batgrbproduct analysis for trigger=574935

batgrbproduct Analysis for Trigger=574935

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): Sat Jan 11 22:44:42 EST 2014
             Host Name: batevent1
   Current Working Dir: /local/data/batevent/batevent_reproc/trigger574935
======================================================================

  Trigger: 00574935      Segment: 000

  BAT Trigger Time: 403793280   [s; MET]
      Trigger Stop: 403793344   [s; MET]
               UTC: 2013-10-18T12:47:48.834540    [includes UTCF correction] 
       Where From?: TDRSS position message

  BAT 
    RA: 98.4618116856018   Dec: -19.8820304441863  [deg; J2000]

     Catalogged Source?: NO
     Point Source?:      YES
     GRB Indicated?:     YES    [ by BAT flight software ]
     Image S/N Ratio:    16.77
     Image Trigger?:     YES
     Rate S/N Ratio:     0  [ if not an image trigger ]
     Image S/N Ratio:    16.77

  Flight Position:   [ source = BAT ]
    RA: 98.4618116856018   Dec: -19.8820304441863  [deg; J2000]

  Ground Position:   [ source = BAT pre-slew burst ]
    RA: 98.4685450877152   Dec: -19.8994638741002  [deg; J2000]  
        { 06h 33m 52.5s , -19d 53' 58.1" }
         +/- 1.27550544202634 [arcmin] (estimated 90% radius based on SNR)
         +/- 0.552306285333286 [arcmin] (formal 1-sigma fit error)
    SNR: 21.4854098701745
 
  Angular difference between Flight and Ground position is 1.112858 arcmin
 
  Partial Coding Fraction: 1.015625    [ including projection effects ]

  Duration
     T90: 73.2159999608994 +/- 18.9734095686505
        Measured from: 24.8080000281334
                   to: 98.0239999890327     [s; relative to TRIGTIME]
     T50: 31.2960000038147 +/- 5.21393821144733
        Measured from: 39.3360000252724
                   to: 70.6320000290871     [s; relative to TRIGTIME]



  Fluence
     Peak Flux  (peak 1 second)
        Measured from: 59.4120000004768     
                   to: 60.4120000004768     [s; relative to TRIGTIME]
     Total Fluence        
        Measured from: 21.0960000157356     
                   to: 117.736000001431     [s; relative to TRIGTIME]
     
             Band 1     Band 2     Band 3     Band 4
              15-25      25-50     50-100    100-350     keV
 Total     0.989807   0.908741   0.358349   0.040430
           0.049879   0.050775   0.043518   0.037216 [error]
 Peak      0.023897   0.025402   0.011467   0.008017
           0.005045   0.005297   0.004479   0.003797 [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 2.98e-07 3.49e-07 2.95e-07 4.21e-07 1.09e-06 1.36e-06   erg/cm2
              Error 2.79e-08 2.41e-08 3.89e-08 1.08e-07 8.79e-08 1.54e-07   erg/cm2
Peak flux Power-law 1.96e-01 1.62e-01 9.05e-02 7.49e-02 4.81e-01 5.23e-01   ph/cm2/s
              Error 6.59e-02 3.90e-02 3.50e-02 5.59e-02 1.16e-01 1.31e-01   ph/cm2/s
 
Fluence   Cutoff-PL 2.87e-07 3.69e-07 2.76e-07 1.54e-07 1.03e-06 1.09e-06   erg/cm2
              Error 3.06e-08 3.23e-08 4.83e-08 1.96e-07 1.08e-07 2.30e-07   erg/cm2
Peak flux Cutoff-PL 1.89e-01 1.72e-01 8.98e-02 3.68e-02 4.75e-01 4.88e-01   ph/cm2/s
              Error 7.20e-02 5.31e-02 4.07e-02 4.52e-02 1.17e-01 1.04e-01   ph/cm2/s
 
Fluence        Band 2.85e-07 3.65e-07 2.73e-07 3.29e-07 1.05e-06 1.25e-06   erg/cm2
              Error -------- 3.11e-08 4.45e-08 -------- 9.44e-08 --------   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    2.245    0.140    -      -           1.19e-03 1.13e-04   57.470 57
CPL   1.712    0.477      20.8   15.9      2.50e-03 2.43e-03   54.940 56
 
 
=== 1-s peak spectral analysis ===
 
Model Ph_index Ph_90err Epeak  Epeak_90err Norm     Nomr_90err chi2   dof
PL    1.836    0.441    -      -           3.44e-03 1.03e-03   75.130 57
CPL   1.349    1.641      54.9    0.0      6.68e-03 0.00e+00   74.920 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: 59.392000 sec.
T50 in the 50-300 keV band: 40.896000 sec.

 
=== Table of the duration information ==
 
        Value   tstart    tstop
T100   96.640   21.096  117.736
T90    73.216   24.808   98.024
T50    31.296   39.336   70.632
Peak    1.000   59.412   60.412

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
   98.4685   -19.8995   0.0090     1.9149    59.9138         1.5992914     21.485 TRIG_00574935                 
 
Foreground time interval of the image:
 21.096  72.901 (delta_t =  51.805 [sec])
Background time interval of the image:
-239.000  21.096 (delta_t = 260.096 [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)

The mask-weighted light curves based on cleaned DPHs

Spectral Evolution

Spectra

Notes:

1) The fitting includes the systematic errors.
2) When the burst includes telescope slew time periods, the fitting uses an average response file made from multiple 5-s response files through out the slew time plus single time preiod for the non-slew times, and weighted by the total counts in the corresponding time period using addrmf. An average response file is needed becuase a spectral fit using the pre-slew DRM will introduce some errors in both a spectral shape and a normalization if the PHA file contains a lot of the slew/post-slew time interval.
3) For fits to more complicated models (e.g. a power-law over a cutoff power-law), the BAT team has decided to require a chi-square improvement of more than 6 for each extra dof.

Time averaged spectrum fit using the average DRM

Power-law model

Time interval is from   21.096 sec. to  117.736 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 2.24462     ( -0.136883   0.142607 )
Norm@50keV  : 1.19428E-03    ( -0.000113898   0.000112442 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          57.47 using 59 PHA bins.
# Reduced chi-squared =          1.008 for     57 degrees of freedom 
# Null hypothesis probability =   4.577727e-01
 
Photon flux (15-150 keV)    in 96.64 sec: 0.202474 ( -0.0136141  0.0136199 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.09246e-06 ( -8.71246e-08  8.86601e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from   21.096 sec. to  117.736 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.71234     ( -0.668119   0.285758 )
Epeak [keV] : 20.7575      ( -19.2289 12.4732 )
Norm@50keV  : 2.50313E-03    ( -0.000999266   0.00385717 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          54.94 using 59 PHA bins.
# Reduced chi-squared =         0.9811 for     56 degrees of freedom 
# Null hypothesis probability =   5.148766e-01
 
Photon flux (15-150 keV)    in 96.64 sec: 0.197522 ( -0.01449  0.014539 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.02553e-06 ( -1.04878e-07  1.11861e-07 ) ergs/cm2

Band function

Time interval is from   21.096 sec. to  117.736 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : 0.716847   ( -4.97158   -2.6122 )
beta        : -2.42347    ( -0.243507   0.197334 )
Epeak [keV] : 23.6622      ( -5.31119 3.67469 )
Norm@50keV   : 0.180415    ( -0.177758   246.875 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          53.36 using 59 PHA bins.
# Reduced chi-squared =         0.9702 for     55 degrees of freedom 
# Null hypothesis probability =   5.373922e-01
 
Photon flux (15-150 keV)    in 96.64 sec:  (    ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.05146e-06 ( -1.05079e-06  -9.36674e-08 ) ergs/cm2

Single BB

 
Spectral model blackbody:
------------------------------------------------------------
Parameters  : value    Lower 90%  Upper 90%
kT [keV]    : 8.39447  (-0.674078  0.733848)
R^2/D10^2   : 0.176062  (-0.0506161   0.0714352)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          93.59 using 59 PHA bins.
# Reduced chi-squared =          1.642 for     57 degrees of freedom 
# Null hypothesis probability =   1.613326e-03
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  2.242e-07   2.464e-08
25- 50  4.258e-07   3.605e-08
50-150  1.307e-07   2.942e-08
15-150  7.807e-07   6.586e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 44.4225       (-7.62876      10.3148)
Norm        : 1.21022       (-0.156157     0.185171)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          55.87 using 59 PHA bins.
# Reduced chi-squared =         0.9801 for     57 degrees of freedom 
# Null hypothesis probability =   5.176518e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  2.774e-07   2.513e-08
25- 50  3.812e-07   2.890e-08
50-150  3.295e-07   7.118e-08
15-150  9.880e-07   9.026e-08

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 5.06361        (-0.927608      1.02402)
R1^2/D10^2  : 0.980507        (-0.48399      1.20516)
kT2 [keV]   : 15.8227        (-3.19317      5.51811)
R2^2/D10^2  : 9.43488E-03    (-0.00674936   0.0130171)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          53.78 using 59 PHA bins.
# Reduced chi-squared =         0.9778 for     55 degrees of freedom 
# Null hypothesis probability =   5.213530e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  2.896e-07   8.925e-08
25- 50  3.605e-07   1.061e-07
50-150  3.506e-07   1.875e-07
15-150  1.001e-06   2.827e-07

Peak spectrum fit

Power-law model

Time interval is from   59.412 sec. to   60.412 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.83598     ( -0.417389   0.46419 )
Norm@50keV  : 3.44213E-03    ( -0.00105243   0.00100201 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          75.13 using 59 PHA bins.
# Reduced chi-squared =          1.318 for     57 degrees of freedom 
# Null hypothesis probability =   5.406302e-02
 
Photon flux (15-150 keV)    in 1 sec: 0.481098 ( -0.115906  0.115907 ) ph/cm2/s
Energy fluence (15-150 keV)             : 3.1656e-08 ( -9.29286e-09  9.75795e-09 ) ergs/cm2

Cutoff power-law model

Time interval is from   59.412 sec. to   60.412 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.34864     ( -2.45037   0.830929 )
Epeak [keV] : 54.9362      (   )
Norm@50keV  : 6.68349E-03    (     )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          74.92 using 59 PHA bins.
# Reduced chi-squared =          1.338 for     56 degrees of freedom 
# Null hypothesis probability =   4.648464e-02
 
Photon flux (15-150 keV)    in 1 sec: 0.474833 ( -0.117911  0.116662 ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.9971e-08 ( -1.00648e-08  1.10425e-08 ) ergs/cm2

Band function

Time interval is from   59.412 sec. to   60.412 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : 4.96804   ( -4.96804   -4.96804 )
beta        : -1.94846    ( -0.749614   0.470682 )
Epeak [keV] : 21.1506      ( -21.1506 8.88648 )
Norm@50keV   : 1404.48    ( -335.786   4.62677e+06 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          74.42 using 59 PHA bins.
# Reduced chi-squared =          1.353 for     55 degrees of freedom 
# Null hypothesis probability =   4.165341e-02
 
Photon flux (15-150 keV)    in 1 sec:  (    ) ph/cm2/s
Energy fluence (15-150 keV)             : 3.01494e-08 ( 0  0 ) ergs/cm2

Single BB

 
Spectral model blackbody:
------------------------------------------------------------
Parameters  : value    Lower 90%  Upper 90%
kT [keV]    : 10.5627  (-2.77689  3.67023)
R^2/D10^2   : 0.188586  (-0.126671   0.396013)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          78.42 using 59 PHA bins.
# Reduced chi-squared =          1.376 for     57 degrees of freedom 
# Null hypothesis probability =   3.147505e-02
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  4.356e-09   2.313e-09
25- 50  1.168e-08   5.004e-09
50-150  7.126e-09   4.405e-09
15-150  2.316e-08   1.335e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 84.8498       (-45.8286      -84.8498)
Norm        : 2.23930       (-0.639354     1.01428)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          74.91 using 59 PHA bins.
# Reduced chi-squared =          1.314 for     57 degrees of freedom 
# Null hypothesis probability =   5.597629e-02
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  5.830e-09   2.413e-09
25- 50  9.731e-09   5.615e-09
50-150  1.428e-08   1.166e-08
15-150  2.984e-08   1.892e-08

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 4.54760        (-2.6812      6.74501)
R1^2/D10^2  : 2.64848        (-2.45911      226.298)
kT2 [keV]   : 15.7574        (-5.86376      -15.7555)
R2^2/D10^2  : 3.34617E-02    (-0.033265   0.187539)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          74.78 using 59 PHA bins.
# Reduced chi-squared =          1.360 for     55 degrees of freedom 
# Null hypothesis probability =   3.920740e-02
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  6.062e-09   3.478e-09
25- 50  9.383e-09   4.817e-09
50-150  1.240e-08   7.550e-09
15-150  2.785e-08   1.510e-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: 2.21794     ( -0.130461   0.135542 )
Norm@50keV  : 1.69870E-03    ( -0.000155113   0.000153283 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          62.99 using 59 PHA bins.
# Reduced chi-squared =          1.105 for     57 degrees of freedom 
# Null hypothesis probability =   2.726709e-01
 
Photon flux (15-150 keV)    in 51.8 sec: 0.283905 ( -0.0186725  0.0186798 ) ph/cm2/s
Energy fluence (15-150 keV)             : 8.29458e-07 ( -6.44729e-08  6.5541e-08 ) ergs/cm2

Cutoff power-law model

Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.47029     ( -0.706973   0.524608 )
Epeak [keV] : 26.8386      (   )
Norm@50keV  : 4.84525E-03    (     )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          58.19 using 59 PHA bins.
# Reduced chi-squared =          1.039 for     56 degrees of freedom 
# Null hypothesis probability =   3.945346e-01
 
Photon flux (15-150 keV)    in 51.8 sec: 0.274795 ( -0.019815  0.019865 ) ph/cm2/s
Energy fluence (15-150 keV)             : 7.5972e-07 ( -7.66847e-08  8.24138e-08 ) ergs/cm2

Band function

 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : 0.877259   ( -1.33634   5.01643 )
beta        : -2.53991    ( -0.376495   0.251249 )
Epeak [keV] : 26.3145      ( -4.37004 4.2456 )
Norm@50keV   : 0.252705    ( -0.24864   178.093 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          53.90 using 59 PHA bins.
# Reduced chi-squared =         0.9800 for     55 degrees of freedom 
# Null hypothesis probability =   5.167897e-01
 
Photon flux (15-150 keV)    in 51.8 sec:  (    ) ph/cm2/s
Energy fluence (15-150 keV)             : 7.80196e-07 ( -7.79833e-07  -6.93084e-08 ) ergs/cm2

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

S(25-50 keV)  = 3.49e-07
S(50-100 keV) = 2.95e-07

T90 vs. Hardness ratio plot

T90                                   = 73.2159999608994 sec.
Hardness ratio (energy fluence ratio) = 0.845272

Color vs. Color plot

Count Ratio  (25-50 keV) / (15-25 keV) = 0.918099
Count Ratio (50-100 keV) / (15-25 keV) = 0.362039

Mask shadow pattern

IMX = 1.676086241716447E-02, IMY = -2.893002242861716E-02

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:
-239.000000 21.096000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
 83.6423  22.0215    0.6  44.2  153.2  10.7513  18.8    0.7	Crab                          
135.5930 -40.5239    1.8  37.0  -51.3   1.9653   6.5    3.5	Vela X-1                      
 64.4819   2.7856    2.7  41.5  113.5   3.3406   4.3 ------	UNKNOWN                       
 76.8144 -58.0095    2.4  42.6   13.7   1.6351   4.8 ------	UNKNOWN                       
 83.7341 -59.1164    2.9  41.8    8.2   1.2475   3.9 ------	UNKNOWN                       
 92.4763 -40.7359    2.5  22.7   11.1   0.9097   4.7 ------	UNKNOWN                       
107.4238 -38.7993    2.6  20.7  -20.3   0.8678   4.5 ------	UNKNOWN                       
110.9571 -39.2946    2.2  22.2  -26.7   0.9997   5.4 ------	UNKNOWN                       
119.5836  -8.9615    2.5  21.2 -120.2   0.9266   4.7 ------	UNKNOWN                       
129.7111  21.4686    3.2  49.7 -147.6   1.8640   3.6 ------	UNKNOWN                       
139.3189   7.1541    2.3  46.5 -125.1   4.4598   4.9 ------	UNKNOWN

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

Time interval of the image:
21.096000 72.900600
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
 83.5141  22.0594   16.7  44.3  153.0   0.1303   0.7    7.2	Crab                          
135.5557 -40.6032   10.4  37.0  -51.2  -0.1413  -1.1    3.2	Vela X-1                      
 88.0494  -9.1935    2.1  15.4  123.7   0.4175   5.5 ------	UNKNOWN                       
 98.4686 -19.8995    0.5   1.9   59.9   1.5989  21.5 ------	UNKNOWN                       
116.8525 -33.9556    2.3  20.9  -45.8   0.3908   5.0 ------	UNKNOWN

Post-slew image of 15-350 keV band

Time interval of the image:
97.700600 963.157200
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
 83.6363  22.0199    0.5  44.3  145.9  35.3048  22.6    0.4	Crab                          
135.5422 -40.5441    2.0  37.7  -62.8   7.0128   5.7    0.9	Vela X-1                      
 61.8123 -59.8268    3.4  47.7    9.6   3.3336   3.4 ------	UNKNOWN                       
107.4301  19.4387    2.5  40.3  178.8   3.1086   4.6 ------	UNKNOWN                       
112.5538  31.5532    3.1  53.2 -179.3   5.7331   3.7 ------	UNKNOWN                       
114.3916 -41.6078    2.8  25.6  -42.7   1.9926   4.1 ------	UNKNOWN                       
135.1635 -75.6264    3.8  58.9  -24.3  10.8253   3.0 ------	UNKNOWN                       
142.1600 -18.9200    4.7  41.1  -98.0   7.6233   2.5 ------	UNKNOWN                       
141.2322   0.3896    2.6  46.5 -125.0  10.2383   4.4 ------	UNKNOWN                       
141.0129   3.6796    2.9  48.0 -129.0   8.7098   3.9 ------	UNKNOWN

Plot creation:
Sat May 30 15:22:32 EDT 2015