Planck pre-launch status: the Planck-LFI programme
N. Mandolesi, M. Bersanelli, R.C. Butler, E. Artal, C. Baccigalupi, A., Balbi, A.J. Banday, R.B. Barreiro, M. Bartelmann, K. Bennett, P. Bhandari, A., Bonaldi, J. Borrill, M. Bremer, C. Burigana, R.C. Bowman, P. Cabella, C., Cantalupo, B. Cappellini, T. Courvoisier, G. Crone

TL;DR
This paper reviews the development, testing, and expected performance of the Planck-LFI instrument, designed to produce high-precision microwave sky maps for cosmology and astrophysics, prior to its launch.
Contribution
It provides a comprehensive overview of the LFI instrument's design, testing, calibration, and data processing strategies within the Planck mission, highlighting its readiness for scientific operations.
Findings
Instrument performance tests demonstrate excellent functionality.
Data processing pipeline verified for accuracy.
Calibration and verification phases scheduled post-launch.
Abstract
This paper provides an overview of the Low Frequency Instrument (LFI) programme within the ESA Planck mission. The LFI instrument has been developed to produce high precision maps of the microwave sky at frequencies in the range 27-77 GHz, below the peak of the cosmic microwave background (CMB) radiation spectrum. The scientific goals are described, ranging from fundamental cosmology to Galactic and extragalactic astrophysics. The instrument design and development are outlined, together with the model philosophy and testing strategy. The instrument is presented in the context of the Planck mission. The LFI approach to ground and inflight calibration is described. We also describe the LFI ground segment. We present the results of a number of tests demonstrating the capability of the LFI data processing centre (DPC) to properly reduce and analyse LFI flight data, from telemetry…
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