Planck 2015 results
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Table 17

List of known instrumental systematic effects in Planck-LFI.

Effect Source Control/removal

Effects independent of sky signal (T and P)
White noise correlation Phase switch imbalance Diode weighting
1/f noise RF amplifiers Pseudo-correlation and destriping
Bias fluctuations RF amplifiers, back-end electronics Pseudo-correlation and destriping
Thermal fluctuations 4-K, 20-K and 300-K thermal stages Calibration, destriping
1-Hz spikes Back-end electronics Template fitting and removal
Effects dependent on the sky signal (T and P)
Main beam ellipticity Main beams Accounted for in window function
Near sidelobe Optical response at angles Masking of Galaxy and point
pickup <5° from the main beam sources
Far sidelobe pickup Main and sub-reflector spillover Model sidelobes removed from timelines
Analogue-to-digital Back-end analogue-to-digital Template fitting and removal
converter non-linearity converter
Imperfect photometric Sidelobe pickup, radiometer noise Adaptive smoothing algorithm using 4π
calibration temperature changes and other beam, 4-K reference load voltage output
non-idealities temperature sensor data
Pointing Uncertainties in pointing reconstru- Negligible impact on anisotropy
ction, thermal changes affecting measurements
focal plane geometry
Effects specifically impacting polarization
Bandpass asymmetries Differential orthomode transducer Spurious polarization removal
and receiver bandpass response
Polarization angle Uncertainty in the polarization Negligible impact
uncertainty angle in-flight measurement
Orthomode transducer Imperfect polarization separation Negligible impact
cross-polarization

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