Zobrazeno 1 - 10
of 403
pro vyhledávání: '"M, N'diaye"'
Autor:
K. Wagner, A. Boehle, P. Pathak, M. Kasper, R. Arsenault, G. Jakob, U. Käufl, S. Leveratto, A.-L. Maire, E. Pantin, R. Siebenmorgen, G. Zins, O. Absil, N. Ageorges, D. Apai, A. Carlotti, É. Choquet, C. Delacroix, K. Dohlen, P. Duhoux, P. Forsberg, E. Fuenteseca, S. Gutruf, O. Guyon, E. Huby, D. Kampf, M. Karlsson, P. Kervella, J.-P. Kirchbauer, P. Klupar, J. Kolb, D. Mawet, M. N’Diaye, G. Orban de Xivry, S. P. Quanz, A. Reutlinger, G. Ruane, M. Riquelme, C. Soenke, M. Sterzik, A. Vigan, T. de Zeeuw
Publikováno v:
Nature Communications, Vol 12, Iss 1, Pp 1-7 (2021)
Imaging of low-mass exoplanets can be achieved once the thermal background in the mid-infrared (MIR) wavelengths can be mitigated. Here, the authors present a ground-based MIR observing approach enabling imaging low-mass temperate exoplanets around n
Externí odkaz:
https://doaj.org/article/34b7ac7a6b0c49a6be4c1b54f6499593
Autor:
K. Wagner, A. Boehle, P. Pathak, M. Kasper, R. Arsenault, G. Jakob, U. Käufl, S. Leveratto, A.-L. Maire, E. Pantin, R. Siebenmorgen, G. Zins, O. Absil, N. Ageorges, D. Apai, A. Carlotti, É. Choquet, C. Delacroix, K. Dohlen, P. Duhoux, P. Forsberg, E. Fuenteseca, S. Gutruf, O. Guyon, E. Huby, D. Kampf, M. Karlsson, P. Kervella, J.-P. Kirchbauer, P. Klupar, J. Kolb, D. Mawet, M. N’Diaye, G. Orban de Xivry, S. P. Quanz, A. Reutlinger, G. Ruane, M. Riquelme, C. Soenke, M. Sterzik, A. Vigan, T. de Zeeuw
Publikováno v:
Nature Communications, Vol 12, Iss 1, Pp 1-1 (2021)
Externí odkaz:
https://doaj.org/article/329fa377055a44578bed32083379eef6
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:
N. Cvetojevic, F. Martinache, P. Chingaipe, R. Laugier, K. Ławniczuk, R. G. Broeke, R. Ligi, M. N'Diaye, D. Mary
Publikováno v:
Astronomy & Astrophysics.
Publikováno v:
EMC - Tratado de Medicina. 25:1-6
Resumen El dolor facial asociado a la masticacion es un motivo frecuente de consulta en odontologia, en medicina general y en cirugia oral y maxilofacial. El acto de comer es una funcion constituida por varias acciones, comenzando por la toma de los
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
Publikováno v:
2022 Intermountain Engineering, Technology and Computing (IETC).
Akademický článek
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Publikováno v:
Lebensmittelchemie. 75
Autor:
A. Vigan, K. Dohlen, M. N’Diaye, F. Cantalloube, J. H. Girard, J. Milli, J.-F. Sauvage, Z. Wahhaj, G. Zins, J.-L. Beuzit, A. Caillat, A. Costille, J. Le Merrer, D. Mouillet, S. Tourenq
Publikováno v:
Astronomy and Astrophysics
Coronagraphic imaging of exoplanets using ground-based instruments on large telescopes is intrinsically limited by speckles induced by uncorrected aberrations. These aberrations originate from the imperfect correction of the atmosphere by an extreme