The HFI DPC
The HFI DPC has been organized into different "Levels": 1, 2, 3, 4 and "S". In brief, during operations, L1 feeds the database resulting in time-ordered information (TOI) objects. L2 is the core of the processing, which turns TOIs into clean calibrated sky maps. L3 transforms these maps at specific frequencies into more scientific products, like catalogues, maps and spectra of astrophysical components. L3 can rely on simulation provided by the LS, while L4 refers to delivering the DPC products to ESA.
(L1): consists in receiving the telemetry and ancillary data files and ingesting them into the DPC database. This involves decompressing, in some cases changing data formats, computing the time of individual data samples from the time of the compression slices, but otherwise no processing proper. Other steps are:
- data ingestion (science, HK, ancillary, other?)
- construction of ToS in science data group
- pointing interpolation
- construction of other TOI and ROI objects from AHF, ...
This is further described in the Pre-processing section
(L2): this is where the data are processed from timelines into maps. The main processing steps are
- Timeline (or Time-Ordered Information = TOI) processing, which includes conversion from ADUs to engineering units (Volts), demodulation, deglitching, conversion from engineering to physical units (Watts), removal of known systematic effects (non-linearities, 4K lines, Jumps, ring flagging), removal of the instrumental signature (time transfer function), temporal noise Estimation. See section TOI_processing.
- Pointing and beam of each detector. See section Pointing&Beams.
- map-making & photomoetric calibration: projecting the TOIs onto all-sky maps, etc. See section Map-making.
- Characterisation/validation through angular power spectra. See section PowerSpectra.
- Overal HFI data validation, through difference tests, comparison to detailed simulations, etc., See section HFI-Validation
- The resulting data characteristics are given in section Summary
(L3): This is where the data in the form of frequency maps are converted to catalogues and astrophysical component maps. Much of this is done in common with the LFI, and is further described in the HFI/LFI common sections
Level 4 is the "Archive Level". No processing done, but rather exporting, reformating, documenting.
Level S is the so-called "Simulation Level", common to both instruments, and further described in the HFI/LFI common section. HFI specific developments are described in the HFI data validation section.
(Planck) High Frequency Instrument
Data Processing Center
European Space Agency
Time of Sample
Ring-Ordered Information (DMC group/object)
Attitude History File
EMI/EMC influence of the 4K cooler mechanical motion on the bolometer readout electronics.
(Planck) Low Frequency Instrument