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%ما هو (من)٪ 1 - تعريف
K-band multi-object spectrograph
INSTRUMENT MOUNTED ON ESO’S VERY LARGE TELESCOPE
K-band Multi-Object Spectrograph
The K-band multi-object spectrograph, or KMOS for short, is an instrument mounted on ESO’s Very Large Telescope Antu (UT1) at the Paranal Observatory in Chile. KMOS is able to observe 24 objects at the same time in infrared light and to map out how their properties vary from place to place.
Visible Multi Object Spectrograph
![Galaxy [[NGC 7424]] seen by VIMOS](https://commons.wikimedia.org/wiki/Special:FilePath/Magnificent Spiral Galaxy NGC 7424.jpg?width=200 "Galaxy [[NGC 7424]] seen by VIMOS")
![first light image]] of galaxy [[NGC 5364]]](https://commons.wikimedia.org/wiki/Special:FilePath/NGC 5317 (also NGC 5364).jpg?width=200 "first light image]] of galaxy [[NGC 5364]]")
![The [[Antennae Galaxies]], one of VIMOS' first images](https://commons.wikimedia.org/wiki/Special:FilePath/Phot-09a-02-normal.jpg?width=200 "The [[Antennae Galaxies]], one of VIMOS' first images")
![The [[Chandra Deep Field South]]](https://commons.wikimedia.org/wiki/Special:FilePath/A Pool of Distant Galaxies.jpg?width=200 "The [[Chandra Deep Field South]]")
![galaxy cluster]] ''ACO 3341''](https://commons.wikimedia.org/wiki/Special:FilePath/ACO 3341.jpg?width=200 "galaxy cluster]] ''ACO 3341''")
![Galaxy ''NGC 2613'', a [[spiral galaxy]] that resembles our own [[Milky Way]]](https://commons.wikimedia.org/wiki/Special:FilePath/Phot-09g-02-hires.jpg?width=200 "Galaxy ''NGC 2613'', a [[spiral galaxy]] that resembles our own [[Milky Way]]")
![VIMOS sees cluster [[NGC 6118]] at a distance of 80 million light-years](https://commons.wikimedia.org/wiki/Special:FilePath/NGC 6118 (captured by ESO’s Very Large Telescope).jpg?width=200 "VIMOS sees cluster [[NGC 6118]] at a distance of 80 million light-years")
![FORS 1]]. ''(Note supernova [[SN 2006X]] in the middle of the right image, just above the lower main spiral arm)''.](https://commons.wikimedia.org/wiki/Special:FilePath/ESO- SN 2006X in Messier 100-Phot-08b-06.jpg?width=200 "FORS 1]]. ''(Note supernova [[SN 2006X]] in the middle of the right image, just above the lower main spiral arm)''.")
WIDE FIELD IMAGER AND A MULTI-OBJECT SPECTROGRAPH INSTALLED AT THE EUROPEAN SOUTHERN OBSERVATORY'S VERY LARGE TELESCOPE
VIMOS; Visible Multi-Object Spectrograph
The Visible Multi-Object Spectrograph (VIMOS) is a wide field imager and a multi-object spectrograph installed at the European Southern Observatory's Very Large Telescope (VLT), in Chile. The instrument used for deep astronomical surveys delivers visible images and spectra of up to 1,000 galaxies at a time.
SOPHIE échelle spectrograph
FRENCH ASTRONOMICAL INSTRUMENT
SOPHIE spectrograph; SOPHIE echelle spectrograph
The SOPHIE (Spectrographe pour l’Observation des Phénomènes des Intérieurs stellaires et des Exoplanètes, literally meaning "spectrograph for the observation of the phenomena of the stellar interiors and of the exoplanets") échelle spectrograph is a high-resolution echelle spectrograph installed on the 1.93m reflector telescope at the Haute-Provence Observatory located in south-eastern France.
