0479093)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          41.55 using 59 PHA bins.
# Reduced chi-squared =         0.7554 for     55 degrees of freedom 
# Null hypothesis probability =   9.099141e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  6.583e-08   1.482e-08
25- 50  1.649e-07   2.115e-08
50-150  6.051e-07   6.505e-08
15-150  8.358e-07   9.560e-08

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

Power-law model

 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.19077     ( -0.0330796   0.0329668 )
Norm@50keV  : 4.96817E-02    ( -0.000899266   0.000897249 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          39.83 using 59 PHA bins.
# Reduced chi-squared =         0.6988 for     57 degrees of freedom 
# Null hypothesis probability =   9.591727e-01
 
Photon flux (15-150 keV)    in 17.89 sec: 5.82416 ( -0.115356  0.115632 ) ph/cm2/s
Energy fluence (15-150 keV)             : 9.04096e-06 ( -1.61418e-07  1.61489e-07 ) ergs/cm2

Cutoff power-law model

Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.13022     ( -0.132776   0.072091 )
Epeak [keV] : 885.843      ( -886.056 -886.056 )
Norm@50keV  : 5.26041E-02    ( -0.00127659   0.0068331 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          39.20 using 59 PHA bins.
# Reduced chi-squared =         0.7001 for     56 degrees of freedom 
# Null hypothesis probability =   9.569346e-01
 
Photon flux (15-150 keV)    in 17.89 sec: 5.82673 ( -0.1416  0.11055 ) ph/cm2/s
Energy fluence (15-150 keV)             : 9.02481e-06 ( -1.67307e-07  1.6423e-07 ) ergs/cm2

Band function

 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : 1.04462   ( -3.06922   -0.719754 )
beta        : -1.20685    ( -0.0389498   0.0369423 )
Epeak [keV] : 35.2324      ( -10.2805 72.0031 )
Norm@50keV   : 2.06148    ( -2.07478   1228.66 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          36.07 using 59 PHA bins.
# Reduced chi-squared =         0.6559 for     55 degrees of freedom 
# Null hypothesis probability =   9.772996e-01
 
Photon flux (15-150 keV)    in 17.89 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)  = 4.17e-06
S(50-100 keV) = 6.20e-06

T90 vs. Hardness ratio plot

T90                                   = 72.2319999337196 sec.
Hardness ratio (energy fluence ratio) = 1.48681

Color vs. Color plot

Count Ratio  (25-50 keV) / (15-25 keV) = 1.49777
Count Ratio (50-100 keV) / (15-25 keV) = 1.2572

Mask shadow pattern

IMX = 4.919435740203281E-01, IMY = 5.568786709476784E-01

TIME vs. PHA plot around the trigger time

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.024000

TIME vs. DetID plot around the trigger time

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.024000

100 us light curve (15-350 keV)

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.024000

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:
-87.795410 -5.488000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
285.1561 -24.9888    7.2  46.0  -38.5  -0.3362  -1.6    7.7	HT1900.1-2455                 
342.8159 -34.6587    2.3   6.5   90.3   0.4205   5.0 ------	UNKNOWN                       
284.9946 -78.8026    3.2  44.2 -117.9   1.3695   3.7 ------	UNKNOWN

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

Time interval of the image:
-5.488000 12.404590
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
285.0548 -24.7574    6.8  46.2  -38.3  -0.4890  -1.7    9.8	HT1900.1-2455                 
  9.5546 -29.1200    3.4  28.2  127.2   0.4029   3.4 ------	UNKNOWN                       
  9.2486 -63.3341    2.8  30.1 -158.6   0.4787   4.1 ------	UNKNOWN                       
299.2617 -17.3331    2.4  40.0  -17.9   0.7685   4.8 ------	UNKNOWN                       
 20.4876 -68.3878    2.4  36.7 -155.4   0.6419   4.7 ------	UNKNOWN                       
291.3767 -35.1404    0.2  36.6  -48.5  12.8686  75.1 ------	UNKNOWN

Post-slew image of 15-350 keV band

Time interval of the image:
70.004590 154.470900
155.304000 962.343300
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
256.0341 -37.8469    2.3  28.4  -98.6   3.5538   5.0    2.3	4U 1700-377                   
256.4912 -36.4742    3.0  28.2  -95.7   2.8566   3.8    4.1	GX 349+2                      
262.9807 -24.7623    1.9  26.6  -67.4   3.6888   6.0    1.8	GX 1+4                        
264.8649 -44.5009    6.2  22.3 -115.5   1.0415   1.9    6.0	4U 1735-44                    
268.3402  -1.4844    2.5  39.9  -30.2   3.4539   4.5    2.5	SW J1753.5-0127               
270.3341 -25.1828    3.7  20.7  -59.6   1.5960   3.2    6.8	GX 5-1                        
270.2710 -25.8413    3.1  20.4  -61.3   1.9082   3.8    6.1	GRS 1758-258                  
274.0008 -14.0405    2.6  26.3  -33.6   2.2527   4.4    0.4	GX 17+2                       
275.9202 -30.3191    2.3  13.9  -66.6   2.6344   5.1    2.9	H1820-303                     
285.0808 -24.9133    3.7  11.6  -22.4   1.5817   3.1    2.5	HT1900.1-2455                 
288.7901  10.9466    0.9  46.1    3.8  14.3785  13.0    0.5	GRS 1915+105                  
262.9511 -33.8002    2.0  23.4  -87.6   3.6134   5.7    2.8	GX 354-0                      
319.1765   2.8422    3.5  46.0   47.7  10.1798   3.3 ------	UNKNOWN                       
332.5738 -60.3626    3.0  36.4  154.1   3.7187   3.9 ------	UNKNOWN                       
284.5344  -0.7623    3.8  35.0   -4.6   2.1275   3.0 ------	UNKNOWN                       
267.0142 -24.8491    2.1  23.4  -63.2   3.5441   5.6 ------	UNKNOWN                       
255.1966 -41.6395    1.9  28.9 -106.6   4.5468   5.9 ------	UNKNOWN

Plot creation:
Sat May 30 23:40:45 EDT 2015