Zobrazeno 1 - 10
of 177
pro vyhledávání: '"M. Carbillet"'
Autor:
R. Pourcelot, E. H. Por, M. N’Diaye, H. Benard, G. Brady, L. Canas, M. Carbillet, K. Dohlen, I. Laginja, J. Lugten, J. Noss, M. D. Perrin, P. Petrone, L. Pueyo, S. F. Redmond, A. Sahoo, A. Vigan, S. D. Will, R. Soummer
Context. Wavefront sensing and control (WFSC) will play a key role in improving the stability of future large segmented space telescopes while relaxing the thermo-mechanical constraints on the observatory structure. Coupled with a coronagraph to reje
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::728cf23b2312600ce2f04879a69a9864
http://arxiv.org/abs/2301.03242
http://arxiv.org/abs/2301.03242
Autor:
R. Pourcelot, M. N’Diaye, E. H. Por, I. Laginja, M. Carbillet, H. Benard, G. Brady, L. Canas, K. Dohlen, J. Fowler, O. Lai, M. Maclay, E. McChesney, J. Noss, M. D. Perrin, P. Petrone, L. Pueyo, S. F. Redmond, A. Sahoo, A. Vigan, S. D. Will, R. Soummer
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2022, 663, pp.A49. ⟨10.1051/0004-6361/202243145⟩
Astronomy and Astrophysics-A&A, 2022, 663, pp.A49. ⟨10.1051/0004-6361/202243145⟩
Context.The combination of large segmented space telescopes, coronagraphy, and wavefront control methods is a promising solution for producing a dark hole (DH) region in the coronagraphic image of an observed star in order to study planetary companio
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8c00dbd45da480958756a1d7ae961055
https://hal-insu.archives-ouvertes.fr/insu-03780768
https://hal-insu.archives-ouvertes.fr/insu-03780768
Akademický článek
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Publikováno v:
Publications of the Astronomical Society of the Pacific. 134:074501
We analyze, in the framework of high angular resolution imaging, a novel image reconstruction method denoted as PSE (which stands for power spectrum extended). It works in the Fourier space, combining the information from both the average power spect
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::47b5e658f353bbf2d01f048f4d020a41
https://doi.org/10.1088/1538-3873/ac6699
https://doi.org/10.1088/1538-3873/ac6699
Akademický článek
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Akademický článek
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Autor:
M. Carbillet
Publikováno v:
EAS Publications Series. 59:59-76
This course/paper deals with adaptive optics in the frame- work of astronomical imaging. It does not pretend to be an exhaustive course of astronomical adaptive optics. It is rather intended to give an introductory overview of it, from my very partia
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::63a953a5a72a385a62f0917c153a7618
https://doi.org/10.1051/eas/1359004
https://doi.org/10.1051/eas/1359004
Autor:
A. Vigan, C. Moutou, M. Langlois, F. Allard, A. Boccaletti, M. Carbillet, D. Mouillet, I. Smith
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 407:71-82
The direct detection of exoplanets has been the subject of intensive research in the recent years. Data obtained with future high-contrast imaging instruments optimized for giant planets direct detection are strongly limited by the speckle noise. Spe
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::686e2a31b289a555efce4f9398a5616e
https://doi.org/10.1111/j.1365-2966.2010.16916.x
https://doi.org/10.1111/j.1365-2966.2010.16916.x
Publikováno v:
2006, France
In this paper we give a survey of the methods we have developed for multiple image deconvolution, with application to the reconstruction of the images of the Large Binocular Telescope (LBT). We first describe the main features of LBT and of the Fizea
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e334b1107e23d98c9a0f59b5f56d3815
https://doi.org/10.1051/eas:2006124
https://doi.org/10.1051/eas:2006124
Autor:
M. Carbillet
Publikováno v:
EAS Publications Series. 12:137-156
Due to its capacity in retrieving the angular resolution of ground-based optical telescopes together with their intrinsic sensitivity, adaptive optics (AO) is well known to be of fundamental importance for a wide range of astronomical applications. I
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::893b18f594aaacebdf7bd0268b36a4df
https://doi.org/10.1051/eas:2004028
https://doi.org/10.1051/eas:2004028