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ALMA deep view of part of the Hubble Ultra Deep Field
A trove of galaxies, rich in carbon monoxide (indicating star-forming potential) were imaged by ALMA (orange) in the Hubble Ultra Deep Field. The blue features are galaxies imaged by Hubble.
This image is based on the very deep ALMA survey by Manuel Aravena, Fabian Walter and colleagues, covering about one sixth of the full HUDF area.
B. Saxton (NRAO/AUI/NSF); ALMA (ESO/NAOJ/NRAO); NASA/ESA Hubble
À propos de l'image
Identification: | eso1633e |
Type: | Observation |
Date de publication: | 22 septembre 2016 20:00 |
Communiqués de presse en rapport: | eso1633 |
Taille: | 1351 x 1002 px |
À propos de l'objet
Type: | Early Universe : Cosmology : Morphology : Deep Field |
Constellation: | Fornax |
Catégorie: | Cosmology |
Fonds d'écran
1024x768
206,5 Kio
1280x1024
289,1 Kio
1600x1200
393,7 Kio
1920x1200
447,9 Kio
2048x1536
583,8 Kio
Coordinates
Position (RA): | 3 32 37.93 |
Position (Dec): | -27° 46' 33.03" |
Field of view: | 1.35 x 1.00 arcminutes |
Orientation: | North is 0.0° right of vertical |
Couleurs & filtres
Domaine | Longueur d'onde | Télescope |
---|---|---|
Visible B | 435 nm | Hubble Space Telescope ACS |
Visible V | 606 nm | Hubble Space Telescope ACS |
Visible i | 775 nm | Hubble Space Telescope ACS |
Visible I | 814 nm | Hubble Space Telescope ACS |
Visible I | 850 nm | Hubble Space Telescope ACS |
Infrarouge Z | 1.05 μm | Hubble Space Telescope WFC3 |
Infrarouge J | 1.25 μm | Hubble Space Telescope WFC3 |
Infrarouge H | 1.6 μm | Hubble Space Telescope WFC3 |
Millimétrique 231.2 GHZ | 1.3 mm | Atacama Large Millimeter/submillimeter Array |