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Proceedings Paper

Increasing the imaging capabilities of the VLTI using integrated optics
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Paper Abstract

Several scientific topics linked to the observation of extended structures around astrophysical sources (dust torus around AGN, disks around young stars, envelopes around AGBs) require imaging capability with milli-arcsecond spatial resolution. The current VLTI instruments, AMBER and MIDI, will provide in the coming months the required high angular resolution, yet without actual imaging. As a rule of thumb, the image quality accessible with an optical interferometer is directly related to the number of telescopes used simultaneously: the more the apertures, the better and the faster the reconstruction of the image. We propose an instrument concept to achieve interferometric combination of N telescopes (4 ≤ N ≤ 8) thanks to planar optics technology: 4 x 8-m telescopes in the short term and/or 8 x 1.8-m telescopes in the long term. The foreseen image reconstruction quality in the visible and/or in the near infrared will be equivalent to the one achieved with millimeter radio interferometers. Achievable spatial resolution will be better than the one foreseen with ALMA. This instrument would be able to acquire routinely 1 mas resolution images. A 13 to 20 magnitude sensitivity in spectral ranges from 0.6 to 2.5 μm is expected depending on the choice of the phase referencing guide source. High dynamic range, even on faint objects, is achievable thanks to the high accuracy provided by integrated optics for visibility amplitude and phase measurements. Based on recent validations of integrated optics presented here an imaging instrument concept can be proposed. The results obtained using the VLTI facilities give a demonstration of the potential of the proposed technique.

Paper Details

Date Published: 21 February 2003
PDF: 9 pages
Proc. SPIE 4838, Interferometry for Optical Astronomy II, (21 February 2003); doi: 10.1117/12.459074
Show Author Affiliations
Pierre Y. Kern, Lab. d'Astrophysique de l'Observatoire de Grenoble (France)
Fabien Malbet, Lab. d'Astrophysique de l'Observatoire de Grenoble (France)
Jean-Philippe Berger, Lab. d'Astrophysique de l'observatoire de Grenoble (France)
Pierre Haguenauer, IMEP/INPG (France)
Isabelle Schanen-Duport, IMEP/INPG (France)
Pierre Labeye, CEA-LETI (France)
Karine Perraut-Rousselet, Lab. d'Astrophysique de l'Observatoire de Grenoble (France)
Brahim Arezki, Lab. d'Astrophysique de l'Observatoire de Grenoble (France)
Alain Delboulbe, Lab. d'Astrophysique de l'Observatoire de Grenoble (France)
Laurent Jocou, Lab. d'Astrophysique de l'Observatoire de Grenoble (France)
Christian Perrier-Bellet, Lab. d'Astrophysique de l'Observatoire de Grenoble (France)
Wesley A. Traub, Harvard-Smithsonian Ctr. for Astrophysics (United States)
Rafael Millan-Gabet, Harvard-Smithsonian Ctr. for Astrophysics (United States)
John D. Monnier, Harvard-Smithsonian Ctr. for Astrophysics (United States)
Ettore Pedretti, Harvard-Smithsonian Ctr. for Astrophysics (United States)
Andreas Glindemann, European Southern Observatory (Germany)
Pierre Kervella, European Southern Observatory (Germany)
Emmanuel di Folco, European Southern Observatory (Germany)
Philippe B. Gitton, European Southern Observatory (Germany)


Published in SPIE Proceedings Vol. 4838:
Interferometry for Optical Astronomy II
Wesley A. Traub, Editor(s)

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