Always private
DuckDuckGo never tracks your searches.
Learn More
You can hide this reminder in Search Settings
All regions
Argentina
Australia
Austria
Belgium (fr)
Belgium (nl)
Brazil
Bulgaria
Canada (en)
Canada (fr)
Catalonia
Chile
China
Colombia
Croatia
Czech Republic
Denmark
Estonia
Finland
France
Germany
Greece
Hong Kong
Hungary
Iceland
India (en)
Indonesia (en)
Ireland
Israel (en)
Italy
Japan
Korea
Latvia
Lithuania
Malaysia (en)
Mexico
Netherlands
New Zealand
Norway
Pakistan (en)
Peru
Philippines (en)
Poland
Portugal
Romania
Russia
Saudi Arabia
Singapore
Slovakia
Slovenia
South Africa
Spain (ca)
Spain (es)
Sweden
Switzerland (de)
Switzerland (fr)
Taiwan
Thailand (en)
Turkey
Ukraine
United Kingdom
US (English)
US (Spanish)
Vietnam (en)
Safe search: moderate
Strict
Moderate
Off
Any time
Any time
Past day
Past week
Past month
Past year
  1. 5 days agoIn a nutshell, MATISSE is able to resolve features as small as 3 mas (milli-arcsecond) in the L-band and as small as 8 mas in the N-band with the ATs, respectively 5mas and 12.5 mas with the UTs. The complete pre-requisites for MATISSE service mode observations and the up-to-date flux limits can be found on the instrument description page.
  2. The MATISSE ETC is available to determine visibilities and feasibility. However, signal-to-noise calculations still need to be verified. The instrument is offered to the community for regular science programme for the first time in P103. Reference. Publications based on MATISSE should cite the following reference paper:
  3. MATISSE is designed to address a broad range of important science goals. In particular, it will contribute to several fundamental research topics in astronomy, focusing on the inner regions of disks around young stars where planets are formed, the evolution of stars at different stages of their lives, and the environment around black holes in ...
  4. astrobiology.nasa.gov

    PICASSO. The Planetary Instrument Concepts for the Advancement of Solar System Observations (PICASSO) Program supports the development of spacecraft-based instrument systems that show promise for use in future planetary missions.The goal of the program is to conduct planetary and astrobiology science instrument feasibility studies, concept formation, proof of concept instruments, and advanced ...
  5. ui.adsabs.harvard.edu

    We present an overview of the scientific potential of MATISSE, the Multi Aperture mid-Infrared SpectroScopic Experiment for the Very Large Telescope Interferometer. For this purpose we outline selected case studies from various areas, such as star and planet formation, active galactic nuclei, evolved stars, extrasolar planets, and solar system minor bodies and discuss strategies for the ...
  6. Oct 21, 2024The use of GRA4MAT is recommended as soon as fringe tracking is possible on a MATISSE science target. Please find below more details of the modes offered. MATISSE stand-alone. Hybrid is the only observing mode offered. The hybrid mode consists of the following two steps: 1. acquisition of fringes in SiPhot mode LM + HiSens mode N; 2.
  7. We present an overview of the scientific potential of MATISSE, the Multi Aperture mid-Infrared SpectroScopic Experiment for the Very Large Telescope Interferometer. For this purpose we outline selected case studies from various areas, such as star and planet formation, active galactic nuclei, evolved stars, extrasolar planets, and solar system minor bodies and discuss strategies for the ...

    Can’t find what you’re looking for?

    Help us improve DuckDuckGo searches with your feedback

Custom date rangeX