ISOCAM Interactive Analysis User's Manual Version 5.0 - ISO - ESA

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34 CHAPTER 4. STARING OBSERVATION (CAM01) 9. As in the end of Section 3.2 you can save the data using IDL’s SAVE. CIA> save, file=’staring_pds.xdr’, staring_pds AndexporttoaFITSfilewithCIA’simagette2fits. This routine will place the data in the PDS field .IMAGE into the primary array of the FITS file. CIA> imagette2fits, staring_pds, name=’staring.fits’ Additionally you can correct the staring EXPOSUREs in .IMAGE for distortion (see Section 20.15.5).
Chapter 5 Solar System Object observation (CAM01) 5.1 Description of the observation The data used here is from a CAM solar system object observation of the comet Tempel-Tuttle. This observation is comprised of four CONFIGURATIONs. These four CONFIGURATIONs together make up the entire observation or AOT. Each CONFIGURATION has roughly the same duration of 180 seconds. In order to keep the object in ISOCAM’s FOV, multiple (5 − 6) re-pointings of ISO had to be made during each CONFIGURATION. To accommodate this repointing of the satellite, solar system observations are implemented as a one-dimensional raster, with the first raster-point identification (M RASTER) being incremented for each re-pointing. 5.2 Data analysis It is assumed in this section that you have read Chapter 3. Generally concepts described in that section will not be re-described here. 1. Start your CIA session # cia 2. Convert your CISP data into SCDs with spdtoscd CIA> spdtoscd, ’cisp81200202.fits’, sscd, dir=’$cia_vers/test’, /nowrite During the slicing, CIA will print the following warning: pixel [14,17] is affected by saturation at SCD 3 with the average value 4093.00 (value for End-of-Integration, 3 readouts) This indicates that pixel [14,17] was saturated, and its photometry has to be carefully assessed. 3. Get an overview of the SCDs: 35
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ISOCAM Interactive Analysis User’
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Page 16 and 17: xvi LIST OF FIGURES 14.13The raster
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Page 22 and 23: 2 CHAPTER 1. ABOUT THE CIA USER’S
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Page 41: Introduction The Quick Start Guide
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96 CHAPTER 13. DATA CALIBRATION 13.
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Introduction The purpose of this pa
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Chapter 15 CIA data structure high-
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15.2. OBSERVATION DATA STRUCTURES 1
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15.5. PREPARED DATA STRUCTURE (PDS)
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Chapter 16 Data structure manipulat
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16.1. CIA DATA STRUCTURE INTERFACE
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16.1. CIA DATA STRUCTURE INTERFACE
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16.2. AN EXAMPLE OF SAD MANIPULATIO
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16.4. MANIPULATING THE MASK 195 and
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16.5. CDS DATA EXTRACTION 197 16.5
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16.6. MANIPULATING CIA DATA STRUCTU
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Chapter 17 Importing ISO data produ
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17.2. IMPORTING FITS TO REGULAR IDL
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Chapter 18 Export of CIA data struc
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18.3. EXPORT FOR ARCHIVING 207 CIA>
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Part IV Advanced Use of CIA 209
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214 CHAPTER 19. ADVANCED SLICING 19
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274 CHAPTER 21. USING SLICE WITHIN
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294 CHAPTER 22. SECOND ORDER CORREC
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298 CHAPTER 23. X CIA REFERENCE GUI
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306 APPENDIX A. GLOSSARY beam-switc
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308 APPENDIX A. GLOSSARY FITS (data
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310 APPENDIX A. GLOSSARY raster dat
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312 APPENDIX A. GLOSSARY
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314 APPENDIX B. CIA COMMAND SHORT-L
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320 APPENDIX C. THE ISO CD-ROM C.2.
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322 APPENDIX C. THE ISO CD-ROM Vari
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324 APPENDIX D. GUIDELINES FOR WRIT
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326 APPENDIX D. GUIDELINES FOR WRIT
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328 APPENDIX E. ISOCAM ASTROMETRY:
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338 APPENDIX F. WHAT IS NEW IN CIA
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344 APPENDIX G. WARNING MESSAGES IN
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346 APPENDIX H. PATCHED ASTROLIB AN
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348 APPENDIX I. UPGRADING OLD CIA S
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350 APPENDIX I. UPGRADING OLD CIA S
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352 APPENDIX J. REPORTING PROBLEMS
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354 APPENDIX K. TECHNICAL REPORTS S
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356 BIBLIOGRAPHY Okumura K., 1998,
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