Increasing the imaging capabilities of the VLTI using integrated optics

Pierre Y. Kern; Fabien Malbet; Jean-Philippe Berger; Pierre Haguenauer; Isabelle Schanen-Duport; Pierre Labeye; Karine Perraut-Rousselet; Brahim Arezki; Alain Delboulbé; Laurent Jocou; Christian Perrier-Bellet; Wesley A. Traub; Rafael Millan-Gabet; John D. Monnier; Ettore Pedretti; Andreas Glindemann; Pierre Kervella; Emmanuel di Folco; Philippe B. Gitton

Increasing the imaging capabilities of the VLTI using integrated optics

Pierre Y. Kern
, Fabien Malbet
, Jean-Philippe Berger
, Pierre Haguenauer
, Isabelle Schanen-Duport
, Pierre Labeye
, Karine Perraut-Rousselet
, Brahim Arezki
, Alain Delboulbé
, Laurent Jocou
, Christian Perrier-Bellet
, Wesley A. Traub
, Rafael Millan-Gabet
, John D. Monnier
, Ettore Pedretti
, Andreas Glindemann
, Pierre Kervella
, Emmanuel di Folco
, Philippe B. Gitton

The Scottish Association for Marine Science, Scottish Marine Institute

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ملخص

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

اللغة الأصلية	English
الصفحات (من إلى)	312-320
دورية	Interferometry for Optical Astronomy II
مستوى الصوت	4838
حالة النشر	Published - 1 فبراير 2003

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http://adsabs.harvard.edu/abs/2003SPIE.4838..312K

قم بذكر هذا

Kern, P. Y., Malbet, F., Berger, J.-P., Haguenauer, P., Schanen-Duport, I., Labeye, P., Perraut-Rousselet, K., Arezki, B., Delboulbé, A., Jocou, L., Perrier-Bellet, C., Traub, W. A., Millan-Gabet, R., Monnier, J. D., Pedretti, E., Glindemann, A., Kervella, P., di Folco, E., & Gitton, P. B. (2003). Increasing the imaging capabilities of the VLTI using integrated optics. Interferometry for Optical Astronomy II, 4838, 312-320. http://adsabs.harvard.edu/abs/2003SPIE.4838..312K

@article{7016a61c763f4aa89731ef08fcc26dab,

title = "Increasing the imaging capabilities of the VLTI using integrated optics",

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 ",

author = "Kern, \{Pierre Y.\} and Fabien Malbet and Jean-Philippe Berger and Pierre Haguenauer and Isabelle Schanen-Duport and Pierre Labeye and Karine Perraut-Rousselet and Brahim Arezki and Alain Delboulb{\'e} and Laurent Jocou and Christian Perrier-Bellet and Traub, \{Wesley A.\} and Rafael Millan-Gabet and Monnier, \{John D.\} and Ettore Pedretti and Andreas Glindemann and Pierre Kervella and \{di Folco\}, Emmanuel and Gitton, \{Philippe B.\}",

year = "2003",

month = feb,

day = "1",

language = "English",

volume = "4838",

pages = "312--320",

journal = "Interferometry for Optical Astronomy II",

publisher = "SPIE",

}

Kern, PY, Malbet, F, Berger, J-P, Haguenauer, P, Schanen-Duport, I, Labeye, P, Perraut-Rousselet, K, Arezki, B, Delboulbé, A, Jocou, L, Perrier-Bellet, C, Traub, WA, Millan-Gabet, R, Monnier, JD, Pedretti, E, Glindemann, A, Kervella, P, di Folco, E & Gitton, PB 2003, 'Increasing the imaging capabilities of the VLTI using integrated optics', Interferometry for Optical Astronomy II, المجلد 4838, الصفحات 312-320. <http://adsabs.harvard.edu/abs/2003SPIE.4838..312K>

TY - JOUR

T1 - Increasing the imaging capabilities of the VLTI using integrated optics

AU - Kern, Pierre Y.

AU - Malbet, Fabien

AU - Berger, Jean-Philippe

AU - Haguenauer, Pierre

AU - Schanen-Duport, Isabelle

AU - Labeye, Pierre

AU - Perraut-Rousselet, Karine

AU - Arezki, Brahim

AU - Delboulbé, Alain

AU - Jocou, Laurent

AU - Perrier-Bellet, Christian

AU - Traub, Wesley A.

AU - Millan-Gabet, Rafael

AU - Monnier, John D.

AU - Pedretti, Ettore

AU - Glindemann, Andreas

AU - Kervella, Pierre

AU - di Folco, Emmanuel

AU - Gitton, Philippe B.

PY - 2003/2/1

Y1 - 2003/2/1

N2 - 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

AB - 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

M3 - Article

VL - 4838

SP - 312

EP - 320

JO - Interferometry for Optical Astronomy II

JF - Interferometry for Optical Astronomy II

ER -

Increasing the imaging capabilities of the VLTI using integrated optics

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