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Example Report

Here is an example of the report produced by ASTROM. It is the result of a run using the specimen input file presented in Section 3. The first part of the report lists the raw data. The second part gives the results of the 4-coefficient solution. The third part (next page) gives the results of the 6-coefficient solution. The fourth part gives the predictions for the unknown stars.

It should be noted that the report file contains Fortran printer codes.

1* * * * * * * * * * * * *
 *  A S T R O M E T R Y  *
 * * * * * * * * * * * * *



 Equinox for mean coordinates of results:  B1950.0

 Projection geometry:  Schmidt                                 

 Plate centre:  19 04 00.0   -65 00 00     Equinox B1950.0     Epoch B1974.500


 Reference stars:

                n              RA            Dec         pmR    pmD   Equinox   Epoch      px         Xmeas        Ymeas

                1         18 56 39.426  -63 25 13.23  -0.0002 -0.036  B1950.0  B1950.000  0.000      +44.791      +85.643
                2         19 11 53.909  -63 17 57.57  +0.0058 -0.044  B1950.0  B1950.000  0.000      -46.266      +92.337
                3         19 01 13.606  -63 49 14.84  +0.0020 -0.026  B1950.0  B1950.000  0.000      +17.246      +64.945
                4         19 08 29.088  -63 57 42.79  +0.0016 +0.018  B1950.0  B1950.000  0.000      -25.314      +57.456
                5         19 02 10.088  -63 29 16.73  +0.0012 -0.019  B1950.0  B1950.000  0.000      +11.890      +82.766

1Plate solution: 4-coefficient
 -----------------------------

     X,Y = expected plate coordinates (radians)

     X =  +0.2328072E-03                            Y =  -0.7392285E-03
          -0.3274547E-03 * Xmeas                         -0.5543943E-06 * Xmeas
          -0.5543943E-06 * Ymeas                         +0.3274547E-03 * Ymeas


 Xmeas =  +0.7071360                            Ymeas =   +2.258696    
           -3053.849     * X                              -5.170293     * X
           -5.170293     * Y                              +3053.849     * Y


      Plate scale (in measuring units):           67.5425 arcsec
                           Orientation:           +0.097  deg and laterally inverted


 Reference stars:
                             Mean RA,Dec         Equinox B1950.0      Epoch B1974.500           Residuals (arcsec)
                n                    catalogue                     calculated                 dX        dY        dR

                1            18 56 39.421  -63 25 14.11    18 56 39.468  -63 25 14.27      +0.319    -0.145     0.350
                2            19 11 54.051  -63 17 58.65    19 11 54.082  -63 17 58.00      +0.226    +0.638     0.677
                3            19 01 13.655  -63 49 15.48    19 01 13.580  -63 49 15.88      -0.489    -0.407     0.636
                4            19 08 29.127  -63 57 42.35    19 08 29.016  -63 57 42.72      -0.738    -0.365     0.824
                5            19 02 10.117  -63 29 17.20    19 02 10.220  -63 29 16.92      +0.682    +0.280     0.738

                                                                                  RMS :     0.530     0.401     0.665

1Plate solution: 6-coefficient
 -----------------------------

     X,Y = expected plate coordinates (radians)

     X =  +0.2457761E-03                            Y =  -0.7296778E-03
          -0.3274742E-03 * Xmeas                         -0.5253092E-06 * Xmeas
          -0.7235166E-06 * Ymeas                         +0.3273299E-03 * Ymeas


 Xmeas =  +0.7455928                            Ymeas =   +2.230379    
           -3053.665     * X                              -4.900618     * X
           -6.749697     * Y                              +3055.011     * Y


     Plate scales (in measuring units):      X    67.5465 arcsec
                                             Y    67.5168 arcsec
                                          mean    67.5316 arcsec
                   Nonperpendicularity:           +0.035  deg
                           Orientation:           +0.109  deg and laterally inverted


 Reference stars:
                             Mean RA,Dec         Equinox B1950.0      Epoch B1974.500           Residuals (arcsec)
                n                    catalogue                     calculated                 dX        dY        dR

                1            18 56 39.421  -63 25 14.11    18 56 39.395  -63 25 14.22      -0.174    -0.112     0.207
                2            19 11 54.051  -63 17 58.65    19 11 54.031  -63 17 58.70      -0.134    -0.047     0.142
                3            19 01 13.655  -63 49 15.48    19 01 13.633  -63 49 15.48      -0.149    -0.006     0.149
                4            19 08 29.127  -63 57 42.35    19 08 29.132  -63 57 42.37      +0.034    -0.026     0.043
                5            19 02 10.117  -63 29 17.20    19 02 10.181  -63 29 17.01      +0.422    +0.191     0.463

                                                                                  RMS :     0.224     0.102     0.246






1Unknown stars:    B1950.0 mean places for epoch B1974.500

             :               4-coefficient model               :                6-coefficient model                :
             :   Xmeas    Ymeas          RA            Dec     :   Xmeas    Ymeas          RA             Dec      :     
             :                                                 :                                                   :
             :   -5.103  +58.868 -> 19 05 01.697  -63 56 17.13 :   -5.103  +58.868 -> 19 05 01.7942  -63 56 16.702 :     
             :   -5.120  +58.862 <- 19 05 01.874  -63 56 17.54 :   -5.111  +58.856 <- 19 05 01.8741  -63 56 17.539 :






The residuals dX and dY are, loosely, in standard coordinates; except at the poles, positive dX means that the measured position of the image lies to the east of the expected position, and positive dY means that the measured position lies to the north of the expected position.

If a 7-9 coefficient fit is requested, and providing there are at least ten reference stars, an extra section of report precedes the unknowns. If the fit is successful, the two solutions used to process the unknown stars are the 6 and 7-9 coefficient ones, and the 4-coefficient model is not used.



next up previous 68
Next: Effective Wavelengths
Up: ASTROM Basic astrometry program
Previous: The Input File

ASTROM Basic astrometry program
Starlink User Note 5
P. T. Wallace, Norman Gray
2nd May 2003
E-mail:ussc@star.rl.ac.uk

Copyright © 2003 Council for the Central Laboratory of the Research Councils