batgrbproduct analysis for trigger=503525

batgrbproduct Analysis for Trigger=503525

Analysis Summary

Notes:

1) No attempt has been made to eliminate the non-significant decimal places.
2) This batgrbproduct analysis is done of the amount of data for this trigger downloaded to date.
3) This batgrbproduct analysis is using the flight position for the mask-weighting calculation.
4) This page will be updated for up to 10 downlinks after the trigger.

======================================================================
                  BAT GRB EVENT DATA PROCESSING REPORT
    Process Script Ver: batgrbproduct v2.46
    Process Start Time (local time): Mon Oct  3 16:40:40 EDT 2011
             Host Name: gcn5
   Current Working Dir: /local/data/raid16/prebascript_archive/trigger503525/batgroup_hand_proc
======================================================================

  Trigger: 00503525      Segment: 000

  BAT Trigger Time: 338159778.916   [s; MET]
      Trigger Stop: 338159778.96   [s; MET]
               UTC: 2011-09-19T21:16:11.533640    [includes UTCF correction] 
       Where From?: Command line

  BAT 
    RA: 251.75181767584   Dec: -45.8429090422137  [deg; J2000]

     Catalogged Source?: NO
     Point Source?:      YES
     GRB Indicated?:     YES    [ by BAT flight software ]
     Image S/N Ratio:    7.03
     Image Trigger?:     NO
     Rate S/N Ratio:     13.9642400437689  [ if not an image trigger ]
     Image S/N Ratio:    7.03

  Flight Position:   [ source = EXTERNAL ]
    RA: 251.7189   Dec: -45.8334  [deg; J2000]


  Partial Coding Fraction: 1.015625    [ including projection effects ]

 
  Angular difference between Flight and Ground position is 0.000000 arcmin
 
  Partial Coding Fraction: 1.015625    [ including projection effects ]

  Duration
     T90: 29.1360000371933 +/- 6.5942762958167
        Measured from: -29.1319999098778
                   to: 0.00400012731552124     [s; relative to TRIGTIME]
     T50: 11.5199999809265 +/- 12.8135178662698
        Measured from: -18.3159998655319
                   to: -6.79599988460541     [s; relative to TRIGTIME]



  Fluence
     Peak Flux  (peak 1 second)
        Measured from: -5.56000000238419     
                   to: -4.56000000238419     [s; relative to TRIGTIME]
     Total Fluence        
        Measured from: -34.2200000286102     
                   to: 0.0519999861717224     [s; relative to TRIGTIME]
     
             Band 1     Band 2     Band 3     Band 4
              15-25      25-50     50-100    100-350     keV
 Total     0.207284   0.106714   0.011935   0.025590
           0.035913   0.031858   0.027511   0.025562 [error]
 Peak      0.022858   0.004590   0.005325   0.002083
           0.006253   0.005463   0.004549   0.004464 [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 1.54e-09 3.53e-10 4.11e-11 5.33e-12 1.94e-09 1.94e-09   erg/cm2
              Error 5.46e-10 1.47e-10 3.00e-11 7.21e-12 6.65e-10 6.66e-10   erg/cm2
Peak flux Power-law 1.83e-01 7.41e-02 1.77e-02 5.12e-03 2.77e-01 2.79e-01   ph/cm2/s
              Error 9.05e-02 4.86e-02 2.55e-02 1.78e-02 1.28e-01 1.30e-01   ph/cm2/s
 
Fluence   Cutoff-PL 3.35e-09 1.58e-09 2.04e-12 6.75e-21 4.94e-09 4.93e-09   erg/cm2
              Error 7.72e-10 5.00e-10 2.38e-12 1.10e-19 1.08e-09 1.08e-09   erg/cm2
Peak flux Cutoff-PL 1.82e-01 7.40e-02 1.76e-02 5.39e-03 9.36e-06 2.78e-01   ph/cm2/s
              Error 9.04e-02 5.29e-02 3.23e-03 1.28e-01 1.00e-01 0.00e+00   ph/cm2/s
 
Fluence        Band 0.00e+00 0.00e+00 0.00e+00 0.00e+00 0.00e+00 0.00e+00   erg/cm2
              Error 0.00e+00 0.00e+00 0.00e+00 0.00e+00 0.00e+00 0.00e+00   erg/cm2
Peak flux      Band 0.00e+00 0.00e+00 0.00e+00 0.00e+00 0.00e+00 0.00e+00   ph/cm2/s
              Error 0.00e+00 0.00e+00 0.00e+00 0.00e+00 0.00e+00 0.00e+00   ph/cm2/s

 
=== Time-averaged spectral analysis ===
 
Model Ph_index Ph_90err Epeak  Epeak_90err Norm     Nomr_90err chi2   dof
PL    5.104    0.639    -      -           8.16e-04 4.98e-04   86.710 57
CPL   1.000    0.000      50.0    0.0      1.84e-03 0.00e+00  107.280 56
 
The chi2 of BB fit is 67.23 which shows a significant improvement in the fit over a PL.
Check the BB fit.
 
=== 1-s peak spectral analysis ===
 
Model Ph_index Ph_90err Epeak  Epeak_90err Norm     Nomr_90err chi2   dof
PL    3.068    1.429    -      -           9.60e-04 1.07e-03   65.100 57
CPL   1.000    0.000      50.0    0.0      5.07e-03 0.00e+00   69.190 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   34.272  -34.220    0.052
T90    29.136  -29.132    0.004
T50    11.520  -18.316   -6.796
Peak    1.000   -5.560   -4.560

Click here for the BAT GCN circular template

Image

Pre-slew 15.0-50.0 keV image (Event data)

#   RAcent    DECcent   POSerr    Theta     Phi              Peak Cts       SNR   Name
  251.7189   -45.8334   0.0281    10.3313  -167.6020         0.0166700      6.825 TRIG_00503525                 
 
Foreground time interval of the image:
  0.000   0.044 (delta_t =   0.044 [sec])
Background time interval of the image:
-10.004  -2.004 (delta_t =   8.000 [sec])

Lightcurves

Notes:

1) All plots contain as much data as has been downloaded to date.
2) The mask-weighted light curves are using the flight position.
3) Multiple plots of different time binning/intervals are shown to cover all scenarios of short/long GRBs, rate/image triggers, and real/false positives.
4) 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.
5) 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.
6) 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 -0.004000 to 0.060000

8 ms binning

From T100_start-3 s to T100_start+3 s

Blue+Cyan dotted lines: Time interval of the scaled map
From -0.004000 to 0.060000

2 ms binning

From T100_start-1 s to T100_start+1 s

Blue+Cyan dotted lines: Time interval of the scaled map
From -0.004000 to 0.060000

SN=5 or 10 sec. binning (whichever binning is satisfied first)

SN=5 or 10 sec. binning (T < 200 sec)

Flight mask-tagged light curves

Caution: Mask-weight map is always using the same on-axis map

Quad-rate summed light curves (from T0-300 to T0+1000)

The mask-weighted light curves based on cleaned DPHs

Spectra

Notes:

1) The fitting includes the systematic errors.
2) For long bursts, a spectral fit of 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.
4) For short bursts (T90<1sec), the specrtum is also fit with Blackbody, OTTB, and Double Blackbody.

Time averaged spectrum fit using the pre-slew DRM

Power-law model

Time interval is from    0.000 sec. to    0.044 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 5.10385     ( -0.569206   0.708552 )
Norm@50keV  : 8.15726E-04    ( -0.000460017   0.000536343 )
------------------------------------------------------------
# Chi-Squared =          86.71 using 59 PHA bins.
# Reduced chi-squared =          1.521 for     57 degrees of freedom 
# Null hypothesis probability =   6.792281e-03
 
Photon flux (15-150 keV)    in 0.044 sec: 1.38970 ( -0.482154  0.482029 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.94212e-09 ( -6.651e-10  6.651e-10 ) ergs/cm2

Cutoff power-law model

Time interval is from    0.000 sec. to    0.044 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.00000     (     )
Epeak [keV] : 50.0000      (   )
Norm@50keV  : 1.84439E-03    (     )
------------------------------------------------------------
# Chi-Squared =         107.28 using 59 PHA bins.
# Reduced chi-squared =         1.9157 for     56 degrees of freedom 
# Null hypothesis probability =   4.501839e-05
 
Photon flux (15-150 keV)    in 0.044 sec: 3.19047 ( -0.69751  0.69762 ) ph/cm2/s
Energy fluence (15-150 keV)             : 4.93601e-09 ( -1.08158e-09  1.07963e-09 ) ergs/cm2

Band function

Time interval is from    0.000 sec. to    0.044 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -9.98125   ( 230.875   240.711 )
beta        : -5.09153    ( -0.774821   0.502485 )
Epeak [keV] : 79.4819      ( -79.4819 -79.4819 )
Norm@50keV   : 0.112059    ( -0.0633738   0.0720586 )
------------------------------------------------------------
# Chi-Squared =          86.71 using 59 PHA bins.
# Reduced chi-squared =          1.577 for     55 degrees of freedom 
# Null hypothesis probability =   4.094432e-03
 
Photon flux (15-150 keV)    in 0.044 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]    : 3.82554  (-0.367766  0.326751)
R^2/D10^2   : 85.9796  (-38.5192   68.4795)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
# Chi-Squared =          67.23 using 59 PHA bins.
# Reduced chi-squared =          1.180 for     57 degrees of freedom 
# Null hypothesis probability =   1.665139e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  2.761e-09   8.787e-10
25- 50  8.760e-10   3.329e-10
50-150  8.084e-12   6.562e-12
15-150  3.645e-09   1.209e-09

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 7.19870       (-1.18366      1.21909)
Norm        : 150.302       (-67.4699     108.528)
------------------------------------------------------------
# Chi-Squared =          76.42 using 59 PHA bins.
# Reduced chi-squared =          1.341 for     57 degrees of freedom 
# Null hypothesis probability =   4.393459e-02
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  2.239e-09   8.956e-10
25- 50  5.835e-10   2.484e-10
50-150  1.431e-11   1.182e-11
15-150  2.837e-09   1.001e-09

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 3.80882        (-3.83392      196.15)
R1^2/D10^2  : 32.1379        (-32.1797      -32.1797)
kT2 [keV]   : 3.83319        (-3.82237      196.154)
R2^2/D10^2  : 54.0093    (-54.0547   -54.0547)
------------------------------------------------------------
# Chi-Squared =          67.23 using 59 PHA bins.
# Reduced chi-squared =          1.222 for     55 degrees of freedom 
# Null hypothesis probability =   1.246066e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  2.761e-09   3.969e-01
25- 50  8.752e-10   4.143e+00
50-150  8.063e-12   8.897e+01
15-150  3.644e-09   9.555e+01

Peak spectrum fit

Power-law model

Time interval is from   -5.560 sec. to   -4.560 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 3.06801     ( -1.11993   1.7371 )
Norm@50keV  : 9.59707E-04    ( -0.000959707   0.00117867 )
------------------------------------------------------------
# Chi-Squared =          65.10 using 59 PHA bins.
# Reduced chi-squared =          1.142 for     57 degrees of freedom 
# Null hypothesis probability =   2.156610e-01
 
Photon flux (15-150 keV)    in 1 sec: 0.277424 ( -0.127132  0.128373 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.19066e-08 ( -6.46889e-09  8.38055e-09 ) ergs/cm2

Cutoff power-law model

Time interval is from   -5.560 sec. to   -4.560 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.00000     (     )
Epeak [keV] : 50.0000      (   )
Norm@50keV  : 5.07320E-03    (     )
------------------------------------------------------------
# Chi-Squared =          69.19 using 59 PHA bins.
# Reduced chi-squared =          1.236 for     56 degrees of freedom 
# Null hypothesis probability =   1.108914e-01
 
Photon flux (15-150 keV)    in 1 sec: 0.277684 ( -0.127463  0.127659 ) ph/cm2/s
Energy fluence (15-150 keV)             : 9.61819e-09 ( -5.13658e-09  1.0532e-08 ) ergs/cm2

Band function

Time interval is from   -5.560 sec. to   -4.560 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : 3.48708   ( 1.47728   1.47728 )
beta        : -3.54222    ( 3.22242   1.23886 )
Epeak [keV] : 16.6444      ( -8.1098 450.755 )
Norm@50keV   : 332.323    ( -509.313   3.36156e+06 )
------------------------------------------------------------
# Chi-Squared =          64.50 using 59 PHA bins.
# Reduced chi-squared =          1.173 for     55 degrees of freedom 
# Null hypothesis probability =   1.784971e-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]    : 4.58017  (-1.85441  2.90126)
R^2/D10^2   : 3.55546  (-3.55565   52.3058)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
# Chi-Squared =          65.12 using 59 PHA bins.
# Reduced chi-squared =          1.143 for     57 degrees of freedom 
# Null hypothesis probability =   2.149975e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  6.007e-09   3.943e-09
25- 50  3.140e-09   2.116e-09
50-150  8.196e-11   8.535e-11
15-150  9.228e-09   5.920e-09

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 14.1670       (-8.55337      40.3849)
Norm        : 5.30827       (-5.30823     27.4298)
------------------------------------------------------------
# Chi-Squared =          65.07 using 59 PHA bins.
# Reduced chi-squared =          1.142 for     57 degrees of freedom 
# Null hypothesis probability =   2.163342e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  5.756e-09   3.744e-09
25- 50  3.706e-09   2.550e-09
50-150  5.803e-10   6.175e-10
15-150  1.004e-08   7.115e-09

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 4.29994        (-4.29994      2.79743)
R1^2/D10^2  : 4.65378        (-4.65387      -4.65387)
kT2 [keV]   : 46.7712        (-46.7707      -46.7707)
R2^2/D10^2  : 2.87280E-04    (-0.000287291   -0.000287291)
------------------------------------------------------------
# Chi-Squared =          64.31 using 59 PHA bins.
# Reduced chi-squared =          1.169 for     55 degrees of freedom 
# Null hypothesis probability =   1.828920e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  6.016e-09   3.563e-09
25- 50  3.139e-09   2.006e-09
50-150  5.917e-09   3.103e-09
15-150  1.507e-08   8.465e-09

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: 3.15823     ( -0.85232   1.19235 )
Norm@50keV  : 2.30263E-04    ( -0.000230264   0.000228822 )
------------------------------------------------------------
# Chi-Squared =          39.78 using 59 PHA bins.
# Reduced chi-squared =         0.6979 for     57 degrees of freedom 
# Null hypothesis probability =   9.597078e-01
 
Photon flux (15-150 keV)    in 21.47 sec: 7.12132E-02 ( -0.0266821  0.0270741 ) ph/cm2/s
Energy fluence (15-150 keV)             : 6.41519e-08 ( -2.84881e-08  3.48149e-08 ) ergs/cm2

Cutoff power-law model

Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: -5.67078     (     )
Epeak [keV] : 21.4784      ( -20.8506 5.37005 )
Norm@50keV  : 1244.99    (     )
------------------------------------------------------------
# Chi-Squared =          36.32 using 59 PHA bins.
# Reduced chi-squared =         0.6486 for     56 degrees of freedom 
# Null hypothesis probability =   9.808407e-01
 
Photon flux (15-150 keV)    in 21.47 sec: 7.07223E-02 ( -0.0242258  0.0252615 ) ph/cm2/s
Energy fluence (15-150 keV)             : 5.42534e-08 ( -1.89756e-08  2.12497e-08 ) ergs/cm2

Band function

 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : 4.98944   ( -192.833   -182.833 )
beta        : -9.37112    ( 9.99936   19.638 )
Epeak [keV] : 21.4028      ( -4.4517 4.67771 )
Norm@50keV   : 359.205    ( -358.426   3465.83 )
------------------------------------------------------------
# Chi-Squared =          36.40 using 59 PHA bins.
# Reduced chi-squared =         0.6618 for     55 degrees of freedom 
# Null hypothesis probability =   9.749744e-01
 
Photon flux (15-150 keV)    in 21.47 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)  = 3.52543e-10
S(50-100 keV) = 4.11447e-11

T90 vs. Hardness ratio plot

T90                                   = 29.1360000371933 sec.
Hardness ratio (energy fluence ratio) = 0.116708

Color vs. Color plot

Count Ratio  (25-50 keV) / (15-25 keV) = 0.51482
Count Ratio (50-100 keV) / (15-25 keV) = 0.057578

Mask shadow pattern

IMX = -1.780446603934030E-01, IMY = 3.913918760327067E-02

TIME vs. PHA plot around the trigger time

Blue+Cyan dotted lines: Time interval of the scaled map
From -0.004000 to 0.060000

TIME vs. DetID plot around the trigger time

Blue+Cyan dotted lines: Time interval of the scaled map
From -0.004000 to 0.060000

100 us light curve (15-350 keV)

Blue+Cyan dotted lines: Time interval of the scaled map
From -0.004000 to 0.060000

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:

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

Time interval of the image:
0.000000 0.044000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
170.5096 -60.4707    6.9  57.4 -153.8  -0.0208  -1.7   10.8	Cen X-3                       
186.4994 -62.8151   30.9  49.5 -155.0   0.0022   0.4    5.1	GX 301-2                      
245.0582 -15.5086    3.9  23.5  -40.1  -0.0074  -2.9    9.1	Sco X-1                       
255.8982 -37.6791    5.6   1.7 -151.0  -0.0047  -2.1   10.8	4U 1700-377                   
256.2844 -36.2493    0.0   0.8  -91.1   0.0001   0.0   12.7	GX 349+2                      
262.9604 -24.6824    8.0  12.7   14.9   0.0036   1.4    4.6	GX 1+4                        
264.9385 -44.5629    4.5  10.1  137.4   0.0060   2.5   10.8	4U 1735-44                    
268.3954  -1.3063    3.7  36.6    9.5   0.0106   3.1    8.9	SW J1753.5-0127               
270.1193 -25.1668    4.4  15.7   38.7  -0.0072  -2.9   10.4	GX 5-1                        
270.1430 -25.6352    6.7  15.4   39.9   0.0055   2.2   10.8	GRS 1758-258                  
274.0885 -14.1559    7.8  26.8   29.0  -0.0045  -1.5    8.6	GX 17+2                       
275.7765 -30.5116    8.1  16.5   65.1   0.0040   1.4   11.6	H1820-303                     
285.0516 -25.0370    5.7  26.3   62.9   0.0074   2.0    7.0	HT1900.1-2455                 
262.9943 -33.8619  802.6   5.3   54.2   0.0000   0.0    1.7	GX 354-0                      
265.3295   3.2790    1.9  40.4    3.1   0.0234   6.0 ------	UNKNOWN                       
251.7218 -45.8353    1.7  10.3 -167.6   0.0167   6.8 ------	UNKNOWN                       
235.3619 -27.4278    2.7  20.5  -79.9   0.0121   4.3 ------	UNKNOWN

Post-slew image of 15-350 keV band

Time interval of the image:
39.584600 95.891500
97.084000 296.814000
301.084000 302.130000
360.084000 422.123600
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
170.4988 -60.4696    5.4  47.4 -150.3  -1.4881  -2.1   10.7	Cen X-3                       
186.4596 -62.9644    0.0  39.5 -151.3  -0.7581  -1.5   12.8	GX 301-2                      
244.9889 -15.6406    0.2  30.7  -24.5  17.6859  53.4    0.5	Sco X-1                       
256.0123 -37.8377    1.5   8.6   11.4   2.0977   7.9    1.3	4U 1700-377                   
256.4923 -36.4386    2.8  10.0   10.7   1.1083   4.1    2.9	GX 349+2                      
263.1574 -24.8144    5.3  22.9   15.7   0.6349   2.2    9.1	GX 1+4                        
264.7711 -44.5215    5.8   9.3   74.8   0.5358   2.0    4.5	4U 1735-44                    
268.2625  -1.3884    6.9  46.7   11.2  -1.0906  -1.7    7.4	SW J1753.5-0127               
270.3403 -25.0999    1.8  25.5   30.3   2.1337   6.5    3.3	GX 5-1                        
270.1497 -25.8157   11.4  24.8   30.9   0.3193   1.0    9.3	GRS 1758-258                  
274.1391 -14.0628    4.1  36.9   26.2   1.2554   2.8    7.9	GX 17+2                       
275.9269 -30.3049    3.6  24.4   47.2   1.2098   3.2    3.7	H1820-303                     
285.2286 -25.0462    0.0  33.9   52.0   0.9583   1.8   12.9	HT1900.1-2455                 
263.0045 -33.7852    3.6  14.8   27.7   0.9740   3.2    3.1	GX 354-0                      
267.8737 -22.7059    2.5  26.6   23.2   1.4564   4.6 ------	UNKNOWN                       
261.8549 -21.0506    2.9  26.1   10.1   1.1965   4.0 ------	UNKNOWN                       
228.4877 -76.2436    3.0  31.9  178.5   1.2387   3.9 ------	UNKNOWN                       
195.3426 -61.6033    2.2  35.5 -148.7   2.3432   5.3 ------	UNKNOWN                       
168.8145 -50.8862    3.6  52.4 -139.5   5.1712   3.2 ------	UNKNOWN                       
226.9113  -0.0828    3.4  50.7  -44.6   5.8783   3.4 ------	UNKNOWN                       
217.5488 -13.0106    4.4  43.7  -64.2   4.0764   2.7 ------	UNKNOWN                       
	UNKNOWN

Plot creation:
Mon Oct  3 17:32:47 EDT 2011