Zobrazeno 1 - 10
of 61
pro vyhledávání: '"Martin Vannier"'
Publikováno v:
Astronomical Telescopes + Instrumentation Conference on Optical and Infrared Interferometry and Imaging {V} ({ATI'16})
Astronomical Telescopes + Instrumentation Conference on Optical and Infrared Interferometry and Imaging, 2016, Edimburgh, United Kingdom. ⟨10.1117/12.2233010⟩
Astronomical Telescopes + Instrumentation Conference on Optical and Infrared Interferometry and Imaging {V} ({ATI'16}), 2016, Edimburgh, United Kingdom. ⟨10.1117/12.2233010⟩
Astronomical Telescopes + Instrumentation Conference on Optical and Infrared Interferometry and Imaging, 2016, Edimburgh, United Kingdom. ⟨10.1117/12.2233010⟩
Astronomical Telescopes + Instrumentation Conference on Optical and Infrared Interferometry and Imaging {V} ({ATI'16}), 2016, Edimburgh, United Kingdom. ⟨10.1117/12.2233010⟩
International audience; This paper presents an extension of the spatio-spectral (" 3D ") image reconstruction algorithm called PAINTER (Polychromatic opticAl INTErferometric Reconstruction software). The algorithm is able to solve large scale problem
Autor:
Martin Vannier, John Young, Guillaume Mella, Gilles Duvert, Paulo J. V. Garcia, Eric Thiébaut
Publikováno v:
Scopus-Elsevier
OPTICON currently supports a Joint Research Activity (JRA) dedicated to providing easy to use image reconstruction algorithms for optical/IR interferometric data. This JRA aims to provide state-of-the-art image reconstruction methods with a common in
Autor:
Dieter Schertl, Gerd Weigelt, A. Ferrari, David Mary, Florentin Millour, M. Heininger, Martin Vannier, Eric Thiébaut, Antony Schutz, Karl-Heinz Hofmann, John Young, J. Sanchez-Bermudez
Publikováno v:
SPIE Proceedings.
Image reconstruction in optical interferometry has gained considerable importance for astrophysical studies during the last decade. This has been mainly due to improvements in the imaging capabilities of existing interferometers and the expectation o
An overview of the mid-infrared spectro-interferometer MATISSE: science, concept, and current status
Autor:
Paul Jolley, M. Heininger, Martin Vannier, Marco Delbo, Y. Fantei, Udo Beckmann, Thomas Henning, Tibor Agócs, Farrokh Vakili, Stephane Lagarde, Eric Pantin, G. Martinot-Lagarde, C. Connot, Walter Jaffe, P. Antonelli, Pierre Cruzalèbes, R. Brast, Pierre Haguenauer, E. Nussbaum, Klaus Meisenheimer, L. Labadie, S. Morel, Karl-Heinz Hofmann, Bruno Lopez, Andreas Glindemann, G. Kroes, Werner Laun, M. Schuil, William C. Danchi, Sebastian Wolf, Paul Bristow, C. Bailet, Ch. Lucuix, F. Allouche, Dieter Schertl, A. van Duin, Eszter Pozna, Ralf Conzelmann, M. Lehmitz, Gert Finger, M. Mellein, Florentin Millour, Jean-Charles Augereau, Romain Petrov, Isabelle Percheron, Ralf Palsa, F. Martinache, Derek Ives, Eddy Elswijk, Gero Rupprecht, Ralph Hofferbert, N. Mauclert, S. Kiraly, Markus Schoeller, G. Csepany, A. Marcotto, Yves Bresson, C. Schmidt, Leander Mehrgan, Udo Neumann, T. Lanz, Pierre Bourget, Alain Spang, Michiel R. Hogerheijde, Ronald Roelfsema, S. Ottogalli, Carsten Dominik, Jean-Michel Clausse, M. de Haan, A. Gabasch, Felix Bettonvil, Josef Hron, Johana Panduro, Uwe Graser, J. Isderda, H. Hanenburg, Alexis Matter, Lars Venema, Christian A. Hummel, Sylvie Robbe-Dubois, A. Jasko, Anthony Meilland, Frédéric Gonté, R. van Boekel, Serge Menardi, Ph. Berio, Karl Wagner, J.-L. Lizon, Julien Woillez, Jean-Phillipe Berger, J. Kragt, Jörg-Uwe Pott, Serge Guniat, J. Behrend, R. ter Horst, G. Avila, Antoine Mérand, G. van Belle, F. Guitton, T. Phan Duc, N. Tromp, S. Kuindersma, J. Stegmeier, Gerd Jakob, Gerd Weigelt, T. Kroener, Christoph Leinert
Publikováno v:
NASA Astrophysics Data System
MATISSE is the second-generation mid-infrared spectrograph and imager for the Very Large Telescope Interferometer (VLTI) at Paranal. This new interferometric instrument will allow significant advances by opening new avenues in various fundamental res
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1a5e7c06f6e56172562ecd8df15df8e8
Publikováno v:
EAS Publications Series. 28:95-103
We present high spatial resolution observations of the mid-infrared core of the dusty symbiotic system HM Sge. The MIDI interferometer was used with the VLT Unit Telescopes and Auxiliary Telescopes providing baselines oriented from PA=42° to 105°.
Autor:
C. Martayan, Fabien Malbet, Martin Vannier, Francesco Paresce, Alain Spang, Florentin Millour, Andrea Richichi, Philippe Stee, Romain Petrov, Anthony Meilland, A. Domiciano de Souza
Publikováno v:
Astronomy & Astrophysics. 464:59-71
Aims. We aim to study the geometry and kinematics of the disk around the Be star α Arae as a function of wavelength, especially across the Brγ emission line. The main purpose of this paper is to understand the nature of the disk rotation around Be
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2006, 367, pp.825-837
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2006, 367, pp.825-837. ⟨10.1111/j.1365-2966.2006.10015.x⟩
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2006, 367, pp.825-837
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2006, 367, pp.825-837. ⟨10.1111/j.1365-2966.2006.10015.x⟩
International audience; We present the high angular resolution technique of colour-differential interferometry for direct detection of extrasolar giant planets (EGPs). The measurement of differential phase with long-baseline ground-based interferomet
Publikováno v:
EAS Publications Series. 8:171-180
The color-differential astrometry method consists in measuring the variations of the photocenter position with wavelength. This yields spectral information on the spatial structure of an unresolved source, and could allow, among other applications, t
Publikováno v:
EAS Publications Series. 8:297-309
This paper describes our strategy and presents the specific additional calibration tool added to the near-infrared focal instrument AMBER of the Very Large Telescope Interferometer, to achieve the direct detection of extrasolar planets with color-dif
Autor:
S. Bonhomme, Marco Delbo, Andrea Richichi, J.-U. Pott, Martin Vannier, Paul Jolley, M. Heininger, Farrokh Vakili, Johana Panduro, Gero Rupprecht, S. Ottogalli, Jean-Philippe Berger, P. Antonelli, J. L. Lizon, A. Jaskó, William C. Danchi, Francoise Delplancke, Jan Kragt, G. Martinot-Lagarde, Eric Pantin, Lucas Labadie, Isabelle Percheron, Dieter Schertl, Felix Bettonvil, Udo Neumann, Frank Przygodda, M. Lehmitz, Th. Henning, Jean-Charles Augereau, Michiel R. Hogerheijde, Yves Bresson, E. Nussbaum, Uwe Graser, Gert Finger, Werner Laun, Gerd Weigelt, T. Lanz, Y. Fantei, F. Martinache, L. Thiam, A. Crida, Tibor Agócs, C. Connot, Niels Tromp, Florentin Millour, Leander Mehrgan, Karl-Heinz Hofmann, R. Brast, Eszter Pozna, Sebastien Morel, J. Hron, F. Rigal, Stephane Lagarde, Sebastian Wolf, Walter Jaffe, Philippe B. Gitton, Ramón Navarro, Ch. Leinert, A. Glazenborg, Carsten Dominik, M. Mellein, L. Mosoni, Gabby Kroes, Pierre Haguenauer, A. Gabasch, C. Bailet, Pierre Bourget, J. C. Gonzalez, Jean-Michel Clausse, M. de Haan, Andreas Glindemann, G. Csepany, Paul Bristow, Eddy Elswijk, G. T. van Belle, Y. Hughes, Ch. Lucuix, Romain Petrov, N. Mauclert, Ralf Palsa, V. Girault, Roy von Boekel, A. Marcotto, Markus Schöller, D. Ives, H. Hanenburg, Alexis Matter, Olivier Chesneau, J. L. Menut, M. Dugué, F. Guitton, Anthony Meilland, Lars Venema, Sylvie Robbe-Dubois, G. Avila, Frédéric Gonté, U. Beckman, Serge Menardi, Klaus Meisenheimer, Ph. Berio, Karl Wagner, Julien Woillez, Rainer Köhler, Serge Guniat, J. Behrend, R. ter Horst, T. Kroener, Gerd Jakob, P. Girard, T. Phan Duc, J. Stegmeier, Bruno Lopez
Publikováno v:
SPIE Proceedings.
MATISSE is the mid-infrared spectrograph and imager for the Very Large Telescope Interferometer (VLTI) at Paranal. This second generation interferometry instrument will open new avenues in the exploration of our Universe. Mid-infrared interferometry