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

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92 CHAPTER 12. DATA SLICING title description displayed? staring SC SCD Number always St. starting readout of the SCD always La. last readout of the SCD always N. maximum number of images that can be built always Ent. Whl entrance wheel position if selected Sel. Whl. selection wheel position if selected LW Lns. LW lens wheel position if selected LW Flt. LW filter wheel position if selected SW Lns. SW lens wheel position if selected SW Flt. SW filter wheel position if selected Ch channel (which detector is on) if selected Beam Switching Beam Switching if selected A.O.T AOT variable if selected Ob. T. observation type if selected Off. detector offset if selected Integ. Ti integration time if selected G. detector gain if selected Obs. observation mode if selected OTF on target flag if selected R.M raster mode if selected M R.P M raster position if selected N R.P N raster position if selected S. N. sequence number if selected P. M. parallel mode flag if selected Table 12.1: Conversion table for the variable names displayed by x handle slice.
12.3. DATA SLICING WITH X SLICER 93 • Print the slicer display: will print the big table in a text file. The name of this file will be the official name of the observation, with the .prn extension. For example: 1380302.prn. • Save Slicer File: save the work done under a form re-usable by the slicer (see Handling big datasets in the Advanced Slicing section). • Quit: Quit x slicer. • Back to last Choice: will redisplay the state of the slicing operation before you hit the button ‘Redisplay’. • Back to First Choice: will redisplay the first screen that appeared just after the slicing proposal was computed. • Back to Main Window: will go back to the x slicer window. WARNING: you will lose all the slicing work that has been done, unless it has been saved. The Advanced Slicing pull-down menu contains the list of all lens, filters, gains and integration times used in your data, plus a Number of exposures menu. 12.3.6 Selecting SCDs and SSCDs Let us now begin the real slicing work. Looking at the big board where the proposition of slicing has been displayed, you will soon notice that there are many SCDs that you will not need, especially in the beginning of observations and between two filters or PFOV when more than a configuration was programmed in a single AOT. You now have to select which SCDs you want to create and in which SSCD you want to put them. Let’s examine together a concrete example: Figure 12.2 displays the x handle slice for an observation of a cluster. This observation consists of two 4x4 rasters made with the 3 arcsec PFOV lens, one with the LW2 filter, the other with the LW3 filter. Of course, we are going to make two different SSCDs with these ERD, one for the LW2 filter, the other for the LW3 filter. Let’s begin with the LW2 raster: • First click on the ‘Unselect All SCDs’ button. All the ‘toggle’ buttons on the ‘Make your Choice’ column are now unselected, and the ‘Merge’ buttons are insensitive. • Select the ‘lwfil 2’ item in the Advanced Slicing/Filters menu. All LW2 SCDs are now selected. • Click on the ‘Redisplay’ button. You are back in the same situation as before making any choices, but the x handle slice window displays only data obtained with LW2 filter. A way to select the frames of our LW2 observation is to use the number of exposures: all the lens and filters motions take only a few frames, but (in this case), at least 30 frames have been taken per raster position. Here it goes again: • First click on the ‘Unselect All SCDs’ button.
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ISOCAM Interactive Analysis User’
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Michael Rupen (NRAO) Jaqui Sam Lone
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vi CONTENTS 8 Polarization observat
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viii CONTENTS 14.4.6 x3d as a calib
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x CONTENTS 19.3 A beam-switch obser
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xii CONTENTS B CIA command short-li
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xiv CONTENTS
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xvi LIST OF FIGURES 14.13The raster
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xviii LIST OF FIGURES
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xx LIST OF TABLES
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2 CHAPTER 1. ABOUT THE CIA USER’S
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4 CHAPTER 2. ABOUT CIA 2.2 System r
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6 CHAPTER 2. ABOUT CIA Figure 2.2:
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8 CHAPTER 2. ABOUT CIA In addition,
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10 CHAPTER 2. ABOUT CIA 2.3.4 Custo
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12 CHAPTER 2. ABOUT CIA LOG Log fil
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14 CHAPTER 2. ABOUT CIA This will p
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16 CHAPTER 2. ABOUT CIA % device, p
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18 CHAPTER 2. ABOUT CIA
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Introduction The Quick Start Guide
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24 CHAPTER 3. RASTER OBSERVATION (C
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32 CHAPTER 4. STARING OBSERVATION (
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34 CHAPTER 4. STARING OBSERVATION (
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36 CHAPTER 5. SOLAR SYSTEM OBJECT O
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Page 79: Introduction The purpose of Part II
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142 CHAPTER 14. IMAGE ANALYSIS AND
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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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15.3. CALIBRATION DATA STRUCTURE (C
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15.4. AUXILIARY CALIBRATION DATA 17
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15.4. AUXILIARY CALIBRATION DATA 17
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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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212
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214 CHAPTER 19. ADVANCED SLICING 19
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216 CHAPTER 19. ADVANCED SLICING Fi
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226 CHAPTER 19. ADVANCED SLICING va
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228 CHAPTER 19. ADVANCED SLICING Fo
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230 CHAPTER 19. ADVANCED SLICING
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232 CHAPTER 20. ADVANCED DATA CALIB
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274 CHAPTER 21. USING SLICE WITHIN
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294 CHAPTER 22. SECOND ORDER CORREC
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296 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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