Difference between revisions of "HFI design, qualification, and performance"
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== Cold optics == | == Cold optics == | ||
<span style="color:red">(Lamarre)</span> | <span style="color:red">(Lamarre)</span> | ||
− | === Horns,lenses | + | === Horns,lenses=== |
− | === filters, band | + | links to Peter's paper |
+ | === filters, band=== | ||
+ | Includes Locke's very detailed document. | ||
== Detection chain == | == Detection chain == |
Revision as of 13:16, 15 October 2012
The inversion of HFI data requires that one knows how the instrument selects photons, how these photons are transformed in data transmitted by telemetry and what spurious signals are added in this process.
Contents
HFI high level description and Architecture[edit]
(Lamarre/Pajot) Should be short, understandable and point through links to the relevant sections and papers.
Cryogenics[edit]
(F .Pajot)
Dilution[edit]
including PIDs
4K[edit]
including PIDs for details links to the early cryogenic paper (need to add data ?)
Cold optics[edit]
(Lamarre)
Horns,lenses[edit]
links to Peter's paper
filters, band[edit]
Includes Locke's very detailed document.
Detection chain[edit]
(Francesco Piacentini)
Bolometers[edit]
JFETs[edit]
Readout[edit]
Data compression[edit]
Time response.[edit]
Links to Brendan's paper. Additional data if needed. Written by Brendan.
System (Ken)[edit]
List of systematics[edit]
Summary[edit]
(Lamarre) here remind worse sytematics and point to DPC Summary of sucess and limitations. JML. Link to early HFI in flight perf.
(Planck) High Frequency Instrument
Data Processing Center