batgrbproduct analysis for trigger=513505

batgrbproduct Analysis for Trigger=513505

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 Feb  6 01:38:43 EST 2012
             Host Name: gcn5
   Current Working Dir: /local/data/raid16/prebascript_archive/trigger513505/GCN5_download_cron
======================================================================

  Trigger: 00513505      Segment: 000

  BAT Trigger Time: 350135252.476   [s; MET]
      Trigger Stop: 350135252.54   [s; MET]
               UTC: 2012-02-05T11:47:24.617420    [includes UTCF correction] 
       Where From?: (*SHORT BURST*) TDRSS scaled map message

  BAT 
    RA: 40.1003583767653   Dec: 61.220476106393  [deg; J2000]

     Catalogged Source?: NO
     Point Source?:      YES
     GRB Indicated?:     YES    [ by BAT flight software ]
     Image S/N Ratio:    7.53
     Image Trigger?:     NO
     Rate S/N Ratio:     15.0332963783729  [ if not an image trigger ]
     Image S/N Ratio:    7.53

  Flight Position:   [ source = BAT ]
    RA: 40.1003583767653   Dec: 61.220476106393  [deg; J2000]

  Ground Position:   [ source = BAT pre-slew burst ]
    RA: 40.0594015847184   Dec: 61.2349598468358  [deg; J2000]  
        { 02h 40m 14.3s , +61d 14' 05.9" }
         +/- 2.7879991206673 [arcmin] (estimated 90% radius based on SNR)
         +/- 1.52913956983674 [arcmin] (formal 1-sigma fit error)
    SNR: 7.03049733442349
 
  Angular difference between Flight and Ground position is 1.467745 arcmin
 
  Partial Coding Fraction: 0.765625    [ including projection effects ]

  Duration
     T90: 0.0399999618530273 +/- 0.0113137314268704
        Measured from: 0.0200001001358032
                   to: 0.0600000619888306     [s; relative to TRIGTIME]
     T50: 0.0199999213218689 +/- 0.00894429003608426
        Measured from: 0.0280001163482666
                   to: 0.0480000376701355     [s; relative to TRIGTIME]



  Fluence
     Peak Flux  (peak 1 second)
        Measured from: -0.456000030040741     
                   to: 0.543999969959259     [s; relative to TRIGTIME]
     Total Fluence        
        Measured from: 0.0199999809265137     
                   to: 0.0640000104904175     [s; relative to TRIGTIME]
     
             Band 1     Band 2     Band 3     Band 4
              15-25      25-50     50-100    100-350     keV
 Total     0.013271   0.008279   0.000983   0.000684
           0.002055   0.001830   0.000857   0.000955 [error]
 Peak      0.023772   0.008933   0.000962  -0.004435
           0.006183   0.005892   0.005040   0.004517 [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 4.04e-09 1.78e-09 4.69e-10 1.53e-10 6.38e-09 6.44e-09   erg/cm2
              Error 9.49e-10 4.69e-10 2.01e-10 1.04e-10 1.46e-09 1.48e-09   erg/cm2
Peak flux Power-law 2.22e-01 7.69e-02 1.50e-02 3.46e-03 3.17e-01 3.18e-01   ph/cm2/s
              Error 9.71e-02 5.67e-02 2.50e-02 1.41e-02 1.44e-01 1.47e-01   ph/cm2/s
 
Fluence   Cutoff-PL 4.19e-09 3.51e-09 6.84e-10 1.75e-11 8.40e-09 0.00e+00   erg/cm2
              Error 1.04e-09 1.11e-09 5.50e-10 3.53e-11 1.82e-09 0.00e+00   erg/cm2
Peak flux Cutoff-PL 2.22e-01 7.67e-02 1.49e-02 3.41e-03 3.16e-01 3.14e-01   ph/cm2/s
              Error 1.26e-01 6.99e-02 2.50e-02 1.39e-02 1.46e-01 1.51e-01   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    3.924    0.361    -      -           6.95e-03 2.48e-03   49.440 57
CPL   1.000    0.000      50.0    0.0      7.26e-03 0.00e+00   96.040 56
 
The chi2 of BB fit is 41.76 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    3.354    1.547    -      -           8.80e-04 1.11e-03   55.210 57
CPL   1.000    0.000      50.0    0.0      5.91e-03 0.00e+00   60.910 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    0.044    0.020    0.064
T90     0.040    0.020    0.060
T50     0.020    0.028    0.048
Peak    1.000   -0.456    0.544

Click here for the BAT GCN circular template

Image

Pre-slew 15-350 keV image (Event data; bkg subtracted)

#   RAcent  DECcent POSerr  Theta    Phi     Peak Cts     SNR  Name
   40.0594 +61.2350 0.0274   28.1 -135.7       0.0221     7.0  TRIG_00513505       
------------------------------------------
 
Foreground time interval of the image:
  0.020   0.064 (delta_t =   0.044 [sec])
Background time interval of the image:
-239.476   0.020 (delta_t = 239.496 [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 0.000000 to 0.064000

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 0.064000

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 0.064000

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    0.020 sec. to    0.064 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 3.92384     ( -0.305257   0.416848 )
Norm@50keV  : 6.94963E-03    ( -0.00254454   0.00242303 )
------------------------------------------------------------
# Chi-Squared =          49.44 using 59 PHA bins.
# Reduced chi-squared =         0.8674 for     57 degrees of freedom 
# Null hypothesis probability =   7.513139e-01
 
Photon flux (15-150 keV)    in 0.044 sec: 4.01097 ( -0.911574  0.911334 ) ph/cm2/s
Energy fluence (15-150 keV)             : 6.37701e-09 ( -1.4572e-09  1.45595e-09 ) ergs/cm2

Cutoff power-law model

Time interval is from    0.020 sec. to    0.064 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.00000     (     )
Epeak [keV] : 50.0000      (   )
Norm@50keV  : 7.25545E-03    (     )
------------------------------------------------------------
# Chi-Squared =          96.04 using 59 PHA bins.
# Reduced chi-squared =          1.715 for     56 degrees of freedom 
# Null hypothesis probability =   6.973182e-04
 
Photon flux (15-150 keV)    in 0.044 sec: 4.79790 ( -1.00418  1.00418 ) ph/cm2/s
Energy fluence (15-150 keV)             : 8.40426e-09 ( -1.81504e-09  1.81786e-09 ) ergs/cm2

Band function

Time interval is from    0.020 sec. to    0.064 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -0.775827   ( -1.06044   0.979235 )
beta        : -9.99955    ( 7046.47   7056.46 )
Epeak [keV] : 16.0060      ( -14.6273 9.41142 )
Norm@50keV   : 0.663137    ( -0.66332   162.843 )
------------------------------------------------------------
# Chi-Squared =          39.55 using 59 PHA bins.
# Reduced chi-squared =         0.7191 for     55 degrees of freedom 
# Null hypothesis probability =   9.422338e-01
 
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]    : 5.68602  (-1.11605  1.32724)
R^2/D10^2   : 23.5604  (-14.6074   40.7225)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
# Chi-Squared =          41.76 using 59 PHA bins.
# Reduced chi-squared =         0.7327 for     57 degrees of freedom 
# Null hypothesis probability =   9.350967e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  4.105e-09   1.795e-09
25- 50  3.634e-09   1.511e-09
50-150  2.655e-10   1.858e-10
15-150  8.004e-09   3.435e-09

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 16.7157       (-4.05948      3.47239)
Norm        : 74.4093       (-23.544     38.2167)
------------------------------------------------------------
# Chi-Squared =          39.89 using 59 PHA bins.
# Reduced chi-squared =         0.6998 for     57 degrees of freedom 
# Null hypothesis probability =   9.585954e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  4.288e-09   1.045e-09
25- 50  3.235e-09   8.012e-10
50-150  7.041e-10   3.560e-10
15-150  8.227e-09   1.910e-09

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 4.22300        (-4.223      2.18706)
R1^2/D10^2  : 63.2040        (-63.204      -63.204)
kT2 [keV]   : 8.83373        (-8.83373      90.0142)
R2^2/D10^2  : 1.49784    (-1.49784   30.667)
------------------------------------------------------------
# Chi-Squared =          39.34 using 59 PHA bins.
# Reduced chi-squared =         0.7152 for     55 degrees of freedom 
# Null hypothesis probability =   9.451589e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  4.261e-09   2.451e-09
25- 50  3.421e-09   1.862e-09
50-150  7.600e-10   5.773e-10
15-150  8.441e-09   4.380e-09

Peak spectrum fit

Power-law model

Time interval is from   -0.456 sec. to    0.544 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 3.35416     ( -1.14508   1.94875 )
Norm@50keV  : 8.79872E-04    ( -0.000879872   0.0013425 )
------------------------------------------------------------
# Chi-Squared =          55.21 using 59 PHA bins.
# Reduced chi-squared =         0.9686 for     57 degrees of freedom 
# Null hypothesis probability =   5.425693e-01
 
Photon flux (15-150 keV)    in 1 sec: 0.316641 ( -0.143325  0.14559 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.26987e-08 ( -6.91732e-09  9.21892e-09 ) ergs/cm2

Cutoff power-law model

Time interval is from   -0.456 sec. to    0.544 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.00000     (     )
Epeak [keV] : 50.0000      (   )
Norm@50keV  : 5.90950E-03    (     )
------------------------------------------------------------
# Chi-Squared =          60.91 using 59 PHA bins.
# Reduced chi-squared =          1.088 for     56 degrees of freedom 
# Null hypothesis probability =   3.037727e-01
 
Photon flux (15-150 keV)    in 1 sec: 0.315667 ( -0.145226  0.145879 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.25194e-16 ( 0  0 ) ergs/cm2

Band function

Time interval is from   -0.456 sec. to    0.544 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : 4.32569   ( -0.290159   -0.290159 )
beta        : -3.92809    ( 3.99198   1.72363 )
Epeak [keV] : 15.7750      ( -13.0376 34.065 )
Norm@50keV   : 3547.31    ( -3631.08   5.22799e+06 )
------------------------------------------------------------
# Chi-Squared =          54.72 using 59 PHA bins.
# Reduced chi-squared =         0.9950 for     55 degrees of freedom 
# Null hypothesis probability =   4.851765e-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]    : 3.86765  (-1.40729  2.2091)
R^2/D10^2   : 9.65646  (-9.65647   114.391)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
# Chi-Squared =          55.11 using 59 PHA bins.
# Reduced chi-squared =         0.9668 for     57 degrees of freedom 
# Null hypothesis probability =   5.464650e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  7.444e-09   4.377e-09
25- 50  2.439e-09   1.672e-09
50-150  2.411e-11   2.906e-11
15-150  9.907e-09   6.160e-09

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 10.7666       (-6.1692      25.9891)
Norm        : 9.22735       (-9.22731     60.0947)
------------------------------------------------------------
# Chi-Squared =          55.25 using 59 PHA bins.
# Reduced chi-squared =         0.9692 for     57 degrees of freedom 
# Null hypothesis probability =   5.411247e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  7.031e-09   4.345e-09
25- 50  3.333e-09   2.414e-09
50-150  2.779e-10   3.788e-10
15-150  1.064e-08   6.890e-09

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 3.56999        (-3.552      2.11662)
R1^2/D10^2  : 13.6275        (-13.8885      -13.8885)
kT2 [keV]   : 19.0736        (-18.4207      -18.4207)
R2^2/D10^2  : 4.24251E-03    (-0.00448724   -0.00448724)
------------------------------------------------------------
# Chi-Squared =          54.30 using 59 PHA bins.
# Reduced chi-squared =         0.9872 for     55 degrees of freedom 
# Null hypothesis probability =   5.014100e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  7.250e-09   4.533e-09
25- 50  3.252e-09   1.942e-09
50-150  3.920e-09   3.463e-09
15-150  1.442e-08   8.680e-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: 3.92384     ( -0.305257   0.416848 )
Norm@50keV  : 6.94963E-03    ( -0.00254454   0.00242303 )
------------------------------------------------------------
# Chi-Squared =          49.44 using 59 PHA bins.
# Reduced chi-squared =         0.8674 for     57 degrees of freedom 
# Null hypothesis probability =   7.513139e-01
 
Photon flux (15-150 keV)    in 0.044 sec: 4.01097 ( -0.911574  0.911334 ) ph/cm2/s
Energy fluence (15-150 keV)             : 6.37701e-09 ( -1.4572e-09  1.45595e-09 ) ergs/cm2

Cutoff power-law model

Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.00000     (     )
Epeak [keV] : 50.0000      (   )
Norm@50keV  : 7.25545E-03    (     )
------------------------------------------------------------
# Chi-Squared =          96.04 using 59 PHA bins.
# Reduced chi-squared =          1.715 for     56 degrees of freedom 
# Null hypothesis probability =   6.973182e-04
 
Photon flux (15-150 keV)    in 0.044 sec: 4.79790 ( -1.00418  1.00418 ) ph/cm2/s
Energy fluence (15-150 keV)             : 8.40426e-09 ( -1.81504e-09  1.81786e-09 ) ergs/cm2

Band function

 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -0.775827   ( -0.85009   5.73071 )
beta        : -9.99955    ( 7046.47   7056.46 )
Epeak [keV] : 16.0060      ( -14.6273 9.41142 )
Norm@50keV   : 0.663137    ( -0.66332   162.843 )
------------------------------------------------------------
# Chi-Squared =          39.55 using 59 PHA bins.
# Reduced chi-squared =         0.7191 for     55 degrees of freedom 
# Null hypothesis probability =   9.422338e-01
 
Photon flux (15-150 keV)    in 0.044 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)  = 1.77951e-09
S(50-100 keV) = 4.6941e-10

T90 vs. Hardness ratio plot

T90                                   = 0.0399999618530273 sec.
Hardness ratio (energy fluence ratio) = 0.263786

Color vs. Color plot

Count Ratio  (25-50 keV) / (15-25 keV) = 0.623841
Count Ratio (50-100 keV) / (15-25 keV) = 0.0740713

Mask shadow pattern

IMX = 0, IMY = 0

TIME vs. PHA plot around the trigger time

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.064000

TIME vs. DetID plot around the trigger time

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.064000

100 us light curve (15-350 keV)

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.064000

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:
-239.476000 0.020000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
 83.6589  22.0097    1.8  51.6  150.6   6.3633   6.3    1.5	Crab                          
 79.5176  24.9409    2.7  49.5  156.2   2.9284   4.3 ------	UNKNOWN                       
 84.5014  51.5942    4.0  22.9  162.8   0.5097   2.9 ------	UNKNOWN                       
203.5578  58.1086    2.4  37.4   -1.1   1.1357   4.8 ------	UNKNOWN                       
223.3970  56.2185    2.2  44.2  -14.2   1.4794   5.2 ------	UNKNOWN                       
229.2068  76.3988    2.1  27.8  -35.3   0.9866   5.5 ------	UNKNOWN                       
 28.7428  60.4766    2.6  32.1 -128.0   0.8959   4.4 ------	UNKNOWN

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

Time interval of the image:
0.020000 0.064000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
 83.6735  21.9055    5.8  51.7  150.6   0.0268   2.0    6.9	Crab                          
203.8420  41.7900    2.6  51.9    9.5   0.0385   4.5 ------	UNKNOWN                       
 56.3913  44.2530    2.7  37.2 -168.3   0.0143   4.3 ------	UNKNOWN                       
 40.0595  61.2350    1.6  28.1 -135.7   0.0221   7.0 ------	UNKNOWN                       
 37.1777  36.0354    2.4  50.8 -153.9   0.0323   4.8 ------	UNKNOWN                       
351.7033  67.6818    2.3  35.1  -96.8   0.0269   5.0 ------	UNKNOWN

Post-slew image of 15-350 keV band

Time interval of the image:
61.224600 747.124600
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
 73.5808  18.3572    2.5  48.9  151.3   7.8878   4.7 ------	UNKNOWN                       
 48.8674  47.3174    2.7  14.8  171.5   1.4542   4.3 ------	UNKNOWN                       
 31.4230  36.8316    3.2  25.0 -148.1   1.3495   3.7 ------	UNKNOWN

Plot creation:
Mon Feb  6 13:56:06 EST 2012