Sentences with phrase «in submillimeter wavelengths»

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It combines a mosaic of millimetre wavelength images from the Atacama Large Millimeter / submillimeter Array (ALMA) and the IRAM 30 - metre telescope, shown in red, with a more familiar infrared view from the HAWK - I instrument on ESO's Very Large Telescope, shown in blue.
It combines a mosaic of millimetre - wavelength images from the Atacama Large Millimeter / submillimeter Array (ALMA) and the IRAM 30 - metre telescope, shown in red, with a more familiar infrared view from the HAWK - I instrument on ESO's Very Large Telescope, shown in blue.
AzTEC - 3, which is located in the direction of the constellation Sextans, is what astronomers refer to as a submillimeter galaxy, since it shines brightly in that portion of the spectrum, but is remarkably dim at optical and infrared wavelengths.
It combines a mosaic of millimeter - wavelength images from the Atacama Large Millimeter / submillimeter Array (ALMA) and the IRAM 30 - metre telescope, shown in red, with a more familiar infrared view from the HAWK - I instrument on ESO's Very Large Telescope shown in blue.
The telescope will observe the universe at millimeter and submillimeter wavelengths, between infrared light and radio waves in the electromagnetic spectrum.
These are expected to have become rapidly enshrouded in the dust produced by the first stars; the dust absorbs much of the starlight making the galaxies difficult to see in the optical wavebands, but these same galaxies shine brightly at millimeter and submillimeter wavelengths.
This research was presented in a paper «First Detection of Equatorial Dark Dust Lane in a Protostellar Disk at Submillimeter Wavelength,» by Lee et al. to appear in the journal Science Advances.
ALMA can detect this dust from the early Universe, which is present in the most distant and ancient galaxies, thanks to submillimeter wavelengths.
Therefore, the research group targeted molecular line emissions from hydrogen cyanide (HCN), formyl ion (HCO +), and hydrogen sulfide (CS) at millimeter / submillimeter wavelengths (* 4) in the galaxy called NGC 1097 (about 50 million light years away) with the ALMA Telescope in the Atacama Desert in Chile.
That altitude is above the primary part of the atmosphere that blocks infrared light, which means the telescope can observe at wavelengths longer than the ones we see in our Disk Detective WISE data, but shorter than the submillimeter wavelengths we've observed at with the James Clerk Maxwell Telescope.
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