batgrbproduct analysis for trigger=339696

batgrbproduct Analysis for Trigger=339696

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 Jan 19 19:09:15 EST 2014
             Host Name: batevent1
   Current Working Dir: /local/data/batevent/batevent_reproc/trigger339696
======================================================================

  Trigger: 00339696      Segment: 000

  BAT Trigger Time: 253411106.112   [s; MET]
      Trigger Stop: 253411107.136   [s; MET]
               UTC: 2009-01-11T23:58:21.703320    [includes UTCF correction] 
       Where From?: TDRSS position message

  BAT 
    RA: 251.645117762436   Dec: 0.0910882533427581  [deg; J2000]

     Catalogged Source?: NO
     Point Source?:      YES
     GRB Indicated?:     YES    [ by BAT flight software ]
     Image S/N Ratio:    7.11
     Image Trigger?:     NO
     Rate S/N Ratio:     10.2469507659596  [ if not an image trigger ]
     Image S/N Ratio:    7.11

  Flight Position:   [ source = BAT ]
    RA: 251.645117762436   Dec: 0.0910882533427581  [deg; J2000]

  Ground Position:   [ source = BAT pre-slew burst ]
    RA: 251.652519911681   Dec: 0.0625914250328804  [deg; J2000]  
        { 16h 46m 36.6s , +00d 03' 45.3" }
         +/- 1.42779614575988 [arcmin] (estimated 90% radius based on SNR)
         +/- 0.562278298975681 [arcmin] (formal 1-sigma fit error)
    SNR: 18.2880187436005
 
  Angular difference between Flight and Ground position is 1.766550 arcmin
 
  Partial Coding Fraction: 0.8203125    [ including projection effects ]

  Duration
     T90: 25.2600000202656 +/- 2.65513238362588
        Measured from: -1.63199999928474
                   to: 23.6280000209808     [s; relative to TRIGTIME]
     T50: 13.7320000231266 +/- 1.45813578614825
        Measured from: 2.19600000977516
                   to: 15.9280000329018     [s; relative to TRIGTIME]



  Fluence
     Peak Flux  (peak 1 second)
        Measured from: 10.7080000042915     
                   to: 11.7080000042915     [s; relative to TRIGTIME]
     Total Fluence        
        Measured from: -2.87999999523163     
                   to: 26.0360000133514     [s; relative to TRIGTIME]
     
             Band 1     Band 2     Band 3     Band 4
              15-25      25-50     50-100    100-350     keV
 Total     0.543534   0.518783   0.206302   0.064775
           0.034258   0.032814   0.028541   0.026517 [error]
 Peak      0.036706   0.039291   0.021636   0.012242
           0.006621   0.006304   0.005403   0.004908 [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 1.87e-07 2.15e-07 1.76e-07 2.42e-07 6.66e-07 8.21e-07   erg/cm2
              Error 2.01e-08 1.67e-08 2.68e-08 7.19e-08 6.00e-08 1.03e-07   erg/cm2
Peak flux Power-law 3.49e-01 2.99e-01 1.75e-01 1.53e-01 8.90e-01 9.76e-01   ph/cm2/s
              Error 9.56e-02 5.24e-02 4.57e-02 7.98e-02 1.56e-01 1.71e-01   ph/cm2/s
 
Fluence   Cutoff-PL 1.81e-07 2.26e-07 1.66e-07 9.69e-08 6.30e-07 6.70e-07   erg/cm2
              Error 2.22e-08 2.21e-08 3.24e-08 1.44e-07 7.34e-08 1.56e-07   erg/cm2
Peak flux Cutoff-PL 3.42e-01 3.05e-01 1.76e-01 1.21e-01 8.83e-01 9.43e-01   ph/cm2/s
              Error 1.04e-01 6.19e-02 4.77e-02 1.21e-01 1.60e-01 1.94e-01   ph/cm2/s
 
Fluence        Band 1.79e-07 2.25e-07 1.65e-07 1.24e-07 6.30e-07 6.95e-07   erg/cm2
              Error -------- -------- -------- -------- -------- --------   erg/cm2
Peak flux      Band 3.36e-01 3.09e-01 1.76e-01 1.02e-01 8.78e-01 9.23e-01   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    2.284    0.162    -      -           2.42e-03 2.62e-04   47.430 57
CPL   1.793    0.588      16.4   15.7      4.76e-03 5.27e-03   45.740 56
 
 
=== 1-s peak spectral analysis ===
 
Model Ph_index Ph_90err Epeak  Epeak_90err Norm     Nomr_90err chi2   dof
PL    1.774    0.325    -      -           6.52e-03 1.30e-03   48.610 57
CPL   1.609    1.074     105.9   -0.0      8.05e-03 2.31e-02   48.540 56
 
Model      : spectral model: simple power-law (PL) and cutoff power-law (CPL)
Ph_index   : photon index: E^-{Ph_index} (minus sign is not included in the index)
Ph_90err   : 90% error of the photon index
Epeak      : Epeak in keV
Epeak_90err: 90% error of Epeak
Norm       : normalization at 50 keV in PL model and at 1 keV in CPL model
Nomr_90err : 90% error of the normalization
chi2       : Chi-Squared
dof        : degree of freedom

 
=== T90/T50 calculation in the 50-300 keV band (BATSE band) using 64 ms lc ===
 
T90 in the 50-300 keV band: 0.000000 sec.
T50 in the 50-300 keV band: 0.000000 sec.

 
=== Table of the duration information ==
 
        Value   tstart    tstop
T100   28.916   -2.880   26.036
T90    25.260   -1.632   23.628
T50    13.732    2.196   15.928
Peak    1.000   10.708   11.708

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
  251.6525     0.0626   0.0105    25.1077  -139.9929         1.0743764     18.288 TRIG_00339696                 
 
Foreground time interval of the image:
 -2.880  19.789 (delta_t =  22.669 [sec])
Background time interval of the image:
-239.112  -2.880 (delta_t = 236.232 [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

8 ms binning

From T100_start-3 s to T100_start+3 s

2 ms binning

From T100_start-1 s to T100_start+1 s

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   -2.880 sec. to   26.036 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 2.28406     ( -0.158001   0.165797 )
Norm@50keV  : 2.41804E-03    ( -0.000264247   0.000260292 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          47.43 using 59 PHA bins.
# Reduced chi-squared =         0.8322 for     57 degrees of freedom 
# Null hypothesis probability =   8.128211e-01
 
Photon flux (15-150 keV)    in 28.92 sec: 0.418857 ( -0.031869  0.0318956 ) ph/cm2/s
Energy fluence (15-150 keV)             : 6.66334e-07 ( -5.94268e-08  6.06111e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from   -2.880 sec. to   26.036 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.79312     ( -0.760212   0.415767 )
Epeak [keV] : 16.3566      ( -15.1433 16.2496 )
Norm@50keV  : 4.75747E-03    ( -0.00165146   0.00888659 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          45.74 using 59 PHA bins.
# Reduced chi-squared =         0.8168 for     56 degrees of freedom 
# Null hypothesis probability =   8.343861e-01
 
Photon flux (15-150 keV)    in 28.92 sec: 0.408904 ( -0.034191  0.034239 ) ph/cm2/s
Energy fluence (15-150 keV)             : 6.2993e-07 ( -7.09639e-08  7.58369e-08 ) ergs/cm2

Band function

Time interval is from   -2.880 sec. to   26.036 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -1.78420   ( 1.78288   1.78288 )
beta        : -2.96588    ( 3.04625   0.861346 )
Epeak [keV] : 16.7901      ( -16.7952 15.7843 )
Norm@50keV   : 4.80655E-03    ( -0.00164997   0.129868 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          45.73 using 59 PHA bins.
# Reduced chi-squared =         0.8315 for     55 degrees of freedom 
# Null hypothesis probability =   8.089717e-01
 
Photon flux (15-150 keV)    in 28.92 sec:  (    ) ph/cm2/s
Energy fluence (15-150 keV)             : 6.29687e-07 ( 0  0 ) ergs/cm2

Single BB

 
Spectral model blackbody:
------------------------------------------------------------
Parameters  : value    Lower 90%  Upper 90%
kT [keV]    : 8.37745  (-0.745609  0.824253)
R^2/D10^2   : 0.364568  (-0.115461   0.169773)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          76.52 using 59 PHA bins.
# Reduced chi-squared =          1.342 for     57 degrees of freedom 
# Null hypothesis probability =   4.325281e-02
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.382e-07   1.802e-08
25- 50  2.616e-07   2.423e-08
50-150  7.975e-08   2.007e-08
15-150  4.795e-07   4.396e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 43.0449       (-8.14703      11.0175)
Norm        : 2.54065       (-0.37461     0.456357)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          46.82 using 59 PHA bins.
# Reduced chi-squared =         0.8215 for     57 degrees of freedom 
# Null hypothesis probability =   8.297346e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.727e-07   1.774e-08
25- 50  2.343e-07   1.993e-08
50-150  1.960e-07   4.642e-08
15-150  6.030e-07   5.466e-08

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 4.95206        (-1.18157      1.24728)
R1^2/D10^2  : 2.21196        (-1.25422      4.58063)
kT2 [keV]   : 15.4772        (-3.55585      6.4625)
R2^2/D10^2  : 2.12300E-02    (-0.0163961   0.0471458)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          46.19 using 59 PHA bins.
# Reduced chi-squared =         0.8399 for     55 degrees of freedom 
# Null hypothesis probability =   7.951902e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.803e-07   6.623e-08
25- 50  2.206e-07   7.084e-08
50-150  2.105e-07   1.183e-07
15-150  6.114e-07   2.319e-07

Peak spectrum fit

Power-law model

Time interval is from   10.708 sec. to   11.708 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.77403     ( -0.316713   0.333234 )
Norm@50keV  : 6.52003E-03    ( -0.00131613   0.00127437 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          48.61 using 59 PHA bins.
# Reduced chi-squared =         0.8528 for     57 degrees of freedom 
# Null hypothesis probability =   7.778578e-01
 
Photon flux (15-150 keV)    in 1 sec: 0.889562 ( -0.155791  0.156022 ) ph/cm2/s
Energy fluence (15-150 keV)             : 6.0088e-08 ( -1.21662e-08  1.25133e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from   10.708 sec. to   11.708 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.60850     ( -1.36542   0.781827 )
Epeak [keV] : 105.912      ( -106.406 -106.422 )
Norm@50keV  : 8.04626E-03    ( -0.00804135   0.0381407 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          48.54 using 59 PHA bins.
# Reduced chi-squared =         0.8668 for     56 degrees of freedom 
# Null hypothesis probability =   7.501359e-01
 
Photon flux (15-150 keV)    in 1 sec: 0.883149 ( -0.159669  0.160191 ) ph/cm2/s
Energy fluence (15-150 keV)             : 5.90984e-08 ( -1.38608e-08  1.32535e-08 ) ergs/cm2

Band function

Time interval is from   10.708 sec. to   11.708 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -1.60905   ( 1.65819   1.27959 )
beta        : -10.00000    ( 10   20 )
Epeak [keV] : 106.405      ( -74.1099 -106.405 )
Norm@50keV   : 8.03942E-03    ( -0.00281781   0.0113627 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          48.54 using 59 PHA bins.
# Reduced chi-squared =         0.8826 for     55 degrees of freedom 
# Null hypothesis probability =   7.181643e-01
 
Photon flux (15-150 keV)    in 1 sec: 0.877518 (    ) 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]    : 11.0163  (-2.26076  3.2452)
R^2/D10^2   : 0.286043  (-0.17628   0.395686)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          57.42 using 59 PHA bins.
# Reduced chi-squared =          1.007 for     57 degrees of freedom 
# Null hypothesis probability =   4.595999e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  7.255e-09   2.665e-09
25- 50  2.055e-08   5.770e-09
50-150  1.411e-08   6.470e-09
15-150  4.192e-08   1.274e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 99.9932       (-45.5737      -101.455)
Norm        : 3.92417       (-0.876773     1.14818)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          48.76 using 59 PHA bins.
# Reduced chi-squared =         0.8554 for     57 degrees of freedom 
# Null hypothesis probability =   7.731462e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.026e-08   2.753e-09
25- 50  1.773e-08   4.910e-09
50-150  2.874e-08   1.717e-08
15-150  5.673e-08   2.854e-08

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 5.62956        (-3.41667      3.34423)
R1^2/D10^2  : 2.22284        (-0.999143      12.5603)
kT2 [keV]   : 20.8953        (-11.8772      94.1822)
R2^2/D10^2  : 1.98208E-02    (-0.0084612   0.0762624)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          49.16 using 59 PHA bins.
# Reduced chi-squared =         0.8939 for     55 degrees of freedom 
# Null hypothesis probability =   6.960832e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.013e-08   6.005e-09
25- 50  1.574e-08   8.675e-09
50-150  2.782e-08   1.793e-08
15-150  5.370e-08   2.957e-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: 2.30269     ( -0.160917   0.169224 )
Norm@50keV  : 2.68036E-03    ( -0.000300776   0.000296315 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          54.97 using 59 PHA bins.
# Reduced chi-squared =         0.9644 for     57 degrees of freedom 
# Null hypothesis probability =   5.516496e-01
 
Photon flux (15-150 keV)    in 22.67 sec: 0.469119 ( -0.0362744  0.0363014 ) ph/cm2/s
Energy fluence (15-150 keV)             : 5.80955e-07 ( -5.27105e-08  5.37846e-08 ) ergs/cm2

Cutoff power-law model

Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.78998     ( -0.735253   0.427769 )
Epeak [keV] : 15.9742      (   )
Norm@50keV  : 5.42347E-03    (     )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          53.05 using 59 PHA bins.
# Reduced chi-squared =         0.9472 for     56 degrees of freedom 
# Null hypothesis probability =   5.874075e-01
 
Photon flux (15-150 keV)    in 22.67 sec: 0.457713 ( -0.038593  0.038678 ) ph/cm2/s
Energy fluence (15-150 keV)             : 5.49303e-07 ( -6.10412e-08  6.52261e-08 ) ergs/cm2

Band function

 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -1.78903   ( 1.90785   1.90785 )
beta        : -10.0000    ( 10   2.66454e-14 )
Epeak [keV] : 16.0102      ( -7.84267 9.68294 )
Norm@50keV   : 5.42960E-03    ( -0.00187309   0.00948772 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          53.05 using 59 PHA bins.
# Reduced chi-squared =         0.9645 for     55 degrees of freedom 
# Null hypothesis probability =   5.496441e-01
 
Photon flux (15-150 keV)    in 22.67 sec: 0.460508 (    ) ph/cm2/s
Energy fluence (15-150 keV)             : 5.65929e-07 ( 0  0 ) ergs/cm2

S(25-50 keV) vs. S(50-100 keV) plot

S(25-50 keV)  = 2.15e-07
S(50-100 keV) = 1.76e-07

T90 vs. Hardness ratio plot

T90                                   = 25.2600000202656 sec.
Hardness ratio (energy fluence ratio) = 0.818605

Color vs. Color plot

Count Ratio  (25-50 keV) / (15-25 keV) = 0.954463
Count Ratio (50-100 keV) / (15-25 keV) = 0.379557

Mask shadow pattern

IMX = -3.589301383745268E-01, IMY = 3.012539309384202E-01

TIME vs. PHA plot around the trigger time

TIME vs. DetID plot around the trigger time

100 us light curve (15-350 keV)

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:
-239.112000 -2.880000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
244.9631 -15.6340    0.3  17.6  -96.5   7.4133  34.5    1.0	Sco X-1                       
254.5183  35.3052   11.6  50.9  178.0  -0.5469  -1.0    3.7	Her X-1                       
255.9490 -37.8262    2.0  38.1  -66.5   2.5023   5.7    2.1	4U 1700-377                   
256.6737 -36.3421    0.0  37.6  -68.9   0.4377   1.0   12.5	GX 349+2                      
263.2071 -24.6842   37.8  36.8  -90.4  -0.1592  -0.3   11.4	GX 1+4                        
268.4872  -1.5177    3.1  40.8 -128.2   1.3849   3.7    8.1	SW J1753.5-0127               
262.8608 -33.6915    0.0  40.2  -77.0   0.5112   0.8   10.7	GX 354-0                      
213.9117 -47.2102    2.1  40.0  -14.7   1.4240   5.5 ------	UNKNOWN

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

Time interval of the image:
-2.880000 19.788600
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
245.0063 -15.6116   10.7  17.7  -96.6   0.0617   1.1    2.3	Sco X-1                       
254.5327  35.4229    5.0  51.0  177.9   0.3261   2.3    6.1	Her X-1                       
255.9014 -37.7019    4.5  38.0  -66.6   0.3037   2.6    9.4	4U 1700-377                   
256.6526 -36.3833   26.5  37.6  -68.9  -0.0485  -0.4   10.8	GX 349+2                      
262.9140 -24.6943    5.5  36.6  -90.2   0.2600   2.1    6.0	GX 1+4                        
268.3991  -1.5049   13.8  40.7 -128.2  -0.0851  -0.8    3.6	SW J1753.5-0127               
263.2004 -33.7833    8.4  40.5  -77.1   0.2780   1.4   11.0	GX 354-0                      
251.6525   0.0626    0.6  25.1 -140.0   1.0742  18.3 ------	UNKNOWN

Post-slew image of 15-350 keV band

Time interval of the image:
65.588600 962.963000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
244.9839 -15.6414    0.2  17.0   -8.2  29.0078  54.0    0.3	Sco X-1                       
254.4851  35.3093   11.5  35.3  153.5   0.9558   1.0    2.4	Her X-1                       
255.9954 -37.8463    0.8  38.1  -36.2  13.0618  14.0    0.4	4U 1700-377                   
256.5819 -36.3793    3.9  36.8  -37.2   2.4594   3.0    7.5	GX 349+2                      
263.0055 -24.7400    1.6  27.2  -53.7   4.7436   7.1    0.4	GX 1+4                        
264.7511 -44.3829   90.9  46.0  -43.6   0.1883   0.1    4.0	4U 1735-44                    
268.3463  -1.4647    1.4  16.8 -115.2   4.3931   8.1    1.5	SW J1753.5-0127               
270.2412 -25.1340    3.1  31.0  -64.7   3.0264   3.7    4.0	GX 5-1                        
270.3727 -25.8296    6.0  31.6  -64.1   1.6540   1.9    6.4	GRS 1758-258                  
273.9968 -14.0010    1.6  26.2  -87.2   5.7080   7.3    2.2	GX 17+2                       
275.8341 -30.3443    5.1  38.2  -65.5   3.0014   2.3    4.9	H1820-303                     
285.1095 -25.0184    8.2  41.0  -80.3   3.2809   1.4    7.1	HT1900.1-2455                 
288.7977  10.9650    1.2  38.5 -138.2   8.5641   9.4    1.2	GRS 1915+105                  
299.6128  35.1877    1.6  56.8 -164.0  16.5298   7.2    1.4	Cyg X-1                       
262.8164 -33.8736    4.3  35.5  -46.7   2.0063   2.7    8.9	GX 354-0                      
214.7964  13.8037    3.0  39.0   81.6  10.5867   3.8 ------	UNKNOWN                       
241.0534  45.1675    3.7  46.0  139.1   8.6581   3.1 ------	UNKNOWN                       
235.7804  -8.8932    5.0  18.2   29.4   1.3320   2.3 ------	UNKNOWN                       
237.0105 -28.3248    3.7  31.7   -5.5   2.0637   3.1 ------	UNKNOWN                       
258.2240 -16.0223    3.0  17.4  -52.3   1.9827   3.9 ------	UNKNOWN

Plot creation:
Sun May 31 05:03:07 EDT 2015