CoRoT data: final pipe-line for faint stars

CoRoT data: final pipe-line for faint stars

The observations made by the CoRoT satellite were divided into short and long periods called runs; for a detailed description of the runs see [1]. 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, w...

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Main Authors: Deru A., Chaintreuil S., Baudin F., Ferrigno A., Baglin A.
Format: Article
Language:English
Published: EDP Sciences 2015-01-01
Series:EPJ Web of Conferences
Online Access:http://dx.doi.org/10.1051/epjconf/201510106023
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spelling doaj-ef3c1c8ec59244ea83256db65d1735032021-08-02T02:09:19ZengEDP SciencesEPJ Web of Conferences2100-014X2015-01-011010602310.1051/epjconf/201510106023epjconf_sphr2014_06023CoRoT data: final pipe-line for faint starsDeru A.0Chaintreuil S.1Baudin F.2Ferrigno A.3Baglin A.4LESIA, Observatoire de Paris, CNRS (UMR 8109)LESIA, Observatoire de Paris, CNRS (UMR 8109)Institut d’Astrophysique Spatiale, Universitè Paris Sud, CNRS (UMR 8617)LESIA, Observatoire de Paris, CNRS (UMR 8109)LESIA, Observatoire de Paris, CNRS (UMR 8109)The observations made by the CoRoT satellite were divided into short and long periods called runs; for a detailed description of the runs see [1]. 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 faint stars channel, which was previously called the exo channel.http://dx.doi.org/10.1051/epjconf/201510106023
collection DOAJ
language English
format Article
sources DOAJ
author Deru A.
Chaintreuil S.
Baudin F.
Ferrigno A.
Baglin A.
spellingShingle Deru A.
Chaintreuil S.
Baudin F.
Ferrigno A.
Baglin A.
CoRoT data: final pipe-line for faint stars
EPJ Web of Conferences
author_facet Deru A.
Chaintreuil S.
Baudin F.
Ferrigno A.
Baglin A.
author_sort Deru A.
title CoRoT data: final pipe-line for faint stars
title_short CoRoT data: final pipe-line for faint stars
title_full CoRoT data: final pipe-line for faint stars
title_fullStr CoRoT data: final pipe-line for faint stars
title_full_unstemmed CoRoT data: final pipe-line for faint stars
title_sort corot data: final pipe-line for faint stars
publisher EDP Sciences
series EPJ Web of Conferences
issn 2100-014X
publishDate 2015-01-01
description The observations made by the CoRoT satellite were divided into short and long periods called runs; for a detailed description of the runs see [1]. 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 faint stars channel, which was previously called the exo channel.
url http://dx.doi.org/10.1051/epjconf/201510106023
work_keys_str_mv AT derua corotdatafinalpipelineforfaintstars
AT chaintreuils corotdatafinalpipelineforfaintstars
AT baudinf corotdatafinalpipelineforfaintstars
AT ferrignoa corotdatafinalpipelineforfaintstars
AT baglina corotdatafinalpipelineforfaintstars
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