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  2. Christopher Adam Tout - Research Interests

    https://people.ast.cam.ac.uk/~cat/res.html
    1 Jul 1999: This algorithm can be used to look at the statistics of stellar distributions and was applied to the Bright Star Catalogue to test our theory of stellar evolution and to constrain
  3. The Electronics

    https://people.ast.cam.ac.uk/~mike/casu/pds/pdselec.html
    18 Aug 1999: Tests showed that the PID algorithm was prone to instabilities and that better performance was obtained using the original tachos to provide the velocity rather than the "Integral" part of the
  4. Model Calculations of Sky Brightness

    https://people.ast.cam.ac.uk/~rgm/vista/site/pachon_sky/page3.html
    9 Jul 1999: The model calculates V magnitude light output at zenith. Since the street light are all Sodium and there are virtually no Mercury lamps, the V band is a good test case.
  5. WFC - Known Problems

    https://people.ast.cam.ac.uk/~mike/casu/WFCsur/foibles.html
    14 Mar 1999: Linearity tests using sequences of dome flats revealed CCD#2 and CCD#4 to have significant non-linearities over the whole dynamic range.
  6. Night Sky Brightness at Cerro Pachon

    https://people.ast.cam.ac.uk/~rgm/vista/site/pachon_sky/
    12 Jul 1999: The model calculates V magnitude light output at zenith. Since the street light are all Sodium and there are virtually no Mercury lamps, the V band is a good test case.
  7. WFS Pipeline Processing

    https://people.ast.cam.ac.uk/~mike/casu/WFCsur/pipeline.html
    4 Jun 1999: Non-linearity correction. linearity tests using sequences of dome flats revealed CCD#2 and CCD#4 to have significant non-linearities over the whole dynamic range.
  8. WFC - Filters & library fringe frames

    https://people.ast.cam.ac.uk/~mike/casu/WFCsur/defringing.html
    13 Dec 1999: A series of tests on R-band data taken since October 1998 indicates that the fringe pattern is sufficiently stable that the above October fringe frames can be used to successfully

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