batgrbproduct analysis for trigger=533060

batgrbproduct Analysis for Trigger=533060

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): Sun Nov 23 17:33:56 EST 2014
             Host Name: bat1
   Current Working Dir: /local/data/bat1/alien/Swift_3rdBATcatalog/event/batevent_reproc/trigger533060
======================================================================

  Trigger: 00533060      Segment: 000

  BAT Trigger Time: 368847732.864   [s; MET]
      Trigger Stop: 368847734.272   [s; MET]
               UTC: 2012-09-09T01:42:03.235040    [includes UTCF correction] 
       Where From?: TDRSS position message

  BAT 
    RA: 275.684892653149   Dec: -59.4263133760398  [deg; J2000]

     Catalogged Source?: NO
     Point Source?:      YES
     GRB Indicated?:     YES    [ by BAT flight software ]
     Image S/N Ratio:    7.77
     Image Trigger?:     NO
     Rate S/N Ratio:     13  [ if not an image trigger ]
     Image S/N Ratio:    7.77

  Flight Position:   [ source = BAT ]
    RA: 275.684892653149   Dec: -59.4263133760398  [deg; J2000]

  Ground Position:   [ source = BAT pre-slew burst ]
    RA: 275.72523148817   Dec: -59.4389804814466  [deg; J2000]  
        { 18h 22m 54.1s , -59d 26' 20.3" }
         +/- 2.08641847400824 [arcmin] (estimated 90% radius based on SNR)
         +/- 0.976648402226871 [arcmin] (formal 1-sigma fit error)
    SNR: 10.6372811448241
 
  Angular difference between Flight and Ground position is 1.446602 arcmin
 
  Partial Coding Fraction: 0.4882812    [ including projection effects ]

  Duration
     T90: 220.595999956131 +/- 304.966835064435
        Measured from: 253.227999985218
                   to: 473.823999941349     [s; relative to TRIGTIME]
     T50: 114.503999948502 +/- 363.404444880196
        Measured from: 297.243999958038
                   to: 411.74799990654     [s; relative to TRIGTIME]



  Fluence
     Peak Flux  (peak 1 second)
        Measured from: 0.899999976158142     
                   to: 1.89999997615814     [s; relative to TRIGTIME]
     Total Fluence        
        Measured from: -31.460000038147     
                   to: 566.708000004292     [s; relative to TRIGTIME]
     
             Band 1     Band 2     Band 3     Band 4
              15-25      25-50     50-100    100-350     keV
 Total     2.885854   3.884830   3.568242   1.009578
           0.195425   0.200093   0.185861   0.190517 [error]
 Peak      0.033339   0.076469   0.094177   0.023912
           0.009553   0.010755   0.010425   0.010719 [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 8.71e-07 1.73e-06 2.68e-06 9.13e-06 7.50e-06 1.44e-05   erg/cm2
              Error 9.07e-08 1.05e-07 1.84e-07 1.42e-06 4.52e-07 1.53e-06   erg/cm2
Peak flux Power-law 4.07e-01 5.47e-01 5.41e-01 9.64e-01 1.81e+00 2.46e+00   ph/cm2/s
              Error 1.16e-01 9.61e-02 8.10e-02 3.06e-01 2.62e-01 3.71e-01   ph/cm2/s
 
Fluence   Cutoff-PL 8.56e-07 1.75e-06 2.70e-06 8.01e-06 7.45e-06 1.33e-05   erg/cm2
              Error 8.25e-08 1.16e-07 1.98e-07 2.49e-06 4.95e-07 2.54e-06   erg/cm2
Peak flux Cutoff-PL 2.72e-01 5.73e-01 6.24e-01 3.39e-01 1.70e+00 1.81e+00   ph/cm2/s
              Error 1.48e-01 1.15e-01 1.09e-01 3.13e-01 2.81e-01 4.27e-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    1.369    0.101    -      -           1.29e-03 7.00e-05   48.110 57
CPL   1.281    0.265     416.2    0.0      1.42e-03 4.69e-04   47.980 56
 
 
=== 1-s peak spectral analysis ===
 
Model Ph_index Ph_90err Epeak  Epeak_90err Norm     Nomr_90err chi2   dof
PL    1.015    0.237    -      -           1.57e-02 2.22e-03   49.930 57
CPL  -0.411    1.431      97.8   99.1      6.52e-02 1.50e-01   45.510 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: 191.296000 sec.
T50 in the 50-300 keV band: 191.296000 sec.

 
=== Table of the duration information ==
 
        Value   tstart    tstop
T100  598.168  -31.460  566.708
T90   220.596  253.228  473.824
T50   114.504  297.244  411.748
Peak    1.000    0.900    1.900

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
  275.7252   -59.4390   0.0181    40.4914     4.1902         2.1358034     10.637 TRIG_00533060                 
 
Foreground time interval of the image:
-31.460  23.037 (delta_t =  54.497 [sec])
Background time interval of the image:
-60.864 -31.460 (delta_t =  29.404 [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 1.408000

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 1.408000

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 1.408000

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  -31.460 sec. to  566.708 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.36879     ( -0.10073   0.100446 )
Norm@50keV  : 1.28883E-03    ( -6.99931e-05   6.9938e-05 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          48.11 using 59 PHA bins.
# Reduced chi-squared =         0.8441 for     57 degrees of freedom 
# Null hypothesis probability =   7.929164e-01
 
Photon flux (15-150 keV)    in 598.2 sec: 0.155880 ( -0.00880988  0.00883635 ) ph/cm2/s
Energy fluence (15-150 keV)             : 7.49886e-06 ( -4.50514e-07  4.52832e-07 ) ergs/cm2

Cutoff power-law model

Time interval is from  -31.460 sec. to  566.708 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.28139     ( -0.395732   0.134999 )
Epeak [keV] : 416.214      ( -442.485 -442.485 )
Norm@50keV  : 1.41986E-03    ( -0.000188263   0.000749425 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          47.98 using 59 PHA bins.
# Reduced chi-squared =         0.8567 for     56 degrees of freedom 
# Null hypothesis probability =   7.684561e-01
 
Photon flux (15-150 keV)    in 598.2 sec: 0.155099 ( -0.009398  0.009314 ) ph/cm2/s
Energy fluence (15-150 keV)             : 7.45261e-06 ( -5.02727e-07  4.86995e-07 ) ergs/cm2

Band function

Time interval is from  -31.460 sec. to  566.708 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : 4.97409   ( -4.97409   -4.97409 )
beta        : -1.38876    ( -0.105944   0.104753 )
Epeak [keV] : 21.6051      ( -21.6051 5.11053 )
Norm@50keV   : 280.413    ( -15.1533   420976 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          47.25 using 59 PHA bins.
# Reduced chi-squared =         0.8591 for     55 degrees of freedom 
# Null hypothesis probability =   7.618476e-01
 
Photon flux (15-150 keV)    in 598.2 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]    : 16.9408  (  )
R^2/D10^2   : 1.16067E-02  (   )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =         122.50 using 59 PHA bins.
# Reduced chi-squared =         2.1491 for     57 degrees of freedom 
# Null hypothesis probability =   1.086180e-06
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  4.062e-07   4.301e-08
25- 50  1.792e-06   1.349e-07
50-150  3.668e-06   3.766e-07
15-150  5.867e-06   3.963e-07

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 200.000       (      )
Norm        : 0.645738       (-0.0351192     0.0351145)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          58.58 using 59 PHA bins.
# Reduced chi-squared =          1.028 for     57 degrees of freedom 
# Null hypothesis probability =   4.171827e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  9.621e-07   5.563e-08
25- 50  1.851e-06   1.229e-07
50-150  4.059e-06   7.190e-07
15-150  6.872e-06   7.618e-07

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 7.42602        (-1.50449      1.7859)
R1^2/D10^2  : 0.122893        (-0.06049      0.144851)
kT2 [keV]   : 29.9921        (-5.60713      10.9189)
R2^2/D10^2  : 1.40387E-03    (-0.000884919   0.00148499)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          50.40 using 59 PHA bins.
# Reduced chi-squared =         0.9164 for     55 degrees of freedom 
# Null hypothesis probability =   6.506044e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  8.078e-07   1.653e-07
25- 50  1.785e-06   3.194e-07
50-150  4.849e-06   1.304e-06
15-150  7.442e-06   1.580e-06

Peak spectrum fit

Power-law model

Time interval is from    0.900 sec. to    1.900 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.01501     ( -0.241091   0.232382 )
Norm@50keV  : 1.56945E-02    ( -0.00222654   0.00221698 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          49.93 using 59 PHA bins.
# Reduced chi-squared =         0.8760 for     57 degrees of freedom 
# Null hypothesis probability =   7.350502e-01
 
Photon flux (15-150 keV)    in 1 sec: 1.80846 ( -0.261117  0.262107 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.68836e-07 ( -2.52065e-08  2.53626e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from    0.900 sec. to    1.900 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: -0.411099     ( -1.67863   1.18398 )
Epeak [keV] : 97.7578      ( -24.2854 173.856 )
Norm@50keV  : 6.52069E-02    ( -0.0652133   0.235029 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          45.51 using 59 PHA bins.
# Reduced chi-squared =         0.8126 for     56 degrees of freedom 
# Null hypothesis probability =   8.406271e-01
 
Photon flux (15-150 keV)    in 1 sec: 1.69589 ( -0.28168  0.28042 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.57594e-07 ( -2.744e-08  2.7627e-08 ) ergs/cm2

Band function

Time interval is from    0.900 sec. to    1.900 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : 0.410905   ( -1.00136   0.800808 )
beta        : -10.00000    ( 10   4.99144e-08 )
Epeak [keV] : 97.7475      ( -18.7577 173.478 )
Norm@50keV   : 6.52068E-02    ( -0.0652068   0.235869 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          45.51 using 59 PHA bins.
# Reduced chi-squared =         0.8274 for     55 degrees of freedom 
# Null hypothesis probability =   8.155347e-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]    : 21.2301  (-3.11972  3.97754)
R^2/D10^2   : 7.44390E-02  (-0.0315507   0.0502605)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          46.45 using 59 PHA bins.
# Reduced chi-squared =         0.8150 for     57 degrees of freedom 
# Null hypothesis probability =   8.396078e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  6.309e-09   1.733e-09
25- 50  3.265e-08   7.940e-09
50-150  1.098e-07   2.971e-08
15-150  1.487e-07   3.005e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 200.000       (      )
Norm        : 7.44484       (-1.08657     1.0865)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          62.72 using 59 PHA bins.
# Reduced chi-squared =          1.100 for     57 degrees of freedom 
# Null hypothesis probability =   2.805731e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.853e-08   1.050e-08
25- 50  3.565e-08   2.001e-08
50-150  7.818e-08   4.418e-08
15-150  1.324e-07   7.450e-08

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 4.37382        (-4.23418      -4.23418)
R1^2/D10^2  : 3.52673        (-3.6258      -3.6258)
kT2 [keV]   : 22.7806        (-3.83819      -22.735)
R2^2/D10^2  : 5.73745E-02    (-0.0574953   0.0468436)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          44.67 using 59 PHA bins.
# Reduced chi-squared =         0.8122 for     55 degrees of freedom 
# Null hypothesis probability =   8.387706e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.029e-08   5.005e-09
25- 50  3.150e-08   1.140e-08
50-150  1.135e-07   4.303e-08
15-150  1.553e-07   4.992e-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: 1.27150     ( -0.0922941   0.0920012 )
Norm@50keV  : 5.58119E-03    ( -0.000291306   0.000291295 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          48.87 using 59 PHA bins.
# Reduced chi-squared =         0.8574 for     57 degrees of freedom 
# Null hypothesis probability =   7.696032e-01
 
Photon flux (15-150 keV)    in 54.5 sec: 0.662480 ( -0.0358476  0.0359064 ) ph/cm2/s
Energy fluence (15-150 keV)             : 3.02726e-06 ( -1.74456e-07  1.75197e-07 ) ergs/cm2

Cutoff power-law model

Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 0.621485     ( -0.432412   0.39286 )
Epeak [keV] : 114.805      ( -25.8577 88.6801 )
Norm@50keV  : 1.12264E-02    ( -0.00378539   0.00636496 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          40.44 using 59 PHA bins.
# Reduced chi-squared =         0.7222 for     56 degrees of freedom 
# Null hypothesis probability =   9.416882e-01
 
Photon flux (15-150 keV)    in 54.5 sec: 0.640295 ( -0.038151  0.038155 ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.90356e-06 ( -1.92227e-07  1.9196e-07 ) ergs/cm2

Band function

 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -0.621443   ( -0.291649   0.426877 )
beta        : -10.0000    ( 10   20 )
Epeak [keV] : 114.786      ( -18.0859 88.5561 )
Norm@50keV   : 1.12266E-02    ( -0.00378478   0.00636806 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          40.44 using 59 PHA bins.
# Reduced chi-squared =         0.7353 for     55 degrees of freedom 
# Null hypothesis probability =   9.290393e-01
 
Photon flux (15-150 keV)    in 54.5 sec: 0.645080 (    ) 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)  = 1.73e-06
S(50-100 keV) = 2.68e-06

T90 vs. Hardness ratio plot

T90                                   = 220.595999956131 sec.
Hardness ratio (energy fluence ratio) = 1.54913

Color vs. Color plot

Count Ratio  (25-50 keV) / (15-25 keV) = 1.34616
Count Ratio (50-100 keV) / (15-25 keV) = 1.23646

Mask shadow pattern

IMX = 8.515402123272447E-01, IMY = -6.238669160080063E-02

TIME vs. PHA plot around the trigger time

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.408000

TIME vs. DetID plot around the trigger time

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.408000

100 us light curve (15-350 keV)

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.408000

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:
-60.864000 -31.460000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
170.0549 -60.5389 2456.5  40.8  -71.3  -0.0006  -0.0    9.2	Cen X-3                       
186.9783 -62.7919   26.9  40.7  -58.5   0.0513   0.4    8.9	GX 301-2                      
264.7704 -44.4074    5.0  56.8    1.1   0.6370   2.3    2.8	4U 1735-44                    
275.7364 -59.4338    0.6  40.5    4.2   1.3449  17.7 ------	UNKNOWN                       
101.7010 -29.1276    2.9  55.1 -145.1   1.0798   3.9 ------	UNKNOWN

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

Time interval of the image:
-31.460000 23.036600
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
170.2582 -60.5920   16.9  40.8  -71.1   0.2754   0.7    2.5	Cen X-3                       
186.6956 -62.6996    6.5  40.7  -58.7   0.6117   1.8    4.4	GX 301-2                      
264.6946 -44.4251   10.2  56.8    1.0  -0.8679  -1.1    2.6	4U 1735-44                    
275.7300 -59.4379    1.1  40.5    4.2   2.1896  10.9 ------	UNKNOWN                       
209.9058 -58.2303    2.7  46.6  -43.2   1.5507   4.3 ------	UNKNOWN                       
139.2037 -53.8083    2.9  41.3  -98.5   2.1410   3.9 ------	UNKNOWN                       
123.0414 -46.3574    2.4  44.3 -116.8   2.8270   4.8 ------	UNKNOWN

Post-slew image of 15-350 keV band

Time interval of the image:
82.636600 135.636600
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
170.5460 -60.7321    0.0  46.7 -126.5   0.3331   0.9    9.4	Cen X-3                       
186.5940 -62.8420    9.9  39.7 -121.3  -0.2379  -1.2    4.6	GX 301-2                      
245.0246 -15.6568    2.3  49.2  -27.4   1.0542   5.0    2.8	Sco X-1                       
256.0839 -37.7542    2.7  25.0  -25.8   0.3621   4.2    7.1	4U 1700-377                   
256.4337 -36.3695    4.7  26.2  -23.9   0.2141   2.4    3.2	GX 349+2                      
263.1372 -24.6192    9.1  35.9   -6.7  -0.1480  -1.3   10.3	GX 1+4                        
264.9131 -44.5477    6.4  16.2  -15.4   0.1564   1.8    9.3	4U 1735-44                    
270.4423 -25.1987    6.2  34.4    4.6  -0.2241  -1.9   11.2	GX 5-1                        
270.4680 -25.8669    4.7  33.7    4.6   0.2851   2.4   11.6	GRS 1758-258                  
274.0776 -14.1613    5.4  45.3   10.8   0.3878   2.2    8.6	GX 17+2                       
275.8827 -30.2830    3.2  29.1   13.4   0.3816   3.5    5.5	H1820-303                     
285.2140 -25.0264   10.2  35.0   28.2   0.1475   1.1   11.6	HT1900.1-2455                 
262.8491 -33.7190    4.8  27.1  -10.9   0.2256   2.4    9.8	GX 354-0                      
271.3724 -21.2759    2.6  38.3    6.5   0.5635   4.4 ------	UNKNOWN                       
275.7560 -59.4912    1.3   0.1  168.8   0.7153   8.9 ------	UNKNOWN

Plot creation:
Sat May 30 18:33:33 EDT 2015