Planck 2015 results
We present an updated description of the Planck Low Frequency Instrument (LFI) data processing pipeline, associated with the 2015 data release. We point out the places where our results and methods have remained unchanged since the 2013 paper and we highlight the changes made for the 2015 release, d...
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Published in | Astronomy and astrophysics (Berlin) Vol. 594 |
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Main Authors | , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , |
Format | Journal Article |
Language | English |
Published |
EDP Sciences
2016
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Subjects | |
Online Access | Get full text |
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Summary: | We present an updated description of the Planck Low Frequency Instrument (LFI) data processing pipeline, associated with the 2015 data release. We point out the places where our results and methods have remained unchanged since the 2013 paper and we highlight the changes made for the 2015 release, describing the products (especially timelines) and the ways in which they were obtained. We demonstrate that the pipeline is self-consistent (principally based on simulations) and report all null tests. For the first time, we present LFI maps in Stokes Q and U polarization. We refer to other related papers where more detailed descriptions of the LFI data processing pipeline may be found if needed. |
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Bibliography: | bibcode:2016A%26A...594A...2P publisher-ID:aa25818-15 dkey:10.1051/0004-6361/201525818 istex:CD306DFB67F900E994628A30BD1761B2BB08D1EC ark:/67375/80W-FDRVZ6JW-1 |
ISSN: | 0004-6361 1432-0746 |
DOI: | 10.1051/0004-6361/201525818 |