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The EPICS project: Exoplanets detection with OWL
by
Baudoz, P.
, Chalabaev, A.
, Rahoui, F.
, Mouillet, D.
, Turatto, M.
, Dohlen, K.
, Le Coarer, E.
, Thalmann, C.
, Yaitskova, N.
, Kuntschner, H.
, Boccaletti, A.
, Gratton, R.
, Kerber, F.
, Tinbergen, J.
, Hubin, N.
, Le Louarn, M.
, Gandorfer, A.
, Lenzen, R.
, Navarro, R.
, Antichi, J.
, Rabou, P.
, Stam, D.
, Fedrigo, E.
, Schmid, H.M.
, Verinaud, C.
, Longmore, A.
, Selsis, F.
, Kasper, M.
, Fusco, T.
, Paillet, J.
, Soummer, R.
, Beuzit, J.-L.
, Feldt, M.
, Da Silva, C. Correia
in
Astronomy
/ Contributed Papers
2005
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The EPICS project: Exoplanets detection with OWL
by
Baudoz, P.
, Chalabaev, A.
, Rahoui, F.
, Mouillet, D.
, Turatto, M.
, Dohlen, K.
, Le Coarer, E.
, Thalmann, C.
, Yaitskova, N.
, Kuntschner, H.
, Boccaletti, A.
, Gratton, R.
, Kerber, F.
, Tinbergen, J.
, Hubin, N.
, Le Louarn, M.
, Gandorfer, A.
, Lenzen, R.
, Navarro, R.
, Antichi, J.
, Rabou, P.
, Stam, D.
, Fedrigo, E.
, Schmid, H.M.
, Verinaud, C.
, Longmore, A.
, Selsis, F.
, Kasper, M.
, Fusco, T.
, Paillet, J.
, Soummer, R.
, Beuzit, J.-L.
, Feldt, M.
, Da Silva, C. Correia
in
Astronomy
/ Contributed Papers
2005
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Do you wish to request the book?
The EPICS project: Exoplanets detection with OWL
by
Baudoz, P.
, Chalabaev, A.
, Rahoui, F.
, Mouillet, D.
, Turatto, M.
, Dohlen, K.
, Le Coarer, E.
, Thalmann, C.
, Yaitskova, N.
, Kuntschner, H.
, Boccaletti, A.
, Gratton, R.
, Kerber, F.
, Tinbergen, J.
, Hubin, N.
, Le Louarn, M.
, Gandorfer, A.
, Lenzen, R.
, Navarro, R.
, Antichi, J.
, Rabou, P.
, Stam, D.
, Fedrigo, E.
, Schmid, H.M.
, Verinaud, C.
, Longmore, A.
, Selsis, F.
, Kasper, M.
, Fusco, T.
, Paillet, J.
, Soummer, R.
, Beuzit, J.-L.
, Feldt, M.
, Da Silva, C. Correia
in
Astronomy
/ Contributed Papers
2005
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Journal Article
The EPICS project: Exoplanets detection with OWL
2005
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Overview
This paper presents the status of the EPICS project, an Earth-like Planets Imaging Camera Spectrograph for OWL. We present the Top-Level-Requirements of the instrument and we describe the baseline of the Adaptive Optics system with optimized wave-front sensor. The expected performance in rejection of starlight in the near infrared and in the visible is given. The instruments concepts for detection and characterization of exo-planets will be briefly described. The Signal-to-Noise ratio estimation shows that Earth-like planets can be detected up to 20 pc in a reasonable amount of time. The extremely challenging requirements in terms of static residual errors and differential aberrations are discussed.
Publisher
Cambridge University Press
Subject
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