batgrbproduct analysis for trigger=1159434

batgrbproduct Analysis for Trigger=1159434

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 12 21:03:44 EDT 2023
             Host Name: batproc1
   Current Working Dir: /local/data/bat1/prebascript/trigger1159434/GCN5_download_cron
======================================================================

  Trigger: 01159434      Segment: 000

  BAT Trigger Time: 700255520   [s; MET]
      Trigger Stop: 700255584   [s; MET]
               UTC: 2023-03-11T19:24:49.094260    [includes UTCF correction] 
       Where From?: TDRSS position message

  BAT 
    RA: 245.066957005906   Dec: -15.8906021868497  [deg; J2000]

     Catalogged Source?: NO
     Point Source?:      YES
     GRB Indicated?:     YES    [ by BAT flight software ]
     Image S/N Ratio:    17.72
     Image Trigger?:     YES
     Rate S/N Ratio:     0  [ if not an image trigger ]
     Image S/N Ratio:    17.72

  Flight Position:   [ source = BAT ]
    RA: 245.066957005906   Dec: -15.8906021868497  [deg; J2000]

  Ground Position:   [ source = BAT pre-slew burst ]
    RA: 245.06376051322   Dec: -15.897581451149  [deg; J2000]  
        { 16h 20m 15.3s , -15d 53' 51.3" }
         +/- 1.21573880694128 [arcmin] (estimated 90% radius based on SNR)
         +/- 0.570162590937613 [arcmin] (formal 1-sigma fit error)
    SNR: 23.010072141404
 
  Angular difference between Flight and Ground position is 0.457582 arcmin
 
  Partial Coding Fraction: 0.4570312    [ including projection effects ]

  Duration
     T90: 115.379999995232 +/- 52.6633451861103
        Measured from: -53.3119999170303
                   to: 62.0680000782013     [s; relative to TRIGTIME]
     T50: 42.472000002861 +/- 18.1569677337846
        Measured from: -35.663999915123
                   to: 6.80800008773804     [s; relative to TRIGTIME]



  Fluence
     Peak Flux  (peak 1 second)
        Measured from: 5.24399995803833     
                   to: 6.24399995803833     [s; relative to TRIGTIME]
     Total Fluence        
        Measured from: -55.0319999456406     
                   to: 113.468000054359     [s; relative to TRIGTIME]
     
             Band 1     Band 2     Band 3     Band 4
              15-25      25-50     50-100    100-350     keV
 Total     9.495866   1.050928  -0.227293  -0.118442
           0.167739   0.150050   0.126364   0.106108 [error]
 Peak      0.085284   0.025787   0.014057   0.012643
           0.013860   0.012042   0.010142   0.008040 [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 3.74e-06 4.63e-07 2.47e-08 1.39e-09 4.23e-06 4.23e-06   erg/cm2
              Error 3.56e-07 7.48e-08 1.02e-08 9.89e-10 3.53e-07 3.53e-07   erg/cm2
Peak flux Power-law 1.09e+00 2.72e-01 3.53e-02 5.15e-03 1.40e+00 1.40e+00   ph/cm2/s
              Error 2.80e-01 1.24e-01 4.16e-02 1.09e-02 3.47e-01 3.48e-01   ph/cm2/s
 
Fluence   Cutoff-PL 3.75e-06 3.57e-07 1.35e-09 3.73e-14 4.10e-06 4.10e-06   erg/cm2
              Error 3.80e-07 1.10e-07 7.98e-09 1.20e-10 3.81e-07 3.81e-07   erg/cm2
Peak flux Cutoff-PL 1.14e+00 2.40e-01 3.75e-03 1.10e-06 1.38e+00 1.38e+00   ph/cm2/s
              Error 3.08e-01 2.02e-01 3.86e-02 9.47e-03 3.38e-01 3.38e-01   ph/cm2/s
 
Fluence        Band -------- -------- -------- -------- -------- --------   erg/cm2
              Error -------- -------- -------- -------- -------- --------   erg/cm2
Peak flux      Band 1.09e+00 2.76e-01 3.41e-02 4.46e-03 1.40e+00 1.40e+00   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    6.225    0.367    -      -           1.66e-04 5.59e-05   61.670 57
CPL   1.000    0.000      50.0    0.0      3.12e-03 0.00e+00  428.680 56
 
 
=== 1-s peak spectral analysis ===
 
Model Ph_index Ph_90err Epeak  Epeak_90err Norm     Nomr_90err chi2   dof
PL    3.943    0.893    -      -           2.39e-03 1.94e-03   59.180 57
CPL   1.000    0.000      50.0    0.0      1.87e-02 0.00e+00   84.070 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  168.500  -55.032  113.468
T90   115.380  -53.312   62.068
T50    42.472  -35.664    6.808
Peak    1.000    5.244    6.244

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
  245.0638 -15.8976 0.0083   42.1    1.3       5.4507    23.0  TRIG_01159434       
------------------------------------------
 
Foreground time interval of the image:
-17.599  29.710 (delta_t =  47.309 [sec])
 31.000  71.801 (delta_t =  40.801 [sec])
Background time interval of the image:

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
-55.032000 -47.510000
-46.000000 29.710000
31.000000 113.468000
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 6.22485     ( -0.364486   0.369189 )
Norm@50keV  : 1.66376E-04    ( -4.82965e-05   6.35122e-05 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          61.67 using 59 PHA bins.
# Reduced chi-squared =          1.082 for     57 degrees of freedom 
# Null hypothesis probability =   3.126385e-01
 
Photon flux (15-150 keV)    in 165.7 sec: 0.858939 ( -0.0777894  0.0783349 ) ph/cm2/s
Energy fluence (15-150 keV)             : 4.22934e-06 ( -3.52098e-07  3.54055e-07 ) ergs/cm2

Cutoff power-law model

Multiple GTIs in the spectrum
tstart tstop
-55.032000 -47.510000
-46.000000 29.710000
31.000000 113.468000
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.00000     (     )
Epeak [keV] : 50.0000      (   )
Norm@50keV  : 3.11661E-03    (     )
------------------------------------------------------------
#Fit statistic : Chi-Squared =         428.68 using 59 PHA bins.
# Reduced chi-squared =         7.6550 for     56 degrees of freedom 
# Null hypothesis probability =   7.479867e-59
 
Photon flux (15-150 keV)    in 165.7 sec: 0.840838 ( -0.084715  0.083551 ) ph/cm2/s
Energy fluence (15-150 keV)             : 4.10376e-06 ( -3.84507e-07  3.78127e-07 ) ergs/cm2

Band function

Multiple GTIs in the spectrum
tstart tstop
-55.032000 -47.510000
-46.000000 29.710000
31.000000 113.468000
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : 3.48759   ( -12.3282   -3.4877 )
beta        : -7.13681    ( -1.87863   0.80466 )
Epeak [keV] : 11.0880      ( -1.40625 1.26324 )
Norm@50keV   : 2.76264E+04    ( -27815.3   154200 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          56.39 using 59 PHA bins.
# Reduced chi-squared =          1.025 for     55 degrees of freedom 
# Null hypothesis probability =   4.225573e-01
 
Photon flux (15-150 keV)    in 165.7 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]    : 2.52802  (-0.160416  0.180406)
R^2/D10^2   : 377.000  (-164.692   282.364)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          59.40 using 59 PHA bins.
# Reduced chi-squared =          1.042 for     57 degrees of freedom 
# Null hypothesis probability =   3.883001e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  3.714e-06   5.543e-07
25- 50  2.856e-07   5.965e-08
50-150  1.006e-10   6.486e-11
15-150  4.000e-06   5.990e-07

Thermal bremsstrahlung (OTTB)

XSPEC12>exit
 XSPEC: quit
 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 4.37090       (-0.40326      0.479649)
Norm        : 324.292       (-123.014     195.554)
------------------------------------------------------------
 Reduced chi-squared = 
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  3.747e-06   5.957e-07
25- 50  3.437e-07   6.703e-08
50-150  8.633e-10   5.157e-10
15-150  4.092e-06   5.791e-07

Double BB

XSPEC12>exit
 XSPEC: quit
 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 4.88903        (-2.3256      6.82307)
R1^2/D10^2  : 0.970538        (-0.931582      328.721)
kT2 [keV]   : 2.26493        (-2.26781      0.311695)
R2^2/D10^2  : 800.990    (-483.148   -791.021)
------------------------------------------------------------
 Reduced chi-squared = 
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  2.364e-06   1.472e-02
25- 50  5.715e-07   1.669e-01
50-150  2.913e-09   3.810e+00
15-150  2.938e-06   3.678e+00

Peak spectrum fit

Power-law model

Time interval is from    5.244 sec. to    6.244 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 3.94332     ( -0.770463   1.01552 )
Norm@50keV  : 2.39033E-03    ( -0.00155551   0.00232054 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          59.18 using 59 PHA bins.
# Reduced chi-squared =          1.038 for     57 degrees of freedom 
# Null hypothesis probability =   3.960463e-01
 
Photon flux (15-150 keV)    in 1 sec: 1.40310 ( -0.34684  0.347694 ) ph/cm2/s
Energy fluence (15-150 keV)             : 5.05411e-08 ( -1.44743e-08  1.58739e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from    5.244 sec. to    6.244 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.00000     (     )
Epeak [keV] : 50.0000      (   )
Norm@50keV  : 1.87444E-02    (     )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          84.07 using 59 PHA bins.
# Reduced chi-squared =          1.501 for     56 degrees of freedom 
# Null hypothesis probability =   8.976476e-03
 
Photon flux (15-150 keV)    in 1 sec: 1.37988 ( -0.33432  0.34203 ) ph/cm2/s
Energy fluence (15-150 keV)             : 4.59515e-08 ( -1.24027e-08  1.85607e-08 ) ergs/cm2

Band function

Time interval is from    5.244 sec. to    6.244 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -9.31371   ( 6.45176   9.31371 )
beta        : -3.94312    ( -1.01554   0.770788 )
Epeak [keV] : 209.596      ( -209.596 -209.596 )
Norm@50keV   : 0.324939    ( -0.211421   0.31539 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          59.18 using 59 PHA bins.
# Reduced chi-squared =          1.076 for     55 degrees of freedom 
# Null hypothesis probability =   3.257156e-01
 
Photon flux (15-150 keV)    in 1 sec: 1.40191 (    ) ph/cm2/s
Energy fluence (15-150 keV)             : 0 ( 0  0 ) ergs/cm2

Single BB

 XSPEC: quit
 
 
Spectral model blackbody:
------------------------------------------------------------
Parameters  : value    Lower 90%  Upper 90%
kT [keV]    : 3.73641  (-0.812517  1.02973)
R^2/D10^2   : 53.2380  (-53.238   168.321)
(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  3.446e-08   2.022e-08
25- 50  1.020e-08   6.220e-09
50-150  8.093e-11   8.535e-11
15-150  4.474e-08   2.641e-08

Thermal bremsstrahlung (OTTB)

XSPEC12>exit
 XSPEC: quit
 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 9.00619       (-3.15658      5.75631)
Norm        : 60.5259       (-36.2541     118.782)
------------------------------------------------------------
 Reduced chi-squared = 
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  3.351e-08   1.844e-08
25- 50  1.247e-08   7.735e-09
50-150  6.351e-10   6.965e-10
15-150  4.662e-08   2.790e-08

Double BB

XSPEC12>exit
 XSPEC: quit
 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 3.52673        (-3.52365      1.13906)
R1^2/D10^2  : 69.7203        (-69.8152      -69.8152)
kT2 [keV]   : 13.7290        (-13.5974      -13.5974)
R2^2/D10^2  : 2.37921E-02    (-0.0245002   -0.0245002)
------------------------------------------------------------
 Reduced chi-squared = 
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  3.424e-08   1.965e-08
25- 50  1.172e-08   7.050e-09
50-150  4.296e-09   3.658e-09
15-150  5.026e-08   2.803e-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: 6.23972     ( -0.431179   0.443937 )
Norm@50keV  : 1.59270E-04    ( -5.6119e-05   7.84993e-05 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          48.15 using 59 PHA bins.
# Reduced chi-squared =         0.8448 for     57 degrees of freedom 
# Null hypothesis probability =   7.917448e-01
 
Photon flux (15-150 keV)    in 88.11 sec: 0.834717 ( -0.0818768  0.0821003 ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.18404e-06 ( -2.02723e-07  2.03008e-07 ) 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  : 3.60069E-03    (     )
------------------------------------------------------------
#Fit statistic : Chi-Squared =         313.50 using 59 PHA bins.
# Reduced chi-squared =         5.5982 for     56 degrees of freedom 
# Null hypothesis probability =   1.737491e-37
 
Photon flux (15-150 keV)    in 88.11 sec: 0.823749 ( -0.089465  0.088184 ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.12112e-06 ( -2.16336e-07  2.13024e-07 ) ergs/cm2

Band function

 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -9.29202   ( 6.63061   9.29202 )
beta        : -6.25122    ( -0.434504   0.440872 )
Epeak [keV] : 338.924      ( -338.924 -338.924 )
Norm@50keV   : 2.13491E-02    ( -0.00747177   0.0108274 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          48.16 using 59 PHA bins.
# Reduced chi-squared =         0.8756 for     55 degrees of freedom 
# Null hypothesis probability =   7.314700e-01
 
Photon flux (15-150 keV)    in 88.11 sec:  (    ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.83506e-06 ( 0  0 ) ergs/cm2

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

S(25-50 keV)  = 4.63e-07
S(50-100 keV) = 2.47e-08

T90 vs. Hardness ratio plot

T90                                   = 115.379999995232 sec.
Hardness ratio (energy fluence ratio) = 0.0533477

Color vs. Color plot

Count Ratio  (25-50 keV) / (15-25 keV) = 0.110672
Count Ratio (50-100 keV) / (15-25 keV) = -0.023936

Mask shadow pattern

IMX = 9.031645455006951E-01, IMY = -2.050299161781746E-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:

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

Time interval of the image:
-17.599400 29.710000
31.000000 71.800590
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
245.0459 -15.7828    1.2  42.0    1.3   2.2511   9.5    9.4	Sco X-1                       
254.5575  35.1968    2.5  15.6 -121.3   0.7084   4.6   10.0	Her X-1                       
263.0025 -24.7468  133.8  55.3  -17.0   0.0506   0.1    0.4	GX 1+4                        
268.4934  -1.5376    4.7  38.9  -40.9   0.6604   2.4    9.1	SW J1753.5-0127               
270.1678 -25.1583    6.6  58.8  -23.5  -1.7108  -1.7    7.9	GX 5-1                        
273.8744 -14.1114    7.2  51.9  -34.8   1.1122   1.6    8.9	GX 17+2                       
297.2807  59.9461    2.6  51.6 -138.7   3.9282   4.5 ------	UNKNOWN

Post-slew image of 15-350 keV band

Time interval of the image:
160.100590 248.630000
250.000000 296.850000
298.000000 303.059600
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
245.0725 -15.8044    0.3   0.1  179.5   9.6417  39.2   11.2	Sco X-1                       
254.5893  35.4328    7.7  52.1 -178.2   1.3730   1.5    8.4	Her X-1                       
255.9635 -37.9908    4.9  24.1  -29.5   0.6839   2.3    8.9	4U 1700-377                   
256.2753 -36.2742    0.0  22.7  -32.0  -0.2129  -0.7   11.8	GX 349+2                      
262.8851 -24.6807    6.1  18.9  -67.4  -0.6120  -1.9    7.8	GX 1+4                        
264.9227 -44.5783    0.0  33.2  -34.3   0.7869   2.2   10.9	4U 1735-44                    
268.4752  -1.6083    9.9  27.1 -127.5  -0.3988  -1.2   11.3	SW J1753.5-0127               
270.1734 -24.9466   12.2  25.2  -72.9  -0.3426  -0.9   10.0	GX 5-1                        
270.2832 -25.7953    9.4  25.5  -71.1   0.4501   1.2    3.3	GRS 1758-258                  
274.0046 -14.0401   97.9  28.0  -98.0   0.0488   0.1    0.2	GX 17+2                       
275.7545 -30.3326    8.3  31.6  -65.4  -0.6655  -1.4    9.1	H1820-303                     
284.8657 -24.8408    7.9  38.2  -77.9   1.0477   1.5   10.4	HT1900.1-2455                 
263.1238 -33.7658    7.5  24.2  -47.1   0.5042   1.5    7.9	GX 354-0                      
211.4714 -33.0274    3.3  34.8   46.3   1.4171   3.5 ------	UNKNOWN                       
252.5231  39.2754    3.0  55.6  179.0   6.1770   3.9 ------	UNKNOWN                       
248.5142 -47.6485    1.9  31.9  -12.5   1.9392   6.2 ------	UNKNOWN

Plot creation:
Sun Mar 12 21:07:17 EDT 2023