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NICMOS Data Products

Standard NICMOS Dataset Structure

NICMOS data are represented by five arrays for each readout. These arrays contain the:

Figure 13.4: Data Format for ACCUM, RAMP, BRIGHTOBJ and ACQ Modes

Science Image

The science image contains the information recorded by the NICMOS camera. The data may be represented as counts (i.e., data numbers) or as count rates (i.e., data numbers per second). Generally the latter is desirable since it is easier to interpret in mosaiced datasets and corresponds closely to flux.

Error Array

The error array contains an estimate of the statistics error at each pixel. It is expressed as a real number of standard deviations. This is a calculated quantity based on a model of the instrument and its environment.

Quality Flags Array

The quality flags array provides 16 independent flags for each pixel. Each flag has a true (set) or false (unset) state and is encoded as a bit in a 16 bit (short integer) word. Users are advised that this word should not be interpreted as an integer.

Samples Array

The samples array is used for one of two purposes:

Integration Time Array

The integration time array contains the total integration time at each pixel. While initially a simple parameter in some observing modes, combining datasets into composite mosaics and using the information obtained by multiple non-destructive readouts during an integration requires us to keep track of the actual exposure time for each pixel. This array is useful for simple conversions between counts and count rates.

The MULTIACCUM mode (Figure 13.5) produces multiple images. The file structure for such a dataset consists of a lattice of the 5 image arrays which are created for each readout, as shown in Figure 13.5.

Figure 13.5: MULTIACCUM Data Format

IRAF Access

Backwards Compatibility

This data structure will be implemented so that the default array is the most meaningful science image array. For example, if you request IRAF to display a dataset, the first science image array would be displayed. Access to the other arrays within a dataset will be via element numbers (1-5; mod 5 for datasets containing multiple readouts) or via a standardized naming convention (see Figure 13.4 and Figure 13.5). It is a critical requirement that existing IRAF tasks be able to access any array in a NICMOS dataset.

FITS File Format

The physical format of NICMOS datasets will be FITS with image extensions. Data will both be delivered to observers and used within IRAF and STSDAS in this format. A modified version of the IRAF kernel has been developed at STScI to support this data format directly. This permits the use of NICMOS data without conversion (i.e., the strfits task is not necessary). This will be distributed with the STSDAS system before Cycle 7.



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