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pro vyhledávání: '"ANALYSE DONNEE"'
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
