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  1. www.eso.org › sci › facilitiesESO - About ALMA

    Il y a 3 jours · ALMA (Atacama Large Millimeter/submillimeter Array) is the world-largest ground-based facility for observations in themillimeter/submillimeter regime located on the Chajnantor plateau, 5000 meters altitude in northern Chile.. It enables transformational research into the physics of the cold Universe, probes the first stars and ...

  2. Il y a 1 jour · It has also demonstrated the power of interferometers like ALMA, and the ongoing importance of large, ground-based single-dish telescopes like the JCMT. Above all, it has shown that to make progress in any field of astronomy in the modern era, it is necessary to put together the findings from many telescopes, both old and new, as well as state-of-the-art model simulations.

  3. Il y a 1 jour · New Tarantula Nebula observations from the Atacama Large Millimeter/submillimeter Array (ALMA) are combined with imagery from ESO’s Very Large Telescope and the Visible and Infrared Survey ...

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  4. Il y a 3 jours · As a 50m single dish telescope with a 1–2 ∘ field of view, the strength of the Atacama Large Aperture Submillimeter Telescope (AtLAST) is in science where a large field of view, highly multiplexed instrumentation and sensitivity to faint large-scale structure is important. AtLAST aims to be a sustainable, upgradeable, multipurpose facility that will deliver orders of magnitude increases in ...

  5. Il y a 4 jours · La construction du télescope géant européen (TGE) a franchi une nouvelle étape majeure avec l’achèvement du squelette en acier de son dôme. Ce projet ambitieux, dirigé par l’Observatoire européen austral (ESO), promet de révolutionner l’astronomie en offrant des capacités d’observation sans précédent.

  6. Il y a 3 jours · We present a detailed analysis of the disk and circumstellar environment of the forming O-type star AFGL 4176 mm1, placing results from the Atacama Large Millimeter/submillimeter Array (ALMA) into context with multiwavelength data. With ALMA, we detect seventeen 1.2 mm continuum sources within 5″ (21,000 au) of AFGL 4176 mm1. We find that mm1 has a spectral index of 3.4 0.2 across the ALMA ...

  7. Il y a 3 jours · De Pater has been observing Io for decades, mostly using ground-based infrared telescopes, such as the Keck Observatory and Gemini Observatory in Hawaii, and radio telescopes like the Atacama Large (sub)Millimeter Array (ALMA) in Chile. Infrared observations capture hot features, such as lava flows, but are inherently lower resolution.

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