… 1.5 m aperture class to ensure the desired resolution with an adequate rejection of straylight
contamination (Mandolesi et al… The two detectors in radiometer R0 are named (M-00, M-01), …

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 …

… as measured on the ground are included in Bersanelli et al. (2010), Mennella et al. (… systematic
effects of thermal or electrical origin (Bersanelli et al. 2010). The main sources of potential …

… We focus first on (Ω m ,σ 8 ), assuming that n s follows a Gaussian prior centred on the
best-fit Planck CMB value 4 (n s = 0.9603 � 0.0073). We combine our SZ counts likelihood with …

The scientific performance of the Planck Low Frequency Instrument (LFI) after one year of in-orbit
operation is presented. We describe the main optical parameters and discuss …

… For all four of our estimators, we find that this normalization factor is within 0.5% of that given
by N xβ ν f ∥ ,sky , as is already apparent from the triangles along the horizontal axis of Fig. …

We present the scaling relation between Sunyaev-Zeldovich (SZ) signal and stellar mass for
almost 260,000 locally brightest galaxies (LBGs) selected from the Sloan Digital Sky Survey …

We present a system-level description of the Low Frequency Instrument (LFI) considered as
a differencing polarimeter, and evaluate its expected performance. The LFI is one of the two …

We describe the processing of data from the Low Frequency Instrument (LFI) used in
production of the Planck Early Release Compact Source Catalogue (ERCSC). In particular, we …

We present the current accounting of systematic effect uncertainties for the Low Frequency
Instrument (LFI) that are relevant to the 2015 release of the Planck cosmological results, …