Skip to main content

Introducing the Near Infrared VLTI Instrument AMBER to Its Users

  • Chapter
  • 149 Accesses

Abstract

AMBER is the General User near infrared focal instrument of the Very Large Telescope Interferometer. It is a single mode, dispersed fringes, three telescope instrument. A limiting magnitude of the order of H=13 will allow tackling of a fair sample of extra galactic targets. A very high accuracy, in particular in color differential phase and closure phase modes gives good hope for very high dynamical range observations, possibly including hot extra solar planets. The relatively high maximum spectral resolution, up to 10000, will allow stellar activity observations. Between these extreme goals, AMBER has a wide range of applications including Young Stellar Objects, Evolved Stars, circumstellar material and many others.

This is a preview of subscription content, log in via an institution.

Buying options

Chapter
USD   29.95
Price excludes VAT (USA)
  • Available as PDF
  • Read on any device
  • Instant download
  • Own it forever
eBook
USD   129.00
Price excludes VAT (USA)
  • Available as PDF
  • Read on any device
  • Instant download
  • Own it forever
Softcover Book
USD   169.99
Price excludes VAT (USA)
  • Compact, lightweight edition
  • Dispatched in 3 to 5 business days
  • Free shipping worldwide - see info
Hardcover Book
USD   169.99
Price excludes VAT (USA)
  • Durable hardcover edition
  • Dispatched in 3 to 5 business days
  • Free shipping worldwide - see info

Tax calculation will be finalised at checkout

Purchases are for personal use only

Learn about institutional subscriptions

Preview

Unable to display preview. Download preview PDF.

Unable to display preview. Download preview PDF.

References

  • Chelli, A., Tatulli, E., Malbet, F. et al.: 2002, AMBER data processing, SPIE conference 4838 Interferometry for Optical Astronomy II, Waikoloa, Hawaii, USA, 2002, in publication.

    Google Scholar 

  • Gai, M., Bonino, D., Corcione, L. et al.: 2001, in: J. Bergeron and G. Monnet (eds.), FINITO: A Fringe Sensor for the VLTI in Two and Three Beam Configuration,ESO symposia Scientific drivers for ESO future VLT/VLTI instrumentation, pp. 328–330.

    Google Scholar 

  • Glindemann, A., Ballester, P., Bauvir B. et al.: 2002, Very large telescope interferometer: a status report, SPIE conference 4838 Interferometry for Optical Astronomy II, Waikoloa, Hawaii, USA, 2002, in publication.

    Google Scholar 

  • Malbet, F., Bloecker, T., Foy, R. et al.: 2002, Astrophysical potential of the AMBER/VLTI instrument, SPIE conference 4838 Interferometry for Optical Astronomy II, Waikoloa, Hawaii, USA, 2002, in publication.

    Google Scholar 

  • Malbet, F., Petrov, R.G., Tallon-Bosc, I. et al.: 2002, System analysis of the AMBER instrument on VLTI, SPIE conference 4838 Interferometry for Optical Astronomy II, Waikoloa, Hawaii, USA, 2002, in publication.

    Google Scholar 

  • Marconi, A., Maiolino, R. and Petrov, R.G.: 2002, Extragalactic astronomy with the VLTI: a new window on the universe, Proceedings of JENAM 2002 Conference, Porto, Portugal, September 2002 (these proceedings).

    Google Scholar 

  • Petrov, R.G.: 1989, Differential interferometry, in: D. Alloin and J.M. Mariotti (eds.), Diffraction Limited Imaging with Very Large Telescopes, NATO ASI Series C, 274, Kluwer. Ac., pp. 249, 272.

    Google Scholar 

  • Petrov, R.G., Malbet, F., Weigelt, G. et al.: 2002, Using the near infrared VLTI instrument AMBER, SPIE conference 4838 Interferometry for Optical Astronomy Il, Waikoloa, Hawaii, USA, 2002, in publication.

    Google Scholar 

  • Petrov, R.G., Vannier, M., Lopez, B., Bresson, Y., Robbe-Dubois, S. and Lagarde, S.: 2002, Orbits and spectra of extra solar planets with the VLTI focal instrument AMBER, in: G. Aime and R. Soumer (eds.), Proceedings of the Workshop on Very High Dynamics Imagery and Extra Solar Planets, Nice, France, May 2002. EDP Science Series.

    Google Scholar 

  • Robbe-Dubois, S., Antonelli, P., Bresson, Y. et al.: 2002, VLTI focal instrument AMBER: results of the laboratory commissioning of the warm optics, SPIE conference 4838 Interferometry for Optical Astronomy I I, Waikoloa, Hawaii, USA.

    Google Scholar 

  • Segransan, D. et al.: 2001, How AMBER will contribute to the search of brown dwarfs and extrasolar planets, SPIE proceedings 4006, Munich, March 2000, pp. 269–276.

    Google Scholar 

  • Vannier, M., Petrov, R.G., Robbe-Dubois, S. et al.: 2002, Optimizing a Differential Interferometric Instrument, in: J. Bergeron and G. Monnet (eds.), ESO Symposia Scientific Drivers for ESO Future VLT/VLTI Instrumentation, pp. 340, 346.

    Google Scholar 

Download references

Author information

Authors and Affiliations

Authors

Consortia

Editor information

Editors and Affiliations

Rights and permissions

Reprints and permissions

Copyright information

© 2003 Springer Science+Business Media Dordrecht

About this chapter

Cite this chapter

Petrov, R.G., The Amber Consortium. (2003). Introducing the Near Infrared VLTI Instrument AMBER to Its Users. In: Garcia, P.J.V., Glindemann, A., Henning, T., Malbet, F. (eds) The Very Large Telescope Interferometer Challenges for the Future. Springer, Dordrecht. https://doi.org/10.1007/978-94-017-0157-0_5

Download citation

  • DOI: https://doi.org/10.1007/978-94-017-0157-0_5

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-90-481-6379-3

  • Online ISBN: 978-94-017-0157-0

  • eBook Packages: Springer Book Archive

Publish with us

Policies and ethics