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|
PLATO: PSF modelling using a micro-scanning technique
1 Stellar Astrophysics Centre (SAC), Aarhus University, Ny Munkegade 120 Aarhus C, Denmark,
2 Seaview Sensing, Sheffield, South Yorkshire S1 2NS - United Kingdom
3 LESIA, Observatoire de Paris, 5 place Jules Janssen 92195 Meudon cedex, France
a e-mail: firstname.lastname@example.org
Published online: 23 September 2015
The PLATO space mission is designed to detect telluric planets in the habitable zone of solar type stars, and simultaneously characterise the host star using ultra high precision photometry. The photometry will be performed on board using weighted masks. However, to reach the required precision, corrections will have to be performed by the ground segment and will rely on precise knowledge of the instrument PSF (Point Spread Function). We here propose to model the PSF using a microscanning method.
© 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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