2008
DOI: 10.3917/res.147.0149
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La « sécurité routière », un programme sans risque

Abstract: Distribution électronique Cairn.info pour Lavoisier. © Lavoisier. Tous droits réservés pour tous pays.La reproduction ou représentation de cet article, notamment par photocopie, n'est autorisée que dans les limites des conditions générales d'utilisation du site ou, le cas échéant, des conditions générales de la licence souscrite par votre établissement. Toute autre reproduction ou représentation, en tout ou partie, sous quelque forme et de quelque manière que ce soit, est interdite sauf accord préalable et écr… Show more

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Cited by 8 publications
(7 citation statements)
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“…Images of the θ Orionis C astrometric field were acquired with an identical setup on September, 24 2010. They were properly reduced with the Eclipse software (Devillard 1997). The position of the stars on the detector were compared to their position on sky measured by McCaughrean & Stauffer (1994) to derive the instrument orientation to the North of −0.36 ± 0.11 • and a detector plate scale of 27.13 ± 0.09 mas.…”
Section: Data Reductionmentioning
confidence: 99%
“…Images of the θ Orionis C astrometric field were acquired with an identical setup on September, 24 2010. They were properly reduced with the Eclipse software (Devillard 1997). The position of the stars on the detector were compared to their position on sky measured by McCaughrean & Stauffer (1994) to derive the instrument orientation to the North of −0.36 ± 0.11 • and a detector plate scale of 27.13 ± 0.09 mas.…”
Section: Data Reductionmentioning
confidence: 99%
“…Therefore, we analyzed publicly available data of Θ Orionis C obtained with the same setup as our K s -band data on 2012 November 16 UT. 15 Data were reduced using the ESO Eclipse software (Devillard 1997) using a method similar to that described in Bonnefoy et al (2009). The reduction included standard corrections for bias, sky, and bad pixels and also frame re-centering and averaging.…”
Section: Vlt-nacomentioning
confidence: 99%
“…Optical and NIR data were reduced following standard procedures with the tools of the ESO-ECLIPSE package (Devillard 1997). Polarimetric data were reduced again following standard procedures as discussed in Covino et al (1999Covino et al ( , 2002Covino et al ( , 2003.…”
Section: Vltmentioning
confidence: 99%