English: The three panels show different components of near-infrared background light detected by the Hubble Space Telescope in deep-sky surveys. The one on the left is a mosaic of images taken over a 10-year period. When all the stars and galaxies are masked, the background signals can be isolated, as seen in the second and third panels. The middle panel reveals "intra-halo light" from rogue stars torn from their host galaxies, and the panel on the right captures the signature of the first galaxies formed in the universe.
Tarix
Mənbə
Müəllif
NASA, ESA, and K. Mitchell-Wynne (University of California, Irvine)
Lisenziya
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Şəkil başlığı
The three panels show different components of near-infrared background light detected by the Hubble Space Telescope in deep-sky surveys. The one on the left is a mosaic of images taken over a 10-year period. When all the stars and galaxies are masked, the background signals can be isolated, as seen in the second and third panels. The middle panel reveals "intra-halo light" from rogue stars torn from their host galaxies, and the panel on the right captures the signature of the first galaxies formed in the universe. Link: NASA Press release
Təmin edici
NASA, ESA, and K. Mitchell-Wynne (University of California, Irvine)
Mənbə
ESA/Hubble
İstifadə qaydası
Creative Commons Attribution 4.0 International License