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Planck 2015 results. V. LFI calibration

Author(s)
Planck Collaboration
Ade, P. A. R.
Aghanim, N.
Natoli, Paolo  
Polenta, Gianluca  
Subjects

Astrophysics - Instru...

Astrophysics - Cosmol...

16 figures

part of the Planck 20...

Date Issued
2015-05-01
Mission(s)
Planck  
Abstract
We present a description of the pipeline used to calibrate the Planck Low Frequency Instrument (LFI) timelines into thermodynamic temperatures for the Planck 2015 data release, covering 4 years of uninterrupted operations. As in the 2013 data release, our calibrator is provided by the spin-synchronous modulation of the CMB dipole, exploiting both the orbital and solar components. Our 2015 LFI analysis provides an independent Solar dipole estimate in excellent agreement with that of HFI and within $1sigma$ (0.3 % in amplitude) of the WMAP value. This 0.3 % shift in the peak-to-peak dipole temperature from WMAP and a global overhaul of the iterative calibration code increases the overall level of the LFI maps by 0.45 % (30 GHz), 0.64 % (44 GHz), and 0.82 % (70 GHz) in temperature with respect to the 2013 Planck data release, thus reducing the discrepancy with the power spectrum measured by WMAP. We estimate that the LFI calibration uncertainty is at the level of 0.20 % for the 70 GHz map, 0.26 % for the 44 GHz map, and 0.35 % for the 30 GHz map. We provide a detailed description of the impact of all the changes implemented in the calibration since the previous data release.
URI
https://hdl.handle.net/20.500.13025/4413
URL
http://adsabs.harvard.edu/abs/2015arXiv150508022P
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