EPJ Web of Conferences
Volume 101, 2015The Space Photometry Revolution – CoRoT Symposium 3, Kepler KASC-7 Joint Meeting
|Number of page(s)||2|
|Section||Session 6 – Posters|
|Published online||23 September 2015|
CoRoT data: final pipe-line for bright stars
1 LESIA, Observatoire de Paris, CNRS (UMR 8109), Meudon France
2 Institut d’Astrophysique Spatiale, Universitè Paris Sud, CNRS (UMR 8617), Orsay France
Published online: 23 September 2015
The observations made by the CoRoT satellite were divided into short and long periods called runs; for a detailed description of the runs see . The global processing pipeline is divided in two sub-pipelines: the first one is dedicated to the corrections that can be applied to simultaneous data, while the second one needs the whole duration of each run to be applied. We present here the final form of the entire processing pipeline for the bright stars channel, which was previously called the seismo channel.
© Owned by the authors, published by EDP Sciences, 2015
This is an Open Access article distributed under the terms of the Creative Commons Attribution License 4.0, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
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