batgrbproduct analysis for trigger=382399

batgrbproduct Analysis for Trigger=382399

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 20:18:56 EST 2014
             Host Name: batevent1
   Current Working Dir: /local/data/batevent/batevent_reproc/trigger382399
======================================================================

  Trigger: 00382399      Segment: 000

  BAT Trigger Time: 284875974.464   [s; MET]
      Trigger Stop: 284875974.976   [s; MET]
               UTC: 2010-01-11T04:12:49.036100    [includes UTCF correction] 
       Where From?: TDRSS position message

  BAT 
    RA: 247.038118029266   Dec: 15.5569602813662  [deg; J2000]

     Catalogged Source?: NO
     Point Source?:      YES
     GRB Indicated?:     YES    [ by BAT flight software ]
     Image S/N Ratio:    12.08
     Image Trigger?:     NO
     Rate S/N Ratio:     18.1107702762748  [ if not an image trigger ]
     Image S/N Ratio:    12.08

  Flight Position:   [ source = BAT ]
    RA: 247.038118029266   Dec: 15.5569602813662  [deg; J2000]

  Ground Position:   [ source = BAT pre-slew burst ]
    RA: 247.02890122076   Dec: 15.5426809549622  [deg; J2000]  
        { 16h 28m 06.9s , +15d 32' 33.7" }
         +/- 1.25716852205968 [arcmin] (estimated 90% radius based on SNR)
         +/- 0.426029092349492 [arcmin] (formal 1-sigma fit error)
    SNR: 21.9344964190425
 
  Angular difference between Flight and Ground position is 1.008899 arcmin
 
  Partial Coding Fraction: 1.015625    [ including projection effects ]

  Duration
     T90: 14 +/- 2.23606797749979
        Measured from: -7.46399998664856
                   to: 6.53600001335144     [s; relative to TRIGTIME]
     T50: 4 +/- 2.23606797749979
        Measured from: -1.46399998664856
                   to: 2.53600001335144     [s; relative to TRIGTIME]



  Fluence
     Peak Flux  (peak 1 second)
        Measured from: 0.53600001335144     
                   to: 1.53600001335144     [s; relative to TRIGTIME]
     Total Fluence        
        Measured from: -9.46399998664856     
                   to: 8.53600001335144     [s; relative to TRIGTIME]
     
             Band 1     Band 2     Band 3     Band 4
              15-25      25-50     50-100    100-350     keV
 Total     0.387662   0.474853   0.268634   0.038031
           0.025821   0.025744   0.024121   0.024279 [error]
 Peak      0.065453   0.090880   0.053896   0.009022
           0.006732   0.007002   0.006513   0.006003 [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 1.18e-07 1.87e-07 2.23e-07 5.17e-07 6.77e-07 1.04e-06   erg/cm2
              Error 1.27e-08 1.23e-08 2.38e-08 1.17e-07 5.40e-08 1.37e-07   erg/cm2
Peak flux Power-law 6.29e-01 6.02e-01 4.01e-01 4.17e-01 1.80e+00 2.05e+00   ph/cm2/s
              Error 9.36e-02 5.63e-02 5.35e-02 1.12e-01 1.65e-01 1.97e-01   ph/cm2/s
 
Fluence   Cutoff-PL 1.17e-07 1.88e-07 2.23e-07 4.72e-07 6.73e-07 9.97e-07   erg/cm2
              Error 1.38e-08 1.43e-08 2.39e-08 2.63e-07 6.26e-08 2.36e-07   erg/cm2
Peak flux Cutoff-PL 6.12e-01 6.17e-01 4.03e-01 3.02e-01 1.78e+00 1.93e+00   ph/cm2/s
              Error 1.05e-01 7.06e-02 5.58e-02 2.07e-01 1.74e-01 2.76e-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    1.745    0.131    -      -           4.07e-03 3.08e-04   55.390 57
CPL   1.699    0.542     286.0    0.0      4.32e-03 0.00e+00   55.380 56
 
 
=== 1-s peak spectral analysis ===
 
Model Ph_index Ph_90err Epeak  Epeak_90err Norm     Nomr_90err chi2   dof
PL    1.584    0.168    -      -           1.41e-02 1.43e-03   49.210 57
CPL   1.366    0.524     129.8    0.0      1.86e-02 1.76e-02   48.870 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: 8.064000 sec.
T50 in the 50-300 keV band: 4.160000 sec.

 
=== Table of the duration information ==
 
        Value   tstart    tstop
T100   18.000   -9.464    8.536
T90    14.000   -7.464    6.536
T50     4.000   -1.464    2.536
Peak    1.000    0.536    1.536

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
  247.0289    15.5427   0.0088    16.0596  -159.3538         1.1467217     21.934 TRIG_00382399                 
 
Foreground time interval of the image:
 -9.464   8.536 (delta_t =  18.000 [sec])
Background time interval of the image:
-239.464  -9.464 (delta_t = 230.000 [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   -9.464 sec. to    8.536 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.74492     ( -0.129898   0.13239 )
Norm@50keV  : 4.07430E-03    ( -0.000310386   0.000306276 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          55.39 using 59 PHA bins.
# Reduced chi-squared =         0.9718 for     57 degrees of freedom 
# Null hypothesis probability =   5.355467e-01
 
Photon flux (15-150 keV)    in 18 sec: 0.549885 ( -0.0364177  0.0364576 ) ph/cm2/s
Energy fluence (15-150 keV)             : 6.76913e-07 ( -5.35793e-08  5.44473e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from   -9.464 sec. to    8.536 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.69868     ( -0.524713   0.560128 )
Epeak [keV] : 285.997      (   )
Norm@50keV  : 4.32020E-03    (     )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          55.38 using 59 PHA bins.
# Reduced chi-squared =         0.9889 for     56 degrees of freedom 
# Null hypothesis probability =   4.983580e-01
 
Photon flux (15-150 keV)    in 18 sec: 0.548280 ( -0.039595  0.037705 ) ph/cm2/s
Energy fluence (15-150 keV)             : 6.73202e-07 ( -6.79032e-08  5.72742e-08 ) ergs/cm2

Band function

Time interval is from   -9.464 sec. to    8.536 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -1.04233   ( 1.15051   1.15051 )
beta        : -1.84077    ( 1.83909   0.201412 )
Epeak [keV] : 44.5147      ( -44.6391 -44.6391 )
Norm@50keV   : 1.15945E-02    ( -0.0120973   625.169 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          54.51 using 59 PHA bins.
# Reduced chi-squared =         0.9910 for     55 degrees of freedom 
# Null hypothesis probability =   4.933966e-01
 
Photon flux (15-150 keV)    in 18 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]    : 11.1935  (-0.951664  1.07424)
R^2/D10^2   : 0.163706  (-0.0471448   0.0646385)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =         106.18 using 59 PHA bins.
# Reduced chi-squared =         1.8627 for     57 degrees of freedom 
# Null hypothesis probability =   8.401324e-05
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  7.739e-08   9.657e-09
25- 50  2.238e-07   1.620e-08
50-150  1.605e-07   3.037e-08
15-150  4.616e-07   3.816e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 121.480       (-35.1021      48.6346)
Norm        : 2.28275       (-0.188423     0.267386)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          57.27 using 59 PHA bins.
# Reduced chi-squared =          1.005 for     57 degrees of freedom 
# Null hypothesis probability =   4.648719e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.070e-07   1.036e-08
25- 50  1.918e-07   1.958e-08
50-150  3.443e-07   1.301e-07
15-150  6.430e-07   1.493e-07

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 7.32074        (-1.24716      1.25062)
R1^2/D10^2  : 0.613636        (-0.251062      0.303257)
kT2 [keV]   : 31.9068        (-9.58447      24.6064)
R2^2/D10^2  : 2.87452E-03    (-0.00227216   0.00691244)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          54.80 using 59 PHA bins.
# Reduced chi-squared =         0.9963 for     55 degrees of freedom 
# Null hypothesis probability =   4.824117e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.073e-07   2.248e-08
25- 50  1.983e-07   3.786e-08
50-150  3.797e-07   1.792e-07
15-150  6.854e-07   2.102e-07

Peak spectrum fit

Power-law model

Time interval is from    0.536 sec. to    1.536 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.58441     ( -0.166413   0.16951 )
Norm@50keV  : 1.40874E-02    ( -0.00143593   0.00141652 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          49.21 using 59 PHA bins.
# Reduced chi-squared =         0.8633 for     57 degrees of freedom 
# Null hypothesis probability =   7.588303e-01
 
Photon flux (15-150 keV)    in 1 sec: 1.80166 ( -0.165461  0.165497 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.32003e-07 ( -1.46379e-08  1.49108e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from    0.536 sec. to    1.536 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.36552     ( -0.725861   0.321993 )
Epeak [keV] : 129.765      ( -129.795 -129.795 )
Norm@50keV  : 1.86127E-02    ( -0.00725527   0.027866 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          48.87 using 59 PHA bins.
# Reduced chi-squared =         0.8726 for     56 degrees of freedom 
# Null hypothesis probability =   7.393018e-01
 
Photon flux (15-150 keV)    in 1 sec: 1.78278 ( -0.17461  0.17255 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.285e-07 ( -1.7927e-08  1.6959e-08 ) ergs/cm2

Band function

Time interval is from    0.536 sec. to    1.536 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : 4.92226   ( -5.91966   -4.92226 )
beta        : -1.72424    ( -0.260654   0.201999 )
Epeak [keV] : 24.9078      ( -9.90084 9.90084 )
Norm@50keV   : 1479.38    ( -134.722   8944.01 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          45.92 using 59 PHA bins.
# Reduced chi-squared =         0.8349 for     55 degrees of freedom 
# Null hypothesis probability =   8.034614e-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]    : 12.0850  (-1.41981  1.67028)
R^2/D10^2   : 0.424284  (-0.157935   0.242823)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          73.72 using 59 PHA bins.
# Reduced chi-squared =          1.293 for     57 degrees of freedom 
# Null hypothesis probability =   6.740147e-02
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.311e-08   2.398e-09
25- 50  4.161e-08   4.615e-09
50-150  3.671e-08   7.995e-09
15-150  9.144e-08   1.088e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 169.154       (-64.9223      -169.086)
Norm        : 7.37910       (-0.713671     0.826258)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          48.85 using 59 PHA bins.
# Reduced chi-squared =         0.8569 for     57 degrees of freedom 
# Null hypothesis probability =   7.704283e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.874e-08   9.413e-09
25- 50  3.531e-08   1.852e-08
50-150  7.309e-08   4.064e-08
15-150  1.271e-07   6.691e-08

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 7.71053        (-1.86167      1.98154)
R1^2/D10^2  : 1.61349        (-0.824584      2.22621)
kT2 [keV]   : 33.4138        (-12.6623      82.4612)
R2^2/D10^2  : 8.98073E-03    (-0.00815425   0.0372773)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          46.77 using 59 PHA bins.
# Reduced chi-squared =         0.8503 for     55 degrees of freedom 
# Null hypothesis probability =   7.773719e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.832e-08   5.668e-09
25- 50  3.706e-08   1.134e-08
50-150  7.708e-08   3.974e-08
15-150  1.325e-07   5.386e-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: 1.74492     ( -0.129898   0.13239 )
Norm@50keV  : 4.07430E-03    ( -0.000310386   0.000306276 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          55.39 using 59 PHA bins.
# Reduced chi-squared =         0.9718 for     57 degrees of freedom 
# Null hypothesis probability =   5.355467e-01
 
Photon flux (15-150 keV)    in 18 sec: 0.549885 ( -0.0364177  0.0364576 ) ph/cm2/s
Energy fluence (15-150 keV)             : 6.76913e-07 ( -5.35793e-08  5.44473e-08 ) ergs/cm2

Cutoff power-law model

Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.69868     ( -0.524713   0.560128 )
Epeak [keV] : 285.997      (   )
Norm@50keV  : 4.32020E-03    (     )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          55.38 using 59 PHA bins.
# Reduced chi-squared =         0.9889 for     56 degrees of freedom 
# Null hypothesis probability =   4.983580e-01
 
Photon flux (15-150 keV)    in 18 sec: 0.548280 ( -0.039595  0.037705 ) ph/cm2/s
Energy fluence (15-150 keV)             : 6.73202e-07 ( -6.79032e-08  5.72742e-08 ) ergs/cm2

Band function

 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -1.04233   ( 1.15051   1.15051 )
beta        : -1.84077    ( 1.83909   0.201412 )
Epeak [keV] : 44.5147      ( -44.6391 -44.6391 )
Norm@50keV   : 1.15945E-02    ( -0.0120973   625.277 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          54.51 using 59 PHA bins.
# Reduced chi-squared =         0.9910 for     55 degrees of freedom 
# Null hypothesis probability =   4.933966e-01
 
Photon flux (15-150 keV)    in 18 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)  = 1.87e-07
S(50-100 keV) = 2.23e-07

T90 vs. Hardness ratio plot

T90                                   = 14 sec.
Hardness ratio (energy fluence ratio) = 1.19251

Color vs. Color plot

Count Ratio  (25-50 keV) / (15-25 keV) = 1.22492
Count Ratio (50-100 keV) / (15-25 keV) = 0.692959

Mask shadow pattern

IMX = -2.693824269417192E-01, IMY = 1.015023599969543E-01

TIME vs. PHA plot around the trigger time

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.512000

TIME vs. DetID plot around the trigger time

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.512000

100 us light curve (15-350 keV)

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.512000

Spacecraft aspect plot

Bright source in the pre-burst/pre-slew/post-slew images

Pre-burst image of 15-350 keV band

Time interval of the image:
-239.464000 -9.464000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
244.9820 -15.6339    0.4  26.1  -65.4   8.9686  30.5    0.4	Sco X-1                       
254.4534  35.3263    8.3  34.2  174.4   0.4351   1.4    1.0	Her X-1                       
268.3707  -1.4173    6.4  36.5 -115.3   0.8524   1.8    2.1	SW J1753.5-0127               
213.2346  39.3218    3.3  36.4  116.1   2.0327   3.5 ------	UNKNOWN                       
261.6320  54.9962    2.9  52.8  162.3   4.0836   4.1 ------	UNKNOWN                       
256.8271 -19.6603    3.0  36.0  -78.6   1.9418   3.9 ------	UNKNOWN                       
262.5379 -15.3096    2.4  37.2  -90.2   3.0587   4.9 ------	UNKNOWN                       
270.9866  -9.8699    2.3  41.8 -104.0   4.9854   5.1 ------	UNKNOWN

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

Time interval of the image:
-9.464000 8.536000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
245.1677 -15.5986    5.8  26.1  -65.8   0.1395   2.0   11.2	Sco X-1                       
254.2688  35.2849    6.8  34.0  174.2   0.1213   1.7    9.9	Her X-1                       
268.2504  -1.3675   11.6  36.4 -115.3  -0.1023  -1.0    8.7	SW J1753.5-0127               
198.8071  12.4915    2.2  33.9   63.3   0.5260   5.2 ------	UNKNOWN                       
247.0289  15.5427    0.5  16.1 -159.4   1.1467  21.9 ------	UNKNOWN                       
274.9814  21.5880    2.1  43.0 -151.8   0.5028   5.6 ------	UNKNOWN

Post-slew image of 15-350 keV band

Time interval of the image:
47.236600 962.588500
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
244.9766 -15.6376    0.2  31.3  -34.8  32.0482  46.5    0.2	Sco X-1                       
254.7089  35.3538   35.2  21.0  159.1  -0.2192  -0.3   12.3	Her X-1                       
263.0536 -24.8940  202.3  43.4  -60.0  -0.1324  -0.1    9.2	GX 1+4                        
268.3929  -1.5251    3.4  27.2  -91.6   2.8021   3.4    4.6	SW J1753.5-0127               
274.1525 -13.9979    3.8  39.9  -82.2   7.5205   3.0    8.8	GX 17+2                       
288.7892  10.9751    2.0  40.8 -127.5   7.7399   5.9    1.8	GRS 1915+105                  
299.5909  35.1968    0.6  50.7 -161.7  31.6408  20.1    0.3	Cyg X-1                       
307.9733  40.8522    8.1  58.0 -167.4   4.6786   1.6    8.7	Cyg X-3                       
213.9222  44.1664    7.2  40.0  103.8   4.5587   1.6 ------	UNKNOWN                       
205.4097   6.0197    4.9  41.9   42.9   4.7318   2.4 ------	UNKNOWN                       
297.9000  34.7916    3.0  49.3 -161.5   5.2671   3.9 ------	UNKNOWN                       
237.0392 -29.8797    3.7  46.4  -26.7   3.7905   3.1 ------	UNKNOWN                       
296.0178  13.1376    2.7  47.4 -132.3   9.7768   4.3 ------	UNKNOWN                       
268.0451 -22.3333    1.3  43.1  -67.7  28.2532   8.8 ------	UNKNOWN                       
282.0096  -6.8690    2.9  41.3  -98.3   9.4750   4.0 ------	UNKNOWN

Plot creation:
Sun May 31 02:23:50 EDT 2015