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

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

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15.2. OBSERVATION DATA STRUCTURES 169<br />

12. WAVELENGTH START, WAVELENGTH END, WAVE INCREMENT: Applies<br />

to a CVF AOT only. WAVELENGTH START and WAVELENGTH END are the<br />

wavelengths at the beginning and end of a CVF scan. WAVE INCREMENT is the number<br />

of wheel steps between each position in the scan. Type: float (WAVELENGTH START,<br />

WAVELENGTH END) and byte (WAVE INCREMENT). Unit: microns.<br />

13. RA: RA(J2000) of the centre of the final MOSAIC that is constructed from the EXPO-<br />

SUREs in the SCD. Type: double. Unit: decimal degrees.<br />

14. DEC: DEC(J2000) of the centre of the final MOSAIC that is constructed from the EX-<br />

POSUREs in the SCD. Type: double. Unit: decimal degrees.<br />

15. ROLL: As for SCD (see Section 15.2.2).<br />

15.2.4 Science Analysed Data (SAD)<br />

The SAD may contain an EXPOSURE or a MOSAIC. In CIA programming terminology the set<br />

of EXPOSUREs used to create the MOSAIC is referred to as the origin and the actual MOSAIC<br />

itself as the future. This gives rise to two flavours of SAD: origin SAD and future SAD.<br />

Two array substructures exist in the SAD data structure: CCIM and CMAP. (Don’t confuse<br />

these substructures with the data products of the same name, they have been named ‘CCIM’<br />

and ‘CMAP’ for historical reasons.) We use these substructures for:<br />

1. CCIM<br />

Holds an averaged EXPOSURE in detector coordinates. It may be used to hold your CIA<br />

processed data or AAR from the CCIM data product file.<br />

2. CMAP<br />

In the origin SAD it holds an EXPOSURE calibrated in astronomical coordinates. In<br />

the future SAD it holds a MOSAIC. It may be used to hold your CIA processed data or<br />

AAR from the CMAP data product file or the CMOS data product file. Because the size<br />

of the MOSAIC may vary, IDL pointers are used to handle the CMAP data structure.<br />

The routines of Chapter 16 make this transparent to the user, so you need only think of<br />

this structure in terms of fields that you may manipulate. The CMAP substructure is of<br />

dimensions: 32 × 32 for holding an EXPOSURE; dynamic when used to hold a MOSAIC.<br />

The SAD contains all the standard fields of Section 15.2.1 and in addition extra fields associated<br />

with the type of analysis which may have been performed on the data. For example, the<br />

PFOV is a standard field because it is relevant to an image regardless of the processing, but the<br />

unit of pixel intensity, TUNIT, is dependent on how the data has been processed. Below is a<br />

list of fields that are considered most useful to the CIA user.<br />

1. CCIM/CMAP: Both CCIM and CMAP each contain further subfields. To access these<br />

replace DATA with either CCIM or CMAP.

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