next up previous contents index
Next: 6. ISOCAM Calibration Files Up: 5. The Data Products Previous: 5.4 TDF_First_Scan and Derive_ERD

Subsections



5.5 Derive_SPD Products

Derive_SPD performs a number of intermediate tasks on ERD in order to prepare an observation's data for the scientific analysis performed by AAC in the pipeline. In conjunction with the pointing files, SPD is also the recommended starting point for other analysis systems, including CIA, as it contains all the ISOCAM information necessary for most astronomical requirements.


5.5.1 Standard Processed Data: CISP or CPSP

Derive_SPD makes one CISP or CPSP row for every pair of EOI and RESET CIER or CPER records, unless subtraction was already performed on board. The imaging data are accompanied by RESET data, where available; 15 columns of image-description data, such as the various wheel settings; 3 types of image statistics; and the most important temperature, bias-voltage and blackbody housekeeping data. Given the importance of the CAM SPD, the contents of the CISP[1].TABLE are shown in Table 5.5.1.

The CISPDISC discrepancy flags have bits set to show any differences between the record's optical configuration as defined by its instrument settings and the commanded values from the Compact Status that sometimes occur because of the time it takes for the wheels to move. While it is possible to interrogate individual bits, the recommendation to use only data with CISPDISC=0 is followed by the pipeline. Similarly, CISPQFLG=7 shows a record with QLA, OTF and OTFSUM flags all set although the user may choose to ignore the zero$^{th}$ order QLA stabilisation flag during transient modelling.

It is, of course, necessary to use appropriate calibration data during analysis dependent on the instrument configuration which often changes during the course of an observation. These instrument changes are reflected in a set of CISP[1].HEADER keywords including some that were originally designed to give recommendations of which calibration data should be used. However, the proper calibration selection scheme is more complicated than allowed by the CISP[1].HEADER scheme and users should ignore them and follow instead the advices provided in Chapter 6.


Table 5.3: Columns of the CISP[1].TABLE
column type description
GPSCTKEY 1J Instrument time key
GPSCRPID 2B Raster point ID
CISPBOOT 1J Time since processor's boot [CAMTU]
CISPDEID 1B Detector ID (SW:0, LW:1)
CISPCNFG 1B Configuration number within AOT
CISPQFLG 1B CAM's QLA flag: F2_QLA + $2 \times$ OTFLAG + $4\times$ OTFSUM
CISPPROC 1B PROCessing mode 0:Normal, 1:Accumulated, 2:Sampled
CISPDISC 1I CSH/ERD `Discrepancy Flags'
CISPPFOV 1I Lens wheel step number
CISPITIM 1I Elementary integration time (CAMTU)
CISPFCVF 1I Filter wheel step number
CISPWAVE 1E Filter or CVF central wavelength
CISPEWHL 1I Entrance wheel step number
CISPSWHL 1I Selection wheel step number
CISPWDTH 1I Filter/CVF width in millimicrons
CISPOBST 1B Current op-mode 1:OBS, 2:DRK, 3:CAL, 4:CLN, 0:IDLE
CISPCVFS 1B CVF scan on/off (1/0)
CISPTEMP 10E CAM temperatures [K]
CISPBLKB 2E Black body current & voltage
CISPGAIN 1B Electronics gain (0, 1, 2)
CISPOFFS 1B Electronics offset (0...3)
CISPBSFG 1I Beams flag: $256\times$C+R; C:cycle, R:ref#, Add 16 on Ref#
CISPMEAN 1E Frame mean of CISPDATA (this - last)
CISPMEDI 1E Frame median of CISPDATA (this)
CISPSRMS 1E Frame rms of CISPDATA (this - last)
CISPICNT 1I Current internal image counter
CISPACSA 1B ACcumulated/SAmpled image register
CISPAOBS 1B F2_AOT_AOT + $16 \times$ F2_AOT_OBS
CISPBIAS 10E Bias voltages
CISPDATA 1024I Detector data (EOI$-$RESET)
CISPRESE 1122I RESET level for NORMAL processing
CISP3334 64I Columns 33 & 34 of SW readout


next up previous contents index
Next: 6. ISOCAM Calibration Files Up: 5. The Data Products Previous: 5.4 TDF_First_Scan and Derive_ERD
ISO Handbook Volume II (CAM), Version 2.0, SAI/1999-057/Dc