batgrbproduct analysis for trigger=1218404

batgrbproduct Analysis for Trigger=1218404

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 15 downlinks after the trigger.

======================================================================
                  BAT GRB EVENT DATA PROCESSING REPORT
    Process Script Ver: batgrbproduct v2.48
    Process Start Time (local time): Sun Mar  3 20:43:27 EST 2024
             Host Name: batproc1
   Current Working Dir: /local/data/bat1/prebascript/trigger1218404/GCN5_download_cron
======================================================================

  Trigger: 01218404      Segment: 000

  BAT Trigger Time: 731110168   [s; MET]
      Trigger Stop: 731110232   [s; MET]
               UTC: 2024-03-02T22:08:54.984140    [includes UTCF correction] 
       Where From?: TDRSS position message

  BAT 
    RA: 83.9211995347879   Dec: 21.7069229314846  [deg; J2000]

     Catalogged Source?: NO
     Point Source?:      YES
     GRB Indicated?:     YES    [ by BAT flight software ]
     Image S/N Ratio:    8.75
     Image Trigger?:     YES
     Rate S/N Ratio:     0  [ if not an image trigger ]
     Image S/N Ratio:    8.75

  Flight Position:   [ source = BAT ]
    RA: 83.9211995347879   Dec: 21.7069229314846  [deg; J2000]

  Ground Position:   [ source = BAT pre-slew burst ]
    RA: 83.9029284361916   Dec: 21.7268285549533  [deg; J2000]  
        { 05h 35m 36.7s , +21d 43' 36.6" }
         +/- 3.43376292467517 [arcmin] (estimated 90% radius based on SNR)
         +/- 1.94668072536896 [arcmin] (formal 1-sigma fit error)
    SNR: 5.22074194353608
 
  Angular difference between Flight and Ground position is 1.569617 arcmin
 
  Partial Coding Fraction: 0.734375    [ including projection effects ]

  Duration
     T90: 224 +/- 16
        Measured from: -62.9999998807907
                   to: 161.000000119209     [s; relative to TRIGTIME]
     T50: 96 +/- 22.6274169979695
        Measured from: -14.9999998807907
                   to: 81.0000001192093     [s; relative to TRIGTIME]



  Fluence
     Peak Flux  (peak 1 second)
        Measured from: 24.5     
                   to: 25.5     [s; relative to TRIGTIME]
     Total Fluence        
        Measured from: -63     
                   to: 193     [s; relative to TRIGTIME]
     
             Band 1     Band 2     Band 3     Band 4
              15-25      25-50     50-100    100-350     keV
 Total     3.283612   3.439159   1.898380   0.247368
           0.135037   0.153235   0.140510   0.143365 [error]
 Peak      0.026170   0.018166   0.018280   0.000976
           0.009338   0.010673   0.009541   0.009370 [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 1.09e-06 1.47e-06 1.46e-06 2.60e-06 4.87e-06 6.63e-06   erg/cm2
              Error 8.99e-08 7.85e-08 1.38e-07 5.00e-07 3.09e-07 6.37e-07   erg/cm2
Peak flux Power-law 1.90e-01 1.61e-01 9.27e-02 7.94e-02 4.79e-01 5.24e-01   ph/cm2/s
              Error 1.35e-01 1.22e-01 7.34e-02 1.46e-01 2.46e-01 2.80e-01   ph/cm2/s
 
Fluence   Cutoff-PL 1.07e-06 1.51e-06 1.45e-06 1.77e-06 4.76e-06 5.79e-06   erg/cm2
              Error 1.01e-07 9.93e-08 1.45e-07 9.42e-07 3.69e-07 1.08e-06   erg/cm2
Peak flux Cutoff-PL 1.91e-01 1.61e-01 9.24e-02 7.76e-02 4.79e-01 5.15e-01   ph/cm2/s
              Error 1.32e-01 1.16e-01 1.19e-02 1.35e-01 2.46e-01 3.25e-01   ph/cm2/s
 
Fluence        Band 1.04e-06 1.52e-06 1.41e-06 2.29e-06 4.76e-06 6.28e-06   erg/cm2
              Error 1.11e-07 -------- 1.52e-07 -------- 3.37e-07 --------   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    2.014    0.109    -      -           2.12e-03 1.42e-04   67.670 57
CPL   1.803    0.389      40.3   -2.5      2.78e-03 1.52e-03   66.830 56
 
 
=== 1-s peak spectral analysis ===
 
Model Ph_index Ph_90err Epeak  Epeak_90err Norm     Nomr_90err chi2   dof
PL    1.796    1.048    -      -           3.48e-03 2.19e-03   63.670 57
CPL  -9.981   -0.904      25.8    4.9      2.82e+06 1.31e+07   60.420 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  256.000  -63.000  193.000
T90   224.000  -63.000  161.000
T50    96.000  -15.000   81.000
Peak    1.000   24.500   25.500

Click here for the BAT GCN circular template

Estimated redshift from machine learning (Ukwatta et al. 2016) - may take a few minutes to calcaulte

Image

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

#   RAcent  DECcent POSerr  Theta    Phi     Peak Cts     SNR  Name
   83.9029 +21.7268 0.0368   31.8    4.8       5.2326     5.2  TRIG_01218404       
------------------------------------------
 
Foreground time interval of the image:
-63.000 -26.460 (delta_t =  36.540 [sec])
-25.000  12.680 (delta_t =  37.680 [sec])
 14.000  42.450 (delta_t =  28.450 [sec])
 43.000  70.101 (delta_t =  27.101 [sec])
Background time interval of the image:
-239.000 -201.870 (delta_t =  37.130 [sec])
-119.000 -63.000 (delta_t =  56.000 [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

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)

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

Multiple GTIs in the spectrum
tstart tstop
-63.000000 -26.460000
-25.000000 12.680000
14.000000 42.450000
43.000000 179.570000
181.000000 190.960000
192.000000 192.210000
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 2.01378     ( -0.107485   0.110565 )
Norm@50keV  : 2.11764E-03    ( -0.000142899   0.000140981 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          67.67 using 59 PHA bins.
# Reduced chi-squared =          1.187 for     57 degrees of freedom 
# Null hypothesis probability =   1.574693e-01
 
Photon flux (15-150 keV)    in 249.4 sec: 0.319676 ( -0.0172999  0.0173157 ) ph/cm2/s
Energy fluence (15-150 keV)             : 4.8741e-06 ( -3.06777e-07  3.10458e-07 ) ergs/cm2

Cutoff power-law model

Multiple GTIs in the spectrum
tstart tstop
-63.000000 -26.460000
-25.000000 12.680000
14.000000 42.450000
43.000000 179.570000
181.000000 190.960000
192.000000 192.210000
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.80324     ( -0.427195   0.350866 )
Epeak [keV] : 40.3444      ( -35.3843 -40.3443 )
Norm@50keV  : 2.77753E-03    ( -0.0010311   0.00199947 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          66.83 using 59 PHA bins.
# Reduced chi-squared =          1.193 for     56 degrees of freedom 
# Null hypothesis probability =   1.524732e-01
 
Photon flux (15-150 keV)    in 249.4 sec: 0.315829 ( -0.018588  0.018593 ) ph/cm2/s
Energy fluence (15-150 keV)             : 4.76207e-06 ( -3.68164e-07  3.69137e-07 ) ergs/cm2

Band function

Multiple GTIs in the spectrum
tstart tstop
-63.000000 -26.460000
-25.000000 12.680000
14.000000 42.450000
43.000000 179.570000
181.000000 190.960000
192.000000 192.210000
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -1.80343   ( 1.73544   0.372743 )
beta        : -10.0000    ( 10   4.79616e-14 )
Epeak [keV] : 40.3287      ( -29.293 -40.3287 )
Norm@50keV   : 2.77628E-03    ( -0.000720569   0.00200024 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          66.83 using 59 PHA bins.
# Reduced chi-squared =          1.215 for     55 degrees of freedom 
# Null hypothesis probability =   1.317196e-01
 
Photon flux (15-150 keV)    in 249.4 sec: 0.272982 (    ) ph/cm2/s
Energy fluence (15-150 keV)             : 4.75708e-06 ( -4.75533e-06  -3.35992e-07 ) ergs/cm2

Single BB

 
Spectral model blackbody:
------------------------------------------------------------
Parameters  : value    Lower 90%  Upper 90%
kT [keV]    : 9.80432  (  )
R^2/D10^2   : 0.152332  (   )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =         147.00 using 59 PHA bins.
# Reduced chi-squared =         2.5790 for     57 degrees of freedom 
# Null hypothesis probability =   6.938362e-10
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  7.385e-07   6.734e-08
25- 50  1.785e-06   1.107e-07
50-150  8.796e-07   1.319e-07
15-150  3.403e-06   2.182e-07

Thermal bremsstrahlung (OTTB)

XSPEC12>exit
 XSPEC: quit
 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 67.9432       (-11.3679      15.072)
Norm        : 1.56193       (-0.143287     0.163381)
------------------------------------------------------------
 Reduced chi-squared = 
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  9.961e-07   7.482e-08
25- 50  1.572e-06   8.729e-08
50-150  1.974e-06   2.837e-07
15-150  4.542e-06   3.105e-07

Double BB

XSPEC12>exit
 XSPEC: quit
 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 6.10800        (-0.767387      0.794482)
R1^2/D10^2  : 0.731216        (-0.267466      0.490825)
kT2 [keV]   : 23.1011        (-4.09358      5.93857)
R2^2/D10^2  : 4.13760E-03    (-0.0023249   0.00463327)
------------------------------------------------------------
 Reduced chi-squared = 
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.027e-06   1.546e-07
25- 50  1.503e-06   2.245e-07
50-150  2.253e-06   7.708e-07
15-150  4.782e-06   1.080e-06

Peak spectrum fit

Power-law model

Time interval is from   24.500 sec. to   25.500 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.79641     ( -0.97972   1.11714 )
Norm@50keV  : 3.47964E-03    ( -0.00225003   0.00213646 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          63.67 using 59 PHA bins.
# Reduced chi-squared =          1.117 for     57 degrees of freedom 
# Null hypothesis probability =   2.534300e-01
 
Photon flux (15-150 keV)    in 1 sec: 0.478821 ( -0.245961  0.246066 ) ph/cm2/s
Energy fluence (15-150 keV)             : 3.20376e-08 ( -1.91009e-08  2.20525e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from   24.500 sec. to   25.500 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: -9.98083     ( 9.99207   8.18429 )
Epeak [keV] : 25.7549      ( -4.50514 5.2874 )
Norm@50keV  : 2.81783E+06    ( -2.91223e+06   2.33612e+07 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          60.42 using 59 PHA bins.
# Reduced chi-squared =          1.079 for     56 degrees of freedom 
# Null hypothesis probability =   3.193867e-01
 
Photon flux (15-150 keV)    in 1 sec: 0.478856 ( -0.246004  0.245408 ) ph/cm2/s
Energy fluence (15-150 keV)             : 5.34844e-16 ( 0  0 ) ergs/cm2

Band function

Time interval is from   24.500 sec. to   25.500 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : 5.00000   ( -5   -5 )
beta        : -3.19481    ( 3.23633   1.92029 )
Epeak [keV] : 26.2849      ( -26.3335 9.03945 )
Norm@50keV   : 492.872    ( -226.756   4.31882e+06 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          61.41 using 59 PHA bins.
# Reduced chi-squared =          1.117 for     55 degrees of freedom 
# Null hypothesis probability =   2.571390e-01
 
Photon flux (15-150 keV)    in 1 sec:  (    ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.32536e-08 ( -2.32466e-08  -2.32536e-08 ) ergs/cm2

Single BB

 XSPEC: quit
 
 
Spectral model blackbody:
------------------------------------------------------------
Parameters  : value    Lower 90%  Upper 90%
kT [keV]    : 6.73321  (-2.28833  5.56669)
R^2/D10^2   : 1.06710  (-1.06875   4.7235)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
 Reduced chi-squared = 
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  7.451e-09   4.769e-09
25- 50  9.453e-09   6.440e-09
50-150  1.358e-09   1.361e-09
15-150  1.826e-08   1.226e-08

Thermal bremsstrahlung (OTTB)

XSPEC12>exit
 XSPEC: quit
 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 79.0758       (-79.2752      -79.2752)
Norm        : 2.26143       (-1.28609     4.70243)
------------------------------------------------------------
 Reduced chi-squared = 
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  5.864e-09   3.887e-09
25- 50  9.625e-09   6.415e-09
50-150  1.348e-08   1.343e-08
15-150  2.897e-08   2.232e-08

Double BB

XSPEC12>exit
 XSPEC: quit
 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 6.27083        (-6.06456      4.39811)
R1^2/D10^2  : 1.31169        (-1.3534      6.84229)
kT2 [keV]   : 78.9927        (-79.446      -79.446)
R2^2/D10^2  : 3.00409E-04    (-0.000298293   2.78666)
------------------------------------------------------------
 Reduced chi-squared = 
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  6.386e-09   5.000e-09
25- 50  8.496e-09   5.125e-09
50-150  1.796e-08   8.935e-09
15-150  3.285e-08   1.705e-08

Pre-slew spectrum (Pre-slew PHA with pre-slew DRM)

Power-law model

 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.86598     ( -0.124829   0.128846 )
Norm@50keV  : 2.63084E-03    ( -0.00021667   0.000213507 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          82.15 using 59 PHA bins.
# Reduced chi-squared =          1.441 for     57 degrees of freedom 
# Null hypothesis probability =   1.626057e-02
 
Photon flux (15-150 keV)    in 129.8 sec: 0.372217 ( -0.0248989  0.0249023 ) ph/cm2/s
Energy fluence (15-150 keV)             : 3.13937e-06 ( -2.56053e-07  2.59893e-07 ) ergs/cm2

Cutoff power-law model

Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.47136     ( -0.5573   0.460755 )
Epeak [keV] : 56.7222      ( -15.456 -56.7226 )
Norm@50keV  : 4.42470E-03    ( -0.00193971   0.0047869 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          80.20 using 59 PHA bins.
# Reduced chi-squared =          1.432 for     56 degrees of freedom 
# Null hypothesis probability =   1.863114e-02
 
Photon flux (15-150 keV)    in 129.8 sec: 0.365724 ( -0.026069  0.026056 ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.99789e-06 ( -3.0673e-07  3.10585e-07 ) ergs/cm2

Band function

 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -1.47139   ( 1.55517   0.859939 )
beta        : -10.0000    ( 10   1.77636e-15 )
Epeak [keV] : 56.7122      ( -15.4555 -56.7122 )
Norm@50keV   : 4.42378E-03    ( -0.00182714   0.00479969 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          80.20 using 59 PHA bins.
# Reduced chi-squared =          1.458 for     55 degrees of freedom 
# Null hypothesis probability =   1.491292e-02
 
Photon flux (15-150 keV)    in 129.8 sec: 0.367580 (    ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.71313e-06 ( 0  0 ) ergs/cm2

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

S(25-50 keV)  = 1.47e-06
S(50-100 keV) = 1.46e-06

T90 vs. Hardness ratio plot

T90                                   = 224 sec.
Hardness ratio (energy fluence ratio) = 0.993197

Color vs. Color plot

Count Ratio  (25-50 keV) / (15-25 keV) = 1.04737
Count Ratio (50-100 keV) / (15-25 keV) = 0.578138

Mask shadow pattern

IMX = 6.180300649375540E-01, IMY = -5.188463605202472E-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 -201.870000
-119.000000 -63.000000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
 83.6395  21.9159    4.2  32.0    4.4   0.2077   2.8    5.9	Crab                          
 47.3680  31.8653    2.2  56.0  -31.0   1.9023   5.1 ------	UNKNOWN                       
 45.3163  21.2182    2.6  50.9  -42.9   1.3936   4.4 ------	UNKNOWN

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

Time interval of the image:
-63.000000 -26.460000
-25.000000 12.680000
14.000000 42.450000
43.000000 70.100610
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
 83.7947  21.8857    6.7  32.0    4.6   1.7544   1.7   11.9	Crab                          
107.7598  36.5693    3.5  50.7   31.3  11.9345   3.3 ------	UNKNOWN                       
104.3387  40.0227    3.0  52.7   26.4  15.0955   3.8 ------	UNKNOWN                       
101.6998  38.2027    2.7  50.3   24.8  11.4933   4.2 ------	UNKNOWN                       
107.2829  17.6642    3.5  34.6   46.0   3.8570   3.3 ------	UNKNOWN                       
119.6019 -42.9359    2.3  43.9  153.6   8.6954   5.1 ------	UNKNOWN                       
101.2549  23.3020    3.2  36.4   32.6   3.9799   3.6 ------	UNKNOWN                       
106.7808 -36.0852    2.4  32.0  156.9   4.8554   4.8 ------	UNKNOWN                       
 83.2334  30.4004    3.0  40.5    5.0   4.3322   3.9 ------	UNKNOWN                       
 69.8201 -55.1387    2.3  47.0 -158.1   8.7250   5.0 ------	UNKNOWN

Post-slew image of 15-350 keV band

Time interval of the image:
142.100600 179.570000
181.000000 190.960000
192.000000 192.210000
194.000000 195.560000
197.000000 239.020000
240.000000 295.100000
296.000000 303.055700
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
 83.7644  22.1710    5.3   0.5  -15.4  -0.7576  -2.2   11.9	Crab                          
118.9455  26.4422    3.2  32.2   77.4   2.1782   3.5 ------	UNKNOWN                       
111.7448  50.8614    2.8  36.3   32.7   2.3028   4.2 ------	UNKNOWN                       
 55.3794 -12.3675    1.9  44.1 -135.0   5.1391   6.1 ------	UNKNOWN                       
 55.8670 -20.5314    2.3  50.4 -142.2   5.3971   4.9 ------	UNKNOWN                       
 24.7450  56.5374    1.8  55.2  -32.3  11.7124   6.3 ------	UNKNOWN

Plot creation:
Sun Mar  3 20:46:03 EST 2024