Zobrazeno 1 - 10
of 47
pro vyhledávání: '"Bresson, Yves"'
Autor:
Bresson, Yves1,2 (AUTHOR) ybresson@enit.fr, Tongne, Amèvi1 (AUTHOR), Baili, Maher1 (AUTHOR), Arnaud, Lionel1 (AUTHOR)
Publikováno v:
International Journal of Advanced Manufacturing Technology. Aug2023, Vol. 127 Issue 9/10, p4727-4744. 18p. 3 Color Photographs, 6 Charts, 18 Graphs.
Autor:
Bresson, Yves1,2 (AUTHOR) ybresson@enit.fr, Tongne, Amèvi1 (AUTHOR), Baili, Maher1 (AUTHOR), Arnaud, Lionel1 (AUTHOR)
Publikováno v:
International Journal of Advanced Manufacturing Technology. Jul2023, Vol. 127 Issue 5/6, p2687-2706. 20p. 10 Color Photographs, 3 Black and White Photographs, 6 Diagrams, 3 Charts.
Autor:
Petrov, Romain G., Boskri, Abdelkarim, Bresson, Yves, Agabi, Karim, Folcher, Jean-Pierre, Elhalkouj, Thami, Lagarde, Stephane, Benkhaldoun, Zouhair
Publikováno v:
Proc. SPIE 9907, Optical and Infrared Interferometry and Imaging V, 99071F (August 4, 2016)
The full scientific potential of the VLTI with its second generation instruments MATISSE and GRAVITY require fringe tracking up to magnitudes K>14 with the UTs and K>10 with the ATs. The GRAVITY fringe tracker (FT) will be limited to K~10.5 with UTs
Externí odkaz:
http://arxiv.org/abs/1610.08287
Autor:
Petrov, Romain G., Elhalkouj, Thami, Boskri, Abdelkarim, Folcher, Jean-Pierre, Lagarde, Stephane, Bresson, Yves, Benkhaldoum, Zouhair, Lazrek, Mohamed, Rakshit, Suvendu
Publikováno v:
Proc. SPIE 9146, Optical and Infrared Interferometry IV, 91462P (July 24, 2014)
The limiting magnitude is a key issue for optical interferometry. Pairwise fringe trackers based on the integrated optics concepts used for example in GRAVITY seem limited to about K=10.5 with the 8m Unit Telescopes of the VLTI, and there is a genera
Externí odkaz:
http://arxiv.org/abs/1410.4822
Autor:
Millour, Florentin, Petrov, Romain, Lagarde, Stéphane, Berio, Philippe, Bresson, Yves, Abe, Lyu
Pupil-remapping is a new high-dynamic range imaging technique that has recently demonstrated feasibility on sky. The current prototypes present however deceiving limiting magnitude, restricting the current use to the brightest stars in the sky. We pr
Externí odkaz:
http://arxiv.org/abs/1403.4207
Autor:
Robbe-Dubois, Sylvie, Bresson, Yves, Aristidi, Eric, Lagarde, Stephane, Antonelli, Pierre, Lopez, Bruno, Petrov, Romain G.
While doing optical study in an instrument similar to the interferometers dedicated to the Very Large Telescope (VLT), we have to take care of the pupil and focus conjugations. Modules with artificial sources are designed to simulate the stellar beam
Externí odkaz:
http://arxiv.org/abs/1008.4218
Autor:
Robbe-Dubois, Sylvie, Lagarde, Stephane, Bresson, Yves, Petrov, Romain G., Carbillet, Marcel, Lecoarer, Etienne, Rantakyrö, Frederik, Tallon-Bosc, Isabelle, Vannier, Martin, Antonelli, Pierre, Martinot-Lagarde, Gregoire, Roussel, Alain, Tasso, Daniel
This paper presents a study of the atmospheric refraction and its effect on the light coupling efficiency in an instrument using single-mode optical fibers. We show the analytical approach which allowed us to assess the need to correct the refraction
Externí odkaz:
http://arxiv.org/abs/0902.2158
Autor:
Bresson, Yves1,2 (AUTHOR) yves.bresson@enit.fr, Tongne, Amèvi1 (AUTHOR), Selva, Pierre1 (AUTHOR), Arnaud, Lionel1 (AUTHOR)
Publikováno v:
International Journal of Advanced Manufacturing Technology. Apr2022, Vol. 119 Issue 9/10, p5727-5742. 16p.
Autor:
Bresson, Yves
Th.--Chir. dent.--Clermont-Ferrand 1, 1978. N°: 33.
Externí odkaz:
http://catalogue.bnf.fr/ark:/12148/cb36078746t
Autor:
Petrov, Romain, Boskri, Abdelkarim, Allouche, Fatme, Agabi, Karim, Bailet, Christophe, Benkhaldoun, Zouhair, Berio, Philippe, Bresson, Yves, Dejonghe, Julien, Elhalkouj, Thami, Folcher, Jean-Pierre, Lagarde, Stéphane, Lopez, Bruno, Matter, Alexis, Meilland, Anthony, Mourard, Denis, Rakshit, Suvendu
Publikováno v:
The Very Large Telescope in 2030
The Very Large Telescope in 2030, Jun 2019, Garching, Germany. ⟨10.5281/zenodo.3356288⟩
The Very Large Telescope in 2030, Jun 2019, Garching, Germany. ⟨10.5281/zenodo.3356288⟩
International audience; The VLTI has a huge potential for the study of Active Galactic Nuclei. It allows to resolve the BLR by phase differential interferometry and to make images of the inner dust « torus ». The first generation VLTI instruments A
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::e39b3a2a48ccb89fb8f768400d752c55
https://hal.archives-ouvertes.fr/hal-03058931
https://hal.archives-ouvertes.fr/hal-03058931