Summary
After an introduction summarizing the reasons for developing DWARF, those aspects which in our view distinguish it from other data processing environments are presented. Subjects covered are:
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The rationale for committing ourselves to VAX/VMS.
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The program parameter interface as seen by the user; defaulting mechanisms; generation of multiple functionally distinct versions of a single program.
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Messages, logging and file history.
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The tree-structured data file catalogue.
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Virtual vs programmed I/O.
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Processing of files from different sources with different layouts though one table-driven interface.
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The major benefits of using dynamic core for control arrays.
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© 1985 Plenum Press, New York
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Hamaker, J.P., Harten, R.H., van Diepen, G.N.J., Kombrink, K. (1985). Dwarf: The Dwingeloo-Westerbork Astronomical Reduction Facility. In: Gesù, V.D., Scarsi, L., Crane, P., Friedman, J.H., Levialdi, S. (eds) Data Analysis in Astronomy. Ettore Majorana International Science Series, vol 24. Springer, Boston, MA. https://doi.org/10.1007/978-1-4615-9433-8_40
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DOI: https://doi.org/10.1007/978-1-4615-9433-8_40
Publisher Name: Springer, Boston, MA
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