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- {{DISPLAYTITLE:LFI design, qualification and performance}} ...ription of the LFI instrument is given in {{PlanckPapers|bersanelli2010}}, and references therein.3 KB (487 words) - 17:09, 4 February 2015
- |+ '''Spectral transmission for CO transitions for HFI detectors''' [[Category:HFI design, qualification and performance|011]]4 KB (313 words) - 08:11, 10 December 2014
- ...ning the relative spectral response functions for the Planck HFI detectors and frequency bands. <small>Reference bolometer spectra and S/N.</small>2 KB (227 words) - 07:48, 10 December 2014
- ...also calculated using the Planck function. The ratio of the received power and the theoretical power provides the optical efficiency term. To remove any o ...). The spectral transmission is scaled for λ<sup>2</sup> throughput and then re-normalized as follows:4 KB (636 words) - 07:36, 10 December 2014
- This is a list of all annexes for the HFI instrument section. ** [[HFI_optical_efficiency|HFI spectral response optical efficiency measurements]];812 bytes (97 words) - 06:52, 10 December 2014
- ##[[Ground Segment and Operations|Ground Segment and Operations]] ##[[HFI design, qualification, and performance|HFI design, qualification, and performance]]5 KB (581 words) - 09:33, 31 March 2014
- The Planck spacecraft was designed, built and tested around two major modules. ...adiative insulation between the warm service module and the cold telescope and instruments.14 KB (2,136 words) - 09:37, 3 February 2015
- ##[[HFI design, qualification, and performance|HFI design, qualification, and performance]] ###[[HFI_performance_summary | Performance summary]]6 KB (744 words) - 09:45, 31 March 2014
- The heart of the HFI - the detectors - are bolometers, solid-state devices in which the channels at central frequencies of 100, 143, 217, 353, 545, and 857 GHz.13 KB (2,128 words) - 15:29, 4 June 2014