# AMBER, the near-infrared spectro-interferometric three-telescope VLTI instrument

@article{Petrov2007AMBERTN,
title={AMBER, the near-infrared spectro-interferometric three-telescope VLTI instrument},
author={Romain G. Petrov and Fabien Malbet and G. Weigelt and Pierre Antonelli and Udo Beckmann and Yves Bresson and Alain E. Chelli and Michel Dugu{\'e} and G. Duvert and Sandro Gennari and L. Gl{\"u}ck and Pierre Y. Kern and St'ephane Lagarde and Etienne Le Coarer and Franco Lisi and Florentin A. Millour and K. Perraut and Pascal Puget and Fredrik T. Rantakyr{\"o} and Sylvie Robbe-Dubois and Alain Roussel and Piero Salinari and Eric Tatulli and G{\'e}rard Zins and Matteo Accardo and Bram Acke and Karim Agabi and Evelyne Altariba and Brahim Arezki and Eric Aristidi and Carlo Baffa and Jack Behrend and Thomas Bl{\"o}cker and Serge Bonhomme and Simone Busoni and Fr'ed'eric Cassaing and J. M. Clausse and Jacques Colin and Claus Connot and Alain Delboulb{\'e} and A. Domiciano de Souza and Thomas Driebe and Philippe Feautrier and Debora Ferruzzi and Thierry Forveille and Eric G. Fossat and Renaud Foy and Didier Fraix-Burnet and A. Gallardo and E. Giani and Carla S. Gil and Andre Glentzlin and M. Heiden and Matthias Heininger and Oscar Hern{\'a}ndez Utrera and K. H. Hofmann and D. Kamm and Mario J. Kiekebusch and Stefan Kraus and D. Le Contel and J. M. Le Contel and T. Lesourd and Bruno Lopez and Morgan Lopez and Yves Magnard and Alessandro Marconi and G. A. de Mars and Gr{\'e}goire Martinot‐Lagarde and Ph. Mathias and Pierre Mege and J. L. Monin and David Mouillet and Denis Mourard and Eddy Nussbaum and Keiichi Ohnaka and Jos{\'e} Pacheco and Christian Perrier and Yves Rabbia and Sylvestre Rebattu and François Reynaud and A Richichi and A. Robini and Michel Sacchettini and Dieter Schertl and M. Sch{\"o}ller and Walter Solscheid and Alain Spang and P. Stee and Paolo Stefanini and Michel Tallon and I. Tallon-Bosc and D. Tasso and Leonardo Testi and Farrokh Vakili and Oskar von der L{\"u}he and J. C. Valtier and Martin Vannier and No{\"e}l Ventura},
journal={Astronomy and Astrophysics},
year={2007},
volume={464},
pages={1-12}
}
Context: Optical long-baseline interferometry is moving a crucial step forward with the advent of general-user scientific instruments that equip large aperture and hectometric baseline facilities, such as the Very Large Telescope Interferometer (VLTI). Aims: AMBER is one of the VLTI instruments that combines up to three beams with low, moderate and high spectral resolutions in order to provide milli-arcsecond spatial resolution for compact astrophysical sources in the near-infrared wavelength… Expand
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#### References

SHOWING 1-10 OF 48 REFERENCES
Near-Infrared interferometry of Eta Carinae with high spatial and spectral resolution using the VLTI and the AMBER instrument
• Physics
• 2006
We present the first NIR spectro-interferometry of the LBV Eta Carinae. The K band observations were performed with the AMBER instrument of the ESO Very Large Telescope Interferometer using threeExpand
MIDI – the 10 μm instrument on the VLTI
After more than five years of preparation, the mid-infrared interferometric instrument MIDI has been transported to Paranal where it will undergo testing and commissioning on theVery Large TelescopeExpand
The Palomar Testbed Interferometer
• Physics
• 1999
The Palomar Testbed Interferometer (PTI) is a long-baseline infrared interferometer located at Palomar Observatory, California. It was built as a testbed for interferometric techniques applicable toExpand
First scientific results from the VLT interferometer
The VLT interferometer has been operating since the time of first fringes in March 2001 with a pair of 40 cm diameter siderostats at baselines of 16 and 66 m and a pair of 8 m diameter telescopesExpand
Probing the close environment of young stellar objects with interferometry
The study of Young Stellar Objects (YSOs) is one of the most exciting topics that can be undertaken by long baseline optical interferometry. The magnitudes of these objects are at the edge ofExpand
Star separator system for the dual-field capability (PRIMA) of the VLTI
In the framework of the Phase-Referenced Imaging and Micro-arcsecond Astrometry facility (PRIMA) developed for the Very Large Telescope Interferometer (VLTI), a sophisticated opto-mechanical systemExpand
Near-infrared interferometry of eta Carinae with spectral resolutions of 1 500 and 12 000 using AMBER/VLTI
Aims. We present the first NIR spectro-interferometry of the LBV ? Carinae. The observations were performed with the AMBER instrument of the ESO Very Large Telescope Interferometer (VLTI) usingExpand
VLTI/VINCI observations of the nucleus of NGC 1068 using the adaptive optics system MACAO
• Physics
• 2004
We present the first near-infrared K -band long-baseline interferometric measurement of the nucleus of the prototype Seyfert 2 Galaxy NGC 1068 with resolution $\lambda/B \sim$ 10 mas obtained withExpand
VLTI technical advances: present and future
The Very Large Telescope Interferometer (VLTI) on Cerro Paranal (2635 m) in Northern Chile reached a major milestone in September 2003 when the mid infrared instrument MIDI was offered for scientificExpand
Interferometric data reduction with AMBER/VLTI. Principle, estimators, and illustration.
• Physics
• 2007
Aims. In this paper, we present an innovative data reduction method for single-mode interferometry. It has been specifically developed for the AMBER instrument, the three-beam combiner of the VeryExpand