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| HST Data Handbook for NICMOS | |||||
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Preface
The HST Data Handbook is comprised of three separate sections which are merged together to form a single document:
- Part I is a general introduction which describes the process of retrieving and reducing Hubble Space Telescope (HST) data.
- Part II is an instrument-specific document which describes the reduction procedures, calibrations, and sources of error specific to each active HST instrument.
- Part III is a general set of appendices which includes an IRAF primer, a description of HST file names, and a summary of the observation log files.
Use of HST data necessarily involves using software to retrieve, analyze, and view it. With regard to analysis and visualization, there are many different tools and packages available. It would be impractical for a handbook to show how to do this for all available software. Since much of the software developed by STScI for calibrating, analyzing, and visualizing HST data has been based on the IRAF system, the focus of this handbook will be on use of IRAF, STSDAS, and TABLES for doing so.
Chapter 3 will briefly mention other software tools for accessing HST data and where to get more information about these tools. PyRAF is a new command language (CL) for IRAF and as such, allows use of almost all IRAF tools. It is briefly discussed in Chapter 3, but for the most part, the IRAF examples shown will work exactly the same for PyRAF.
The specifics of the data produced by each of these five active instruments (FGS, WFPC2, STIS, NICMOS, and ACS) are described in separate versions of Part II, while the general information from Parts I and III, referred to as 'the introductory chapters', are tacked onto the beginning and end of each. We recommend a careful reading of the introductory chapters before proceeding to the instrument-specific data handbooks and before starting to work on your HST data.
The present introductory chapters are based on information available as of June 2004. Many changes in the HST Data Archive and HST data reduction software have occurred since the last revision of the Hubble Data Handbook introductory chapters.
Future changes in this handbook are anticipated as the Multimission Archive at STScI (MAST) expands to cover additional missions, and as StarView, PyRAF, and STSDAS software continue to evolve. The reader is advised to consult the STScI web site at
http://www.stsci.edu/hstfor the latest information.
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Space Telescope Science Institute http://www.stsci.edu Voice: (410) 338-1082 help@stsci.edu |